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April 30, 2002

 NASA ADMINISTRATOR NAMES NEW
ASSOCIATE ADMINISTRATOR FOR SAFETY

Bryan D. O'Connor, a former NASA Space Shuttle program
director, astronaut and Marine Corps test pilot, was named
Associate Administrator for the Office of Safety and Mission
Assurance (OSMA) at NASA Headquarters in Washington. He
replaces Fredrick D. Gregory, who has been leading the Office
of Space Flight since December.

O'Connor, 55, will be responsible for the oversight of all
agency safety issues through the development, implementation
and oversight of reliability, maintainability and quality
assurance policies. He will report to NASA on June 3, 2002.

"Bryan's distinguished career as both a naval aviator and
NASA astronaut give him the perspective necessary to ensure
the continued safety of our programs," said NASA
Administrator Sean O'Keefe. "His attention and dedication to
safety were signature characteristics during his NASA career,
and I look forward to his stewardship of this vital office."

O'Connor was selected as an astronaut in May 1980 and is a
veteran of two Space Shuttle missions. He was pilot on STS-
61B in 1985 and crew commander of STS-40 in 1991.

When the Space Shuttle Challenger was lost in 1986, he was
given a number of safety and management assignments over the
next three years. O'Connor organized the initial wreckage
reassembly activities at Cape Canaveral, Fla., and
established and managed the operation of the NASA
Headquarters Action Center, the link between the agency and
the Presidential Blue Ribbon Accident Investigation Panel.

In 1986, he was appointed chairman of NASA's new Space Flight
Safety Panel. O'Connor also served as Aviation Safety Officer
for the astronaut corps.

Before joining NASA, O'Connor was a U.S. Marine Corps test
pilot and graduated from the U.S. Naval Academy at Annapolis,
Md., in 1968. He flew the A-4 Skyhawk and AV-8A Harrier on
land and sea assignments in the United States, Europe and the
Western Pacific.

O'Connor left NASA in August 1991 to become commanding
officer of the Marine Aviation Detachment, Naval Air Test
Center, Patuxent River, Md. After retiring from the U.S.
Marine Corps, he returned to NASA Headquarters as Deputy
Associate Administrator for the Office of Space Flight and
Space Shuttle program director. Among his other
responsibilities, he developed a comprehensive flight safety
improvement plan for the Space Shuttle.

O'Connor left NASA in February 1996 to become an aerospace
consultant. He rejoins NASA after serving as director of
engineering at Futron Corp., a Washington-based aerospace
safety and risk-management consulting firm.

Additional information about O'Connor and OSMA can be found
on the Internet at:

http://www.hq.nasa.gov/office/codeq

http://www.jsc.nasa.gov/Bios/htmlbios/oconnor-bd.html

Hubble's Advanced Camera unveils a panoramic new view of the Universe [heic0206]

 Jubilant astronomers today unveiled humankind's most spectacular
views of the Universe as captured by the NASA/ESA Hubble Space Telescope's
new Advanced Camera for Surveys (ACS). They also reported that Hubble
is operating superbly since the March servicing mission and are
looking forward to more pictures from the newly revived NICMOS camera.

More at:
http://sci.esa.int/hubble/news/index.cfm?oid=29876

 MILESTONE REVIEW BRINGS NASA ONE STEP CLOSER TO NEW LAUNCH
VEHICLE

NASA is another step closer to defining the next-
generation reusable space transportation system and successor
to the Space Shuttle.

The Space Launch Initiative (SLI), a NASA-wide effort
defining the future of human space flight, has completed its
first milestone review -- resulting in a narrower field of
potential candidates for the nation's second-generation
reusable space transportation system.

"To use the resources afforded by space, it's critical to
increase reliability and safety while at the same time
reducing the cost of space transportation," said Art
Stephenson, director of NASA's Marshall Space Flight Center,
Huntsville, Ala., which manages the SLI for the Office of
Aerospace Technology. "The Space Launch Initiative is doing
the groundwork to accomplish these goals and create a second-
generation launch system."

"We're not just designing a launch vehicle," added Dennis
Smith, also of Marshall, program manager of the Space Launch
Initiative. "We're designing the complete system."

The recent review, called the Initial Architecture Technology
Review, analyzed and evaluated competing second-generation
reusable space transportation architectures and technologies
against NASA and commercial mission requirements, as well as
safety and cost goals.

Architecture refers to the complete transportation system
design -- that is, the vehicles and their components that fly
into space, as well as the ground operations needed for
launch. The transportation system design includes an Earth-
to-orbit reusable launch vehicle (the Space Shuttle is the
first-generation reusable launch vehicle); on-orbit transfer
vehicles and upper stages to put satellites into orbits;
mission planning; ground and flight operations; and support
infrastructure, both on orbit and on the ground.

Three contractor architecture teams -- The Boeing Company of
Seal Beach, Calif.; Lockheed Martin Corp. of Denver; and a
team including Orbital Sciences Corp. of Dulles, Va., and
Northrop Grumman of El Segundo, Calif. -- presented dozens of
potential architectures for review. Following the review,
each retained a handful of possible candidates for the
nation's next-generation reusable space launch system.

The review allows the Space Launch Initiative to target
investments and support what the program manager called the
"up-front, homework part of the program" -- furthering
technologies to aid in the development of a second-generation
reusable launch vehicle. Another review will be held in
November to further narrow potential space transportation
architectures to two or three choices.

"We're going to seek the final and best ideas from industry,
academia and government," said Smith. With the final
selection of an architecture, full-scale development of a
reusable launch vehicle could begin around the middle of this
decade.

Since propulsion systems require a long lead-time to design,
develop, test and evaluate, it isn't surprising that
propulsion analysis was a chief driver through the recently
completed review activity.

"We spent a lot of time analyzing propulsion technologies,"
said Smith. "Among the outcomes is a focus on kerosene-fueled
main engines." This focus is based on studies, conducted by
the architecture contractors, that examine performance of
competing technologies in safety, reliability, cost and
operability. Studies indicated that kerosene main engines
have excellent potential to meet government and commercial
needs. The second-generation vehicle will have a two-stage-
to-orbit propulsion system based on engines fueled by all
kerosene, all hydrogen or a combination of kerosene and
hydrogen.

Dependable, long-life engines, along with crew escape and
survival systems, and long-life, lightweight integrated
airframes are among the Space Launch Initiative's highest
priorities. Each greatly impacts the program's bottom line of
increased safety, reliability and cost effectiveness.

All NASA's field centers and the Air Force Research
Laboratory are actively participating in the Space Launch
Initiative. Additional information on NASA's Space Launch
Initiative, including a list of the selected contractors, is
available on the Internet at:

http://www.slinews.com
http://www.spacetransportation.com

 HUBBLE'S NEW CAMERA DELIVERS BREATHTAKING VIEWS OF THE
UNIVERSE

"Remarkable, breathtaking" are words jubilant
astronomers are using to describe the first four views of the
universe taken by the Hubble Space Telescope's new Advanced
Camera for Surveys, released by NASA today.

The new camera was installed on Hubble by astronauts during a
shuttle mission last March, the fourth Hubble Space Telescope
servicing mission. During five of the most challenging
spacewalks ever attempted, the crew successfully upgraded the
orbiting telescope with the new camera, a new power unit, new
solar arrays and an experimental cooling unit for an infrared
camera. Hubble managers say the orbiting telescope has been
operating superbly since the servicing mission.

"Today marks the beginning of a new era of exploration with
Hubble," said Dr. Ed Weiler, Associate Administrator for
Space Science at NASA Headquarters, Washington. "Our team of
scientists and engineers on the ground and the astronauts in
space once again did the impossible. After 12 years in space,
Hubble not only was given a major overhaul, its new camera
has already shown us that, even after 12 years of great
science and astounding images, we haven't seen anything yet."

Among the suite of four "suitable-for-framing" Advanced
Camera for Surveys (ACS) science-demonstration pictures
released today is a stunning view of a colliding galaxy,
dubbed the "Tadpole," located 420 million light-years away.
Unlike textbook images of stately galaxies, the "Tadpole" --
with a long tail of stars -- captures the essence of a
dynamic, restless and violent universe, looking like a
runaway pinwheel firework.

"The ACS is opening a wide new window onto the universe.
These are among the best images of the distant universe
humans have ever seen," said astronomer Holland Ford of Johns
Hopkins University in Baltimore, lead scientist in the
camera's seven-year development.

The camera's tenfold increase in efficiency will open up much
anticipated new capability for discovery. "ACS will allow us
to push back the frontier of the early universe. We will be
able to enter the 'twilight zone' period when galaxies were
just beginning to form out of the blackness following the
cooling of the universe from the big bang," said Ford.

The ACS is a camera of superlatives. It is expected to
surpass the sensitivity of the largest ground-based telescope
to eventually see the very faintest objects ever recorded.
The camera delivers a panoramic crispness comparable to that
of a wide-screen movie, containing 16 million picture
elements (megapixels) per image. By comparison, digital
photos from typical consumer cameras are 2 to 4 megapixels.

The ACS image of the Tadpole illustrates the dramatic gains
over the Wide Field Planetary Camera 2 resulting from
doubling the area and resolution, and demonstrates a five-
fold improvement in sensitivity. An unexpected bonus is the
enormous number of galaxies in the new Hubble image beyond
the Tadpole galaxy, giving it an appearance like the galaxy-
filled Hubble Deep Field (HDF) image, taken in 1995. However,
the ACS picture was taken in one-twelfth the time it took for
the original HDF. Like the Hubble Deep Field, the ACS
galaxies contain myriad shapes that are snapshots of galaxies
throughout the universe's 13 billion-year evolution. The ACS
images are so sharp astronomers can identify "building
blocks" of galaxies, colliding galaxies and extremely distant
galaxies in the field -- an exquisite sampler of galaxies.

"The ACS will let us obtain the deepest image of the universe
for the foreseeable future," added astronomer Garth
Illingworth of the University of California, Lick
Observatory, Santa Cruz, the deputy leader for the camera
team.

The other pictures include a stunning collision between two
spiral galaxies, dubbed "the Mice," that presage what might
happen to our own Milky Way several billion years in the
future when it collides with the neighboring galaxy in the
constellation Andromeda. Computer simulations show that we
are seeing the collision of the Mice approximately 160
million years after their closest encounter. Running the
simulations forward in time shows that the two galaxies will
eventually merge. A similar fate may await the Milky Way and
the Andromeda galaxy.

Looking closer to home, ACS imaged the "Cone Nebula," a
craggy-looking mountaintop of cold gas and dust that is a
cousin to Hubble's iconic "pillars of creation" in the Eagle
Nebula, photographed in 1995.

Peering into a celestial maternity ward called the M17 Swan
Nebula, the ACS revealed a watercolor fantasy-world tapestry
of vivid colors and glowing ridges of gas. Embedded in this
crucible of star creation are embryonic planetary systems.

In addition to the ACS, spacewalking astronauts installed a
new high-tech mechanical "refrigerator" on Hubble during the
servicing mission. This "cryocooler" has successfully pumped
most of the heat out of the interior of the Near Infrared
Camera and Multi-Object Spectrometer (NICMOS), achieving and
maintaining to within a few hundredths of one degree the
target temperature for neon gas passing through the
instrument of 70 degrees Kelvin (minus 203 degrees Centigrade
or minus 333 degrees Fahrenheit).

Engineers are now in the process of checking out the
operation of the resuscitated NICMOS instrument. By early
June, scientists expect to release the first astronomical
images taken with the NICMOS since 1998, when it was still
being cooled by a rapidly depleting block of solid nitrogen
ice.

The new rigid solar arrays, working with the new Power
Control Unit, are generating 27 percent more electrical power
than the previous arrays. This doubles the electrical power
that can be allocated to the scientific instruments on
Hubble. The new reaction wheel is operating normally. Nearly
a month ago, the Space Telescope Imaging Spectrograph and the
Wide Field and Planetary Camera 2 resumed science
observations.

"This servicing mission has turned out to be an extraordinary
success," said Preston Burch, Hubble Project Manager at
NASA's Goddard Space Flight Center in Greenbelt, Md. "It was
the most difficult and complicated Hubble servicing mission
attempted to date and our
observatory came through it with flying colors."

Electronic image files, animation and additional information
are available on the Internet at:
http://oposite.stsci.edu/pubinfo/pr/2002/11
http://oposite.stsci.edu/pubinfo/latest.html
http://oposite.stsci.edu/publinfo/pictures.html
and
http://hubblesite.org/go/news

April 29, 2002

 http://mars.jpl.nasa.gov/spotlight/mgscontinuesAll.html

Global Surveyor Continues Its Watch on the Red Planet
Jet Propulsion Laboratory

Weather reports from Mars, global mapping, inspection of potential landing
sites, more data about the red planet than from all previous missions - no
problem for the hardworking Mars Global Surveyor spacecraft.

In fact, the Global Surveyor has been so successful that it earned an
extension following conclusion of its prime mapping mission early in 2001.
The second extension began in April 2002 and will continue the mission into
late 2004.

"Things are going well," said Tom Thorpe, Mars Global Surveyor project
manager at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "We've
accomplished all of our primary mission objectives to date and the science
instruments have returned a tremendous amount of data. Now we're looking
forward to all the science to come in the second extension."

In addition to mapping operations, the spacecraft is targeting images of
potential landing sites for the 2003 Mars Exploration Rovers. In its
extended mission, the Surveyor has been given latitude to take pictures at
different angles and target areas missed in the prime mission.

One of the tasks that scientists want to do is obtain stereo
(three-dimensional) images of some areas already covered. To do this, the
spacecraft has to be pointed off-nadir. Nadir is the point directly below
the observer; hence if the spacecraft is "tipped," the target can be imaged
up to 30 degrees away from the original ground track. When a place imaged
from one angle is pictured again from another angle, the images can be
overlaid to create a stereo picture.

This technique is useful for providing dramatic views of the planet's
surface and to study the vertical profile of its atmosphere. For example,
scientists want as complete a picture as possible of potential landing sites
for the 2003 Mars Exploration Rovers. The stereo images taken by Global
Surveyor will help substantially in the final site selection.

"There is still so much to learn about Mars," said Mars scientist Dr. Ken
Edgett, Malin Space Science Systems, San Diego, Calif. "Our high-resolution
camera is testing hypotheses formulated over the past two decades using
Mariner 9 and Viking data and even new theories from Surveyor and Mars
Odyssey images. We're seeking to understand previous observations, and to
monitor changes that are taking place due to weather and changes in polar
frost."

So How's the Weather on Mars?

Mars has seasons, just as Earth does. Using the Mars orbiter camera on
Surveyor, scientists are now able to monitor the red planet's weather
changes from one martian year (about twice as long as an Earth year) to the
next. One of their discoveries has been that the southern polar ice cap,
long thought to be permanent, isn't so permanent.

"What we're finding is just short of incredible," said Edgett. "For most of
the Mars year, the weather patterns are very predictable. Last year, in late
June, we had global dust storms that obscured the planet for three months -
an event that did not fit the patterns we'd otherwise seen. We found that
there were lots of storms going on at once, not that there was one gigantic
global dust storm, as was thought during previous events."

Thorpe said, "The weather reports are very important, since weather will
affect future spacecraft landings and operations on the surface of Mars,
including the 2003 Mars Exploration Rovers."

Weekly Mars weather reports are available by going to the Mars Exploration
page at
http://mars.jpl.nasa.gov and clicking on the How's the Weather on
Mars box.

Students interested in exploring Mars further can go to
http://mars.jpl.nasa.gov/classroom/students.html for more information on the
red planet.

Extensions Lead to Discoveries

"One of the reasons I'm so very excited about the second extension is
because every week there is something new and surprising in our data," said
Mars scientist Ken Edgett. "And what's really cool is that every four to six
months we discover something totally amazing. Last year, we were
flabbergasted to find that the southern polar "permanent" ice cap isn't so
permanent. We're now tracking changes to the cap on shorter time scales."

Each winter, frost forms a seasonal polar cap covering everything from 60
degrees latitude to 90 degrees latitude; it retreats in spring. The
permanent ice cap, which is mostly carbon dioxide, remains through the
entire summer and was previously thought to be permanent.

"We now know that even in summer the ice is subliming (converting directly
from solid to vapor) at a rate that suggests the entire cap could disappear
in a few thousand to tens of thousands of years," said Edgett. "There's a
lot of carbon dioxide in the permanent cap, but we're finding that it is
going away on a larger time scale [than the seasonal frost], independent of
season."

For more information and images, please see
http://www.msss.com/mars_images/moc/CO2_Science_rel/ .

April 28, 2002

 MARS ODYSSEY THEMIS IMAGES
April 22-26, 2002

o Alba Patera (Released 22 April 2002)
http://themis.la.asu.edu/zoom-20020422a.html

o Eastern Floor of Holden Crater (Released 15 April 2002)
http://themis.la.asu.edu/zoom-200204.html

o Cerberus (Released 24 April 2002)
http://themis.la.asu.edu/zoom-20020424a.html

o Knobby terrain in Northern Arabia Terra (Released 25 April 2002)
http://themis.la.asu.edu/zoom-20020425a.html

o Noctis Labyrinthus (Released 26 April 2002)
http://themis.la.asu.edu/zoom-20020426a.html

All of the THEMIS images are archived here:

http://themis.la.asu.edu/latest.html

NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission
for NASA's Office of Space Science, Washington, D.C. The Thermal Emission
Imaging System (THEMIS) was developed by Arizona State University,
Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing.
The THEMIS investigation is led by Dr. Philip Christensen at Arizona State
University. Lockheed Martin Astronautics, Denver, is the prime contractor
for the Odyssey project, and developed and built the orbiter. Mission
operations are conducted jointly from Lockheed Martin and from JPL, a
division of the California Institute of Technology in Pasadena.

----------------------------------------------------------------------------
http://themis.la.asu.edu/zoom-20020422a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
Alba Patera (Released 22 April 2002)

The Science

This image, centered near 46.5 N and 119.3 W
(240.7 E), is on the northwestern flank of a
large, broad shield volcano called Alba Patera.
This region of Mars has a number of unique
valley features that at first glance look dendritic
much in the same pattern that rivers and
tributaries form on Earth. A closer look reveals
that the valleys are quite discontinuous and
must form through a different process than
surface runoff of liquid water that is common on
Earth. A number of processes might have taken
place at some point in the Martian past to form
these features. Some of the broad valley
features bear some resemblance to karst
topography, where material is removed
underground by melting or dissolving in
groundwater causing the collapse of the surface
above it. The long narrow valleys resemble
surfaces where groundwater sapping has
occurred. Sapping happens when groundwater
reaches the surface and causes headward
erosion, forming long valleys with fewer
tributaries than is seen with valleys formed by
surface water runoff. The volcano itself might
have been a source of heat and energy, which
played a role in producing surfaces that indicate
an active groundwater system.

The Story

Fluid, oozing lava poured somewhat lazily over this area long
ago. It happened perhaps thousands of times, over hundreds of
thousands of Martian years, creating the nearly smooth,
plaster-of-Paris-looking terrain seen today. (Small craters
also dent the area, though they may deceive you and look like
raised bumps instead. That's just a trick of the eye and the
lighting - tilt your head to your left shoulder, and you should
see the craters pit the surface as expected.)

The lava flows came from a Martian "shield" volcano named
Alba Patera. Shield volcanoes get their name from their
appearance: from above, they look like large battle shields lying
face up to the sky as if a giant, geological warrior had lain them
down. Perhaps one did - if you think of a volcano as a "geologic
warrior," that is. These volcanoes aren't too fierce, however.
Because of the gentle layering of lava over time, they don't
stand tall and angry against the horizon, but instead have
relatively gentle slopes and are spread out over large areas.
(On Earth, the Hawaiian Islands are examples of shield
volcanoes, but you can't see much of their expanse, since they
rise almost three miles from the ocean floor before popping out
above the water's surface.)

What's most interesting in this picture are all of the branching
features that lightly texture the terrain. The patterns may look
like those caused by rivers here on Earth, but geologists say
that no surface streams on Mars were responsible. That's no
disappointment, however, to those who'd like to find water on
Mars, because there are still intriguing water-related
possibilities here.

Some of the broad valley features in this image look like karsts,
a terrain found on Earth in Karst, a limestone area on the
Adriatic Sea in modern-day Croatia, and in other world regions
including France, China, the American Midwest, Kentucky, and
Florida. Karst terrain on Earth is barren land with all kinds of
caves, sinkholes, and underground rivers that excavate the
subsurface, causing the surface above it to collapse. So,
perhaps it's like that in this region on Mars as well. Future
Martian spelunkers should be excited, because most caves on
Earth are in karst areas.

Other suggestions of water here are some long, narrow valleys
that resemble Earth surfaces where groundwater has sapped
away the terrain. Sapping occurs when groundwater erodes
slopes, creating valleys. Water action can be concentrated at
valley heads, leading to what is called their "headward growth."
That may be what has happened here on Alba Patera as well.

All of these features suggest the action of liquid water, but
Mars is so cold, you might wonder if any water would have to
be as frozen as the world it is on. Well . . . that depends!
Remember that this area is part of a volcano, and volcanoes can
put out enough heat and energy below the surface to keep
water warm enough to flow - if not now, then at least in the
past when the volcano was more active.

 

----------------------------------------------------------------------------
http://themis.la.asu.edu/zoom-20020423a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
A Cloudy Day on Mars (Released 23 April 2002)


The Science

This image, centered near 49.7 N and 43.0 W
(317.0 E), displays splotchy water ice clouds
that obscure the surface. Most of Mars was in
a relatively clear period when this image was
acquired, which is why many of the other
THEMIS images acquired during the same
period do not have obvious signs of
atmospheric dust or water ice clouds. This
image is far enough north to catch the edge of
the north polar hood that develops during the
northern winter. This is a cap of water ice and
CO2 ice clouds that form over the Martian
north pole. Mars has a number of interesting
atmospheric phenomena which THEMIS will be
able to view in addition to water ice clouds,
including dust devils, dust storms, and tracking
atmospheric temperatures with the infrared
camera.

The Story

Anyone who's been on an airplane in a storm knows how
clouds on Earth can block the view below. The thin water ice
clouds on Mars might make things slightly blurry, but at least
we can still see the surface.

While the surface features may not be as clear in this image,
it's actually kind of fascinating to see clouds at work, because
we can get a sense of how the north pole on Mars influences
the weather and the climate. In this image, the north pole is
responsible for the presence of the clouds. Made of water ice
and carbon dioxide, these clouds "mist out" in a atmospheric
"hood" that caps the surface during the northern Martian
winter, hiding it from full view of eager observers here on Earth.

----------------------------------------------------------------------------
http://themis.la.asu.edu/zoom-20020424a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
Cerberus (Released 24 April 2002)

The Science

The Cerberus feature is a relatively dark region
at the southeastern edge of the huge Elysium
Mons volcanic complex. It was visible to early
astronomers of Mars because it was a
distinctive dark spot on a large bright region of
the planet. Today we recognize that the
Cerberus region encompasses a range of
geologic terrains from relatively young and
smooth lava flows to the very rugged, ancient
eroded landscape seen in this THEMIS image.
The Cerberus feature has also proven to be
ephemeral. Compared to just 20 years ago when
the Viking orbiter instruments viewed the
planet, the Cerberus feature has shrunk down
from its original length of roughly 1000
kilometers to just a few isolated dark splotches
of just a few 100 kilometers. This is testament
to the active eolian environment on Mars where
global dust storms can lift and then later deposit
significant amounts of dust, brightening formerly
dark surfaces. The THEMIS image occurs in a
portion of Cerberus that remains relatively dark
and dust-free although in the bottommost
portion of the image are faint, criss-crossing
lines that likely are dust devil tracks. The
abundant dune-like features covering many of
the low, smooth surfaces are similar to those
found in many places across the planet. They
are evidence of the interaction of wind and
movable particles at the surface but not
necessarily in today's environment. In many
other places on Mars they are clearly inactive;
relicts of a different climate.

The Story

Hellhound of Greek mythology, Cerberus was the
three-headed, dragon-tailed dog that stood guard at the
opening to the underworld. This rough-and-tumble Mars
terrain looks just as fierce and foreboding. At the edge of the
huge Elysium Mons volcano complex, the Cerberus area
appeared as a dark spot to early Mars astronomers in an
otherwise bright region of the planet. If this dark area seems
somewhat hellish to your imagination too, you'll be glad to
know that the Martian wind has been brightening up the area.

Just twenty years ago, the Viking orbiters reached Mars for the
first long-term studies of Mars up close. The Cerberus feature
was then almost 600 miles long, but has now been vanquished
down to few small splotches about 60 miles long. Call that a
triumph of lightness upon the surface, but don't think that the
force bringing back the light is gentle and kind. The Martian
wind can kick up a fierce global dust storm that lifts up the
bright Martian dust into the air and then blankets the surface
with the brighter material as it settles down again.

The ancient, eroded terrain in this image is still rather dark and
dust free, so you might say it's one area where a mythical
Cerberus still guards its shrinking territory. The wind teases it,
however, by kicking up small, whirling dust devils that leave
long, dark, scratchy tracks upon the land. Fields of dunes
wrinkle the surface in places as well, but they may be
permanently cemented upon the surface now, no longer able to
blow and drift as they did in their younger days.

----------------------------------------------------------------------------
http://themis.la.asu.edu/zoom-20020425a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
Knobby terrain in Northern Arabia Terra (Released 25 April 2002)

The Science

This THEMIS visible image shows a region in
northern Arabia Terra near 44° N, 322° W (38°
E). Knobby or "scabby" plains units that mantle
and modify a pre-existing cratered surface
dominate the unusual landscape in this region.
Several large (5-8 km diameter) impact craters
seen in the upper left of the image have been
extensively modified since their initial
formation. The rims of these craters can still be
seen, but the ejecta deposits and the
surrounding plains have been buried by a layer
of material. This mantling layer has itself been
modified to produce a pitted, knobby surface.
Circular depressions of all sizes, presumably
the remnants of impact craters, are filled with
smooth deposits. In some places large regions
have been covered by this smooth material; an
example can be seen in the lower right portion
of this image. In many cases the impact craters
have been extensively modified prior to their
being filled. This modification indicates an
erosion process that has removed material from
the walls to produce shapes that vary from
circular with crisp rims, to circular with no rims,
to oblong and elliptical forms, and finally to
irregular shapes whose initial circular outline
can barely be detected. The slope of the channel
at the top of the image has an unusual deposit
of material that occurs preferentially on the
cold, north-facing slope. Similar deposits are
seen frequently at mid- northern and southern
latitudes on Mars, and have a characteristic,
rounded boundary that typically occurs at
approximately the same distance below the
ridge crest. It has been suggested that these
deposits once draped the entire surface and
have since been removed from all but the cold
north-facing slopes. The presence and removal
of ground ice may play an important role in the
formation of this layer, as well as the knobby
terrain and unusual features seen in this image.

This image is the 22nd image in a series of
daily images released by the THEMIS Team.

The Story

There's no way these impact craters are in their original,
pristine shape. Check out their strange deformities and register
the geological gross-out factor of all the "scabs" upon the land.
You can still see the rims of craters in this savaged land, but an
aggressive layer of material once spread out across it, burying
the ejected material and all the surrounding plains. This
cloaking layer didn't win the battle of dominance, however, as it
too has been battered over time, producing the pitted, knobby
surface seen today.

Only a few smooth deposits in the area are spared from the
scabby, scarred look of the long barraged (see lower right
portion of the image). Circular depressions, the probable
remains of impact craters, are filled with this smooth material.
Some were already well eroded prior to being filled, with
material removed from their walls used to sculpt the varying
shapes.

The dark, shadowed channel at the top of this image has an
unusual deposit of material on its cold, north-facing slope.
Since this material is found elsewhere on Mars, at
approximately the same distance below the ridge crest, could it
have draped the entire surface of Mars long ago? Why has it
been lost from all but the northern slopes? Could ice in the
ground play a role in forming and preserving this layer? And did
it craft the knobby terrain and other strange features in this
area?

These are the kinds of questions geologists are asking. As this
image proves, the more you discover, the more questions you
have. That's what keeps exploration so exciting.

----------------------------------------------------------------------------
http://themis.la.asu.edu/zoom-20020426a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
Noctis Labyrinthus (Released 26 April 2002

The Science

This image shows a portion of Noctis
Labyrinthus, a large valley system at the
western end of the Valles Marineris canyon
system. Noctis Labyrinthus is notable for its
unusual pattern of intersecting valleys, which
give the region a maze-like appearance when
viewed from above. The walls of these valleys
are very high (~5 km) and quite steep, with
slopes approaching 35°. Dust covers most of this
region, leading to its rather uniform appearance.
At the tops of the ridgelines, small dark streaks
can be observed trailing downslope; these
streaks suggest that the sediments covering this
area occasionally become unstable and slide.
Ridges of resistant material also can be observed
in the highest terrains. In the lower half of the
image, a small linear feature appears to cut
across the generally NE/SW-trending slopes.
This feature is not continuous, indicating that
geologic activity has disrupted it since its
formation. The northeastern termination of the
feature is on a mesa, where it is joined by a less
pronounced but similar feature that trends
NE/SW. These small features may have
originated in several ways: they may be ridges
formed by compression, they may be small fault
scarps, or they may represent the edges of
ancient lava flows that have been disrupted by
the formation of the valley system.

The Story

The smoothly sculpted surface in this close-up image belies
the bizarre and twisted Martian landscape of which it is a part
(seen at a larger scale in the context image). Labyrinths have
long been in the human imagination, and it's no wonder that
this area conjured up for early viewers all of the legends of
antiquity, of a land where a Minotaur hides and a conquering
hero needs a spool of thread to guide him through an inner
maze.

As writer Jorge Luis Borges might say, this Martian region is
a real-life example of a geological "garden of forking paths," a
dangerous-seeming place where "the paths of the labyrinth
converge." Noctis Labyrinthus, as it's called, is an area of
sprawling, intersecting valleys on Mars, and like a Borgesian
story, holds within it elusive truths about the passage of time
and a multi-layered landscape of possibility.

At the western end of Valles Marineris, the largest canyon in
the solar system, Noctis Labyrinthus holds the secrets to
long-term geologic change in the area. It would be easy to
lose oneself on a wandering path through the terrain. The
walls of this Martian valley maze rise swiftly and steeply to
their three-mile heights, and a layer of long-settled dust
deceives the eye, making everything look the same. (Well,
almost everything. Look closely, and some of realities of the
labyrinth are revealed.)

From the tops of ridge lines, small, dark streaks trail down
the sides, leaving scant but clear evidence of the sediment
that once slid downslope. A long, jagged slash cuts the land
(lower third of the image), but is broken in the middle by some
unknown geologic force that moved the land through it,
"erasing it" sometime later. And then the mysteries: what are
the features seen in this image and how did they come to be?
Ridges formed by compression? Small cliff lines ("scarps")
caused by faults? Or perhaps the edges of ancient lava flows,
disrupted by the formation of the valley system?

Whatever they are, they represent well the strange and
misleading passageways of legend and lore, where the way to
the truth of the matter and back again is hard to find.

April 27-28, 2002

Most Recent OBPR News - 4/26/2002
___________________________________

1) An Awesome Global Experience! Global Science and Technology Week
The Office of Science and Technology Policy of the Executive Office of the President has joined with representatives from over 2...
For more info:
http://spaceresearch.nasa.gov/news.html#159

2) Dizziness in Astronauts Leads NASA Researchers to Find Genetic Cause for Orthostatic Intolerance
Studies of astronauts before, during, and after spaceflight not only will help stop the dizziness that occurs after returning to...
For more info:
http://spaceresearch.nasa.gov/news.html#158

3) Research on Station Weekly Update
In this week's update, the Space Shuttle Atlantis delivers new and returned experiments and a new facility to the Station. <P></...
For more info:
http://spaceresearch.nasa.gov/news.html#157

4) Workshop for Fundamental Physics in Space
The workshop provides the Fundamental Physics investigators an opportunity to report on progress in their research and to descri...
For more info:
http://spaceresearch.nasa.gov/news.html#156

5) Research Update: Serendipity in the Laboratory - Dust Busters and Dust Seekers Find Common Ground
Thanks to new tools that allowed researchers to create dusty plasmas in the laboratory for the first time, researchers are using...
For more info:
http://spaceresearch.nasa.gov/news.html#155

 

Navigate to http://spaceresearch.nasa.gov/ for more OBPR news, information and features.

Cassini Significant Events
for 04/18/02 - 04/24/02

The most recent spacecraft telemetry was acquired from the Goldstone
tracking station on Tuesday, April 23. The Cassini spacecraft is in an
excellent state of health and is operating normally. Information on the
present position and speed of the Cassini spacecraft may be found on the
"Present Position" web page located at
http://saturn.jpl.nasa.gov/cassini/english/where/ .

Magnetospheric and Plasma Science data collection has resumed following
last week's Probe checkout. Quiet cruise activities continued with
minimal onboard activities being performed.

The Satellite Orbiter Science Team (SOST) and Project Science Group -
Satellite Surfaces Working Group met to make a decision on the Enceladus
flybys in Orbits 3, 4, and 11. A plan was developed and SOST will
request a change to the flyby altitude for the non-targeted Enceladus
flyby on Orbit 3 with the understanding that this may be very difficult
for the Project to accommodate.

A Planetary Data System (PDS) archive workshop was held this week at the
Huygens Science Working Team meeting in Paris, France. The meeting was
attended by Huygens team Principal and Co-Investigators,
Interdisciplinary Scientists, and Cassini and PDS archive
representatives. The workshop was an introduction to the work involved
in archiving with the PDS, and contained examples of Cassini orbiter
work and demonstrations of Galileo and Pathfinder imaging CDs. Huygens
team members responded positively to the presentation of proposed roles
and responsibilities, which included help in generating instrument
description files based on the European Space Agency SP-1177 document.

Additional progress was made in archiving for the Visual and Infrared
Mapping Spectrometer (VIMS), Ultraviolet Imaging Spectrograph (UVIS),
and Cosmic Dust Analyzer (CDA). JPL Imaging node representatives
traveled to Tucson to meet with the VIMS team to discuss archiving.
Samples of UVIS data products were sent to the PDS Atmospheres node for
review, and the iterative process for reviewing label contents and file
structures has begun. Small Bodies PDS Node and CDA personnel met to
further define data products. CDA has identified EKernel and CKernel
data to archive.

Instrument Operations reported that the Events Kernel System Design
document D-22965 was distributed last week. In addition, unit and
system testing of E-Kernel software components has begun. Testing is
going well, and development is on schedule.

Uplink Office (ULO) personnel presented a tutorial on the use of the
Solid State Recorder Management Tool to users from the Spacecraft
Operations Office, Mission Planning, and Science Planning. Work on
Mission Sequence Subsystem (MSS) D8.0.1 began this week. This patch
delivery is intended to release the Science Opportunity Analyzer and SSR
Management tools, synchronize the versions of the Inertial Vector
Propagator/Kinematic Prediction Tool in use by the Pointing Design Tool
(PDT) and ACS operations, and address miscellaneous clean-up of items in
PDT, APGEN, SEG and SEQGEN that are needed for the Science Operations
Plan development process.

ULO chaired a meeting where plans for the development of the Automated
Sequence Process (ASP) were discussed and agreed upon. A preliminary
version of ASP is scheduled for delivery in late September '02. The
software will perform basic processing of a command request, but not
include automated notification. Prototype development work is underway,
with preliminary requirements to be finished and final coding started
in late April '02. ULO began work on a presentation outlining a
long-term plan for the Cassini Information Management System (CIMS)
through the end of its development. The purpose is to inform users of
the functionality available at critical milestones, and provide a forum
to discuss processes currently under construction that CIMS will be
required to support.

Cassini is a cooperative project of NASA, the European Space Agency and
the Italian Space Agency. The Jet Propulsion Laboratory, a division of
the California Institute of Technology in Pasadena, Calif., manages the
Cassini mission for NASA's Office of Space Science, Washington, D.C.

Cassini Outreach
Cassini Mission to Saturn and Titan
Jet Propulsion Laboratory
California Institute of Technology
National Aeronautics and Space Administration

ESA finds a black-hole flywheel in the Milky Way

Far away among the stars, in the Ara constellation of the southern sky,
a small black hole is whirling space around it. If you tried to stay
still in its vicinity, you couldn't. You'd be dragged around at high
speed as if you were riding on a giant flywheel. In reality, gas
falling into the black hole is whirled in that way. It radiates energy,
in the form of X-rays, more intensely than it would do if space were
still by tapping into the black hole's internal energy stream.

Read more about this at:
http://sci.esa.int/content/news/index.cfm?aid=1&cid=1&oid=29877

WHERE ON EARTH CAN YOU SEE PLANETARY SPACECRAFT?

2002 is a special year for NASA's Jet Propulsion Laboratory, Pasadena, Calif.,
and for space enthusiasts worldwide.

"This year marks the 40th anniversary of planetary exploration," said Anita Sohus,
JPL's museum liaison. "The celebration is widespread and space aficionados now have
the opportunity to see exhibits throughout California and the country that feature products
from JPL."

A full-scale replica of the Saturn-bound Cassini spacecraft is on display at the
California Science Center in Los Angeles. The spacecraft is the centerpiece of the newly
reopened Air and Space Gallery. Rounding out the display are full-scale models of the
Mars Viking lander (1976), Mariner 4 (first U.S. spacecraft to fly by Mars, in 1965) and
Explorer 1, America's first spacecraft (1958). The permanent exhibit opened March 9.
For more information visit
www.casciencectr.org .

The Chabot Space and Science Center in Oakland, Calif., features "Spaceflight:
Journey to the Stars" through June 9, 2002. Visitors can see models of the Cassini,
Stardust and Mars Odyssey spacecraft. The display also includes a model of a small
rover, or nanorover, like one that may someday land on an asteroid or other solar system
body. For more information, visit
http://www.chabotspace.org/visit/exhibits.asp .

An exhibit at the Tech Museum of Innovation in San Jose, Calif., features an
ultrasonic drill developed by JPL senior research scientist Dr. Yoseph Bar-Cohen and
Cybersonics, Inc. During future space missions, the device could extract samples using
lightweight landers with robotic arms and small rovers that roam the surface of an
asteroid or planet. With the help of docents, visitors can operate the drill at the
"Curiosity Counter." For more information visit
http://www.thetech.org/ .

"Footsteps Through Time," an exhibit at San Diego's Museum of Man, displays
videos of JPL technology innovations with applications to health care, the environment,
communications, education, transportation and computer technology. They include
infrared cameras that can be used to detect breast cancer, as well as inflatable membranes
that form large spaceborne telescopes. For more information visit
www.museumofman.org .

Many space-themed exhibits are geared toward children. At Kidspace, an
interactive children's museum in Pasadena, Calif., children can view a model of a Ranger
spacecraft. The Ranger missions in the 1960s provided high-quality pictures of the moon.
These images were used for scientific study and selection of landing sites for the manned
Apollo missions.

Children and adults visiting Disneyland, in Anaheim, Calif., can experience space
exploration at an exhibit in Tomorrowland, featuring a model of the Sojourner rover that
landed on Mars in 1997, as well as Explorer 1 and Pioneer 4 spacecraft models.

Space enthusiasts in many other parts of the country can see JPL products in
museums and displays.

* In Washington, D.C., the National Air and Space Museum has full-scale models
of JPL spacecraft, including Voyager and Explorer 1. For more info, visit
http://www.nasm.si.edu/galleries/gal111/universe/etu_artifacts.htm .

* At the National Mall in Washington, D.C. visitors can roam a scale model of the
solar system, developed by the Challenger Center, the National Air and Space
Museum and NASA's Office of Space Science, Washington, D.C.. For more
information visit:
http://www.challenger.org/ .

* Also in Washington, D.C., JPL images from Mars Global Surveyor data and
Shuttle Radar Topography data are on display at National Geographic's
Explorer's Hall in the building's large display windows that face the street.
* A full-scale replica of Cassini is on loan to the Chicago Museum of Science and
Industry.

* Both the Kansas Cosmosphere in Hutchinson, and the Virginia Air and Space
Center in Hampton, display full-scale models of the Viking (Mars) lander.

* The American Museum of Natural History in New York City has added models of
the Stardust and Space Interferometry Mission spacecraft to the space gallery.

JPL is managed for NASA by the California Institute of Technology in Pasadena.
 

 

WHERE ON EARTH CAN YOU SEE PLANETARY SPACECRAFT?

2002 is a special year for NASA's Jet Propulsion
Laboratory, Pasadena, Calif., and for space enthusiasts
worldwide.

"This year marks the 40th anniversary of planetary
exploration," said Anita Sohus, JPL's museum liaison. "The
celebration is widespread and space aficionados now have the
opportunity to see exhibits throughout California and the
country that feature products from JPL."

A full-scale replica of the Saturn-bound Cassini spacecraft
is on display at the California Science Center in Los Angeles.
The spacecraft is the centerpiece of the newly reopened Air
and Space Gallery. Rounding out the display are full-scale
models of the Mars Viking lander (1976), Mariner 4 (first
U.S. spacecraft to fly by Mars, in 1965) and Explorer 1,
America's first spacecraft (1958). The permanent exhibit
opened March 9. For more information visit

www.casciencectr.org .

The Chabot Space and Science Center in Oakland, Calif.,
features "Spaceflight: Journey to the Stars" through June 9,
2002. Visitors can see models of the Cassini, Stardust and
Mars Odyssey spacecraft. The display also includes a model
of a small rover, or nanorover, like one that may someday
land on an asteroid or other solar system body. For more
information, visit

http://www.chabotspace.org/visit/exhibits.asp .

An exhibit at the Tech Museum of Innovation in San Jose,
Calif., features an ultrasonic drill developed by JPL senior
research scientist Dr. Yoseph Bar-Cohen and Cybersonics, Inc.
During future space missions, the device could extract samples
using lightweight landers with robotic arms and small rovers
that roam the surface of an asteroid or planet. With the
help of docents, visitors can operate the drill at the
"Curiosity Counter." For more information visit

http://www.thetech.org/ .

"Footsteps Through Time," an exhibit at San Diego's Museum
of Man, displays videos of JPL technology innovations with
applications to health care, the environment, communications,
education, transportation and computer technology. They include
infrared cameras that can be used to detect breast cancer, as
well as inflatable membranes that form large spaceborne
telescopes. For more information visit

www.museumofman.org .

Many space-themed exhibits are geared toward children. At
Kidspace, an interactive children's museum in Pasadena, Calif.,
children can view a model of a Ranger spacecraft. The Ranger
missions in the 1960s provided high-quality pictures of the moon.
These images were used for scientific study and selection of
landing sites for the manned Apollo missions.

Children and adults visiting Disneyland, in Anaheim, Calif.,
can experience space exploration at an exhibit in Tomorrowland,
featuring a model of the Sojourner rover that landed on Mars in
1997, as well as Explorer 1 and Pioneer 4 spacecraft models.

Space enthusiasts in many other parts of the country can see
JPL products in museums and displays.

* In Washington, D.C., the National Air and Space Museum has
full-scale models of JPL spacecraft, including Voyager and
Explorer 1. For more info, visit

http://www.nasm.si.edu/galleries/gal111/universe/etu_artifacts.htm .

* At the National Mall in Washington, D.C. visitors can roam a
scale model of the solar system, developed by the Challenger
Center, the National Air and Space Museum and NASA's Office of
Space Science, Washington, D.C.. For more information visit:

http://www.challenger.org/ .

* Also in Washington, D.C., JPL images from Mars Global
Surveyor data and Shuttle Radar Topography data are on display
at National Geographic's Explorer's Hall in the building's large
display windows that face the street.

* A full-scale replica of Cassini is on loan to the Chicago
Museum of Science and Industry.

* Both the Kansas Cosmosphere in Hutchinson, and the Virginia
Air and Space Center in Hampton, display full-scale models of the
Viking (Mars) lander.

* The American Museum of Natural History in New York City has
added models of the Stardust and Space Interferometry Mission
spacecraft to the space gallery.

JPL is managed for NASA by the California Institute of Technology
in Pasadena.

April 26, 2002

Because of the extraordinary opportunity to see all five naked-eye
planets at once, the Observatory has posted a set of charts that show
the western sky at two-day intervals through June 3 at:

http://www.GriffithObs.org/planets_daily.html

Use these charts to follow the planets night by night in weeks to come.

 NASA SCIENTISTS DISCUSS COMMERCIAL USES OF REMOTE-SENSING TOOLS

Satellite technologies that could lead to more effective monitoring of crops, natural resources and disease outbreaks will be the focus of the Space-Based Tools for Valley Economic Growth Conference on April 26 at the Castle Airport Aviation and Development Center in California's Central Valley.

Attendees will hear David Peterson, chief of NASA Ames Research Center's Earth Sciences Division, speak about NASA's geospatial technologies that have applications for agriculture and natural resource assessment.

"NASA's remote sensing data and models of the Earth system are being used to understand the entire Earth system and predict its response to natural and human-induced change," said Peterson. "These same tools can be applied to many practical applications, from weather prediction to disasters to agriculture and resources. What I hope to illustrate during the conference is how 'space based tools,' including commercial ones, can be used in a meaningful way by the end user community."

In addition to the introduction of NASA's latest developments, the audience also will be able to learn more about the licensing and commercialization of space innovations.

"NASA technologies and knowledge are valuable resources often overlooked by many traditional industries," said executive director of the Far West Regional Technology Transfer Center Ken Dozier. "New high-velocity markets demand that competitive firms examine all options, and hopefully, this event will begin a series of dialogs that will lead to economic development in the Merced community."

For more information regarding the Space-Based Tools for Valley Economic Growth event, contact the County of Merced at 209/385-7686.

 NASA Marshall Center boosts Alabama economy with $829 million in Fiscal 2001 expenditures

Editor's Note: This release is an annual roundup of information that is
intended for reporters and editors in the business and education beats.

NASA's Marshall Space Flight Center in Huntsville, Ala., contributed $829
million to Alabama's economy in fiscal year 2001 -- a 6 percent increase
over fiscal year 2000 spending - and significantly more than spending in any
other state.

Included in the 2001 spending was $247 million in salaries for civil service
personnel and related costs, as well as travel. Also included was $582
million spent on locally procured services, prime contractor and
subcontractor support, and local construction.

Since it was established in 1960, the Marshall Center has had budget
responsibility for more than $69 billion. When yearly figures are adjusted
for inflation, this total is equivalent to more than $169 billion in today's
dollar value.

In addition, during 2001, The Boeing Company spent approximately $94
million in NASA funding in North Alabama for International Space Station
hardware development.

Another $47 million was spent by the Marshall Center for NASA
programs where Marshall had a supporting role, and an additional $18 million
was spent on programs where Marshall performed work for other agencies.

Marshall received approximately 15.5 percent - or $2.2 billion - of NASA's
total budget of $14.3 billion during fiscal 2001. By program areas, 73
percent of Marshall's budget was spent for Human Exploration and Development
of Space, including Space Shuttle and Space Station activities; 26 percent
for Space Science, Earth Science, Aero-Space Technology and Biological &
Physical Research activities; and the about 1 percent was spent on Strategic
Support of Marshall Center programs.

Also in 2001, approximately $70 million in retirement annuities were paid to
2,460 Marshall retirees residing in Alabama. The 1,680 retirees in
Huntsville and Madison received $47 million of that amount.

Since the Marshall Center's creation, a total of $5.2 billion in federal
salaries have been paid. In 2001, Marshall civil service employees
collectively paid about $192 million in federal income taxes and about $7
million in Alabama state income taxes.

At the end of September 2001, Marshall's permanent and temporary civil
service employees totaled 2,740, including employees at resident offices at
prime contractor facilities and at NASA's Michoud Assembly Facility near New
Orleans.

Of that workforce, 2,262 were college graduates, with 1,487 holding
bachelor's degrees. There were 183 employees with doctorate degrees and 592
with master's degrees in the fields of engineering and science --
predominantly mathematics and physics - as well as business administration
and other disciplines.

During 2001, 23,653 contractor personnel were engaged in work for the
Marshall Center, including 3,264 in mission support, 11,141 on prime
contract work and 9,248 as subcontractors and vendors. Of the total, 6,878
worked in Alabama. Additionally, 463 contractors were associated with
International Space Station work being done by Boeing in Huntsville, and 802
jobs were related to other NASA work supported by Marshall.

Also during fiscal 2001, approximately 62,000 people toured Marshall,
including educators, conference and symposium visitors and news media.
Attendance at the U.S. Space & Rocket Center -- Marshall's official NASA
Visitor Center -- was 341,411 for the year.

In addition, Marshall's education programs reached more than 84,269 students
and 20,263 teachers and faculty representing all 50 states during the year.
And the Marshall Center donated $5.5 million in research equipment and made
some $203 million in grants, contracts and cooperative agreements through
its education programs. Marshall's education program also recorded 609
partnerships and collaborations with other federal, state and local
programs, professional societies, nonprofit organizations, industry and
contractor communities, and with all levels of the educational community,
but primarily secondary education.

Continuing its ongoing work in the community, Marshall employees and
retirees volunteered last year to participate in the NASA Project LASER
(Learning About Science, Engineering and Research) Program, serving locally
as speakers, tutors, consultants and science fair judges. Marshall's
Educator Resource Center also distributed more than 113,014 pieces of
NASA-produced materials to the 5,711 educators it contacted through
workshops, on-site visits and postal and electronic requests. Staff at the
Educator Resource Center developed and delivered 153 workshops and overviews
to 1,408 teachers and home-school parents. Additionally, NASA's education
programs reached more than 10.2 million participants electronically.

The Marshall Center also gives back to the community through monthly Red
Cross Blood Drives - collecting 959 pints of blood in fiscal 2001 from civil
service and on-site contractors - and by contributing to the Combined
Federal Campaign -- collecting $559,703 in fiscal 2001, of which $294,893
was designated to help agencies in Alabama.

As Marshall marks its 41st year in Alabama and looks to the future, the
Center continues its role as a vital contributor to America's future in
space -- as well as to the economy of Huntsville and the state.

The Web

News release
http://www1.msfc.nasa.gov/NEWSROOM/news/releases/2002/02-098.html

 NATO picks promising pollution solution at
NASA,s Marshall Center for pilot study program

A project to treat groundwater and soil contamination at NASA,s Marshall
Space Flight Center in Huntsville, Ala., has attracted international
attention and been added to a pilot program sponsored by the North Atlantic
Treaty Organization (NATO).

The NATO Committee on the Challenges of Modern Society has picked one of the
Marshall Center,s in-situ remediation projects as one of just four worldwide
for further study and evaluation.

The Marshall Center studies are evaluating various technologies that can be
used at locations where hazardous materials or their residues are present in
the soil, subsoil and ground water. In this case, the focus is on removing
chlorinated volatile organic compounds from soils and ground water. This
contamination occurred from former waste management activities at the
facility before the potentially harmful results of such activities were
known.

In 1994, the U.S. Environmental Protection Agency (EPA) placed the Marshall
Center on the National Priorities List of sites eligible for cleanup under
the Superfund, an environmental program managed by the EPA to clean up
hazardous waste sites throughout the United States. The Marshall Center
studies are part of a process to identify, investigate, sample and restore
67 sites at Marshall where hazardous material was used. Since 1994, the
Marshall Center has spent an estimated $24 million on identifying,
investigating, sampling and restoring the sites.

The project selected by the NATO committee involves injection into the
ground of zero-valent iron powder - small solid iron particles -- in slurry
form using the Ferox sm process patented by ARS Technologies Inc., of
Highland Park, N.J., an environmental engineering firm.

These chemical reduction pilot tests are to be conducted beneath two
contaminated areas and are directed primarily at the treatment of
trichloroethene, a solvent that was used to clean rocket engines, in the
sub-surface soil and water. Investigations indicate that there are man-made
chemicals, like these solvents, still present in the water. These types of
contaminants are heavier than water and will keep moving through the
subsurface until they find a resting spot. Along the way they can also leave
small deposits at various depths, a result referred to as residual
contamination.

The Marshall Center,s Environmental Engineering Department developed and
implemented the remediation project in collaboration with CH2M HILL, an
international consulting engineering and project delivery firm headquartered
in Greenwood Village, Colo.

The study,s focus is on treatment of naturally oxygenated, contaminated
groundwater within an interval area called the rubble zone - a transitional
area between the clay soil and the limestone bedrock -- as well as on
treatment of the clay soil above the rubble zone where there is a
significant amount of contamination.
In one area, designated SA-2, trichloroethene groundwater contamination was
as high as 70 milligrams per liter. The federal standard for allowable
groundwater contamination of this substance is .005 milligrams per liter.

The SA-2 site is in a test area where in the 60,s and 70,s rocket
engine parts were routinely cleaned following tests. Unexploded ordnance
remaining from the World War II era was also present in the area,
eliminating the simpler option of doing a general treatment of the entire
contaminated area. Therefore, the approach taken was to inject zero-valent
iron powder where possible in the most contaminated areas. Then overlapping
injections were inserted into areas where water would naturally flow,
creating a treatment zone for untreated water to flow through. Monitoring of
the area after the injections showed contaminant concentrations in the
affected area were reduced by more than 90 percent.

Monitoring results at another site, called SA-12, near a building
where routine cleaning and degreasing of parts occurred (during development
of the U.S. space program) were not as encouraging. Much higher levels of
contamination than anticipated were found in this area that contains
trichloroethene with some perchloroethene and Freon in both saturated and
unsaturated zones.

During the first tests unexpectedly high SA-12 trichloroethene
concentrations -- approximately 350 milligrams per liter in the groundwater
and 46 milligrams per kilogram in the unsaturated zone -- were encountered.
The zero-valent iron powder injection was used for this area because of the
groundwater depth and the presence of underground utilities in the area.

It was determined that not enough of the slurry was injected for the
conditions being encountered. Therefore, follow-up laboratory tests were
conducted to re-assess the use of the zero-valent iron powder slurry
injections. Results indicate that the conditions at SA-12 are potentially
treatable with this approach. However, other types of treatment are also
under consideration.

Additional information about the project can be obtained from Amy
Keith, a Marshall Space Flight Center environmental engineer, (256)
544-7434, by e-mail: Amy.Keith@msfc.nasa.gov or from Bill McElroy, project
manager, at CH2M HILL, (352) 335-7991, or by e-mail: bmcelroy@ch2m.com.

To learn more about the technology, visit the ARS Technologies Web
site at:
http://www.arstechnologies.com.

 HELIOS ENERGY STORAGE SYSTEM PASSES MAJOR FUNCTIONAL TEST

In a major breakthrough which met a NASA performance requirement,
engineers from AeroVironment, Inc., and NASA have successfully
completed functional tests of a prototype regenerative Energy Storage
System for the Helios Prototype solar-powered aircraft.

The prototype system, housed within a pod that is designed to replace
one of the existing landing gear pods, contains a hydrogen-oxygen
regenerative fuel cell system that could be used to power the Helios
aircraft through the night in future flight demonstrations. The
energy storage system is the crucial element required to enable a
solar-powered aircraft to fly longer than a single day and
potentially for unlimited duration.

The energy storage system is based on proton exchange membrane (also
known as polymer electrolyte membrane) fuel cell technology now
rapidly emerging in automotive applications. The system is designed
to capture excess electric power produced by the Helios Prototype's
solar arrays during daytime flight and use it to electrolyze water
into its constituent gases, hydrogen and oxygen. These gases would
be stored under pressure and recombined in a fuel cell, producing
electricity as a byproduct to enable night flight.

The recently completed tests, conducted at National Technical Systems
in Saugus, Calif., climaxed more than two years of development work
and demonstrated the viability of a flight-configured,
hydrogen-oxygen aerospace regenerative fuel cell energy storage
system. During the simulated day portion of the test, the prototype
system absorbed 16 kilowatts of electrical energy for a period of
about 5.5 hours until the storage tanks were fully charged by the
electrolyzer. During the simulated night phase of testing, gas was
discharged from the tanks over a period of about five hours into the
fuel cell stack, producing up to 4.6 kW.

The prototype tests were conducted at sea level conditions with a
system that, although not yet as light as will be required for flight
on the Helios Prototype, has the essential attributes to fulfill the
form, fit and function requirements of a flightworthy energy storage
system.

"The significance of this system cannot be overstated," said John Del
Frate, solar aircraft project manager at NASA Dryden Flight Research
Center. "A flight-weight energy storage system not only gives Helios
the ability to fly through the night, but eventually the capability
to fly continuously as a stratospheric platform with its duration
limited only by the reliability of onboard systems."

"The Helios project office believes this may be the first
demonstration of a portable high power regenerative energy storage
device based on environmentally friendly fuel cell technology," Del
Frate commented. "The new technology demonstrates an energy storage
density better than double the most advanced secondary battery
systems yet devised.

"This lightweight portable regenerative energy storage technology can
also be configured and scaled for non-aircraft applications," he
added. "Some of those applications include NASA space exploration and
planetary surface power, electric vehicles, and both fixed and
portable solar power on Earth."

The completion of this effort successfully fulfilled a milestone
established under NASA's Environmental Research Aircraft and Sensor
Technology (ERAST) project, which is managed at NASA Dryden. The
Helios Prototype met another ERAST milestone last August when it flew
to an unofficial world altitude record for non-rocket-powered
aircraft of 96,863 feet near Hawaii and maintained stable horizontal
flight above 96,000 feet for more than 40 minutes.

The energy storage system design team was led by AeroVironment, with
technical assistance from NASA Dryden Flight Research Center at
Edwards, Calif., and NASA Glenn Research Center, Cleveland, Ohio.

Still photos and video footage of the Helios Prototype solar aircraft
and graphic illustrations of the Helios' energy storage system are
available from the Dryden Public Affairs Office to support this
release. Still photos of the aircraft are available on the NASA
Dryden Flight Research Center Internet web site, URL:

http://www.dfrc.nasa.gov/gallery/photo/Helios/index.html

 The Next Four Weeks on Galileo
April 22 - May 19, 2002

The pace with which Galileo is receding from Jupiter is slowing now, as the
spacecraft stretches out towards its most distant point in the orbit, which
it will reach in early June. During these four weeks, the distance from the
spacecraft to Jupiter increases from 320 to 342 Jupiter radii (22.9 million
to 24.5 million kilometers or 14.2 million to 15.2 million miles).

Diagnostic work continues as we attempt to resolve an anomaly seen in the
on-board tape recorder during the routine maintenance activity on April 12.
Since the playback of all of the data from the January Io flyby is now
complete, we can keep the recorder in an inactive state without losing
science data. A deliberate approach to understanding and solving the
problem is called for. The important point is to have a fully functional
tape recorder in time to support the November flyby of the small inner
moon, Amalthea.

Routine hardware maintenance activities for the spacecraft this month
include one exercise of the propulsion thruster system on May 10. Also
included is another exercise of the tape recorder on May 12. If the ongoing
diagnostic work indicates that the exercise is unadvisable, that activity
can be cancelled pending resolution of the problem.

On Saturday, May 4, the spacecraft will turn in place by just over 4
degrees to keep the communications antenna pointed towards Earth.

With the spacecraft well outside the magnetosphere of Jupiter on the
sunward side of the planet, continuous data collection by the Magnetometer,
the Dust Detector, and the Extreme Ultraviolet Spectrometer instruments
provides scientists with information about the interplanetary medium.

For more information on the Galileo spacecraft and its mission to Jupiter,
please visit the Galileo home page at one of the following URL's:

http://galileo.jpl.nasa.gov
http://www.jpl.nasa.gov/galileo

 HUBBLE UNCOVERS OLDEST "CLOCKS" IN SPACE TO READ AGE OF UNIVERSE

Pushing the limits of its powerful vision, NASA's Hubble Space Telescope
has uncovered the oldest burned-out stars in our Milky Way Galaxy. These
extremely old, dim stars provide a completely independent reading of the
universe's age without relying on measurements of the universe's
expansion. The ancient white dwarf stars, as seen by Hubble, turn out to
be 12 to 13 billion years old. Because earlier Hubble observations show
that the first stars formed less than 1 billion years after the
universe's birth in the big bang, finding the oldest stars puts
astronomers well within arm's reach of calculating the absolute age of
the universe.

To see and read more about this, please click on:
http://oposite.stsci.edu/pubinfo/pr/2002/10
http://oposite.stsci.edu/pubinfo/latest.html
http://oposite.stsci.edu/pubinfo/pictures.html and
http://hubblesite.org/go/news

The Space Telescope Science Institute (STScI) is operated by the
Association of Universities for Research in Astronomy, Inc. (AURA),
for NASA, under contract with the Goddard Space Flight Center,
Greenbelt, MD. The Hubble Space Telescope is a project of international
cooperation between NASA and the European Space Agency (ESA).

 Fabrication of EuroMARS Begins!

The fabrication of the European Mars Analog Research Station
(EuroMARS) has begun in earnest. The work, led by Project Architect
Frank Schubert and funded by Starchaser Industries and the United
Association of Plumbers and Pipefitters (UA), is being done on the
premises of the Rio Grande company in Denver, Colorado. Fabrication
is expected to be complete by the end of May 2002, after which the
station will be put on display in a major public exhibit in the
United States. It will then be shipped to Europe for deployment in
the field in the Spring of 2003.

Several sites are being considered for the EuroMARS, with Iceland as
the current leading candidate. Deployed there, the EuroMARS will
provide an opportunity for European and other researchers to engage
in a substantial program of Mars exploration operations research,
complementing the work the Mars Society will continue to do at its
Flashline Mars Arctic Research Station on Devon Island and the Mars
Desert Research Station in southern Utah. The Mars Society plans to
follow the building of the EuroMARS with a fourth station located in
the Australian desert, which is the site of the discovery of the
oldest known fossils of microscopic life on Earth.

A photograph of the EuroMARS in the process of fabrication can be
viewed on the Mars Society website at www.marssociety.org. More
photos will be posted as construction proceeds.

To find out more about the Mars Society, visit our website at
www.marssociety.org. Or contact info@marssociety.org.

 NEW MEXICO MESA STUDENTS VISIT KSC

High school seniors from New Mexico took over the Kennedy Space Center Visitor Complex last week to question a number of KSC employees about everything from career paths to balancing personal and professional roles.

External Relations and Business Development Director JoAnn Morgan and Education Programs and University Research Division Chief Pam Biegert welcomed the 87 New Mexico Mathematics, Engineering and Science Achievement (MESA) Program participants.

The students also listened to lectures, toured the space center, participated in student educational workshops at the Center for Space Education, and witnessed the landing of the Space Shuttle Atlantis following its STS-110 mission.

"I'm just so excited to see what's out here," said Valerie Salim, a student at Rio Grande High School in Albuquerque. "I plan to spend my four days in Florida looking for new career ideas."

The visit is part of the year-round, nonprofit New Mexico MESA program. The national initiative promotes educational enrichment for pre-college students from historically underrepresented ethnic groups. Starting in middle school, MESA prepares students for college majors in mathematics, engineering, science and related fields. The MESA program receives financial support from the state of New Mexico, numerous other state and national corporations and foundations, federal agencies, and private donations.

"I'd like to do something involving biology and engineering-maybe a physical therapist for astronauts," said Jonathan Vigil from Robertson High School, Las Vegas, Nev. "I'm also enjoying the weather and learning about the employees' extraordinary accomplishments."

Living in New Mexico is not the only acceptance criteria. The visiting seniors were a selected group who earned the incentive field trip to KSC based upon grades, completion of four years of high school math and science classes (which exceeds the required graduation minimum), participation in fields trips and community volunteer projects, and a career interest in NASA. (Historically, 98 percent of participants go on to college.)

"The number of students in college earning math, science, technology or engineering degrees continues to decline for U.S. students. But the number of jobs in these fields that need to be filled continues to increase," said Pre-College Programs Lead Steve Dutczak. "A major segment of pre-college students are the historically under-represented ethnic groups. It is to this group that programs like MESA offer the way to help fill the future needs of the scientific and technical world."

MESA students at KSC represented six regions of New Mexico-from the most northern to the most southern parts of the state, as well as some surrounding areas. Many of the students took part in fundraisers and worked various jobs to help pay for their trip to Florida.

"MESA students are our future engineers, scientists, and technicians," said Karroll Purer, KSC education specialist. "Many have faced challenges, such as financial constraints and being first generation college students. MESA students are achievers!"

 NASA'S AQUA SPACECRAFT TO STUDY EARTH'S WATER CYCLE

NASA's mission to understand and protect our home planet will mark a major milestone
this spring with the launch of the Aqua satellite, carrying the NASA Jet Propulsion Laboratory-
managed Atmospheric Infrared Sounder instrument. Aqua, due to bring us unprecedented
insight into our world's global water cycle, is the latest sibling in a family of Earth Observing
System satellites dedicated to studying Earth and expanding our knowledge of global climate
change.

The primary role of Aqua, as the name implies, is to gather information about water in
the Earth's system. Equipped with six state-of-the-art instruments, Aqua will collect data on
global precipitation, evaporation and the cycling of water.

During its six-year mission, Aqua will gather information on changes in ocean circulation
and study how clouds and surface water processes affect our climate. This information will help
scientists better understand how global ecosystems are changing, and how they respond to and
affect global environmental change.

JPL's Atmospheric Infrared Sounder will measure Earth's atmosphere and surface; this
will allow scientists to improve weather prediction and to observe changes in Earth's climate.

"Aqua will provide unprecedented information on the global water cycle. The spacecraft
will enable operational agencies to create more accurate weather forecasts in the future," said Dr.
Ghassem Asrar, associate administrator for NASA's Earth Science Enterprise, NASA
Headquarters, Washington, D.C.

"Aqua will observe our Earth's oceans, atmosphere, land, ice and snow covers and
vegetation," said Dr. Claire Parkinson, the Aqua project scientist at NASA's Goddard Space
Flight Center, Greenbelt, Md. "This comprehensive approach enables scientists to study the
interactions among key elements of the Earth system so as to better understand our planet."

Aqua is expected to launch no earlier than May 2 from Vandenberg Air Force Base,
Calif. on a Boeing Delta-7920-10L expendable launch vehicle. The 10-minute launch window
opens at 2:55 a.m. Pacific Time (5:55 a.m. Eastern Time). Aqua will fly at an altitude of
approximately 705 kilometers (438 miles) above Earth in a near polar and sun synchronous orbit.

Aqua is the sister satellite to NASA's Terra spacecraft, launched in December of 1999.
Aqua will cross the equator daily at 1:30 p.m. as it heads north. The early afternoon observation
time contrasts with the Terra satellite, which crosses the equator between 10:30 and 10:45 a.m.
daily. The two satellites, Aqua's afternoon observations and Terra's morning observations, will
yield important insights into the "diurnal variability," or the daily cycling of key scientific
parameters such as precipitation and ocean circulation.

Aqua is a joint project between the United States, Japan and Brazil. The United States
provided the spacecraft and four of Aqua's six scientific instruments. NASA's Goddard Space
Flight Center provided the Moderate Resolution Imaging Spectroradiometer and the Advanced
Microwave Sounding Unit. JPL provided the Atmospheric Infrared Sounder, and NASA's
Langley Research Center, Hampton, Va., provided the Clouds and the Earth's Radiant Energy
System instrument.

Japan's National Space Development Agency provided the Advanced Microwave
Scanning Radiometer. The Instituto Nacional de Pesquisas Espaciais (the Brazilian Institute for
Space Research) provided the Humidity Sounder for Brazil.

Aqua is part of NASA's Earth Science Enterprise, a long-term research effort dedicated to
understanding and protecting our home planet. Through the study of Earth, NASA will help to
provide sound science to policy and economic decision makers so as to better life here, while
developing the technologies needed to explore the universe and search for life beyond our home
planet. More information about NASA's Earth Science Enterprise can be found at:

http://www.earth.nasa.gov .

More information about the Aqua program is available at:

http://aqua.nasa.gov .

More information about the Atmospheric Infrared Sounder can be found at:

http://www-airs.jpl.nasa.gov/ .

JPL is a division of the California Institute of Technology in Pasadena.

 http://www.estec.esa.nl/conferences/hvis2003/index.html

Third Announcement and Final Call for Papers

HVIS 2003

Hosted by the European Space Agency's Research & Technology Centre (ESTEC)

7-10 April 2003
Grand Hotel Huis ter Duin
Noordwijk, The Netherlands

The Hypervelocity Impact Symposium is a regular event that is dedicated to
enabling and promoting an understanding of the basic physics of high
velocity impact and related technical areas. This international event
provides a forum for researchers to share and exchange a wealth of knowledge
through oral and poster presentations and technical exhibits.

HVIS 2003 will be the eighth symposium in a series. It will be hosted by
ESTEC and held in Noordwijk, The Netherlands. The dates of the conference
coincide with the tourist season in the bulb district and Noordwijk is
located in this district.

The technical sessions will be held at the Grand Hotel Huis ter Duin,
Noordwijk during April 7-10, 2003.

All papers presented at the Symposium will be published in a refereed volume
of the International Journal of Impact Engineering.

Symposium topics

* Hypervelocity phenomenology studies
* High-velocity launchers and diagnostics
* Spacecraft meteoroid and debris shielding and failure analysis
* Material behaviour under high velocity impacts
* Fracture and fragmentation
* High velocity penetration mechanics and target response
* Analytical and numerical simulation techniques
* Asteroid impact and planetary defence technology
* Penetration mechanics of shaped charges and explosively formed
penetrators
* Planetary impacts

Call for papers

Abstract of proposed papers are solicited from those actively interested and
involved in hypervelocity impact. The preferred method of submitting
abstracts is using the form on this web site.

If it is not possible to submit your abstract through the web site, it may
be submitted by e-mail as an attachment or by mailing a printed copy, along
with a diskette copy to the following address:

HVIS 2003
ESTEC Conference Bureau
Postbus 299
NL-2200 AG Noordwijk
The Netherlands
Tel: +31-71-565-5005
Fax: +31-71-565-5658
E-mail: confburo@esa.int

Abstract must be received no later than May 15, 2002

Authors will be notified in June 2002 of the review decision for their
proposed paper. An author's packet will be mailed to authors whose abstracts
are accepted.

Acceptance of an abstract indicates preliminary acceptance of a paper for
publication in the International Journal of Impact Engineering, subject to a
technical peer review with final recommendation on the basis of such review.

Abstract Guidelines

* Abstracts should be at least 500 words plus figures and references.

* The official language is English.

* Abstracts must be cleared for public release with unlimited
distribution. An abstract booklet of accepted papers will be
distributed at the symposium.

* Include name, address, affiliation, phone number, fax number and e-mail
address of the primary author.

* Indicate author's preference for oral or poster presentation

* Indicate appropriate topic.

Commercial Exhibits

Commercial Exhibits will be on display during the entire symposium giving
attendees ample opportunity to meet with company representatives. Companies
interested in exhibiting should contact the ESTEC Conference Bureau, P.O.Box
299, 2200 AG Noordwijk, NL. Tel.. +31 71 5655005, Fax: +31 71 5655658,
e-mail: confburo@esa.int

Schedule

August 2001 Abstract 1st call
January 2002 Abstract 2nd call
May 2002 Abstracts due
June 2002 Notification to authors
September 2002 Papers due for review
October 2002 Preliminary Programme and Registration details
February 2003 Deadline for Hotel Reservation
March 2003 Final papers due
April 2003 HVIS Symposium

Distinguished Scientist Award HVIS 2003

The Hypervelocity Impact Society makes an award for Distinguished Scientist
at each of its Symposia.

The next Symposium is to be held in Noordwijk, The Netherlands in April 2003
and the Society is seeking nominations for this prestigious award.

The award for Distinguished Scientist is based upon the following criterion:

* Significant and lasting contributions to the field of hypervelocity
science.

The award is normally given to an individual but a research team of two
individuals is also eligible.

Formal letters of nomination are invited from the HVIS Membership and anyone
who has been involved in hypervelocity science.

In preparing the letter of nomination, which should include supporting
information about the candidate, proposers may wish to address the
candidate's technical recognition within the community, the importance of
their work and its contribution to hypervelocity science and their personal
contribution and service to the Society.

Written nominations can be emailed to the following members of the Society:

* Ian Cullis, email: igcullis@qinetiq.com
* Gene Hertel, email: esherte@sandia.gov
* Volker Hohler, email: hohler@emi.fhg.de
* Tim Holmquist, email: tjholm@networkcs.com

The closing date for nominations is December 2002.

Best Paper Award HVIS 2003

At the forthcoming HVIS 2003 an award will be made for the best paper
submitted for presentation to the Symposium.

The selection criteria are:

* Originality
* Difficulty of Research
* Importance of Research
* Excellence of the Written Paper.

The selection of the best paper will be made at the manuscript review
meeting.

All authors are invited to submit a paper worthy of inclusion in the Best
Paper Review.

Alex Charters Student Scholars Program

http://www.hvis.org/students.html

HVIS Web site

http://www.hvis.org/

Travel , Accommodation and Registration

Air travel: Noordwijk is located 30 km south of Amsterdam. The nearest
international airport is Schiphol-Amsterdam Airport, detailed information is
available at www.schiphol.nl.

Accommodations: The host hotel for this meeting is the Grand Hotel Huis ter
Duin in Noordwijk (www.huisterduin.com). special rates for the Conference
hotel and other hotels in the Noordwijk area are negotiated.

Further details on registration and hotel accommodation will be published in
the preliminary programme that will be issued in October 2002.

Symposium Chairmen

Michel Lambert
ESA/ESTEC
michel.lambert@esa.int
phone: 00 31 71 565 3434

Dr. Eberhard Schneider
EMI
schneider@emi.fhg.de
phone: 0049 761 2714 326

Technical Chairmen

Frank Schaefer
EMI
schaefer@emi.fhg.de
phone: 0049 761 2714 421

Peter Buchwald
ESA/ESTEC
peter.buchwald@esa.int
phone: 00 31 71 565 3396

Technical Committee

Detlef Alwes DLR
Charles Anderson Southwest Research Institute
Werner Arnold EADS-TDW
Stefan Bless Institute for Advanced Technology
Dennis Baum Lawrence Livermore National Laboratories
Lalit Chhabildas Sandia National Laboratories
Eric Christiansen NASA Johnson Space Center
Jeanne Crews NASA Johnson Space Center
Ian Cullis Defence Evaluation Research Agency
Roberto Destefanis Alenia
Steve Evans NASA Marshall Space Flight Center
Eric Fahrenthold University of Texas at Austin
Harry Fair Institute for Advanced Technology
Walter Flury European Space Agency
Joseph Foster U.S. Air Force - Eglin AFB
William Gooch Army Research Laboratory
Donald Grosch Southwest Research Institute
Colin Hayhurst Century Dynamics
Eugene Hertel Sandia National Laboratories
Stefan Hiermaier Ernst Mach Institut
Volker Hohler Ernst Mach Institut
Tim Holmquist Network Computing Services Inc.
Reiner Huehn BWB
Eduard Igenbergs Technical University Muenchen
Andrey Ioilev RFNC-VNIIEF
Masahide Katayama CRC Research Institute
Thomas Kenkmann HU-Berlin
Justin Kerr NASA Johnson Space Center
Erhardt Lach Institut Saint Louis
Christian Loupias Centre d'Etudes de Gramat
Jean Claude Mandeville DERTS
Tony McDonnell Open University
Scott Mullin Southwest Research Institute
Michael Normandia Army Research Laboratory
Dennis Orphal International Research Associates Inc.
Andrew Piekutowski University of Dayton Research Institute
Hans-Guenther Reimerdes RWTH Aachen
Andre Rolfo CNES
Hans Werner Schmidt BWB
William Schonberg University of Missouri - Rolla
Jean Marc Sibeaud Centre d'Etudes de Gramat
Emma Taylor Astrium
Klaus Thoma Ernst Mach Institut
Joel Williamsen University of Denver Research Institute
Jerome Yatteau Applied Research Associates Inc.

 KSC TESTS SMART UMBILICAL MATING SYSTEM FOR NASA'S SPACE LAUNCH INITIATIVE

Engineers at Kennedy Space Center are testing the newest in umbilical technology in support of NASA's Space Launch Initiative (SLI)-a technology development effort to establish reliable, affordable space access.

"Umbilicals are the lifeline for any Space Launch Vehicle," said Warren Wiley, KSC's SLI program manager. "Fluids including propellants, pressurization gasses, and cooling systems, power, communications, and instrumentation readings all flow through the umbilical. They are large devices that are manpower intensive to mate, test, and maintain."

Traditional umbilical systems release at vehicle lift-off (T-0) and can also take extensive connection time-reducing potential flight rate. The Smart Umbilical Mating System, three years in development by Rohwetter Systems, Oviedo, Fla., and NASA will serve as a modern, next-generation umbilical system.

"The concept is to replace a T-0 umbilical with an automated umbilical which has a mate, demate and remate capability," said Tom Lippitt, KSC's spaceport engineering and technology lead engineer. "The ability to quickly and reliably mate and demate umbilical connectors under automated control, along with remote connection verification would reduce the time and labor hours required to prepare for launch. The Smart Umbilical Mating System will also be used as a testbed for quick disconnect development and for advance control and leak detection technologies."

The system will be used as a development tool for future launch vehicle technology development. According to Lippitt, several technologies being developed relate to umbilicals, such as ice suppression, leak sensing, quick disconnects and others. By using the Smart Umbilical Mating System, the new technologies can be tested in cryogenic conditions.

"In addition to ground-based applications, planetary systems and rovers will require umbilical mating for propellant loading and electrical and data connection," said Lippitt. "The technology developed as part of this project may be applied to develop simple, reliable, self-sufficient mating. Some of this work will be required to make certain missions and systems feasible such as the Mars methane fueled rovers."

Kennedy Space Center is responsible for managing SLI's Ground Operations Project-NASA's effort to reduce the risk associated with developing a second generation Reusable Launch Vehicle (RLV) by defining, developing and testing technologies needed to safely and cheaply access space.

"The project will address the SLI goals of reducing operating costs by reducing the maintenance and manpower needed to do the connections and increase safety by automatically performing hazardous tasks and reducing potential failure modes," said Wiley.

Space Launch Initiative is a NASA wide research and development program managed by the Marshall Space Flight Center, Huntsville, Ala. It is designed to improve safety, reliability and cost effectiveness of space travel for second generation reusable launch vehicles.

April 25, 2002

 NASA AMES ASTROBIOLOGY EXPLORER TELESCOPE CHOSEN FOR FEASIBILITY STUDY

A mission proposal from NASA Ames Research Center to measure the
pre-biological chemical building blocks of life in deep space has
been selected as a next-mission candidate under NASA'S Explorer
Program -- a roster of low-cost, focused next-generation spacecraft.

The Astrobiology Explorer, known as ABE, has a hydrogen ice-chilled
telescope that will search for interstellar organic compounds, such
as carbon-containing ices, dust and molecules, throughout the
universe. If chosen, the $180 million mission will fly as early as
2007. The ABE spacecraft will be put into an orbit around the sun,
gradually drifting 14 million miles away from Earth during its
18-month mission lifetime.

"This is the next step," said Ames principal investigator Dr. Scott
Sandford. "We need an infrared telescope in space because we can't
measure signals at these wavelengths using even the largest
ground-based telescopes."

The ABE telescope must be chilled and put into space in order to
detect the very weak signals it seeks, which would otherwise be lost
in the flood of infrared radiation produced by the Earth's own
warmth. "It's as if we were trying to detect the light from a candle
that is held in front of a searchlight," Sandford added. "Chilling
the telescope and putting it in space is like turning off the
searchlight."

The telescope and its instruments will measure light at wavelengths
in the infrared spectrum, which are wavelengths about 10 times longer
than what the human eye can see, and that we experience as heat.

ABE's primary goal is to understand the molecular chemistry that
occurs in space, and to identify the molecules that are found in
different space environments. ABE observations also will provide new
insights into the physical nature of young stars, comets, galaxies
and other objects in the universe.

ABE's science team will look for the spectral signatures of complex
organic molecules and the simpler molecules from which they are
formed, such as water, ammonia and methanol. In recent laboratory
simulations of cold, space-like conditions, Sandford and other Ames
scientists found that organic molecules, including those necessary
for life, such as ketones and complex hydrocarbons, can be produced
in deep interstellar space.

One advantage ABE will have over previous infrared space
observatories, the researchers say, is its large, sensitive infrared
light detectors. These Ames-developed devices will allow researchers
to collect millions of pixels of information at once, much more than
previously.

"ABE will have three instruments called spectrometers, which will
slice up the light collected by the telescope," said Ames' Dr. Tom
Greene, ABE's mission architect. "The detectors in these
spectrometers will sense the unique infrared signatures of many
atoms, molecules and dust grains."

Sylvia Cox and other Ames personnel will serve as members of the ABE team.
The team will partner with Ball Aerospace and Technologies Corp.,
which will build the instrument and spacecraft. A group of 18
scientists from Ames, as well as other U.S. and international
institutes, also will work on ABE.

NASA will select two of the Explorer mission proposals by early 2003 for full
development as Medium-class Explorer flights. The Explorer program is
managed by NASA's Goddard Space Flight Center, Greenbelt, Md., for
the Office of Space Science, Washington.

More information about ABE is available at:

http://www.astrochem.org/abe.html

More information about the Explorer program and the other selected
proposals is available at:

http://fpd.gsfc.nasa.gov/410/index.html

 New Chandra Results: The 2002 joint meeting of the American Physical
Society & the High Energy Astrophysics Division (AAS) met in
Albuquerque, New Mexico from April 20-23. New X-ray results from two
colliding galaxies and a bustling star-forming region were released:

**Arp 220**
When Worlds Collide: Chandra Observes Titanic Merger
NASA's Chandra X-ray Observatory has provided the best X-ray image yet
of two Milky Way-like galaxies in the midst of a head-on collision.
Since all galaxies - including our own - may have undergone mergers,
this provides insight into how the Universe came to look as it does today.
<
http://chandra.harvard.edu/photo/2002/1181/index.html >

**The Tarantula Nebula (30 Doradus)**
A Drama of Star Formation and Evolution
The Tarantula, also known as 30 Doradus, is in one of the most active
star-forming regions in our Local Group of galaxies. Massive stars are
producing intense radiation and searing winds of multimillion-degree gas
that carve out gigantic super-bubbles in the surrounding gas.
<
http://chandra.harvard.edu/photo/2002/0057/index.html >

===================================

** Operations CXO Status Report (Friday 04/19/02)
Last week the observing schedule was interrupted due to high radiation
associated with solar flare activity. The loads were halted on April 17
at 8:55am EDT through a ground command to execute the SI Safing SCS 107.

< http://chandra.harvard.edu/press/updates/update_041902.html >

===================================

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 JPL DEVELOPS NEW PORTABLE FUEL CELL TECHNOLOGY

NASA researchers have reached an important milestone in developing a portable energy
source that may someday give that hot pink, shades-wearing, drum-beating bunny a run for its
money.

A team of fuel cell experts at NASA's Jet Propulsion Laboratory, Pasadena, Calif., has
taken what have been traditionally large, bulky stacks of layered fuel cells and altered their
design dramatically. They have designed a compact, flat fuel cell, reducing its weight
substantially. The result is a portable fuel cell technology that may someday operate small,
portable electronic devices, such as cell phones, laptops, handheld organizers and camcorders,
for hours and even days at a time without recharging or using expensive, heavy batteries.

"This is a significant advance in fuel cell development because by going small, you make
the fuel cell portable and viable for use as a power source to operate small appliances that require
long operating time, such as a laptop," said Dr. S. R. Narayanan, fuel cell technical team lead at
JPL.

Work on the portable fuel cell technology is sponsored by a public company, TechSys,
Inc., Florham Park, N.J., through a technology affiliates agreement with JPL. By becoming a
technology affiliate member, TechSys, Inc., gained access to JPL engineers and technologists
who specialize in fuel cell technology development.

A major advantage of fuel cells over rechargeable batteries is that they can operate for
longer periods of time without recharging or interruption. "Instead of recharging your laptop
every two hours, imagine being able to use it for ten hours at a time," said Narayanan. Unlike
batteries, these fuel cells can be recharged almost instantaneously by refueling with liquid
methanol. Batteries contain toxic materials and must be disposed of properly.

A fuel cell works on the same principle as a battery but is continually fed with fuel. In
this new power source, methanol is put in on one side of the unit while air circulates on the other
side. Both are circulated past electrodes and converted to electricity. This process produces no
toxic emissions, only carbon dioxide and water as byproducts. Methanol, better known as
methyl alcohol, is a common, inexpensive chemical used, for example, in windshield washer
fluid.

Existing fuel cells typically operate at high temperatures, require bulky thermal insulation
and use hydrogen as their energy source. Much of their weight and size is due to the bipolar
plates needed to connect several cells to form a stack. JPL researchers have eliminated bipolar
plates and created what's called a monopolar pack, which is flat with the cells linked by
electrical interconnects.

To demonstrate the feasibility of the portable fuel cell technology, JPL developed a 5-
watt portable power unit. The power source uses the new lightweight monopolar flat pack
technology and is roughly the size of two paperback books standing tall, back-to-back. It
operates efficiently at ambient temperature without a fan, unlike conventional designs.

JPL engineers rigged a cell phone to this power unit and placed several phone calls as a
demonstration. They estimate that the 5-watts could simultaneously power five cell phones. The
system could be refueled instantly to extend the talk-time as long as needed.

Now that the concept of making a portable, flat stack has been demonstrated, the next
phase underway at JPL is to make it smaller, more robust and user-friendly.

JPL's fuel cell group has been working on direct methanol fuel cells since the early 1990s
and is credited with inventing the technology, largely under funding from the U.S. Defense
Advanced Research Projects Agency. The creation of the portable power source builds on that
work and experience.

TechSys, Inc., has the rights to an exclusive license on the development of this micro
direct methanol fuel cell technology from JPL's parent institution, the California Institute of
Technology, also in Pasadena. TechSys, Inc., intends to commercialize the JPL portable fuel cell
technology for civil and defense applications.

Through JPL's Technology Affiliates Program, large and small businesses can work with
JPL engineers to transfer technologies for commercial use. The program is just one of several
JPL technology transfer programs designed to bring the benefits of the space program to
American industry.

Caltech manages JPL for NASA.

 AN EARTH DAY PRESENT FROM SPACE: EUROPE AND ASIA'S WATERY GATEWAY

Considered to be the boundary between Europe and Asia, the Bosporus (Turkish
Bogazici) Strait connects the Black Sea with the Sea of Marmara in northwest Turkey. In
celebration of Earth Day, NASA has released a new shaded relief and radar image of this
geologically complex and historically rich region, taken by NASA's Shuttle Radar Topography
Mission in February 2000.

The image is available from NASA's Jet Propulsion Laboratory, Pasadena, Calif., on the
JPL Planetary Photojournal at:

http://photojournal.jpl.nasa.gov/cgi-bin/PIAGenCatalogPage.pl?PIA03349 .

The Bosporus Strait is depicted in the center of the view. The Black Sea at the top of the
image and Sea of Marmara below the center are colored blue, along with several large lakes.
The largest lake, to the lower right of the Sea of Marmara, is Iznik Lake.

The large city of Istanbul, Turkey is located on both sides of the southern end of the
strait. Its stronger reflection of radar causes it to appear as a brighter (light green to white) area
on the image. Istanbul is the modern name for a city with a long history, previously known as
both Constantinople and Byzantium. In 330 A.D., Constantine rebuilt Istanbul on the site of an
earlier Greek city as the capital of the Roman Empire. It later served as the capital of the
Byzantine and Ottoman empires until 1922.

The narrow Gulf of Izmit extends to the east (right) from the Sea of Marmara. On
August 17, 1999, a magnitude 7.4 earthquake, often called the Izmit or Kocaeli, Turkey
earthquake, heavily damaged the city of Izmit at the end of the gulf and killed at least 17,000
people. A previous earthquake under the Gulf of Izmit in 1754 killed at least 2,000 people. The
Izmit earthquake ruptured a long section of the North Anatolian Fault system from off the right
side of this image continuing under the Gulf of Izmit. Another strand of the North Anatolian
Fault system is visible as a sharp linear feature in the topography south of Iznik Lake. Surveys
measuring water depth in the area show that the North Anatolian Fault system extends beneath
and has formed the Sea of Marmara, in addition to the Gulf of Izmit and Iznik Lake. Scientists
are studying the North Anatolian Fault system closely to determine the risk of future large
earthquakes on the faults close to Istanbul.

Three visualization methods were combined to produce this image: shading and color
coding of topographic height, and radar image intensity. The shade image was derived by
computing topographic slope in the northwest-southeast direction. Northwest-facing slopes
appear dark and southeast-facing slopes appear bright. Color-coding is directly related to
topographic height, with green at the lower elevations, rising through yellow and brown to white
at the highest elevations. The shade image was combined with the radar intensity image to add
detail, especially in the flat areas.

The Shuttle Radar Topography Mission was flown aboard Space Shuttle Endeavour
February 11-22, 2000. It used modified versions of the same instruments that comprised the
Space Shuttle Imaging Radar-C/X-Band Synthetic Aperture Radar that flew twice on Endeavour
in 1994. The mission collected 3-D measurements of Earth's land surface using radar
interferometry, which compares two radar images taken at slightly different locations to obtain
elevation or surface-change information. To collect the data, engineers added a 60-meter
(approximately 200-foot) mast, installed additional C-band and X-band antennas, and improved
tracking and navigation devices. More information is available at:

http://www.jpl.nasa.gov/srtm .

NASA's Earth Science Enterprise is a long-term research and technology program
designed to examine Earth's land, oceans, atmosphere, ice and life as a total integrated system.

JPL is a division of the California Institute of Technology in Pasadena.

April 23, 2002

CONTOUR Ships to the Cape


NASA Comet-Chasing Spacecraft on Track for July 1 Launch
All packed up and ready for its long-awaited trip, NASA's CONTOUR spacecraft

left home in Maryland today for Cape Canaveral, Fla., site of its scheduled

July 1 launch toward an unprecedented comet study.
Secured in an air-ride, climate-controlled shipping container,

CONTOUR set out from NASA's Goddard Space

Flight Center in Greenbelt and will reach Cape Canaveral Air Force

Station/Kennedy Space Center later this week. CONTOUR -- short for Comet

Nucleus Tour -- had spent the past eight weeks being baked, frozen, spun,

shaken and probed in Goddard's test facilities, getting a dose of the

conditions it will face during launch and in space.
"Our spacecraft is ready and the team is anxious to start final preparations

for launch," says CONTOUR Project Manager Mary C. Chiu, of the Johns Hopkins

University Applied Physics Laboratory in Laurel, Md., which designed and

built the compact 8-sided, 6-foot by 7-foot spacecraft.
After a predawn launch aboard a Boeing Delta II rocket, CONTOUR will

encounter two very different comets as they zoom through the inner solar

system. From as close as 60 miles (about 100 kilometers) away, the

spacecraft will snap the sharpest pictures yet of a comet's nucleus, map the

types of rock and ice on the surface and analyze the surrounding gas and

dust. CONTOUR's target comets include Encke in November 2003 and

Schwassmann-Wachmann 3 in June 2006, though the mission team can steer the

solar-powered probe toward a scientifically attractive "new" comet should

the opportunity arise.
"CONTOUR will provide the most detailed data yet on these ancient building

blocks of the solar system," says Dr. Joseph Veverka, the mission's

principal investigator from Cornell University, Ithaca, N.Y. "By studying at

least two comets, we'll be able to assess their diversity and begin to clear

up the many mysteries of how comets evolve."
CONTOUR is part of NASA's Discovery Program of

lower-cost, highly focused space science investigations. APL manages the

mission for NASA and will operate the spacecraft. Veverka leads a team of 18

co-investigators from universities, industry and government agencies in the

U.S. and Europe. For more information on CONTOUR, visit
www.contour2002.org.

 

JPL DEVELOPS NEW PORTABLE FUEL CELL TECHNOLOGY

NASA researchers have reached an important milestone in developing a portable energy
source that may someday give that hot pink, shades-wearing, drum-beating bunny a run for its
money.

A team of fuel cell experts at NASA's Jet Propulsion Laboratory, Pasadena, Calif., has
taken what have been traditionally large, bulky stacks of layered fuel cells and altered their
design dramatically. They have designed a compact, flat fuel cell, reducing its weight
substantially. The result is a portable fuel cell technology that may someday operate small,
portable electronic devices, such as cell phones, laptops, handheld organizers and camcorders,
for hours and even days at a time without recharging or using expensive, heavy batteries.

"This is a significant advance in fuel cell development because by going small, you make
the fuel cell portable and viable for use as a power source to operate small appliances that require
long operating time, such as a laptop," said Dr. S. R. Narayanan, fuel cell technical team lead at
JPL.

Work on the portable fuel cell technology is sponsored by a public company, TechSys,
Inc., Florham Park, N.J., through a technology affiliates agreement with JPL. By becoming a
technology affiliate member, TechSys, Inc., gained access to JPL engineers and technologists
who specialize in fuel cell technology development.

A major advantage of fuel cells over rechargeable batteries is that they can operate for
longer periods of time without recharging or interruption. "Instead of recharging your laptop
every two hours, imagine being able to use it for ten hours at a time," said Narayanan. Unlike
batteries, these fuel cells can be recharged almost instantaneously by refueling with liquid
methanol. Batteries contain toxic materials and must be disposed of properly.

A fuel cell works on the same principle as a battery but is continually fed with fuel. In
this new power source, methanol is put in on one side of the unit while air circulates on the other
side. Both are circulated past electrodes and converted to electricity. This process produces no
toxic emissions, only carbon dioxide and water as byproducts. Methanol, better known as
methyl alcohol, is a common, inexpensive chemical used, for example, in windshield washer
fluid.

Existing fuel cells typically operate at high temperatures, require bulky thermal insulation
and use hydrogen as their energy source. Much of their weight and size is due to the bipolar
plates needed to connect several cells to form a stack. JPL researchers have eliminated bipolar
plates and created what's called a monopolar pack, which is flat with the cells linked by
electrical interconnects.

To demonstrate the feasibility of the portable fuel cell technology, JPL developed a 5-
watt portable power unit. The power source uses the new lightweight monopolar flat pack
technology and is roughly the size of two paperback books standing tall, back-to-back. It
operates efficiently at ambient temperature without a fan, unlike conventional designs.

JPL engineers rigged a cell phone to this power unit and placed several phone calls as a
demonstration. They estimate that the 5-watts could simultaneously power five cell phones. The
system could be refueled instantly to extend the talk-time as long as needed.

Now that the concept of making a portable, flat stack has been demonstrated, the next
phase underway at JPL is to make it smaller, more robust and user-friendly.

JPL's fuel cell group has been working on direct methanol fuel cells since the early 1990s
and is credited with inventing the technology, largely under funding from the U.S. Defense
Advanced Research Projects Agency. The creation of the portable power source builds on that
work and experience.

TechSys, Inc., has the rights to an exclusive license on the development of this micro
direct methanol fuel cell technology from JPL's parent institution, the California Institute of
Technology, also in Pasadena. TechSys, Inc., intends to commercialize the JPL portable fuel cell
technology for civil and defense applications.

Through JPL's Technology Affiliates Program, large and small businesses can work with
JPL engineers to transfer technologies for commercial use. The program is just one of several
JPL technology transfer programs designed to bring the benefits of the space program to
American industry.

 AN EARTH DAY PRESENT FROM SPACE: EUROPE AND ASIA'S WATERY GATEWAY

Considered to be the boundary between Europe and Asia, the Bosporus (Turkish
Bogazici) Strait connects the Black Sea with the Sea of Marmara in northwest Turkey. In
celebration of Earth Day, NASA has released a new shaded relief and radar image of this
geologically complex and historically rich region, taken by NASA's Shuttle Radar Topography
Mission in February 2000.

The image is available from NASA's Jet Propulsion Laboratory, Pasadena, Calif., on the
JPL Planetary Photojournal at:

http://photojournal.jpl.nasa.gov/cgi-bin/PIAGenCatalogPage.pl?PIA03349 .

The Bosporus Strait is depicted in the center of the view. The Black Sea at the top of the
image and Sea of Marmara below the center are colored blue, along with several large lakes.
The largest lake, to the lower right of the Sea of Marmara, is Iznik Lake.

The large city of Istanbul, Turkey is located on both sides of the southern end of the
strait. Its stronger reflection of radar causes it to appear as a brighter (light green to white) area on the image. Istanbul is the modern name for a city with a long history, previously known as both Constantinople and Byzantium. In 330 A.D., Constantine rebuilt Istanbul on the site of an earlier Greek city as the capital of the Roman Empire. It later served as the capital of the Byzantine and Ottoman empires until 1922.

The narrow Gulf of Izmit extends to the east (right) from the Sea of Marmara. On
August 17, 1999, a magnitude 7.4 earthquake, often called the Izmit or Kocaeli, Turkey
earthquake, heavily damaged the city of Izmit at the end of the gulf and killed at least 17,000
people. A previous earthquake under the Gulf of Izmit in 1754 killed at least 2,000 people. The Izmit earthquake ruptured a long section of the North Anatolian Fault system from off the right side of this image continuing under the Gulf of Izmit. Another strand of the North Anatolian Fault system is visible as a sharp linear feature in the topography south of Iznik Lake.

Surveys measuring water depth in the area show that the North Anatolian Fault system extends beneath and has formed the Sea of Marmara, in addition to the Gulf of Izmit and Iznik Lake. Scientists are studying the North Anatolian Fault system closely to determine the risk of future large earthquakes on the faults close to Istanbul.

Three visualization methods were combined to produce this image: shading and color
coding of topographic height, and radar image intensity. The shade image was derived by
computing topographic slope in the northwest-southeast direction. Northwest-facing slopes
appear dark and southeast-facing slopes appear bright. Color-coding is directly related to
topographic height, with green at the lower elevations, rising through yellow and brown to white at the highest elevations. The shade image was combined with the radar intensity image to add detail, especially in the flat areas.

The Shuttle Radar Topography Mission was flown aboard Space Shuttle Endeavour
February 11-22, 2000. It used modified versions of the same instruments that comprised the
Space Shuttle Imaging Radar-C/X-Band Synthetic Aperture Radar that flew twice on Endeavour
in 1994. The mission collected 3-D measurements of Earth's land surface using radar
interferometry, which compares two radar images taken at slightly different locations to obtain
elevation or surface-change information. To collect the data, engineers added a 60-meter
(approximately 200-foot) mast, installed additional C-band and X-band antennas, and improved
tracking and navigation devices. More information is available at:

http://www.jpl.nasa.gov/srtm .

NASA's Earth Science Enterprise is a long-term research and technology program
designed to examine Earth's land, oceans, atmosphere, ice and life as a total integrated system.

JPL is a division of the California Institute of Technology in Pasadena.

April 22, 2002

 Recent news bits at http://spacescience.nasa.gov/ :

------------------

Scientists using our RXTE spacecraft have observed a rare thermonuclear
explosion on a neutron star that brightened it for so long that they could
detect its motion as it moved towards and away from us on its orbit around
a companion star. This enabled them to measure the star's orbital velocity
using the Doppler effect, and revealed the neutron star's spin frequency,
confirming two key theories about neutron stars.

Story at http://www.gsfc.nasa.gov/news-release/releases/2002/02-056.htm
RXTE at
http://heasarc.gsfc.nasa.gov/docs/xte/xte_1st.html

------------------

Nearby "retired" quasar galaxies, billions of years past their glory days
as the brightest beacons in the Universe, may be the current source of
rare, high-energy cosmic rays, the fastest-moving bits of matter known and
whose origin has been a long-standing
mystery.
http://www.gsfc.nasa.gov/news-release/releases/2002/02-055.htm

------------------

We have selected four new mission proposals as candidates for the next
MIDEX missions in our Explorer Program. We have also decided to fund U.S.
participation in a European Space Agency observatory on the International
Space Station. The story, with descriptions of the proposed missions, is
at ftp://ftp.hq.nasa.gov/pub/pao/pressrel/2002/02-069.txt ; I'll have links
to the mission pages posted at
http://spacescience.nasa.gov/missions/studies.htm asap.

------------------

Our Chandra X-ray Observatory has provided the best X-ray image yet of two
Milky Way-like galaxies in the midst of a head-on collision. This may help
understand the outcome of such collisions in the past, explaining a lot
about why the Universe looks the way it does
now.
http://chandra.harvard.edu/press/02_releases/press_041902.html

------------------

Binary asteroids -- two rocky objects orbiting about one another -- appear
to be common in Earth-crossing orbits. If one is ever found headed our
way, it could be double
trouble. http://www.jpl.nasa.gov/releases/2002/release_2002_83.html

And in unrelated news: Hubble Hunts Down Binary Objects at the Fringe of
Our Solar System -- story, pics, animations and more at
http://oposite.stsci.edu/pubinfo/pr/2002/04/

------------------

Lots of comets have been discovered over the Internet by amateur
astronomers visiting the website for our Solar and Heliospheric Observatory
(SOHO) spacecraft. Update at
ftp://ftp.hq.nasa.gov/pub/pao/pressrel/2002/02-071.txt

------------------

NASA Administrator Sean O'Keefe recently outlined his strategic vision for
NASA's future, saying in part: "Our future decisions will be
science-driven, not destination-driven." Good stuff for policy wonks at
ftp://ftp.hq.nasa.gov/pub/pao/pressrel/2002/02-066.txt

 Livermore Lab Physicist to Theorize On Hydrogen's Equation of State in
Jupiter

ALBUQUERQUE, N.M. -- Through laser experiments, Lawrence Livermore National
Laboratory physicists determined that deuterium, an isotope of hydrogen, turns
into a metal at a higher density than research performed at Sandia National
Laboratory.

The behavior of hydrogen at extreme pressures provides crucial
information on how Jupiter, made primarily of hydrogen, formed and
evolved.

LLNL Physicist Robert Caule will present the Livermore research Sunday,
April 21, at a press conference titled "Extreme Hydrogen Physics"
during a joint meeting of the American Physical Society and the High
Energy Astrophysics Division of the American Astronomical Society in
Albuquerque, N.M.

Cauble said the Livermore research shows that laser shocks compressing
liquid deuterium at 300 kilobars of pressure -- about 300,000 times
more than the atmospheric pressure of Earth at sea level -- turns the
liquid to a metal.

"Hydrogen is all around the universe and a lot of it is at high
pressure," Cauble said. "It's important to know its equation of state
(the relationship between pressure, density, and temperature)."

Hydrogen's equation of state dictates at what pressures and densities
hydrogen transforms into a metal and so determines the depth where
Jupiter's metallic hydrogen layer begins and the amount of metallic
hydrogen it contains.

In the Livermore experiment, scientists used the now-decommissioned
Nova laser to shock compress liquid deuterium and found it turned into
a metal at a higher density than similar experiments conducted later
by Sandia researchers. Using a different technique on Sandia's Z
Machine, Sandia scientists discovered that they also metallized
deuterium but at densities lower than in the laser experiments. The
two different equations of state implied by the disparate results
affect how researchers view large planets like Jupiter.

Cauble and Marcus Knudson of Sandia will meet to discuss the
experimental results as well as each group's computer simulations
of high-pressure hydrogen during Sunday's press conference.

Cauble said it's possible that the groups' different results could
both be right. It may depend on how the sample is shocked.

The research will be applied to inertial confinement fusion in which
the hydrogen isotopes -- deuterium and tritium -- are used as fuel
to attain fusion. Mega lasers, such as the National Ignition Facility,
offer new opportunities for pursuing experimental science under
extreme conditions of temperature and density.

Cauble said Livermore scientists are conducting further research,
using diamond anvil cells to probe the properties of matter under the
relevant extreme conditions of pressure and compression found in the
interiors of giant gas planets, such as Jupiter.

Other conference presentations featuring Livermore scientists include:

* National Security Fellow Jay Davis of Livermore's Center for Global
Security Research will speak about counter-terrorism contributions
from the national labs during the Monday session: "Physics and
Anti-Terrorism."

* On Saturday, Physicist Chris Fragile will describe the simulation
of black holes "eating" nearby matter, stars and gas clouds and the
dynamics of those accretion flows during "The Secret Life of Black
Holes."

* Physicist Bruce Remington will describe the new field of high energy
density physics in understanding astrophysical phenomena during the
Saturday session "Extreme Physics."

Founded in 1952, Lawrence Livermore National Laboratory is a national
security laboratory, with a mission to ensure national security and
apply science and technology to the important issues of our time.
Lawrence Livermore National Laboratory is managed by the University
of California for the U.S. Department of Energy's National Nuclear
Security Administration.

 MASSIVE ICEBERGS MAY AFFECT ANTARCTIC SEA LIFE AND FOOD CHAIN

NASA-funded research using satellite data has shown
large icebergs that have broken off from Antarctica's Ross
Ice Shelf are dramatically affecting the growth of minute
plant life in the ocean around the region -- plant life vital
to the local food chain.

Scientists say the icebergs appear to have caused a 40
percent reduction in the size of the 2000-2001 plankton bloom
in one of Antarctica's most biologically productive areas.
The icebergs decrease the amount of open water that the
plants need for reproduction.

After the calving, or "breaking off," of the B-15 iceberg in
March of 2000, researchers used imagery from NASA's SeaWiFS
(Sea-viewing Wide Field-of-view Sensor) satellite and data
from the Defense Meteorological Satellite Program to see the
effect that large icebergs have on phytoplankton (minute
floating plants) blooms. The B-15 iceberg that broke off the
Ross Ice Shelf and drifted into the southwestern Ross Sea was
as large as the state of Connecticut (approximately 10,000
square kilometers or 3,900 square miles)

"This is the first time that satellite imagery has been used
to document the potential for large icebergs to substantially
alter the dynamics of a marine ecosystem," said Kevin Arrigo,
a researcher at Stanford University, Stanford, Calif. Arrigo
and his colleagues are publishing their results in a paper
titled "Ecological Impact of a Large Antarctic Iceberg," in
an upcoming issue of Geophysical Research Letters.

NASA's Thorsten Markus of the Goddard Space Flight Center,
Greenbelt, Md., a co-author on the paper, noted that SeaWiFS
satellite imagery enabled researchers to see that large
icebergs such as the B-15 restricted the normal drift of pack
ice. Normally, when the winds shift, ice is carried out into
the Ross Sea, creating open ocean space and a breeding ground
for phytoplankton. The icebergs, however, created a blockage
that resulted in heavier spring/summer pack-ice cover than
previously recorded.

Since the area of sea ice was more extensive, the area
suitable for phytoplankton growth was reduced, and as a
result, so was the length of the algal growing season. Since
the B-15 iceberg was so large, plankton productivity
throughout the region was more than 40 percent below normal.

The southwestern Ross Sea is one of the most biologically
productive regions in the Southern Ocean surrounding
Antarctica. This is partly due to the large and persistent
areas of open water that form during the Antarctic spring
when pack ice drifts out of the Ross Sea.

In the springtime, winds shift in the area of the Ross Sea
and clear away sea ice, forming the Ross Sea polynya (an area
of open water surrounded by sea ice) where phytoplankton
flourish. However, when large icebergs calve, such as B-15,
sea ice is not as easily moved by winds, severely reducing
the area of open water.

Phytoplankton are a critical part of the entire ecosystem in
the Ross Sea, since they sustain marine mammals and birds in
the region. During periods where there are no large icebergs,
phytoplankton thrive, and so do those organisms that feed on
them. The region also is home to 22 percent of the world
population of circumpolar Emperor penguins and 30 percent of
Adélie penguins.

This research is a part of NASA's Earth Science Enterprise, a
long-term research effort dedicated to help us better
understand and protect our home planet.

Images and video are available at:
http://www.gsfc.nasa.gov/topstory/20020416iceberg.html

Information on SeaWiFS can be found at:
http://SeaWiFS.gsfc.nasa.gov/SEAWIFS.html

Information on icebergs is available on the National Snow and
Ice Data Center Web site at:
http://nsidc.org

 NASA'S AQUA SPACECRAFT TO STUDY EARTH'S WATER CYCLE

NASA's mission to understand and protect our home planet
will mark a major milestone this spring with the launch of
the Aqua satellite. Aqua, due to bring us unprecedented
insight of our world's global water cycle, is the latest
sibling in a family of Earth Observing System satellites
dedicated to studying the Earth and our knowledge of global
climate change.

The primary role of Aqua, as the name implies, is to gather
information about water in the Earth's system. Equipped with
six state-of-the-art instruments, Aqua will collect data on
global precipitation, evaporation, and the cycling of water.

During its six-year mission, Aqua will gather information on
changes in ocean circulation and how clouds and surface water
processes affect our climate. This information will help
scientists better understand how global ecosystems are
changing, and how they respond to and affect global
environmental change.

"Aqua will provide unprecedented information on the global
water cycle. The spacecraft will enable operational agencies
to create more accurate weather forecasts in the future,"
said Dr. Ghassem Asrar, Associate Administrator for NASA's
Earth Science Enterprise, NASA Headquarters, Washington.

"Aqua will observe our Earth's oceans, atmosphere, land, ice
and snow covers and vegetation," said Claire Parkinson, the
Aqua project scientist at NASA's Goddard Space Flight Center,
Greenbelt, Md. "This comprehensive approach enables
scientists to study the interactions among key elements of
the Earth system so as to better understand our planet."

Aqua is expected to be launched May 2 from Vandenberg Air
Force Base, Calif. on a Boeing Delta-7920-10L expendable
launch vehicle. The 10-minute launch window opens at 2:55
a.m. Pacific Daylight Time (5:55 a.m. EDT). Aqua will fly at
an altitude of approximately 705 kilometers (438 miles) above
Earth in a near polar and sun synchronous orbit.

Aqua is the sister satellite to NASA's Terra spacecraft,
launched in December of 1999. Aqua will cross the equator
daily at 1:30 p.m. as it heads North. The early afternoon
observation time contrasts with the Terra satellite which
crosses the equator between 10:30 and 10:45 a.m. daily. The
two satellites, Aqua's afternoon observations and Terra's
morning observations, will yield important insights into the
"diurnal variability," or the daily cycling of key scientific
parameters such as precipitation and ocean circulation.

Aqua is a joint project between the United States, Japan and
Brazil. The United States provided the spacecraft and four of
Aqua's six scientific instruments. NASA's Goddard Space
Flight Center provided the Moderate Resolution Imaging
Spectroradiometer and the Advanced Microwave Sounding Unit.
NASA's Jet Propulsion Laboratory, Pasadena, Calif., provided
the Atmospheric Infrared Sounder, and NASA's Langley Research
Center, Hampton, Va., provided the Clouds and the Earth's
Radiant Energy System instrument.

Japan's National Space Development Agency provided the
Advanced Microwave Scanning Radiometer. The Instituto
Nacional de Pesquisas Espaciais (the Brazilian Institute for
Space Research) provided the Humidity Sounder for Brazil.

Aqua is part of NASA's Earth Science Enterprise, a long-term
research effort dedicated to understanding and protecting our
home planet. Through the study of Earth, NASA will help to
provide sound science to policy and economic decision makers
so as to better life here, while developing the technologies
needed to explore the universe and search for life beyond our
home planet.

More information about the Aqua program is available at:

hhttp://www.earth.nasa.gov/ttp://aqua.nasa.gov

Information about NASA's Earth Science Enterprise can be
found at:

http://www.earth.nasa.gov

 WOMEN'S CONTRIBUTIONS TO FLIGHT FOCUS OF 'DAUGHTERS' DAY' / 'AERO EXPO'

NASA will pay tribute to women's contributions to a century of
powered flight with two events on April 24 - 25, portions of which
will be broadcast via the Internet on April 25.

Women pilots and other experts will take part in NASA Internet
'Webcasts' and 'chats' intended for young people across the world on
April 25 for 'Take Our Daughters to Work Day,' and for 'Aero Expo
II.' Many of the activities also will be seen live by about 1,100 San
Francisco Bay area students at NASA Ames Research Center in the heart
of California's Silicon Valley from April 24 through April 25 as part
of 'Aero Expo II.'

"Both events celebrate women's contributions to aviation over the
last hundred years," said NASA 'Quest' Web site developer Susan Lee.
"Women have made some significant contributions to aerospace, and
there are many careers in that field that young girls might
eventually pursue."

"Our goal is to accommodate as many students as possible from
underrepresented and/or underserved schools," said Antoinette
Battiste, who organized of much of the Aero Expo II effort at Ames.
Students from 24 different California community schools -- King City
to San Pablo, Oakland to San Jose, Salinas to Atherton -- are
participating, she said.

Three women -- an aerobatic champion pilot, a Civil Air Patrol pilot
and a Boeing 737 pilot --- will discuss women's contributions to the
first century of flight as part of a one-hour Webcast that begins at
10 a.m. PDT (1 p.m. EDT) on April 25 in the Ames main auditorium,
N201. This and other Internet NASA Quest events can be accessed on
the World Wide Web from:

http://quest.nasa.gov/calendar/

Webcasts enable students to watch live video, listen to audio and
interact in real-time on the Internet with experts. Locally,
employees and their children -- both boys and girls -- can
participate in a myriad of events at NASA Ames on April 25.

"The kind of flying I do (aerobatic maneuvers like loops, rolls,
spins and hammerhead turns) is very physically demanding," said
Cecilia Aragon, a computer scientist at NASA Ames who will
participate in the Webcast. "I sustain G-forces of up to 12 G's
positive and 9 G's negative. What this means is that my body can
weigh up to 12 times its normal weight -- or 9 times its normal
weight hanging in the straps."

Since 1990, Aragon has been a professional air show pilot and has
logged more than 4,800 hours, flying at shows and competitions in the
United States and Europe in front of millions of spectators. At her
NASA Ames job, Aragon develops software for aircraft and spacecraft
flight-testing.

A search and rescue pilot for the Civil Air Patrol, Wendy Holforty is
a second member of the Webcast panel. "As a search-and-rescue pilot,
I fly in search of downed aircraft and during disaster relief," she
said. After college, she became the first female patrol police
officer in East Lansing, Mich. "During my career as a police officer,
I learned to fly airplanes and decided to make aviation a larger part
of my life."

"At first I wanted to be an airline pilot. I then realized, that
while being a pilot was glamorous, the only time it became really
exciting was when something went wrong," Holforty said. "This made me
turn to engineering and aircraft design. So I quit the police force
and went back to school to get a degree in engineering." She now
works at NASA Ames as an aerospace engineer.

The third member of the webcast panel is Mitzi Saylor, a captain for
United Airlines. "Shortly before graduating college in 1986, I
changed job positions to the NASA Aviation Safety Reporting System,
and shortly after graduation I acquired my instrument rating,
commercial pilot license, and multi-engine rating. Over the next
several months I also acquired part-time jobs flying skydivers and
flying traffic watch for KGO (San Francisco)," she said. In early
1998, she became a Boeing 737-300 captain.

"I just love science and aviation so much, and I want to expose the
students to another aspect of life out there. There are thousands of
interests in the world, and I'm happy to share my one small part of
the world. Some kids think it might be unattainable and out of their
reach, but anybody can do this as long as you have a strong interest
in it," Saylor said. More information about the women and their
careers is on the Internet at
http://quest.arc.nasa.gov/projects/aero/centennial/

Also on April 25, at 11 a.m. PDT (2 p.m. EDT) there will be an
hour-long 'Web chat' in both Spanish and English with Fanny Zuniga,
who works in the NASA Ames Virtual Motion Simulator where NASA
astronauts and pilots train. During Internet chats, youngsters use
computers to converse with mentors by typing questions and reading
responses and dialogue via the World Wide Web.

"I currently am working on developing new design tools and processes
that will incorporate new information technologies to help design
better-performing and safer space vehicles," she said. During this
bilingual chat, questions asked in English will be answered in
English, and those asked in Spanish will be answered in Spanish.
Young people will be able to see the simulator in person at Ames on
April 24 and April 25 during on-site tours for Aero Expo II and on
April 25 for employees' children.

April 25 Daughters' (and sons') Day activities at Ames for employees
and their children also include a one-hour session in the main
auditorium, N201, beginning at 8 a.m. PDT (11 a.m. EDT). During the
'Leisure flying' session, private pilots and aeronautics experts
will teach student how to prepare a flight plan. This program also
will be Webcast via the NASA Quest Web site.

'Aero Village' hands-on activities for students will take place in
Hangar 211 from 11:30 a.m. to 2:30 p.m. PDT on both April 24 and
April 25. Students also will see an exhibit of the Stratospheric
Observatory for Infrared Astronomy (SOFIA), a modified Boeing 747SP
aircraft that will house the largest airborne telescope in the world.
In addition, students will climb behind the controls of a Hiller H-4
Interactive Helicopter provided by the Hiller Aviation Museum and a
flight simulator from the California Antique Aircraft Museum. Other
hands-on events include a hang-gliding simulation, a paper airplane
contest and a computer lab where students can design their own
airplanes. Various aircraft will be on display in Hangar 211, too.

Internet Events, April 25 (accessible from
http://quest.arc.nasa.gov/calendar/):

8 a.m. - 9 a.m. PDT (11 a.m. - noon EDT) - Main auditorium, N201,
Webcast, 'Leisure Flying.' Pilots and aeronautics experts teach
students to prepare flight plans.
8 a.m. - 3 p.m. PDT (11 a.m. - 6 p.m. EDT) - Day-long Internet forum,
'Centennial of Flight.' Six NASA women will 'chat' with Internet
visitors about women and aeronautics.
9 a.m. - 10 a.m. PDT (noon - 1 p.m. EDT) - 'Interactive Webchat with
Amelia.' During this interactive event, Web visitors may 'chat' with
historian and author Carol Osborne about aviator Amelia Earhart.
10 a.m. - 11 a.m. PDT (1 - 2 p.m. EDT) - Main auditorium, N201,
'Centennial of Flight Webcast Panel Discussion,' features three woman
pilots, an aerobatic champion, a Civil Air Patrol pilot and an
airline captain.
11 a.m. - noon PDT (2 - 3 p.m. EDT) - 'Bi-lingual Webchat with Fanny
Zuniga.' Zuniga, who works with a simulator in which astronauts
train, will answer questions in Spanish when they are asked in
Spanish. She will answer in English questions posed in English.
Noon - 1 p.m. PDT (3 - 4 p.m. EDT) - 'Astronaut Video Contest.'
Features videotaped interviews with three NASA astronauts: Eileen
Collins, Susan Helms and Shannon Lucid.
1 p.m. - 2 p.m. PDT (4 - 5 p.m. EDT) - 'Chat on Human Factors and
Medical Innovations That Have Improved Flying for Pilots.'
2 p.m. - 3 p.m. PDT (5 - 6 p.m. EDT) - Main auditorium, N201,
'Interactive Webcast on Jets.' A female corporate jet pilot will
discuss the field of corporate flying.
3 p.m. PDT (6 p.m. EDT) - 'Contest winner announced.' Answers and
winners to aero trivia hunt and astronaut video contest will be
announced.
____________________________________________________________________________________
Aero Expo II 'on-site' events for 1,100 local students
(Will take place on Wednesday, April 24, 2002 and Thursday, April 25,
2002, from 8:30 a.m. to 2:30 p.m. PDT each day)

9 a.m. - 10 a.m. PDT and 10 a.m. - 11 a.m. PDT (April 24 and April
25) - Main auditorium, N201, Two panel discussions each day by three
woman pilots, an aerobatic champion, a Civil Air Patrol pilot and an
airline captain.
10 a.m. - Noon PDT (April 24 and April 25) - Facility Tours. First
shift 10:15 a.m. - 10:45 a.m. PDT; second shift 11:15 a.m. - 11:45
a.m. PDT. Facilities on tour: Vertical Motion Simulator, Bldg. N243;
Crew Vehicle Systems Research Facility (airline simulators), Bldg.
N257; FutureFlight Central (air tower/airport simulator), Bldg. N262;
80 Foot X 120 Foot Wind Tunnel, Bldg. N221B; and Airspace Operations
Lab, Bldg. N262, room 280.
11:30 a.m. - 2:30 p.m. PDT - Hangar 211, Aero Village, Hand-on
activities, exhibits, aircraft display.
_____________________________________________________________________________________
'On site' events, April 25 for employees' children (Take Our
Daughters to Work Day)

8 a.m. - 9 a.m. PDT - Main auditorium, N201, 'Leisure Flying.' See
production of Webcast. Pilots and aeronautics experts to teach
students to prepare flight plans.
10 a.m. - noon PDT - Bldg. N226, 'Tour Aerospace Encounter.'
Interactive facility teaches 4th - 6th grade students science and
mathematics.
11:30 a.m. - 2:30 p.m. PDT - Hangar 211, 'Aero Village.' Hands-on
activities, demonstrations, exhibits and aircraft.
2 - 3 p.m. PDT - Main auditorium, N201, see 'Interactive Webcast on
Jets.' A female corporate jet pilot will discuss the field of
corporate flying.
3 - 4 p.m. PDT - Main auditorium, N201, 'Panel Discussion,' featuring
three woman pilots, an aerobatic champion, a Civil Air Patrol pilot
and an airline captain.

 HUBBLE USES OLDEST, FAINTEST STARS TO DATE THE UNIVERSE

New findings by NASA's Hubble Space Telescope, which
give a verification of the age of the Universe, will be the
subject of the next Space Science Update, scheduled for
Wednesday, April 24, at 1 p.m. EDT, at NASA Headquarters.
The Update will feature a discussion on observations of the
faintest and oldest stars called White Dwarfs.

Panelists will be:
* Dr. Harvey Richer, astronomer, University of British
Columbia in Vancouver, Canada
* Dr. Wendy Freedman is an astronomer at the Carnegie
Observatories in Pasadena, Calif.
* Dr. Bruce Margon, associate director for science, Space
Telescope Science Institute (STScI), Baltimore
* Dr. Anne L. Kinney, Director of NASA's Origins Program,
NASA Headquarters, Washington, is panel moderator

The Update will originate from the James E. Webb Auditorium
at NASA Headquarters, 300 E St., S.W., in Washington and
will be carried live on NASA TV with two-way question-and-
answer capability for reporters covering the event from
participating NASA centers.

NASA TV is broadcast on the GE2 satellite which is located
on Transponder 9C, at 85 degrees West longitude, frequency
3880.0 MHz, audio 6.8 MHz. Audio of the broadcast will be
available on voice circuit at the Kennedy Space Center on
407/867-1220.

In addition, the update will be webcast live on the Internet
at:

http://www.nasa.gov

 When galaxies collide: Chandra observes titanic merger

NASA's Chandra X-ray Observatory has provided the best X-ray image
yet of two Milky Way-like galaxies in the midst of a head-on collision.
Since all galaxies - including our own - may have undergone mergers, this
provides insight into how the Universe came to look as it does today.

Astronomers believe the mega-merger in the galaxy known as Arp 220
triggered the formation of huge numbers of new stars, sent shock waves
rumbling through intergalactic space, and could possibly lead to the
formation of a supermassive black hole in the center of the new conglomerate
galaxy. The Chandra data also suggest that merger of these two galaxies
began only 10 million years ago, a short time in astronomical terms.

"The Chandra observations show that things really get messed up when
two galaxies run into each other at full speed," said David Clements of the
Imperial College, London, one of the team members involved in the study.
"The event affects everything from the formation of massive black holes to
the dispersal of heavy elements into the universe."

Arp 220 is considered to be a prototype for understanding what
Conditions were like in the early Universe, when massive galaxies and
supermassive black holes were presumably formed by numerous galaxy
collisions. At a relatively nearby distance of about 250 million light
years, Arp 220 is the closest example of an "ultra-luminous" galaxy, one
that gives off a trillion times as much radiation as our Sun.

The Chandra image shows a bright central region at the waist of a
Glowing, hour-glass-shaped cloud of multimillion-degree gas. Rushing out of
the galaxy at hundreds of thousands of miles per hour, the super-heated as
forms a "superwind," thought to be due to explosive activity generated by
the formation of hundreds of millions of new stars.

Farther out, spanning a distance of 75,000 light years, are giant
lobes of hot gas that could be galactic remnants flung into intergalactic
space by the early impact of the collision. Whether the lobes will
continue to expand into space or fall back into Arp 220 is unknown.

The center of Arp 220 is of particular interest. Chandra
observations allowed astronomers to pinpoint an X-ray source at the exact
location of the nucleus of one of the pre-merger galaxies. Another fainter
X-ray source nearby may coincide with the nucleus of the other galaxy
remnant. The X-ray power output of these point-like sources is greater than
expected for stellar black holes accreting from companion stars. The
authors suggest that these sources could be due to supermassive black holes
at the centers of the merging galaxies.

These two remnant sources are relatively weak, and provide strong
evidence to support the theory that the extraordinary luminosity of Arp 220
- about a hundred times that of our Milky Way galaxy - is due to the rapid
rate of star formation and not to an active, supermassive black hole in the
center.

However, in a few hundred million years, this balance of power may
change. The two massive black holes could merge to produce a central
supermassive black hole. This new arrangement could cause much more gas to
fall into the central black hole, creating a power source equal to or
greater than that due to star formation.

"The unusual concentration of X-ray sources in the very center of
Arp 220 suggests that we could be observing the early stages of the creation
of a supermassive black hole and the eventual rise to power of an active
galactic nucleus," said Jonathan McDowell of the Harvard-Smithsonian Center
for Astrophysics, Cambridge, MA, another member of the team Studying Arp
220.

Clements and McDowell were joined on this research by an
international group of researchers from the United States, United Kingdom
and Spain. Chandra observed Arp 220 on June 24, 2000, for approximately
56,000 Seconds using the Advanced CCD Imaging Spectrometer (ACIS)
instrument.

ACIS was developed for NASA by Pennsylvania State University,
University Park, Pa., and the Massachusetts Institute of Technology,
Cambridge, Mass. NASA's Marshall Space Flight Center in Huntsville, Ala.,
manages the Chandra program, and TRW, Inc., Redondo Beach, Calif., is the
prime Contractor. The Smithsonian's Chandra X-ray Center controls science
and flight operations from Cambridge.

Images and additional information about this result are available
at:

http://chandra.harvard.edu
and
http://chandra.nasa.gov

The Web

News release
http://www1.msfc.nasa.gov/NEWSROOM/news/releases/2002/02-094.html

Photos
http://www1.msfc.nasa.gov/NEWSROOM/news/photos/2002/photos02-094.htm

Fact Sheet
http://www1.msfc.nasa.gov/NEWSROOM/background/facts/axaf.htm

 WOMEN'S CONTRIBUTIONS TO FLIGHT FOCUS OF 'DAUGHTERS' DAY' / 'AERO EXPO'

NASA will pay tribute to women's contributions to a century of
powered flight with two events on April 24 - 25, portions of which
will be broadcast via the Internet on April 25.

Women pilots and other experts will take part in NASA Internet
'Webcasts' and 'chats' intended for young people across the world on
April 25 for 'Take Our Daughters to Work Day,' and for 'Aero Expo
II.' Many of the activities also will be seen live by about 1,100 San
Francisco Bay area students at NASA Ames Research Center in the heart
of California's Silicon Valley from April 24 through April 25 as part
of 'Aero Expo II.'

"Both events celebrate women's contributions to aviation over the
last hundred years," said NASA 'Quest' Web site developer Susan Lee.
"Women have made some significant contributions to aerospace, and
there are many careers in that field that young girls might
eventually pursue."

"Our goal is to accommodate as many students as possible from
underrepresented and/or underserved schools," said Antoinette
Battiste, who organized of much of the Aero Expo II effort at Ames.
Students from 24 different California community schools -- King City
to San Pablo, Oakland to San Jose, Salinas to Atherton -- are
participating, she said.

Three women -- an aerobatic champion pilot, a Civil Air Patrol pilot
and a Boeing 737 pilot --- will discuss women's contributions to the
first century of flight as part of a one-hour Webcast that begins at
10 a.m. PDT (1 p.m. EDT) on April 25 in the Ames main auditorium,
N201. This and other Internet NASA Quest events can be accessed on
the World Wide Web from:

http://quest.nasa.gov/calendar/

Webcasts enable students to watch live video, listen to audio and
interact in real-time on the Internet with experts. Locally,
employees and their children -- both boys and girls -- can
participate in a myriad of events at NASA Ames on April 25.

"The kind of flying I do (aerobatic maneuvers like loops, rolls,
spins and hammerhead turns) is very physically demanding," said
Cecilia Aragon, a computer scientist at NASA Ames who will
participate in the Webcast. "I sustain G-forces of up to 12 G's
positive and 9 G's negative. What this means is that my body can
weigh up to 12 times its normal weight -- or 9 times its normal
weight hanging in the straps."

Since 1990, Aragon has been a professional air show pilot and has
logged more than 4,800 hours, flying at shows and competitions in the
United States and Europe in front of millions of spectators. At her
NASA Ames job, Aragon develops software for aircraft and spacecraft
flight-testing.

A search and rescue pilot for the Civil Air Patrol, Wendy Holforty is
a second member of the Webcast panel. "As a search-and-rescue pilot,
I fly in search of downed aircraft and during disaster relief," she
said. After college, she became the first female patrol police
officer in East Lansing, Mich. "During my career as a police officer,
I learned to fly airplanes and decided to make aviation a larger part
of my life."

"At first I wanted to be an airline pilot. I then realized, that
while being a pilot was glamorous, the only time it became really
exciting was when something went wrong," Holforty said. "This made me
turn to engineering and aircraft design. So I quit the police force
and went back to school to get a degree in engineering." She now
works at NASA Ames as an aerospace engineer.

The third member of the webcast panel is Mitzi Saylor, a captain for
United Airlines. "Shortly before graduating college in 1986, I
changed job positions to the NASA Aviation Safety Reporting System,
and shortly after graduation I acquired my instrument rating,
commercial pilot license, and multi-engine rating. Over the next
several months I also acquired part-time jobs flying skydivers and
flying traffic watch for KGO (San Francisco)," she said. In early
1998, she became a Boeing 737-300 captain.

"I just love science and aviation so much, and I want to expose the
students to another aspect of life out there. There are thousands of
interests in the world, and I'm happy to share my one small part of
the world. Some kids think it might be unattainable and out of their
reach, but anybody can do this as long as you have a strong interest
in it," Saylor said. More information about the women and their
careers is on the Internet at
http://quest.arc.nasa.gov/projects/aero/centennial/

Also on April 25, at 11 a.m. PDT (2 p.m. EDT) there will be an
hour-long 'Web chat' in both Spanish and English with Fanny Zuniga,
who works in the NASA Ames Virtual Motion Simulator where NASA
astronauts and pilots train. During Internet chats, youngsters use
computers to converse with mentors by typing questions and reading
responses and dialogue via the World Wide Web.

"I currently am working on developing new design tools and processes
that will incorporate new information technologies to help design
better-performing and safer space vehicles," she said. During this
bilingual chat, questions asked in English will be answered in
English, and those asked in Spanish will be answered in Spanish.
Young people will be able to see the simulator in person at Ames on
April 24 and April 25 during on-site tours for Aero Expo II and on
April 25 for employees' children.

April 25 Daughters' (and sons') Day activities at Ames for employees
and their children also include a one-hour session in the main
auditorium, N201, beginning at 8 a.m. PDT (11 a.m. EDT). During the
'Leisure flying' session, private pilots and aeronautics experts
will teach student how to prepare a flight plan. This program also
will be Webcast via the NASA Quest Web site.

'Aero Village' hands-on activities for students will take place in
Hangar 211 from 11:30 a.m. to 2:30 p.m. PDT on both April 24 and
April 25. Students also will see an exhibit of the Stratospheric
Observatory for Infrared Astronomy (SOFIA), a modified Boeing 747SP
aircraft that will house the largest airborne telescope in the world.
In addition, students will climb behind the controls of a Hiller H-4
Interactive Helicopter provided by the Hiller Aviation Museum and a
flight simulator from the California Antique Aircraft Museum. Other
hands-on events include a hang-gliding simulation, a paper airplane
contest and a computer lab where students can design their own
airplanes. Various aircraft will be on display in Hangar 211, too.

Internet Events, April 25 (accessible from
http://quest.arc.nasa.gov/calendar/):

8 a.m. - 9 a.m. PDT (11 a.m. - noon EDT) - Main auditorium, N201,
Webcast, 'Leisure Flying.' Pilots and aeronautics experts teach
students to prepare flight plans.
8 a.m. - 3 p.m. PDT (11 a.m. - 6 p.m. EDT) - Day-long Internet forum,
'Centennial of Flight.' Six NASA women will 'chat' with Internet
visitors about women and aeronautics.
9 a.m. - 10 a.m. PDT (noon - 1 p.m. EDT) - 'Interactive Webchat with
Amelia.' During this interactive event, Web visitors may 'chat' with
historian and author Carol Osborne about aviator Amelia Earhart.
10 a.m. - 11 a.m. PDT (1 - 2 p.m. EDT) - Main auditorium, N201,
'Centennial of Flight Webcast Panel Discussion,' features three woman
pilots, an aerobatic champion, a Civil Air Patrol pilot and an
airline captain.
11 a.m. - noon PDT (2 - 3 p.m. EDT) - 'Bi-lingual Webchat with Fanny
Zuniga.' Zuniga, who works with a simulator in which astronauts
train, will answer questions in Spanish when they are asked in
Spanish. She will answer in English questions posed in English.
Noon - 1 p.m. PDT (3 - 4 p.m. EDT) - 'Astronaut Video Contest.'
Features videotaped interviews with three NASA astronauts: Eileen
Collins, Susan Helms and Shannon Lucid.
1 p.m. - 2 p.m. PDT (4 - 5 p.m. EDT) - 'Chat on Human Factors and
Medical Innovations That Have Improved Flying for Pilots.'
2 p.m. - 3 p.m. PDT (5 - 6 p.m. EDT) - Main auditorium, N201,
'Interactive Webcast on Jets.' A female corporate jet pilot will
discuss the field of corporate flying.
3 p.m. PDT (6 p.m. EDT) - 'Contest winner announced.' Answers and
winners to aero trivia hunt and astronaut video contest will be
announced.
____________________________________________________________________________________
Aero Expo II 'on-site' events for 1,100 local students
(Will take place on Wednesday, April 24, 2002 and Thursday, April 25,
2002, from 8:30 a.m. to 2:30 p.m. PDT each day)

9 a.m. - 10 a.m. PDT and 10 a.m. - 11 a.m. PDT (April 24 and April
25) - Main auditorium, N201, Two panel discussions each day by three
woman pilots, an aerobatic champion, a Civil Air Patrol pilot and an
airline captain.
10 a.m. - Noon PDT (April 24 and April 25) - Facility Tours. First
shift 10:15 a.m. - 10:45 a.m. PDT; second shift 11:15 a.m. - 11:45
a.m. PDT. Facilities on tour: Vertical Motion Simulator, Bldg. N243;
Crew Vehicle Systems Research Facility (airline simulators), Bldg.
N257; FutureFlight Central (air tower/airport simulator), Bldg. N262;
80 Foot X 120 Foot Wind Tunnel, Bldg. N221B; and Airspace Operations
Lab, Bldg. N262, room 280.
11:30 a.m. - 2:30 p.m. PDT - Hangar 211, Aero Village, Hand-on
activities, exhibits, aircraft display.
_____________________________________________________________________________________
'On site' events, April 25 for employees' children (Take Our
Daughters to Work Day)

8 a.m. - 9 a.m. PDT - Main auditorium, N201, 'Leisure Flying.' See
production of Webcast. Pilots and aeronautics experts to teach
students to prepare flight plans.
10 a.m. - noon PDT - Bldg. N226, 'Tour Aerospace Encounter.'
Interactive facility teaches 4th - 6th grade students science and
mathematics.
11:30 a.m. - 2:30 p.m. PDT - Hangar 211, 'Aero Village.' Hands-on
activities, demonstrations, exhibits and aircraft.
2 - 3 p.m. PDT - Main auditorium, N201, see 'Interactive Webcast on
Jets.' A female corporate jet pilot will discuss the field of
corporate flying.
3 - 4 p.m. PDT - Main auditorium, N201, 'Panel Discussion,' featuring
three woman pilots, an aerobatic champion, a Civil Air Patrol pilot
and an airline captain.

 When galaxies collide: Chandra observes titanic merger

NASA's Chandra X-ray Observatory has provided the best X-ray image
yet of two Milky Way-like galaxies in the midst of a head-on collision.
Since all galaxies - including our own - may have undergone mergers, this
provides insight into how the Universe came to look as it does today.

Astronomers believe the mega-merger in the galaxy known as Arp 220
triggered the formation of huge numbers of new stars, sent shock waves
rumbling through intergalactic space, and could possibly lead to the
formation of a supermassive black hole in the center of the new conglomerate
galaxy. The Chandra data also suggest that merger of these two galaxies
began only 10 million years ago, a short time in astronomical terms.

"The Chandra observations show that things really get messed up when
two galaxies run into each other at full speed," said David Clements of the
Imperial College, London, one of the team members involved in the study.
"The event affects everything from the formation of massive black holes to
the dispersal of heavy elements into the universe."

Arp 220 is considered to be a prototype for understanding what
Conditions were like in the early Universe, when massive galaxies and
supermassive black holes were presumably formed by numerous galaxy
collisions. At a relatively nearby distance of about 250 million light
years, Arp 220 is the closest example of an "ultra-luminous" galaxy, one
that gives off a trillion times as much radiation as our Sun.

The Chandra image shows a bright central region at the waist of a
Glowing, hour-glass-shaped cloud of multimillion-degree gas. Rushing out of
the galaxy at hundreds of thousands of miles per hour, the super-heated as
forms a "superwind," thought to be due to explosive activity generated by
the formation of hundreds of millions of new stars.

Farther out, spanning a distance of 75,000 light years, are giant
lobes of hot gas that could be galactic remnants flung into intergalactic
space by the early impact of the collision. Whether the lobes will
continue to expand into space or fall back into Arp 220 is unknown.

The center of Arp 220 is of particular interest. Chandra
observations allowed astronomers to pinpoint an X-ray source at the exact
location of the nucleus of one of the pre-merger galaxies. Another fainter
X-ray source nearby may coincide with the nucleus of the other galaxy
remnant. The X-ray power output of these point-like sources is greater than
expected for stellar black holes accreting from companion stars. The
authors suggest that these sources could be due to supermassive black holes
at the centers of the merging galaxies.

These two remnant sources are relatively weak, and provide strong
evidence to support the theory that the extraordinary luminosity of Arp 220
- about a hundred times that of our Milky Way galaxy - is due to the rapid
rate of star formation and not to an active, supermassive black hole in the
center.

However, in a few hundred million years, this balance of power may
change. The two massive black holes could merge to produce a central
supermassive black hole. This new arrangement could cause much more gas to
fall into the central black hole, creating a power source equal to or
greater than that due to star formation.

"The unusual concentration of X-ray sources in the very center of
Arp 220 suggests that we could be observing the early stages of the creation
of a supermassive black hole and the eventual rise to power of an active
galactic nucleus," said Jonathan McDowell of the Harvard-Smithsonian Center
for Astrophysics, Cambridge, MA, another member of the team Studying Arp
220.

Clements and McDowell were joined on this research by an
international group of researchers from the United States, United Kingdom
and Spain. Chandra observed Arp 220 on June 24, 2000, for approximately
56,000 Seconds using the Advanced CCD Imaging Spectrometer (ACIS)
instrument.

ACIS was developed for NASA by Pennsylvania State University,
University Park, Pa., and the Massachusetts Institute of Technology,
Cambridge, Mass. NASA's Marshall Space Flight Center in Huntsville, Ala.,
manages the Chandra program, and TRW, Inc., Redondo Beach, Calif., is the
prime Contractor. The Smithsonian's Chandra X-ray Center controls science
and flight operations from Cambridge.

Images and additional information about this result are available
at:

http://chandra.harvard.edu
and
http://chandra.nasa.gov

The Web

News release
http://www1.msfc.nasa.gov/NEWSROOM/news/releases/2002/02-094.html

Photos
http://www1.msfc.nasa.gov/NEWSROOM/news/photos/2002/photos02-094.htm

Fact Sheet
http://www1.msfc.nasa.gov/NEWSROOM/background/facts/axaf.htm

 NEXT SPACE SCIENCE UPDATE APRIL 24:
HUBBLE USES OLDEST, FAINTEST STARS TO DATE THE UNIVERSE

New findings by NASA's Hubble Space Telescope, which
give a verification of the age of the Universe, will be the
subject of the next Space Science Update, scheduled for
Wednesday, April 24, at 1 p.m. EDT, at NASA Headquarters. The
Update will feature a discussion on observations of the
faintest and oldest stars called White Dwarfs.

Panelists will be:
* Dr. Harvey Richer, astronomer, University of British
Columbia in Vancouver, Canada
* Dr. Wendy Freedman is an astronomer at the Carnegie
Observatories in Pasadena, Calif.
* Dr. Bruce Margon, associate director for science, Space
Telescope Science Institute (STScI), Baltimore
* Dr. Anne L. Kinney, Director of NASA's Origins Program,
NASA Headquarters, Washington, is panel moderator

The Update will originate from the James E. Webb Auditorium
at NASA Headquarters, 300 E St., S.W., in Washington and will
be carried live on NASA TV with two-way question-and-answer
capability for reporters covering the event from
participating NASA centers.

NASA TV is broadcast on the GE2 satellite which is located
on Transponder 9C, at 85 degrees West longitude, frequency
3880.0 MHz, audio 6.8 MHz. Audio of the broadcast will be
available on voice circuit at the Kennedy Space Center on
407/867-1220.

In addition, the update will be webcast live on the Internet
at:

http://www.nasa.gov

April 19, 2002

 MARS ODYSSEY THEMIS IMAGES
April 15-19, 2002

o Eastern Floor of Holden Crater (Released 15 April 2002)
http://themis.la.asu.edu/zoom-20020415a.html

o Medusae Fossae Formation (Released 16 April 2002)
http://themis.la.asu.edu/zoom-20020416a.html

o Holden Crater/Uzboi Valles (Released 17 April 2002)
http://themis.la.asu.edu/zoom-20020417a.html

o Bosporus Planum (Released 18 April 2002)
http://themis.la.asu.edu/zoom-20020418a.html

o White Rock (Released 19 April 2002)
http://themis.la.asu.edu/zoom-20020419a.html

All of the THEMIS images are archived here:

http://themis.la.asu.edu/latest.html

NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission
for NASA's Office of Space Science, Washington, D.C. The Thermal Emission
Imaging System (THEMIS) was developed by Arizona State University,
Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing.
The THEMIS investigation is led by Dr. Philip Christensen at Arizona State
University. Lockheed Martin Astronautics, Denver, is the prime contractor
for the Odyssey project, and developed and built the orbiter. Mission
operations are conducted jointly from Lockheed Martin and from JPL, a
division of the California Institute of Technology in Pasadena.

----------------------------------------------------------------------------
http://themis.la.asu.edu/zoom-20020415a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
Eastern Floor of Holden Crater (Released 15 April 2002)

The Story

With its beautiful symmetry and gullies radially streaming
down to the floor, the dominant crater in this image is an
impressive focal point. Yet, it is really just a small crater
within a much larger one named Holden Crater. Take a look at
the context image to the right to see just how much bigger
Holden Crater is. Then come back to the image strip that
shows the mottled surface of Holden Crater's eastern floor in
greater detail, and count how many hills, ridges, channels, and
small impact craters can be seen. No perfectly smooth terrain
abounds there, that's for sure.

The textured terrain of Holden Crater has been particularly
intriguing ever since the Mars Orbital Camera on the Mars
Global Surveyor spacecraft found evidence of sedimentary rock
layers there that might have formed in lakes or shallow seas
in Mars' ancient past. This finding suggests that Mars may
have been more like Earth long ago, with water on its surface.
Holden Crater might even have held a lake long ago. No one
knows for sure, but it's an exciting possibility. Why?

If water was once on the surface of Mars long enough to form
sedimentary materials, maybe it was there long enough for
microbial life to have developed too. (Life as we know it just
isn't possible without the long-term presence of liquid
water.) The question of life on the red planet is certainly
tantalizing, but scientists will need to engage in a huge
amount of further investigation to begin to know the answer.
That's why orbital images of Holden Crater like this one are
so important. They continue to help scientists piece together
the answers to their fundamental questions about the planet's
environment and its potential as a past or present habitat for
life.

The Science

Today's THEMIS image covers territory on the
eastern floor of Holden Crater, which is located
in region of the southern hemisphere called
Noachis Terra. Holden Crater is 154 km in
diameter and named after American Astronomer
Edward Holden (1846-1914). This image shows
a mottled surface with channels, hills, ridges and
impact craters. The largest crater seen in this
image is 5 km in diameter. This crater has
gullies and what appears to be horizontal layers
in its walls.

This image is the 14th image in a series of daily
images released by the THEMIS Team.

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http://themis.la.asu.edu/zoom-20020416a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
Medusae Fossae Formation (Released 16 April 2002)


The Story

"Yardang!"

Now, that may seem like a peculiar-sounding curse word, but
nobody would get in trouble for using it. A yardang is one of the
very cool-sounding words geologists use to describe long,
irregular features like the ones seen in this image. Yardangs
are grooved, furrowed ridges that form as the wind erodes
away weakly cemented material in the region. Rippling across
the surface, yardangs tell the story of how the powerful
Martian wind carved the surface into such a gorgeous pattern
over time. (Don't miss clicking on the above image to see a
detailed view, in which the beauty and almost dance-like
symmetry of the waving terrain pops out in highly compelling,
three-dimensional texture.)

It may be easy to see which way the wind blows in this area,
since these streamlined features point in the direction of
prevailing winds. But how can geologists understand the
various kinds of terrain seen here? First, they have to study
the different patterns of erosion, looking closely at how the
wind has stripped off certain layers and not others.

Want to be a geologist yourself? Start at the bottom of the
image and scroll upward, and see how the relatively smooth,
higher terrain toward the south gradually becomes more and
more eroded. Moving up the image, at first you'll see only a
few, isolated regions of parallel ridges and knolls. Go a little
farther north with your eyes (toward the center of the image),
and you'll see how these linear knobs really get going! Once
you get to the top of the image, only patches of these grooved
ridges remain, leaving an incredibly smooth, wind-scrubbed
surface behind. You know this layer has to be made of pretty
hard material, because it seems impervious to further erosion.

Geologists studying Mars can compare these Martian
yardangs to examples found on Earth, such as those in the Lut
desert of Iran. Humans have even been known to use the wind
as their inspiration, sculpting the shape of yardangs
themselves. The famous sphynx at Giza in Egypt is thought to
be a yardang that's been whittled down a little more by ancient
human chiselers.

The Science

This THEMIS visible image was acquired near
11° N, 159° W and shows examples of the
remarkable variations that can be seen in the
erosion of the Medusae Fossae Formation.
This Formation is a soft, easily eroded deposit
that extends for nearly 1,000 km along the
equator of Mars. In this region, like many others
throughout the Medusae Fossae Formation, the
surface has been eroded by the wind into a
series of linear ridges called yardangs. These
ridges generally point in direction of the
prevailing winds that carved them, and
demonstrate the power of martian winds to
erode the landscape of Mars. The easily eroded
nature of the Medusae Fossae Formation
suggests that it is composed of weakly
cemented particles, and was most likely formed
by the deposition of wind-blown dust or
volcanic ash. Within this single image it is
possible to see differing amounts of erosion and
stripping of layers in the Medusae Fossae
Formation. Near the bottom (southern) edge of
the image a rock layer with a relatively smooth
upper surface covers much of the image. Moving
upwards (north) in the image this layer
becomes more and more eroded. At first there
are isolated regions where the smooth unit has
been eroded to produce sets of parallel ridges
and knobs. Further north these linear knobs
increase in number, and only small, isolated
patches of the smooth upper surface remain.
Finally, at the top of the image, even the ridges
have been removed, exposing the remarkably
smooth top of hard, resistant layer below. This
sequence of layers with differing hardness and
resistance to erosion is common on Earth and
on Mars, and suggests significant variations in
the physical properties, composition, particle
size, and/or cementation of these martian
layers. As is common throughout the Medusae
Fossae Formation, very few impact craters are
visible, indicating that the surface exposed is
relatively young, and that the process of erosion
may be active today.

This image is the 15th image in a series of daily
images released by the THEMIS team.

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http://themis.la.asu.edu/zoom-20020417a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
Holden Crater/Uzboi Valles (Released 17 April 2002)

The Story

Mars doesn't have a shortage of rugged terrain, and this area
is no exception. While things look pretty quiet now, this
cratered region was once the scene of some tremendous
action. Long ago in Martian history, an incoming meteroid
probably smashed into the planet and produced a giant impact
crater named Holden Crater, which stretches 88 miles across
the Martian surface. The history of the area around Holden
Crater doesn't stop there. At some point, a catastrophic flood
burst forth on the surface, forming an impressive outflow
channel called Uzboi Valles. No one knows exactly how that
happened, or whether the water might even have rushed into
Holden Crater at some point, forming a long-ago lake. What
we do know is that there is a lot of sedimentary material that
could have formed in two hypothesized ways: in an ancient
lake environment or as volcanic-ash deposits.

Scientists are searching for the answers by studying the
region where Uzboi Valles meets the crater. You can see the
rough edge of Holden Crater running diagonally down in a
sharply edged swath (from the top left-hand corner of this
image to the center right-hand side). Just below it, running
almost smoothly down the right-hand side of the image is an
intriguing channel where water may once have flowed. Much of
the terrain in the bottom half of the image, in fact, seems to be
cut into a swish-swash of dissected sedimentary terrain.
Sliced through in such a way, the terrain ends up carrying
bunches of small, rounded hills called "hummocks." Earth can
boast of its own rolling, hummocky terrain too, such as that
found in the ravine-cut Missouri Hills and High Plains areas
of South Dakota.

The Science

This image, located near 27.0S and 35.5W,
displays the intersection of Holden Crater with
Uzboi Valles. This region of Mars contains a
number of features that could be related to liquid
water on the surface in the Martian past. Holden
Crater contains finely layered sedimentary units
that have been subsequently dissected. The
hummucky terrain in the bottom half of the image
is the remnants of this terrain, though the fine
layers are not visible in this image at this
resolution. The sedimentary units could have
formed through deposition of material in a
lacustrine type environment. Alternately, these
layers could also be volcanic ash deposits.
Uzboi Valles, which enters the crater from the
southwest, is a catastrophic outflow channel
that formed in the Martian past. The streamlined
nature of the topographic features at the
intersection of the crater with Uzboi Valles
record the erosional pattern of flowing liquid
water on the surface of Mars during the episodic
outflow event.

This image is the 16th image in a series of daily
images released by the THEMIS team.

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http://themis.la.asu.edu/zoom-20020418a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
Bosporus Planum (Released 18 April 2002)

The Story

Splat! Take a look at the lumpy edge of the large crater half
(left-hand side of the image) and compare it to the much
neater rims of other craters in the region. Why is there such a
difference? Scientists believe that when something hit the
surface of Mars long ago, ice may have been present in the
subsurface and was "regurgitated" upward into the Martian air
along wih dirt and rock, "splooshing" outward. When that
happened, the mixed-up, ejected material created a wavering,
batter-like edge that is not typical for most (ice-free) craters.
More ejected material from this same impact radiates much
farther out from the crater, giving it a vague, sun-like
appearance.

Many of the small craters in this image appear much fainter
and more subdued than the others. Their ghostly appearance
may be due to a lava flow that smoothed out most of the
terrain in this image, partially burying them . . . . Or???? Maybe
it was a layer of dust that settled in this region to accomplish
the same concealed look.

And what about that scar-like trek that cuts through the upper
third of the image? It's an elongated fault created when a
crust-breaking, tectonic force ripped apart the Martian terrain,
leaving a long depression on the surface. This feature is called
a graben, and we find them on Earth too (think of Death
Valley, the lowest dry land in the United States, or the Jordan
Dead Sea depression). The graben's rumpled, scar-like
appearance is only enhanced by the stitchy-looking sand
dunes that run down its sides. This dune pattern shows that
the Martian wind probably blew down through the graben
canyon to create their ruffled appearance.

The wind doesn't have its way everywhere, though. The
brighter surface material on the western side of the two
diagonally positioned smaller craters is probably a layer of
dust that has been shielded from removal by the craters'
higher rims. Dark streaks (possibly dark sand) on the
opposite side of these craters reveal that the wind has been
blowing to no avail in the opposite direction too.

So, think that explains everything in this image? Here's a
quick geology quiz! Which features happened first? The
dunes, the lava plains, the big crater, or the linear
depression called a graben? To find out if you're right, check
out the last paragraph in The Science caption. Hint! Whatever
happened later has to be on top of whatever came before.

The Science

This THEMIS image is of Bosporus Planum,
located in a region of smooth plains that appear
to have formed from lava flows. A crater, ~7 km
in diameter, on the left edge of the image has
produced an ejecta blanket that can be seen
radiating from the crater. Lobes of ejecta such as
those seen close to the crater rim are not formed
at most typical craters and may indicate that
there was a ice component in the sub-surface
material when the impact occurred. A linear
depression trending from the northwest to
southeast along the top of the image is about 1
to 2 km wide. This may be a tectonic feature,
known as a graben, that forms when a region is
under stresses that are pulling it apart. There
are numerous small bright dunes or ripples along
the margins of the floor of this linear feature that
have formed perpendicular to the sides of the
graben. This pattern of ripples suggests that the
wind was blowing down the graben canyon.
Similar small bright dunes can be faintly seen on
top of the crater ejecta along ridges (most
apparent directly to the east of the crater) and
along the southern margin of the interior
deposits in the crater. Bright wind streaks are
also apparent in this area to the west (right) of
several large craters. These streaks likely
formed when very small particle size materials
(like dust) is deposited on the surface and then
protected from removal by the wind shadow
produced by the crater's rim. Shorter dark
streaks, possible deposits of dark sand, have
formed to the east side of the smaller craters.
These streaks on opposite sides of craters may
indicate that there have been different wind
patterns in the area, blowing in opposite
directions. Subtle ridges near the south end of
the image hint that there may have been other
graben that have been nearly filled in. Many of
the craters in this image have a subdued, buried
appearance and may have been partially filled by
lava flows or mantled by dust.

A short geologic history of the area in this image
can be created using the basic principles of
geology, such as the principle of superposition
(deposits that lie on top of other materials are
younger). The linear depression must have
formed after the deposition of the lava plains
since it is a feature that would not have been
otherwise preserved. Ejecta from the large
crater has been deposited inside and over the
edges of the linear depression, thus the crater
must have formed after the linear depression.
Finally, the bright dunes and dust streaks
formed last because they have been deposited
on top of all of these different features.

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http://themis.la.asu.edu/zoom-20020419a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
White Rock (Released 19 April 2002)


The Story
Fingers of hard, white rock seem to jut out like icy daggers
across a moody Martian surface, but appearances can be
deceiving. These bright, jagged features are neither white, nor
icy, nor even hard and rocky!

So what are they, and why are they so different from the
surrounding terrain?

Scientists know that you can't always trust what your eyes
see alone. You have to use other kinds of science instruments
to measure things that our eyes can't see . . . things like
information about what kinds of minerals make up the
landforms. Mars scientists once thought, for instance, that
these unusual features might be vast hills of salt, the dried up
remains of a long-ago, evaporated lake.

Not so, said an instrument on the Mars Global Surveyor
spacecraft, which revealed that the bright material is probably
made up of volcanic ash or windblown dust instead. And talk
about a cyclical "ashes to ashes, dust to dust" story! Particles
of this material fell and fell until they built up quite a
sedimentary deposit, which was then only eroded away again
by the wind over time, leaving the spiky terrain seen today. It
looks white, but its apparent brightness arises from the fact
that the surrounding material is so dark.

Of course, good eyesight always helps in understanding. A
camera on Mars Global Surveyor with close-up capabilities
revealed that sand dunes are responsible for the smudgy dark
material in the bright sediment and around it. But that's not
all. The THEMIS camera on the Mars Odyssey spacecraft
that took this image reveals that this ashy or dusty deposit
once covered a much larger area than it does today. Look
yourself for two small dots of white material on the floor of a
small crater nearby (center right in this image). They preserve
a record that this bright deposit once reached much farther.
Since so little of it remains, you can figure that the material
probably isn't very hard, and simply blows away.

One thing's for sure. No one looking at this image could ever
think that Mars is a boring place. With all of its bright and
dark contrasts, this picture would be perfect for anyone who
loves Ansel Adams and his black-and-white photography.

The Science

"White Rock" is the unofficial name for this
unusual landform which was first observed during
the Mariner 9 mission in the early 1970's. As
later analysis of additional data sets would
show, White Rock is neither white nor dense
rock. Its apparent brightness arises from the fact
that the material surrounding it is so dark.
Images from the Mars Global Surveyor MOC
camera revealed dark sand dunes surrounding
White Rock and on the floor of the troughs within
it. Some of these dunes are just apparent in the
THEMIS image. Although there was speculation
that the material composing White Rock could be
salts from an ancient dry lakebed, spectral data
from the MGS TES instrument did not support
this claim. Instead, the White Rock deposit may
be the erosional remnant of a previously more
continuous occurrence of air fall sediments, either
volcanic ash or windblown dust. The THEMIS
image offers new evidence for the idea that the
original deposit covered a larger area.
Approximately 10 kilometers to the southeast of
the main deposit are some tiny knobs of similarly
bright material preserved on the floor of a small
crater. Given that the eolian erosion of the main
White Rock deposit has produced isolated knobs
at its edges, it is reasonable to suspect that the
more distant outliers are the remnants of a once
continuous deposit that stretched at least to this
location. The fact that so little remains of the
larger deposit suggests that the material is very
easily eroded and simply blows away.

Cassini Significant Events
for 04/11/02 - 04/17/02

The most recent spacecraft telemetry was acquired from the Goldstone
tracking station on Wednesday, April 17. The Cassini spacecraft is in an
excellent state of health and is operating normally. Information on the
present position and speed of the Cassini spacecraft may be found on the
"Present Position" web page located at
http://saturn.jpl.nasa.gov/cassini/english/where/ .

The primary activity on board the spacecraft this week was Probe
Checkout (PCO) #9. The checkout was completed successfully. However,
during the checkout, Goldstone Deep Space Station (DSS) 25 was required
to end track and stow its antenna early due to high winds. The resulting
telemetry outage caused the loss of PCO #9 real-time data and was
expected to continue though the time allotted for PCO recorded data
playback. At the request of Huygens Probe Operations Center personnel,
with Cassini Program Manager concurrence, and with prior notification
given to affected instruments, the Spacecraft Office built a real-time
command to inhibit writing of Magnetospheric and Plasma Science (MAPS)
data on the Solid State Recorder. This preserved the PCO data for
playback at the next scheduled track. About 20 hours of MAPS data was
lost. The pass over DSS 45 was then used to playback the PCO data and
resume normal C31 activities.

Additional instrument and spacecraft activities included the uplink of
real-time commands to modify the Radio and Plasma Wave Science
Instrument Expanded Block to fine tune resolution of data collected,
clearing of the ACS high water marks, an autonomous CDS Solid State
Recorder memory load partition repair, a demonstration over DSS 45 of
the new Version 26.4 Command System, and uplink of a Privileged Action
Program to disable/enable the Solid State Power Switch trip Fault
Protection in support of the Probe checkout.

Science Planning reported that all Target Working Teams made the
delivery for the Science Operations Plan integration activity for orbits
15 through 20. The Instrument Operations Science Data Archive Engineer
is conducting a Planetary Data Archive Workshop in conjunction with the
Huygens Science Working Team meeting being held this week in Paris,
France.

After last week's delivery coordination meeting for Cosmic Dust Analyzer
flight software, it was identified that V9 may generate invalid packet
IDs. Workarounds were discussed and a final decision regarding uplink
will be determined by next week.

Mission Support and Services Office (MSSO) personnel met with Radio
Science and the DSN Network Operations Project Engineer to discuss
uplink transfers for the next Superior Conjunction Experiment. During
the Gravitational Wave Experiment last December, about a dozen uplink
transfers failed, each causing more than 2 hours outage in prime mission
science data. The most likely cause identified was the setting DSS
waiting too long to initiate tune-out. It was resolved that a briefing
message will be sent to the DSN specifying begin tune-out time based on
Spacecraft Office telecom analysis.

All teams and offices supported the Cassini Monthly Management Review.

The Program Manager gave a presentation to the JPL Executive Council on
the issue of providing real-time communications during the SOI burn by
doing the burn at Earth-line attitude. It is feasible to provide
telemetry during all of the burn except for a period where the
spacecraft is occulted by the rings, but at a cost in science return and
propellant usage. Further studies were requested.

MSSO personnel gave a talk and museum tour to attendees of a NASA
Administrative Issues Conference held at the Jet Propulsion Laboratory.

Cassini is a cooperative project of NASA, the European Space Agency and
the Italian Space Agency. The Jet Propulsion Laboratory, a division of
the California Institute of Technology in Pasadena, Calif., manages the
Cassini mission for NASA's Office of Space Science, Washington, D.C.

Cassini Outreach
Cassini Mission to Saturn and Titan
Jet Propulsion Laboratory
California Institute of Technology
National Aeronautics and Space Administration

Spot the targets of Europe's space explorers

 The next few weeks offer the chance of a lifetime to observe
the five brightest planets appearing close together in the sky.
Look to the west after sunset, and even an inexperienced watcher
without a telescope will see the planets changing their relative
positions in a slow dance from night to night. And you can take
the opportunity to pick out the destinations of three,
perhaps four, of ESA's interplanetary spacecraft.

Read more at:
http://sci.esa.int/content/news/index.cfm?aid=1&cid=1&oid=29818

 AQUA MISSION MEDIA BRIEFINGS SET FOR APRIL 22

The launch of Aqua, NASA's latest Earth Science
satellite, is scheduled for Thursday, May 2, from Vandenberg
Air Force Base, Calif. The primary role of Aqua, as the name
implies, is to gather information about water in the Earth's
system. Equipped with six state-of-the-art instruments, Aqua
will collect data on global precipitation, evaporation and
the cycling of water -- information vital to better
understand and protect the Earth.

In preparation for the launch, NASA will hold a mission media
briefing at 1 p.m. EDT Monday, April 22, in the James Webb
Memorial Auditorium, NASA Headquarters, 300
E Street SW, Washington.

Speakers for the Aqua mission briefing will be:

* Ghassem R. Asrar, Associate Administrator for Earth
Science, NASA Headquarters, Washington
* Claire Parkinson, Aqua project scientist, Goddard Space
Flight Center, Greenbelt, Md.
* Phil Sabelhaus, Aqua project manager, Goddard Space Flight
Center

The briefing will be carried live on NASA Television with
two-way question-and-answer capability for reporters covering
the briefing from participating NASA centers. Reporters must
coordinate in advance with NASA Center Newsrooms to
participate remotely. NASA TV is broadcast on satellite GE-2,
transponder 9C, at 85 degrees West longitude, vertical
polarization, frequency 3880 MHz, audio of 6.8 MHz. The
briefing also will available on the Internet at:
http://www.nasa.gov/ntv/ntvweb.html

More information about Aqua can be found at:
http://aqua.nasa.gov

 MARS VIKING LEADER, JAMES S. MARTIN, JR., DIES

Former NASA manager of the Viking missions to Mars,
James S. Martin, Jr., died April 14, in Rising Sun, Md.,
after a long battle with cancer. Martin was 81.

Viking 1 and Viking 2, twin spacecraft launched to Mars in
1975, reached the Red Planet a year later. The two orbiting
spacecraft provided the first global maps of Mars and when
the two Viking landers touched down on the Martian surface,
they made history by becoming the first successful mission
to soft-land on the surface of another planet. Martin led
this unprecedented effort and its 750-person nationwide team
of NASA, industry and university engineers, scientists and
technicians.

"America lost a great explorer and superb leader in space
exploration, and those around the world who push back the
frontiers of the unknown mourn the loss of Jim Martin," said
Dr. Ed Weiler, Associate Administrator for Space Science,
NASA Headquarters, Washington. "He will always be remembered
as a giant among space explorers. He was able, against
tremendous odds and obstacles, to succeed with perhaps the
most ambitious space mission ever attempted. The legacy of
Viking, and Jim Martin, lives on in our new Mars Exploration
Program."

The Viking landers and orbiters operated in orbit and on the
surface of Mars for over five years, laying laid the
groundwork for more recent NASA successes including Mars
Pathfinder, the rover Sojourner, the Mars Global Surveyor
orbiter, and the 2001 Mars Odyssey orbiter which launched in
April 2001.

"Jim Martin was the epitome of leadership," said Tom Young,
Viking's mission director and former president of Lockheed
Martin, on the occasion of the project's silver anniversary
in July. "Jim had the experience. He knew what it took to
make a project successful. He had the strength and the
integrity to do those things that were necessary to make it
work."

Martin joined NASA's Langley Research Center in September
1964 as assistant project manager for Lunar Orbiter. The
five successful Lunar Orbiter missions provided significant
new information about the Moon's surface and a wealth of
photographic detail that stood as the definitive source of
lunar surface information for years. In recognition of his
contribution to this project, Martin was awarded the NASA
Exceptional Service Medal in 1967.

Martin was born in Washington, D.C. on June 21, 1920. He
earned a bachelor's degree in aeronautical engineering from
the University of Michigan in 1942. He later completed the
Harvard Graduate School of Business Middle Management
Program.

From 1942 to 1964, Martin worked for Republic Aviation
Corporation, assuming greater responsibility first as
assistant chief technical engineer, then chief research
engineers and, finally, as manager of space systems
requirements.

Martin left NASA in 1976 to become vice president of
advanced programs and planning, for Martin Marietta
Aerospace, Bethesda, Md. In 2000, Martin was asked by NASA
to come out of retirement and lead the effort to restructure
the agency's Mars Exploration Program. He is survived by his
wife Frieda and their children Neil Martin (now an employee
at NASA's Goddard Space Flight Center, Greenbelt, Md.) and
Laurie Martin.

 DISCOVER A COMET WHILE ON THE INTERNET WITH SOHO

A new comet was discovered over the Internet by a
Chinese amateur astronomer visiting the website for the Solar
and Heliospheric Observatory (SOHO) spacecraft. The comet
"C/2002 G3 (SOHO)" was first reported on Friday, April 12, by
XingMing Zhou of BoLe city, in the XinJiang province of
China, who discovered the comet while watching SOHO real-time
images of the Sun on the Internet. The comet is a new comet,
not belonging to any known group.

SOHO, launched over six years ago as a project of
international cooperation between the European Space Agency
(ESA) and NASA, has discovered more than 420 comets in just
under six years. This makes the spacecraft the most prolific
comet finder in the history of astronomy. Most of the comets
were first spotted by amateurs around the world who
downloaded SOHO's real-time images to their home computers.
Anyone with Internet access can take part in the hunt for new
comets and be a comet discoverer.

"From September 2000 to now I have been trying to find SOHO
comets, and I've discovered 13 comets, one of which,
designated '2001U9' and initially cataloged by the SOHO
project as 'SOHO-367,' was the brightest one in the last two
years," said Zhou, who previously spent more than 1,600 hours
since his 1985 graduation scanning the heavens with his 15cm
F/5.3 reflector telescope to discover a single comet.

"What's exciting about these near-sun comets is that we are
exploring a population of comets that has never been seen
before because they are very small and faint," said Douglas
Biesecker, a solar physicist with L3 Com Analytics
Corporation, Vienna, Va. "By the time their orbits take them
close to the Sun so they become bright, they are lost in the
Sun's glare and require a space-based coronagraph like that
on SOHO to be seen." Biesecker, who is affiliated with the
SOHO program at NASA's Goddard Space Flight Center in
Greenbelt, Md., confirms potential comet discoveries as they
are posted to the SOHO website.

C/2002 G3 (SOHO) will be visible in SOHO's Large Angle and
Spectrometric Coronagraph (LASCO) C3 images until Saturday,
April 20. The comet was first visible late in the day on
Thursday, April 11. It entered the field of view at the
bottom edge, almost directly under the Sun. It is moving
upward to the left, and will eventually move back toward the
right, exiting from the LASCO C3 field of view at the top
edge, to the right of the Sun. First cataloged by the SOHO
project as "SOHO-422," it has been officially designated
C/2002 G3 (SOHO) by the International Astronomical Union.

The comet reached the point closest to the Sun in its orbit
on April 17 at about 1:30 a.m. Eastern Daylight Time, at a
distance of about 7.6 million miles (12.3 million
kilometers). As the week goes on, the comet will move through
the field of view more quickly.

In all these images, the shaded disk is a mask in the
instrument that blots out direct sunlight, making faint
comets and the dim outer atmosphere of the Sun, or the
corona, visible. The white circle added within the disk shows
the size and position of the visible Sun.

Solar radiation heats the comet, which in turn causes the
outgassing of its water molecules and dust. The dust scatters
sunlight at visible wavelengths, making the comet bright in
LASCO images. The water molecules break down into oxygen and
hydrogen atoms, and the hydrogen atoms interact with the
coronal plasma (electrified gas that comprises the extended
atmosphere of the Sun).

All the SOHO images are freely available on the SOHO web
site:
http://sohowww.nascom.nasa.gov/

More information about sun-grazing comets and how to spot new
ones can be found at:
http://sungrazer.nascom.nasa.gov/
Images and movies of the comet's passage are available at:
http://soho.nascom.nasa.gov/hotshots/2002_04_15/

 NASA EARTH DAY FEATURES BIRD HIKES, 'GREEN' BUILDING & BUYING TALKS

Hiking to see some of the many birds that live near south San
Francisco Bay, a street fair and lectures about 'green' home building
and 'green' purchasing are a few of many activities in which
employees can take part to celebrate Earth Day during the week of
April 22, at NASA Ames Research Center in California's Silicon Valley.

The theme of Earth Day this year at NASA Ames is 'Sustainable
Communities by the Bay.' Although Earth Day is Monday, April 22,
Ames' events during that week begin on Tuesday, April 23.

"We want to sustain environmental quality, health, economic growth
and prosperity by encouraging a life style that will decrease human
use of Earth's resources," said Julie Quanz of Ames, who helped
organize Ames' Earth Day events. "At our street fair there will be
people representing alternative fuel vehicle companies, local
environmental educational groups, municipalities,
pollution-prevention programs, the San Francisco Bay Trail and
various Ames organizations." The street fair with about 25 exhibitors
will take place on Durand Road at Ames from 11 a.m. to 2 p.m., PDT
Tuesday, April 23.

Also on Tuesday, Ames wildlife biologist Chris Alderete will lead two
bird-watching hikes for employees and reporters. "During the walks,
there's a good chance to see the burrowing owl, which is listed as a
California species of special concern, a status that has legal
implications," Alderete said. He expects that bird watchers could get
as close as 50 feet to an owl. The morning hike will be from 9 a.m.
to 10:30 a.m. PDT, and the afternoon hike will be from 3 p.m. to 4:30
p.m. PDT. Both hikes will start at the soccer field next to Bldg.
N245. Reporters may leave the walks early.

"The western burrowing owl population has been in serious decline
over the past few decades in California. We have upland grassland
habitat where 18 to 27 breeding pairs of owls live each year,"
Alderete explained. The small birds live in ground squirrel burrows
and have long legs, buff white breasts and lemon-yellow eyes.

"We also might see golden eagles, red tailed hawks and loggerhead
shrikes," Alderete added. "We have wetlands where four endangered
species live, including salt marsh harvest mice, and three types of
birds -- California clapper rail, California least tern and snowy
plover."

'Green Building Demystified,' a talk by Darren Bouton, 'green'
building coordinator for the city of San José's Environmental
Services Dept., will begin at 12:15 p.m. PDT on Wednesday, April 24,
in the second floor auditorium in Bldg. N245. The city of San José
defines a 'green' building as any building that is sited, designed,
constructed, operated and maintained for the health and well-being of
the occupants, while minimizing impact on the environment.

'Green' buildings promote resource conservation by including design
features that encourage energy efficiency, use of renewable energy
and water conservation, according to the city's Web page. More
information about the 'green' building program is on the World Wide
Web at:

http://www.ci.san-jose.ca.us/esd/gb-home.htm

'Green Purchasing at Ames,' a one-hour presentation by procurement
specialist Shannah Trout of NASA's Kennedy Space Center, Florida,
will start at 10 a.m., PDT Thursday, April 25, in Bldg. N239, room 39.

April 18, 2002

 NASA TV COVERS RUSSIAN SOYUZ SPACE STATION MOVE

NASA Television will broadcast the relocation of a
Russian Soyuz spacecraft at the International Space Station
beginning at 4 a.m. EDT Saturday, April 20, from the NASA
Johnson Space Center in Houston. The short 40-minute
relocation flight begins with undocking at about 5 a.m. EDT.

Expedition Four Commander Yury Onufrienko and Flight
Engineers Carl Walz and Dan Bursch will climb aboard the
current Soyuz vehicle for the fly around from the Earth-
facing docking port on the Zarya module to the Pirs docking
compartment. The move is necessary to clear the way for the
arrival of a new Soyuz ferry craft on April 27.

NASA TV is available on GE-2, Transponder 9C, at 85 degrees
West longitude, vertical polarization, with a frequency of
3880 MHz and audio of 6.8 MHz.

 NASA Marshall Center's Art Stephenson, Ann Whitaker elected AIAA Fellows

The director of NASA's Marshall Space Flight Center in Huntsville, Ala., and
the director of its Science Directorate have been elected Fellows by the
American Institute of Aeronautics and Astronautics, the nation's largest
society devoted to the advancement of aviation, space and defense.

Art Stephenson, Marshall Center director, and Dr. Ann Whitaker, who heads
the Science Directorate, will be honored at the American Institute of
Aeronautics and Astronautics (AIAA) Global Air and Space '02 International
Business Forum and Exhibition, April 23-25, in Arlington, Va.

To be distinguished as a Fellow by AIAA, a candidate must be an Associate
Fellow in the institute and have made valuable contributions to the arts,
science and technology of their field.

Stephenson leads the Marshall Center -- NASA's premier organization for
development of space transportation and propulsion systems, and NASA's
leader in microgravity research and advanced large optics manufacturing
technology. He administers a broad range of research and development
activities, along with more than 6,500 civil service and contract employees
and an annual budget currently at $2.3 billion.

Since joining Marshall in 1998, Stephenson has overseen the Center's work on
critical NASA initiatives such as development of new reusable launch
vehicles, Space Shuttle propulsion, advanced space transportation systems,
research in microgravity, and science payload operations aboard the
International Space Station, and the launch and continuing successful
operation of the Chandra X-ray Observatory -- the world's most powerful
X-ray telescope.

Stephenson began his career in 1964 with TRW in Redondo Beach, Calif. In his
first assignment, he designed a computer test set to verify performance of
the Apollo Lunar Excursion Abort Guidance System. He later led development
of the Pioneer Jupiter Spacecraft receiver, the first spacecraft to leave
our solar system, and development of the Space Shuttle S-band communication
network transponder, still in use today.

From 1988 to 1992, Stephenson was director of space transportation and
advanced programs, heading TRW's study teams for NASA's Assured Crew Return
Vehicle De-Orbit Module as well as projects for U.S. military and
international space programs.

In 1992, he joined Oceaneering International Inc., and served as vice
president and general manager of Oceaneering Space Systems in Houston. Under
his leadership, the organization grew from 30 to 220 employees in five
years, serving Marshall, Johnson Space Center in Houston, the Departments of
Defense and Energy, and many prime contractors.

Stephenson was promoted to president of Oceaneering Advanced Technologies in
1997. This position combined Oceaneering Space Systems with responsibilities
for Oceaneering's U.S. Navy, Department of Energy and entertainment
businesses, including submarine rescue system design, robotics for hazardous
waste cleanup at nuclear waste sites in the United States, and attractions
for theme parks in Florida, California and Japan.

Stephenson is a member of the National Space Society and American
Astronautical Society. He was awarded NASA's Outstanding Leadership Medal in
2000 and NASA's Exceptional Achievement Medal in 2001, both at NASA
Headquarters in Washington, D.C.

A graduate in electrical engineering from the University of Redlands,
Calif., he also completed the executive program in management at the John E.
Anderson Graduate School of Management at the University of California at
Los Angeles.

Stephenson is a native of New London, Conn. He and his wife, Loa, have two
adult children, Kristin and John, and three grandsons.

Ann Whitaker, a pioneer in developing methods for predicting the performance
of materials in the space environment, began her NASA career in 1963,
joining the Marshall Center as a physicist in the former Propulsion and
Vehicle Engineering Laboratory.

Her early career included contributions to the Saturn program that launched
Americans to the Moon, and the Long Duration Exposure Facility - a series of
flight experiments to characterize environmental effects on materials in
space. Information gleaned from Whitaker's early research continues to
support material selection for present-day space systems, including the
International Space Station.

Whitaker became chief of Marshall's Physical Sciences Branch in 1977, chief
of the Engineering Physics Division in 1984, and chief of the Project and
Environmental Engineering Division in 1993.

In 1995, she was selected for the Senior Executive Service, and held key
leadership positions within Marshall's Science and Engineering Directorate.
These included deputy director of the Space Sciences Laboratory and director
of the Materials, Processes and Manufacturing Department. As the director
of the Science Directorate, she is responsible for materials and
biotechnology microgravity science, Earth and Space Science, and Advanced
Optics Manufacturing Technology.

She has a bachelor's degree in physics from Berry College in Rome, Ga., a
master's degree in physics from the University of Alabama in Huntsville and
a doctorate in materials engineering from Auburn University in Auburn, Ala.

Whitaker has received numerous awards during her career, including NASA's
Exceptional Service Medal, Exceptional Engineering Achievement Medal, Women
in Science and Engineering Lifetime Achievement Award, and Rank of
Meritorious Executive. She is the author or co-author of 70 publications.

She is a native of Plainsville, Ga. She and her husband, John, are the
parents of one daughter, Leann.

 JPL EXPLORER MISSION PROPOSAL CHOSEN FOR FEASIBILITY STUDY

A mission to discover the brightest galaxy in the universe is one of four proposals
selected by NASA as candidates for the next missions in the agency's Explorer Program of
lower cost, highly focused, rapid-development scientific spacecraft. The mission is managed
by NASA's Jet Propulsion Laboratory, Pasadena, Calif.

NASA has also decided to fund as a "Mission of Opportunity" U.S. participation in a
European Space Agency observatory on the International Space Station.

Following detailed mission concept studies, NASA intends to select two of the mission
proposals by early 2003 for full development as Medium-class Explorer flights. The two
missions developed for flight will be launched in 2007 and 2008.

"The Medium-class Explorer program provides an excellent opportunity to explore
fundamental questions of science and technology," said Dr. Ed Weiler, associate administrator
for space science at NASA Headquarters, Washington, D.C. "The missions we've chosen fully
support NASA's vision to understand and protect our home planet, to explore the universe and
to search for life."

The selected proposals were judged to have the best science value among 42 proposals
submitted to NASA in October 2001. Each will receive $450,000 ($250,000 for the Mission of
Opportunity) to conduct a four-month implementation feasibility study. The selected Medium-
Explorer proposals are:

-- The Next Generation Sky Survey -- an infrared telescope designed to survey the entire sky
with 1,000 times more sensitivity than previous missions. It would discover the brightest
galaxy and the closest star, or failed star, to the Sun. Currently, Alpha Centauri is the closest
known star system to the Sun. However, many scientists believe there may be brown dwarfs,
or failed stars, that are even closer. The survey would be led by Dr. Edward L. Wright of the
University of California, Los Angeles, at a total mission cost to NASA of $180 million. JPL
would manage the mission. Science operations and data processing would be handled by the
JPL/Caltech Infrared Processing and Analysis Center in Pasadena.

-- The Astrobiology Explorer -- a cryogenic telescope to determine the abundance, distribution
and identities of the chemical building blocks of life. The mission would measure interstellar
organic compounds and would be led by Dr. Scott Sandford of NASA's Ames Research Center
in Moffett Field, Calif., at a total mission cost to NASA of $180 million.

-- The Time History of Events and Macroscale Interactions during Substorms mission -- a
study of the onset of magnetic storms within the tail of Earth's magnetosphere. The mission
would fly five microsatellite probes through different regions of the magnetosphere and
observe the onset and evolution of storms. The mission would be led by Dr. Vassilis
Angelopoulos of the University of California, Berkeley, at a total mission cost to NASA of
$150 million.

-- The Advanced Spectroscopic and Coronagraphic Explorer -- solar telescopes that would
reveal the physical processes in the outer atmosphere of the Sun leading to the
solar wind and explosive coronal mass ejections. The mission would carry three solar
instruments 100 times better than previous coronal telescopes and would be led by Dr. John L.
Kohl of the Smithsonian Astrophysical Observatory, Cambridge, Mass., at a total mission cost
to NASA of $177 million.

NASA also selected an investigation to be flown on the International Space Station in
partnership with the European Space Agency. At the end of the study, NASA will make a final
decision on participating in the European Space Agency-led mission. The Extreme Universe
Space Observatory would detect the highest-energy cosmic rays known by using the entire
Earth as a particle detector. As extremely energetic particles pass through Earth's atmosphere
they emit a form of blue light that that would be observed by the Extreme Universe Space
Observatory's large telescope from its vantage point on the International Space Station. The
Extreme Universe Space Observatory is under study by the European Space Agency for flight
on the Columbus module of the Space Station, and NASA would provide the large Fresnal lens
for the telescope. NASA's contribution to the Extreme Universe Space Observatory would be
led by Dr. James H. Adams Jr. of NASA's Marshall Space Flight Center, Huntsville, Ala., at a
total mission cost to NASA of $21 million.

NASA also selected a proposed mission for technology-development funding of the
proposed instrument. Dr. Stephan S. Meyer of the University of Chicago will develop a
frequency-selective bolometer to study dusty galaxies in the early universe from a balloon-
borne telescope over Antarctica. Meyer will receive $500,000 over the next two years for his
study.

The current Medium-explorer missions are the Imager for Magnetopause-to-Aurora
Global Exploration, launched in March 2000, and the Microwave Anisotropy Probe, launched
in June 2001. The third Medium-explorer mission is the Swift Gamma-Ray Burst Explorer
which will be launched in September 2003. The Explorer Program is designed to provide
frequent, low-cost access to space for physics and astronomy missions with small to mid-sized
spacecraft. The Explorer Program is managed by NASA's Goddard Space Flight Center,
Greenbelt, Md., for the Office of Space Science, Washington.

More information on the Explorer program is available at
http://fpd.gsfc.nasa.gov/410/index.html .

 NASA EARTH DAY WEBCAST: ANY MORE EARTHS OUT THERE?

Is there any planet like Earth beyond our solar system?
If so, what might it teach us about Earth's past and future?
NASA scientists will explore the topic and answer questions
from the public during a live webcast on Earth Day, Monday,
April 22, from 2 to 3 p.m. Eastern time (11 a.m. to noon
Pacific time).

The panel will examine the conditions that make Earth a
habitable environment and discuss the possibility of Earth-
like planets around other stars. The scientists will discuss
what the discovery of such planets might teach us about Earth
and its environment.

The panelists represent the Origins and astrobiology
programs at NASA's Jet Propulsion Laboratory, Pasadena, Calif.
They are:

-- Dr. Victoria Meadows, leader of JPL's astrobiology research
team, which is exploring the origin, evolution, distribution
and future of life in the universe
-- Dr. Rolf Danner, research scientist for JPL's planet-
finding missions
-- Dr. Rachel Akeson, research scientist at the California
Institute of Technology in Pasadena; involved in the study of
planetary origins
-- Dr. Karl Stapelfeldt, JPL Origins program research
scientist studying planets beyond our solar system

The panelists will take questions in real-time from
audiences at science museums around the country. Questions
from the public will be accepted via e-mail on the day of the
webcast, starting at 11 a.m. Eastern time (8 a.m. Pacific
time). E-mail questions should be sent to
pqfeedback@jpl.nasa.gov with Earth Day in the subject line.

The webcast, in Real Player format, will be available at
http://planetquest.jpl.nasa.gov . The Web site also includes
information, animation and interactive features explaining
JPL's search for planets.

NASA's Origins program, managed by JPL, includes a series
of missions to search for Earth-like planets around other
stars and answer the questions: Where did we come from? Are
we alone? More information on Origins is available at
http://origins.jpl.nasa.gov .

JPL is a division of the California Institute of
Technology in Pasadena.

 NEW BIOSATELLITE TO STUDY LIFE IN MARTIAN GRAVITY

The Mars Society has announced a landmark private space mission that
willhelp researchers understand the long-term effects of living on
Mars. MIT(Cambridge, MA), the University of Washington (Seattle, WA),
and the University of Queensland (Brisbane, Australia) are leading
the project.

Mission highlights include:

* The first privately developed biosatellite
* The first mammalian births in space
* The first in-depth study of mammals in a partial-gravity environment
* The first student-led launch and recovery of a spacecraft

The privately funded, pioneering mission will study the effects of
prolonged exposure to Martian gravity on mammals, a vital step on the
road to human exploration of Mars. Student teams at three leading
universities will design, construct, and launch a satellite with a
payload of mice on board. The mice will experience Martian gravity---
3/8 that of Earth. While in space, some will give birth to a second
generation, who will grow and develop entirely in this new
environment. After nearly two months, the craft will return to Earth,
where teams of scientists will study the crew and their offspring to
obtain the first clues about life and development in reduced gravity.

The Translife Mars Gravity Biosatellite, as the mission will be
called, will fly the mice aboard a spinning spacecraft that generates
artificial gravity identical to that on the surface of Mars. The
satellite is scheduled to launch in mid-2005, orbit for about 50
days, and then return the crew safely to Earth. The team is
considering a number of launch vehicle options.

The mission will conduct basic scientific research necessary before
humans can safely explore Mars. Astronauts living in space stations
have encountered serious health problems, such as bone loss, due to
the weightless environment. The first crew on Mars could experience
similar effects, and scientists do not yet know whether Martian
gravity is sufficient to prevent these long-term health hazards.

The mission's crew of mice will provide the first answers to this
important question, and the equally important question of whether
higher life from Earth will ever be able to settle Mars. During the
seven-week mission, their offspring will grow from
birth to nearly adulthood in Martian gravity. At the end of the
flight, the satellite will re-enter the atmosphere, bringing the
original crew and their progeny safely back to Earth for scientific
study.

Three universities will collaborate to develop this complex
spacecraft: MIT will manage scientific objectives and the mission
payload; the University of Washington will design the carrier
spacecraft; and the University of Queensland (Australia) will devise
the re-entry and recovery systems.

The Mars Gravity Biosatellite is expected to cost nearly $10 million.
The students are seeking financial and in-kind support from both
public and private sectors to complete the project. An anonymous
donor has pledged to match all contributions at 50%.

The Mars Society is a private organization that works toward the
exploration and settlement of our neighboring planet. It furthers
these goals through public outreach to instill the vision of
pioneering Mars, supporting aggressive government Mars exploration
programs, and conducting exploratory research on a private basis.

Before we can explore and settle the planet Mars, we must determine
whether mammals can live, function, reproduce, and develop normally
in its weak gravity field. This mission's groundbreaking research
will provide the first insight into humans' ability to one day travel
beyond the Earth and inhabit new worlds.

A complete report on the Translife Mission will be presented at the
5th International Mars Society Convention, August 8-11, University of
colorado at Boulder. Registration is now open at www.marssociety.org.

Read more about the Translife Mars Gravity Biosatellite project at
http://www.marsgravity.org/.

More information about the Mars Society's Translife Initiative is
available at
http://www.marssociety.org/translife/.

Rift Valley Fever

 Scientists are learning that the key to predicting certain epidemics --
like Rift Valley fever in Africa or Hanta virus in the U.S. -- lies in an
unexpected place: the ocean.

FULL STORY at

http://science.nasa.gov/headlines/y2002/17apr_rvf.htm?list448368

 NASA SELECTS EXPLORER MISSION PROPOSALS
FOR FEASIBILITY STUDIES

Mission proposals that would discover the brightest
galaxy in the universe, measure the chemical building blocks
of life, track magnetic storms in the Earth's magnetosphere
and study massive explosions on the Sun were recently
selected by NASA as candidates for the next missions in the
agency's Explorer Program of lower cost, highly focused,
rapid-development scientific spacecraft.

NASA has also decided to fund as a "Mission of Opportunity"
U.S. participation in a European Space Agency (ESA)
observatory on the International Space Station.

Following detailed mission concept studies, NASA intends to
select two of the mission proposals by early 2003 for full
development as Medium-class Explorer, or MIDEX, flights. The
two missions developed for flight will be launched in 2007
and 2008.

"The MIDEX program provides an excellent opportunity to
explore fundamental questions of science and technology,"
said Dr. Ed Weiler, associate administrator for space science
at NASA Headquarters, Washington. "The missions we've chosen
fully support NASA's vision to understand and protect our
home planet, to explore the universe and to search for life."

The selected proposals were judged to have the best science
value among 42 proposals submitted to NASA in October 2001.
Each will receive $450,000 ($250,000 for the Mission of
Opportunity) to conduct a four-month implementation
feasibility study. The selected MIDEX proposals are:

* The Astrobiology Explorer (ABE) -- a cryogenic telescope
to determine the abundance, distribution and identities of
the chemical building blocks of life. ABE would measure
interstellar organic compounds and would be led by Scott
Sandford of NASA's Ames Research Center in Moffett Field,
Calif., at a total mission cost to NASA of $180 million.

* The Next Generation Sky Survey (NGSS) -- an infrared
telescope designed to survey the entire sky with 1,000 times
more sensitivity than previous missions. NGSS would be led by
Edward L. Wright of the University of California, Los
Angeles, at a total mission cost to NASA of $180 million.

* The Time History of Events and Macroscale Interactions
during Substorms (THEMIS) mission -- a study of the onset of
magnetic storms within the tail of the Earth's magnetosphere.
THEMIS would fly five microsatellite probes through different
regions of the magnetosphere and observe the onset and
evolution of storms. THEMIS would be led by Vassilis
Angelopoulos of the University of California, Berkeley, at a
total mission cost to NASA of $150 million.

* The Advanced Spectroscopic and Coronagraphic Explorer
(ASCE) -- solar telescopes that would reveal the physical
processes in the outer atmosphere of the Sun leading to the
solar wind and explosive coronal mass ejections. ASCE would
carry three solar instruments 100 times better than previous
coronal telescopes and would be led by John L. Kohl of the
Smithsonian Astrophysical Observatory, Cambridge, Mass., at a
total mission cost to NASA of $177 million.

NASA also selected an investigation to be flown on the
International Space Station in partnership with the European
Space Agency. At the end of the study, NASA will make a final
decision on participating in the ESA-led mission. The Extreme
Universe Space Observatory (EUSO) would detect the highest-
energy cosmic rays known by using the entire Earth as a
particle detector. As extremely energetic particles pass
through the Earth's atmosphere they emit a form of blue light
that that would be observed by EUSO's large telescope from
its vantage point on the ISS. EUSO is under study by ESA for
flight on the Columbus module of the ISS, and NASA would
provide the large Fresnal lens for the telescope. NASA's
contribution to EUSO would be led by James H. Adams Jr. of
NASA's Marshall Space Flight Center, Huntsville, Ala., at a
total mission cost to NASA of $21 million.

NASA also selected a proposed mission for technology-
development funding of the proposed instrument. Stephan S.
Meyer of the University of Chicago will develop a frequency-
selective bolometer to study dusty galaxies in the early
universe from a balloon-borne telescope over Antarctica.
Meyer will receive $500,000 over the next two years for his
study.

The current MIDEX missions are the Imager for Magnetopause-
to-Aurora Global Exploration (IMAGE), launched in March 2000,
and the Microwave Anisotropy Probe (MAP), launched in June
2001. The third MIDEX mission is the Swift Gamma-Ray Burst
Explorer which will be launched in September 2003. The
Explorer Program is designed to provide frequent, low-cost
access to space for physics and astronomy missions with small
to mid-sized spacecraft. The Explorer Program is managed by
NASA's Goddard Space Flight Center, Greenbelt, Md., for the
Office of Space Science, Washington.

More information on the Explorer program is available at:
http://fpd.gsfc.nasa.gov/410/index.html

 HUBBLE HUNTS DOWN ODD COUPLES AT THE FRINGES OF OUR SOLAR SYSTEM

NASA's Hubble Space Telescope is hot on the trail of a puzzling new
class of solar system object that might be called a Pluto "mini-me."
Together, these objects are 5,000 times less massive than Pluto and
Charon. Like Pluto and Charon, these dim and fleeting objects travel
in pairs in the frigid, mysterious outer realm of the solar system
called the Kuiper Belt, a long-hypothesized "junkyard" of countless
icy bodies left over from the solar system's formation. A total of
seven binary Kuiper Belt objects have been seen so far by Hubble and
ground-based observatories. Among them is a pair called 1998 WW31,
which the Hubble telescope studied in detail.

To see and read more, please click on:
http://oposite.stsci.edu/pubinfo/pr/2002/04
http://oposite.stsci.edu/pubinfo/latest.html
http://oposite.stsci.edu/pubinfo/pictures.html and
http://hubblesite.org/go/news

The Space Telescope Science Institute (STScI) is operated by the
Association of Universities for Research in Astronomy, Inc. (AURA),
for NASA, under contract with the Goddard Space Flight Center,
Greenbelt, MD. The Hubble Space Telescope is a project of
international cooperation between NASA and the European Space
Agency (ESA).

 NEW IMAX FILM TAKES MOVIEGOERS ON 3D SPACE STATION TOUR

NASA astronauts-turned-film-makers will be joined by
Hollywood's top gun at the Smithsonian's National Air and
Space Museum in Washington tonight to help launch the first
3D cinematic journey to the International Space Station.

The new IMAX 3D movie "SPACE STATION 3D," photographed by
NASA astronauts, Russian cosmonauts and narrated by Academy
Award nominee Tom Cruise, premieres Wednesday night at a
special event at the museum's newly renovated theater.
Cruise, along with NASA Administrator Sean O'Keefe and a host
of dignitaries and aerospace executives, is expected to be on
hand for the movie's debut. Lockheed Martin sponsors the film
in cooperation with NASA.

Transported by the visually stunning effects of IMAX 3D
technology, moviegoers blast off into space with the
astronauts and cosmonauts who are hard at work building the
most complicated research project ever attempted.

"The 3D imagery captured by the IMAX cameras allows those of
us on the ground to experience life in the weightlessness of
space," said NASA Administrator Sean O'Keefe. "It's an
amazing piece of work that we hope may help inspire a new
generation of explorers. You see what it's really like to
live in orbit, 24 hours a day, seven days a week, traveling
around the world at more than 17,000 miles per hour."

Between December 1998 and August 2000, more than 13 miles of
film flew into space for use in two IMAX 3D cameras. Working
closely with IMAX, 25 astronauts and cosmonauts were trained
to use the high-tech equipment. They had to learn how to be
directors, cinematographers, and lighting and sound experts.

"We at Lockheed Martin are proud to have helped in educating
millions around the world on both the importance of space to
our planet's future and the joy of working and living in
orbit," said Dennis Boxx, Lockheed Martin's Senior Vice
President, Corporate Communications. "Through these films,
the corporation has helped foster international understanding
of space, build stronger relations with our NASA customer,
and aided the National Air and Space Museum by providing a
series of films that have generated visitors to our country's
most import and popular museum."

The successful team of NASA, IMAX and Lockheed Martin has
produced five challenging and inspiring space films,
including "The Dream Is Alive" (1985), "Blue Planet" (1990),
"Destiny in Space" (1994) and "Mission to Mir" (1997),
exposing people around the world to the wonders of space
exploration.

This latest achievement details the challenges, setbacks and
ultimately the shared victory of the pioneering men and women
who are making possible the first international space
laboratory. "Space Station" is the story of the unique
partnership of 16 nations to build a permanent science
outpost in low Earth orbit.

"We are very excited by the enthusiasm "SPACE STATION 3D" is
generating in the IMAX theatre network," said IMAX co-CEOs
Richard L. Gelfond and Bradley J. Wechsler. "Only a handful
of highly skilled individuals will ever actually travel to
space but the astronauts and cosmonauts involved in this
project have told us that only IMAX captures their experience
and recreates the excitement and awe that they have felt in
this unique environment. We believe that this ground-
breaking film will inspire generations of students to focus
on the next frontier and enable millions of people to
experience space."

Additional details about the film are available on a special
interactive Web site, filled with in-depth information, a
photo gallery, astronaut interviews and a complete guide to
showings. The Web site is at:

http://www.imax.com/spacestation

More information about the International Space Station and
the four expedition crews is available on the Web at:

http://spaceflight.nasa.gov

In SOHO's pictures, watch a comet passing near the Sun 

Between now and Saturday, 20 April, you can follow via
the Internet the progress of the new-found Comet SOHO-422.
Usually, comets seen by the SOHO spacecraft quickly burn
up in the Sun's hot atmosphere. This one won't, so there
is still time to monitor its progress.

Read more about this at:
http://sci.esa.int/content/news/index.cfm?aid=1&cid=1&oid=29838

 FREE LECTURES GIVE A BREATH OF FRESH AIR TO OZONE DEPLETION STUDIES

The effects of subtle changes in Earth's climate on the ozone layer will be explored in two
free, public lectures entitled "The Changing Ozone Layer: A Greenhouse Gas Connection?" at NASA's Jet Propulsion Laboratory Thursday, April 18, and at Pasadena City College Friday, April 19.

Dr. Ross Salawitch, a research scientist in the atmospheric chemistry group at JPL, will
discuss how industrial emissions of chlorofluorocarbons deplete the ozone layer and how recent research by JPL and elsewhere reveals subtle climate changes may also cause ozone depletion.

Salawitch's past research focused on measuring how human activities affect stratospheric
ozone levels. His research contributed to ratification of the Montreal Protocol on Substances that Deplete the Ozone Layer and subsequent amendments; agreements that led to the international ban and phase-out of chlorofluorocarbon production. He also authored a chapter for the 1998 World Meteorological Organization Scientific Assessment of Ozone Depletion, which proved conclusively the link between the industrial build-up of chlorine and ozone depletion. His current research is focused on understanding how the ozone layer will evolve as chlorine levels recede and climatic change affects stratospheric humidity and temperature.

Salawitch came to JPL in 1994 from Harvard University, Cambridge, Mass., where he was a research associate and postdoctoral fellow in atmospheric chemistry. He is currently a visiting research associate at the California Institute of Technology in Pasadena, and he has authored nearly 100 research papers.

Both lectures begin at 7 p.m. Seating is on a first-come, first-served basis. The JPL lecture
will be webcast live and will also be available after the event at
http://www.jpl.nasa.gov/events/lectures/apr02.html .

The lecture at JPL, located at 4800 Oak Grove Dr., Pasadena, off the Oak Grove Drive exit
of the 210 (Foothill) Freeway, will be held in the von Karman Auditorium. The Friday lecture will
be held in Pasadena City College's Vosloh Forum at 1570 E. Colorado Blvd.

For more information, visit http://www.jpl.nasa.gov/events/lectures/apr02.html or call
(818) 354-0112. JPL is a division of the California Institute of Technology in Pasadena.

April 17, 2002

 HISTORY-MAKING NAVIGATORS WIN AWARD

The team that made history last year by navigating a
spacecraft to a remarkably safe landing on an asteroid
received a laureate prize today from Aviation Week & Space
Technology magazine.

Dr. Bobby G. Williams of NASA's Jet Propulsion
Laboratory, Pasadena, Calif., accepted the laureate's award
for the Near Earth Asteroid Rendezvous mission navigation
team at the National Air and Space Museum, Washington, D. C.

"Working on the project has been the high point of my career,"
said Williams. "A maneuver like this had never been done
before - our team had to go back to school and rethink the
way we do things."

On February 12, 2001, the spacecraft was coaxed into a soft
landing on the surface of asteroid Eros. "The feat of landing
on a body with only one-thousandth of Earth's gravity was all
the more remarkable given that the spacecraft was not designed
to land at all, " said James Asker, Washington bureau chief
for Aviation Week & Space Technology magazine.

The team included navigators from both JPL and the mission's
managing center, Johns Hopkins' Applied Physics Laboratory,
Laurel, Md. Besides landing the spacecraft, the navigation
team recorded many firsts, accomplishments that will be
recounted in the April 29, 2002 issue of Aviation Week &
Space Technology.

In addition to navigating the first spacecraft to come close
to and orbit around an asteroid, the navigation team also
added orbits that were not part of the original plan, once
brushing by the asteroid just 2.7 kilometers (about 1.7 miles)
from the surface so that scientists could get more data about
the space rock.

The JPL navigation team included James K. Miller, Peter J.
Antreasian, Cliff E. Helfrich, William M. Owen, Jr., Eric
Carranza, Steven R. Chesley, Tseng-Chan Wang, Jon D. Giorgini,
and John J. Bordi.

More information on the Near Earth Asteroid Rendezvous mission
is available at

http://near.jhuapl.edu/

Launched on Feb. 17, 1996, the Near Earth Asteroid Rendezvous
mission was the first in NASA's Discovery Program of low-cost
planetary missions. The Johns Hopkins University Applied Physics
Laboratory designed and built the spacecraft. The mission team
includes members from JPL as well as Cornell University, Ithaca,
N.Y.; University of Maryland, College Park; Massachusetts
Institute of Technology, Cambridge; University of Arizona,
Tucson; the National Oceanic and Atmospheric Administration's
Space Environment Center, Boulder, Colo.; NASA's Goddard Space
Flight Center, Greenbelt, Md.; NASA's Solar Data Analysis Center,
Greenbelt, Md.; Malin Space Science Systems Inc., San Diego, Calif.;
Southwest Research Institute, San Antonio, Texas.; Northwestern
University, Evanston, Ill.; University of California, Los Angeles;
Catholic University, Washington, D.C.; Computer Sciences Corporation,
El Segundo, Calif.; and the Max Planck Institute for Chemistry,
Mainz, Germany.

JPL, a division of the California Institute of Technology,
manages many space missions for NASA's Office of Space Science,
Washington D.C.

April 16, 2002

 Crew Selected for Flashline Mars Arctic Research Station

The crew for the Flashline Mars Arctic Research Station (FMARS) for
the summer of 2002 has been selected. The crew, chosen from over 400
volunteers from around the world, comprises men and women in equal
numbers, and includes 3 Americans, two Germans, and 1 British
subject.

The crew will serve a 3-week rotation in the Flashline Mars Arctic
Research Station on Devon Island beginning July 6 and ending July 27.
During this time they will employ the Mars-like polar desert of
Canada's Devon Island to experiment with techniques for the human
exploration of Mars.

The following is the crew roster:

Dr. Robert Zubrin, Pioneer Astronautics, Astronautical Engineer, USA,
Commander
Nell Beedle, Fugro Seafloor Surveys, Geologist, USA
Dr. Frank Eckardt, University of Botswana, Geologist, German citizen
living in Botswana.
Shannon Hinsa, Dartmouth Medical School, Microbiologist, USA
Dr. Markus Landgraf, European Space Agency, Physicist, German
Emily MacDonald, Oxford University, Astrophysicist, British

The Mars Society thanks all those who volunteered. Additional crew
slots will be available in the Mars Desert Research Station, which
will open its fall season in Hanksville Utah in October.

A special session reporting devoted to crew reports on the activities
of the Flashline Mars Arctic Research Station and Mars Desert
Research Station will be held at the 5th International Mars Society
Convention, August 8-11 at the University of Colorado at Boulder.
Registration for the conference is now open at www.marssociety.org.

 PRESS BRIEFING SCHEDULED WITH NASA ADMINISTRATOR
AND ASTRONAUT BARBARA MORGAN

NASA Administrator Sean O'Keefe and astronaut Barbara
Morgan will hold a news conference from 10:15 a.m. to 10:45
a.m. EDT tomorrow, April 16, from NASA's Johnson Space Center
(JSC), Houston. The briefing will be carried live on NASA
Television with live question-and-answer capability from
participating NA\SA centers.

Friday, Administrator O'Keefe announced Morgan would fly on a
Space Shuttle mission to the International Space Station
shortly after the completion of the core elements of the
orbiting outpost.

Morgan was selected as a Mission Specialist member of the
Astronaut Class of 1998. Since then, she has undergone
training for spaceflight and currently serves as the
communications interface between Mission Control and the
Expedition Four Crew aboard the orbiting station.

Prior to joining NASA, Morgan served as the backup candidate
for the Teacher in Space Program and trained along with
Christa McAuliffe and the STS-51L crew of Challenger, which
was lost shortly after launch on Jan. 28, 1986.

Media wishing to cover the press conference at JSC should
notify the center's newsroom at 281/483-5111 NO LATER THAN 5
p.m. EDT today to arrange for credentials. Reporters should
arrive at JSC NO LATER THAN 9:30 a.m. EDT for badging and
escort.

NASA TV is available on GE-2, Transponder 9C, at 85 degrees
West longitude, vertical polarization, with a frequency of
3880 MHz and audio of 6.8 MHz.

April 15, 2002

 Radar reveals five double asteroid systems orbiting each other near Earth,
likely formed in close encounters with planet

ITHACA, N.Y. -- Binary asteroids -- two rocky objects orbiting about one
another -- appear to be common in Earth-crossing orbits, astronomers using
the world's two most powerful astronomical radar telescopes report. And it
is probable, they say, that these double asteroid systems have been formed
as a result of gravitational effects during close encounters with at least
two of the inner planets, including Earth.

Writing in a report published by the journalScience on its Science Express
web site (April 11, 2002), the researchers estimate that about 16 percent of
so-called near-Earth asteroids (NEAs) larger than 200 meters (219 yards) in
diameter are likely to be binary systems, with about a three-to-one relative
size of the two encircling bodies. To date, five such binary systems have
been identified by radar, says lead researcher Jean-Luc Margot, an O.K. Earl
postdoctoral fellow in the Division of Geological and Planetary Sciences at
the California Institute of Technology.

Margot, who at the time of the observations was a research associate in the
planetary studies/radar group at the National Science Foundation's (NSF)
Arecibo Observatory in Puerto Rico (managed at Cornell University), says
that theoretical and modeling results show the binary asteroids appear to be
formed extremely close to Earth -- within a distance equal to a few times
the planet's radius (6,378 kilometers or 3,963 miles). "The fact that one
out of every six large NEAs is a binary and that they typically survive on
the order of 10 million years, implies that these close encounters must
happen frequently compared to the lifetime of the binary asteroids," says
Margot.

The Science article, "Binary Asteroids in the Near-Earth Object Population,"
is coauthored by Michael Nolan, research associate at Arecibo; Lance Benner,
Steven Ostro, Raymond Jurgens, Jon Giorgini and Martin Slade at the Jet
Propulsion Laboratory (JPL); and Donald Campbell, professor of astronomy at
Cornell. The observations were made at the 70-meter Goldstone NASA tracking
telescope in California and at Arecibo Observatory.

NEAs are formed in the asteroid belt, between the orbits of Mars and
Jupiter, and nudged by the gravitational attraction of nearby planets,
largely Jupiter, into orbits that allow them to enter the Earth's
neighborhood. Most of the asteroids are the remnants of the initial
agglomeration of the inner planets.

Astronomers have long speculated about the existence of binary NEAs, based
in part on impact craters on Earth. Of about 28 known terrestrial impact
craters with diameters greater than 20 kilometers, at least three are double
craters formed by impacts of objects about the same size as the newly
discovered binaries. Astronomers also have noted the changes in brightness
of reflected sunlight for some NEAs, indicating a double system was causing
an eclipse or occultation of one by the other.

In 2000, Margot and his co-researchers, using measurements from the
Goldstone radar, found that a small, roughly 800-meter-diameter
(half-a-mile) asteroid, 2000 DP107 (discovered only months before by a team
from the Massachusetts Institute of Technology), was a binary system.
Observations over eight days last October with the much more sensitive
Arecibo telescope clearly established the physical characteristics of
DP107's two asteroids as well as their orbit about each other. The smaller
object called the secondary, it was found, is about 300 meters (1,000 feet)
in diameter and is orbiting the larger asteroid, the primary, every 42 hours
at a distance of 2.6 kilometers (1.6 miles). The two asteroids appear to be
locked in synchronous rotation, with the smaller always with the same face
oriented to the larger.

Since that observation, says Margot, four more binary NEAs have been
discovered, all in Earth-crossing orbits and each with a main asteroid
significantly larger than the smaller body. "The primary is rotating much
faster than most NEAs in all five binaries that have been discovered," says
Cornell's Campbell. The Science Express article speculates that the most
likely way the binaries are created is by close encounters of asteroids with
the inner planets Earth or Mars. Of the five binary NEAs discovered to date,
none has an orbit that brings it as close to the sun as Venus or Mercury.

NEAs, basically piles of rubble held together by gravity, are on
trajectories that bring them within a few thousand miles of the planets,
where tidal forces ---- essentially the pull of gravity -- can increase the
spin rate of the asteroid, causing it to fly apart. The ejected rubble then
reforms in orbit around the larger asteroid.

"The asteroid is already rotating very quickly as it approaches the planet.
A little extra boost from tidal forces can be enough to exceed its breakup
limits, and it sheds mass. This mass can end up forming another object in
orbit around the asteroid. Right now this seems the most likely
explanation," says Margot.

There is an important reason for studying binary asteroids, says JPL's
Ostro: their potential for colliding with Earth. Knowing the density of
so-called PHAs (for potentially hazardous asteroids), he observes, "is an
extremely important input to any mitigation plans." He says, "Getting NEA
densities from radar is dirt cheap compared with getting a density with a
spacecraft. Of course, the most important thing to know about any PHA is
whether it is two objects or one, and this is why we want to observe these
binaries with radar whenever possible."

Margot notes, "Radar gives us very precise measurements of the size of the
objects and their shape. The radar measurements of the distance and velocity
of each component allows us to obtain precise information on their orbits.
From this we can obtain the mass of each of the objects allowing, for the
Þrst time, measurements of NEA densities, a very important indicator of
their composition and internal structure."

Arecibo Observatory is operated by the National Astronomy and Ionosphere
Center at Cornell under a cooperative agreement with the NSF. The research
was supported by the NSF, with NASA providing additional support for the
planetary radar program at Arecibo.

Related World Wide Web sites: The following sites provide additional
information on this news release. Some might not be part of the Cornell
University community, and Cornell has no control over their content or
availability.

o Science Express: http://www.sciencexpress.org

o Images of binary asteroid 2000 DP107:

http://www.gps.caltech.edu/~margot/2000DP107

 A team from Fullerton's Troy High School wins a state contest for the eighth time

LONG BEACH, Ca, April 14 - One combed his hair forward. One let it hang down. One let it stick up.

Together, they lowered their purple goggles, waved the crowd back, counted to three and set off a chain reaction of meticulously planned mayhem.

A minute and twenty seconds later, it was over. As flashbulbs popped and parents closed in for embarrassing hugs, Peter Chueh, Peter Pawlowski and Derrick Tan, aspiring scientists at Fullerton's Troy High School, let out their breath.

"I can sleep tonight," said Chueh, surveying the smoking remains of a device that used circuits, matches, old CDs and a tangle of wiring to set off as many combustions as possible in less than two minutes.

The boys, whose appearance ranged from Chueh's long-haired cool look to Pawlowski's slightly scruffier fashion indifference, had just spent five months of sleepless nights and blissful afternoons crafting the science experiment that would help propel their school to the top of the 18th annual California Science Olympiad.

The event, which drew about 2,000 students, teachers and parents from 53 Southern California junior high and high schools to California State University, Long Beach on Saturday, was the eighth won by Troy. El Rancho Middle School of Anaheim Hills posted its fifth win in the junior high category.

Both schools will travel to the University of Delaware next month for the national finals, which Troy won in 1996, 1999 and 2000, but lost last year by one agonizing point. This year, students vowed to exact revenge.

"These are the kinds of kids you make fun of on some campuses," said teacher Dan Jundanian, pointing to the 15-member Troy team he helped coach. "But these are the kids you'll be working for some day."

At 9 a.m., each team was given instructions for 23 tests ranging from making musical instruments from scratch to exams on topics like planimetric maps. Some events, like the combustion machine, allowed students to make their devices ahead of time. Others, like a test of weather knowledge, required them to solve problems on the spot.

The competition can push already ambitious, high-strung students to the breaking point, especially when high-powered schools like Troy go head to head with formidable rivals like Torrey Pines High School of San Diego.

As Killeen Kirkconnell, a 16-year-old Torrey Pines student, sat doodling furiously in the robot competition room, she sheepishly admitted she was spying on other schools' designs. Chueh conceded he had dropped by the San Diego regional finals recently to probe Torrey Pines' weaknesses.

Other schools were less serious. For every student like MIT-bound Derek Tan, there was a Kate Cheney from Fullerton, who said she divides her time between the Ladera Vista Junior High science and soccer teams, and had eschewed the event-issued white lab coat in favor of bell-bottom jeans and a sweatshirt reading, "Heavenly."

"I don't think we'll do very well," Cheney said, conceding that science-team membership is not exactly a route to social stardom at Ladera Vista.

The situation is slightly different at Troy, where Tan said the science squad holds a status most schools reserve for "a really good sports team. People admire it. Lots of people want to be on it."

This, after all, is the school where students often spend more of their spring break on campus than off. Nancy Chen and Angie Shih, Troy 16-year-olds who effortlessly rattled off a portion of Bidet's "Carmen" in the homemade-instrument contest, said they spent much of their recent vacation honing their performance.

As for pressing questions, like whether being on the science team helps land a date, these mathematical minds were firmly made up.

"Uh, no," said Janet Lee, 17, of Troy. "I don't know anyone who would say, 'He's on the Science Olympiad, I've got to ask him out.'

"Most people at our school aren't very into that. They're more into academics."

Competition winners

Top five junior high and high school finishers at the 18th annual California Science Olympiad.

Junior High School:

1. El Rancho Middle School, Anaheim Hills

2. Ladera Vista Middle School, Fullerton

3. Joe Walker Middle School, Los Angeles

4. Muirlands Middle School, San Diego

5. Black Mountain Middle School, San Diego

High School:

1. Troy High School, Fullerton

2. Torrey Pines High School, San Diego

3. Mount Carmel High School, San Diego

4. North Hollywood High School, Los Angeles

5. Villa Park High School, Villa Park

April, 14 2002

 LAKE ONTARIO DATA BUOY WILL PROVIDE MORE DATA TO FORECASTERS, MARINE
COMMUNITY

A new data buoy, deployed last week in central Lake Ontario by the National
Oceanic and Atmospheric Administration (NOAA) will provide added critical,
real-time weather observations that local National Weather Service (NOAA
Weather Service) meteorologists said would help improve forecasts and
increase safety for mariners. NOAA is an agency of the Commerce Department.
The National Data Buoy Center (NDBC), part of NOAA Weather Service, and the
Canadian Coast Guard combined efforts to deploy the new buoy 30 miles
northeast of Rochester, N.Y. The buoy, identified as 45012, is the ninth
NDBC buoy in the Great Lakes, joining two others in Lake Ontario operated
by the Meteorological Service of Canada.

"The Great Lakes region creates fast-changing weather conditions that can
be frightening if you're out on the water," said Darin Figurskey,
meteorologist in charge of the NOAA Weather Service forecast office in
Buffalo, N.Y. "Having another buoy to give real-time observations about
wind speed, wave heights and temperature will help us deliver better
forecasts."

The new buoy's observations will be relayed through the Geostationary
Operational Environmental Satellite to computers at NOAA Weather Service
headquarters in Silver Spring, Md. From there, the observations will be
transmitted to local weather forecast offices, international weather
agencies and the private sector.

"Mariners make decisions based on the buoy observations and marine
forecasts they receive," said Dave Gilhousen, an NDBC meteorologist. "It's
crucial for these observations to be accurate and timely."

The buoy's real-time weather observations will be posted under the Recent
Data Section of the NDBC's Web site,
http://www.ndbc.noaa.gov. The latest
observations also will be available through the Dial-A-Buoy system, (228)
688-1948.

The NDBC, located at Stennis Space Center in Mississippi, first began
deploying weather buoys in the Great Lakes in 1979, after the sinking of
the Edmund Fitzgerald. NOAA Weather Service is the primary source of
weather data, forecasts and warnings for the United States and its
territories. NOAA Weather Service operates the most advanced weather
warning and forecast system in the world, helping to protect lives and
property and enhance the national economy.

NOAA Weather Service is the primary source of weather data, forecasts and
warnings for the United States and its territories. NOAA Weather Service
operates the most advanced weather and flood warning and forecast system in
the world, helping to protect lives and property and enhance the national
economy. To learn more about the NOAA Weather Service, visit:
http://www.weather.gov.

 http://sci.esa.int/content/news/index.cfm?aid=1&cid=1&oid=29787

European Space Agency to probe asteroid blind spot
European Space Agency

In the past five weeks two asteroids have passed close by Earth,
at distances of 1.2 and 3 times the distance to the Moon. Another asteroid
has recently been shown to be on course for a collision with Earth in 2880.
Monitoring known asteroids allows astronomers to predict which may collide
with Earth. But that is only true for the asteroids we know of. What about
those that lie in the asteroid blind spot between the Sun and Earth? The
European Space Agency is studying ways in which its missions can assist in
monitoring these unseen but potentially hazardous asteroids.

It is difficult to estimate the danger posed by asteroids. This is, in part,
because astronomers do not yet know how many asteroids there are. A recent
discovery, made using data from ESA's Infrared Space Observatory (ISO),
showed that there could be nearly two million asteroids larger than one
kilometre in the main asteroid belt, between Mars and Jupiter. That is more
than twice as many as previously thought.

In addition, even when an asteroid is identified many observations must be
made before it is known whether or not it will come close to, or even
collide with, Earth.

If the asteroids remained in the main-belt, they would pose no danger to
Earth. However, they can be thrown into different orbits by collisions with
other asteroids or by the influence of Jupiter's gravitational field. If
their new orbits cross the Earth's orbit, they could one day collide with
our planet, inflicting unprecedented devastation.

A number of ground-based searches are already underway to find as many
potentially hazardous asteroids (PHAs) as possible but there is a notorious
'blind spot' that telescopes on Earth can never peer into. It is the region
of space inside Earth's orbit, towards the Sun. From Earth, astronomical
observations close to the Sun are almost impossible because it means
observing during the daytime when only the brightest celestial objects stand
out from the blue sky. That means asteroids lurking in this region of space
can 'sneak up' on the Earth undetected. Asteroid 2002 EM7, which passed
close by the Earth on 8 March this year, was one such object and was only
detected after it crossed Earth's orbit to appear briefly in the night sky,
before it crossed back into the glare of the Sun.

About 550 similar asteroids are known. They are called the Atens and spend
most of their time inside Earth's orbit, close to the Sun. Traditional
estimates suggest there may be several thousand in total and tracking them
from Earth is next to impossible. However, a study performed for ESA has
shown that the Gaia spacecraft will be able to see clearly into this 'blind
spot' and keep precise track of the Aten population.

François Mignard of Observatoire de la Côtes d'Azur, France, conducted the
study. He found that Gaia would be ideal because it is designed to measure
the position of celestial objects with unprecedented accuracy. In addition,
since there is no atmosphere in space to scatter the Sun's rays and create a
blinding blue sky, Gaia can see close to the Sun without disturbance.

Gaia is expected to be launched around 2010. Even if ground-based searches
have spotted more Atens by that time, the mission still has an essential
role to play because it will reveal their orbits to a precision 30 times
better than any observation from the ground, thus identifying whether any
pose a danger to Earth.

"To know how close these objects will come to Earth is very dependent on how
accurately one can measure their orbits. That's the main contribution that
Gaia can be expected to make," says Michael Perryman, project scientist for
Gaia, at ESA's European Space Research and Technology Centre in the
Netherlands.

Gaia's data will also provide astronomers with a first estimate of these
objects' composition. This knowledge could help to determine methods to
divert or destroy asteroids that are set on a collision course with Earth.

Several ESA missions are contributing, or will contribute, to our
understanding of minor bodies of the Solar System: these include ISO, Gaia
and Rosetta, which will study asteroids Siwa and Otawara. ESA is also
considering the addition of an asteroid spotting telescope to its
BepiColombo mission.

April 13, 2002

 SIBLING RIVALRY? CHILIQUES, THREE SISTERS VOLCANOES SHOW SIGNS OF LIFE

Previously dormant volcanoes in two widely separated areas of the Pacific "ring of
fire" are showing signs of life, as documented by new images taken by the Advanced
Spaceborne Thermal Emission and Reflection Radiometer (Aster) on NASA's Terra
satellite.

The images are available at:

http://www.jpl.nasa.gov/images/earth/volcano/index.html .

Geologists had previously considered Chiliques, a simple 5,778-meter (18,957-foot)
stratovolcano with a 500-meter (1,640-foot)-diameter circular summit crater in northern
Chile, to be dormant. However, a January 6, 2002 nighttime thermal infrared image from
Aster found a hot spot in the summit crater, as well as several others along the upper flanks
of the volcano's edifice, indicating new volcanic activity. Examination of an earlier
nighttime thermal infrared image from May 24, 2000 showed no such hot spots.

Stratovolcanoes such as Chiliques account for approximately 60 percent of Earth's
volcanoes. They are marked by eruptions of cooler, stickier lavas such as andesite, dacite
and rhyolite. Because these lavas tend to plug up volcanic plumbing, gas pressures can
more easily build up to high levels, often resulting in explosive eruptions. They are
typically made up of about half lava and half loose or fragmented rock ejected from the
volcano, and are therefore also commonly known as composite volcanoes. Mount Saint
Helens in Washington and Mount Pinatubo in the Philippines are examples of
stratovolcanoes.

The daytime image of Chiliques was acquired on November 19, 2000 and was
created by displaying Aster bands 1, 2 and 3 in blue, green and red. The nighttime image is
a color-coded display of a single thermal infrared band. The hottest areas are white, and
colder areas are darker shades of red. Both images cover an area of 7.5 by 7.5 kilometers
(4.7 by 4.7 miles), and are centered at 23.6 degrees south latitude, 67.6 degrees west
longitude.

Meanwhile, a couple of thousand miles to the northwest, a 10-by-20-kilometer (6.2-
by-12.4-mile) section of ground near one of the long-dormant Three Sisters volcanoes in
the Cascade Mountains of west-central Oregon has risen approximately 10 centimeters
(3.94 inches) since 1996. According to the U.S. Geological Survey, this indicates the slow
flow of magma or underground lava into the area. A simulated natural color image from
Aster has been draped over digital topography from the U.S. Geological Survey National
Elevation Dataset to create this new perspective view of Three Sisters.

The Three Sisters area -- which contains five volcanoes -- is only about 273.6
kilometers (170 miles) from Mount St. Helens, which erupted in 1980. Both are part of the
Cascades Range, a line of 27 volcanoes stretching from British Columbia in Canada to
northern California.

With its 14 spectral bands from the visible to the thermal infrared wavelength
region, and its high spatial resolution of 15 to 90 meters (about 50 to 300 feet), Aster will
image Earth for the next six years to map and monitor the changing surface of our planet.

Aster is one of five Earth-observing instruments on Terra, and is its only high-
resolution imaging sensor. Japan's Ministry of Economy, Trade and Industry built the
instrument. JPL is responsible for the American side of the joint U.S.-Japan science team
that is validating and calibrating the instrument and data products.

Aster's broad spectral coverage and high spectral resolution will provide scientists
in numerous disciplines with critical information for surface mapping, and monitoring
dynamic conditions and temporal change. Example applications are: monitoring glacial
advances and retreats; monitoring potentially active volcanoes; identifying crop stress;
determining cloud morphology and physical properties; evaluating wetlands; monitoring
thermal pollution; monitoring coral reef degradation; mapping soil and geology surface
temperatures; and measuring surface heat balance.

More information on Aster is available at:

http://asterweb.jpl.nasa.gov .

NASA's Earth Science Enterprise is a long-term research and technology program
designed to examine Earth's land, oceans, atmosphere, ice and life as a total integrated
system.

JPL is a division of the California Institute of Technology in Pasadena.

 MARS ODYSSEY THEMIS IMAGES
April 8-13, 2002

o Gorgonum Chaos (Released 8 April 2002)
o Uzboi Vallis, Nirgal Vallis, and Luki Crater (Released 9 April 2002)
o Medusae Fossae Formation (Released 10 April 2002)
o Southern rim of Isidis Planitia basin (Released 11 April 2002)
o The so-called "Face on Mars" (Released 13 April 2002)

Note: These images have not been radiometrically nor geometrically calibrated
for this preliminary release. An empirical correction has been performed to
remove instrumental effects. A linear shift has been applied in the
cross-track and down-track direction to approximate spacecraft and planetary
motion. Fully calibrated and geometrically projected images will be released
through the Planetary Data System in accordance with Project policies at a
later time.

NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for
NASA's Office of Space Science, Washington, D.C. The Thermal Emission
Imaging System (THEMIS) was developed by Arizona State University, Tempe, in
collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS
investigation is led by Dr. Philip Christensen at Arizona State University.
Lockheed Martin Astronautics, Denver, is the prime contractor for the
Odyssey project, and developed and built the orbiter. Mission operations are
conducted jointly from Lockheed Martin and from JPL, a division of the
California Institute of Technology in Pasadena.

Image Credit: NASA/JPL/Arizona State University

----------------------------------------------------------------------------

http://themis.asu.edu/zoom-20020408a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
Gorgonum Chaos (Released 8 April 2002)

This image shows the cratered highlands of Terra Sirenum in the
southern hemisphere. Near the center of the image running from left to
right one can see long parallel to semi-parallel fractures or troughs
called graben. Mars Global Surveyor initially discovered gullies on the
south-facing wall of these fractures. This image is located at 38°S,
174°W.

----------------------------------------------------------------------------
http://themis.asu.edu/zoom-20020409a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
Uzboi Vallis, Nirgal Vallis, and Luki Crater (Released 9 April 2002)

This THEMIS image captures two channels (Nirgal Vallis the smaller sinuous
channel on the left and Uzboi Vallis the larger channel located in the
lower right) and Luki Crater located in the upper right. The mouth of Nirgal
Vallis appears to be truncated by Uzboi Vallis. This indicates that Nirgal
Vallis is an older channel than Uzboi Vallis. The floor of Uzboi Vallis was
subsequently bombarded by an asteroid or comet which gouged out the 21 km
diameter crater named Luki. Luki is named after a town in the Ukraine. Uzboi
is the name of a dry river in Russia. Nirgal is the Babylonian name for Mars.
Gullies and alluvial deposits discovered by Mars Global Surveyor are clearly
visible on the polar-facing (south) wall and floor of Nirgal Vallis and also
in the inner rim of Luki crater. These gullies appear to emanate from a
specific layer in the walls. There is a pronounced sparsity of gullies on
the equator-ward facing slopes but some are present in this image. The
gullies have been proposed to have formed by the subsurface release of water.
The western channel wall of Uzboi Vallis does not appear to have the
fine-scale gullying as does Nirgal Vallis. However, the western channel wall
of Uzboi Vallis does show some evidence of downslope movement (mass wasting).
Some patches of dunes are also seen on the channel floor, notably along the
edges of the channel floor near the canyon walls. There is also a landslide
located along the southern wall of Luki Crater. '

----------------------------------------------------------------------------
http://themis.asu.edu/zoom-20020410a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
Medusae Fossae Formation (Released 10 April 2002)

The Story

Medusa of Greek mythology fame, the name-giver to this
region, had snaky locks of hair that could turn a person to stone.
Wild and unruly, this monster of the underworld could certainly
wreak havoc on the world of the human imagination. As scary
as she was, Medusa would have no advantage over the fierce,
masterful winds blowing across Mars, which once carved the
streaky, terrain at the top of this image. Wild and whipping,
these winds have slowly eroded away the "topsoil," revealing
ancient craters and other surface features they once covered.
The loosely cemented particles of this "topsoil" are likely made
up of dust or volcanic ash, and are thus more susceptible to
windblown erosion. The Martian winds have actually been
strong and relentless enough over time to strip the land in the
bottom of this image of the material that once covered it, leaving
it hard and bare to the eye.

The Science

This THEMIS visible image was acquired near
7° S, 172° W and shows a remarkable martian
geologic deposit known as the Medusae Fossae
Formation. This Formation, seen here as the
raised plateau in the upper two-thirds of the
image, is a soft, easily eroded deposit that
extends for nearly 1,000 km along the equator of
Mars. In this region the deposit has been heavily
eroded by the wind to produce a series of linear
ridges called yardangs. These parallel ridges
point in direction of the prevailing winds that
carved them, and demonstrate the power of
martian winds to sculpt the dry landscape of
Mars. The Medusae Fossae Formation has been
completely stripped from the surface in the lower
third of the image, revealing a harder layer below
that is more resistant to wind erosion. The easily
eroded nature of the Medusae Fossae Formation
suggests that it is composed of weakly cemented
particles, and was most likely formed by the
deposition of wind-blown dust or volcanic ash.
Several ancient craters that were once
completely buried by this deposit are being
exposed, or exhumed, as the overlying Medusae
Formation is removed. Very few impact craters
are visible on this Formation, indicating that the
surface seen today is relatively young, and that
the processes of erosion are likely to be actively
occurring.

----------------------------------------------------------------------------
http://themis.asu.edu/zoom-20020411a.html

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
Southern rim of Isidis Planitia basin (Released 11 April 2002)

The Story

Battered and beaten up, the surface of Mars reads like a
history book to geologists, who want to study what has
happened to the red planet over its geological history. Look
for two larger craters diagonal from one another in the
northern part of this image, and then for the smattering of
tinier craters near them. How did these smaller craters come
to be? Did a large meteoroid streak in through the Martian
atmosphere and get broken up as it passed through,
pummeling Mars moments later with its smaller, scattered
pieces? Or were rocks and dirt blasted off the surface when
the two larger craters were formed, only to rain down again on
Mars shortly afterwards? No one quite knows for sure....

Another enigmatic-looking feature is near the left center of
this image. Dark and shadowy-seeming, it looks something
like an exclamation point with the small crater just below it.
Look closely, and you'll see dunes within the large, dark,
blurry patch, which is itself probably composed of moving
sands. Dark, streaky features also appear on the eastern side
of the ridge that runs down the right side of the image,
showing how debris once tumbled down its steepened slopes

 

The Science

This image, crossing the southern rim of the
Isidis Planitia basin, displays the contrasting
morphologies of the relatively rough highland
terrain (in the lower portion of the image) and the
relatively smooth materials of the basin (at top).
Upon closer viewing, the basin materials display
an extensive record of cratering, including a small
cluster of craters just north and west of the two
prominent craters in the upper part of the image.
This cluster of craters may represent what are
called 'secondary' craters, which are craters that
form as a result of the ejection of debris from a
nearby impact. Alternatively, these craters may
have formed simultaneously by the impact of
many pieces of a larger meteoroid that broke up
upon entry into Mars' atmosphere. The large
craters in the image are approximately 800
meters (~875 yards) in diameter. Also visible in
the image are dark streaks on the east-facing
side of the north-south trending ridge. These
streaks are likely the result of debris movement
down slope. A dark patch of material is visible at
the left of the image; dark materials are typically
mobile sands, and linear duneforms are apparent
within the dark patch.

----------------------------------------------------------------------------

Mars 2001 Odyssey
Thermal Emission Imaging System (THEMIS)
The so-called "Face on Mars" (Released 13 April 2002)

The Story

Nature is an imaginative artist, creating all kinds of wonderful
landforms, cloud shapes, and other patterned features that
remind people of familiar things in our lives. We see a "man in
the moon" when it is full in the night sky, and dream of a
dromedary-dotted desert when coming upon Arizona's
Camelback Mountain or Colorado's "Kissing Camels" in the
"Garden of the Gods." Near Ludlow, California, a lonely
prospector once noticed that the appealing outline of the
mountains resembled a reclining woman, and named the place
Sleeping Beauty. And this naming delight isn't limited to
Earth. The Mars Pathfinder mission team couldn't help but
name the rocks at the landing site, including a
bear-headed-looking one named Yogi.

Part of the fun of exploration is not just visiting a strange
world, but relating to it in human terms. On Mars, we've
already seen a valentine heart-shaped crater, a happy-faced
crater, and even a murky and mysterious "face" on Mars. This
face (seen here about halfway down the image and to the
right) is really just a hill with slopes and ridges that are
shadowed in a way that can sometimes resemble a face from
far away. The first picture of this area was taken by the Viking
spacecraft in the 1970s, and people have been intrigued ever
since. However, orbiter camera technologies have actually
become so good in providing a clear view of the hill that it's
almost a disappointment to see how normal an eroded hill this
well-liked feature is. Well, disappointing unless you're a
geologist, that is!

This whole area is, in fact, a geologist's dream. Erosion has
been Nature's sculptor throughout the area, and all kinds of
remarkably shaped knobs and hills speckle the region. While
their shapes are fun to contemplate, it's no mystery to
geologists how they formed. Several flat ledges part way up
the slopes of these hills are made of layers of rock that stand
strong against erosion's relentless carving. Less resistant
layers in the region have eroded away completely in most
places, leaving behind only the small, isolated hills and knobs
we see today. Don't think everything in this scene is easily
understandable, however. What captures the attention of
scientists is a bunch of unusual deposits of material on the
cold, north-facing slopes of the hills. Did Nature mix some
Martian dirt and ice from the planet's "pallet," and then
"paste" on a slightly cemented deposit over the northern
slopes? Or did an upper layer of material slowly creep
downslope over time, carried by the movement of ice? Ground
ice, in this case, has probably been more of a preserver than an
eroder, keeping a record of the formation and existence of
these deposits over time. Geologists are grateful for that peek
into the Martian past and the chance to study it in-depth.

The Science

The so called "Face on Mars" can be seen
slightly above center and to the right in this
THEMIS visible image. This 3-km long knob,
located near 10° N, 40° W, was first imaged by
the Viking spacecraft in the 1970's and was
seen by some to resemble a face carved into the
rocks of Mars. Since that time the Mars Orbiter
Camera on the Mars Global Surveyor spacecraft
has provided detailed views of this hill that
clearly show that it is a normal geologic feature
with slopes and ridges carved by eons of wind
and downslope motion due to gravity. A
similar-size hill in Phoenix, Arizona resembles
a camel lying on the ground, and Phoenicians
whimsically refer to it as Camelback Mountain.
Like the hills and knobs of Mars, however,
Camelback Mountain was carved into its
unusual shape by thousands of years of erosion.
The THEMIS image provides a broad
perspective of the landscape in this region,
showing numerous knobs and hills that have
been eroded into a remarkable array of different
shapes. Many of these knobs, including the
"Face", have several flat ledges partway up the
hill slopes. These ledges are made of more
resistant layers of rock and are the last
remnants of layers that once were continuous
across this entire region. Erosion has
completely removed these layers in most places,
leaving behind only the small isolated hills and
knobs seen today.

Many of the hills and ridges in this area also
show unusual deposits of material that occur
preferentially on the cold, north-facing slopes. It
has been suggested that these deposits were
pasted on the slopes, with the distinct,
well-defined boundary on their upslope edges
being the highest point of this pasted-on layer.
Alternatively, these unique features could be the
result of the slow downslope motion of the
surface layer, possibly enhanced by the
presence of ground ice. In this model the top
layer of material has separated from the
sub-surface near the crest of the slope and
moved downslope, creating the rounded
boundary seen at the top of the detached layer.
In several cases, such as in the large knob
directly south of the "Face" these deposits occur
at several different heights on the hill, providing
evidence that downslope motion may be the
more likely explanation. In either case, ground
ice likely plays an important role in the formation
and preservation of these deposits because they
only occur on the cold slopes facing away from
the Sun where ground ice is more stable and
may still be present today.

This image is the 13th image in a series of daily
images released by the THEMIS Team.

 NASA Science News for April 12, 2002

Scientists have learned that April and May are the best months to spot one
of the loveliest sights in the heavens: Earthlight reflected from the
Moon. A good observing opportunity is just around the corner.

FULL STORY at

http://science.nasa.gov/headlines/y2002/12apr_earthshine.htm?list448368

 Canadarm2 on the Job

Saint-Hubert, Quebec, April 12, 2002 - Marc Garneau, President of the
Canadian Space Agency (CSA) reports that Canadarm2 successfully completed
yesterday's operations on the International Space Station as planned.
Mission Specialist Ellen Ochoa, assisted by Expedition Four Flight Engineer
Dan Bursch, operated Canadarm2 to lift a major truss segment out and away
from Shuttle Atlantis' cargo bay and attach it on the Destiny laboratory
module of the International Space Station. Canadarm2 was then used for the
first time to move Mission Specialist Rex Walheim to different worksites
around the newly installed truss segment during the first spacewalk of
mission STS-110, which lasted 7 hours and 48 minutes.

Teams of engineers from the CSA and MD Robotics, prime contractor for
Canadarm2, were closely monitoring the arm's first major assembly activity
since an anomaly was detected on one of its joints several weeks ago. The
engineers developed a software patch that successfully bypassed the joint in
the arm's primary channel. In actual fact, Canadarm2's secondary channel was
used to execute all of yesterday's operations. "Canadarm2 is a unique and
highly complex robot working in an extremely hostile environment. Problems
are bound to occur and are part of the normal course of space activities.
Thanks to the team of engineers in St. Hubert and Brampton, Canadarm2
operations went smoothly and flawlessly yesterday," said Garneau.

To return Canadarm2 to full redundancy, a spare joint will be transported to
the Station onboard Mission STS-111, scheduled to launch May 31. On this
mission, two astronauts will replace the malfunctioning wrist roll joint
during a spacewalk. They are currently being trained for this new task. "We
have anticipated this type of situation, that's why Canadarm2 has been
designed in a way that allows astronauts to replace its parts on orbit
during its lifetime, and why spare components are ready to go at a moment's
notice, " added Garneau. Mission STS-111 will also transport the second
major Canadian element to the ISS: the Mobile Base System.
About the Canadian Space Agency

Established in 1989 with its headquarters situated in Saint-Hubert, Quebec,
the Canadian Space Agency co-ordinates all aspects of the Canadian Space
Program. Through its Space Knowledge, Applications and Industry Development
business line, the CSA delivers services involving: Earth and the
Environment; Space Science; Human Presence in Space; Satellite
Communications; Space Technology; Space Qualification Services and
Awareness. The Canadian Space Agency is at the forefront of the development
and application of space knowledge for the benefit of Canadians and
humanity.

 ADMINISTRATOR UNVEILS FUTURE NASA VISION
AND A RENEWED JOURNEY OF LEARNING

In his first major address since being sworn into
office, NASA Administrator Sean O'Keefe today outlined his
strategic vision for the agency's future, including a
component designed to inspire and educate a new generation of
explorers and scientists.

The Administrator shared his vision of NASA's future in a
speech at the Maxwell School of Citizenship and Public
Affairs, located on the campus of Syracuse University. U.S.
Rep. Sherwood L. Boehlert, who oversees the agency as
Chairman of the House Science Committee, and U.S. Rep. James
T. Walsh, who heads the House subcommittee that supervises
NASA's budget, both of New York, joined Administrator O'Keefe
at Maxwell.

"The nation faces extraordinary new challenges. The world is
changing, and if NASA is going to exploit these new
opportunities then America's space program must also change,"
said Administrator O'Keefe. "Our future decisions will be
science-driven, not destination-driven. The investments we
make today must be justified by their contributions to the
long-range goals of the agency."

Administrator O'Keefe spelled out NASA's vision and mission:

The new NASA vision for the future is:

To improve life here,
To extend life to there,
To find life beyond

The NASA mission is:

To understand and protect our home planet
To explore the Universe and search for life
To inspire the next generation of explorers
as only NASA can

In his speech titled "Pioneering the Future," Administrator
O'Keefe outlined the importance of inspiring a new generation
of explorers through education. "Education is part of our
core mission," added Administrator O'Keefe.

In an effort to take students on a new journey of learning,
the Administrator unveiled plans for a new type of space
explorer -- an Educator Mission Specialist. Shortly after
completion of the core elements of the International Space
Station in 2004, NASA will send Barbara Morgan, the agency's
first Educator Mission Specialist, into space.

Morgan was selected as the backup candidate in 1985 for the
Teacher in Space program. She trained side-by-side with
Christa McAuliffe and the Challenger crew at the NASA Johnson
Space Center in Houston. The Teacher in Space program ended
when Challenger exploded Jan. 28, 1986, killing McAuliffe and
her six crewmates.

"The time has come for NASA to complete the mission -- to
send an educator to space to inspire and teach our young
people," Administrator O'Keefe said. "Working in partnership
with Education Secretary Rod Paige, we will make Barbara's
flight the first in a series of missions in the new Educator
in Space program."

Administrator O'Keefe said it is fitting that Morgan complete
the mission of STS-51L. "For the past 16 years, Barbara has
worked with NASA and countless science organizations, keeping
alive Christa McAuliffe's inspiration. She is uniquely
qualified to take our students on a journey of education that
only NASA could make possible."

The new vision for the agency builds on NASA's unique
capabilities as the nation's premiere aeronautics and
aerospace research and technology organization. "The biggest
difference is that we will let specific science objectives
tell us where to go," concluded Administrator O'Keefe.
"NASA's mission of discovery will be carried out with a new
commitment to fiscal responsibility and the synergy that
comes from working with other government agencies, private
industry and academia."

The complete text of the Administrator's address and
additional supporting material are available on the Internet
at:
http://www.nasa.gov/bios/vision.html

Additional information about Education Mission Specialist
Barbara Morgan is online at:
http://www.jsc.nasa.gov/Bios/htmlbios/morgan.html

 In the past five weeks two asteroids have passed close by Earth.
Another asteroid has recently been shown to be on course for a
collision with Earth in 2880. Monitoring known asteroids allows
astronomers to predict which may collide with Earth. But that is
only true for the asteroids we know of. What about those that lie
in the asteroid blind spot between the Sun and Earth?
The European Space Agency is studying ways in which its missions can
assist in monitoring these unseen but potentially hazardous asteroids.

Read more about this at:
http://sci.esa.int/content/news/index.cfm?aid=1&cid=1&oid=29787

 ITHACA, N.Y. -- Carolyn S. Shoemaker, the world's most successful
living "comet hunter," will speak at Cornell University Sunday, April
21, at 1 p.m. in the David L. Call Alumni Auditorium, Kennedy Hall.
The talk is free and is open to the public.

The subject of the talk, which is aimed at science educators, will be
asteroid and comet collisions within the solar system. The talk is
sponsored by NASA's Comet Nucleus Tour (Contour) and the central and
southern sections of the Science Teachers Association of New York
State. Contour, which is scheduled for launch July 1, is managed by
the Applied Physics Laboratory at the Johns Hopkins University, with
Cornell's Department of Astronomy leading the science team.

Shoemaker, who has discovered more than 300 asteroids and 32 comets,
is probably best known for her 1993 co-discovery of the
Shoemaker-Levy 9 comet, which in 1994 collided with Jupiter. The
collision gave planetary scientists the most spectacular and most
widely studied solar system event in history, as each of the comet's
23 individual fragments collided with the giant planet over a number
of days.

Today, astronomers have identified a large population of near-Earth
asteroids and comets and are aware of more than 160 impact
structures, such as craters, on Earth where these objects have
crashed into our planet. A new period of solar system exploration is
beginning, Shoemaker says, thanks to new methods of searching the
skies and studying objects.

Shoemaker, who estimates she puts in 100 search hours for each comet
she finds, studied history and political science, taught high school
and raised three children before she launched her career as a comet
hunter at age 51. She continues to search for asteroids and comets
and to study ancient impact structures at Lowell Observatory in
Flagstaff, Ariz.

For her comet discoveries, she has won the Rittenhouse Medal of the
Rittenhouse Astronomical Society, and in 1990 she was awarded an
honorary doctorate of science by Northern Arizona University in
Flagstaff. She is the widow of the late astronomer Eugene Shoemaker,
who as chief scientist at the United States Geological Survey Center
of Astrogeology played a leading role in organizing geological
activities for the lunar landings of the late 1960s and early 1970s.

 Cassini Significant Events
for 04/04/02 - 04/10/02

The most recent spacecraft telemetry was acquired from the Goldstone
tracking station on Wednesday, April 10. The Cassini spacecraft is in an
excellent state of health and is operating normally. Information on the
present position and speed of the Cassini spacecraft may be found on the
"Present Position" web page located at
http://saturn.jpl.nasa.gov/cassini/english/where/ .

Instrument activities this week included periodic instrument maintenance
for the Radio and Plasma Wave Science subsystem, and an Ultraviolet
Imaging Spectrograph Hydrogen Deuterium Absorption Cell conditioning
exercise. The purpose of conditioning is to regularly exercise the H
and D cell filaments. Additional spacecraft activities included clearing
of the ACS high water marks, and an ACS periodic engineering maintenance
(PEM). The PEM contains the main engine gimbal actuator exercise,
Backup ALF Injection Loader maintenance, and backup reaction wheel
exercise. Results of the PEM were as expected.

The first Science Planning Team input port for C33 occurred this week.
Process output files will now be merged and delivered to ACS for
pointing validation runs.

A Saturn Orbit Insertion (SOI) Target Working Team met for the first
time this week. Integration work has begun on the period immediately
following SOI. A Science Operations Plan (SOP) implementation Tiger Team
met to explore an alternate approach of developing four tour sequences
in two Science Planning Team processes. Some issues were identified and
will be worked over the next couple of weeks. In general, this approach
was agreed to be a good option since it reduces the number of processes
and overhead associated with implementing the SOP.

The Spacecraft Office held a maneuver wrap-up meeting after Trajectory
Correction Maneuver (TCM) 18. At this meeting it was confirmed that the
TCM performance was nominal. The team reviewed the new tour processes
that were used in the design of this TCM to identify desired
improvements or lessons learned.

A Flight Software Monthly Management Review was held this week.
Development progress for Saturn Orbit Insertion, Huygens Probe Relay,
ACS flight software, and CDS flight software were reviewed. All items
are proceeding as scheduled.

Uplink Operations personnel made a presentation to Program Management
for performing a tour Science and Sequence Uplink Process (SSUP)
Verification and Validation (V&V) activity in mid 2003. A series of
smaller pre-tests and demonstrations was proposed, culminating in a
full-up SSUP demonstration mid-year.

To make the needed personnel available, the proposal included plans to
create a minimal set of activities in C38, moving most of them into C37
and C39. V&V would then be performed during the C38
development/execution period. Program Management approved the plan, and
directed the team to proceedas proposed.

All of the planned Mission Sequence Subsystem D8 deliverable
applications are in hard-freeze and system testing is proceeding as
planned. May 8, 2002, is still a firm date for the delivery to support
the May 13, 2002, start of Science Operations Plan integration.

User acceptance testing for the Cassini adaptation of the Command System
Version 26.4 was completed this week. An in-flight demonstration was
also performed. Additional demonstrations have been scheduled for mid
April and early June.

A scale model of the Huygens Probe is now on loan to the Space Center
Museum in Houston, Texas. The model will be part of a summer exhibition
and will be returned to the Space Flight Operations Facility at JPL for
display in September.

Cassini is a cooperative project of NASA, the European Space Agency and
the Italian Space Agency. The Jet Propulsion Laboratory, a division of
the California Institute of Technology in Pasadena, Calif., manages the
Cassini mission for NASA's Office of Space Science, Washington, D.C.

Cassini Outreach
Cassini Mission to Saturn and Titan
Jet Propulsion Laboratory
California Institute of Technology
National Aeronautics and Space Administration

CHANGING ANTARCTICA VIEWED BY NASA SATELLITE

NASA instruments flying on the Terra satellite have
observed the calving of an iceberg and the breakup of an ice
shelf in Antarctica, roughly 2,100 kilometers (1,300 miles)
from one another.

Last month, a large crack developed in the Thwaites
Tongue, a large sheet of glacial ice that extends from the
West Antarctica mainland into the southern Amundsen Sea. A
piece broke away, or calved, forming an iceberg designated B-
22 by the National Ice Center. In February, a section of the
Larsen B ice shelf, located on the familiar finger-like
Antarctic Peninsula, collapsed and broke away from the
peninsula.

The progression of both breakups were initially observed
by NASA's Moderate Resolution Imaging Spectroradiometer.
Images of the subsequent calving and ice shelf breakup were
captured by NASA's Multi-angle Imaging SpectroRadiometer.

The B-22 iceberg images are available at:

http://www-misr.jpl.nasa.gov/gallery/galhistory/2002_mar_27a.html .

The B-22 iceberg measures approximately 82 kilometers
(about 32 miles) long by 62 kilometers (about 24 miles) wide.
Comparison of the images shows the iceberg, located below and
to the left of center, has drifted away from the ice shelf.
The breakup of ice near the shelf edge, in the area
surrounding B-22, is also visible in the later image.

These natural-color images were acquired on March 10 and
24, 2002, respectively. Antarctic researchers have reported
an increase in the frequency of iceberg calving in recent
years. It has not yet been established if this is a result of
regional climate variation or the global warming trend.

The two views of the ice shelf breakup, acquired on March
7, 2002, provide helpful chemical and topographical
perspectives. In the left-hand image, near-infrared, red and
blue data from the Multi-angle Imaging SpectroRadiometer's
nadir (vertical-viewing) camera causes water ice within the
ice shelf to appear vibrant blue. Water has an intrinsic blue
color due to the selective absorption of longer wavelengths
such as red and infrared, and the translucent properties of
ice within the collapsing shelf enables this absorption to be
observed.

The ice shelf images are available at:

http://photojournal.jpl.nasa.gov/cgi-bin/PIAGenCatalogPage.pl?PIA03702

Data from three different cameras on the instrument and
one color channel were combined to create the multi-angle
composite on the right. Because vertical protrusions or
depressions within textured surfaces appear brighter on their
illuminated faces, the orange color in the multi-angle
composite suggests a rough ice surface.

The Multi-angle Imaging SpectroRadiometer, built and
managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif.,
is one of several Earth-observing experiments aboard Terra,
launched in December 1999. The instrument acquires images of
Earth at nine angles simultaneously, using nine separate
cameras pointed forward, downward, and backward along its
flight path. The Terra mission supports NASA's Earth Science
Enterprise, a long-term research effort designed to help
better understand and protect our home planet. More
information about the radiometer is available at

http://www-misr.jpl.nasa.gov .

JPL is a division of the California Institute of
Technology in Pasadena.

 Moon Passes Four Planets in Five Nights, April 14 - 18

The moon passes - and is in close conjunction with - four bright
planets in five nights. Almost never can you see the moon so close to
four planets in so short a span of time. Anyone can watch this series
of conjunctions from their own home. Through binoculars, you'll see
both the moon and one planet at the same time.

Four planets are presently lined up in the western sky as twilight
ends. From top to bottom they are Jupiter, Saturn, Mars, and Venus.
Jupiter and Venus are the two brightest objects in the nighttime sky,
other than the moon, and they are very conspicuous. Jupiter is
two-thirds of the way up the western sky and Venus is low in the
west. Saturn looks like a bright star midway between Jupiter and
Venus. Saturn is a very short distance to the right of an actual
star, Aldebaran, which is the brightest star in Taurus the Bull. Mars
is much fainter, and it is midway between Saturn and Venus. Look
between 8:00 and 8:30 p.m. It is a grand alignment of planets.

Mercury joins these four planets during the second half of April when
it appears below Venus and very near to the horizon. Mercury is
difficult to see on the 14th, but it sets later night by night and is
more easily visible on the 20th.

The moon passes each planet in turn as the moon orbits the earth.
Here is an evening-by-evening account.

Sunday, April 14: The moon is 4 degrees to the upper left of Venus.
(The width of a finger held at arm's length spans about 2 degrees.)
Notice that the moon is a very thin crescent that grows thicker from
one evening to the next.

Monday, April 15: The moon is 2-1/4 degrees straight to the left of
Mars. Once the sky is fully dark, notice the pretty Pleiades star
cluster a slightly greater distance to the right of Mars. The
crescent moon, Mars, and the Pleiades can be seen at the same time
through most binoculars.

Tuesday, April 16: The moon is 3 degrees straight above Saturn.

Wednesday, April 17: The moon is between Jupiter and Saturn and
closer to Jupiter.

Thursday, April 18: The moon is 2 degrees above Jupiter.

After the 18th, the moon moves eastward and leaves the planets behind.

This series of close moon-planet conjunctions is possible because the
four planets are lined up so closely in the evening sky that the moon
can go from one to the next each night. The spread of the four
planets is growing narrower, and Mercury is joining them. Each planet
is moving too, and by the first part of June, Venus will have passed
Mars, Saturn, and Jupiter and Mars will have passed Saturn. On the
evening of May 5th Venus, Saturn, and Mars form a compact triangle
only 3 degrees on a side. In May, the moon once again passes the
planets, although not almost one each night as in April.

The planetary grouping spans two months in time. It is a series of
events with several highlights, and it is an excellent opportunity to
watch motions in the sky and to see change from night to night. It
can be enjoyed from an urban area; a dark sky is nice but not needed.
A telescope does not help, but binoculars will enhance the view.

A graphic that shows the planets and moon each night is posted at
http://www.GriffithObs.org/skygathering.html.

The moon is visibly in conjunction with four planets in five
consecutive nights roughly once a decade (next on July 12-16, 2010,
and April 24-27, 2022), although seldom does the moon pass as close
to the planets as it does this year. This April's series of
conjunctions will not be equaled until the mornings of July 23-26,
2060 (although many impressive alignments and groupings will happen
during the intervening years).

For additional information on other astronomical events, please visit
the Sky Information page of Griffith Observatory's web site at
http://www.GriffithObs.org/Skyinfo.html or call the Sky Report at
(323) 663-8171. The Observatory, including its telescope, is closed
for renovation and expansion until 2005, but people are welcome to
view the planets on their own from the Observatory lawn.

 SOME ASTEROIDS HAVE ASTRONOMERS SEEING DOUBLE

Binary asteroids -- two rocky objects orbiting about one
another -- appear to be common in Earth-crossing orbits,
astronomers report today in the journal Science. This makes
them an important new asteroid class to study in case future
generations find one coming near Earth.

"If you see two bodies orbiting each other, you can tell
how far away from each other they are and how fast they go
around each other," said Dr. Lance Benner, an asteroid
researcher and an author of the paper from NASA's Jet
Propulsion Laboratory, Pasadena, Calif. "This helps us to
determine the asteroids' mass, volume, internal structure and
what they're made of."

Using the world's two most powerful astronomical radar
telescopes, Benner and his colleagues, led by Jean-Luc Margot
of the California Institute of Technology, Pasadena, estimate
that about 16 percent of near-Earth asteroids larger than 200
meters (219 yards) across are likely to be binary systems.
These systems may have been formed by the pull of gravity
during close encounters with our planet, Mercury, Venus or
Mars.

The first near-Earth binary asteroid ever detected, 2000
DP107, was found by radar in September 2000 at NASA's
Goldstone, Calif., tracking telescope facility. Subsequent
observations were made at the National Science Foundation's
Arecibo Observatory in Puerto Rico, operated by Cornell
University. Like Earth's Moon, the smaller (300-meter or
1,000-foot diameter) body always presents the same face to the
larger (800 meters, or about a half-mile diameter) asteroid
body as it orbits. To date, five near-Earth binary systems
have been identified by radar. But none of them, adds radar
astronomer Jon Giorgini, have orbits that could threaten
Earth, at least through this century.

Near-Earth asteroids may become binaries when the
planets' much larger gravities pull on their rubble-clustered
bodies, distorting them and sometimes breaking off a
satellite. Theoretical and modeling results show that binary
asteroids most likely form when the asteroids closely
encounter the inner planets Earth or Mars, sometimes just
10,000 miles from a planet's surface.

"Of course, the most important thing to know about any
asteroid is whether it is two objects or one, and this is why
we want to observe these binaries with radar whenever
possible," said Dr. Steve Ostro, a senior research scientist
at JPL. "Radar is the best way to identify interesting and
potentially hazardous asteroids. Radar observations provide
information that can be later used by spacecraft to do more
detailed studies efficiently and at lower cost."

Previous evidence that near-Earth binary asteroids were
common came from craters on the Earth and Moon that formed in
pairs and were exactly the same age. Astronomers also have
noted the changes in brightness of reflected sunlight for some
near-Earth asteroids, suggesting that a double system was
causing an eclipse or occultation of one by the other.

Jean-Luc Margot, of the California Institute of
Technology, led the research. The article is also co-authored
by Michael Nolan, research associate at Arecibo; Raymond
Jurgens, Jon Giorgini and Martin Slade at the Jet Propulsion
Laboratory; and Donald Campbell, professor of astronomy at
Cornell University, Ithaca, New York. The observations were
made at the 70-meter Goldstone NASA tracking telescope in
California and at Arecibo Observatory, which is operated by
the National Astronomy and Ionosphere Center at Cornell under
a cooperative agreement with the National Science Foundation.
JPL, a division of the California Institute of Technology,
manages many missions for NASA's Office of Space Science,
Washington, D.C. More information on asteroid radar research
is available at
http://www.gps.Caltech.edu/~margot/2000DP107
and
http://echo.jpl.nasa.gov/ .

 NASA's HISTORIC B-52B and "NEW" B-52H PARTICIPATING IN 50th
ANNIVERSARY ACTIVITIES

The oldest flying B-52 will take part in ceremonies commemorating the
50th anniversary of the B-52 in Wichita, Kansas, on April 12, 2002.

Operated by NASA's Dryden Flight Research Center, Edwards, Calif.,
for nearly 40 years, the B-52B, serial number 52-008, is NASA's
oldest aircraft, as well as the oldest B-52 still flying.

NASA 008 was built in 1955 and has been used on some of the most
significant projects in aerospace history. The aircraft was the 10th
B-52 to come off the Boeing assembly line and was a U.S. Air Force
test aircraft for four years before it was assigned to support the
X-15 research aircraft program at Dryden. NASA 008 was one of two
B-52s used as "mother ships" to air launch the three rocket-powered
X-15 aircraft for research flights. Aircraft 008 was the launch
aircraft on 106 of the X-15 flights and flew a total of 159
captive-carry and launch missions for the X-15 program.

The X-15 was flown over a period of nearly 10 years - June 1959 to
October 1968 - and set the world's unofficial speed and altitude
records of 4,520 mph (Mach 6.7) and 354,200 feet in a program to
investigate all aspects of manned hypersonic flight. Information
gained from the highly successful X-15 program contributed to
development of the Mercury, Gemini, and Apollo manned space flight
programs, and also the Space Shuttle program.

Between 1966 and 1975, B-52 008 was the launch aircraft for 127 of
the 144 flights of the wingless lifting body aircraft that
contributed to development of the space shuttle.

NASA 008 was the launch aircraft for several remotely piloted
aircraft flown by Dryden in the 1970s and 1980s to study spin-stall,
high angle of attack, and maneuvering characteristics.

In 1977 and 1978, and again in the 1983-1985 time period, 008 was
used as the launch
aircraft to test and develop the parachute recovery system used for
the space shuttle's solid rocket booster casings.

The first of four lengthy series of test flights began in 1979 for an
Air Force project to certify an extension of the operational life of
the parachute recovery system on the F-111 crew escape module. The
tests concluded in 1992. The tests, using 008 as the airdrop vehicle
for the parachute test articles, were part of a continuing Air Force
program to improve the recovery system's capability.

From July to October of 1990, the veteran B-52 was used for eight
tests of a drag chute deployment system for space shuttle orbiters.
The drag chutes permit the orbiters to land safely in a shorter
distance and also help reduce tire and brake wear. First operational
use of the drag chute system was on Shuttle Endeavour, newest of the
space shuttle fleet, during its first landing, May 16, 1992.

NASA 008 was used as the air launch platform for the first six
commercially developed Pegasus rocket boosters. The three-stage
Pegasus is designed to put a payload into earth orbit after being
launched horizontally from an aircraft.

In recent years, Dryden's B-52B has supported the X-38 crew return
vehicle prototype captive-carry and drop tests which began in March
1998. Current support includes the X-43 Hyper-X program, which is
slated to be the world's first free-flight scramjet powered vehicle.

At about 2,410 flying hours, the NASA B-52B has the lowest number of
hours of any B-52 in operation, having been used almost exclusively
in the testbed and mother ship role it continues to perform. During
that time it has logged more than 1,030 flights.

NASA's recently acquired B-52H-model, U.S. Air Force serial number
61-0025, will attend the event fresh from depot maintenance at Tinker
AFB, Oklahoma.

High resolution photos are available on the Internet under NASA
Dryden Research Aircraft Photo Gallery, URL:
http://www.dfrc.nasa.gov/gallery/photo/index.html

Dryden's B-52B fact sheet, as well as fact sheets on the X-15 and
other research programs, is available on-line at:
http://www.dfrc.nasa.gov/PAO/PAIS/index.html

An article on the B-52B's 1000th flight is available on-line at:
http://www.dfrc.nasa.gov/PAO/X-Press/1999/Oct15/newsart0.html

NOAA REPORTS U.S. COULD SOON FEEL IMPACTS OF EL NIÑO

National Oceanic and Atmospheric Administration (NOAA) Scientists said
today the United States could start feeling the impacts of the developing
El Niño as early as mid-summer. The scientists cautioned that the strength
of the expected El Niño is still unknown. Depending on its strength, the
El Niño impacts could range between fewer Atlantic hurricanes and a
drier-than-normal summer monsoon season in the southwest, to more
Nor'easters next winter. NOAA is an agency of the U.S. Commerce Department.
"This El Niño is still forming, and it's unclear now at what level of
intensity it will be once it's fully developed," said Vice Adm. Conrad C.
Lautenbacher, USN (ret.), NOAA's administrator. "If sea-surface
temperatures continue their warming trend in the equatorial Pacific, we'll
likely know the intensity by late May or June." He added April and May
typically have been the best months for clues on intensity as El Niño
episodes take shape.

Scientists observed a continuation of warmer-than-normal sea-surface and
sub-surface temperatures across much of the equatorial Pacific. Last
month, ocean surface temperatures were as high as 2 to 3? C (4 to 6 F)above
average near the coasts of Ecuador and northern Peru. (Average ocean
surface temperatures are about 27? C [81 F] in this region during March.)

Also, increased rainfall and cloudiness were observed over the extreme
eastern tropical Pacific, including the Galapagos Islands, and over the
west-central equatorial Pacific. As El Niño continues to develop,
scientists said the possible impacts on the United States include:

* fewer tropical systems during the Atlantic hurricane season;
* higher number of Nor'easters along the East Coast during the 2002-03 winter;
* a drier-than-normal summer monsoon season in the southwest;
* a drier-than-normal fall and winter for the Pacific Northwest;
* a warmer-than-normal late fall and winter in the northern Great Plains
and upper Midwest, and
* a wetter-than-normal winter for the Gulf Coast states.
* if the intensity of the El Niño is strong, central and Southern
California could experience wetter-than-normal conditions.

"One of our major research findings is no two El Niño episodes are alike,"
said Brig. Gen. Jack Kelly USAF (ret.), director of NOAA's National Weather
Service. "Americans have vivid memories of the effects of the strong
1997-98 El Niño, making many people wary of this one. But we will need to
follow developments closely in the coming months to determine just how
strong or weak this El Niño may get."

El Niño conditions occur when water temperatures have warmed sufficiently
to alter the normal patterns of cloudiness and rainfall in the tropical
Pacific basin. A typical El Niño features persistent, increased
precipitation along the equator near the international dateline, and
warmer-than-normal sea-surface temperatures (at least 0.5? C [1 F] above
normal) extending eastward to the South American coast.

El Niño episodes occur about every four-to-five years and can last up to
12-to-18 months. NOAA will continue monitoring El Niño developments and
provide monthly updates. The El Niño/Southern Oscillation (ENSO)
Diagnostic Discussion is a team effort consisting of the Climate Prediction
Center (lead), Climate Diagnostics Center, Geophysical Fluid Dynamics
Laboratory, National Climatic Data Center, Atlantic Oceanographic and
Meteorological Laboratory, and the International Research Institute for
Climate Prediction.

NOAA's National Weather Service is the primary source of weather data,
fore-casts and warnings for the United States and its territories. The
National Weather Service operates the most advanced weather and flood
warning and forecast system in the world, helping to protect lives and
property and enhance the national economy. To learn more online, visit:
http://weather.gov.

Relevant Web Links:

El Niño/Southern Oscillation (ENSO) Diagnostic Discussion:
http://www.cpc.ncep.noaa.gov/products/analysis_monitoring/enso_advisoryMost
Recent 2 Months Sea Surface Temperature Anomaly Animation:
http://orbit-net.nesdis.noaa.gov/orad/sub/crbfrm_sstanom2m.html

El Niño and La Niña-related Winter Features over North America:
http://www.cpc.ncep.noaa.gov/products/analysis_monitoring/ensocycle/enso_cyc

April 11, 2002

 Something Unexpected in the Pacific Ocean

Scientists have discovered something nearly invisible that straddles the
vast Pacific Ocean: Hawaii's surprising island wake.

FULL STORY at

http://science.nasa.gov/headlines/y2002/10apr_hawaii.htm?list448368

 ADMINISTRATOR O'KEEFE'S ADDRESS
NOW AVAILABLE ON NASA TELEVISION

As a result of the delayed launch of the Space Shuttle Atlantis on STS-110,
Friday's address by NASA Administrator Sean O'Keefe will be available on NASA
Television.

The Administrator outlines the future direction of the agency in a major address
April 12 at the Maxwell School of Citizenship and Public Affairs on the campus of
Syracuse University in New York. The address is scheduled to begin at 2 p.m. EDT
at the Maxwell School's main auditorium and will be carried live by satellite,
NASA TV, and webcast on the Internet by both Maxwell and NASA.

Following the Administrator's remarks, a press briefing will be held from 3:30
p.m. to 4 p.m. EDT in the Public Events Room located at 200 Eggers Hall. Media
representatives wishing to cover the address and press conference are asked to
contact either Jill Leonhardt or Bob Jacobs. Reporters who cannot attend the
press event will be able to participate by telephone.

Administrator O'Keefe's remarks will be available live by satellite on Telstar 5,
Ku Band, transponder 19, located at 97 degrees West Longitude with vertical
polarization. The downlink frequency is 12053 MHz, with audio at 6.2 MHz and 6.8
MHz. NASA TV can be found on GE-2, Transponder 9C, vertical polarization at 85
degrees West longitude, 3880 MHz, with audio at 6.8 MHz

A webcast of the address will be available on the World Wide Web at:
http://www.maxwell.syr.edu/news
http://www.nasa.gov

Rocket Fragement, Not Meteorite, Landed in Uganda 

POLICE yesterday said the alien spherical object that landed in Kasambya,
Kikandwa sub-county in Mubende district last month was not a meteorite but a
suspected rocket fragment from outer space.

Police spokesman Asuman Mugenyi, whose personnel collected the object for
scrutiny, said yesterday that they were still scrutinising the object whose
whereabouts he did not disclose.

Full story here:

http://allafrica.com/stories/200204100271.html

Mars Society Special Bulletin #60 - Conference Announcements 

Poster Contest

Once again, the Mars Society is soliciting designs for a conference
poster. The winning design will be featured not only posters and
handbills, but also on the annual conference t-shirt. Posters should
feature a design relevant to The Mars Society mission and include the
following:

The Mars Society
5th International Conference
University of Colorado at Boulder
August 8-11th, 2002
www.MarsSociety.org

The winning designer will receive complimentary admission to the
conference and annual banquet. Send a hard copy of your design to
Lorraine Bell, c/o The Mars Society, P.O. Box 273, Indian Hills, CO
80454. All entries must be received by May 15th, 2002.

Hakluyt Prize Contest

Once again, we invite students ages 15-22 to participate in this fun
activity. Each entrant should compose a letter explaining why manned
exploration of Mars is important to the people of the earth, then
send this letter to world leaders, either via the post or
email. Send a copy of your letter with a list of those you have
contacted and any responses you receive to Maggie Zubrin,
mzubrin@aol.com.

The winner will receive an all expense paid trip to the conference in
August. In addition, The Mars Society will award certificates to all
entrants as well as special awards for the winners. All entries must
be received by June 15th, 2002.

Writers and Artists Wanted

Open reading

Each year we present a series of interesting and unique events in
conjunction with our annual conference. This year we are inviting
any one who has written a story revolving around Mars exploration or
colonization to participate in our open microphone session.
Professional or Amateur, novelist or poet, you are all invited to
share your vision. Each author will be given a 5 minute time slot to
read from your work. Filkers are welcome to sing their original
composition. Work must be relevant to the Mars Society mission and
the selection you read must be suitable for general audiences.
Please email your name and a brief description of your reading no
later than July 1 to Maggie Zubrin, mzubrin@aol.com.

Mars Art Gallery

In addition to our vendors area, we will be including a display of
Mars related artwork this year. We invite artists to display
paintings, models and crafts which are illustrative of Mars
exploration and space science in general. You are welcome to display
your art for sale at the conference. Depictions of star clusters,
space ships, Mars colonies, are welcome, but please, no Star Trek or
Dragon Riders. If you would like to display your work, please send a
brief description no later than July 1 to Maggie Zubrin,
mzubrin@aol.com.

Silent Auction

Due to the overwhelming success of last year's not-so-silent
auction, we will be repeating the event this year at the conference.
We will be offering some unique items including original art works,
travel, etc. We are seeking donations of space related items as well
as items and services of any generally useful nature. If you have an
item you would like to donate or if you are willing to help procure
items for the auction, contact Lorraine Bell, LMB3000@speakeasy.net.
Items may be delivered to the conference site as late as the first
morning of the conference. The Mars Society may arrange shipping of
larger items.

Artists, Vendors and Chapters, your donations are particularly
sought. Failed dot.coms, donate your lightly used computers
Remember, all donations to the Mars Society are tax deductible and
the cost above the retail value of any item purchased considered a
donation.

Door Prizes

For the first time, the Mars Society will be presenting door prizes
to lucky conference attendees. All registered attendees at the
conference will be eligible for the drawing. So far, we have rounded
up the following items:

Original signed books
Original Oil Painting from KSC exhibit
Sterling Silver Logo Key Chain
Crew Slot at the MDRS (must be physically qualified)
Miscellaneous smaller items.

So, for the 400 plus applicants who weren't selected for a crew
slot, this is your chance. You must be present to win. See you there!

Maggie Zubrin
Executive Director

 Canadian Space Agency Astronaut Dr. Dave Williams
in London to Speak About First NASA Undersea Mission

Saint-Hubert, Quebec, April 10, 2002 - Media are cordially invited to attend
a reception at the London Regional Children's Museum where Marylin
Steinberg, Manager, Youth Outreach at the Canadian Space Agency will
announce a contribution to the space gallery project.

In addition, Canadian Space Agengy Astronaut and first Canadian Aquanaut Dr.
Dave Williams will talk about the first NASA undersea mission.

>From October 22 to 28, 2001, Dr. Williams joined two NASA astronauts in the
Aquarius habitat, the world's only undersea laboratory located 5.5 km
offshore, near Key Largo. As part of the NASA Extreme Environment Mission
Objectives (NEEMO) project, the astronauts conducted experiements on the
relevance of the undersea environment, and its application to space. A
number of tasks performed inside Aquarius were designed to simulate
functions performed during space missions.

What:
Cocktail Reception

When:
Friday, April 12 at 5 p.m.

Where:
London Regional Children's Museum
21 Wharncliffe Road South, London

 Cosmic X-rays reveal evidence for new form of matter

NASA's Chandra X-ray Observatory has found two stars - one too
small, one too cold - that reveal cracks in our understanding of the
structure of matter. These discoveries open a new window on nuclear
physics, offering a link between the vast cosmos and its tiniest
constituents.

Chandra's observations of RXJ1856.5-3754 and 3C58 suggest that the
matter in these stars is even denser than nuclear matter found on Earth.
This raises the possibility these stars are composed of pure quarks or
contain crystals of sub-nuclear particles that normally have only a fleeting
existence following high-energy collisions.

By combining Chandra and Hubble Space Telescope data, astronomers
found that RXJ 1856 radiates like a solid body with a temperature of 1.2
million degrees Fahrenheit (700,000 degrees Celsius) and has a diameter of
about 7 miles (11.3 kilometers). This size is too small to reconcile with
standard models for neutron stars -- until now the most extreme form of
matter known.

"Taken at face value, the combined observational evidence points to
a star composed not of neutrons, but of quarks in a form know as strange
quark matter," said Jeremy Drake of the Harvard-Smithsonian Center for
Astrophysics (CfA) in Cambridge, Mass., and lead author of a paper on
RXJ1856 to appear in June 20, 2002 issue of The Astrophysical Journal.
"Quarks, thought to be the fundamental constituents of nuclear particles,
have never been seen outside a nucleus in Earth-bound laboratories."

Observations by Chandra of 3C58 also yielded startling results. A
team composed of Patrick Slane and Steven Murray, also of CfA, and David
Helfand of Columbia University, New York, failed to detect the expected
X-radiation from the hot surface of 3C58, a neutron star believed to have
been created in an explosion witnessed by Chinese and Japanese astronomers
in 1181 AD. The team concluded that the star has a temperature of less than
one million degrees Celsius, which is far below the predicted value.

"Our observations of 3C58 offer the first compelling test of models
for how neutron stars cool and, the standard theory fails," said Helfand.
"It appears that neutron stars aren't pure neutrons after all -- new forms
of matter are required."

A teaspoonful of neutron star material weighs a billion tons, as
much as all the cars, trucks and buses on Earth. Its extraordinary density
is equivalent to that of the nucleus of an atom with all of the typical
space between the atoms and their nuclei removed. An atom's nucleus is
composed of positively charged protons and neutral neutrons, particles so
small that 100 billion trillion of them would fit on the head of a pin.

Protons and neutrons are composed of even smaller particles called
quarks, the basic building blocks of matter. Enormous atom smashers are
designed to probe the forces between quarks and the structure of the nucleus
by smashing high-energy beams of nuclei into each other and observing the
violent aftermath for a fraction of a second.

Drake cautioned that the observations of RXJ1856 could be
interpreted as a more normal neutron star with a hot spot. Such a model is
under consideration by Fred Walter of the State University of New York,
Stony Brook, one of the discoverers of RXJ1856, which was originally found
in 1996 by the German Roetgen satellite. However, the hot spot model
requires a very special orientation of the star with respect to the Earth to
explain the absence of pulsations, which would be expected from the hot
spot. The probability of such an orientation is quite small.

"Regardless of how these mysteries are resolved, these precise
observations are highly significant," said Michael Turner of the University
of Chicago. "They demonstrate our ability to use the universe as a
laboratory where we can study some of the most fundamental questions in
physics."

NASA's Marshall Space Flight Center in Huntsville, Ala., manages the
Chandra program, and TRW, Inc., Redondo Beach, Calif., is the prime
contractor. The Smithsonian's Chandra X-ray Center controls science and
flight operations from Cambridge, Mass.

Images and additional information about this result are available
at:

http://chandra.harvard.edu
AND
http://chandra.nasa.gov

 RECORD SET FOR MOST-DISTANT SPACECRAFT MAINTENANCE

Astronauts can make service visits to the Earth-orbiting
Hubble Space Telescope, but what do you do if the spacecraft
needing a replacement part is the farthest human-made object
from Earth, more than twice as distant as Pluto?

The answer, as the flight team for the Voyager
Interstellar Mission recently demonstrated, is to plan ahead
and keep top-notch engineers available.

Last month, the team cautiously activated a backup
position-sensing system, including a Sun sensor and star
tracker, on Voyager 1. The spacecraft had been carrying those
components and other spare parts since it was launched in 1977
on what was then slated as a four-year mission.

"After sitting on the shelf for 25 years, it's like new
equipment," said Ed Massey, Voyager project manager at NASA's
Jet Propulsion Laboratory, Pasadena, Calif. Voyager 1 and its
twin, Voyager 2, completed their history-making tour of outer
planets in 1989 and are now headed toward the boundary zone --
called the heliopause -- where the Sun's influence cedes way
to interstellar space. Both spacecraft have adequate power and
communication capabilities to explore that frontier for about
20 more years, if other onboard systems hold up.

The original designers' foresight in building backup
systems into the Voyagers helps, but making changeovers aboard
a spacecraft more than 12.5 billion kilometers (7.8 billion
miles) away presents enormous challenges. Anything that could
go wrong needs to be foreseen, because reaction time is
unforgivingly slow. Communication signals take nearly 12 hours
each way traveling to or from Voyager 1 at the speed of light.
And the task now falls to a Voyager flight team of just 14
people, compared with a Voyager team of more than 300 in the
1980s.

The success of the recent modifications gives the team
confidence in switching to other backup systems on both
spacecraft when concerns arise about original systems, Massey
said.

Voyager 1's original attitude-control system showed
slowly increasing signs of trouble in the past two years, said
Tim Hogle, a flight-team engineer at JPL. Diagnostics pointed
to an electronic component that takes analog signals from
position-sensing devices and converts them into digital values
for an onboard computer. Because of the system's design,
switching to that component's backup also meant activating the
backup Sun sensor and star tracker, which provide the
reference points for the spacecraft's orientation in space.

"We had to plan this switch very carefully," Hogle said.
This backup equipment hadn't been tested since Voyager 1 was
approaching Saturn in 1980. If it didn't work right, switching
to it could confuse the onboard computer about the
spacecraft's orientation, which could lead to faulty pointing
of the antenna and loss of communications with Earth.

Among other precautions, the team programmed a temporary
changeover with an automatic reversion to the original system,
allowing just enough time to evaluate the backup. The planning
effort identified potential trouble points in advance and made
provisions to be able to correct them, if necessary, before
the final changeover, nine days after the temporary one. The
cautious approach paid off. The system made an unexpected lock
onto the Sun during the temporary switch, so the spacecraft
was instructed to keep itself steady with gyroscopes during
the final switch.

Calibration of the backup system was completed April 1.

"By switching to the backup before the original system
failed, we now have the original as a backup if we need it,"
said flight-team member Steve Howard of JPL.

The changeover plan benefited from soliciting experienced
advice from several Voyager veterans now working on other JPL
projects. "We have resources here you just could not find
anywhere else," Howard said.

Massey said, "The switchover went relatively smoothly. It
is certainly a testament to the people who designed and built
the spacecraft, and to the expertise and dedication of the
flight team."

Information about Voyager's grand tour of the outer
planets and the current Voyager Interstellar Mission is
available online at
http://voyager.jpl.nasa.gov . JPL, a
division of the California Institute of Technology in
Pasadena, manages Voyager for NASA's Office of Space Science,
Washington, D.C.

April 10, 2002

 HUBBLE ASTRONOMER CREATES SPECTACULAR GALAXY COLLISION VISUALIZATION FOR THE NATIONAL AIR AND SPACE MUSEUM

Someday our Milky Way Galaxy and the neighboring Andromeda Galaxy may
come crashing together in a horrendous collision that will twist and
distort their shapes beyond recognition. Of course, to see that, you'll
have to wait several billion years. But thanks to a combination of
research science, Hollywood computer graphics, and large-scale
visualization, visitors to the Smithsonian Institution's National Air
and Space Museum in Washington, DC, can witness such an event today.
The Space Telescope Science Institute (STScI), the scientific home of
NASA's Hubble Space Telescope, is extending its tradition of stunning
imagery by creating a spectacular scientific visualization of two
galaxies colliding. This incredibly detailed, full-dome video sequence
will be a highlight of "Infinity Express: A 20-Minute Tour of the
Universe," the inaugural show in the National Air and Space Museum's
newly renovated Einstein Planetarium, opening Saturday, April 13.

The scientific visualization by Dr. Frank Summers, an astrophysicist
in STScI's Office of Public Outreach, depicts a tremendous collision
of two spiral galaxies. Because such events take hundreds of millions
of years to occur, researchers use supercomputer simulations to study
how galaxies are transformed and merge together. Dr. Summers has taken
research data provided by Dr. Chris Mihos (Case Western Reserve
University) and Dr. Lars Hernquist (Harvard University), and visualized
it using the same software that Hollywood uses to produce blockbuster
visual effects.

To see and read more, please click on:
http://oposite.stsci.edu/pubinfo/pr/2002/09 and links in
http://oposite.stsci.edu/pubinfo/latest.html
http://oposite.stscie.du/pubinfo/pictures.html
http://hubblesite.org/go/news and
http://www.nasm.si.edu/nasm/planetarium/

The Space Telescope Science Institute (STScI) is operated by the
Association of Universities for Research in Astronomy, Inc. (AURA),
for NASA, under contract with the Goddard Space Flight Center,
Greenbelt, MD. The Hubble Space Telescope is a project of international
cooperation between NASA and the European Space Agency (ESA). This work
is partially supported by the National Science Foundation through the
National Computational Science Alliance and the Partnerships for
Advanced Computational Infrastructure. The National Air and Space Museum
is owned and operated by the Smithsonian Institution.

To receive STScI press releases electronically, send an Internet
electronic mail message to public-request@stsci.edu. Leave the subject
line blank, and type the word subscribe in the body of the message. The
system will respond with a confirmation of the subscription, and you
will receive new press releases as they are issued. Please subscribe
using the email account with which you would like to receive list
messages. To unsubscribe, send mail to public-request@stsci.edu. Leave
the subject line blank, and type the word unsubscribe in the body of
the message. Please unsubscribe using the email account that you used
to subscribe to the list.

 PERSONAL REPORTS FROM SPACE STATION REFLECT ASTRONAUTS' THOUGHTS

More than 100 days into a planned six-month stay aboard
the International Space Station, Expedition Four flight
engineers Dan Bursch and Carl Walz have provided a rare
glimpse of life in orbit.

In an open letter sent from the space station this weekend,
Bursch shares his thoughts and experiences over 122 days in
space. The letter may be found at:
http://spaceflight.nasa.gov

Bursch, along with Walz and commander Yury Onufrienko, has
been living and working on the station since early December.
In the ensuing months, crewmembers celebrated Christmas in
space and performed two spacewalks, and currently are
preparing for the arrival of the next Shuttle crew later this
week.

Bursch's "letter home" provides an intimate look at life on
board the station, including day-to-day operations, the
challenges of being away from family and the excitement of
life in space. Walz compares his experience as a Shuttle-
based spacewalker to that of the February spacewalk he and
Bursch conducted from the space station.

The Expedition Four crew will return to Earth in June aboard
Endeavour after spending more than six months in orbit. They
will be replaced by another three-person crew, extending more
than 17 months of continued human occupancy on board the
station.

Around-the-clock coverage of the ongoing space station
mission and the current STS-110 mission is available on NASA
Television. NASA TV is accessible through GE2, transponder
9C, with a frequency of 3880 MHz, an orbital position of 85
degrees West Longitude and audio at 6.8 MHz.

Most Distant Group of Galaxies Known in the Universe 

Observations with the VLT have identified an
extremely distant group of galaxies - it is the most
distant and therefore the earliest known in the
Universe so far.

This major new result is described in ESO PR 07/02, just
published at:

http://www.eso.org/outreach/press-rel/pr-2002/pr-07-02.html

 GALILEO MISSION TEAM CHOSEN FOR SPACE FOUNDATION AWARD

Hundreds of people who helped make NASA's Galileo mission to Jupiter a
long-running success are drawing recognition from the Space Foundation with an
award being presented today in Colorado Springs, Colo.

The Space Foundation, a non-profit group supporting space activities, space
professionals and education, selected Galileo's NASA and industry team to receive a
Space Achievement Award. "The selection recognizes the design, development,
launch and operation of the Galileo space probe, which resulted in a more-than-10-
year odyssey of solar system exploration," said Steve Eisenhart, foundation vice
president. "We're focusing on the abundance of scientific discoveries that Galileo has
sent us."

Galileo was launched aboard the space shuttle Atlantis in 1989. The spacecraft
flew by Venus, Earth and two asteroids on its way to Jupiter, and has been orbiting
Jupiter since Dec. 7, 1995. On arrival day, a probe released by the orbiter parachuted
into Jupiter's atmosphere for the first in-place measurements of a gas giant planet.
Since then, Galileo has flown 33 close approaches past Jupiter's four largest moons. It
found evidence for subsurface liquid layers of saltwater on Europa, Ganymede and
Callisto, and it documented extensive volcanic activity on Io. Galileo returned about
14,000 images from its camera and 650 infrared images.

"This award is a tribute to the team of people at all phases of the project who
made this mission the successful legacy of discovery that it is," said Dr. Eilene
Theilig, Galileo project manager at NASA's Jet Propulsion Laboratory, Pasadena,
Calif.

Galileo continues to return new scientific information after more than three
times its originally scheduled two-year orbital tour. It will examine the high-radiation
environment near Jupiter and the density of the small inner moon Amalthea when it
flies near Amalthea for the first time in November.

Galileo information is available online at http://galileo.jpl.nasa.gov . JPL, a
division of the California Institute of Technology in Pasadena, manages the mission for
NASA's Office of Space Science, Washington, D.C. NASA's Ames Research Center,
Moffett Field, Calif., managed the atmospheric probe. The Space Foundation is based in
Colorado Springs.

April 9, 2002

Canadian Space Agency Astronaut Dr. Dave Williams
in Regina to Speak About First NASA Undersea Mission

Saint-Hubert, Quebec, April 8, 2002 - Canadian Space Agency Astronaut and
first Canadian Aquanaut Dr. Dave Williams will be in Regina on Wednesday,
April 10 to talk to students about the first NASA undersea mission and to
present Saskatchewan's Lieutenant Governor with a Saskatchewan flag that
flew in space.

>From October 22 to 28, 2001, Dr. Williams joined two NASA astronauts in the
Aquarius habitat, the world's only undersea laboratory located 5.5 km
offshore, near Key Largo. As part of the NASA Extreme Environment Mission
Objectives (NEEMO) project, the astronauts conducted experiements on the
relevance of the undersea environment, and its application to space. A
number of tasks performed inside Aquarius were designed to simulate
functions performed during space missions.

Media are invited to attend the following events:

Wednesday, April 10

9:30 - 11:30 a.m.

Who:
300 grade 5 and 6 students

Theme:
>From Sea to Space

Where:
Saskatchewan Science Centre
Winnipeg St. and Wascana Drive

4:30 - 5:30 p.m.

What:
Presentation to Lieutenant Governor

Where:
Government House
4607 Dewdney Avenue, Regina

 Strange lights in the sky baffle Bavarians
Reuters

MUNICH, Germany - Strange lights in the sky baffled Bavarians late on Saturday
as hundreds of panicked callers jammed police telephone lines seeking an
explanation for the phenomenon.

Reports of an unsettling late-night natural light show came from all over
the southern German state as well as the neighboring region of
Baden-Wuerttemberg.

Scientists said the lights may have been the result of a meteor breaking
through the Earth's atmosphere.

Full story here:

http://www.cnn.com/2002/TECH/space/04/08/germany.lights.reut/index.html

GALILEO MISSION TEAM CHOSEN FOR SPACE FOUNDATION AWARD

Hundreds of people who helped make NASA's Galileo
mission to Jupiter a long-running success are drawing recognition
from the Space Foundation with an award being presented today
in Colorado Springs, Colo.

The Space Foundation, a non-profit group supporting
space activities, space professionals and education, selected
Galileo's NASA and industry team to receive a Space Achievement
Award. "The selection recognizes the design, development,
launch and operation of the Galileo space probe, which resulted
in a more-than-10-year odyssey of solar system exploration,"
said Steve Eisenhart, foundation vice president. "We're focusing
on the abundance of scientific discoveries that Galileo has
sent us."

Galileo was launched aboard the space shuttle Atlantis in
1989. The spacecraft flew by Venus, Earth and two asteroids on its
way to Jupiter, and has been orbiting Jupiter since Dec. 7, 1995.
On arrival day, a probe released by the orbiter parachuted into
Jupiter's atmosphere for the first in-place measurements of a gas
giant planet. Since then, Galileo has flown 33 close approaches
past Jupiter's four largest moons. It found evidence for
subsurface liquid layers of saltwater on Europa, Ganymede and
Callisto, and it documented extensive volcanic activity on Io.
Galileo returned about 14,000 images from its camera and 650
infrared images.

"This award is a tribute to the team of people at all
phases of the project who made this mission the successful legacy
of discovery that it is," said Dr. Eilene Theilig, Galileo project
manager at NASA's Jet Propulsion Laboratory, Pasadena, Calif.

Galileo continues to return new scientific information
after more than three times its originally scheduled two-year
orbital tour. It will examine the high-radiation environment near
Jupiter and the density of the small inner moon Amalthea when it
flies near Amalthea for the first time in November.

Galileo information is available online at

http://galileo.jpl.nasa.gov

Most Recent OBPR News 

1) Human Physiology Research and the ISS: Staying Fit Along the Journey
The human body undergoes numerous adaptations when it leaves Earth's gravity. Researchers are studying how to minimize those phy...
For more info:
http://spaceresearch.nasa.gov/news.html#154

2) Tick-Tock Atomic Clock
Scientists are building atomic clocks that keep time with mind-boggling precision. Such devices will help farmers, physicists, a...
For more info:
http://spaceresearch.nasa.gov/news.html#153

3) My Pet Neutron Star
Using a new form of matter called Bose-Einstein condensates, researchers are bringing astrophysics from deep space right into th...
For more info:
http://spaceresearch.nasa.gov/news.html#152

4) REMAP Task Force Established to Review and Assess OBPR Research
NASA Administrator Sean O'Keefe has selected an independent task force to provide recommendations regarding the research priorit...
For more info:
http://spaceresearch.nasa.gov/news.html#151

5) Antibiotics from Space
Test tubes of bacteria produce more antibiotics in space than they do on Earth. Researchers aren't sure why ... but they aim to ...
For more info:
http://spaceresearch.nasa.gov/news.html#150

 NOTED BERKELEY ASTRONOMER TO LECTURE ON 'BIG-BANG' THEORY

"Why I Believe in the Big-Bang: Evidence about the Origin of the
Universe" will be the topic of a free, non-technical talk at 7 p.m.
PDT on Wednesday, April 10, at
Foothill College in Los Altos Hills, Calif. The public is invited.

Astronomer Dr. Alex Filippenko of the University of California,
Berkeley, will discuss the strong evidence that exists for the
'big-bang' theory of the creation of the universe as well as recent
modifications to the original theory. This includes the idea of rapid
inflation during the first blink of an eye of the universe's
existence. It also addresses the hypothesis that the universe may be
just one small part of a grand collective of universes or
'multi-verse.'

"The Silicon Valley Astronomy Lecture Series is a wonderful community
resource that brings the latest scientific research in astrobiology
and astronomy to a general audience," said NASA Ames Center Director
Dr. Henry McDonald. "NASA Ames is proud to be a partner in these
efforts."

Filippenko is one of the leaders of the research team that discovered
evidence for the accelerating theory of the universe, which suggests
that the expansion of the universe is speediing up. The work was
tapped as 'discovery of the year' by Science magazine.

Filippenko is co-author of an introductory college textbook in
astronomy and his video astronomy course has taught thousands of lay
people about cosmology and the universe. He is the current president
of the Astronomical Society of the Pacific.

This is the fifth talk in this year's Silicon Valley Astronomy
Lecture Series, co-sponsored by NASA Ames, Foothill College's
Division of Physical Science, Mathematics and

Engineering, the Astronomical Society of the Pacific and the SETI Institute.

The lecture series is held at Foothill College's Smithwick Theater in
Los Altos Hills. From interstate 280, exit at El Monte Road and
travel west to the campus. Visitors must purchase a one-day
campus-parking permit for $2. Admission is free and the public is
invited. Seating is on a first-come, first-served basis. Children
over the age of 13 are welcome. More information is available by
calling the series hotline at 650/949-7888.

April 8, 2002

Tick-Tock Atomic Clock

 Scientists are building atomic clocks that keep time with mind-boggling
precision. Such devices will help farmers, physicists, and interstellar
travelers alike.

FULL STORY at

http://science.nasa.gov/headlines/y2002/08apr_atomicclock.htm?list448368

 Mars Odyssey Observes First Anniversary in Space
Jet Propulsion Laboratory

What a year this has been for the Mars Odyssey team!

The excitement of launch last April 7, the arrival at Mars, the long,
sometimes tedious aerobraking concluded so successfully, the beginning of
the mapping phase ....

The detailed pictures the camera system is taking, letting scientists get
closer and closer to Mars' mysteries ....

The evidence from the gamma ray spectrometer showing more hydrogen in Mars'
southern hemisphere than was known before ....

The drama of the martian radiation environment experiment - as it turned
out, the instrument was just taking a long nap ....

Anniversary Toasts From the Odyssey Team

"We have an A-plus spacecraft," said Roger Gibbs, Odyssey project manager at
NASA's Jet Propulsion Laboratory. "Everything is going smoothly and we're
looking forward to another great year."

Bob Berry, Lockheed Martin Astronautics Odyssey program manager, said, "The
performance of the spacecraft and the spacecraft team has been virtually
flawless during cruise, orbit insertion and aerobraking. Now it's payoff
time and we're ecstatic to finally start seeing the fruits of our labor -
great science."

He added, "Early results are amazing and the team is looking forward to
Odyssey adding another chapter in our Mars book of knowledge."

Still early in the mapping mission, Odyssey has already begun to return
surprising new views of the red planet.

"Odyssey's unique instrument set is working nearly perfectly," said JPL's
Odyssey project scientist Dr. Steve Saunders. "We are getting new insights
into the physical and chemical makeup of Mars."

Camera system principal investigator Dr. Phil Christensen, Arizona State
University, Tempe, said, "We now have night vision on Mars and have acquired
images taken in complete darkness on the planet. The daytime images help
scientists map minerals and study safe places for future Mars landings.

A new Mars image is posted daily by Christensen's team. To see the images,
go to http://themis.asu.edu/latest.html .

Dr. Bill Boynton, University of Arizona, Tucson, the gamma ray spectrometer
scientist and team leader, said, "We can see a strong hydrogen signature in
Mars' southern hemisphere, even without boom deployment [scheduled for May].
There's a lot of water there."

Neutron spectrometer scientist Dr. Bill Feldman, Los Alamos National
Laboratory, New Mexico, agreed and said, "We're finding a lot of water ice
in the soil of Mars."

Rounding out the gamma ray spectrometer team is Dr. Igor Mitrofanov,
principal investigator for the Russian high energy neutron detector.

He said, "A vast area of permafrost has been discovered in the southern
hemisphere and we start to see the northern permafrost as well in high
energy neutrons."

More information, including links, about the gamma ray spectrometer suite of
instruments is available at
http://grs.lpl.arizona.edu/ .

The martian radiation instrument did not communicate for about six months,
but after extensive troubleshooting is now "talking" with scientists again.
The experiment measures radiation that could endanger humans and provides a
check on overall radiation that might affect other Odyssey instruments.

"This experiment is important for any future human exploration of Mars,"
said principal investigator Dr. Frank Cucinotta, NASA Johnson Space Center,
Houston, Texas.

http://marie.jsc.nasa.gov/ has more information on the radiation instrument.

April 6, 2002

 Below are excerpts from a Meteoritical Bulletin announcement sent out today
on seven recent Mars meteorites finds. Of these
Mars meteorites, SAU 060 and SAU 090 are new. Since these two
Mars meteorite were found near the other four SAU Mars meteorites and are
also basaltic shergottites, they are assumed to be paired with this group.
Taking into account pairings, the number of Mars meteorites remains at 24.

 

THE METEORITICAL BULLETIN
Announcement 86-1, April 5, 2002
Sara Russell, Editor (sara.russell@nhm.ac.uk)
Jutta Zipfel, Assoc. Ed. for Saharan Meteorites
(zipfel@mpch-mainz.mpg.de)
Jeffrey N. Grossman, Assoc. Ed. for Web (jgrossman@usgs.gov)
Monica M. Grady, Co-Editor

Announcements of new meteorites
to be published in Meteoritical Bulletin, No. 86, 2002 July. Here,
you will find the complete text of announcements of Martian meteorites
described in the past year.

Marian meteorites described below:

Dhofar 378 Basaltic shergottite (Oman)
Grove Mountains 99027 Lherzolitic shergottite (Antarctica)
Northwest Africa 856 Basaltic shergottite (Africa*)
Northwest Africa 1068 Basaltic shergottite (Africa*)
Northwest Africa 1110 Basaltic shergottite (Africa*)
Sayh al Uhaymir 060 Basaltic shergottite (Oman)
Sayh al Uhaymir 090 Basaltic shergottite (Oman)

*) Morocco or surrounding countries.

The preliminary text of the 2002 Meteoritical Bulletin, including the
above meteorites and those in E-mail Announcements 86-2 and 86-3,
may by viewed at:

http://www.uark.edu/campus-resources/metsoc/metbull/mb86.pdf

***PLEASE REPORT ERRORS BY 14 APRIL 2002 TO: jgrossman@usgs.gov

All information in this e-mail and on the above-cited Meteoritical
Bulletin webpage is subject to revision until final publication in
the summer of 2002.

===========================================================
ANNOUNCEMENTS
===========================================================

Dhofar 378 18°9.5' N, 54°6.8' E
Oman
Found 2000 June 17
Martian meteorite (basaltic shergottite)
A single stone of 15 g, covered with fresh black fusion crust, was
recovered by an anonymous finder within the province of other Dhofar
meteorites. Classification and description: (Y. Ikeda and M. Kimura,
Dept. of Materials and Biological Sciences Ibaraki; H. Takeda,
Chiba): It has a doleritic or microgabbroic texture, and the grain
sizes of the main minerals (pyroxenes and plagioclase glass) are
about 1 mm across. It consists mainly of ferroan pyroxenes (augite
and pigeonite), and plagioclase glass with quenched plagioclase
rims. Minor minerals are hedenbergite, pyroxferroite, fayalite,
silica, Ti-rich magnetite, ilmenite, sulfide, phosphate, and
rhyolitic glass. The Fe/(Mg+Fe) ratios of pyroxenes (augite and
pigeonite) range from 0.40 to more than 0.90, those of hedenbergite
from 0.97 to 0.99, and olivine from 0.90 to 0.98. The original
plagioclase grains were transformed to plagioclase glass (An35 to
An55) by an intense impact shock, then quenched plagioclase of the
same composition a few tens of mm up to one hundred mm in width at
the boundaries between the plagioclase glass and other minerals.
Oxygen isotopic composition (T.K. Mayeda and R.N. Clayton, UChi):
d18O == +4.46 permil, d17O == +2.52 permil. This meteorite was
recovered from an area near the Dhofar 019 basaltic shergottite, but
the two meteorites are probably not paired. Dhofar 019 is doleritic
and contains olivine grains with Fe/(Mg+Fe) ratios of 0.4-0.75,
whilst these seem to be absent from Dhofar 378. Pyroxenes in Dhofar
019 are more magnesian than in Dhofar 378. Specimens: type specimens
0.445 g & 0.054 g, Ibaraki; 2.74 g MPI; main mass is with the
anonymous finder.

 

Grove Mountains (GRV) 99027 73°06'01" S, 75°14'13" E
Antarctica
Found 2000 February 8
Martian meteorite (lherzolitic shergottite)
This meteorite weighs 9.97 g, and most of the surface is covered by
fusion crust. Classification and Mineralogy (Lin and B. Miao, GIG;
H. Wang & C. Lin, NU): It is composed mainly of coarse-grained
orthopyroxene, olivine, clinopyroxene and plagioclase, with minor
opaque minerals. There are two textures. In the larger part of the
sections, olivine occurs as rounded euhedral grains, poikilitically
enclosed in a megacryst of orthopyroxene; in the other side of the
sections, it shows a cumulate texture, consisting of euhedral
orthopyroxene, clinopyroxene, olivine and interstitial plagioclase.
Chromite, the most common opaque phase, is euhedral and enclosed in
pyroxenes. The mineral assemblage and textures are similar to the
Allan Hills (ALHA) 77005 lherzolite. The FeO/MnO (wt%) ratio of
orthopyroxene is 34+/-5. Compositions of orthopyroxene (En66-78Fs20-
26Wo2-8), clinopyroxene (En48-52Fs13-15Wo34-39), olivine (Fa22-30)
and plagioclase (An49-55Ab44-50Or<1) overlap with the ranges in
ALHA77005. Fracturing and undulose extinction in silicates are
strong. Plagioclase is commonly deformed, and partially turns into
maskelynite along the boundaries of grains. The shock stage is S4;
weathering grade, W1. The meteorite is curated at PRIC.

Northwest Africa 856
unknown location
Found 2001 March
Martian meteorite (basaltic shergottite)
A single stone of 320 g was found in Morocco in March 2001. The exact
location of find is unknown and the meteorite was referred to under
the pseudonym "Djel Ibone". The meteorite has a fine-grained basaltic
texture consisting mainly of pyroxene (70 vol%) and maskelynite (23
vol%). Accessory minerals include merrillite, apatite, pyrrhotite,
chromite, Fe-Ti oxides, silica (stishovite) and baddeleyite. Melt
pockets with phenocrysts and submicron-sized needles of stishovite
are present. Pyroxenes are highly fractured. Calcite veins formed by
terrestrial weathering cross-cut the specimens. Classification and
mineralogy (A. Jambon, UPVI, V. Sautter, MNHNP, Ph. Gillet, ENSL):
pyroxenes are pigeonite, En48Fs39Wo13, and augite, En36Fs32Wo32;
maskelynite composition is An41-47Ab57-51Or2. Geochemistry (J.-A.
Barrat, UAng and Ch. Göpel, IPGP): bulk composition in wt% is 0.81
TiO2, 6.83 Al2O3, 17.8 FeO*, 0.49 MnO, 9.51 MgO, 10.2 CaO, 1.28
Na2O, 0.13 K2O. Trace elements 77 ppm Ni and a REE pattern similar to
that of Shergotty and Zagami. Key element weight-ratios are FeO*/MnO
~30, Na/Al ~0.40, K/La of 500 and Ga/Al of 4.1x10-4. Abundances of Ba
and Sr and the Th/U ratio indicate that terrestrial weathering is
minor. Specimens: type specimen, 16 g, ENSL; main mass, Fectay.

Northwest Africa 1068
Morocco
Found 2001 April
Martian meteorite (basaltic shergottite)
In 2001 April, meteorite hunters of the local team of "La Mémoire de
la Terre" recovered 23 stones (one large mass, 522 g, and 22 small
fragments, <20 g; total known mass, 576.77 g) in the Moroccan Sahara.
Rocks are greenish-brown and partially coated by desert varnish; no
fusion crust; cracks filled with terrestrial calcium carbonate. Thin
shock veins and small melt pockets are abundant. Classification,
mineralogy and bulk chemistry (J.-A. Barrat, UAng, A. Jambon, UPVI,
M. Bohn, I-CB, Ph. Gillet, ENSL, V. Sautter, MNHNP, Ch. Göpel, IPGP,
M. Lesourd, SCIAM): consists of olivine (50 um to 2 mm) in a fine-
grained groundmass (average grain size ~100 um) of euhedral to
subhedral pyroxene crystals and interstitial maskelynite; minor
phases are chromite, Ti-chromite, ilmenite, ulvöspinel, sulfides,
merrillite, apatite, and a K-rich mesostasis; impact melt pockets (up
to 1.5 mm long) contain pyrrhotite spherules. Modal abundances of
impact melt pockets and calcite free areas: 52 vol% pyroxenes, 22 %
maskelynite, 21 % olivine, 2 % phosphates, 2 % opaque oxides and
sulfides, and 1 % K-rich mesostasis. Mineralogy: olivine (Fa28 to
Fa58); pyroxenes: pigeonite (En57Wo5Fs28 to En40Wo13Fs47; fe# (100
Fe/(Fe+Mg) == 29-54 at. %) and augite (En55Wo21Fs24 to En35Wo28Fs36;
fe# == 29-51 at. %) are present as separate crystals in roughly equal
volume proportions; maskelynite is zoned (An53Ab45Or2 to An49Ab48Or3)
but is locally An-poor (An35Ab57Or8); FeO-rich merrillite (FeO 1.3
and 2.8 wt.%); apatites, Cl 0.5-2.5 wt% and F 1.1-6.4 wt%; chromite
have Ti-rich rims; ulvöspinels contain fine ilmenite lamellae (< 1
um thick). An interstitial K-rich component, probably a shock-
produced glass of alkali feldspar and silica, is generally associated
with Fe-Ti oxides. Bulk chemistry: Al-poor ferroan basaltic rock,
rich in MgO with major element abundances similar to those reported
for EETA79001 lithology A. Key element weight ratios are Fe/Mn == 45,
Al/Ti == 6.6, Na/Ti == 1.83, and Na/Al == 0.28. REE pattern similar to
Shergotty, Zagami, and Los Angeles. Specimens: type specimen, 20 g
and 2 polished sections, ENSL; main mass, Fectay.

Northwest Africa 1110
Morocco
Purchased 2001 November
Martian meteorite (basaltic shergottite)
G. and A. Hupe (Hupe) received a small sample of this meteorite in
2001 September and bought the rest from a dealer in Erfoud, Morocco
in 2001November . The weight of the total material purchased is 118
g. The place of recovery is believed to be in Morocco.
Classification and mineralogy (A. Irving and S. Kuehner, UWS):
consists of olivine phenocrysts in a fine-grained groundmass of
complexly-zoned pigeonite and homogenous maskelynite, Ab46Or2, with
minor ilmenite, Ti-magnetite and pyrrhotite. Euhedral to subhedral
olivine has Mg-rich cores (Fa28, FeO/MnO == 50) and narrow Fe-rich
rims (Fa51, FeO/MnO == 53) and contain inclusions of chromite and
glass; augite (Fs33Wo21) occurs as rare inclusions in olivine;
pigeonite is zoned, Fs28Wo9 to Fs40Wo15 and FeO/MnO == 30; presence
of rare chlorapatite in mesostasis. Secondary features include minor
barite, commonly associated with chromite inclusions in olivine,
calcite, in a cross-cutting glass veinlet, and narrow zones of K-Al-
bearing glass or clay minerals along grain boundaries between
pyoxene and maskelynite. Mineral composition indicates that this rock
is possibly paired with NWA 1068. Specimens: type specimen, 20 g and
several thin sections, UWS; main mass, Hupe.

Sayh al Uhaymir 060 20°58.8' N, 57°19.1' E
Oman
Found 2001 June 27
Martian meteorite (basaltic shergottite)
A small 42.28 g partially crusted grey-greenish stone was found near
to the area of previous finds of Sayh al Uhaymir 005/008/051/094.
All five meteorites seem to be paired. Mineralogy and classification
(S. Afanasiev, Vernad): has a porphyritic texture with large olivine
phenocrysts (Fo63.1-70.8) set in a groundmass consisting of
maskelynite (An61.4-68.3 Or0.5-1.6) and pigeonite (En60-69.6 Wo7.1-
8.6), augite (En47 Wo35) is rare; shock stage, S5; slight weathering.
Analyzed by Dr. N. N. Kononkova (Vernad). Specimens: type specimen,
9.5 g, Vernad; main mass with anonymous finder

Sayh al Uhaymir 090 21°00.0' N, 57°19.2' E
[This 94.84 g stone is probably paired with Sayh al Uhaymir 060, as
well as 005/008/051/094]

 NASA AND VA ROLL OUT NEW PATIENT SAFETY REPORTING SYSTEM

As of March 2002, patients at Department of Veterans
Affairs (VA) hospitals and clinics nationwide will have an
extra pair of eyes looking out for their safety.

In collaboration with NASA, the VA is rolling out a new
medical reporting system, called the Patient Safety Reporting
System (PSRS), to most of its medical facilities nationwide.
The PSRS is an independent, external system that complements
the agency's current internal reporting systems. The PSRS is
modeled after NASA's Aviation Safety Reporting System (ASRS),
an incident-reporting program administered for the Federal
Aviation Administration by NASA Ames Research Center, Moffett
Field, Calif.

"The experience gained in operating the ASRS for 25 years
will be invaluable in establishing the collection of
voluntary, confidential data reported by health care
providers on the front line of patient care in VA
facilities," said Linda Connell, NASA ASRS/PSRS director.

"When individuals feel uncomfortable reporting to the
internal systems, they have a safety valve they can use - the
PSRS," added Dr. James Bagian, director of the VA's National
Center for Patient Safety (NCPS). The guiding principles of
the PSRS are improvement of patient safety through voluntary
participation, confidential reporting, and non-punitive
provisions for VA employees who choose to participate,
according to officials.

The VA operates 163 medical centers across the country and
last year had more than 3 million patients enrolled in its
health-care system. The PSRS invites all VA medical facility
staff to voluntarily report any events or concerns that
involve patient safety.

PSRS forms and information are available at VA medical
facilities and on the Internet at:

http://psrs.arc.nasa.gov

 CHANDRA UNCOVERS EVIDENCE FOR A NEW FORM OF MATTER: SPACE
SCIENCE UPDATE, APRIL 10

New observations from NASA's Chandra X-Ray Observatory
provide a window to new forms of matter. This significant
discovery, which challenges some of the most fundamental
questions in physics, is the topic of a Space Science Update
scheduled for 9 a.m. EDT Wednesday, April 10, in the James E.
Webb Auditorium at NASA Headquarters, 300 E St. SW in
Washington.

The Space Science Update panelists will be:
* Anne Kinney, director of the Astronomy and Physics
Division, Office of Space Science, NASA headquarters,
Washington
* Jeremy Drake, Astrophysicist, Harvard-Smithsonian Center
for Astrophysics, Cambridge, Mass.
* Norman Glendenning, Senior Scientist Emeritus, Lawrence
Berkeley National Laboratory, Berkeley, Calif.
* David Helfand, Professor of Astronomy & Astrophysics,
Columbia University, New York
* Michael Turner, Professor and Chair of the Department of
Astronomy and Astrophysics, University of Chicago

The Space Science Update will be carried live on NASA
Television with two-way question-and-answer capability for
reporters covering the briefing from NASA centers. NASA TV is
broadcast on satellite GE-2, transponder 9C, at 85 degrees
West longitude, vertical polarization, frequency 3880 MHz,
audio of 6.8 MHz.

The briefing will also be webcast live on the Internet at:

http://www.nasa.gov

 NASA SPACECRAFT FINDS COMET HAS HOT, DRY SURFACE

Comets are sometimes described as "dirty snowballs," but
a close flyby of one by NASA's Deep Space 1 spacecraft last
fall detected no frozen water on its surface.

Comet Borrelly has plenty of ice beneath its tar-black
surface, but any exposed to sunlight has vaporized away, say
scientists analyzing data from Deep Space 1, managed by NASA's
Jet Propulsion Laboratory, Pasadena, Calif.

"The spectrum suggests that the surface is hot and dry.
It is surprising that we saw no traces of water ice," said Dr.
Laurence Soderblom of the U.S. Geological Survey's Flagstaff,
Ariz., station, lead author of a report on the Borrelly flyby
results appearing in the online edition of the journal
Science.

"We know the ice is there," he said. "It's just well-
hidden. Either the surface has been dried out by solar heating
and maturation or perhaps the very dark soot-like material
that covers Borrelly's surface masks any trace of surface
ice."

The Deep Space 1 science team released pictures and other
initial findings days after the spacecraft flew within 2,171
kilometers (1,349 miles) of the comet's solid nucleus on
September 22, 2001. This week's report provides additional
details about the nucleus and the surrounding coma of gases
and dust coming off of the comet as measured by one of Deep
Space 1's scientific instruments.

"Comet Borrelly is in the inner solar system right now,
and it's hot, between 26 and 71 degrees Celsius (80 and 161
degrees Fahrenheit), so any water ice on the surface would
change quickly to a gas, " said Dr. Bonnie Buratti, JPL
planetary scientist and co-author of the paper. "As the
components evaporate, they leave behind a crust, like the
crust left behind by dirty snow."

Borrelly is unusually dark for an object in the inner
solar system. The comet's surface is about as dark as a blot
of photocopy toner, possibly the darkest surface in the solar
system. It is more like objects in the outer solar system such
as the dark side of Saturn's moon Iapetus and the rings of
Uranus.

"It seems to be covered in this dark material, which has
been loosely connected with biological material." Buratti
said. "This suggests that comets might be a transport
mechanism for bringing the building blocks of life to Earth."
Comets may have played an important role in supplying organic
materials that are required for life to originate.

Soderblom points out that Borrelly's old, mottled
terrain with dark and very dark spots -- different shades of
black -- are apparently inactive. Ground-based observations
estimated that 90 percent of Borrelly's surface might be
inactive, and the observations taken by Deep Space 1 show that
this is indeed true.

"It's remarkable how much information Deep Space 1 was
able to gather at the comet, particularly given that this was
a bonus assignment for the probe," said Dr. Marc Rayman,
project manager of the mission. Deep Space 1 completed its
original goal to test 12 new space technologies and then
earned extra credit by achieving additional goals, such as the
risky Borrelly flyby. "It's quite exciting now as scientists
working with this rich scientific harvest turn data into
knowledge."

Images of comet Borrelly from Deep Space 1 are available
at
http://www.jpl.nasa.gov/images/ds1/ds1_borrelly.html .

More information on the Deep Space 1 mission is available
at
http://nmp.jpl.nasa.gov/ds1/ .

Deep Space 1 was launched in October 1998 as part of
NASA's New Millennium Program, which is managed by JPL for
NASA's Office of Space Science, Washington, D.C. The
California Institute of Technology, Pasadena, manages JPL for
NASA.

 http://science.nasa.gov/headlines/y2002/05apr_hitchhiker.htm

Hitchhiker's Guide to an Asteroid
NASA Science News

Learning what near-Earth asteroids are made of and how they're put together
is simply prudent. NASA's NEAR spacecraft did just that when it landed on
one in 2001.

April 5, 2002: When NASA's Near Earth Asteroid Rendezvous (NEAR) Shoemaker
spacecraft visited the asteroid 433 Eros last year, no one was on board. It
was strictly excitement from a distance, exploring the potato-shaped
20-by-8-by-8-mile worldlet through robotic eyes.

But what if you could have hitched a ride on the automobile-sized spacecraft
from its launch in February 1996 through its first-ever landing on an
asteroid? What would you have seen--and discovered?

In early 2000, after nearly four years en route, you would have been excited
to be approaching Eros at last--slowly enough to be captured into orbit
despite the relatively small body's weak gravity. Then you would have had a
year to examine the curious object from all angles, both in darkness and in
sunlight, and from distances ranging from 200 miles down to as close as 22
miles. Lastly, in a thrilling four-hour finale on February 14, 2001, you
would have clung to NEAR as it oh-so-gently settled down onto the very
surface of Eros at merely walking speed, to rest on the tips of two solar
panels and the bottom edge of the spacecraft's body--a deliberately planned
interplanetary kiss on Valentine's Day with an asteroid named for the god of
love.

Why 433 Eros? As some asteroids in the main belt between Mars and Jupiter
are hundreds of miles across, wouldn't they have made more interesting
targets?

Bigger, yes, certainly. More interesting? Perhaps not.

433 Eros intrigued NEAR scientists for several reasons.

First, for figuring out what asteroids are made of, smaller is better than
bigger. Astronomers have long speculated that asteroids are remnants left
over from the original creation of the solar system more than 4.5 billion
years ago. But just what was that primoridal material? On Earth, because of
eons of volcanism and weathering, it's impossible to find an unchanged rock
that old. Asteroids the size of Eros, however, never got big enough to melt
and reform, so they are nearly pristine samples of the most primitive stuff
in the solar system.

And what ancient secrets might you have seen on Eros as you swooped down
close to its surface on NEAR?

Well, Eros may be ancient and geologically unchanged, but it also looks
startlingly weathered. Instead of sharp edges where it could have broken off
a larger body or been struck by another asteroid, peaks and crater rims are
rounded and worn--perhaps by a process called "gardening," in which small
impacts from interplanetary dust and gravel over millions of years wear away
sharp projections. Its surface is littered with thousands of loose boulders
the size of houses--most of them apparently having fallen back to the
surface after having been scoured out of the largest impact crater on Eros
(some 5 miles across).

Moreover, Eros is peppered with smaller craters partially filled with flat
ponds of fine bluish dust--dust that appears to settle in the craters as
smoothly as if it were a fluid. Both loose boulders and dust ponds are
astonishing to find on a body whose gravity is so weak that a 200-lb
basketball player would weigh only 2 ounces and would risk launching himself
into orbit with one good jump shot!

Another reason NASA targeted Eros is that, small as it is, it is actually
the second largest of a family of asteroids that can approach within 121
million miles of the sun--that is, possibly within a few million miles of
Earth. Aside from the Moon, such near-Earth asteroids (NEAs) are our closest
neighbors in the solar system--so it's just plain neighborly to go calling
and learn a bit more about them!

Finding out all we can about near-Earth asteroids is prudent. Although Eros
does not come close enough to Earth for a collision, other asteroids in
different orbits might. Indeed, many space rocks have struck Earth in the
distant past. Even now 40 to 100 tons of smaller interplanetary debris and
dust fall into Earth's atmosphere daily. If a rock larger than two-thirds of
a mile (1 kilometer) in diameter should slam into Earth, tidal waves,
firestorms, and other traumas could spell disaster for civilization and
possibly even for all of life on our planet. Right now, one NASA program is
scanning the heavens to inventory all near-Earth asteroids; so far, the
total is more than 1800, but only 400 or so are rated as "potentially
hazardous."

That's another reason for interest in visiting Eros--to find out how it (and
other NEAs) are constructed. Are they solid rock? Or are they--like many
mountains on Earth--more like compacted piles of rubble? To anyone
considering either redirecting an Earth-approaching asteroid into a
different (safer for Earth) orbit or blowing it to smithereens with a
thermonuclear warhead, it's essential to know where best to give the
asteroid an effective push or whether its fragments will disperse as much as
you hope.

The existence on 433 Eros of craters--and of square-shaped craters at
that--seem to suggest the asteroid is one solid body of fractured rock, of
one uniform composition similar to the most ancient known meteorites (called
chondrites) of material probably older than Earth. At least, that's the
prevailing view of most scientists since having seen it close-up through
NEAR's cameras and having probed it with NEAR's gamma-ray spectrometer after
the craft landed.

Perhaps such solid rock might it make a good bedrock foundation for a mining
operation.... (Maybe as the first squatter on Eros, NEAR should file a
prospector's claim.) Could there be ice frozen in the fractures? Cou