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Friday, May 30, 2008

Mars Odyssey THEMIS Images: May 19-23, 2008

MARS ODYSSEY THEMIS IMAGES
May 26-30, 2008

o Labeatis Catenae (Released 26 May 2008)

http://themis.asu.edu/zoom-20080526a

o Tartarus Montes (Released 27 May 2008)

http://themis.asu.edu/zoom-20080527a

o Kasei Channels (Released 28 May 2008)

http://themis.asu.edu/zoom-20080528a

o Kasei Valles (Released 29 May 2008)

http://themis.asu.edu/zoom-20080529a

o Kasei Valles (Released 30 May 2008)

http://themis.asu.edu/zoom-20080530a


All of the THEMIS images are archived here:

http://themis.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 co.oration 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.

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MRO HiRISE Images - May 28, 2008

MARS RECONNAISSANCE ORBITER HIRISE IMAGES
May 28, 2008

o Descent of the Phoenix Lander

http://hirise.lpl.arizona.edu/phoenix-descent.php

o First Image of Phoenix Lander Hardware: EDL + 11

http://hirise.lpl.arizona.edu/phoenix-hardware_11.php

o HiRISE Images Phoenix Lander Hardware: EDL + 22

http://hirise.lpl.arizona.edu/phoenix-hardware.php

o Gullies of Crater Wall in Terra Sirenum

http://hirise.lpl.arizona.edu/PSP_006760_1370


All of the HiRISE images are archived here:

http://hirise.lpl.arizona.edu/

Information about the Mars Reconnaissance Orbiter is online at

http://www.nasa.gov/mro. The mission is managed by NASA's Jet Propulsion
Laboratory, a division of the California Institute of Technology, for the NASA
Science Mission Directorate, Washington, D.C. Lockheed Martin Space Systems,
of Denver, is the prime contractor and built the spacecraft. HiRISE is operated by t
he University of Arizona. Ball Aerospace and Technologies Corp., of Boulder, Colo.,
built the HiRISE instrument.

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NASA'S Phoenix Lander Robotic Arm Camera Sees Possible Ice

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Guy Webster 818-354-5011
Jet Propulsion Laboratory, Pasadena, Calif.
Guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
Dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu

NEWS RELEASE: 2008-090 May 30, 2008

NASA'S Phoenix Lander Robotic Arm Camera Sees Possible Ice

TUCSON, Ariz.-- Scientists have discovered what may be ice that was exposed when soil was blown
away as NASA's Phoenix spacecraft landed on Mars last Sunday, May 25. The possible ice appears
in an image the robotic arm camera took underneath the lander, near a footpad.

"We could very well be seeing rock, or we could be seeing exposed ice in the retrorocket blast zone,"
said Ray Arvidson of Washington University, St. Louis, Mo., co-investigator for the robotic arm.
"We'll test the two ideas by getting more data, including color data, from the robotic arm camera. We
think that if the hard features are ice, they will become brighter because atmospheric water vapor will
collect as new frost on the ice.

"Full confirmation of what we're seeing will come when we excavate and analyze layers in the nearby
workspace," Arvidson said.

Testing last night of a Phoenix instrument that bakes and sniffs samples to identify ingredients
identified a possible short circuit. This prompted commands for diagnostic steps to be developed and
sent to the lander in the next few days. The instrument is the Thermal and Evolved Gas Analyzer. It
includes a calorimeter that tracks how much heat is needed to melt or vaporize substances in a
sample, plus a mass spectrometer to examine vapors driven off by the heat. The Thursday, May 29,
tests recorded electrical behavior consistent with an intermittent short circuit in the spectrometer
portion.

"We have developed a strategy to gain a better understanding of this behavior, and we have identified
workarounds for some of the possibilities," said William Boynton of the University of Arizona,
Tucson, lead scientist for the instrument.

The latest data from the Canadian Space Agency's weather station shows another sunny day at the
Phoenix landing site with temperatures holding at minus 30 degrees Celsius (minus 22 degrees
Fahrenheit) as the sol's high, and a low of minus 80 degrees Celsius (minus 112 degrees Fahrenheit).
The lidar instrument was activated for a 15-minute period just before noon local Mars time, and
showed increasing dust in the atmosphere.

"This is the first time lidar technology has been used on the surface of another planet," said the
meteorological station's chief engineer, Mike Daly, from MDA in Brampton, Canada. "The team is
elated that we are getting such interesting data about the dust dynamics in the atmosphere."

The mission passed a "safe to proceed" review on Thursday evening, meeting criteria to proceed with
evaluating and using the science instruments.

"We have evaluated the performance of the spacecraft on the surface and found we're ready to move
forward. While we are still investigating instrument performance such as the anomaly on TEGA
[Thermal and Evolved Gas Analyzer], the spacecraft's infrastructure has passed its tests and gets a
clean bill of health," said David Spencer of NASA's Jet Propulsion Laboratory, Pasadena, Calif.,
deputy project manager for Phoenix.

"We're still in the process of checking out our instruments," Phoenix project scientist Leslie Tamppari
of JPL said. "The process is designed to be very flexible, to respond to discoveries and issues that
come up every day. We're in the process of taking images and getting color information that will help
us understand soil properties. This will help us understand where best to first touch the soil and then
where and how best to dig."

The Phoenix mission is led by Peter Smith at the University of Arizona with project management at
JPL and development partnership at Lockheed Martin, Denver. International contributions come from
the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of
Copenhagen and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological
Institute. For more about Phoenix, visit:

http://www.nasa.gov/phoenix

and
http://phoenix.lpl.arizona.edu.

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Thursday, May 29, 2008

NASA Phoenix Mars Lander Puts Arm and Other Tools to Work

Contacts: Guy Webster 818-354-5011
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu

News Release: 2008-089 May 29, 2008

NASA Phoenix Mars Lander Puts Arm and Other Tools to Work

TUCSON, Ariz. - NASA's Mars lander is returning more detailed images from the Martian surface
and is now preparing its instruments for science operations.

Phoenix transmitted a 360-degree panorama of its frigid Martian world, freed its nearly 8-foot robotic
arm, tested a laser instrument for studying dust and clouds, and transmitted its second weather report
on Wednesday evening.

"We've imaged the entire landing site, all 360 degrees of it. We see it all," said Phoenix principal
investigator Peter Smith, University of Arizona, Tucson. "You can see the lander in a fish-eye view
that goes all the way out to the entire horizon "We are now making plans for where to dig first, and
what we'll save for later."

Commands were communicated to Phoenix to rotate the robotic arm's wrist to unlatch its launch lock,
raise the forearm and move it upright to release the elbow restraint.

"We're pleased that we successfully unstowed the robotic arm. In fact, this is the first time we have
moved the arm in about a year," said Matthew Robinson of NASA's Jet Propulsion Laboratory in
Pasadena, Calif. The arm deployment brings the Phoenix mission to a significant milestone.

"We have achieved all of our engineering characterization prerequisites, with all the critical
deployments behind us," said JPL's Barry Goldstein, Phoenix project manager. "We're now at a phase
of the mission where we're characterizing the science payload instruments. That's a very important
step for us."

After a health check that tests the arm at a range of warmer and colder temperatures, the titanium and
aluminum arm will soon be tasked with its first assignment: to use its camera to look under the
spacecraft to assess the terrain and underside of the lander.

The robotic arm will later trench into the icy layers of northern polar Mars and deliver samples to
instruments that will analyze what this part of Mars is made of, what its water is like, and whether it
is or has ever been a possible habitat for life.

Another milestone for the mission included the activation of the laser instrument called light
detection and ranging instrument, or lidar.

"The Canadians are walking on moonbeams. It's a huge achievement for us," said Jim Whiteway
Canadian Science lead from York University, Toronto. The lidar is a critical component of Phoenix's
weather station, provided by the Canadian Space Agency. The instrument is designed to detect dust,
clouds and fog by emitting rapid pulses of green laser-like light into the atmosphere. The light
bounces off particles and is reflected back to a telescope.

"One of the main challenges we faced was to deliver the lidar from the test lab in Ottawa, Canada, to
Mars while maintaining its alignment within one one-hundredth of a degree," said Whiteway. "That's
like aiming a laser pointer at a baseball at a distance from home plate to the center field wall, holding
that aim steady after launch for a year in space, then landing," he added.

Lidar data shows dust aloft to a height of 3.5 kilometers (2 miles). The weather at the Phoenix
landing site on the second day following landing was sunny with moderate dust, with a high of minus
30 degrees Celsius (minus 22 degrees Fahrenheit) and a low of minus 80 (minus 112 degrees
Fahrenheit).

The Phoenix mission is led by Smith at the University of Arizona with project management at JPL
and development partnership at Lockheed Martin, Denver. International contributions come from the
Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen
and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute. For
more about Phoenix, visit:

http://www.nasa.gov/phoenix .


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Scientists Hold Seance for Supernova

Media contact: Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov

News Release: 2008-088 May 29, 2008

Scientists Hold Seance for Supernova

Astronomers have unearthed secrets from the grave of a star that blasted apart in a
supernova explosion long ago. By decoding ghostly echoes of light traveling away from
the remains of a supernova called Cassiopeia A, the scientists have pieced together what
the star looked like in life, and ultimately how it met its demise.

The discovery, made using primarily NASA's Spitzer Space Telescope and Japan's
Subaru telescope on Mauna Kea in Hawaii, represents the first time astronomers have
been able to resurrect the life history of a supernova remnant in our own galaxy.

"Cassiopeia A lies in our cosmic backyard and offers the sharpest view of what is left
hundreds of years after a supernova explosion," said Oliver Krause of the Max Planck
Institute for Astronomy in Germany, lead author of a paper about the discovery appearing
in this week's Science. "The echoes of light we found around Cassiopeia A provide us
with a time machine to go back and see its past."

Cassiopeia A is one of the most explored objects in our sky and the subject of more than
1,000 scientific papers. It is the burnt-out corpse of a massive star that ended its life in a
fiery supernova about 11,300 years ago. In fact, until recently, it was the youngest
supernova remnant in our Milky Way galaxy (the new record holder, G1.9+0.3, was
recently discovered using NASA's Chandra X-ray Observatory and other ground-based
telescopes). Because Cassiopeia A is 11,000 light-years from Earth, the light from its
explosion would have reached Earth, sweeping right past it, about 300 years ago.

Astronomers had thought this supernova light was never to be seen again, until 2005,
when Krause and his colleagues discovered hints of it still bouncing around clouds
surrounding the remnant (http://www.spitzer.caltech.edu/Media/releases/ssc2005-
14/index.shtml ). Using Spitzer's infrared eyes, they found so-called infrared echoes,
which occur when a flash of light from the supernova blasts through clouds, heating them
up and causing them to glow in infrared. As the light rolls outward, the infrared echoes
continue to flare up and travel away from the star (see new movie of this effect at

http://www.nasa.gov/mission_pages/spitzer/multimedia/20080529-anim.html).

In the new study, the astronomers used Cassiopeia A's infrared echoes to hone in on faint
visible-light echoes with Subaru and other ground-based telescopes. Visible-light echoes,
known simply as light echoes, occur when visible light from the supernova scatters off
dust. Unlike infrared echoes, they are direct signals from the graves of exploded stars,
bearing all the information about the nature of the original blast.

Next, the astronomers had to act quickly because these echoes can fade within weeks.
They used Subaru's spectrometer instrument to break the light apart and reveal signatures
of atoms present when Cassiopeia A exploded. The resulting spectrum of light revealed
hydrogen and helium -- telltale signs that Cassiopeia A was once a huge red supergiant
star whose core collapsed in a rare supernova referred to as Type IIb. Previously,
scientists did not know the supernova class to which Cassiopeia A belonged.

"This is an exciting result," said Alex Filippenko of the University of California,
Berkeley, a supernova expert not affiliated with the study. "Cassiopeia A has been
studied extensively with many telescopes over a wide range of wavelengths. It is
gratifying that we finally know what kind of star exploded so long ago."

The findings also offer insight into another mystery shrouding Cassiopeia A. When
Cassiopeia A's original star erupted, the event should have been widely witnessed on
Earth as a bright star lighting up the sky. The most likely possible sighting is by the
Astronomer Royal John Flamsteed in 1680, but he made just one observation of a dim
star. The fact that almost no one saw the event is a classic problem in supernova lore.

Now that astronomers have learned how Cassiopeia A was forged, they think they might
know why its death went unnoticed. "Type IIb supernovas fade quickly," said co-author
George Rieke of the University of Arizona in Tucson. "This, plus a few cloudy nights,
might explain the historical enigma around Cassiopeia A."

Recently, astronomers using Chandra, ESA's XMM-Newton Observatory and the Gemini
Observatory in Chile, were able to use light echoes to identify the origins of a supernova
outside our galaxy. That study, together with the new one, demonstrates the power of
light echoes for conjuring up the "ghosts" of long-dead stars.

Other co-authors include Stephan Birkmann and Miwa Goto of the Max Planck Institute
for Astronomy; Tomonori Usuda and Takashi Hattori of the National Astronomical
Observatory of Japan in Hawaii; and Karl Misselt of the University of Arizona. NASA's
Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer Space Telescope
mission for NASA's Science Mission Directorate, Washington. Science operations are
conducted at the California Institute of Technology, also in Pasadena. For more
information about Spitzer, visit http://www.spitzer.caltech.edu/spitzer and

http://www.nasa.gov/spitzer . For more information about Subaru, operated by the
National Astronomical Observatory of Japan, visit

http://subarutelescope.org .

-end-

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Wednesday, May 28, 2008

NASA's Phoenix Spacecraft Commanded to Unstow Arm

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Guy Webster 818-354-5011
Jet Propulsion Laboratory, Pasadena, Calif.
Guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
Dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu

NEWS RELEASE: 2008-087 May 28, 2008

NASA's Phoenix Spacecraft Commanded to Unstow Arm

Scientists leading NASA's Phoenix Mars mission from the University of Arizona in
Tucson sent commands to unstow its robotic arm and take more images of its landing site
early today.

The Phoenix lander sent back new sharp color images from Mars late yesterday. Phoenix
imaging scientists made a color mosaic of images taken by the lander's Surface Stereo
Imager on landing day, May 25, and the first two full "sols," or Martian days, after
landing.

The panorama, now about one-third complete, shows a fish-eye perspective from the
camera, a view from the lander itself all the way to the horizon. Phoenix adjusts its color
vision with "Caltargets," calibrated color targets on disks mounted on the landing deck.
Its color vision isn't quite like human color vision, but close.

"These images are very exciting to the science team," said the Surface Stereo Imager co-
investigator Mark Lemmon of Texas A&M University. "We see the polygons we're
looking for, and we're very excited to fill in the context with more site pan images that go
beyond the workspace." Images to complete the panorama are planned today and
tomorrow, Sols 3 and 4, Lemmon said.

"We appear to have landed where we have access to digging down a polygon trough the
long way, digging across the trough, and digging into the center of a polygon. We've
dedicated this polygon as the first national park system on Mars -- a "keep out" zone
until we figure out how best to use this natural Martian resource," Lemmon said.

Phoenix will use its robotic arm to dig first in another area seen in the panorama, an area
outside the preserved polygon.

Robotic arm manager Bob Bonitz of NASA's Jet Propulsion Laboratory, Pasadena, Calif.,
explained how the arm is to be unstowed today. "It's a series of seven moves, beginning
with rotating the wrist to release the forearm from its launch restraint. Another series of
moves releases the elbow from its launch restraints and moves the elbow from
underneath the biobarrier."

The robotic arm is a critical part of the Phoenix Mars mission. It is needed to trench into
the icy layers of northern polar Mars and deliver samples to instruments that will analyze
what Mars is made of, what its water is like, and whether it is or has ever been a possible
habitat for life.

"Phoenix is in perfect health," JPL's Barry Goldstein, Phoenix project manager, said
Wednesday morning, May 28.

The robotic arm's first movement was delayed by one day when Tuesday's commands
from Earth did not get all the way to the Phoenix lander on Mars. The commands went to
NASA's Mars Reconnaissance Orbiter as planned, but the orbiter's Electra UHF radio
system for relaying commands to Phoenix temporarily shut off. Without new commands,
the lander instead carried out a set of activity commands sent Monday as a backup.
Images and other information from those activities were successfully relayed back to
Earth by the Mars Reconnaissance Orbiter Tuesday evening.

Wednesday morning's uplink to Phoenix and evening downlink from Phoenix were
planned with NASA's Mars Odyssey orbiter as the relay. "We are using Odyssey as our
primary link until we have a better understanding of what happened with Electra,"
Goldstein said.

The Phoenix mission is led by Peter Smith at the University of Arizona with project
management at JPL and development partnership at Lockheed Martin, Denver.
International contributions come from the Canadian Space Agency; the University of
Neuachatel, Switzerland; the universities of Copenhagen and Aarhus, Denmark; Max
Planck Institute, Germany; and the Finnish Meteorological Institute.
For more about Phoenix, visit http://www.nasa.gov/phoenix and

http://phoenix.lpl.arizona.edu.

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Strange Ring Found Circling Dead Star

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011

http://www.jpl.nasa.gov


Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov

NEWS RELEASE: 2008-086 May 28, 2008

Strange Ring Found Circling Dead Star

Pasadena, Calif. -- NASA's Spitzer Space Telescope has found a bizarre ring of material
around the magnetic remains of a star that blasted to smithereens.

The stellar corpse, called SGR 1900+14, belongs to a class of objects known as
magnetars. These are the cores of massive stars that blew up in supernova explosions, but
unlike other dead stars, they slowly pulsate with X-rays and have tremendously strong
magnetic fields.

"The universe is a big place and weird things can happen," said Stefanie Wachter of
NASA's Spitzer Science Center at the California Institute of Technology, Pasadena, who
found the ring serendipitously. "I was flipping through archived Spitzer data of the
object, and that's when I noticed it was surrounded by a ring we'd never seen before."
Wachter is lead author of a paper about the findings in this week's Nature. You can see
the ring at http://www.nasa.gov/mission_pages/spitzer/multimedia/20080528.html .

Wachter and her colleagues think that the ring, which is unlike anything ever seen before,
formed in 1998 when the magnetar erupted in a giant flare. They believe the crusty
surface of the magnetar cracked, sending out a flare, or blast of energy, that excavated a
nearby cloud of dust, leaving an outer, dusty ring. This ring is oblong, with dimensions of
about seven by three light-years. It appears to be flat, or two-dimensional, but the
scientists said they can't rule out the possibility of a three-dimensional shell.

"It's as if the magnetar became a huge flaming torch and obliterated the dust around it,
creating a massive cavity," said Chryssa Kouveliotou, senior astrophysicist at NASA's
Marshall Space Flight Center, Huntsville, Ala., and a co-author of the paper. "Then the
stars nearby lit up a ring of fire around the dead star, marking it for eternity."

The discovery could help scientists figure out if a star's mass influences whether it
becomes a magnetar when it dies. Though scientists know that stars above a certain mass
will "go supernova," they do not know if mass plays a role in determining whether the
star becomes a magnetar or a run-of-the-mill dead star. According to the science team,
the ring demonstrates that SGR 1900+14 belongs to a nearby cluster of young, massive
stars. By studying the masses of these nearby stars, the scientists might learn the
approximate mass of the original star that exploded and became SGR 1900+14.

"The ring has to be lit up by something, otherwise Spitzer wouldn't have seen it," said
Enrico Ramirez-Ruiz of the University of California, Santa Cruz. "The nearby massive
stars are most likely what's heating the dust and lighting it up, and this means that the
magnetar, which lies at the exact center of the ring, is associated with the massive star-
forming region."

Rings and spheres are common in the universe. Young, hot stars blow bubbles in space,
carving out dust into spherical shapes. When stars die in supernova explosions, their
remains are blasted into space, forming short-lived beautiful orbs called supernova
remnants. Rings can also form around exploded stars whose expanding shells of debris
ram into pre-existing dust rings, causing the dust to glow, as is the case with the
supernova remnant called 1987A.

But the ring around the magnetar SGR 1900+14 fits into none of these categories. For
one thing, supernova remnants and the ring around 1987A cry out with X-rays and radio
waves. The ring around SGR 1900+14 only glows at specific infrared wavelengths that
Spitzer can see.

At first, the astronomers thought the ring must be what's called an infrared echo. These
occur when an object sends out a blast wave that travels outward, heating up dust and
causing it to glow with infrared light. But when they went back to observe SGR 1900+14
later, the ring didn't move outward as it should have if it were an infrared echo.

A closer analysis of the pictures later revealed that the ring is most likely a carved-out
cavity in a dust cloud -- a phenomenon that must be somewhat rare in the universe since
it had not been seen before. The scientists plan to look for more of these rings.

"This magnetar is still alive in many ways," said Ramirez-Ruiz. "It is interacting with its
environment, making a big impact on the young star-forming region where it was born."

Other paper authors include V. Dwarkadas of the University of Chicago, Ill.; J. Granot of
the University of Hertfordshire, England; S.K. Patel of the Optical Sciences Corporation,
Huntsville, Ala.; and D. Figer of the Rochester Institute of Technology, N.Y. NASA's Jet
Propulsion Laboratory, Pasadena, Calif., manages the Spitzer mission for NASA's
Science Mission Directorate, Washington. Science operations are conducted at the
Spitzer Science Center. Caltech manages JPL for NASA. Spitzer's infrared array camera,
which made the observations, was built by NASA's Goddard Space Flight Center,
Greenbelt, Md. Its principal investigator is Giovanni Fazio of the Harvard-Smithsonian
Center for Astrophysics. For more information about Spitzer, visit

http://www.spitzer.caltech.edu/spitzer and http://www.nasa.gov/spitzer .

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Tuesday, May 27, 2008

NASA Satellites Illuminate Pollution's Influence on Clouds, Climate

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Alan Buis 818-354-0474
Jet Propulsion Laboratory, Pasadena, Calif.
Alan.buis@jpl.nasa.gov

Lynn Chandler 301-286-2806
NASA Goddard Space Flight Center, Greenbelt, Md.
lynn.chandler-1@nasa.gov

NEWS RELEASE: 2008-085 May 27, 2008

NASA Satellites Illuminate Pollution's Influence on Clouds, Climate

PASADENA, Calif. -- Using data from instruments in a constellation of NASA satellites,
scientists have discovered that they can see deep inside of clouds. The satellites are taking first-
of-a-kind measurements, shedding new light on the link between clouds, pollution and rainfall.

Jonathan Jiang of NASA's Jet Propulsion Laboratory, Pasadena, Calif., and colleagues used
sensors from multiple satellites in the Afternoon Constellation, more commonly called the A-
Train, to find that South American clouds infused with airborne pollution -- classified as
"polluted clouds" -- tend to produce less rain than their "clean" counterparts during the region's
dry season. Details of the findings are presented today at the American Geophysical Union's 2008
Joint Assembly in Fort Lauderdale, Fla.

"The A-Train is providing a new way to examine cloud types," said Mark Schoeberl, A-Train
project scientist at NASA's Goddard Space Flight Center, Greenbelt, Md.

Discovery of the link between rain and pollution was possible due to near-simultaneous
measurements from the A-Train satellites. "Typically, it is very hard to get a sense of how
important the effect of pollution on clouds is," said Anne Douglass, deputy project scientist at
Goddard for NASA's Aura satellite. "With the A-Train, we can see the clouds every day and
we're getting confirmation on a global scale that we have an issue here."

Jiang's team used the JPL-developed and managed Microwave Limb Sounder on the A-Train's
Aura satellite to measure the level of carbon monoxide in clouds. The presence of carbon
monoxide implies the presence of smoke and other aerosols, which usually come from the same
emission source, such a power plant or agricultural fire.

With the ability to distinguish between polluted and clean clouds, the team next used Aqua's
Moderate Resolution Imaging Spectroradiometer to study how ice particle sizes change when
aerosol pollution is present in the clouds. The team also used NASA's Tropical Rainfall
Measuring Mission satellite to measure the amount of precipitation falling from the polluted and
clean clouds. All three measurements together show the relationship between pollution, clouds
and precipitation.

The team found that polluted clouds suppressed rainfall during the June-to-October dry season in
South America, which is also a period of increased agricultural burning. During that period it was
more difficult for the measurably smaller ice particles in aerosol-polluted clouds to grow large
enough to fall as rain.

This trend turned up seasonal and regional differences, however, and aerosol pollution was
found, on average, to be less of a factor during the wet monsoon seasons in South America and in
South Asia. Other physical effects, such as large-scale dynamics and rainy conditions that clear
the air of aerosol particles, might also be at play, the researchers suggest.

"The complexity of interactions between aerosols and clouds poses difficult problems that no one
satellite instrument can solve," said Jiang. "But when you put parameters from multiple satellites
all together, you will find much more information than from a single instrument alone."

The five satellites of the A-Train -- NASA's Aqua, Aura, CloudSat, Cloud-Aerosol Lidar and
Infrared Pathfinder Satellite Observation (Calipso) and the French Space Agency's Polarization
and Anisotropy of Reflectances for Atmospheric Sciences coupled with Observations from a
Lidar, or Parasol -- orbit only eight minutes apart and can be thought of as an extended satellite
observatory, providing unprecedented information about clouds, aerosols and atmospheric
composition.

For information about NASA and agency programs, visit: http://www.nasa.gov/home . For
information about the Microwave Limb Sounder on Aura, visit: http://mls.jpl.nasa.gov/ .

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

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NASA Mars Lander Prepares to Move Arm

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Guy Webster 818-354-5011
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu

NEWS RELEASE: 2008-084 May 27, 2008

NASA Mars Lander Prepares to Move Arm

NASA's Phoenix Lander is ready to begin moving its robotic arm, first unlatching its
wrist and then flexing its elbow.

Mission scientists are eager to move Phoenix's robotic arm, for that arm will deliver
samples of icy terrain to their instruments made to study this unexplored Martian
environment.

The team sent commands for moving the arm on Tuesday morning, May 27, to NASA's
Mars Reconnaissance Orbiter for relay to Phoenix. However, the orbiter did not relay
those commands to the lander, so arm movement and other activities are now
planned for Wednesday. The orbiter's communication-relay system is in a standby mode.
NASA's Mars Odyssey orbiter is available for relaying communications between Earth and
Phoenix.

NASA's Mars Reconnaissance Orbiter did send back spectacular first images of the landed
Phoenix from orbit, views from the Phoenix lander of where it will work for the next three
months, and a preliminary weather report.

A newly processed image from the high-resolution camera known as HiRISE on NASA's
Mars Reconnaissance Orbiter shows a full-resolution view of the Phoenix parachute and
lander during its May 25 descent, with Heimdall crater in the background.

"Phoenix appears to be descending into the 10 kilometer, or 6-mile, crater, but is actually
20 kilometers, or about 12 miles, in front of the crater," said HiRISE principal investigator
Alfred S. McEwen of the University of Arizona, Tucson.

HiRISE has taken a new color image of Phoenix on the ground about 22 hours after
it landed. It shows the parachute attached to the back shell, the heat shield and the lander
itself against red Mars. The parachute and lander are about 300 meters, roughly 1,000 feet,
apart.

Commands to be sent to the lander Wednesday morning include taking more pictures of
the surroundings and making the first movements of the mission's crucial robotic arm.

A covering that had shielded the arm from microbes during its last few months before
launch had not fully retracted on landing day, May 25, but it moved farther from the arm
during the following day.

"The biobarrier had relaxed more and allows more clearance, but it was not a major
concern either way," said Fuk Li, manager of the Mars Exploration Program
at NASA's Jet Propulsion Laboratory, Pasadena, Calif.

During the next three months, the arm will dig into soil near the lander and deliver samples
of soil and ice to laboratory instruments on the lander deck. Following today's commands,
its movements will begin with unlatching the wrist, then moving the arm upwards in a
stair-step manner.

Phoenix principal investigator Peter Smith of the University of Arizona was delighted with
new images of the workspace. "The workspace is ideal for us because it looks very
diggable. We're very happy to see just a few rocks scattered in the digging area."

The Phoenix weather station, provided by the Canadian Space Agency, was activated
within the first hour after landing on Mars, and measurements are now being recorded
continuously. The data from the first 18 hours after landing have been transmitted back to
the science team, and they have provided a weather report. The temperature ranged
between a minimum of minus 80 degrees Celsius (minus 112 degrees Fahrenheit) in the
early morning and a maximum of minus 30 degrees Celsius (minus 22 degrees Fahrenheit)
in the afternoon. The average pressure was 8.55 millibars, which is less than a hundredth
of the sea level pressure on Earth. The wind speed was 20 kilometers per hour (13 miles
per hour), out of the northeast. The skies were clear. More instruments will be activated
over the coming days, and the weather report will expand to include measurements of
humidity and visibility.

Smith presented a new Surface Stereo Imager view of the American flag and a mini-DVD
on the Phoenix's deck, about three feet above the Martian surface. The mini-DVD from the
Planetary Society contains a message to future Martian explorers, science fiction stories
and art inspired by the Red Planet, and the names of more than a quarter million
Earthlings.

The Phoenix mission is led by Smith at the University of Arizona with project
management at JPL and development partnership at Lockheed Martin. International
contributions come from the Canadian Space Agency; the University of Neuchatel,
Switzerland; the universities of Copenhagen and Aarhus, Denmark; Max Planck Institute,
Germany; and the Finnish Meteorological Institute. More Phoenix information is at

http://www.nasa.gov/phoenix .

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Monday, May 26, 2008

Camera on Mars Orbiter Snaps Phoenix During Landing

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Guy Webster 818-354-5011
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu

NEWS RELEASE: 2008-083 May 26, 2008

Camera on Mars Orbiter Snaps Phoenix During Landing

PASADENA, Calif. -- A telescopic camera in orbit around Mars caught a view of NASA's Phoenix
Mars Lander suspended from its parachute during the lander's successful arrival at Mars Sunday
evening, May 25.

The image from the High Resolution Imaging Science Experiment (HiRISE) on NASA's Mars
Reconnaissance Orbiter marks the first time ever one spacecraft has photographed another one in the
act of landing on Mars.

Meanwhile, scientists pored over initial images from Phoenix, the first ever taken from the surface of
Mars' polar regions. Phoenix returned information that it was in good health after its first night on
Mars, and the Phoenix team sent the spacecraft its to-do list for the day.

"We can see cracks in the troughs that make us think the ice is still modifying the surface," said
Phoenix Principal Investigator Peter Smith of the University of Arizona, Tucson. "We see fresh
cracks. Cracks can't be old. They would fill in."

Camera pointing for the image from HiRISE used navigational information about Phoenix updated on
landing day. The camera team and Phoenix team would not know until the image was sent to Earth
whether it had actually caught Phoenix.

"We saw a few other bright spots in the image first, but when we saw the parachute and the lander
with the cords connecting them, there was no question," said HiRISE Principal Investigator Alfred
McEwen, also of the University of Arizona.

"I'm floored. I'm absolutely floored," said Phoenix Project Manager Barry Goldstein of NASA's Jet
Propulsion Laboratory, Pasadena, Calif. A team analyzing what can be learned from the Phoenix
descent through the Martian atmosphere will use the image to reconstruct events.

HiRISE usually points downward. For this image, the pointing was at 62 degrees, nearly two-thirds
of the way from straight down to horizontal. To tilt the camera, the whole orbiter must tilt. Mars
Reconnaissance Orbiter was already pointed toward the expected descent path of Phoenix to record
radio transmissions from Phoenix.

McEwen said, "We've never taken an image at such an oblique angle before."

Monday's tasks for Phoenix include checkouts of some instruments and systems, plus additional
imaging of the lander's surroundings.

The Phoenix mission is led by Smith at the University of Arizona with project management at JPL
and development partnership at Lockheed Martin, Denver. International contributions come from the
Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen
and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute. For
more about Phoenix, visit:

http://www.nasa.gov/phoenix .

JPL manages the Mars Reconnaissance Orbiter mission for NASA. Lockheed Martin Space Systems,
Denver, Colo., is the prime contractor for the project and built the spacecraft. The University of
Arizona operates the High Resolution Imaging Science Experiment camera, which was built by Ball
Aerospace and Technology Corp., Boulder, Colo.

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Sunday, May 25, 2008

NASA'S Phoenix Spacecraft Reports Good Health After Mars Landing

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Guy Webster 818-354-5011
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu

NEWS RELEASE: 2008-082 May 25, 2008

NASA'S Phoenix Spacecraft Reports Good Health After Mars Landing

PASADENA, Calif. -- A NASA spacecraft today sent pictures showing itself in good condition after
making the first successful landing in a polar region of Mars.

The images from NASA's Mars Phoenix Lander also provided a glimpse of the flat valley floor
expected to have water-rich permafrost within reach of the lander's robotic arm. The landing ends a
422-million-mile journey from Earth and begins a three-month mission that will use instruments to
taste and sniff the northern polar site's soil and ice.

"We see the lack of rocks that we expected, we see the polygons that we saw from space, we don't see
ice on the surface, but we think we will see it beneath the surface. It looks great to me," said Peter
Smith of the University of Arizona, Tucson, principal investigator for the Phoenix mission.

Radio signals received at 4:53:44 p.m. Pacific Time (7:53:44 p.m. Eastern Time) confirmed that the
Phoenix Mars Lander had survived its difficult final descent and touchdown 15 minutes earlier. In the
intervening time, those signals crossed the distance from Mars to Earth at the speed of light. The
confirmation ignited cheers by mission team members at NASA's Jet Propulsion Laboratory,
Pasadena, Calif.; Lockheed Martin Space Systems, Denver; and the University of Arizona.

As planned, Phoenix stopped transmitting one minute after landing and focused its limited battery
power on opening its solar arrays, and other critical activities. About two hours after touchdown, it
sent more good news. The first pictures confirmed that the solar arrays needed for the mission's
energy supply had unfolded properly, and masts for the stereo camera and weather station had swung
into vertical position.


"Seeing these images after a successful landing reaffirmed the thorough work over the past five years
by a great team," said Phoenix Project Manager Barry Goldstein of JPL. A key milestone still ahead
is the first use of the lander's 7.7-foot-long robotic arm, not planned before Tuesday.

"Only five of our planet's 11 previous attempts to land on the Red Planet have succeeded. In
exploring the universe, we accept some risk in exchange for the potential of great scientific rewards,"
said Ed Weiler, NASA associate administrator for the Science Mission Directorate, Washington.

Phoenix carries science instruments to assess whether ice just below the surface ever thaws and
whether some chemical ingredients of life are preserved in the icy soil. These are key questions in
evaluating whether the environment has ever been favorable for microbial life. Phoenix will also
study other aspects of the soil and atmosphere with instrument capabilities never before used on
Mars. Canada supplied the lander's weather station.

Transmissions from Phoenix have reported results after a check of several components and systems
on the spacecraft. "Phoenix is an amazing machine, and it was built and flown by an amazing team.
Through the entire entry, descent and landing phase, it performed flawlessly," said Ed Sedivy,
Phoenix program manager at Lockheed Martin Space Systems Company. "The spacecraft stayed in
contact with Earth during that critical period, and we received a lot of data about its health and
performance. I'm happy to report it's in great shape."

Phoenix uses hardware from a spacecraft built for a 2001 launch that was canceled in response to the
loss of a similar Mars spacecraft during a 1999 landing attempt. Researchers who proposed the
Phoenix mission in 2002 saw the unused spacecraft as a resource for pursuing a new science
opportunity. A few months earlier, NASA's Mars Odyssey orbiter discovered that plentiful water ice
lies just beneath the surface throughout much of high-latitude Mars. NASA chose the Phoenix
proposal over 24 other proposals to become the first endeavor in the Mars Scout program of
competitively selected missions.

The signal confirming that Phoenix had survived touchdown and the transmission of the first pictures
were relayed via Mars Odyssey and received on Earth at the Goldstone, Calif., antenna station of
NASA's Deep Space Network.

The Phoenix mission is led by Smith at the University of Arizona with project management at JPL
and development partnership at Lockheed Martin. International contributions come from the
Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen
and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute. For
more about Phoenix, visit http://www.nasa.gov/phoenix .

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NASA'S Phoenix Spacecraft Lands at Martian Arctic Site

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov


Guy Webster 818-354-5011
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu

NEWS RELEASE: 2008-081 May 25, 2008

NASA'S Phoenix Spacecraft Lands at Martian Arctic Site

PASADENA, Calif. -- NASA's Phoenix spacecraft landed in the northern polar region of Mars today
to begin three months of examining a site chosen for its likelihood of having frozen water within
reach of the lander's robotic arm.

Radio signals received at 4:53:44 p.m. Pacific Time (7:53:44 p.m. Eastern Time) confirmed the
Phoenix Mars Lander had survived its difficult final descent and touchdown 15 minutes earlier. The
signals took that long to travel from Mars to Earth at the speed of light.

Mission team members at NASA's Jet Propulsion Laboratory, Pasadena, Calif.; Lockheed Martin
Space Systems, Denver; and the University of Arizona, Tucson, cheered confirmation of the landing
and eagerly awaited further information from Phoenix later tonight.

Among those in the JPL control room was NASA Administrator Michael Griffin, who noted this was
the first successful Mars landing without airbags since Viking 2 in 1976.

"For the first time in 32 years, and only the third time in history, a JPL team has carried out a soft
landing on Mars," Griffin said. "I couldn't be happier to be here to witness this incredible
achievement."

During its 422-million-mile flight from Earth to Mars after launching on Aug. 4, 2007, Phoenix relied
on electricity from solar panels during the spacecraft's cruise stage. The cruise stage was jettisoned
seven minutes before the lander, encased in a protective shell, entered the Martian atmosphere.
Batteries provide electricity until the lander's own pair of solar arrays spread open.

"We've passed the hardest part and we're breathing again, but we still need to see that Phoenix has
opened its solar arrays and begun generating power," said JPL's Barry Goldstein, the Phoenix project
manager. If all goes well, engineers will learn the status of the solar arrays between 7 and 7:30 p.m.
Pacific Time (10 and 10:30 p.m. Eastern Time) from a Phoenix transmission relayed via NASA's
Mars Odyssey orbiter.

The team will also be watching for the Sunday night transmission to confirm that masts for the stereo
camera and the weather station have swung to their vertical positions.

"What a thrilling landing! But the team is waiting impatiently for the next set of signals that will
verify a healthy spacecraft," said Peter Smith of the University of Arizona, principal investigator for
the Phoenix mission. "I can hardly contain my enthusiasm. The first landed images of the Martian
polar terrain will set the stage for our mission."

Another critical deployment will be the first use of the 7.7-foot-long robotic arm on Phoenix, which
will not be attempted for at least two days. Researchers will use the arm during future weeks to get
samples of soil and ice into laboratory instruments on the lander deck.

The signal confirming that Phoenix had survived touchdown was relayed via Mars Odyssey and
received on Earth at the Goldstone, Calif., antenna station of NASA's Deep Space Network.

Phoenix uses hardware from a spacecraft built for a 2001 launch that was canceled in response to the
loss of a similar Mars spacecraft during a 1999 landing attempt. Researchers who proposed the
Phoenix mission in 2002 saw the unused spacecraft as a resource for pursuing a new science
opportunity. Earlier in 2002, Mars Odyssey discovered that plentiful water ice lies just beneath the
surface throughout much of high-latitude Mars. NASA chose the Phoenix proposal over 24 other
proposals to become the first endeavor in the Mars Scout program of competitively selected missions.

The Phoenix mission is led by Smith at the University of Arizona with project management at JPL
and development partnership at Lockheed Martin, Denver. International contributions come from the
Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen
and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute. For
more about Phoenix, visit http://www.nasa.gov/phoenix .

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Mars Pulls Phoenix In

Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu

News Release: 2008-080 May 25, 2008

Mars Pulls Phoenix In

PASADENA, Calif. -- NASA's Phoenix Mars Lander sped on Sunday morning toward its arrival
at Mars, as the tug of the Red Planet's gravity accelerated the craft during the final day of its trip
from Earth to Mars.

"Mars is literally pulling on our spacecraft, and at the same time it is pulling on our emotions,"
Phoenix Principal Investigator Peter Smith, of the University of Arizona, Tucson, said early
Sunday afternoon. "We are excited at how close we are right now to beginning our study of a site
where Martian water ice will be within our reach, after all these years of preparations. Our
science mission begins as the spacecraft settles into its new home on Mars."

The spacecraft's speed relative to Mars increased from 6,300 miles per hour at 8:30 a.m. Pacific
Time to 8,500 mph at 12:30 p.m., headed for a speed higher than 12,000 mph before reaching the
top of the Martian atmosphere.

Phoenix was on track for anticipated entry into the atmosphere at 4:30p.m. Pacific Time and
reaching the surface at 4:38 p.m., although confirmation of those events comes no sooner than 15
minutes, 20 seconds later, due to the time needed for radio signals to travel from Mars to Earth.

Mission controllers decided Saturday night and Sunday morning to forgo the last two
opportunities for adjusting the spacecraft's trajectory.

"We are so well on course that those adjustments were not necessary," said Phoenix Project
Manager Barry Goldstein of NASA's Jet Propulsion Laboratory, Pasadena, Calif.

The most challenging part of the entire mission, getting from the top of the atmosphere to a safe
landing on three legs, still lies ahead. Internationally, only five of the 11 attempts to land a
spacecraft on Mars have succeeded.

The Phoenix mission is led by Smith, with project management at JPL. The development
partnership is with Lockheed Martin, Denver. International contributions are from the Canadian
Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and
Aarhus, Denmark; the Max Planck Institute, Germany; and the Finnish Meteorological Institute.

For more about the Phoenix mission on the Web, visit: http://www.nasa.gov/phoenix .

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Friday, May 23, 2008

Mars Odyssey THEMIS Images: May 19-23, 2008

MARS ODYSSEY THEMIS IMAGES
May 19-23, 2008

o Jovis Tholus (Released 19 May 2008)

http://themis.asu.edu/zoom-20080519a

o Marte Valles (Released 20 May 2008)

http://themis.asu.edu/zoom-20080520a

o Channels (Released 21 May 2008)

http://themis.asu.edu/zoom-20080521a

o Hebrus Valles (Released 22 May 2008)

http://themis.asu.edu/zoom-20080522a

o Hebrus Valles (Released 23 May 2008)

http://themis.asu.edu/zoom-20080523a


All of the THEMIS images are archived here:

http://themis.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 co.oration 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.

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MRO HiRISE Images - May 21, 2008

MARS RECONNAISSANCE ORBITER HIRISE IMAGES
May 21, 2008

o Ridges in Huo Hsing Vallis

http://hirise.lpl.arizona.edu/PSP_008189_2080

o Young Impact Crater in Isidis

http://hirise.lpl.arizona.edu/PSP_008017_2020

o Channel into Jezero Crater Delta

http://hirise.lpl.arizona.edu/PSP_007925_1990

o Gullies of Crater Wall in Terra Sirenum

http://hirise.lpl.arizona.edu/PSP_006760_1370

All of the HiRISE images are archived here:

http://hirise.lpl.arizona.edu/

Information about the Mars Reconnaissance Orbiter is online at

http://www.nasa.gov/mro. The mission is managed by NASA's Jet Propulsion
Laboratory, a division of the California Institute of Technology, for the NASA
Science Mission Directorate, Washington, D.C. Lockheed Martin Space Systems,
of Denver, is the prime contractor and built the spacecraft. HiRISE is operated by t
he University of Arizona. Ball Aerospace and Technologies Corp., of Boulder, Colo.,
built the HiRISE instrument.

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Thursday, May 22, 2008

Phoenix Spacecraft on Course for May 25 Mars Landing

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Guy Webster 818-354-6278/5011
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

STATUS REPORT: 2008-079 May 22, 2008

Phoenix Spacecraft on Course for May 25 Mars Landing

PASADENA, Calif. -- With three days and 3 million miles left to fly before arriving at
Mars, NASA's Phoenix spacecraft is on track for its destination in the Martian arctic.

"The latest calculation from our navigation team shows the center of the area where we're
currently headed lies less than eight miles from the center of our target area," said Barry
Goldstein, Phoenix project manager at NASA's Jet Propulsion Laboratory, Pasadena, Calif.
"We may decide on Saturday that we don't need to use our final opportunity for fine tuning
the trajectory Phoenix is on. Either way, we will continue to monitor the trajectory
throughout Saturday night, on the off chance we need to execute our contingency
maneuver eight hours before entry."

The spacecraft is in fine health.

"All systems are nominal and stable," said Ed Sedivy, Phoenix spacecraft program
manager for Lockheed Martin Space Systems, Denver, which built the spacecraft. "We
have plenty of propellant, the temperatures look good and the batteries are fully charged."

The spacecraft is closing in on the scariest seven minutes of the mission.

On Sunday, shortly after the annual 500-mile race at the Indianapolis Motor Speedway,
Phoenix will be approaching Mars at about 12,750 miles per hour, a speed that could cover
500 miles in 2 minutes and 22 seconds. After it enters the top of the Martian atmosphere at
that velocity, it must use superheated friction with the atmosphere, a strong parachute and a
set of pulsing retrorockets to achieve a safe, three-legged standstill touchdown on the
surface in just seven minutes.

The earliest possible time when mission controllers could get confirmation from Phoenix
indicating it has survived landing will be at 4:53 p.m. Pacific Time on Sunday (7:53 p.m.
Eastern Time). Of 11 previous attempts that various nations have made to land spacecraft
on Mars, only five have succeeded.

Phoenix will land farther north on Mars than any previous mission, at a site expected to
have ice-rich permafrost beneath the surface, but within reach of the lander's robotic arm.

"Last instructions were given to the science team at our final meeting at the University of
Arizona Tuesday," said Phoenix Principal Investigator Peter Smith of the University of
Arizona, Tucson. "This week, we are conducting our dress rehearsal before opening night
on Sunday." The science team is slowly adjusting to working on Mars time, in which each
day lasts 24.66 hours, in preparation for a demanding mission.

Smith said, "We are ready to robotically operate our science lab in the Martian arctic and
dig through the layers of history to the ice-rich soil below."

Phoenix is equipped to study the history of the water now frozen into the site's permafrost,
to check for carbon-containing chemicals that are essential ingredients for life, and to
monitor polar-region weather on Mars from a surface perspective for the first time.

The Phoenix mission is led by Smith at the University of Arizona with project
management at JPL and development partnership at Lockheed Martin. International
contributions come from the Canadian Space Agency; the University of Neuchatel,
Switzerland; the universities of Copenhagen and Aarhus, Denmark; Max Planck Institute,
Germany; and the Finnish Meteorological Institute. For more about Phoenix, visit:

http://www.nasa.gov/phoenix and http://phoenix.lpl.arizona.edu .

- end -


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Tuesday, May 20, 2008

Mars Odyssey THEMIS Images: May 12-16, 2008

MARS ODYSSEY THEMIS IMAGES
May 12-16, 2008

o Storm Clouds (Released 12 May 2008)

http://themis.asu.edu/zoom-20080512a

o Landslide (Released 13 May 2008)

http://themis.asu.edu/zoom-20080513a

o Texture (Released 14 May 2008)

http://themis.asu.edu/zoom-20080514a

o Windstreaks (Released 15 May 2008)

http://themis.asu.edu/zoom-20080515a

o Wind Action (Released 16 May 2008)

http://themis.asu.edu/zoom-20080516a


All of the THEMIS images are archived here:

http://themis.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 co.oration 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.

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MRO HiRISE Images - May 14, 2008

MARS RECONNAISSANCE ORBITER HIRISE IMAGES
May 14, 2008

o Wrinkle Ridge in Hesperia Planum

http://hirise.lpl.arizona.edu/PSP_008082_1560

o Light-Toned Rocks Exposed inside Crater

http://hirise.lpl.arizona.edu/PSP_008075_1590

o Meridiani Region Layers and Phyllosilicates

http://hirise.lpl.arizona.edu/PSP_008060_1770

o Catastrophic Flood Channel of Ares Valles

http://hirise.lpl.arizona.edu/PSP_007810_1885

All of the HiRISE images are archived here:

http://hirise.lpl.arizona.edu/

Information about the Mars Reconnaissance Orbiter is online at

http://www.nasa.gov/mro. The mission is managed by NASA's Jet Propulsion
Laboratory, a division of the California Institute of Technology, for the NASA
Science Mission Directorate, Washington, D.C. Lockheed Martin Space Systems,
of Denver, is the prime contractor and built the spacecraft. HiRISE is operated by t
he University of Arizona. Ball Aerospace and Technologies Corp., of Boulder, Colo.,
built the HiRISE instrument.

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Joint NASA-French Satellite to Track Trends in Sea Level, Climate

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Alan Buis 818-354-0474
Jet Propulsion Laboratory, Pasadena, Calif.
Alan.buis@jpl.nasa.gov

Steve Cole 202-358-0918
NASA Headquarters, Washington
Stephen.e.cole@nasa.gov

NEWS RELEASE: 2008-078 May 20, 2008

Joint NASA-French Satellite to Track Trends in Sea Level, Climate

PASADENA, Calif. – A satellite that will help scientists better monitor and understand rises in
global sea level, study the world's ocean circulation and its links to Earth's climate, and improve
weather and climate forecasts is undergoing final preparations for a June 15 launch from
California's Vandenberg Air Force Base.

The Ocean Surface Topography Mission (OSTM)/Jason 2 is a partnership of NASA, the National
Oceanic and Atmospheric Administration (NOAA), the French Space Agency Centre National
d'Etudes Spatiales (CNES) and the European Organisation for the Exploitation of Meteorological
Satellites (EUMETSAT). The mission will extend into the next decade the continuous record of
sea-surface height measurements started in 1992 by the NASA-French Space Agency's
TOPEX/Poseidon mission and extended by the NASA-French Space Agency Jason 1 mission in
2001.

The satellite will continue monitoring trends in sea-level rise, one of the most important
consequences and indicators of global climate change. Measurements from TOPEX/Poseidon and
Jason 1 have shown that mean sea level has risen by about three millimeters (0.12 inches) a year
since 1993, twice the rate estimated from tide gauges in the past century. But 15 years of data are
not sufficient to determine long-term trends.

"OSTM/Jason 2 will help create the first multi-decadal global record for understanding the vital
roles of the ocean in climate change," said OSTM/Jason 2 project scientist Lee-Lueng Fu of
NASA's Jet Propulsion Laboratory in Pasadena, Calif. "Data from the new mission will allow us
to continue monitoring global sea-level change, a field of study where current predictive models
have a large degree of uncertainty."

Developed and proven through the joint efforts of NASA and the French Space Agency, high-
precision ocean altimetry measures the height of the sea surface relative to Earth's center to
within about 3.3 centimeters (1.3 inches). These measurements, also known as ocean surface
topography, provide information on the speed and direction of ocean currents. Because sea
surface height is strongly influenced by the amount of heat in the ocean, it also is an indicator of
ocean heat storage in most places. Combining ocean current and heat storage data is key to
understanding global climate variations.

OSTM/Jason 2 marks the transition of high-precision altimetry data collection to the world's
weather and climate forecasting agencies. Scientists soon will be able to forecast how ocean
circulation will change from one season to the next and how that circulation is linked to climate
change and weather patterns.

"What began as an investment by NASA and CNES in research tools for studying the ocean has
matured into a proven technique that will now be routinely used by the world's weather and
climate agencies to make better forecasts," said Michael Freilich, director of the Earth Science
Division in NASA's Science Mission Directorate in Washington. "People in coastal areas will
benefit from improved near-real-time data on ocean conditions, while people everywhere will
benefit from better seasonal predictions resulting from the increased understanding of Earth
system processes enabled by these measurements."

OSTM/Jason 2 will ride to space aboard a NASA-provided United Launch Alliance Delta II
rocket, entering orbit about 10 to 15 kilometers (six to nine miles) below the 1,336-kilometer-
high (830-mile-high) orbit of Jason 1. OSTM/Jason 2 will use its thrusters to raise itself into the
same orbital altitude as Jason 1 and move in close behind its predecessor.

The two spacecraft will fly in formation, making nearly simultaneous measurements. For six to
nine months after launch, scientists will verify the instruments are calibrated precisely.
OSTM/Jason 2 then will continue Jason 1's former flight path, and Jason 1 will move into a
parallel ground track midway between two of the OSTM/Jason 2 ground tracks. This tandem
mission will double the amount of data collected, further improving tide models in coastal and
shallow seas and helping researchers better understand ocean currents and eddies. OSTM/Jason
2's mission is designed to last at least three years.

The OSTM/Jason 2 spacecraft, provided by the French Space Agency, carries five primary
instruments similar to those on Jason 1. Its main instrument is the Poseidon 3 altimeter, also
provided by the French Space Agency. NASA's Advanced Microwave Radiometer measures
atmospheric water vapor, which can distort the altimeter measurements. Three location systems
combine to precisely measure the satellite's position in orbit: NASA's Laser Retroreflector Array
and Global Positioning System Payload, and the French Space Agency's Doppler Orbitography
and Radio-positioning Integrated by Satellite instrument. Instrument improvements since Jason 1
will allow scientists to monitor ocean coastal regions with increased accuracy, nearly 50 percent
closer than in the past. Three experimental instruments round out the payload: the French Space
Agency's Environment Characterization and Modelisation-2 and Time Transfer by Laser Link,
and Japan's Light Particle Telescope.

JPL manages the mission for NASA's Science Mission Directorate. After on-orbit spacecraft
commissioning, CNES will hand over mission operations and control to NOAA. NOAA and
EUMETSAT will generate, archive and distribute data products.

For more on OSTM/Jason 2 on the Web, visit: http://www.nasa.gov/ostm .

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

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Thursday, May 15, 2008

NASA Briefings and TV Coverage Schedule for Phoenix Mars Landing

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Guy Webster/Jane Platt 818-354-5011
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov/jane.platt@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu

2008-077 May 15, 2008

NASA Briefings and TV Coverage Schedule for Phoenix Mars Landing

PASADENA, Calif. -- NASA news briefings, live commentary and updates before and after the
scheduled Sunday, May 25 arrival of the agency's Phoenix Mars Lander will be available on NASA
Television and on the Web.

Entry, descent and landing begins at 4:46 p.m. PDT on May 25, when the flight team listens for
radio signals indicating that Phoenix has entered the top of the Martian atmosphere. The spacecraft
must perform a series of challenging transformations and activities during the seven minutes after it
enters the atmosphere to slow it from 12,000 mph to 5 mph and a soft touchdown. The Phoenix team
will be watching for radio signals confirming the landing at 4:53 p.m. More than half of previous
international attempts to land on Mars have been unsuccessful. For a detailed schedule and landing
timeline, visit:

http://www.nasa.gov/phoenix

The deadline for U.S. journalists to request media credentials to cover the Phoenix mission from
NASA's Jet Propulsion Laboratory in Pasadena, Calif., is Tuesday, May 20. Foreign journalists
requesting credentials must apply by Friday, May 16. Requests for media credentials must be made
online at:

https://eis.jpl.nasa.gov/media/index.html

Media wishing to cover the mission from the University of Arizona in Tucson, must apply online at:

http://uanews.org/marsmedia

Briefings on mission goals, challenges, status and final trajectory adjustments will originate from
JPL on Thursday, May 22, at 11:30 a.m. and on Saturday and Sunday, May 25-26, at noon.

On landing day, May 25, live landing commentary will air on NASA TV. A telecast of mission
control -- without roll-in videos and interviews -- will run on NASA TV's Media Channel beginning
at 3 p.m. Another telecast with commentary, interviews and videos will begin at 3:30 p.m. on NASA
TV's Public Channel. For more information on NASA TV and this coverage schedule, visit:

http://www.nasa.gov/multimedia/nasatv/MM_NTV_Breaking.html

Both telecasts will continue through landing and will resume at 6:30 p.m. during the period after
landing when engineers anticipate the receipt of data and possible images confirming that Phoenix
has opened its solar panels successfully.

A news briefing at JPL will be held Sunday, May 25 at 9 p.m., following landing and the first
possible downlink of images. Briefing updates at JPL also are scheduled on Monday, May 26 at 11
a.m. and on Tuesday, May 27 at 11 a.m.

Daily news briefings will continue at 11 a.m. for several days following a successful landing.
Mission control and the site for news briefings will then shift to the University of Arizona in Tucson
after a determination that the spacecraft is in a safe condition for conducting science operations. The
earliest possibility for moving the host site for mission news briefings to the University of Arizona's
Space Operations Center is Wednesday, May 28. Mission briefings from Pasadena and Tucson will
be carried on NASA TV unless preempted by other NASA events.

For NASA TV streaming video, schedules, and downlink information, visit:

http://www.nasa.gov/ntv

-end-


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NASA Satellite Finds Interior of Mars is Colder

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011

http://www.jpl.nasa.gov


Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov

Dwayne Brown
NASA Headquarters, Washington
Dwayne.c.brown@nasa.gov

NEWS RELEASE: 2008-076 May 15, 2008

NASA Satellite Finds Interior of Mars is Colder

New observations from NASA's Mars Reconnaissance Orbiter indicate that the crust and upper
mantle of Mars are stiffer and colder than previously thought.

The findings suggest any liquid water that might exist below the planet's surface, and any
possible organisms living in that water, would be located deeper than scientists had suspected.

"We found that the rocky surface of Mars is not bending under the load of the north polar ice
cap," said Roger Phillips of the Southwest Research Institute in Boulder, Colo. Phillips is the
lead author of a new report appearing in this week's online version of Science. "This implies that
the planet's interior is more rigid, and thus colder, than we thought before."

The discovery was made using the Shallow Radar instrument on the spacecraft, which has
provided the most detailed pictures to date of the interior layers of ice, sand and dust that make
up the north polar cap on Mars. The radar images reveal long, continuous layers stretching up to
600 miles (1,000 kilometers), or about one-fifth the length of the United States.

"In our first glimpses inside the polar ice using the radar on Mars Reconnaissance Orbiter, we
can clearly see stacks of icy material that trace the history of Mars' climate," said Jeffrey Plaut of
NASA's Jet Propulsion Laboratory, Pasadena, Calif. Plaut is a science team member and a co-
author of the paper. "Radar has opened up a new avenue for studying Mars' past."

The radar pictures show a smooth, flat border between the ice cap and the rocky Martian crust.
On Earth, the weight of a similar stack of ice would cause the planet's surface to sag. The fact
that the Martian surface is not bending means that its strong outer shell, or lithosphere -- a
combination of its crust and upper mantle -- must be very thick and cold.

"The lithosphere of a planet is the rigid part. On Earth, the lithosphere is the part that breaks
during an earthquake," said Suzanne Smrekar, deputy project scientist for Mars Reconnaissance
Orbiter at JPL. "The ability of the radar to see through the ice cap and determine that there is no
bending of the lithosphere gives us a good idea of present day temperatures inside Mars for the
first time."

Temperatures in the outer portion of a rocky planet like Mars increase with depth toward the
interior. The thicker the lithosphere, the more gradually the temperatures increase. The discovery
of a thicker Martian lithosphere therefore implies that any liquid water lurking in aquifers below
the surface would have to be deeper than previously calculated, where temperatures are warmer.
Scientists speculate that any life on Mars associated with deep aquifers also would have to be
buried deeper in the interior.

The radar pictures also reveal four zones of finely spaced layers of ice and dust separated by
thick layers of nearly pure ice. Scientists think this pattern of thick, ice-free layers represents
cycles of climate change on Mars on a time scale of roughly one million years. Such climate
changes are caused by variations in the tilt of the planet's rotational axis and in the eccentricity of
its orbit around the sun. The observations support the idea that the north polar ice cap is
geologically active and relatively young, at about 4 million years.

On May 25, NASA's Phoenix Mars Lander is scheduled to touch down not far from the north
polar ice cap. It will further investigate the history of water on Mars, and is expected to get the
first up-close look at ice on the Red Planet.

The Shallow Radar instrument was provided by the Italian Space Agency, and its operations are
led by the InfoCom Department, University of Rome "La Sapienza." Thales Alenia Space Italia,
in Rome, is the Italian Space Agency's prime contractor for the radar instrument. Astro
Aerospace of Carpinteria, Calif., a business unit of Los Angeles-based Northrop Grumman
Corp., developed the instrument's antenna as a subcontractor to Thales Alenia Space Italia.

The Mars Reconnaissance Orbiter mission is managed by JPL for NASA's Science Mission
Directorate in Washington. Lockheed Martin Space Systems in Denver was the prime contractor
for the orbiter and supports its operations.

For more detailed information about the Mars Reconnaissance Orbiter, visit

http://www.nasa.gov/mro.

For more information about the Mars Phoenix Lander, visit

http://www.nasa.gov/phoenix .

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Wednesday, May 14, 2008

Phoenix Mars Landing Preview Webcast for Schools

Phoenix Mars Landing Preview Webcast for Schools

Tune into the live webcast on Thursday, May 22, 2008, to learn about NASA's Phoenix spacecraft and its upcoming mission on Mars.


On Sunday evening, May 25, 2008, the NASA Phoenix spacecraft will arrive at Mars. Phoenix will be the first vehicle intended to land on the surface of Red Planet since the Mars Exploration Rovers "Spirit" and "Opportunity" landed in January 2004.

Phoenix is a three-legged lander that will perform its "entry, descent and landing" sequence and, if successful, will commence a three-month surface science mission. Phoenix will dig down to an ice-rich layer that scientists calculate lies within inches of the surface. The lander will check samples of soil and ice for evidence about whether the site was ever hospitable to life.

NASA's Jet Propulsion Laboratory in California will be conducting a live webcast for schools on Thursday, May 22, at 9:00 a.m. PDT (12:00 p.m. EDT). This webcast will preview the events of the entry, descent and landing, the path to Mars so far, and the science mission.

Appropriate for 4th- through 12th-grade classrooms, the program will feature information and video clips for 30 minutes. Four selected schools connected through the NASA Digital Learning Network will engage in Q&A with JPL staff for an additional 20 minutes.

For information on how to view the webcast live, visit http://dln.nasa.gov/dln/content/webcast/.

To learn more about the Phoenix mission, visit http://mars.jpl.nasa.gov/missions/present/phoenix.html.




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Tuesday, May 13, 2008

New Software Brings the Universe to Your Computer

Feature May 13, 2008

New Software Brings the Universe to Your Computer

The incredible images from NASA's "Great Observatories" and many other NASA space-
and ground-based telescopes are now available to the public in an educational and
innovative manner through the release of the free WorldWide Telescope software from
Microsoft.

Views of the cosmos from such observatories as NASA's Hubble Space Telescope,
Spitzer Space Telescope, and Chandra X-ray Observatory can all be accessed through the
same intuitive interface of exploring the night sky. Several all-sky surveys are also
available through the WorldWide Telescope, including the Two Micron All-Sky Survey
and the Infrared Astronomical Satellite survey. The rich multimedia software enables
browsing through the visible, infrared, x-ray and other views of the universe, allowing for
direct comparison of multi-wavelength observations that reveal surprising contrasts.

Other innovative features include guided tours created by scientists and educators. These
tours guide users through various aspects of astronomy with narration, music, text and
graphics. Members of the public, including children, will also be able to make their own
tours to share with others.

The Two Micron All-Sky Survey is a collaborative effort between the University of
Massachusetts, Amherst, and the Infrared Processing and Analysis Center in Pasadena,
Calif., operated by NASA's Jet Propulsion Laboratory and the California Institute of
Technology, both in Pasadena.

The Infrared Astronomical Satellite is a joint project between NASA, the Netherlands
and the United Kingdom. Its data are archived at the Infrared Processing and Analysis
Center.

JPL manages the Spitzer Space Telescope mission for NASA's Science Mission
Directorate, Washington. Science operations are conducted at the Spitzer Science Center
at Caltech, which manages JPL for NASA.

The WorldWide Telescope is available as of May 13, 2008, at

www.worldwidetelescope.org .






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NASA Phoenix Mission Ready for Mars Landing

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu

NEWS RELEASE: 2008-074 May 13, 2008

NASA Phoenix Mission Ready for Mars Landing

WASHINGTON -- NASA's Phoenix Mars Lander is preparing to end its long journey and begin a
three-month mission to taste and sniff fistfuls of Martian soil and buried ice. The lander is scheduled
to touch down on the Red Planet May 25.

Phoenix will enter the top of the Martian atmosphere at almost 21,000 kilometers per hour (almost
13,000 mph). In seven minutes, the spacecraft must complete a challenging sequence of events to
slow to about 8 kilometers per hour (5 mph) before its three legs reach the ground. Confirmation of
the landing could come as early as 4:53 p.m. PDT (7:53 p.m. EDT).

"This is not a trip to grandma's house. Putting a spacecraft safely on Mars is hard and risky," said Ed
Weiler, associate administrator for NASA's Science Mission Directorate at NASA Headquarters in
Washington. "Internationally, fewer than half the attempts have succeeded."

Rocks large enough to spoil the landing or prevent opening of the solar panels present the biggest
known risk. However, images from the High Resolution Imaging Science Experiment (HiRISE)
camera on NASA's Mars Reconnaissance Orbiter, detailed enough to show individual rocks smaller
than the lander, have helped lessen that risk.

"We have blanketed nearly the entire landing area with HiRISE images," said Ray Arvidson of
Washington University in St. Louis, chairman of the Phoenix landing-site working group.
"This is one of the least rocky areas on all of Mars and we are confident that rocks will not
detrimentally impact the ability of Phoenix to land safely."

Phoenix uses hardware from a spacecraft built for a 2001 launch that was canceled in response to the
loss of a similar Mars spacecraft during a 1999 landing attempt. Researchers who proposed the
Phoenix mission in 2002 saw the unused spacecraft as a resource for pursuing a new science
opportunity.

Earlier in 2002, NASA's Mars Odyssey orbiter discovered that plentiful water ice lies just beneath
the surface throughout much of high-latitude Mars. NASA chose the Phoenix proposal over 24 other
proposals to become the first endeavor in the Mars Scout program of competitively selected
missions. "Phoenix will land farther north on Mars than any previous mission," said Phoenix Project
Manager Barry Goldstein of NASA's Jet Propulsion Laboratory, Pasadena, Calif.

"The Phoenix mission not only studies the northern permafrost region, but takes the next step in
Mars exploration by determining whether this region, which may encompass as much as 25 percent
of the Martian surface, is habitable," said Peter Smith, Phoenix principal investigator at the
University of Arizona, Tucson.

The solar-powered robotic lander will manipulate a 2.35 meter arm (7.7 foot) to scoop up samples of
underground ice and soil lying above the ice. Onboard laboratory instruments will analyze the
samples. Cameras and a Canadian-supplied weather station will supply other information about the
site's environment.

One research goal is to assess whether conditions at the site ever have been favorable for microbial
life. The composition and texture of soil above the ice could give clues to whether the ice ever melts
in response to long-term climate cycles. Another important question is whether the scooped-up
samples contain carbon-based chemicals that are potential building blocks and food for life.

The Phoenix mission is led by Smith, with project management at JPL. The development partnership
is with Lockheed Martin, Denver. International contributions are from the Canadian Space Agency;
the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus, Denmark; the
Max Planck Institute, Germany; and the Finnish Meteorological Institute.

For more about the Phoenix mission on the Web, visit:

http://www.nasa.gov/phoenix

-end-

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Friday, May 9, 2008

Mars Odyssey THEMIS Images: May 5-9, 2008

MARS ODYSSEY THEMIS IMAGES
May 5-9, 2008

o Herschel Dunes (Released 05 May 2008)

http://themis.asu.edu/zoom-20080505a

o Dunes (Released 06 May 2008)

http://themis.asu.edu/zoom-20080506a

o Dunes (Released 07 May 2008)

http://themis.asu.edu/zoom-20080507a

o Landslides (Released 08 May 2008)

http://themis.asu.edu/zoom-20080508a

o Landslide (Released 09 May 2008)

http://themis.asu.edu/zoom-20080509a

All of the THEMIS images are archived here:

http://themis.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 co.oration 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.

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