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Friday, March 28, 2008

Mars Odyssey THEMIS Images: March 24-28, 2008

MARS ODYSSEY THEMIS IMAGES
March 24-28, 2008

o Hellas Dunes (Released 24 March 2008)

http://themis.asu.edu/zoom-20080324a

o Lava Channels (Released 25 March 2008)

http://themis.asu.edu/zoom-20080325a

o Orthogonal Ridges (Released 26 March 2008)

http://themis.asu.edu/zoom-20080326a

o Dunes (Released 27 March 2008)

http://themis.asu.edu/zoom-20080327a

o Hellas Basin (Released 28 March 2008)

http://themis.asu.edu/zoom-20080328a


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.

To remove yourself from all mailings from NASA Jet Propulsion Laboratory, please go to http://www.kintera.org/TR.asp?a=kmKXJfM0IhJ2JuL&s=ddLOJMPlH9KALLOrGnG&m=goKNKXNuH8KSH

MRO HiRISE Images -March 26, 2008

MARS RECONNAISSANCE ORBITER HIRISE IMAGES
March 26, 2008

o North Polar Layered Deposits, Covered by Seasonal Frost

http://hirise.lpl.arizona.edu/PSP_007493_2650

o Large Polygons in Deuteronilus Mensae

http://hirise.lpl.arizona.edu/PSP_007492_2265

o Northern Hemisphere Ice Cap

http://hirise.lpl.arizona.edu/PSP_007392_2650

o Slab of Layered Material in Aureum Chaos

http://hirise.lpl.arizona.edu/PSP_007006_1765

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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Wednesday, March 26, 2008

Feature: A Perspective on Life on Enceladus - A World of Possibilities

Feature March 26, 2008

A Perspective on Life on Enceladus: A World of Possibilities

Could microbial life exist inside Enceladus, where no sunlight reaches, photosynthesis is
impossible and no oxygen is available? To answer that question, we need look no farther
than our own planet to find examples of the types of exotic ecosystems that could make
life possible on Saturn's geyser moon. The answer appears to be, yes, it could be
possible. It is this tantalizing potential that brings us back to Enceladus for further study.

In recent years, life forms have been found on Earth that thrive in places where the sun
doesn't shine and oxygen is not present because no photosynthesis takes place. Microbes
have been discovered that survive on the energy from the chemical interaction between
different kinds of minerals, and others that live off the energy from the radioactive decay
in rocks. The ecosystems are completely independent of oxygen or organic material
produced by photosynthesis at Earth's surface. These extraordinary microbial ecosystems
are models for life that might be present inside Enceladus today.

There are three such ecosystems found on Earth that would conceivably be a basis for life
on Enceladus. Two are based on methanogens, which belong to an ancient group related
to bacteria, called the archaea -- the rugged survivalists of bacteria that thrive in harsh
environments without oxygen. Deep volcanic rocks along the Columbia River and in
Idaho Falls host two of these ecosystems, which pull their energy from the chemical
interaction of different rocks. The third ecosystem is powered by the energy produced in
the radioactive decay in rocks, and was found deep below the surface in a mine in South
Africa.

So the evidence points to the feasibility of life in Enceladus. But how would it get its
start? A major problem in answering that question is that we don't know how life
originated on Earth, nor have we been able to reproduce Earth's first spark of life in the
laboratory. But here's the good news: there are a lot of theories for how life originated
on Earth. Now the question is -- do they apply to Enceladus?

Two of the theories for the origin of life on Earth do seem to apply to Enceladus--the
"primordial soup" theory and the deep sea vent theory.

The Primordial Soup Theory
The theory that the origin of life occurred in a soup of organic material that came together
from non-biological sources traces back to Charles Darwin, and was demonstrated in a
famous experiment in 1953 when the chemists Stanley L. Miller and Harold C. Urey
cooked up a primordial soup of chemicals thought to have been present on early Earth
before life began. A spark, simulating lightning, was passed through this highly reduced
mixture of methane, ammonia, water vapor and hydrogen. Within two weeks, a few
amino acids, some of the building blocks of life, had formed in the soup. While Miller
and Urey did not actually create life, they demonstrated that very complex molecules —
amino-acids — could emerge spontaneously from simpler chemicals.

On Earth, it's possible that the organic ingredients of the soup were produced from
existing materials on the early Earth. Another theory is that the right soup mix
ingredients arrived as incoming comet material and interplanetary dust.

Organic chemicals were part of the raw material from which Enceladus and Saturn's
other moons formed. The origin of Enceladus' heat is less clear, but there are several
possibilities that could have given Enceladus a layer of liquid water that persists today.
Early on, it could have been heated by decay of short-lived radioactivity in rocks, with
the heating prolonged by tidal influences. Or perhaps an earlier oblong orbit could have
brought more tidal heating than exists there today. A past tidal relationship with another
moon could have caused the heat. Another theory says the heat could have been produced
from a process called serpentization, where chemical binding of water and silicate rock
could occur at the upper layer of the moon's core. This increases the volume of the rock
and creates energy in the form of heat.

Any of these heating mechanisms might have created a liquid subsurface aquifer solution
rich in organics, allowing Enceladus to serve up a suitable prebiotic soup.

The Deep Sea Vent Theory
The deep sea vent theory for the origin of life on Earth might apply to Enceladus as well.
In this scenario, life on Earth began at the interface where chemically rich fluids, heated
by tidal or other mechanisms, emerge from below the sea floor. Chemical energy is
derived from the reduced gases, such as hydrogen-sulfide and hydrogen coming out from
the vent in contact with a suitable oxidant, such as carbon dioxide. Hot spots on an
Enceladus sea floor could be locales for this type of process.

We don't know how long it takes for life to start when the ingredients are there and the
environment is suitable, but it appears to have happened quickly on Earth. So maybe it
was possible that on Enceladus, life started in a "warm little pond" below the icy surface
occurring over the last few tens of millions of years.

For life to persist once it has been established requires an environment of liquid water,
the essential elements and nutrients, and an energy source. At Enceladus, we have
evidence for liquid water, but we don't know its origin. We have observed simple organic
chemicals there, and the March 12 close flyby indicates there are some complex organic
chemicals, as well. An energy source of some sort is producing geysers. As Cassini's
exploration continues, we're seeking to bring together more pieces of this intriguing
puzzle.

The first step toward answering the question of whether life exists inside the subsurface
aquifer of Enceladus is to analyze the organic compounds in the plume. Cassini's March
12 passage through the plume provided some measurements that help us move toward an
answer, and preliminary plans call for Cassini to fly through the plume again
for more measurements in the future. Ultimately, another mission in the future could
conceivably land near the plume or even return plume material to Earth for laboratory
analysis.

Chris McKay of NASA's Ames Research Center is an astrobiologist involved in the
search for environments on other worlds where life may have evolved.
Dennis Matson is the project scientist of the Cassini Mission to Saturn.


By Chris McKay and Dennis Matson


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Cassini Tastes Organic Material at Saturn's Geyser Moon

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

Carolina Martinez 818-354-9382
Jet Propulsion Laboratory, Pasadena, Calif.
carolina.martinez@jpl.nasa.gov

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

NEWS RELEASE: 2008-050 March 26, 2008

Cassini Tastes Organic Material at Saturn's Geyser Moon

PASADENA, Calif. -- NASA's Cassini spacecraft tasted and sampled a surprising organic brew
erupting in geyser-like fashion from Saturn's moon Enceladus during a close flyby on March 12.
Scientists are amazed that this tiny moon is so active, "hot" and brimming with water vapor and
organic chemicals.

New heat maps of the surface show higher temperatures than previously known in the south polar
region, with hot tracks running the length of giant fissures. Additionally, scientists say the organics
"taste and smell" like some of those found in a comet. The jets themselves harmlessly peppered
Cassini, exerting measurable torque on the spacecraft, and providing an indirect measure of the
plume density.

"A completely unexpected surprise is that the chemistry of Enceladus, what's coming out from
inside, resembles that of a comet," said Hunter Waite, principal investigator for the Cassini Ion and
Neutral Mass Spectrometer at the Southwest Research Institute in San Antonio. "To have primordial
material coming out from inside a Saturn moon raises many questions on the formation of the Saturn
system."

"Enceladus is by no means a comet. Comets have tails and orbit the sun, and Enceladus' activity is
powered by internal heat while comet activity is powered by sunlight. Enceladus' brew is like
carbonated water with an essence of natural gas," said Waite.

The Ion and Neutral Mass Spectrometer saw a much higher density of volatile gases, water vapor,
carbon dioxide and carbon monoxide, as well as organic materials, some 20 times denser than
expected. This dramatic increase in density was evident as the spacecraft flew over the area of the
plumes.


New high-resolution heat maps of the south pole by Cassini's Composite Infrared Spectrometer show
that the so-called tiger stripes, giant fissures that are the source of the geysers, are warm along
almost their entire lengths, and reveal other warm fissures nearby. These more precise new
measurements reveal temperatures of at least minus 93 degrees Celsius (minus 135 Fahrenheit.) That
is 17 degrees Celsius (63 degrees Fahrenheit) warmer than previously seen and 93 degrees Celsius
(200 degrees Fahrenheit) warmer than other regions of the moon. The warmest regions along the
tiger stripes correspond to two of the jet locations seen in Cassini images.

"These spectacular new data will really help us understand what powers the geysers. The
surprisingly high temperatures make it more likely that there's liquid water not far below the
surface," said John Spencer, Cassini scientist on the Composite Infrared Spectrometer team at the
Southwest Research Institute in Boulder, Colo.

Previous ultraviolet observations showed four jet sources, matching the locations of the plumes seen
in previous images. This indicates that gas in the plume blasts off the surface into space, blending to
form the larger plume.

Images from previous observations show individual jets and mark places from which they emanate.
New images show how hot spot fractures are related to other surface features. In future imaging
observations, scientists hope to see individual plume sources and investigate differences among
fractures.

"Enceladus has got warmth, water and organic chemicals, some of the essential building blocks
needed for life," said Dennis Matson, Cassini project scientist at NASA's Jet Propulsion Laboratory
in Pasadena, Calif. "We have quite a recipe for life on our hands, but we have yet to find the final
ingredient, liquid water, but Enceladus is only whetting our appetites for more."

At closest approach, Cassini was only 30 miles from Enceladus. When it flew through the plumes it
was 120 miles from the moon's surface. Cassini's next flyby of Enceladus is in August.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and
the Italian Space Agency. The mission is managed by JPL for NASA's Science Mission Directorate,
Washington.

For images and more information, visit http://www.nasa.gov/cassini or http://saturn.jpl.nasa.gov/ .

-end-

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Monday, March 24, 2008

Feature: High-Schoolers Go Into Overdrive at FIRST Robotics Competition

Feature

March 24, 2008


High-Schoolers Go Into Overdrive at FIRST Robotics Competition

Fifty-two teams from high schools in Southern California, Arizona and New Hampshire competed
in the Los Angeles FIRST Robotics Competition last Friday and Saturday. Five teams, one
sponsored by JPL and another sponsored by the Dryden Flight Research Center, will go on to the
worldwide competition, to be held April 17-19 in Atlanta.

The teams from Hope Chapel Academy, Hermosa Beach; Delphi Academy, Lake View Terrace;
and Dos Pueblos Engineering Academy, Goleta, won the overall regional competition. The Dryden-
sponsored Lancaster High School, Lancaster, won the Regional Chairman's Award, so it will also
participate in the final competition, as will San Diego's High Tech High School, which received the
Engineering Inspiration Award.

FIRST (For Inspiration and Recognition of Science and Technology) is part of NASA's Robotic
Alliance Project. The students designed, built and tested the robots – which can stand up to six feet
high and weigh up to 120 pounds – with the help of engineers. Thirty engineers at JPL worked with
several of the teams for more than six weeks, and 70 more JPLers volunteered at the event.

In this year's "Overdrive" challenge, robots raced counterclockwise on a track roughly the size of a
tennis court. In each two-minute-and-15 second round, robots scored points by pushing and passing
huge rubber "Trackballs" around the field and over a six-and-a-half foot overpass. Robots had to
operate by themselves for the first 15 seconds of each round, then students were allowed to control
the robots for the remaining two minutes.

2008 Los Angeles Regional FIRST Robotics Awards
* Connotes JPL or other NASA-sponsored team

Regional Winners:
* *"Beach Bots," Hope Chapel Academy, Hermosa Beach
* "Thunderbots," Delphi Academy, Lake View Terrace
* "D'Penguineers," Dos Pueblos High School Engineering Academy, Goleta

Regional Finalists:
* "BCR," Redondo Union High School, Redondo Beach
* "Bagel Bytes," Culver City High School, Culver City
* "RoboWarriors," Bishop Alemany High School, Mission Hills

Regional Chairman's Award: *"Eagle Robotics," Lancaster High School, Lancaster

Engineering Inspiration Award: "The Holy Cows," High Tech High School, San Diego

General Motors Industrial Design Award: *"Beach Bots," Hope Chapel Academy

Motorola Quality Award: "Metalcrafters," Centinela Valley Union High School District, Hawthorne

Johnson & Johnson Gracious Professionalism Award: "Robodox," Granada Hills Charter High
School, Granada Hills

Judges' Awards:
"MorTorq," Beverly Hills High School, Beverly Hills
"The Nerd Herd," California Academy of Mathematics and Science, Carson

Rookie Inspiration Award: *"TNT," John Muir High School, Pasadena

Rookie All-Stars Award: *"LCE," La Canada High School, La Canada

Highest Rookie Seed: "SMERT," Palos Verdes Peninsula High School, Rolling Hills Estates

Underwriters Laboratories Industrial Safety Award: *"Eagle Robotics," Lancaster High School,
Lancaster


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Friday, March 21, 2008

Mars Odyssey THEMIS Images: March 17-21, 2008

MARS ODYSSEY THEMIS IMAGES
March 17-21, 2008

o Russell Crater Dunes (Released 17 March 2008)

http://themis.asu.edu/zoom-20080317a

o Ganges Chasma (Released 18 March 2008)

http://themis.asu.edu/zoom-20080318a

o Small Volcano (Released 19 March 2008)

http://themis.asu.edu/zoom-20080319a

o Windblown Region (Released 20 March 2008)

http://themis.asu.edu/zoom-20080320a

o Cerulli Crater (Released 21 March 2008)

http://themis.asu.edu/zoom-20080321a


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.

To remove yourself from all mailings from NASA Jet Propulsion Laboratory, please go to http://www.kintera.org/TR.asp?a=jwK4JlMXIkJYJmL&s=iiLYI1PFJeIKK0PLIsE&m=hfKNKVMvE9IUG

MRO HiRISE Images -March 19, 2008

MARS RECONNAISSANCE ORBITER HIRISE IMAGES
March 19, 2008

o Yardangs in Tithonium Chasma

http://hirise.lpl.arizona.edu/PSP_007417_1755

o Layered Bedrock with Possible Hydrated Sulfates

http://hirise.lpl.arizona.edu/PSP_007403_1670

o Inverted Fluvial Channels and Craters with Ejecta Rays

http://hirise.lpl.arizona.edu/PSP_007394_1750

o Layered Bedrock in Walls of Ganges Mensa

http://hirise.lpl.arizona.edu/PSP_007376_1725


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.

To remove yourself from all mailings from NASA Jet Propulsion Laboratory, please go to http://www.kintera.org/TR.asp?a=gtIYIcPLJgKRIdI&s=lvL4LaPRLhIQL9NXJvE&m=owJ1LgPXLfK7E

Thursday, March 20, 2008

Cassini Spacecraft Finds Ocean May Exist Beneath Titan's Crust

DC Agle/Carolina Martinez
818-393-9011/818-354-9382
Jet Propulsion Laboratory, Pasadena, Calif.
agle@jpl.nasa.gov/carolina.martinez@jpl.nasa.gov
Dwayne Brown 202-358-2726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

News Release: 2008-048 March 20, 2008

Cassini Spacecraft Finds Ocean May Exist Beneath Titan's Crust

PASADENA, Calif. - NASA's Cassini spacecraft has discovered evidence that points to the
existence of an underground ocean of water and ammonia on Saturn's moon Titan. The findings,
made using radar measurements of Titan's rotation, will appear in the March 21 issue of the
journal Science.

"With its organic dunes, lakes, channels and mountains, Titan has one of the most varied, active
and Earth-like surfaces in the solar system," said Ralph Lorenz, lead author of the paper and
Cassini radar scientist at the Johns Hopkins Applied Physics Laboratory in Laurel, Md., "Now
we see changes in the way Titan rotates, giving us a window into Titan's interior beneath the
surface."

Members of the mission's science team used Cassini's Synthetic Aperture Radar to collect
imaging data during 19 separate passes over Titan between October 2005 and May 2007. The
radar can see through Titan's dense, methane-rich atmospheric haze, detailing never-before-seen
surface features and establishing their locations on the moon's surface.

Using data from the radar's early observations, the scientists and radar engineers established the
locations of 50 unique landmarks on Titan's surface. They then searched for these same lakes,
canyons and mountains in the reams of data returned by Cassini in its later flybys of Titan. They
found prominent surface features had shifted from their expected positions by up to 30
kilometers (19 miles). A systematic displacement of surface features would be difficult to
explain unless the moon's icy crust was decoupled from its core by an internal ocean, making it
easier for the crust to move.

"We believe that about 100 kilometers (62 miles) beneath the ice and organic-rich surface is an
internal ocean of liquid water mixed with ammonia," said Bryan Stiles of NASA's Jet Propulsion
Laboratory in Pasadena, Calif. Stiles is a contributing author to the paper.
The study of Titan is a major goal of the Cassini-Huygens mission because it may preserve, in
deep-freeze, many of the chemical compounds that preceded life on Earth. Titan is the only
moon in the solar system that possesses a dense atmosphere. The moon's atmosphere is 1.5 times
denser than Earth's. Titan is the largest of Saturn's moons, bigger than the planet Mercury.

"The combination of an organic-rich environment and liquid water is very appealing to
astrobiologists," Lorenz said. "Further study of Titan's rotation will let us understand the watery
interior better, and because the spin of the crust and the winds in the atmosphere are linked, we
might see seasonal variation in the spin in the next few years."

Cassini scientists will not have long to wait before another go at Titan. On March 25, just prior to
its closest approach at an altitude of 1,000 kilometers (620 miles), Cassini will employ its Ion
and Neutral Mass Spectrometer to examine Titan's upper atmosphere. Immediately after closest
approach, the spacecraft's Visual and Infrared Mapping Spectrometer will capture high-
resolution images of Titan's southeast quadrant.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency
and the Italian Space Agency. The mission is managed by JPL, a division of the California
Institute of Technology in Pasadena. The Cassini orbiter also was designed, developed and
assembled at JPL. The radar instrument was built by JPL and the Italian Space Agency, working
with team members from the United States and several European countries.

For information about Cassini visit: http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov .

-end-


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NASA Mission Finds New Clues To Guide Search For Life On Mars

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

Robert Burnham 480-458-8207
Arizona State University, Tempe
robert.burnham@asu.edu

Tara Hicks-Johnson (808) 956-3151
University of Hawaii, Manoa
hickst@hawaii.edu

News Release: 2008-047 March 20, 2008

NASA Mission Finds New Clues to Guide Search for Life on Mars

PASADENA, Calif. - NASA's Mars Odyssey orbiter has found evidence of salt deposits.
These deposits point to places where water once was abundant and where evidence might
exist of possible Martian life from the Red Planet's past.

A team led by Mikki Osterloo of the University of Hawaii, Honolulu, found
approximately 200 places on southern Mars that show spectral characteristics consistent
with chloride minerals. Chloride is part of many types of salt, such as sodium chloride or
table salt. The sites range from about a square kilometer (0.6 square mile) to 25 times that
size.

"They could come from groundwater reaching the surface in low spots," Osterloo said.
"The water would evaporate and leave mineral deposits, which build up over years. The
sites are disconnected, so they are unlikely to be the remnants of a global ocean."

Scientists used Odyssey's Thermal Emission Imaging System, a camera designed and
operated by Arizona State University, Tempe, to take images in a range of visible light
and infrared wavelengths.
Thermal infrared wavelengths are useful for identifying different mineral and rock types
on the Martian surface. Osterloo found the sites by looking through thousands of images
processed to reveal, in false colors, compositional differences on the Martian surface.

Plotted on a Mars map, the chloride sites appear only in the southern highlands, the most
ancient rocks on Mars. Osterloo and seven co-authors report the findings in this week's
issue of the journal Science.

"Many of the deposits lie in basins with channels leading into them," said Philip
Christensen, co-author and principal investigator for the camera at Arizona State
University. "This is the kind of feature, like salt-pan deposits on Earth, that's consistent
with water flowing in over a long time."

Scientists think the salt deposits formed approximately 3.5 to 3.9 billion years ago.
Several lines of evidence suggest Mars then had intermittent periods with substantially
wetter and warmer conditions than today's dry, frigid climate.

Scientists looking for evidence of past life on Mars have focused mainly on a handful of
places that show evidence of clay or sulfate minerals. Clays indicate weathering by water,
and sulfates may have formed by water evaporation. The new research, however,
suggests an alternative mineral target to explore for biological remains.

"By their nature, salt deposits point to a lot of water, which potentially could remain
standing in pools as it evaporates," said Christensen. "That's crucial. For life, it's all about
a habitat that endures for some time."

Whether life ever has existed on Mars is the biggest scientific question driving Mars
research. On Earth, salt is good at preserving organic material. Bacteria have been
revived in the laboratory after being preserved in salt deposits for millions of years.

"This discovery demonstrates the continuing value of the Odyssey science mission, now
entering its seventh year. The more we look at Mars, the more fascinating a place it
becomes," said Jeffrey Plaut, Odyssey project scientist at NASA's Jet Propulsion
Laboratory, Pasadena, Calif.

"This is a wonderful and scientifically exciting result obtained from a relatively low cost
NASA Mars orbiter mission which still has years of life left," said Alan Stern, associate
administrator for NASA's Science Mission Directorate in Washington. "Hold on to your
hats, more exciting results from Mars are sure to be coming."

JPL, a division of the California Institute of Technology, Pasadena, manages Odyssey for
the NASA Science Mission Directorate. Lockheed Martin Space Systems, Denver, is the
prime contractor for the project and built the spacecraft. Additional information about
Odyssey is at http://www.nasa.gov/mission_pages/odyssey . More information about
the camera and the new findings is at http://themis.asu.edu .

-end-


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Wednesday, March 19, 2008

Astronomers Detect First Organic Molecule on an Exoplanet

.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

Ray Villard 410-338-4514
Space Telescope Science Institute, Baltimore, Md.
410-338-4514
villard@stsci.edu

NEWS RELEASE: 2008-046 March 19, 2008

Astronomers Detect First Organic Molecule on an Exoplanet

A team of astronomers led by Mark Swain of NASA's Jet Propulsion Laboratory, Pasadena,
Calif., has made the first detection ever of an organic molecule in the atmosphere of a Jupiter-
sized planet orbiting another star. The breakthrough, made with NASA's Hubble Space
Telescope, is an important step in eventually identifying signs of life on a planet outside our
solar system.

The molecule found by Hubble is methane, which under the right circumstances can play a key
role in prebiotic chemistry - the chemical reactions considered necessary to form life as we know
it.

This discovery proves that Hubble and upcoming space missions, such as NASA's James Webb
Space Telescope, can detect organic molecules on planets around other stars by using
spectroscopy, which splits light into its components to reveal the "fingerprints" of various
chemicals.

"This is a crucial stepping stone to eventually characterizing prebiotic molecules on planets
where life could exist," said Swain, lead author of a paper appearing in the March 20 issue of
Nature.

The discovery comes after extensive observations made in May 2007 with Hubble's Near
Infrared Camera and Multi-Object Spectrometer. It also confirms the existence of water
molecules in the planet's atmosphere, a discovery made originally by NASA's Spitzer Space
Telescope in 2007. "With this observation there is no question whether there is water or not -
water is present," said Swain.

The planet now known to have methane and water is located 63 light-years away in the
constellation Vulpecula. Called HD 189733b, the planet is so massive and so hot it is considered
an unlikely host for life. HD 189733b, dubbed a "hot Jupiter," is so close to its parent star it takes
just over two days to complete an orbit. These objects are the size of Jupiter but orbit closer to
their stars than the tiny innermost planet Mercury in our solar system. HD 189733b's atmosphere
swelters at 1700 degrees Fahrenheit, about the same temperature as the melting point of silver.

Though the star-hugger planet is too hot for life as we know it, "this observation is proof that
spectroscopy can eventually be done on a cooler and potentially habitable Earth-sized planet
orbiting a dimmer red dwarf-type star," Swain said. The ultimate goal of studies like these is to
identify prebiotic molecules in the atmospheres of planets in the "habitable zones" around other
stars, where temperatures are right for water to remain liquid rather than freeze or evaporate
away.

The observations were made as the planet HD 189733b passed in front of its parent star in what
astronomers call a transit. As the light from the star passed briefly through the atmosphere along
the edge of the planet, the gases in the atmosphere imprinted their unique signatures on the
starlight from the star HD 189733.

The astronomers were surprised to find that the planet has more methane than predicted by
conventional models for "hot Jupiters." "This indicates we don't really understand exoplanet
atmospheres yet," said Swain.

"These measurements are an important step to our ultimate goal of determining the conditions,
such as temperature, pressure, winds, clouds, etc., and the chemistry on planets where life could
exist. Infrared spectroscopy is really the key to these studies because it is best matched to
detecting molecules," said Swain.

More information on the discovery and artist's concepts are online at:
http://hubblesite.org/news/2008/11 . Swain's co-authors on the paper include Gautam Vasisht
of JPL and Giovanna Tinetti of University College, London.

The Hubble Space Telescope is a project of international cooperation between NASA and the
European Space Agency and is managed by NASA's Goddard Space Flight Center in Greenbelt,
Md. The Space Telescope Science Institute conducts Hubble science operations. The institute is
operated for NASA by the Association of Universities for Research in Astronomy, Inc.,
Washington, DC. Scheduled for launch in 2013, the James Webb Space Telescope is an
international collaboration between NASA, ESA, and the Canadian Space Agency (CSA). GSFC
is managing the development effort. The prime contractor is Northrop Grumman Space
Technologies. STScI will operate JWST after launch.

JPL manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate,
Washington. Science operations are conducted at the Spitzer Science Center at the California
Institute of Technology, also in Pasadena. Caltech manages JPL for NASA. Previous Spitzer
discoveries regarding HD 189733b from Swain and others can be read at

http://www.spitzer.caltech.edu/Media/releases/ssc2007-04/release.shtml .

Read a profile about astronomer Mark Swain at

http://www.jpl.nasa.gov/news/features.cfm?feature=1641

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Tuesday, March 18, 2008

Mars Odyssey THEMIS Images: March 10-14, 2008

MARS ODYSSEY THEMIS IMAGES
March 10-14, 2008

o Resistance (Released 10 March 2008)

http://themis.asu.edu/zoom-20080310a

o Herschel Dunes (Released 11 March 2008)

http://themis.asu.edu/zoom-20080311a

o Small Scale Features (Released 12 March 2008)

http://themis.asu.edu/zoom-20080312a

o Kasei Channels (Released 13 March 2008)

http://themis.asu.edu/zoom-20080313a

o Dark Slope Streaks (Released 14 March 2008)

http://themis.asu.edu/zoom-20080314a


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 -March 10, 2008

MARS RECONNAISSANCE ORBITER HIRISE IMAGES
March 10, 2008

o Light-Toned Rock in Southern Highlands

http://hirise.lpl.arizona.edu/PSP_006962_1520

o Complex Dunes in Kaiser Crater

http://hirise.lpl.arizona.edu/PSP_006609_1330

o Caught in Action: Avalanches on North Polar Scarps

http://hirise.lpl.arizona.edu/PSP_007338_2640

o Layered Rocks in Meridiani (PSP_006873_1800)

http://hirise.lpl.arizona.edu/PSP_006873_1800

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, March 13, 2008

Cassini Flies Through Watery Plumes of Saturn Moon

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

Carolina Martinez 818-354-5011
Jet Propulsion Laboratory, Pasadena, Calif.
carolina.martinez@jpl.nasa.gov

Preston Dyches 720-974-5859
Space Science Institute, Boulder, Colo.
media@ciclops.org

NEWS RELEASE: 2008-044 March 13, 2008

Cassini Flies Through Watery Plumes of Saturn Moon

NASA's Cassini spacecraft performed a daring flyby of Saturn's moon Enceladus on
Wed., March 12, flying about 15 kilometers per second (32,000 mph) through icy water
geyser-like jets. The spacecraft snatched up precious samples that might point to a water
ocean or organics inside the little moon.

Scientists believe the geysers could provide evidence that liquid water is trapped under
the icy crust of Enceladus. The geysers emanate from fractures running along the moon's
south pole, spewing out water vapor at approximately 400 meters per second (800 mph).

The new data provide a much more detailed look at the fractures that modify the surface
and will give a significantly improved comparison between the geologic history of the
moon's north pole and south pole.

New images show that compared to much of the southern hemisphere on Enceladus--the
south polar region in particular--the north polar region is much older and pitted with
craters of various sizes. These craters are captured at different stages of disruption and
alteration by tectonic activity, and probably from past heating from below. Many of the
craters seem sliced by small parallel cracks that appear to be ubiquitous throughout the
old cratered terrains on Enceladus.

"These new images are showing us in great detail how the moon's north pole differs from
the south, an important comparison for working out the moon's obviously complex
geological history," said Carolyn Porco, Cassini imaging team leader, Space Science
Institute, Boulder, Colo. "And the success of yesterday's daring and very low-altitude
flyby means this coming summer's very close encounter, when we get exquisitely
detailed images of the surface sources of Enceladus' south polar jets, should be an
exciting 'next big step' in understanding just how the jets are powered."

This week's flyby and another one planned for Oct. 9, 2008, were designed so that
Cassini's particle analyzers could dissect the "body" of the plume for information on the
density, size, composition and speed of the particles. Among other things, scientists will
use the data gathered this week to figure out whether the gases from the plume match the
gases that make up the halo of particles around Enceladus. This may help determine how
the plumes formed.

During Cassini's closest approach, two instruments were collecting data--the Cosmic
Dust Analyzer and the Ion and Neutral Mass Spectrometer. An unexplained software
hiccup with Cassini's Cosmic Dust Analyzer instrument prevented it from collecting any
data during closest approach, although the instrument did get data before and after the
approach. During the flyby, the instrument was switching between two versions of
software programs. The new version was designed to increase the ability to count particle
hits by several hundred hits per second. The other four fields and particles instruments
on the spacecraft, in addition to the ion and neutral mass spectrometer, did capture all of
their data, which will complement the overall composition studies and elucidate the
unique plume environment of Enceladus.

Cassini's instruments discovered evidence for the geyser-like jets on Enceladus in 2005,
finding that the continuous eruptions of ice water create a gigantic halo of ice dust and
gas around Enceladus, which helps supply material to Saturn's E-ring.

This was the first of four Cassini flybys of Enceladus this year. During Wednesday's
flyby, the spacecraft came within 50 kilometers (30 miles) of the surface at closest
approach, 200 kilometers (120 miles) while flying through the plume. Future trips may
bring Cassini even closer to the surface of Enceladus. Cassini will complete its prime
mission, a four-year tour of Saturn, in June. From then on, a proposed extended mission
would include seven more Enceladus flybys. The next Enceladus flyby would take place
in August of this year.

For more images and more information, visit: http://www.nasa.gov/cassini and

http://saturn.jpl.nasa.gov .

The Cassini-Huygens mission is a cooperative project of NASA, the European Space
Agency and the Italian Space Agency. JPL, a division of the California Institute of
Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science
Mission Directorate, Washington. The Cassini orbiter was designed, developed and
assembled at JPL.

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JPL Technologies Chosen for Space Technology Hall of Fame

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

Rhea Borja 818-354-0850
Jet Propulsion Laboratory, Pasadena, Calif.
Rhea.R.Borja@jpl.nasa.gov

Kendra Horn 719-576-8000
Space Foundation, Colorado Springs, Colo.
Kendra@spacefoundation.org

NEWS RELEASE 2008-041 March 13, 2008

JPL Technologies Chosen for Space Technology Hall of Fame

PASADENA, CALIF. -- Two technologies developed by NASA's Jet Propulsion Laboratory
have been selected for the Space Foundation's 2008 Space Technology Hall of Fame. Judges for
the nonprofit foundation chose ArterioVision, a software that helps better diagnose heart disease,
and Petroleum Remediation Product, a powder made of beeswax microcapsules that cleans up oil
spills in an environmentally-friendly way.

ArterioVision is used with a standard ultrasound to precisely measure the thickness of the two
inner layers of the carotid artery, known as the carotid intima media thickness. Doing so allows
doctors to determine the age and health of a patient's arteries and better predict and minimize his
or her risk for heart disease.

JPL, Medical Technologies International, and the University of Southern California's Keck
School of Medicine-Atherosclerosis Research Unit, will be inducted into the 2008 Space
Technology Hall of Fame for ArterioVision. Initially developed at JPL in the 1990s,
ArterioVision is derived from the Video Imaging Communication and Retrieval software used to
process pictures from NASA spacecraft imagery.

Medical Technologies International, of Palm Desert, Calif., licensed the space-imaging software
and USC tested and adapted it for diagnostic medical use. JPL's Innovative Partnership Program
managed this and other industry partnerships that result in commercialization.

The individuals who developed and adapted ArterioVision will also be honored April 10 in
Colorado Springs at the 24th National Space Symposium, an annual gathering of the global
space community.

These individuals are:

- Robert Selzer, Medical Technologies International's chief engineer and the former head of
JPL's Biomedical Image Processing Group

- Gary Thompson, chairman and chief executive officer of Medical Technologies International

- Dr. Howard N. Hodis, Director of the Atherosclerosis Research Unit at USC's Keck School of
Medicine

In addition, the Space Foundation will commend Helenann Kwong-Fu, a JPL mission-assurance
manager for the Phoenix Mars lander and Spitzer Space Telescope flight projects. She helped
develop the technology and standardize protocols for image acquisition.

Petroleum Remediation Product, the second technology that the Space Foundation will honor,
originated at JPL and NASA's Marshall Space Flight Center, in Huntsville, Ala. JPL
demonstrated the feasibility of encapsulating live cells, while technology developed at Marshall
for experiments in orbital production of microspheres gave the basic design of the delivery
system. Industry scientists then worked with researchers at both NASA centers to develop the
technology.

The natural and biodegradable product cleans up oil and other contaminants via thousands of
microcapsules -- tiny balls of beeswax with hollow centers. Water cannot penetrate the
microcapsule's cell, but oil is absorbed into the beeswax spheres. This way, oil is caught before it
settles into soil or water.

Besides honoring the technology itself, the Space Foundation will also induct the company that
makes and distributes it -- Pittsburgh-based Universal Remediation, Inc. The company stepped
up production and expanded availability of the product to such clients as Alcoa and U.S. Steel.

More information on the Space Technology Hall of Fame is at

http://spacetechhalloffame.org/ .

More information on JPL is at http://jpl.nasa.gov . More information on ArterioVision is at

http://i-mti.com/the_technology.htm . More information on Petroleum Remediation Product is at

http://unireminc.com/ .

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Spitzer Finds Organics and Water Where New Planets May Grow

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

Rosemary Sullivant 818-354-2274
Jet Propulsion Laboratory, Pasadena, Calif.
Rosemary.Sullivant@jpl.nasa.gov

NEWS RELEASE: 2008-042 March 13, 2008

Spitzer Finds Organics and Water Where New Planets May Grow

Researchers using NASA's Spitzer Space Telescope have discovered large amounts of
simple organic gases and water vapor in a possible planet-forming region around an
infant star, along with evidence that these molecules were created there. They've also
found water in the same zone around two other young stars.

By pushing the telescope's capabilities to a new level, astronomers now have a better
view of the earliest stages of planetary formation, which may help shed light on the
origins of our own solar system and the potential for life to develop in others.

John Carr of the Naval Research Laboratory, Washington, and Joan Najita of the
National Optical Astronomy Observatory, Tucson, Ariz., developed a new technique
using Spitzer's infrared spectrograph to measure and analyze the chemical composition of
the gases within protoplanetary disks. These are flattened disks of gas and dust that
encircle young stars. Scientists believe they provide the building materials for planets and
moons and eventually, over millions of years, evolve into orbiting planetary systems like
our own.

"Most of the material within the disks is gas," said Carr, "but until now it has been
difficult to study the gas composition in the regions where planets should form. Much
more attention has been given to the solid dust particles, which are easier to observe."

In their project, Carr and Najita took an in-depth look at the gases in the planet-forming
region in the disk around the star AA Tauri. Less than a million years old, AA Tauri is a
typical example of a young star with a protoplanetary disk.

With their new procedures, they were able to detect the minute spectral signatures for
three simple organic molecules--hydrogen cyanide, acetylene and carbon dioxide--plus
water vapor. In addition, they found more of these substances in the disk than are found
in the dense interstellar gas called molecular clouds from which the disk originated.
"Molecular clouds provide the raw material from which the protoplanetary disks are
created," said Carr. "So this is evidence for an active organic chemistry going on within
the disk, forming and enhancing these molecules."

Spitzer's infrared spectrograph detected these same organic gases in a protoplanetary disk
once before. But the observation was dependent on the star's disk being oriented in just
the right way. Now researchers have a new method for studying the primordial mix of
gases in the disks of hundreds of young star systems.

Astronomers will be able to fill an important gap--they know that water and organics are
abundant in the interstellar medium but not what happens to them after they are
incorporated into a disk. "Are these molecules destroyed, preserved or enhanced in the
disk?" said Carr. "Now that we can identify these molecules and inventory them, we will
have a better understanding of the origins and evolution of the basic building blocks of
life--where they come from and how they evolve." Carr and Najita's research results
appear in the March 14 issue of Science.

Taking advantage of Spitzer's spectroscopic capabilities, another group of scientists
looked for water molecules in the disks around young stars and found them--twice. "This
is one of the very few times that water vapor has been directly shown to exist in the inner
part of a protoplanetary disk--the most likely place for terrestrial planets to form," said
Colette Salyk, a graduate student in geological and planetary sciences at the California
Institute of Technology in Pasadena. She is the lead author on a paper about the results in
the March 20 issue of Astrophysical Journal Letters.

Salyk and her colleagues used Spitzer to look at dozens of young stars with
protoplanetary disks and found water in many. They honed in on two stars and followed
up the initial detection of water with complementary high-resolution measurements from
the Keck II Telescope in Hawaii. "While we don't detect nearly as much water as exists in
the oceans on Earth, we see essentially only the disk's surface, so the implication is that
the water is quite abundant," said Geoffrey Blake, professor of cosmochemistry and
planetary sciences at Caltech and one of the paper's co-authors.

"This is a much larger story than just one or two disks," said Blake. "Spitzer can
efficiently measure these water signatures in many objects, so this is just the beginning of
what we will learn."

"With upcoming Spitzer observations and data in hand," Carr added, "we will develop a
good understanding of the distribution and abundance of water and organics in planet-
forming disks."

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 Spitzer Science Center at Caltech, also in Pasadena.
Caltech manages JPL for NASA. For more information about Spitzer, visit

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

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Monday, March 10, 2008

Mars Odyssey THEMIS Images: March 3-7, 2008

MARS ODYSSEY THEMIS IMAGES
March 3-7, 2008

o Crater Dunes (Released 03 March 2008)

http://themis.asu.edu/zoom-20080303a

o Everywhere Dunes (Released 04 March 2008)

http://themis.asu.edu/zoom-20080304a

o Newton Crater (Released 05 March 2008)

http://themis.asu.edu/zoom-20080305a

o Pavonis Mons (Released 06 March 2008)

http://themis.asu.edu/zoom-20080306a

o Channels (Released 07 March 2008)

http://themis.asu.edu/zoom-20080307a


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 -March 3, 2008

MARS RECONNAISSANCE ORBITER HIRISE IMAGES
March 3, 2008

o Colorful Sulfates in Aureum Chaos

http://hirise.lpl.arizona.edu/PSP_007217_1755

o Slope Streaks on the Rim of Henry Crater

http://hirise.lpl.arizona.edu/PSP_006991_1905

o Complex Folds in Hellas Basin

http://hirise.lpl.arizona.edu/PSP_007346_1405

o Clay Minerals in Nili Fossae

http://hirise.lpl.arizona.edu/PSP_007358_2015

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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Cassini Spacecraft to Dive Into Water Plume of Saturn Moon

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

Carolina Martinez 818-354-9382
Jet Propulsion Laboratory, Pasadena, Calif.
carolina.martinez@jpl.nasa.gov

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

NEWS RELEASE: 2008-040 March 10, 2008

Cassini Spacecraft to Dive Into Water Plume of Saturn Moon

PASADENA, Calif. - NASA's Cassini spacecraft will make an unprecedented "in your face" flyby of
Saturn's moon Enceladus on Wed., March 12.

The spacecraft, orchestrating its closest approach to date, will skirt along the edges of huge Old-
Faithful-like geysers erupting from giant fractures on the south pole of Enceladus. Cassini will
sample scientifically valuable water-ice, dust and gas in the plume.

The source of the geysers is of great interest to scientists who think liquid water, perhaps even an
ocean, may exist in the area. While flying through the edge of the plumes, Cassini will be
approximately 200 kilometers (120 miles) from the surface. At closest approach to Enceladus,
Cassini will be only 50 kilometers (30 miles) from the moon.

"This daring flyby requires exquisite technical finesse, but it has the potential to revolutionize our
knowledge of the geysers of Enceladus. The Cassini mission team is eager to see the scientific
results, and so am I," said Alan Stern, associate administrator of NASA's Science Mission
Directorate, Washington.

Scientists and mission personnel studying the anatomy of the plumes have found that flying at these
close distances poses little threat to Cassini because, despite the high speed of Cassini, the plume
particles are small. The spacecraft routinely crosses regions made up of dust-size particles in its orbit
around Saturn.

Cassini's cameras will take a back seat on this flyby as the main focus turns to the spacecraft's
particle analyzers that will study the composition of the plumes. The cameras will image Enceladus
on the way in and out, between the observations of the particle analyzers.

Images will reveal northern regions of the moon previously not captured by Cassini. The analyzers
will "sniff and taste" the plume. Information on the density, size, composition and speed of the gas
and the particles will be collected.


"There are two types of particles coming from Enceladus, one pure water-ice, the other water-ice
mixed with other stuff," said Sascha Kempf, deputy principal investigator for Cassini's Cosmic Dust
Analyzer at the Max Planck Institute for Nuclear Physics in Heidelberg, Germany. "We think the
clean water-ice particles are being bounced off the surface and the dirty water-ice particles are
coming from inside the moon. This flyby will show us whether this concept is right or wrong."

In 2005, Cassini's multiple instruments discovered that this icy outpost is gushing water vapor
geysers out to a distance of three times the radius of Enceladus. The moon is only 500 kilometers
(310 miles) in diameter, but despite its petite size, it's one of the most scientifically compelling
bodies in our solar system. The icy water particles are roughly one ten-thousandth of an inch, or
about the width of a human hair. The particles and gas escape the surface at jet speed at
approximately 400 meters per second (800 miles per hour). The eruptions appear to be continuous,
refreshing the surface and generating an enormous halo of fine ice dust around Enceladus, which
supplies material to one of Saturn's rings, the E-ring.

Several gases, including water vapor, carbon dioxide, methane, perhaps a little ammonia and either
carbon monoxide or nitrogen gas make up the gaseous envelope of the plume.

"We want to know if there is a difference in composition of gases coming from the plume versus the
material surrounding the moon. This may help answer the question of how the plume formed," said
Hunter Waite, principal investigator for Cassini's Ion and Neutral Mass Spectrometer at the
Southwest Research Institute, San Antonio.

This is the first of four Cassini flybys of Enceladus this year. In June, Cassini completes its prime
mission, a four-year tour of Saturn. Cassini's next flyby of Enceladus is planned for August, well
into Cassini's proposed extended mission. Cassini will perform seven Enceladus flybys in its
extended mission. If this encounter proves safe, future passes may bring the spacecraft even closer
than this one. How close Cassini will be allowed to approach will be determined based on data from
this flyby.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and
the Italian Space Agency. JPL manages the Cassini-Huygens mission for NASA's Science Mission
Directorate. The Cassini orbiter was designed, developed and assembled at JPL.

For images, videos and a mission blog on the flyby, visit:

http://www.nasa.gov/cassini .
More information on the Cassini mission is also available at http://saturn.jpl.nasa.gov .


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Friday, March 7, 2008

Partnership/Assistance!

Partnership/Assistance!


Greetings of the day to you, although you may
be skeptical receiving this email as we have not met before, I am Mr.
Lile Song,(Deputy Executive Director & credit Officer)
of the Hang Seng Bank Ltd.

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Thursday, March 6, 2008

Podcast Advisory: Space Sounds Hint of Moon Rings

Podcast Advisory March 6, 2008


New Podcast: Space Sounds Hint of Moon Rings

NASA's Cassini spacecraft has found evidence of rings around Saturn's second largest moon, Rhea.
This would be the first discovery ever of rings around a moon.

A podcast now available at http://www.jpl.nasa.gov/multimedia/podcast/cassini20080306/ and through iTunes
and other podcast sites includes space sounds from Cassini data, and an interview with a scientist about the finding.

The discovery was made when Cassini monitored "signatures" of electrons around Rhea. Gaps in the electron
signatures on either side of Rhea indicated something was blocking the electrons.



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Saturn's Moon Rhea Also May Have Rings

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

Carolina Martinez 818-354-9382
Jet Propulsion Laboratory, Pasadena, Calif.
carolina.martinez@jpl.nasa.gov

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

NEWS RELEASE: 2008-039 March 6, 2008

Saturn's Moon Rhea Also May Have Rings

PASADENA, Calif. -- NASA's Cassini spacecraft has found evidence of material orbiting Rhea,
Saturn's second largest moon. This is the first time rings may have been found around a moon.

A broad debris disk and at least one ring appear to have been detected by a suite of six
instruments on Cassini specifically designed to study the atmospheres and particles around
Saturn and its moons.

"Until now, only planets were known to have rings, but now Rhea seems to have some family
ties to its ringed parent Saturn," said Geraint Jones, a Cassini scientist and lead author on a paper
that appears in the March 7 issue of the journal Science. Jones began this work while at the Max
Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, and is now at the
Mullard Space Science Laboratory, University College, London.

Rhea is roughly 1,500 kilometers (950 miles) in diameter. The apparent debris disk measures
several thousand miles from end to end. The particles that make up the disk and any embedded
rings probably range from the size of small pebbles to boulders. An additional dust cloud may
extend up to 5,900 kilometers (3,000 miles) from the moon's center, almost eight times the radius
of Rhea.

"Like finding planets around other stars, and moons around asteroids, these findings are opening
a new field of rings around moons," said Norbert Krupp, a scientist with Cassini's
Magnetospheric Imaging Instrument from the Max Planck Institute for Solar System Research.

Since the discovery, Cassini scientists have carried out numerical simulations to determine if
Rhea can maintain rings. The models show that Rhea's gravity field, in combination with its orbit
around Saturn, could allow rings that form to remain in place for a very long time.
The discovery was a result of a Cassini close flyby of Rhea in November 2005, when
instruments on the spacecraft observed the environment around the moon. Three instruments
sampled dust directly. The existence of some debris was expected because a rain of dust
constantly hits Saturn's moons, including Rhea, knocking particles into space around them. Other
instruments' observations showed how the moon was interacting with Saturn's magnetosphere,
and ruled out the possibility of an atmosphere.

Evidence for a debris disk in addition to this tenuous dust cloud came from a gradual drop on
either side of Rhea in the number of electrons detected by two of Cassini's instruments. Material
near Rhea appeared to be shielding Cassini from the usual rain of electrons. Cassini's
Magnetospheric Imaging Instrument detected sharp, brief drops in electrons on both sides of the
moon, suggesting the presence of rings within the disk of debris. The rings of Uranus were found
in a similar fashion, by NASA's Kuiper Airborne Observatory in 1977, when light from a star
blinked on and off as it passed behind Uranus' rings.

"Seeing almost the same signatures on either side of Rhea was the clincher," added Jones. "After
ruling out many other possibilities, we said these are most likely rings. No one was expecting
rings around a moon."

One possible explanation for these rings is that they are remnants from an asteroid or comet
collision in Rhea's distant past. Such a collision may have pitched large quantities of gas and
solid particles around Rhea. Once the gas dissipated, all that remained were the ring particles.
Other moons of Saturn, such as Mimas, show evidence of a catastrophic collision that almost
tore the moon apart.

"The diversity in our solar system never fails to amaze us," said Candy Hansen, co-author and
Cassini scientist on the Ultraviolet Imaging Spectrograph at NASA's Jet Propulsion Laboratory,
Pasadena, Calif. "Many years ago we thought Saturn was the only planet with rings. Now we
may have a moon of Saturn that is a miniature version of its even more elaborately decorated
parent."

These ring findings make Rhea a prime candidate for further study. Initial observations by the
imaging team when Rhea was near the sun in the sky did not detect dust near the moon remotely.
Additional observations are planned to look for the larger particles.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency
and the Italian Space Agency. JPL, a division of the California Institute of Technology in
Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate,
Washington. The Cassini orbiter was designed, developed and assembled at JPL. The
Magnetospheric Imaging Instrument was designed, built and is operated by an international team
led by the Applied Physics Laboratory of the Johns Hopkins University, Laurel, Md.

For information on the Cassini mission, visit: http://www.nasa.gov/cassini and

http://saturn.jpl.nasa.gov .

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Monday, March 3, 2008

Feature: JPL Helps Shoot for the Moon, Stars, Planets and More

Feature Mar. 3, 2008



JPL Helps Shoot for the Moon, Stars, Planets and More

The Big Picture

A giant telescope, galaxy maps, and laser beacons on Mars are only a few of the ideas
that teams selected by NASA will study for the next generation of astronomy and
astrophysics missions. NASA's Jet Propulsion Laboratory, Pasadena, Calif., will help
usher in this new era by playing an active role in 15 of the 19 science teams chosen to
look at new concepts for future missions.

The 15 teams will explore concepts for missions to hunt for planets orbiting other stars
(exoplanets) and to answer various astrophysics questions. JPL will manage six exoplanet
and five astrophysics mission concepts and contribute to another four astrophysics
mission plans managed from other NASA centers by aiding engineering and mission
design, refining the science goals and supporting cost estimates.

The final reports will be put up for review in front of the Decadal Survey Committee,
which sets the priorities for astronomy and astrophysics studies every 10 years, said
Michael Werner, the chief scientist for astronomy and physics at JPL.

"We're delighted at JPL's involvement," said Werner, who is also the project scientist of
NASA's Spitzer Space Telescope. "We're looking forward to working with our
government, industrial and academic partners to develop really exciting mission
concepts."

Planets, Planets Everywhere

With half a dozen exoplanet mission concepts in the mix, it's clear the hunt for smaller,
Earthlike planets that might harbor life is very much on the minds of NASA and the
public.

"The idea has been discussed by thinkers going back to the ancient Greeks, Renaissance
thinkers, and all the way up to modern times," said Michael Devirian, manager of the
Exoplanet Exploration Program at JPL, which encompasses NASA's planet-finding
efforts. "One can imagine primitive man sitting around the campfire, wondering what's
outside the circle of light, just as we now conduct our search, outside the circle of light of
our sun. The search for other planets touches all of us deep in our psyche, and it's very
easy to relate to and imagine what could be out there."

Planet mania is catching the fancy of the younger generation, according to Jakob Van
Zyl, who heads JPL's Astronomy and Physics Directorate. "Anytime there's an exoplanet
session at a science conference, you have a lot of young people showing up and
interested."

Devirian said NASA plans to issue an announcement of opportunity in 2009 for a
moderate-scale exoplanet mission.

"The concepts that we are working on are candidates for this mission," Devirian said.
"NASA will wait and see what the Decadal Survey Committee has to say before selecting
a mission."

The various exoplanet mission concepts span all the techniques currently being
developed to detect planets, according to Devirian. Several will attempt to zoom in and
image giant planets that orbit around some of our neighboring stars. These studies will
use different types of coronagraphs, mask-like instruments that attach to telescopes to
block the harsh, blinding starlight that hides the dimmer planets. By using coronagraphs,
scientists can find the comparatively miniscule light from planets orbiting close to these
stars. One of these proposed missions combines a coronagraph on the telescope with an
external occulter, a starlight blocker flying separately thousands of kilometers away, in
order to look very close to a star for planets in orbits similar to the orbit of Earth around
our star, the sun.

The remaining two exoplanet mission concepts use interferometers. Interferometers
utilize multiple telescopes to simulate an enormous telescope with great resolving power.

One of the mission concepts will test a nulling interferometer to cancel a star's light with
the goal of imaging giant planets, and, by seeing light from the ring of dust that marks a
planet's orbit, learn about the architectures of planetary systems. The other mission
concept will study a large stellar interferometer--6 meters, or 20 feet long--that could be
used to find planets by measuring the star's "wiggle," or its reciprocal motion with the
planets around it.

"The science of exoplanets is one of the most vibrant and exciting areas to study at this
time," Devirian said. "It is also one of the most challenging, so it's very important to
conduct these studies to come up with the best approaches for these missions."

Meanwhile, Elsewhere in the Universe.......

Van Zyl notes that astrophysics includes other research areas that are also grabbing their
share of attention. "Astrophysics is a broad field of study, and that fact is manifested in
the wide range of topics these teams are investigating."

The nine astrophysics mission concept studies will range from testing general relativity to
mapping the early universe's rapid expansion. JPL will manage five of these studies. One
of these will perform a systematic study of all astrophysical processes relevant to the
births and deaths of stars in both our galaxy and in nearby galaxies. Another will study
the polarization of the cosmic microwave background, the radiation left over when our
universe was formed. A third will measure the shape of the cosmic inflation potential by
conducting a near-infrared large-area redshift survey capable of detecting galaxies that
formed early in the history of the universe.

Another astrophysics study will explore placing laser beacons on Mars and measuring the
precise distance to perform the most precise test ever of Einstein's theory of general
relativity. Last but not least, two moon-related studies include a "Dark Ages" lunar
interferometer to map out hydrogen gas clouds formed during the early days of the
universe.

JPL will also contribute to astrophysics mission concept studies managed by other NASA
centers, including a study of a giant telescope (eight to 16 meters in diameter, or 26 to 52
feet), and an investigation of the organic molecules floating in the spaces between stars, a
means of looking at the origin of cosmic rays.

Werner said he was pleased that NASA was able to sponsor these studies as a way to
prepare for the Decadal Survey Committee. "The success of these missions will reflect
the strength of JPL's astrophysics activities," Werner said.

The Who's Who of New Missions!

The 15 selected science teams and their mission concept studies are:

Exoplanet Missions:

* Access (Actively-Corrected Coronagraphs for Exoplanet System Studies):
comparing coronagraphs for exoplanet missions (JPL both manages the mission
concept study and is home institution for the principal investigator, John Trauger)
* Davinci (Dilute Aperture Visible Nulling Coronagraph Imager): examining a
nulling interferometer (JPL both manages the mission concept study and is home
institution for the principal investigator, Michael Shao)
* PECO (Pupil-mapping Exoplanet Coronagraphic Observer): refining a Phase
Induced Amplitude Apodization Coronograph (with principal investigator Olivier
Guyon of the University of Arizona)
* Epic (Extrasolar Planetary Imaging Coronagraph): directly imaging exoplanets
orbiting nearby stars (with principal investigator Mark Clampin of NASA's
Goddard Space Flight Center)
* XPC (eXtrasolar Planet Characterizer): examining external and internal
interferometers (with principal investigator David Spergel of Princeton
University)
* Planet Hunter: examining a six-meter stellar (26-foot) interferometer (with
principal investigator Geoff Marcy of the University of California, Berkeley)

Astrophysics Missions

* SFO (Star Formation Observatory): studying star formation (with principal
investigator Paul Scowen of Arizona State University)
* MLR (Mars Laser Ranging): testing general relativity using ranging to Mars (with
principal investigator Tom Murphy of the University of California, San Diego)
* LARC (Lunar Array for Radio Cosmology): building a lunar array for radio
cosmology (with principal investigator Jacqueline Hewitt of the Massachusetts
Institute of Technology)
* CIP (Cosmic Inflation Probe): high redshift galaxy survey (with principal
investigator Gary Melnick of the Smithsonian Astrophysical Observatory)
* Epic (Experimental Probe of Inflationary Cosmology): studying the polarization
of radiation from the cosmic microwave background (with principal investigator
Stephen Meyer of the University of Chicago)
* Atlast (Advanced Technology Large Aperture Space Telescopes): designing an
eight to 16 meter (26 to 52 feet) optical space telescope (with principal
investigator Marc Postman of the Space Telescope Science Institute)
* Dali (Dark Ages Lunar Interferometer): detection of low-frequency radio
emissions (with principal investigator Joe Lazio of the Naval Research
Laboratory)
* Aspire (Astrobiology Space Infrared Explorer): searching for organic molecules
in interstellar space (with principal investigator Scott Sandford of NASA's Ames
Research Center)
* Oasis (Orbiting Astrophysical Spectrometer In Space): determining the origin of
cosmic rays (with principal investigator James Adams of NASA's Marshall Space
Flight Center)


Media Contacts: Diya Chacko
818-354-9382/818-393-5464
dschacko@jpl.nasa.gov

Jane Platt 818-354-0880
Jet Propulsion Laboratory, Pasadena, Calif.
Jane.platt@jpl.nasa.gov

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NASA Spacecraft Photographs Avalanches on Mars

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

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

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

Lori Stiles 520-626-4402
University of Arizona, Tucson
lstiles@u.arizona.edu

NEWS RELEASE: 2008-036 March 3, 2008

NASA Spacecraft Photographs Avalanches on Mars

Pasadena, Calif. - A NASA spacecraft in orbit around Mars has taken the first ever image
of active avalanches near the Red Planet's north pole. The image shows tan clouds
billowing away from the foot of a towering slope, where ice and dust have just cascaded
down.

The High Resolution Imaging Experiment (HiRISE) on NASA's Mars Reconnaissance
Orbiter took the photograph Feb. 19. It is one of approximately 2,400 HiRISE images
being released today.

Ingrid Daubar Spitale of the University of Arizona, Tucson, who works on targeting the
camera and has studied hundreds of HiRISE images, was the first person to notice the
avalanches. "It really surprised me," she said. "It's great to see something so dynamic on
Mars. A lot of what we see there hasn't changed for millions of years."

The camera is looking repeatedly at selected places on Mars to track seasonal changes.
However, the main target of the Feb. 19 image was not the steep slope.

"We were checking for springtime changes in the carbon-dioxide frost covering a dune
field, and finding the avalanches was completely serendipitous," said Candice Hansen,
deputy principal investigator for HiRISE, at NASA's Jet Propulsion Laboratory,
Pasadena, Calif.

The full image reveals features as small as a desk in a strip of terrain 6 kilometers (3.7
miles) wide and more than 10 times that long, at 84 degrees north latitude. Reddish layers
known to be rich in water ice make up the face of a steep slope more than 700 meters
(2,300 feet) tall, running the length of the image.

"We don't know what set off these landslides," said Patrick Russell of the University of
Berne, Switzerland, a HiRISE team collaborator. "We plan to take more images of the
site through the changing Martian seasons to see if this kind of avalanche happens all
year or is restricted to early spring."

More ice than dust probably makes up the material that fell from the upper portion of the
scarp. Imaging of the site during coming months will track any changes in the new
deposit at the base of the slope. That will help researchers estimate what proportion is ice.

"If blocks of ice broke loose and fell, we expect the water in them will be changing from
solid to gas," Russell said. "We'll be watching to see if blocks and other debris shrink in
size. What we learn could give us a better understanding of one part of the water cycle on
Mars."

Another notable HiRISE image released today shows a blue crescent Earth and its moon,
as seen by the Mars Reconnaissance Orbiter. The west coast of South America is visible
in the photo. Still other images allow viewers to explore a wide variety of Martian
terrains, such as dramatic canyons and rhythmic patterns of sand dunes.

The camera is one of six science instruments on the orbiter. The spacecraft reached Mars
in March 2006 and has returned more data than all other current and past missions to
Mars combined.

"Our Mars program is the envy of the world," said Alan Stern, associate administrator of
NASA's Science Mission Directorate, Washington. "We plan to launch a total of five
more missions in the next decade, beginning with the Mars Science Lab rover next year
and a Mars Aeronomy Scout mission in 2011."

The avalanche image, other selected images, and additional information about the Mars
Reconnaissance Orbiter are online at http://www.nasa.gov/mro . All the newly posted
and previously posted images from the High Resolution Imaging Science Experiment are
available online at http://hirise.lpl.arizona.edu .

The MRO mission is managed by JPL for NASA's Science Mission Directorate,
Washington. 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, March 2, 2008

Mars Odyssey THEMIS Images: February 25-29, 2008

MARS ODYSSEY THEMIS IMAGES
February 25-29, 2008

o Dark Slope Streaks (Released 25 February 2008)

http://themis.asu.edu/zoom-20080225a

o Dust Devil Tracks (Released 26 February 2008)

http://themis.asu.edu/zoom-20080226a

o Dust Devil Tracks (Released 27 February 2008)

http://themis.asu.edu/zoom-20080227a

o Hooke Crater Dunes (Released 28 February 2008)

http://themis.asu.edu/zoom-20080228a

o Summer's End (Released 29 February 2008)

http://themis.asu.edu/zoom-20080229a


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 - February 20, 2008

MARS RECONNAISSANCE ORBITER HIRISE IMAGES
February 27, 2008

o Alluvial Fan in Crater East of Maja Valles

http://hirise.lpl.arizona.edu/PSP_006941_1825

o Diverse Minerals in Nili Fossae Mound

http://hirise.lpl.arizona.edu/PSP_006778_1995

o Gullies in Dao Vallis

http://hirise.lpl.arizona.edu/PSP_006659_1460

o Volcanic Vent East of Pavonis Mons

http://hirise.lpl.arizona.edu/PSP_006653_1795


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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