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Wednesday, November 30, 2011

NASA's Grace Helps Monitor U.S. Drought

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

Written by:
Kelly Helm Smith, National Drought Mitigation Center; and Adam Voiland, NASA's Earth Science
News Team

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

News release: 2011-365 Nov. 30, 2011

NASA's Grace Helps Monitor U.S. Drought

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-365&cid=release_2011-365

The record-breaking drought in Texas that has fueled wildfires, decimated crops and forced cattle
sales has also reduced groundwater levels in much of the state to the lowest levels in more than 60
years, according to new national maps produced by NASA using data from the NASA/German
Aerospace Center Gravity Recovery and Climate Experiment (Grace) mission. The map are
distributed by the National Drought Mitigation Center at the University of Nebraska-Lincoln.

The latest groundwater map, released on Nov. 29, shows large patches of maroon over eastern Texas,
indicating severely depressed groundwater levels. The maps, publicly available on the Drought
Center's website at http://go.unl.edu/mqk , are generated weekly by NASA's Goddard Space Flight
Center in Greenbelt, Md., using Grace gravity field data calculated at NASA's Jet Propulsion
Laboratory, Pasadena, Calif., and the University of Texas Center for Space Research, Austin.

"Texas groundwater will take months or longer to recharge," said Matt Rodell, a hydrologist based at
Goddard. "Even if we have a major rainfall event, most of the water runs off. It takes a longer period
of sustained greater-than-average precipitation to recharge aquifers significantly."

The twin Grace satellites, which JPL developed and manages for NASA, detect small changes in
Earth's gravity field caused primarily by the redistribution of water on and beneath the land surface.
The paired satellites travel about 137 miles (220 kilometers) apart and record small changes in the
distance separating them as they encounter variations in Earth's gravitational field.

To make the maps, scientists use a sophisticated computer model that combines measurements of
water storage from Grace with a long-term meteorological dataset to generate a continuous record of
soil moisture and groundwater that stretches back to 1948. Grace data go back to 2002. The
meteorological data include precipitation, temperature, solar radiation and other ground- and space-
based measurements.

The color-coded maps show how much water is stored now as a probability of occurrence in the 63-
year record. The maroon shading over eastern Texas, for example, shows that the level of dryness
over the last week occurred less than two percent of the time between 1948 and the present.

The groundwater maps aren't the only maps based on Grace data that the Drought Center publishes
each week. The Drought Center also distributes soil moisture maps that show moisture changes in the
root zone down to about 3 feet (1 meter) below the surface, as well as surface soil moisture maps that
show changes within the top inch (2 centimeters) of the land.

"All of these maps offer policymakers new information into subsurface water fluctuations at regional
to national scales that has not been available in the past," said the Drought Center's Brian Wardlow.
The maps provide finer resolution or are more consistently available than other similar sources of
information, and having the maps for the three different levels should help decision makers
distinguish between short-term and long-term droughts.

"These maps would be impossible to generate using only ground-based observations," said Rodell.
"There are groundwater wells all around the United States, and the U.S. Geological Survey does keep
records from some of those wells, but it's not spatially continuous and there are some big gaps."

The maps also offer farmers, ranchers, water resource managers and even individual homeowners a
new tool to monitor the health of critical groundwater resources. "People rely on groundwater for
irrigation, for domestic water supply, and for industrial uses, but there's little information available on
regional to national scales on groundwater storage variability and how that has responded to a
drought," Rodell said. "Over a long-term dry period, there will be an effect on groundwater storage
and groundwater levels. It's going to drop quite a bit, people's wells could dry out, and it takes time to
recover."

The maps are the result of a NASA-funded project at the Drought Center and NASA Goddard to
make it easier for the weekly U.S. Drought Monitor to incorporate data from the Grace satellites. The
groundwater and soil moisture maps are updated each Tuesday.

To learn more about the Grace mission, visit: http://www.csr.utexas.edu/grace/ and
http://grace.jpl.nasa.gov/ .

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

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Saturday, November 26, 2011

NASA Launches Most Capable and Robust Rover to Mars

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109. PHONE 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

News release: 2011-362 Nov. 26, 2011

NASA Launches Most Capable and Robust Rover to Mars

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-362&cid=release_2011-362

CAPE CANAVERAL, Fla. -- NASA began a historic voyage to Mars with the Nov. 26 launch of the
Mars Science Laboratory, which carries a car-sized rover named Curiosity. Liftoff from Cape
Canaveral Air Force Station aboard an Atlas V rocket occurred at 10:02 a.m. EST (7:02 a.m. PST).

"We are very excited about sending the world's most advanced scientific laboratory to Mars," NASA
Administrator Charles Bolden said. "MSL will tell us critical things we need to know about Mars, and
while it advances science, we'll be working on the capabilities for a human mission to the Red Planet
and to other destinations where we've never been."

The mission will pioneer precision landing technology and a sky-crane touchdown to place Curiosity
near the foot of a mountain inside Gale Crater on Aug. 6, 2012. During a nearly two-year prime
mission after landing, the rover will investigate whether the region has ever offered conditions
favorable for microbial life, including the chemical ingredients for life.

"The launch vehicle has given us a great injection into our trajectory, and we're on our way to Mars,"
said Mars Science Laboratory Project Manager Peter Theisinger of NASA's Jet Propulsion
Laboratory in Pasadena, Calif. "The spacecraft is in communication, thermally stable and power
positive."

The Atlas V initially lofted the spacecraft into Earth orbit and then, with a second burst from the
vehicle's upper stage, pushed it out of Earth orbit into a 352-million-mile (567-million-kilometer)
journey to Mars.

"Our first trajectory correction maneuver will be in about two weeks," Theisinger said. "We'll do
instrument checkouts in the next several weeks and continue with thorough preparations for the
landing on Mars and operations on the surface."

Curiosity's ambitious science goals are among the mission's many differences from earlier Mars
rovers. It will use a drill and scoop at the end of its robotic arm to gather soil and powdered samples
of rock interiors, then sieve and parcel out these samples into analytical laboratory instruments inside
the rover. Curiosity carries 10 science instruments with a total mass 15 times as large as the science-
instrument payloads on the Mars rovers Spirit and Opportunity. Some of the tools are the first of their
kind on Mars, such as a laser-firing instrument for checking the elemental composition of rocks from
a distance, and an X-ray diffraction instrument for definitive identification of minerals in powdered
samples.

To haul and wield its science payload, Curiosity is twice as long and five times as heavy as Spirit or
Opportunity. Because of its one-ton mass, Curiosity is too heavy to employ airbags to cushion its
landing as previous Mars rovers could. Part of the Mars Science Laboratory spacecraft is a rocket-
powered descent stage that will lower the rover on tethers as the rocket engines control the speed of
descent.

The mission's landing site offers Curiosity access for driving to layers of the mountain inside Gale
Crater. Observations from orbit have identified clay and sulfate minerals in the lower layers,
indicating a wet history.

Precision landing maneuvers as the spacecraft flies through the Martian atmosphere before opening
its parachute make Gale a safe target for the first time. This innovation shrinks the target area to less
than one-fourth the size of earlier Mars landing targets. Without it, rough terrain at the edges of
Curiosity's target would make the site unacceptably hazardous.

The innovations for landing a heavier spacecraft with greater precision are steps in technology
development for human Mars missions. In addition, Curiosity carries an instrument for monitoring
the natural radiation environment on Mars, important information for designing human Mars missions
that protect astronauts' health.

The mission is managed by JPL, a division of the California Institute of Technology in Pasadena, for
NASA's Science Mission Directorate in Washington. The rover was designed, developed and
assembled at JPL. NASA's Launch Services Program at the Kennedy Space Center in Florida
managed the launch. NASA's Space Network provided space communication services for the launch
vehicle. NASA's Deep Space Network will provide spacecraft acquisition and mission
communication.

For more information about the mission, visit: http://www.nasa.gov/msl and
http://marsprogram.jpl.nasa.gov/msl/ .

For more information about the Deep Space Network, visit: http://deepspace.jpl.nasa.gov/dsn .

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Wednesday, November 23, 2011

Mars Science Laboratory Launch Milestones

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

Feature: 2011-361 Nov. 23, 2011

Mars Science Laboratory Launch Milestones

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-361&cid=release_2011-361

PASADENA, Calif. -- NASA's Mars Science Laboratory is tucked inside its Atlas V
rocket, ready for launch on Saturday, Nov. 26, 2011 from Cape Canaveral Air Force
Station in Florida. The Nov. 26 launch window extends from 7:02 a.m. to 8:45 a.m. PST
(10:02 a.m. to 11:45 a.m. EST). The launch period for the mission extends through Dec.
18.

The spacecraft, which will arrive at Mars in August 2012, is equipped with the most
advanced rover ever to land on another planet. Named Curiosity, the rover will
investigate whether the landing region has had environmental conditions favorable for
supporting microbial life, and favorable for preserving clues about whether life existed.

On Nov. 26, NASA Television coverage of the launch will begin at 4:30 a.m. PST (7:30
a.m. EST). Live launch coverage will be carried on all NASA Television channels. For
NASA Television downlink information, schedule information and streaming video,
visit: http://www.nasa.gov/ntv . The launch coverage will also be streamed live on
Ustream at http://www.ustream.tv/nasajpl .

If the spacecraft lifts off at the start of the launch window on Nov. 26, the following
milestones are anticipated. Times would vary for other launch times and dates.

Launch

--The rocket's first-stage common core booster, and the four solid rocket boosters, will
ignite before liftoff. Launch, or "T Zero", actually occurs before the rocket leaves the
ground. The four solid rocket boosters jettison at launch plus one minute and 52 seconds.

Fairing Separation

--The nose cone, or fairing, carrying Mars Science Laboratory will open like a clamshell
and fall away at about three minutes and 25 seconds after launch. After this, the rocket's
first stage will cut off and then drop into the Atlantic Ocean.

Parking Orbit

--The rocket's second stage, a Centaur engine, is started for the first time at about four
minutes and 38 seconds after launch. After it completes its first burn of about 7 minutes,
the rocket will be in a parking orbit around Earth at an altitude that varies from 102 miles
(165 kilometers) to 201 miles (324 kilometers). It will remain there from 14 to 30
minutes, depending on the launch date and time. If launch occurs at the beginning of the
launch Nov. 26 launch window, this stage will last about 21 minutes.

On the Way to Mars

-- The second Centaur burn, continuing for nearly 8 minutes (for a launch at the opening
of the Nov. 26 launch window), lofts the spacecraft out of Earth orbit and sends it toward
Mars.

Spacecraft Separation

--Mars Science Laboratory will separate from the rocket that boosted it toward Mars at
about 44 minutes after launch, if launch occurs at the opening of the Nov. 26 window.
Shortly after that, the separated Centaur performs its last task, an avoidance maneuver
taking itself out of the spacecraft's flight path to avoid hitting either the spacecraft or
Mars.

Sending a Message of Good Health

--Once the spacecraft is in its cruise stage toward Mars, it can begin communicating with
Earth via an antenna station in Canberra, Australia, part of NASA's Deep Space Network.
Engineers expect to hear first contact from the spacecraft at about 55 minutes after launch
and assess the spacecraft's health during the subsequent 30 minutes. The spacecraft will
arrive at the Red Planet Aug. 6, 2012, Universal Time (evening of Aug. 5, 2012, PDT).

NASA's Jet Propulsion Laboratory, Pasadena, Calif., a division of the California Institute
of Technology, manages the Mars Science Laboratory mission. Launch management is
the responsibility of NASA's Launch Services Program at the Kennedy Space Center in
Florida. The Atlas V launch service is provided by United Launch Alliance, Denver.

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Monday, November 21, 2011

NASA Updates Prelaunch Events for Mars Science Lab

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

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

Allard Beutel 321-867-2468
Kennedy Space Center, Fla.
allard.beutel@nasa.gov

Guy Webster/Priscilla Vega 818-354-6278/354-1357
Jet Propulsion Laboratory, Pasadena, Calif.
Guy.webster@jpl.nasa.gov / Priscilla.r.vega@jpl.nasa.gov

ADVISORY: 2011-360b Nov. 21, 2011

NASA Updates Prelaunch Events for Mars Science Lab

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-360b&cid=release_2011-360b

PASADENA, Calif. – NASA has updated information about the news conferences and other events for
the agency's Mars Science Laboratory Curiosity rover launch. Liftoff is scheduled at 7:02 a.m. PST
(10:02 a.m. EST) on Saturday, Nov. 26 from Cape Canaveral Air Force Station in Florida.

NASA Television's countdown launch commentary begins at 4:30 a.m. PST (7:30 a.m. EST) on Nov. 26.
That also is when a NASA blog will begin providing countdown updates at:
http://www.nasa.gov/mission_pages/msl/launch/launch_blog.html. Originating from Cape Canaveral
Hangar AE, the blog is the definitive Internet source for information leading up to liftoff.

Various news conferences and other events are being held at NASA facilities in Cape Canaveral and
Houston and will be carried live on NASA TV. Downlink information, schedule information and
streaming video are at: http://www.nasa.gov/ntv . The events will also be streamed live on Ustream at:
http://www.ustream.tv/nasajpl .

Detailed lists of news briefing times and participants are at:
http://www.nasa.gov/mission_pages/msl/news/index.html .

The Curiosity rover has 10 science instruments to search for evidence about whether Mars had
environments favorable for microbial life, including the chemical ingredients for life. The rover will use a
laser to look inside rocks and release their gasses so its spectrometer can analyze and send the data back
to Earth. The latest online information on the Mars Science Laboratory mission is at:
http://www.nasa.gov/msl . JPL, a division of the California Institute of Technology in Pasadena,
manages the mission for NASA.

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Thursday, November 17, 2011

Cassini Chronicles Life of Saturn's Giant Storm

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

Jia-Rui Cook 818-354-0850
Jet Propulsion Laboratory, Pasadena, Calif.
jccook@jpl.nasa.gov

Feature: 2011-359 Nov. 17, 2011

Cassini Chronicles the Life and Times of Saturn's Giant Storm

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-359&cid=release_2011-359

New images and animated movies from NASA's Cassini spacecraft chronicle the birth and
evolution of the colossal storm that ravaged the northern face of Saturn for nearly a year.

These new full-color mosaics and animations show the storm from its emergence as a tiny spot in
a single image almost one year ago, on Dec. 5, 2010, through its subsequent growth into a storm
so large it completely encircled the planet by late January 2011.

The monster tempest, which extended north-south approximately 9,000 miles (15,000
kilometers), is the largest seen on Saturn in the past two decades and is the largest by far ever
observed on the planet from an interplanetary spacecraft. On the same day that Cassini's high-
resolution cameras captured the first images of the storm, Cassini's radio and plasma wave
instrument detected the storm's electrical activity, revealing it to be a convective thunderstorm.
The storm's active convecting phase ended in late June, but the turbulent clouds it created linger
in the atmosphere today.

The storm's 200-day active period also makes it the longest-lasting planet-encircling storm ever
seen on Saturn. The previous record holder was an outburst sighted in 1903, which lingered for
150 days. The large disturbance imaged 21 years ago by NASA's Hubble Space Telescope and
comparable in size to the current storm lasted for only 55 days.

The collected images and movies from Cassini's imaging team can be seen at
http://www.nasa.gov/cassini , http://saturn.jpl.nasa.gov and http://ciclops.org . They include
mosaics of dozens of images stitched together and presented in true and false colors.

"The Saturn storm is more like a volcano than a terrestrial weather system," said Andrew
Ingersoll, a Cassini imaging team member at the California Institute of Technology in Pasadena.
"The pressure builds up for many years before the storm erupts. The mystery is that there's no
rock to resist the pressure – to delay the eruption for so many years."

Cassini has taken hundreds of images of this storm as part of the imaging team's "Saturn Storm
Watch" campaign. During this effort, Cassini takes quick looks at the storm in between other
scheduled observations of either Saturn or its rings and moons. The new images, together with
other high-quality images collected by Cassini since 2004, allow scientists to trace back the
subtle changes on the planet that preceded the storm's formation and have revealed insights into
the storm's development, its wind speeds and the altitudes at which its changes occur.

The storm first appeared at approximately 35 degrees north latitude on Saturn and eventually
wrapped itself around the entire planet to cover approximately 2 billion square miles (5 billion
square kilometers). The biggest disturbance Cassini had previously witnessed on Saturn occurred
in a latitude band in the southern hemisphere called "Storm Alley" because of the prevalence of
thunderstorms in this region. That storm lasted several months, from 2009 into 2010. That
disturbance was actually a cluster of thunderstorms, each of which lasted up to five days or so
and affected only the local weather. The recent northern disturbance is a single thunderstorm that
raged continuously for more than 200 days and impacted almost one-fifth of the entire northern
hemisphere.

"This new storm is a completely different kind of beast compared to anything we saw on Saturn
previously with Cassini," said Kunio Sayanagi, a Cassini imaging team associate and planetary
scientist at the University of California, Los Angeles. "The fact that such outbursts are episodic
and keep happening on Saturn every 20 to 30 years or so is telling us something about deep
inside the planet, but we have yet to figure out what it is."

Current plans to continue the mission through 2017 will provide opportunities for Cassini to
witness further changes in the planet's atmosphere as the seasons progress to northern summer.

"It is the capability of being in orbit and able to turn a scrutinizing eye wherever it is needed that
has allowed us to monitor this extraordinary phenomenon," said Carolyn Porco, Cassini imaging
team leader at the Space Science Institute in Boulder, Colo. "Seven years of taking advantage of
such opportunities have already made Cassini one of the most scientifically productive planetary
missions ever flown."

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency
and the Italian Space Agency. NASA's Jet Propulsion Laboratory in Pasadena manages the
mission for the agency's Science Mission Directorate in Washington. The Cassini orbiter and its
two onboard cameras were designed, developed and assembled at JPL. The imaging operations
team is based at the Space Science Institute in Boulder, Colo. JPL is a division of Caltech.

For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and
http://www.nasa.gov/cassini .

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NASA Orbiter Catches Mars Sand Dunes in Motion

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

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

Priscilla Vega 818-354-1357
Jet Propulsion Laboratory, Pasadena, Calif.
priscilla.r.vega@jpl.nasa.gov

News release: 2011-358 Nov. 17, 2011

NASA Orbiter Catches Mars Sand Dunes in Motion

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-358&cid=release_2011-358

PASADENA, Calif. -- Images from NASA's Mars Reconnaissance Orbiter show sand dunes and
ripples moving across the surface of Mars at dozens of locations and shifting up to several yards.
These observations reveal the planet's sandy surface is more dynamic than previously thought.

"Mars either has more gusts of wind than we knew about before, or the winds are capable of
transporting more sand," said Nathan Bridges, planetary scientist at the Johns Hopkins University's
Applied Physics Laboratory in Laurel, Md., and lead author of a paper on the finding published
online in the journal Geology. "We used to think of the sand on Mars as relatively immobile, so these
new observations are changing our whole perspective."

While red dust is known to swirl all around Mars in storms and dust devils, the planet's dark sand
grains are larger and harder to move. Less than a decade ago, scientists thought the dunes and ripples
on Mars either did not budge or moved too slowly for detection.

MRO was launched in 2005. Initial images from the spacecraft's High Resolution Imaging Science
Experiment (HiRISE) camera documented only a few cases of shifting sand dunes and ripples,
collectively called bedforms. Now, after years of monitoring the Martian surface, the spacecraft has
documented movements of a few yards (or meters) per year in dozens of locations across the planet.

The air on Mars is thin, so stronger gusts of wind are needed to push a grain of sand. Wind-tunnel
experiments have shown that a patch of sand would take winds of about 80 mph (nearly 130
kilometers per hour) to move on Mars compared with only 10 mph (about 16 kilometers per hour) on
Earth. Measurements from the meteorology experiments on NASA's Viking landers in the 1970s and
early 1980s, in addition to climate models, showed such winds should be rare on Mars.


The first hints that Martian dunes move came from NASA's Mars Global Surveyor, which operated
from 1997 to 2006. But the spacecraft's cameras lacked the resolution to definitively detect the
changes. NASA's Mars Exploration Rovers also detected hints of shifting sand when they touched
down on the Red Planet's surface in 2004. The mission team was surprised to see grains of sand
dotting the rovers' solar panels. They also witnessed the rovers' track marks filling in with sand.

"Sand moves by hopping from place to place," said Matthew Golombek, a co-author of the new paper
and a member of the Mars Exploration Rover and Mars Reconnaissance Orbiter teams at NASA's Jet
Propulsion Laboratory in Pasadena, Calif. "Before the rovers landed on Mars, we had no clear
evidence of sand moving."

Not all of the sand on Mars is blowing in the wind. The study also identifies several areas where the
bedforms did not move.

"The sand dunes where we didn't see movement today could have larger grains, or perhaps their
surface layers are cemented together," said Bridges, who also is a member of the HiRISE team.
"These studies show the benefit of long-term monitoring at high resolution."

According to scientists, the seemingly stationary areas might move on much larger time scales,
triggered by climate cycles on Mars that last tens of thousands of years. The tilt of Mars' axis relative
to its orbital plane can vary dramatically. This, combined with the oval shape of Mars' orbit, can
cause extreme changes in the Martian climate, much greater than those experienced on Earth. Mars
may once have been warm enough that the carbon dioxide now frozen in the polar ice caps could
have been free to form a thicker atmosphere, leading to stronger winds capable of transporting sand.

HiRISE is operated by the University of Arizona in Tucson. The instrument was built by Ball
Aerospace & Technologies Corp. of Boulder, Colo. The Mars Exploration Rovers Opportunity and
Spirit were built by JPL. JPL also manages the Mars Reconnaissance Orbiter and Mars Exploration
Rover projects for NASA's Science Mission Directorate in Washington. Lockheed Martin Space
Systems of Denver is NASA's industry partner for the Mars Reconnaissance Orbiter Project and built
the spacecraft.

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

MRO images and additional information is available online at:
http://www.nasa.gov/MRO and http://mars.jpl.nasa.gov/mro

For more information about NASA Mars missions, visit the Web at: www.nasa.gov/mars .

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Wednesday, November 16, 2011

NASA Probe Data Show Liquid Water Evidence on Europa

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

Jia-Rui Cook/Priscilla Vega 818-354-0850/354-1357
Jet Propulsion Laboratory, Pasadena, Calif.
jccook@jpl.nasa.gov / priscilla.r.vega@jpl.nasa.gov

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

Marc Airhart 512-471-2241
University of Texas at Austin
mairhart@jsq.utexas.edu

News release: 2011-355 Nov. 16, 2011

NASA Probe Data Show Liquid Water Evidence on Europa

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-355&cid=release_2011-355

PASADENA, Calif. -- Data from a NASA planetary mission have provided scientists evidence of
what appears to be a body of liquid water, equal in volume to the North American Great Lakes,
beneath the icy surface of Jupiter's moon, Europa.

The data suggest there is significant exchange between Europa's icy shell and the ocean beneath.
This information could bolster arguments that Europa's global subsurface ocean represents a
potential habitat for life elsewhere in our solar system. The findings are published in the scientific
journal Nature.

"The data open up some compelling possibilities," said Mary Voytek, director of NASA's
Astrobiology Program at agency headquarters in Washington. "However, scientists worldwide will
want to take a close look at this analysis and review the data before we can fully appreciate the
implication of these results."

NASA's Galileo spacecraft, launched by the space shuttle Atlantis in 1989 to Jupiter, produced
numerous discoveries and provided scientists decades of data to analyze. Galileo studied Jupiter,
which is the most massive planet in our solar system, and some of its many moons.

One of the most significant discoveries was the inference of a global saltwater ocean below the
surface of Europa. This ocean is deep enough to cover the whole surface of Europa and contains
more liquid water than all of Earth's oceans combined. However, being far from the sun, the ocean
surface is completely frozen. Most scientists think this ice crust is tens of miles thick.

"One opinion in the scientific community has been if the ice shell is thick, that's bad for biology.
That might mean the surface isn't communicating with the underlying ocean," said Britney Schmidt,
lead author of the paper and postdoctoral fellow at the Institute for Geophysics, University of Texas
at Austin. "Now, we see evidence that it's a thick ice shell that can mix vigorously and new
evidence for giant shallow lakes. That could make Europa and its ocean more habitable."

Schmidt and her team focused on Galileo images of two roughly circular, bumpy features on
Europa's surface called chaos terrains. Based on similar processes seen on Earth -- on ice shelves
and under glaciers overlying volcanoes -- they developed a four-step model to explain how the
features form. The model resolves several conflicting observations. Some seemed to suggest the ice
shell is thick. Others suggest it is thin.

This recent analysis shows the chaos features on Europa's surface may be formed by mechanisms
that involve significant exchange between the icy shell and the underlying lake. This provides a
mechanism or model for transferring nutrients and energy between the surface and the vast global
ocean already inferred to exist below the thick ice shell. This is thought to increase the potential for
life there.

The study authors have good reason to believe their model is correct, based on observations of
Europa from Galileo and of Earth. Still, because the inferred lakes are several miles below the
surface, the only true confirmation of their presence would come from a future spacecraft mission
designed to probe the ice shell. Such a mission was rated as the second highest priority flagship
mission by the National Research Council's recent Planetary Science Decadal Survey and is being
studied by NASA.

"This new understanding of processes on Europa would not have been possible without the
foundation of the last 20 years of observations over Earth's ice sheets and floating ice shelves," said
Don Blankenship, a co-author and senior research scientist at the Institute for Geophysics, where he
leads airborne radar studies of the planet's ice sheets.

Galileo was the first spacecraft to directly measure Jupiter's atmosphere with a probe and conduct
long-term observations of the Jovian system. The probe was the first to fly by an asteroid and
discover the moon of an asteroid. NASA extended the mission three times to take advantage of
Galileo's unique science capabilities, and the spacecraft was put on a collision course into Jupiter's
atmosphere in September 2003 to eliminate any chance of impacting Europa.

The Galileo mission was managed by NASA's Jet Propulsion Laboratory in Pasadena, Calif., for the
agency's Science Mission Directorate.

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

For images and a video animation of the findings, visit:
http://www.jsg.utexas.edu/news/2011/11/scientists-find-evidence-for-great-lake-on-europa/ .
For more information about the Galileo mission, visit: http://solarsystem.nasa.gov/galileo/ .

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NASA Hosts 150 Twitter Followers at Mars Rover Launch

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

Veronica McGregor 818-354-9452
Jet Propulsion Laboratory, Pasadena, Calif.
veronica.c.mcgregor@jpl.nasa.gov

Stephanie L. Schierholz 202-358-4997
NASA Headquarters, Washington
stephanie.schierholz@nasa.gov

News release: 2011-354 Nov. 16, 2011

NASA Hosts 150 Twitter Followers at Mars Rover Launch

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-354&cid=release_2011-354

PASADENA, Calif. – NASA has invited 150 followers of the agency's Twitter account to
a two-day launch Tweetup on Nov. 23 and 25 at the agency's Kennedy Space Center in
Florida.

The Tweetup is expected to culminate in the launch of the Mars Science Laboratory's
Curiosity rover aboard an Atlas V rocket from nearby Cape Canaveral Air Force Station.

The launch window is scheduled to open at 7:25 a.m. PST (10:25 a.m. EST) on Nov. 25.
Curiosity's arrival at Mars' Gale Crater is anticipated in August 2012. During the nearly
two-year prime mission, the rover will investigate whether a selected area of Mars
offered environmental conditions favorable for microbial life and preserved that
evidence, if it existed.

Tweetup participants were selected from more than 1,050 people who registered online.
They will share their Tweetup experiences with their followers through the social
networking site Twitter and other online forums.

Participants represent the United States, Australia, Belgium, Brazil, Canada, France,
Germany, Ireland, Spain and the United Kingdom. Attendees from the U.S. come from
the District of Columbia and 37 states: Alabama, Arizona, California, Connecticut,
Florida, Georgia, Hawaii, Idaho, Illinois, Indiana, Iowa, Kansas, Kentucky, Louisiana,
Maine, Maryland, Massachusetts, Michigan, Minnesota, Mississippi, Missouri, Nebraska,
New Hampshire, New Jersey, New Mexico, New York, North Carolina, Ohio, Oregon,
Pennsylvania, South Carolina, Tennessee, Texas, Utah, Virginia, Washington and
Wisconsin.

Beginning at 8 a.m. PST (11 a.m. EST) on Wednesday, Nov. 23, NASA will broadcast a
portion of the Tweetup when attendees talk with Jim Green, Planetary Science division
director, and Doug McCuistion, Mars Exploration program director, both from NASA
Headquarters in Washington. Engineers from NASA's Jet Propulsion Laboratory,
Pasadena, Calif., where the rover was designed and built, will speak, as will mission
scientists.

To watch the launch broadcast, visit: http://www.ustream.tv/channel/nasa-tweetup .
The broadcast with live chat will begin at 6:30 a.m. PST (9:30 a.m. EST) on
http://ustream.tv/nasajpl .

Tweetup participants also will tour Kennedy and Cape Canaveral, including a close-up
visit to the launch pad. On launch day, they will speak with NASA Administrator Charles
Bolden; Leland Melvin, NASA's assistant administrator for education; astronaut Doug
Wheelock and Bill Nye the Science Guy.

NASA invited its Twitter followers to attend eight previous launches: NASA's newest
Earth-observing satellite, NPP; the twin GRAIL spacecraft bound for the moon; the Juno
spacecraft on its way to Jupiter; and five space shuttle missions.

To follow participants on Twitter as they experience the prelaunch events and Curiosity's
liftoff, follow the #NASATweetup hashtag and the list of attendees at:
https://twitter.com/NASATweetup/mars-curiosity .

JPL manages the mission. NASA's Launch Services Program at Kennedy is managing the
launch.

For more information about the Mars Curiosity rover, visit: http://www.nasa.gov/msl
and http://mars.jpl.nasa.gov/msl .

Interact with the mission via Twitter and Facebook accounts at:
http://Twitter.com/MarsCuriosity and http://Facebook.com/MarsCuriosity .

To connect with NASA on Twitter and other social networking sites, visit:
http://www.nasa.gov/connect .

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Tuesday, November 15, 2011

NASA Hosting Science Update About Jupiter's Icy Moon Europa

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

Rosemary Sullivant 818-354-0850
Jet Propulsion Laboratory, Pasadena, Calif
Rosemary.sullivant@jpl.nasa.gov

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

Advisory: 2011-353b Nov. 15, 2011

NASA Hosting Science Update About Jupiter's Icy Moon Europa

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-353b&cid=release_2011-353b


PASADENA, Calif. -- NASA will host a Science Update at 10 a.m. PST (1 p.m. EST) on Wednesday,
Nov. 16, to discuss new theories concerning Jupiter's icy moon Europa. The event will be held at NASA
Headquarters in Washington.

NASA Television and the agency's website will broadcast the event live. For NASA TV streaming
video, scheduling and downlink information, visit: http://www.nasa.gov/ntv .

The event will also be streamed live, with a moderated chat, at: http://www.ustream.tv/nasajpl2 .

Europa, which is slightly smaller than Earth's moon, is thought to have an iron core, a rocky mantle and
an ocean of salty water beneath its frozen surface.

Briefing participants are:
- Britney Schmidt, postdoctoral fellow, Institute for Geophysics, University of Texas at Austin
- Tori Hoehler, astrobiologist and senior research scientist, NASA's Ames Research Center, Moffett Field, Calif.
- Louise Prockter, planetary scientist, Johns Hopkins University Applied Physics Laboratory, Laurel, Md.
- Tom Wagner, program scientist, cryospheric sciences, Earth Science Division, NASA Headquarters

For more information about NASA and agency programs, visit: http://www.nasa.gov .

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Friday, November 11, 2011

NASA Releases Updated Radar Movie of Asteroid 2005 YU55

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

DC Agle 818-393-9011
Jet Propulsion Laboratory, Pasadena, Calif.
agle@jpl.nasa.gov

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

Video advisory: 2011-351 Nov. 11, 2011

NASA Releases Updated Radar Movie of Asteroid 2005 YU55

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-351&cid=release_2011-351

PASADENA, Calif. – NASA Scientists working with the 230-foot-wide (70-meter) Deep Space
Network antenna at Goldstone, Calif., have released a second, longer, and more refined, movie
clip of asteroid 2005 YU55. The images were generated from data collected at Goldstone on
Nov. 7, 2011, between 11:24 a.m. and 1:35 p.m. PST (2:24 p.m. and 4:35 p.m. EST).

The movie clip can be found at: http://1.usa.gov/YU55 .

Each of the 28 frames required 20 minutes of data collection by the Goldstone radar. At the time
of the observations, 2005 YU55 was approximately 860,000 miles (1.4 million kilometers) from
Earth. The resolution is about 13 feet (4 meters) per pixel. 2005 YU55 takes approximately 18
hours to complete one rotation, so the rotation in the movie appears much more rapid than the
actual asteroid rotation speed.

The Goldstone observations utilized a new system to obtain images with a resolution of 4 meters,
which is five times finer than the highest resolution previously possible at Goldstone.

"The encounter with 2005 YU55 has produced an enormous amount of data that is still being
processed." said radar astronomer Lance Benner, the principal investigator for the 2005 YU55
Goldstone observations, from NASA's Jet Propulsion Laboratory in Pasadena, Calif. "The
sequence of images we obtained shows unprecedented fine-scale detail on this asteroid, which is
comparable in size to the Empire State Building. The Goldstone images show evidence for
concavities, a ridge near the asteroid's equator, and numerous features that may be large
boulders."

The trajectory of asteroid 2005 YU55 is well understood. Although the asteroid is in an orbit that
regularly brings it to the vicinity of Earth, (and Venus and Mars), 2005 YU55's 2011 encounter
with Earth was the closest for at least the last 200 years.

NASA detects, tracks and characterizes asteroids and comets passing close to Earth using both
ground- and space-based telescopes. The Near-Earth Object Observations Program, commonly
called "Spaceguard," discovers these objects, characterizes a subset of them, and plots their
orbits to determine if any could be potentially hazardous to our planet.

JPL manages the Near-Earth Object Program Office for NASA's Science Mission Directorate in
Washington. JPL is a division of the California Institute of Technology in Pasadena.

More information about asteroids and near-Earth objects is at:
http://www.jpl.nasa.gov/asteroidwatch and via Twitter at http://www.twitter.com/asteroidwatch
. More information about asteroid radar research is at: http://echo.jpl.nasa.gov/ . More
information about the Deep Space Network is at: http://deepspace.jpl.nasa.gov/dsn .

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Thursday, November 10, 2011

NASA Sets Mars Science Laboratory Launch Coverage

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

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

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

George H. Diller 321-867-2468
Kennedy Space Center, Fla.
george.h.diller@nasa.gov

ADVISORY: 2011-349b Nov. 10, 2011

NASA Sets Mars Science Laboratory Launch Coverage

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-349b&cid=release_2011-349b

PASADENA, Calif. -- NASA's Mars Science Laboratory spacecraft with the Curiosity rover is set to
launch to the planet Mars aboard an Atlas V rocket on Nov. 25, 2011 from Space Launch Complex
41 at Cape Canaveral Air Force Station in Florida. The launch window extends from 10:25 a.m. to
12:08 p.m. EST (7:25 a.m. to 9:08 a.m. PST). The launch period for the mission extends through Dec.
18.

The spacecraft will arrive at Mars in August 2012. Curiosity has 10 science instruments to search for
evidence about whether Mars had environments favorable for microbial life, including the chemical
ingredients for life. The unique rover will use a laser to look inside rocks and release their gasses so
that a spectrometer can analyze them and send the data back to Earth.

Briefings about the mission are scheduled throughout the week leading to launch and will be held at
the Kennedy Space Center's Press Site.

Science Briefings and Prelaunch News Conference

Monday, Nov. 21, 1 p.m. EST (10 a.m. PST): "What Do We Know About Mars?"
Participants will be:

Michael Meyer, lead scientist, Mars Exploration Program
NASA Headquarters, Washington

John Grotzinger, project scientist, Mars Science Laboratory
California Institute of Technology, Pasadena, Calif.

Bethany Ehlmann, scientist, NASA Jet Propulsion Laboratory, Pasadena, Calif.
Assistant professor, California Institute of Technology, Pasadena, Calif.

Tuesday, Nov. 22, 11 a.m. EST (8 a.m. PST): "Looking for Signs of Life in the Universe"
Participants will be:

Mary Voytek, director, Astrobiology Program
NASA Headquarters, Washington

Jamie Foster, professor, Department of Microbiology and Cell Science
University of Florida, Gainesville

Pan Conrad, deputy principal investigator, Sample Analysis at Mars, Mars Science Laboratory
NASA Goddard Space Flight Center, Greenbelt, Md.

Steven Benner, director, Foundation for Applied Molecular Evolution
Gainesville, Fla.

Catharine Conley, planetary protection officer
NASA Headquarters, Washington


Tuesday, Nov. 22, 1 p.m. EST (10 a.m. PST): Prelaunch News Conference
Participants will be:

Colleen Hartman, assistant associate administrator, Science Mission Directorate
NASA Headquarters, Washington

Omar Baez, NASA launch director
NASA's Kennedy Space Center, Cape Canaveral, Fla.

Vernon Thorp, program manager, NASA Missions
United Launch Alliance, Denver

Peter Theisinger, Mars Science Laboratory project manager
NASA Jet Propulsion Laboratory, Pasadena, Calif.

Clay Flinn, launch weather officer
45th Weather Squadron, Cape Canaveral Air Force Station, Fla.


Curiosity Mission Science Briefing: This briefing will immediately follow the prelaunch news
conference. Participants will be:

Michael Meyer, lead scientist for Mars Exploration Program
NASA Headquarters, Washington

John Grotzinger, project scientist for Mars Science Laboratory
California Institute of Technology, Pasadena, Calif.

Paul Mahaffy, principal investigator for Sample Analysis at Mars investigation on Curiosity
NASA Goddard Space Flight Center, Greenbelt, Md.

David Blake, principal investigator for Chemistry and Mineralogy investigation on Curiosity
NASA Ames Research Center, Moffett Field, Calif.

Michael Malin, principal investigator for the Mast Camera and Mars Descent Imager investigations
on Curiosity
Malin Space Science Systems, San Diego

Roger Wiens, principal investigator for Chemistry and Camera investigation on Curiosity
Los Alamos National Laboratory, Los Alamos, N.M.


Wednesday, Nov. 23, 1 p.m. EST (10 a.m. PST): "Why Mars Excites and Inspires Us"
Participants will be:

Leland Melvin, associate administrator for Education
NASA Headquarters, Washington

Scott Anderson, teacher and science department chairman
Da Vinci School for Science & the Arts, El Paso, Texas

Clara Ma, student, NASA contest winner for naming Curiosity
Shawnee Mission East High School, Prairie Village, Kansas

Veronica McGregor, manager, Media Relations Office
NASA Jet Propulsion Laboratory, Pasadena, Calif.


Wednesday, Nov. 23, 2 p.m. EST (11 a.m. PST): "Missions to Mars: Robotics and Humans
Together"
(Originating from NASA's Johnson Space Center, Houston)

Doug Ming, manager, Human Exploration Science Office; Mars Science Laboratory Co-Investigator
NASA Johnson Space Center, Houston

Bret Drake, deputy chief architect, Human Spaceflight Architecture Team
NASA Johnson Space Center, Houston

Matt Ondler, assistant director, Advanced Project Development
NASA Johnson Space Center, Houston

Mike Gernhardt, NASA astronaut
NASA Johnson Space Center, Houston

John Charles, program scientist, Human Research Program
NASA Johnson Space Center, Houston

A post-launch news conference will be held at the NASA News Center approximately 2 ½ hours
after launch.

NASA Television Launch Coverage
On Friday, Nov. 25, NASA Television coverage of the launch will begin at 8 a.m. EST (5 a.m. PST)
and conclude after spacecraft separation from the Atlas V occurs 53 minutes, 49 seconds after launch.
Live launch coverage will be carried on all NASA Television channels.

A post-launch news conference will be held at the Kennedy press site approximately 2 ½ hours after
launch.

For NASA Television downlink information, schedule information and streaming video, visit:
http://www.nasa.gov/ntv .

Launch coverage also will be available on local amateur VHF radio frequency 146.940 MHz
broadcast within Brevard County.

Ustream Coverage
The Mars Science Laboratory news conferences, briefings and launch will be streamed live on
Ustream at http://www.ustream.tv/nasajpl .

NASA Web Coverage
Extensive prelaunch and launch day coverage of the liftoff of the Mars Science Laboratory spacecraft
aboard an Atlas V rocket will be available on NASA's home page on the Internet at:
http://www.nasa.gov .

A prelaunch webcast for the mission will be streamed on the Web on Wednesday, Nov. 22, at noon
EST (9 a.m. PST). Live countdown coverage through NASA's Launch Blog begins at 8 a.m. EST (5
a.m. PST) on Friday, Nov. 25. Coverage features live updates as countdown milestones occur, as well
as streaming video clips highlighting launch preparations and liftoff.

To view the webcast and the blog or to learn more about Mars Science Laboratory, visit the mission
home page at: http://www.nasa.gov/msl and http://mars.jpl.nasa.gov/msl .

Twitter
The NASA News Twitter feed will be updated throughout the launch countdown. You can follow the
updates at: http://www.twitter.com/nasa and http://www.twitter.com/nasakennedy and
http://www.twitter.com/nasajpl .

NASA's Jet Propulsion Laboratory, Pasadena, Calif., a division of the California Institute of
Technology, manages the Mars Science Laboratory mission. Launch management is the
responsibility of NASA's Launch Services Program at the Kennedy Space Center in Florida. The
Atlas V launch service is provided by United Launch Alliance, Denver.

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New Study Shows Very First Stars Not Monstrous

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: 2011-348 Nov. 10, 2011

New Study Shows Very First Stars Not Monstrous

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-348&cid=release_2011-348

PASADENA, Calif. -- The very first stars in our universe were not the behemoths scientists had
once thought, according to new simulations performed at NASA's Jet Propulsion Laboratory,
Pasadena, Calif.

Astronomers "grew" stars in their computers, mimicking the conditions of our primordial
universe. The simulations took weeks. When the scientists' concoctions were finally done, they
were shocked by the results -- the full-grown stars were much smaller than expected.

Until now, it was widely believed that the first stars were the biggest of all, with masses
hundreds of times that of our sun. The new research shows they are only tens of times the mass
of sun; for example, the simulations produced one star that was as little as 43 solar masses.

"The first stars were definitely massive, but not to the extreme we thought before," said Takashi
Hosokawa, an astronomer at JPL and lead author of the new study, appearing online Friday,
Nov. 11 in the journal Science. "Our simulations reveal that the growth of these stars is stunted
earlier than expected, resulting in smaller final sizes."

The early universe consisted of nothing more than thin clouds of hydrogen and helium atoms. A
few hundred million years after its birth, the first stars began to ignite. How these first stars
formed is still a mystery.

Astronomers know that all stars form out of collapsing clouds of gas. Gravity from a growing
"seed" at the center of the cloud attracts more and more matter. For so-called normal stars like
our sun, this process is aided by heavier elements such as carbon, which help to keep the gas
falling onto the budding star cool enough to collapse. If the cloud gets too hot, the gas expands
and escapes.

But, in the early universe, stars hadn't yet produced heavy elements. The very first stars had to
form out of nothing but hydrogen and helium. Scientists had theorized that such stars would
require even more mass to form, to compensate for the lack of heavy elements and their cooling
power. At first, it was thought the stars might be as big as one thousand times the mass of our
sun. Later, the models were refined and the first stars were estimated to be hundreds of solar
masses.

"These stars keep getting smaller and smaller over time," said Takashi. "Now we think they are
even less massive, only tens of solar masses."

The team's simulations reveal that matter in the vicinity of the forming stars heats up to higher
temperatures than previously believed, as high as 50,000 Kelvin (90,000 degrees Fahrenheit), or
8.5 times the surface temperature of the sun. Gas this hot expands and escapes the gravity of the
developing star, instead of falling back down onto it. This means the stars stop growing earlier
than predicted, reaching smaller final sizes.

"This is definitely going to surprise some folks," said Harold Yorke, an astronomer at JPL and
co-author of the study. "It was standard knowledge until now that the first stars had to be
extremely massive."

The results also answer an enigma regarding the first stellar explosions, called supernovae. When
massive stars blow up at the end of their lives, they spew ashes made of heavier elements into
space. If the very first stars were the monsters once thought, they should have left a specific
pattern of these elements imprinted on the material of the following generation of stars. But, as
much as astronomers searched the oldest stars for this signature, they couldn't find it. The
answer, it seems, is that it simply is not there. Because the first stars weren't as massive as
previously thought, they would have blown up in a manner akin to the types of stellar explosions
that we see today.

"I am sure there are more surprises in store for us regarding this exciting period of the universe,"
said Yorke. "NASA's upcoming James Webb Space Telescope will be a valuable tool to observe
this epoch of early star and galaxy formation."

The California Institute of Technology manages JPL for NASA. More information about JPL is
online at www.jpl.nasa.gov .

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NASA Ready for November Launch of Car-Size Mars Rover

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 PHONE 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
Headquarters, Washington
dwayne.c.brown@nasa.gov

News release: 2011-347 Nov. 10, 2011

NASA Ready for November Launch of Car-Size Mars Rover

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-347&cid=release_2011-347

PASADENA, Calif. -- NASA's most advanced mobile robotic laboratory, which will examine one of
the most intriguing areas on Mars, is in final preparations for a launch from Florida's Space Coast at
10:25 a.m. EST (7:25 a.m. PST) on Nov. 25.

The Mars Science Laboratory mission will carry Curiosity, a rover with more scientific capability
than any ever sent to another planet. The rover is now sitting atop an Atlas V rocket awaiting liftoff
from Cape Canaveral Air Force Station.

"Preparations are on track for launching at our first opportunity," said Pete Theisinger, Mars Science
Laboratory project manager at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "If weather or
other factors prevent launching then, we have more opportunities through Dec. 18."

Scheduled to land on the Red Planet in August 2012, the one-ton rover will examine Gale Crater
during a nearly two-year prime mission. Curiosity will land near the base of a layered mountain 3
miles (5 kilometers) high inside the crater. The rover will investigate whether environmental
conditions ever have been favorable for development of microbial life and preserved evidence of
those conditions.

"Gale gives us a superb opportunity to test multiple potentially habitable environments and the
context to understand a very long record of early environmental evolution of the planet," said John
Grotzinger, project scientist for the Mars Science Laboratory at the California Institute of Technology
in Pasadena. "The portion of the crater where Curiosity will land has an alluvial fan likely formed by
water-carried sediments. Layers at the base of the mountain contain clays and sulfates, both known to
form in water."

Curiosity is twice as long and five times as heavy as earlier Mars rovers Spirit and Opportunity. The
rover will carry a set of 10 science instruments weighing 15 times as much as its predecessors'
science payloads.

A mast extending to 7 feet (2.1 meters) above ground provides height for cameras and a laser-firing
instrument to study targets from a distance. Instruments on a 7-foot-long (2.1-meter-long) arm will
study targets up close. Analytical instruments inside the rover will determine the composition of rock
and soil samples acquired with the arm's powdering drill and scoop. Other instruments will
characterize the environment, including the weather and natural radiation that will affect future
human missions.

"Mars Science Laboratory builds upon the improved understanding about Mars gained from current
and recent missions," said Doug McCuistion, director of the Mars Exploration Program at NASA
Headquarters in Washington. "This mission advances technologies and science that will move us
toward missions to return samples from, and eventually send humans to, Mars."

The mission is challenging and risky. Because Curiosity is too heavy to use an air-bag cushioned
touchdown, the mission will use a new landing method, with a rocket-powered descent stage
lowering the rover on a tether like a kind of sky-crane.

The mission will pioneer precision landing methods during the spacecraft's crucial dive through Mars'
atmosphere next August to place the rover onto a smaller landing target than any previously for a
Mars mission. The target inside Gale Crater is 12.4 miles (20 kilometers) by 15.5 miles (25
kilometers). Rough terrain just outside that area would have disqualified the landing site without the
improved precision.

No mission to Mars since the Viking landers in the 1970s has sought a direct answer to the question
of whether life has existed on Mars. Curiosity is not designed to answer that question by itself, but its
investigations for evidence about prerequisites for life will steer potential future missions toward
answers.

The mission is managed by JPL for NASA's Science Mission Directorate in Washington. Curiosity
was designed, developed and assembled at JPL. Launch management for the mission is the
responsibility of NASA's Launch Services Program at the Kennedy Space Center in Florida. NASA's
Space Network, managed by the Goddard Space Flight Center in Greenbelt, Md., will provide space
communications services for the rocket. NASA's international Deep Space Network will provide
MSL spacecraft acquisition and communication throughout the mission.

For more information, visit: http://www.nasa.gov/msl and http://mars.jpl.nasa.gov/msl . You can also
follow the mission on Facebook at http://www.facebook.com/marscuriosity and on Twitter at
http://www.twitter.com/marscuriosity .

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Tuesday, November 8, 2011

NASA Releases Radar Movie of Asteroid 2005 YU55

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

DC Agle 818-393-9011
Jet Propulsion Laboratory, Pasadena, Calif.
agle@jpl.nasa.gov

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

Image/Video advisory: 2011-346 Nov. 8, 2011

NASA Releases Radar Movie of Asteroid 2005 YU55

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-346&cid=release_2011-346

PASADENA, Calif. -- Scientists working with the 230-foot-wide (70-meter) Deep Space
Network antenna at Goldstone, Calif., have generated a short movie clip of asteroid 2005 YU55.
The images were generated from data collected at Goldstone on Nov. 7, 2011, between 11:24
a.m. and 1:35 p.m. PST (2:24 p.m. and 4:35 p.m. EST). They are the highest-resolution images
ever generated by radar of a near-Earth object.

The short movie clip can be found at: http://1.usa.gov/uVJvmS .

Each of the six frames required 20 minutes of data collection by the Goldstone radar. At the
time, 2005 YU55 was approximately 860,000 miles (1.38 million kilometers) away from Earth.
Resolution is 4 meters per pixel.

"The movie shows the small subset of images obtained at Goldstone on November 7 that have
finished processing. By animating a sequence of radar images, we can see more surface detail
than is visible otherwise," said radar astronomer Lance Benner, the principal investigator for the
2005 YU55 observations, from NASA's Jet Propulsion Laboratory in Pasadena, Calif. "The
animation reveals a number of puzzling structures on the surface that we don't yet understand.
To date, we've seen less than one half of the surface, so we expect more surprises."

The trajectory of asteroid 2005 YU55 is well understood. At the point of closest approach today
at 3:28 p.m. PST (6:28 p.m. EST/2328 UTC), it was no closer than 201,700 miles (324,600
kilometers), as measured from the center of Earth. The gravitational influence of the asteroid will
have no detectable effect on anything here on Earth, including our planet's tides or tectonic
plates. Although 2005 YU55 is in an orbit that regularly brings it to the vicinity of Earth (and
Venus and Mars), the 2011 encounter with Earth is the closest this space rock has come for at
least the last 200 years.

The last time a space rock as big came as close to Earth was in 1976, although astronomers did
not know about the flyby at the time. The next known approach of an asteroid this large will be
in 2028.

NASA detects, tracks and characterizes asteroids and comets passing close to Earth using both
ground- and space-based telescopes. The Near-Earth Object Observations Program, commonly
called "Spaceguard," discovers these objects, characterizes a subset of them, and plots their
orbits to determine if any could be potentially hazardous to our planet.

JPL manages the Near-Earth Object Program Office for NASA's Science Mission Directorate in
Washington. JPL is a division of the California Institute of Technology in Pasadena.

More information about asteroids and near-Earth objects is at:
http://www.jpl.nasa.gov/asteroidwatch . More information about asteroid radar research is at:
http://echo.jpl.nasa.gov/ . More information about the Deep Space Network is at:
http://deepspace.jpl.nasa.gov/dsn .

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NASA to Hold Media Briefing About Mars Rover Launch

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

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

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

Advisory: 2011-344b Nov. 8, 2011

NASA to Hold Media Briefing About Mars Rover Launch

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-344b&cid=release_2011-344b

PASADENA, Calif. -- NASA will hold a news conference at 10 a.m. PST (1 p.m. EST), Thursday,
Nov. 10, to discuss the upcoming launch of the Mars Science Laboratory, with the largest and most
capable rover going to another planet. The televised event will take place at NASA Headquarters in
Washington and will be carried live on NASA TV and Ustream.

The Mars Science Laboratory mission is scheduled to launch at 7:25 a.m. PST (10:25 a.m. EST), on
Nov. 25. The launch period extends to Dec. 18. The spacecraft will deliver a car-size rover named
Curiosity to the surface of Mars in August 2012.

News conference participants are:
-- Doug McCuistion, director, Mars Program, NASA Headquarters, Washington
-- Ashwin Vasavada, Mars Science Laboratory deputy project scientist, NASA's Jet Propulsion
Laboratory, Pasadena, Calif.
-- Pete Theisinger, Mars Science Laboratory project manager, JPL

NASA TV streaming video, scheduling and downlink information is at: http://www.nasa.gov/ntv .
The news conference will also be carried on JPL's Ustream channel, with a moderated chat, at
http://www.ustream.tv/nasajpl .

For more information about the new rover, visit: http://www.nasa.gov/msl and
http://mars.jpl.nasa.gov/msl .

JPL, a division of the California Institute of Technology in Pasadena, manages the Mars Science
Laboratory mission for NASA.

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Upcoming Workshops at NASA/JPL's Educator Resource Center

Upcoming Educator Workshops Nov. 08, 2011

This is a feature from the NASA/JPL Education Office.

Robotics

Date: Saturday, Nov. 12, 2011, 10 a.m. - 12 p.m.

Target audience: K-12 educators

Location: NASA/JPL Educator Resource Center, Pomona, Calif.

Overview:Did you know that at JPL we talk to Mars robots every day? Discover how engineers use animals to design robots. Come see the exciting extent that we use robotics today and look into the future for space and medicine. Make and take inexpensive classroom activities and bring technology into your classroom! This workshop is being offered at the NASA/JPL Educator Resource Center located in Pomona, please call 909-397-4420 to reserve your spot.

For more information and directions, visit: http://www.jpl.nasa.gov/education/index.cfm?page=115


Go For Flight!

Date: Saturday, Dec. 10, 2011, 10 a.m. - 12 p.m.

Target audience: K-12 educators

Location: NASA/JPL Educator Resource Center, Pomona, Calif.

Overview: Math and science come alive as you construct aircraft models (kite, helicopter and glider), and launch rockets! Use questioning strategies and redesign to make these activities educationally challenging! This workshop is being offered at the NASA/JPL Educator Resource Center located in Pomona, please call 909-397-4420 to reserve your spot.

For more information and directions, visit: http://www.jpl.nasa.gov/education/index.cfm?page=115


Toys In Space ll

Date:Saturday, Jan. 21, 2012, 10 a.m. - 12 p.m.

Target audience: K-12 educators

Location:NASA/JPL Educator Resource Center, Pomona, Calif.

Overview: View the educational video "Toys in Space II," which was taped during the flight of STS-54. The video shows astronauts on the space shuttle and students back on Earth co-investigating the behavior of toys in space. Video program segments show the toys' behavior in 1G (Earth's gravity) and then their behavior in the microgravity environment of space! This workshop is being offered at the NASA/JPL Educator Resource Center located in Pomona, please call 909-397-4420 to reserve your spot.

For more information and directions, visit: http://www.jpl.nasa.gov/education/index.cfm?page=115


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Monday, November 7, 2011

NASA Captures New Images of Large Asteroid Passing Earth

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

DC Agle 818-393-9011
Jet Propulsion Laboratory, Pasadena, Calif.
agle@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov
News release: 2011-343 Nov. 7, 2011

NASA Captures New Images of Large Asteroid Passing Earth

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-343&cid=release_2011-343

PASADENA, Calif. -- NASA's Deep Space Network antenna in Goldstone, Calif. has captured new
radar images of Asteroid 2005 YU55 passing close to Earth.

The asteroid safely will safely fly past our planet slightly closer than the moon's orbit on Nov. 8. The
last time a space rock this large came as close to Earth was in 1976, although astronomers did not
know about the flyby at the time. The next known approach of an asteroid this size will be in 2028.

The image was taken on Nov. 7 at 11:45 a.m. PST (2:45 p.m. EST/1945 UTC), when the asteroid was
approximately 860,000 miles (1.38 million kilometers) away from Earth. Tracking of the aircraft
carrier-sized asteroid began at Goldstone at 9:30 a.m. PDT on Nov. 4 with the 230-foot-wide (70-
meter) antenna and lasted about two hours, with an additional four hours of tracking planned each
day from Nov. 6 - 10.

Radar observations from the Arecibo Planetary Radar Facility in Puerto Rico will begin Nov. 8, the
same day the asteroid will make its closest approach to Earth at 3:28 p.m. PST (6:28 p.m. EST/1128
UTC).

The trajectory of asteroid 2005 YU55 is well understood. At the point of closest approach, it will be
no closer than 201,700 miles (324,600 kilometers) as measured from the center of Earth, or about
0.85 times the distance from the moon to Earth. The gravitational influence of the asteroid will have
no detectable effect on Earth, including tides and tectonic plates. Although the asteroid is in an orbit
that regularly brings it to the vicinity of Earth, Venus and Mars, the 2011 encounter with Earth is the
closest it has come for at least the last 200 years.

NASA detects, tracks and characterizes asteroids and comets passing close to Earth using both
ground- and space-based telescopes. The Near-Earth Object Observations Program at NASA's Jet
Propulsion Laboratory in Pasadena, Calif., commonly called "Spaceguard," discovers these objects,
characterizes some of them, and plots their orbits to determine if any could be potentially hazardous
to our planet. JPL manages the Near-Earth Object Program Office for NASA's Science Mission
Directorate in Washington.

The new radar images are online at:
http://www.nasa.gov/mission_pages/asteroids/multimedia/yu55-20111107.html .

For more information about asteroids and near-Earth objects, visit:
http://www.jpl.nasa.gov/asteroidwatch .

More information about asteroid radar research is available online at: http://echo.jpl.nasa.gov/ .

For more information about NASA's Deep Space Network, visit: http://deepspace.jpl.nasa.gov/dsn
.

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Wednesday, November 2, 2011

NASA Study of Clays Suggests Watery Mars Underground

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 PHONE 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

News release: 2011-337 Nov. 2, 2011

NASA Study of Clays Suggests Watery Mars Underground

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-337&cid=release_2011-337

PASADENA, Calif. -- A new NASA study suggests if life ever existed on Mars, the longest lasting
habitats were most likely below the Red Planet's surface.

A new interpretation of years of mineral-mapping data, from more than 350 sites on Mars examined
by European and NASA orbiters, suggests Martian environments with abundant liquid water on the
surface existed only during short episodes. These episodes occurred toward the end of a period of
hundreds of millions of years during which warm water interacted with subsurface rocks. This has
implications about whether life existed on Mars and how the Martian atmosphere has changed.

"The types of clay minerals that formed in the shallow subsurface are all over Mars," said John
Mustard, professor at Brown University in Providence, R.I. Mustard is a co-author of the study in the
journal Nature. "The types that formed on the surface are found at very limited locations and are quite
rare."

Discovery of clay minerals on Mars in 2005 indicated the planet once hosted warm, wet conditions. If
those conditions existed on the surface for a long era, the planet would have needed a much thicker
atmosphere than it has now to keep the water from evaporating or freezing. Researchers have sought
evidence of processes that could cause a thick atmosphere to be lost over time.

This new study supports an alternative hypothesis that persistent warm water was confined to the
subsurface and many erosional features were carved during brief periods when liquid water was
stable at the surface.

"If surface habitats were short-term, that doesn't mean we should be glum about prospects for life on
Mars, but it says something about what type of environment we might want to look in," said the
report's lead author, Bethany Ehlmann, assistant professor at the California Institute of Technology,
Pasadena, and scientist at NASA's Jet Propulsion Laboratory, also in Pasadena. "The most stable
Mars habitats over long durations appear to have been in the subsurface. On Earth, underground
geothermal environments have active ecosystems."

The discovery of clay minerals by the OMEGA spectrometer on the European Space Agency's Mars
Express orbiter added to earlier evidence of liquid Martian water. Clays form from the interaction of
water with rock. Different types of clay minerals result from different types of wet conditions.

During the past five years, researchers used OMEGA and NASA's Compact Reconnaissance Imaging
Spectrometer, or CRISM, instrument on the Mars Reconnaissance Orbiter to identify clay minerals at
thousands of locations on Mars. Clay minerals that form where the ratio of water interacting with
rock is small generally retain the same chemical elements as those found in the original volcanic
rocks later altered by the water.

The study interprets this to be the case for most terrains on Mars with iron and magnesium clays. In
contrast, surface environments with higher ratios of water to rock can alter rocks further. Soluble
elements are carried off by water, and different aluminum-rich clays form.

Another clue is detection of a mineral called prehnite. It forms at temperatures above about 400
degrees Fahrenheit (about 200 degrees Celsius). These temperatures are typical of underground
hydrothermal environments rather than surface waters.

"Our interpretation is a shift from thinking that the warm, wet environment was mostly at the surface
to thinking it was mostly in the subsurface, with limited exceptions," said Scott Murchie of Johns
Hopkins University Applied Physics Laboratory in Laurel, Md., a co-author of the report and
principal investigator for CRISM.

One of the exceptions may be Gale Crater, the site targeted by NASA's Mars Science Laboratory
mission. Launching this year, the mission's Curiosity rover will land and investigate layers that
contain clay and sulfate minerals.

NASA's Mars Atmosphere and Volatile Evolution Mission, or MAVEN, in development for a 2013
launch, may provide evidence for or against this new interpretation of the Red Planet's environmental
history. The report predicts MAVEN findings consistent with the atmosphere not having been thick
enough to provide warm, wet surface conditions for a prolonged period.

JPL, a division of Caltech, manages the Mars Reconnaissance Orbiter for NASA's Science Mission
Directorate in Washington. APL provided and operates CRISM. For more information about the
Mars Reconnaissance Orbiter, visit: http://www.nasa.gov/mro and http://mars.jpl.nasa.gov/mro .

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