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Tuesday, August 30, 2011

Jupiter-Bound Space Probe Captures Earth And 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

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 advisory: 2011-271 August 30, 2011

Jupiter-Bound Space Probe Captures Earth And Moon

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-271&cid=release_2011-271

PASADENA, Calif. – On its way to the biggest planet in the solar system -- Jupiter, NASA's Juno
spacecraft took time to capture its home planet and its natural satellite -- the moon.

"This is a remarkable sight people get to see all too rarely," said Scott Bolton, Juno principal
investigator from the Southwest Research Institute in San Antonio. "This view of our planet shows
how Earth looks from the outside, illustrating a special perspective of our role and place in the
universe. We see a humbling yet beautiful view of ourselves."

The image was taken by the spacecraft's camera, JunoCam, on Aug. 26 when the spacecraft was
about 6 million miles (9.66 million kilometers) away. The image was taken as part of the mission
team's checkout of the Juno spacecraft. The team is conducting its initial detailed checks on the
spacecraft's instruments and subsystems after its launch on Aug. 5.

Juno covered the distance from Earth to the moon (about 250,000 miles or 402,000 kilometers) in
less than one day's time. It will take the spacecraft another five years and 1,740 million miles (2,800
million kilometers) to complete the journey to Jupiter. The spacecraft will orbit the planet's poles 33
times and use its eight science instruments to probe beneath the gas giant's obscuring cloud cover to
learn more about its origins, structure, atmosphere and magnetosphere, and look for a potential solid
planetary core.

The solar-powered Juno spacecraft lifted off from Cape Canaveral Air Force Station in Florida at
9:25 a.m. PDT (12:25 p.m. EDT) on Aug. 5 to begin its five-year journey to Jupiter.

JPL manages the Juno mission for the principal investigator, Scott Bolton, of Southwest Research
Institute in San Antonio. The Juno mission is part of the New Frontiers Program managed at NASA's
Marshall Space Flight Center in Huntsville, Ala. Lockheed Martin Space Systems, Denver, built the
spacecraft. JPL is a division of the California Institute of Technology in Pasadena.

More information about Juno is online at http://www.nasa.gov/juno and
http://missionjuno.swri.edu . You can follow the mission on Twitter at
http://www.twitter.com/nasajuno .

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NASA Announces Media Telecon About Opportunity Rover

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

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

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

Advisory: 2011-270 Aug. 30, 2011

NASA Announces Media Telecon About Opportunity Rover

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-270&cid=release_2011-270

PASADENA, Calif. -- NASA will host a media teleconference on Thursday, Sept. 1, at 12:30 p.m.
PDT (3:30 p.m. EDT) to discuss progress of NASA's Mars Exploration Rover Opportunity.
Opportunity reached the Martian Endeavour crater earlier this month after years of driving.

The teleconference participants are:

-- Dave Lavery, program executive, Mars Exploration Rovers, NASA Headquarters, Washington
-- Steve Squyres, principal investigator, Mars Exploration Rovers, Cornell University, Ithaca, N.Y.
-- Ray Arvidson, deputy principal investigator, Mars Exploration Rovers, Washington University in St.
Louis.
-- John Callas, project manager, Mars Exploration Rovers, Jet Propulsion Laboratory, Pasadena, Calif.

Opportunity and its twin, Spirit, completed their three-month prime missions on Mars in April 2004.
They continued to work for years in bonus mission extensions. Spirit finished communicating in 2010,
after six years of operation.

Opportunity, still very active, reached the rim of Endeavour crater on Aug. 9. The arrival gives the
rover access to geology different from any it explored during its first 90 months on Mars.

For live audio streaming of the teleconference, visit http://www.nasa.gov/newsaudio .

For more information about the twin rovers, visit http://www.nasa.gov/rovers and
http://marsrovers.jpl.nasa.gov/ .

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Friday, August 26, 2011

Cassini Closes in on Saturn's Tumbling Moon Hyperion

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

Feature: 2011-266 Aug. 26, 2011

Cassini Closes in on Saturn's Tumbling Moon Hyperion

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-266&cid=release_2011-266

NASA's Cassini spacecraft captured new views of Saturn's oddly shaped moon Hyperion
during its encounter with this cratered body on Thursday, Aug. 25. Raw images were
acquired as the spacecraft flew past the moon at a distance of about 15,500 miles (25,000
kilometers), making this the second closest encounter.

Hyperion is a small moon -- just 168 miles (270 kilometers) across. It has an irregular
shape and surface appearance, and it rotates chaotically as it tumbles along in orbit. This
odd rotation prevented scientists from predicting exactly what terrain the spacecraft's
cameras would image during this flyby.

However, this flyby's closeness has likely allowed Cassini's cameras to map new
territory. At the very least, it will help scientists improve color measurements of the
moon. It will also help them determine how the moon's brightness changes as lighting
and viewing conditions change, which can provide insight into the texture of the surface.
The color measurements provide additional information about different materials on the
moon's deeply pitted surface.

The latest raw images of Hyperion are online at: http://saturn.jpl.nasa.gov/photos/raw/ .

Cassini's closest encounter with Hyperion was on September 26, 2005, when the
spacecraft flew approximately 310 miles (500 kilometers) above the moon's surface.
Cassini's next flyby of Hyperion will be on Sept. 16, 2011, when it passes the tumbling
moon at a distance of about 36,000 miles (58,000 kilometers).

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

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

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Thursday, August 25, 2011

NASA Moon Mission in Final Preparations for September 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

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

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

Caroline McCall 617-253-1682
Massachusetts Institute of Technology, Cambridge
cmcall5@mit.edu

News release: 2011-265 August 25, 2011

NASA Moon Mission in Final Preparations for September Launch

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-265&cid=release_2011-265

CAPE CANAVERAL, Fla. -- NASA's Gravity Recovery And Interior Laboratory (GRAIL) mission
to study the moon is in final launch preparations for a scheduled Sept. 8 launch from Cape Canaveral
Air Force Station in Florida.

GRAIL's twin spacecraft are tasked for a nine-month mission to explore Earth's nearest neighbor in
unprecedented detail. They will determine the structure of the lunar interior from crust to core and
advance our understanding of the thermal evolution of the moon.

"Yesterday's final encapsulation of the spacecraft is an important mission milestone," said David
Lehman, GRAIL project manager for NASA's Jet Propulsion Laboratory in Pasadena, Calif. "Our
two spacecraft are now sitting comfortably inside the payload fairing which will protect them during
ascent. Next time the GRAIL twins will see the light of day, they will be about 95 miles up and
accelerating."

The spacecraft twins, GRAIL-A and GRAIL-B, will fly aboard a Delta II rocket launched from
Florida. The twins' circuitous route to lunar orbit will take 3.5 months and cover approximately 2.6
million miles (4.2 million kilometers) for GRAIL-A, and 2.7 million miles (4.3 million kilometers)
for GRAIL-B.

In lunar orbit, the spacecraft will transmit radio signals precisely defining the distance between them.
Regional gravitational differences on the moon are expected to expand and contract that distance.

GRAIL scientists will use these accurate measurements to define the moon's gravity field. The data
will allow mission scientists to understand what goes on below the surface of our natural satellite.

"GRAIL will unlock lunar mysteries and help us understand how the moon, Earth and other rocky
planets evolved as well," said Maria Zuber, GRAIL principal investigator from the Massachusetts
Institute of Technology in Cambridge.

GRAIL's launch period opens Sept. 8 and extends through Oct. 19. On each day, there are two
separate launch opportunities separated by approximately 39 minutes. On Sept. 8, the first launch
opportunity is 8:37 a.m. EDT (5:37 a.m. PDT); the second is 9:16 a.m. EDT (6:16 a.m. PDT).

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the GRAIL mission. The
Massachusetts Institute of Technology, Cambridge, is home to the mission's principal investigator,
Maria Zuber. The GRAIL mission is part of the Discovery Program managed at NASA's Marshall
Space Flight Center in Huntsville, Ala. Lockheed Martin Space Systems, Denver, built the spacecraft.
Launch management for the mission is the responsibility of NASA's Launch Services Program at the
Kennedy Space Center in Florida. JPL is a division of the California Institute of Technology in
Pasadena.

For extensive pre-launch and launch day coverage of the GRAIL spacecraft, visit:
http://www.nasa.gov .

A prelaunch webcast for the mission will be streamed at noon on Wednesday, Sept. 7. Live
countdown coverage through NASA's Launch Blog begins at 6:30 a.m. EDT (3:30 am PDT) on Sept.
8. Coverage features live updates as countdown milestones occur and streaming video clips
highlighting launch preparations and liftoff.

To view the webcast and the blog or to learn more about the GRAIL mission, visit:
http://www.nasa.gov/grail and http://grail.nasa.gov .

The launch will also be streamed live, with a chat available, on http://www.ustream.tv/nasajpl2 .

To view live interviews with lunar scientists from noon to 5 p.m. EDT (2 p.m. PDT) on Sept. 8 and 9,
visit: http://www.livestream.com/grail .

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Wednesday, August 24, 2011

Register for the NASA NPP Educator Launch Conference

Professional Development Aug. 24, 2011

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

NASA NPP Educator Launch Conference

Date: Monday and Tuesday, Oct. 24-25, 2011

Target audience: K-12 educators and administrators

Location: Allan Hancock College's Lompoc Valley Center, 1 Hancock Drive, Lompoc, Calif. 93436

Overview: Witness the launch of NASA's next-generation weather and Earth science mission as part of NASA's NPOESS Preparatory Project (NPP), and learn about real-world Earth, atmospheric and rocket science, as well as NPP's cutting-edge satellite instrument technology.

This educational program will provide a personal tour of the NASA Mission Director Center, close-up viewing of the powerful Delta II launch vehicle on the launch pad, as well as hands-on practical educator workshops and presentations by NASA and NOAA principal investigators and other practitioners. Participants will also have the opportunity to enjoy a delicious dinner at the Vandenberg Air Force Base Officers' Club while meeting with many formal and informal STEM educators, scientists and engineers.

The NPP mission will help link the current generation of Earth-observing satellites called the Earth Observing System (EOS) to a next-generation of operational polar-orbiting environmental satellites called the Joint Polar Satellite System (JPSS), managed by the National Oceanic and Atmospheric Administration (NOAA). NPP's data products will help meteorologists improve weather forecasts and advance Earth and climate science. The remote-sensing instruments aboard NPP will measure the Earth's atmospheric and sea surface temperatures, humidity and pressure profiles, land and ocean biological activity and cloud and aerosol properties. NOAA meteorologists will incorporate the data into their weather and climate prediction models to produce accurate, life-saving forecasts and warnings.

For more information on the NPP program and uses in the classroom go to: http://npp.gsfc.nasa.gov/nppy.html . General NPP program information can be found at: http://npp.gsfc.nasa.gov/ .

For more information about the conference and to register online, visit http://endeavourinstitute.org/launch .

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NASA's Wise Mission Discovers Coolest Class of Stars

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

Trent Perrotto 202-358-0321
Headquarters, Washington
Trent.j.perrotto@nasa.gov

News release: 2011-263 Aug. 23, 2011

NASA'S Wise Mission Discovers Coolest Class of Stars

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-263&cid=release_2011-263

PASADENA, Calif. – Scientists using data from NASA's Wide-field Infrared Survey Explorer
(WISE) have discovered the coldest class of star-like bodies, with temperatures as cool as the
human body.

Astronomers hunted these dark orbs, termed Y dwarfs, for more than a decade without success.
When viewed with a visible-light telescope, they are nearly impossible to see. WISE's infrared
vision allowed the telescope to finally spot the faint glow of six Y dwarfs relatively close to our
sun, within a distance of about 40 light-years.

"WISE scanned the entire sky for these and other objects, and was able to spot their feeble light
with its highly sensitive infrared vision," said Jon Morse, Astrophysics Division director at
NASA Headquarters in Washington. "They are 5,000 times brighter at the longer infrared
wavelengths WISE observed from space than those observable from the ground."

The Y's are the coldest members of the brown dwarf family. Brown dwarfs are sometimes
referred to as "failed" stars. They are too low in mass to fuse atoms at their cores and thus don't
burn with the fires that keep stars like our sun shining steadily for billions of years. Instead, these
objects cool and fade with time, until what little light they do emit is at infrared wavelengths.

Astronomers study brown dwarfs to better understand how stars form, and to understand the
atmospheres of planets beyond our solar system. The atmospheres of brown dwarfs are similar to
those of gas-giant planets like Jupiter, but they are easier to observe because they are alone in
space, away from the blinding light of a parent star.

So far, WISE data have revealed 100 new brown dwarfs. More discoveries are expected as
scientists continue to examine the enormous quantity of data from WISE. The telescope
performed the most advanced survey of the sky at infrared wavelengths to date, from Jan. 2010
to Feb. 2011, scanning the entire sky about 1.5 times.

Of the 100 brown dwarfs, six are classified as cool Y's. One of the Y dwarfs, called WISE
1828+2650, is the record holder for the coldest brown dwarf, with an estimated atmospheric
temperature cooler than room temperature, or less than about 80 degrees Fahrenheit (25 degrees
Celsius).

"The brown dwarfs we were turning up before this discovery were more like the temperature of
your oven," said Davy Kirkpatrick, a WISE science team member at the Infrared Processing and
Analysis Center at the California Institute of Technology in Pasadena, Calif. "With the discovery
of Y dwarfs, we've moved out of the kitchen and into the cooler parts of the house."

Kirkpatrick is lead author of a paper appearing in the Astrophysical Journal Supplement Series,
describing the 100 confirmed brown dwarfs. Michael Cushing, a WISE team member at NASA's
Jet Propulsion Laboratory in Pasadena, Calif., is lead author of a paper describing the Y dwarfs
in the Astrophysical Journal.

The Y dwarfs are in our sun's neighborhood, from approximately nine to 40 light-years away.
The Y dwarf approximately nine light-years away, WISE 1541-2250, may become the seventh
closest star system, bumping Ross 154 back to eighth. By comparison, the star closest to our
solar system, Proxima Centauri, is about four light-years away.

"Finding brown dwarfs near our sun is like discovering there's a hidden house on your block that
you didn't know about," Cushing said. "It's thrilling to me to know we've got neighbors out there
yet to be discovered. With WISE, we may even find a brown dwarf closer to us than our closest
known star."

Once the WISE team identified brown dwarf candidates, they turned to NASA's Spitzer Space
Telescope to narrow their list. To definitively confirm them, the WISE team used some of the
most powerful telescopes on Earth to split apart the objects' light and look for telltale molecular
signatures of water, methane and possibly ammonia. For the very coldest of the new Y dwarfs,
the team used NASA's Hubble Space Telescope. The Y dwarfs were identified based on a change
in these spectral features compared to other brown dwarfs, indicating they have a lower
atmospheric temperature.

The ground-based telescopes used in these studies include the NASA Infrared Telescope Facility
atop Mauna Kea, Hawaii; Caltech's Palomar Observatory near San Diego; the W.M. Keck
Observatory atop Mauna Kea, Hawaii; and the Magellan Telescopes at Las Campanas
Observatory, Chile, among others.

JPL manages WISE for NASA's Science Mission Directorate. The principal investigator is
Edward Wright at UCLA. The WISE satellite was decommissioned in 2011 after completing its
sky survey observations. The mission was selected under NASA's Explorers Program managed
by the Goddard Space Flight Center in Greenbelt, Md. The science instrument was built by the
Space Dynamics Laboratory in Logan, Utah, and the spacecraft by Ball Aerospace &
Technologies Corp., in Boulder, Colo. Science operations and data processing are at the Infrared
Processing and Analysis Center at the California Institute of Technology. JPL is a division of the
California Institute of Technology in Pasadena.

More information is online at http://www.nasa.gov/wise , http://wise.astro.ucla.edu and
http://jpl.nasa.gov/wise .

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NASA Sets GRAIL/DELTA II Launch Coverage Events

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

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

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

Advisory: 2011-264 Aug. 24, 2011

NASA Sets GRAIL/DELTA II Launch Coverage Events

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-264&cid=release_2011-264

CAPE CANAVERAL, Fla. -- NASA's GRAIL spacecraft is set to launch to the moon aboard a
United Launch Alliance Delta II rocket on Sept. 8, 2011, from Cape Canaveral Air Force Station,
Fla. There are two instantaneous (one-second) launch windows at 8:37:06 a.m. and 9:16:12 a.m.
EDT (5:37:06 a.m. and 6:16:12 a.m. EDT). The launch period extends through Oct. 19. The launch
times occur approximately 4 minutes earlier each day.

GRAIL's primary science objectives are to determine the structure of the lunar interior, from crust
to core, and to advance understanding of the thermal evolution of the moon.

GRAIL Prelaunch News Conference

A prelaunch news conference will be held at NASA Kennedy Space Center's Press Site on Sept. 6,
at 1 p.m. EDT (10 a.m. PDT). Participating in the briefing will be:

Ed Weiler, associate administrator, Science Mission Directorate
NASA Headquarters, Washington

Tim Dunn, NASA launch director
NASA's Kennedy Space Center, Cape Canaveral, Fla.

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

David Lehman, GRAIL project manager
Jet Propulsion Laboratory, Pasadena, Calif

John Henk, GRAIL program manager
Lockheed Martin Space Systems, Denver

Joel Tumbiolo, launch weather officer
45th Weather Squadron, Cape Canaveral Air Force Station, Fla.

GRAIL Mission Science Briefing

A GRAIL mission science briefing will be held at Kennedy's Press Site on Sept. 7 at 10 a.m. EDT
(7 a.m. PDT). Participating in the briefing will be:

Robert Fogel, GRAIL program scientist
NASA Headquarters, Washington

Maria Zuber, GRAIL principal investigator
Massachusetts Institute of Technology, Cambridge

Sami Asmar, GRAIL deputy project scientist
Jet Propulsion Laboratory, Pasadena, Calif.

Sally Ride, president and CEO
Sally Ride Science, San Diego

A post-launch news conference will be held at Kennedy's Press Site at a time to be determined after
launch.


NASA Television Coverage

NASA Television will carry the GRAIL prelaunch news conference beginning at 1 p.m. EDT (10
a.m. PDT) on Sept. 6 and the GRAIL mission science briefing on Sept. 7 at 10 a.m. EDT (7 a.m.
PDT).

On Sept. 8, NASA Television coverage of the launch will begin at 6 a.m. EDT (3 a.m. PDT) and
conclude after spacecraft separation from the Delta II has occurred about one hour after launch.
Live launch coverage will be carried on all NASA Television channels and on the agency's website.

A post-launch news conference will be held at Kennedy's Press Site at a time to be determined after
launch.

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

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

NASA Web prelaunch and launch coverage

Extensive prelaunch and launch day coverage of the liftoff of the GRAIL spacecraft aboard the
Delta II rocket will be available on NASA's home page on the Internet at:
http://www.nasa.gov .

A prelaunch webcast for the GRAIL mission will be streamed on the Web on Sept. 7, at noon. Live
countdown coverage through NASA's Launch Blog begins at 6:30 a.m. EDT (3:30 a.m. PDT) on
Sept. 8. 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 the GRAIL mission, visit:
http://www.nasa.gov/grail or http://grail.nasa.gov .

The news conferences and launch coverage will be streamed live, with a chat available, at:
http://www.ustream.tv/nasajpl2 .

Twitter

The NASA News Twitter feed will be updated throughout the launch countdown. To access the
NASA News Twitter feed, visit: http://www.twitter.com/nasa .

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the GRAIL mission for the principal
investigator, Maria Zuber, of the Massachusetts Institute of Technology in Cambridge, Mass. The
GRAIL mission is part of the New Frontiers Program managed at NASA's Marshall Space Flight
Center in Huntsville, Ala. Lockheed Martin Space Systems, Denver, built the spacecraft. Launch
management for the mission is the responsibility of NASA's Launch Services Program at the
Kennedy Space Center in Florida. JPL is a division of the California Institute of Technology in
Pasadena.

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Tuesday, August 23, 2011

NASA Satellites Detect Pothole on Road to Higher Seas

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

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

Feature: 2011-262 Aug. 23, 2011

An Update from NASA's Sea Level Sentinels:
NASA Satellites Detect Pothole on Road to Higher Seas

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-262&cid=release_2011-262

Like mercury in a thermometer, ocean waters expand as they warm. This, along with melting
glaciers and ice sheets in Greenland and Antarctica, drives sea levels higher over the long term.
For the past 18 years, the U.S./French Jason-1, Jason-2 and Topex/Poseidon spacecraft have
been monitoring the gradual rise of the world's ocean in response to global warming.

While the rise of the global ocean has been remarkably steady for most of this time, every once
in a while, sea level rise hits a speed bump. This past year, it's been more like a pothole: between
last summer and this one, global sea level actually fell by about a quarter of an inch, or half a
centimeter.

So what's up with the down seas, and what does it mean? Climate scientist Josh Willis of
NASA's Jet Propulsion Laboratory, Pasadena, Calif., says you can blame it on the cycle of El
Niño and La Niña in the Pacific.

Willis said that while 2010 began with a sizable El Niño, by year's end, it was replaced by one of
the strongest La Niñas in recent memory. This sudden shift in the Pacific changed rainfall
patterns all across the globe, bringing massive floods to places like Australia and the Amazon
basin, and drought to the southern United States.

Data from the NASA/German Aerospace Center's twin Gravity Recovery and Climate
Experiment (Grace) spacecraft provide a clear picture of how this extra rain piled onto the
continents in the early parts of 2011. "By detecting where water is on the continents, Grace
shows us how water moves around the planet," says Steve Nerem, a sea level scientist at the
University of Colorado in Boulder.

So where does all that extra water in Brazil and Australia come from? You guessed it--the
ocean. Each year, huge amounts of water are evaporated from the ocean. While most of it falls
right back into the ocean as rain, some of it falls over land. "This year, the continents got an extra
dose of rain, so much so that global sea levels actually fell over most of the last year," says
Carmen Boening, a JPL oceanographer and climate scientist. Boening and colleagues presented
these results recently at the annual Grace Science Team Meeting in Austin, Texas.

But for those who might argue that these data show us entering a long-term period of decline in
global sea level, Willis cautions that sea level drops such as this one cannot last, and over the
long-run, the trend remains solidly up. Water flows downhill, and the extra rain will eventually
find its way back to the sea. When it does, global sea level will rise again.

"We're heating up the planet, and in the end that means more sea level rise," says Willis. "But El
Niño and La Niña always take us on a rainfall rollercoaster, and in years like this they give us
sea-level whiplash."

For more information on NASA's sea level monitoring satellites, visit:
http://sealevel.jpl.nasa.gov/ , http://sealevel.colorado.edu , http://www.csr.utexas.edu/grace/ and
http://grace.jpl.nasa.gov/ .

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Monday, August 22, 2011

NASA Picks Three Proposals for Flight Demonstration

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

Priscilla Vega/Jane Platt 818-354-5011
Jet Propulsion Laboratory, Pasadena, Calif.
Priscilla.r.vega@jpl.nasa.gov / jane.platt@jpl.nasa.gov

David E. Steitz 202-358-1730
NASA Headquarters, Washington
david.steitz@nasa.gov

News release: 2011-261 Aug. 22, 2011

NASA Picks Three Proposals for Flight Demonstration


The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-261&cid=release_2011-261

PASADENA, Calif. -- NASA has selected three proposals, including one from NASA's
Jet Propulsion Laboratory in Pasadena, Calif., as Technology Demonstration Missions to
transform space communications, deep space navigation and in-space propulsion
capabilities. The projects will develop and fly a space solar sail, deep space atomic clock,
and space-based optical communications system.

These crosscutting flight demonstrations were selected because of their potential to
provide tangible, near-term products and infuse high-impact capabilities into NASA's
future space operations missions. By investing in high payoff, disruptive technology that
industry does not have today, NASA matures the technology required for its future
missions while proving the capabilities and lowering the cost of government and
commercial space activities.

"These technology demonstration missions will improve our communications, navigation
and in-space propulsion capabilities, enable future missions that could not otherwise be
performed, and build the technological capability of America's space industry," said
NASA Chief Technologist Bobby Braun at NASA Headquarters in Washington. "Optical
communication will enable rapid return of the voluminous data associated with sending
spacecraft and humans to new frontiers. High-performance atomic clocks enable a level
of spacecraft navigation precision and autonomous operations in deep space never before
achieved, and solar sails enable new space missions through highly efficient station-
keeping or propellant-less main propulsion capabilities for spacecraft."

The proposals selected for demonstration missions are:
-- Laser Communications Relay Demonstration, David J. Israel, principal investigator at
NASA's Goddard Space Flight Center in Greenbelt, Md.
-- Deep Space Atomic Clock, Todd Ely, principal investigator at the California Institute
of Technology/NASA's Jet Propulsion Laboratory in Pasadena, Calif.
-- Beyond the Plum Brook Chamber; An In-Space Demonstration of a Mission-Capable
Solar Sail, Nathan Barnes, principal investigator at L'Garde Inc., of Tustin, Calif.

Technology Demonstration Missions are a vital element in NASA's space technology
maturation pipeline. They prove feasibility in the environment of space and help advance
innovations from concept to flight and use in missions. The advances anticipated from
communications, navigation and in-space propulsion technology will allow future NASA
missions to pursue bolder and more sophisticated science, enable human missions beyond
low Earth orbit, and enable entirely new approaches to U.S. space operations.

The Laser Communications Relay demonstration mission will fly and validate a reliable,
capable, and cost-effective optical communications technology. Optical communications
technology provides data rates up to 100 times higher than today's systems, which will be
needed for future human and robotic space missions. The technology is directly
applicable to the next generation of NASA's space communications network. After the
demonstration, the developed space and ground assets will be qualified for use by near-
Earth and deep space missions requiring high bandwidth and a small ground station
reception area.

The Deep Space Atomic Clock demonstration mission will fly and validate a
miniaturized mercury-ion atomic clock that is 10-times more accurate than today's
systems. This project will demonstrate ultra-precision timing in space and its benefits for
one-way radio navigation. The investigation will fly as a hosted payload on an Iridium
spacecraft and make use of GPS signals to demonstrate precision orbit determination and
confirm the clock's performance. Precision timing and navigation is critical to the
performance of a wide range of deep space exploration missions.

The Solar Sail demonstration mission will deploy and operate a sail area 7 times larger
than ever flown in space. It is potentially applicable to a wide range of future space
missions, including an advanced space weather warning system to provide more timely
and accurate notice of solar flare activity. This technology also could be applied to
economical orbital debris removal and propellant-less deep space exploration missions.
The National Oceanic and Atmospheric Administration is collaborating with NASA and
L'Garde Inc. on the demonstration.

The clock and solar sail will be ready for flight in three years. The optical
communications team anticipates it will take four years to mature the technology for
flight. NASA's Office of the Chief Technologist plans to make a total investment in these
three missions of approximately $175 million, contingent on future appropriations. Each
of the selected teams also will receive funding from partners who plan on using the
technologies as part of future space missions.

Projects include all elements of the flight test demonstration including test planning,
flight hardware, launch, ground operations, and post-testing assessment and reporting.
Each team has proposed between one and two years of spaceflight operations and data
analysis. To reduce cost, the technology demonstrations will ride to space with other
payloads aboard commercially provided launch vehicles. Launches are anticipated in
2015 and 2016.

The Technology Demonstration Missions program is managed by NASA's Office of the
Chief Technologist. For more information about the program, visit:
http://www.nasa.gov/oct .

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

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NASA Hosts News Conference on Upcoming Moon Mission

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

Advisory: 2011-259 Aug. 22, 2011

NASA Hosts News Conference on Upcoming Moon Mission

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-260&cid=release_2011-260

WASHINGTON -- NASA will host a news conference at 11 a.m. EDT (8 a.m. PDT), on Thursday
Aug. 25, to discuss the upcoming launch of the Gravity Recovery And Interior Laboratory (GRAIL)
mission. Scheduled to launch Sept. 8, GRAIL will help answer longstanding questions about Earth's
moon and provide a better understanding of how Earth and other rocky planets in our solar system
formed.

The event will take place at NASA Headquarters in Washington. It will air live on NASA Television
and the agency's website.

The news conference panelists are:
-- Jim Green, director, Planetary Science Division, NASA Headquarters, Washington
-- Maria Zuber, GRAIL principal investigator, Massachusetts Institute of Technology, Cambridge
-- David Lehman, GRAIL project manager, NASA's Jet Propulsion Laboratory, Pasadena, Calif.
-- Leesa Hubbard, teacher in residence, Sally Ride Science, San Diego

The news conference will also be streamed live, with a chat available, at:
http://www.ustream.tv/nasajpl2 .

For more information about the GRAIL mission, visit: http://www.nasa.gov/grail and
http://grail.nasa.gov .

NASA TV streaming video, downlink and scheduling information is at: http://www.nasa.gov/ntv .

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Thursday, August 18, 2011

Webb Telescope Instrument Completes Cryogenic Testing

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: 2011-258 Aug. 18, 2011

Webb Telescope Instrument Completes Cryogenic Testing

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-258&cid=release_2011-258

A pioneering camera and spectrometer that will fly aboard NASA's James Webb Space Telescope
has completed cryogenic testing designed to mimic the harsh conditions it will experience in space.

The Mid-Infrared Instrument (MIRI) underwent testing inside the thermal space test chamber at the
Science and Technology Facilities Council's Rutherford Appleton Laboratory Space in Oxfordshire,
U.K. The sophisticated instrument is designed to examine the first light in the universe and the
formation of planets around other stars.

A team of more than 50 scientists from 11 countries tested MIRI for 86 days, representing the
longest and most exhaustive testing at cryogenic temperatures of an astronomy instrument in Europe
prior to delivery for its integration into a spacecraft.

"The successful completion of the test program, involving more than 2,000 individual tests, marks a
major milestone for the Webb telescope mission," said Matthew Greenhouse, Webb telescope
project scientist for the Science Instrument Payload, at NASA's Goddard Space Flight Center in
Greenbelt, Md.

Along with the Webb telescope's other instruments, MIRI will help scientists better understand how
the universe formed following the Big Bang and ultimately developed star systems that may be
capable of supporting life. In particular, scientists hope to explore young planets around distant stars
that are shrouded by gas and dust when viewed in visible light. Because infrared light penetrates
these obstructions, MIRI can acquire images of planetary nurseries sharper than ever before
possible. With its spectrometer, MIRI could potentially reveal the existence of water on these planets
as well, informing future investigations into their habitability for humans.

To capture some of the earliest, infrared light in the cosmos, MIRI has to be cooled to 7 Kelvin
(minus 266 Celsius, or minus 447 Fahrenheit), which brings tough challenges for testing the
instrument. Inside the RAL Space thermal space test chamber, specially constructed shrouds, cooled
to 40 Kelvin (minus 233 Celsius, or minus 388 Fahrenheit), surround MIRI while scientists observe
simulated background stars. The tests were designed to ensure that MIRI can operate successfully in
the cold vacuum of space and allow scientists to gather vital calibration and baseline data.

The MIRI team is now analyzing data from the cryogenic test campaign, completing remaining
"warm testing," and will prepare the instrument for delivery to NASA Goddard. There it will be
integrated with the other instruments, and the telescope.

"Thousands of astronomers will use the Webb telescope to extend the reach of human knowledge far
beyond today's limits. Just as the Hubble Space Telescope rewrote textbooks everywhere, Webb will
find new surprises and help to answer some of the most pressing questions in astronomy," said John
Mather, Nobel laureate and Webb senior project scientist at NASA Goddard.

MIRI was built by scientists and engineers from European countries, NASA's Jet Propulsion
Laboratory in Pasadena, Calif., and several U.S. institutions. Its focal plane modules, related
electronics and software were built at JPL. The instrument's cooler is being built by Northrop
Grumman Space Technologies in Redondo Beach, Calif., and managed by JPL.

The Webb telescope is a partnership between NASA, the European Space Agency and the Canadian
Space Agency.

For more information about MIRI, visit http://www.jwst.nasa.gov/miri.html . For more
information about the Webb telescope, visit http://jwst.nasa.gov .

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NASA Research Yields Full Map of Antarctic Ice Flow

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

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

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

News release: 2011-256 Aug. 18, 2011

NASA Research Yields Full Map of Antarctic Ice Flow

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-256&cid=release_2011-256

PASADENA, Calif. – NASA-funded researchers have created the first complete map of the speed
and direction of ice flow in Antarctica. The map, which shows glaciers flowing thousands of miles
from the continent's deep interior to its coast, will be critical for tracking future sea-level increases
from climate change. The team created the map using integrated radar observations from a
consortium of international satellites.

"This is like seeing a map of all the oceans' currents for the first time. It's a game changer for
glaciology," said Eric Rignot of NASA's Jet Propulsion Laboratory in Pasadena, Calif., and the
University of California (UC), Irvine. Rignot is lead author of a paper about the ice flow published
online Thursday in Science Express. "We are seeing amazing flows from the heart of the continent
that had never been described before."

Rignot and UC Irvine scientists Jeremie Mouginot and Bernd Scheuchl used billions of data points
captured by European, Japanese and Canadian satellites to weed out cloud cover, solar glare and land
features masking the glaciers. With the aid of NASA technology, the team painstakingly pieced
together the shape and velocity of glacial formations, including the previously uncharted East
Antarctica, which comprises 77 percent of the continent.

Like viewers of a completed jigsaw puzzle, the scientists were surprised when they stood back and
took in the full picture. They discovered a new ridge splitting the 5.4 million-square-mile (14 million-
square-kilometer) landmass from east to west.

The team also found unnamed formations moving up to 800 feet (244 meters) annually across
immense plains sloping toward the Antarctic Ocean and in a different manner than past models of ice
migration.

"The map points out something fundamentally new: that ice moves by slipping along the ground it
rests on," said Thomas Wagner, NASA's cryospheric program scientist in Washington. "That's
critical knowledge for predicting future sea level rise. It means that if we lose ice at the coasts from
the warming ocean, we open the tap to massive amounts of ice in the interior."

The work was conducted in conjunction with the International Polar Year (IPY) (2007-2008).
Collaborators worked under the IPY Space Task Group, which included NASA; the European Space
Agency (ESA); Canadian Space Agency (CSA); Japan Aerospace Exploration Agency; the Alaska
Satellite Facility in Fairbanks; and MacDonald, Dettwiler and Associates of Richmond, British
Columbia, Canada. The map builds on partial charts of Antarctic ice flow created by NASA, CSA
and ESA using different techniques.

"To our knowledge, this is the first time that a tightly knit collaboration of civilian space agencies has
worked together to create such a huge dataset of this type," said Yves Crevier of CSA. "It is a dataset
of lasting scientific value in assessing the extent and rate of change in polar regions."

For a video animation of the new Antarctic map, visit: http://1.usa.gov/poJq1P .

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

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

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CORRECTED: NASA's GRAIL Moon Twins are Joined to Their Booster

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

Tracy Young 321-867-9284
Kennedy Space Center, Fla.
tracy.g.young@nasa.gov

News release: 2011-257 August 18, 2011

NASA's GRAIL Moon Twins are Joined to Their Booster

NOTE: Includes corrected launch vehicle name and date/timing information.

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-257&cid=release_2011-257

CAPE CANAVERAL, Fla. -- NASA's lunar-bound GRAIL twins were mated to their Delta II
launch vehicle at the Cape Canaveral Air Force Station's Launch Complex 17 at 8:45 a.m. EDT
(5:45 a.m. PDT) today. The 15-mile (25-kilometer) trip from Astrotech Space Operations in
Titusville, Fla., is the last move for GRAIL before it begins its journey to the moon. NASA's
dynamic duo will orbit the moon to determine the structure of the lunar interior from crust to
core and to advance understanding of the thermal evolution of the moon.

"We are about to finish one chapter in the GRAIL story and open another," said Maria Zuber,
GRAIL's principal investigator, based at the Massachusetts Institute of Technology in
Cambridge. "Let me assure you this one is a real page-turner. GRAIL will rewrite the book on the
formation of the moon and the beginning of us."

Now that the GRAIL spacecraft are atop their rocket, a final flurry of checks and tests can begin
to confirm that all is go for launch. The final series of checks begins tomorrow, Aug. 19, with an
on-pad functional test. The test is designed to confirm that the spacecraft is healthy after the
fueling and transport operations. Next week, among all the upcoming final tests, reviews and
closeout operations leading up to liftoff, the GRAIL team will install the launch vehicle fairing
around the spacecraft.

GRAIL's launch period opens Sept. 8 and extends through Oct. 19. On each day, there are two
separate instantaneous launch opportunities separated in time by approximately 39 minutes. On
Sept. 8, the first launch opportunity is at 8:37 a.m. EDT (5:37 a.m. PDT). The second launch
opportunity is 9:16 a.m. EDT (6:16 a.m. PDT).

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the GRAIL mission. The
Massachusetts Institute of Technology, Cambridge, is home to the mission's principal
investigator, Maria Zuber. The GRAIL mission is part of the Discovery Program managed at
NASA's Marshall Space Flight Center in Huntsville, Ala. Lockheed Martin Space Systems,
Denver, built the spacecraft. Launch management for the mission is the responsibility of NASA's
Launch Services Program at the Kennedy Space Center in Florida. JPL is a division of the
California Institute of Technology in Pasadena.

More information about GRAIL is online at: http://www.nasa.gov/grail .

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NASA's GRAIL Moon Twins are Joined to Their Booster

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

Tracy Young 321-867-9284
Kennedy Space Center, Fla.
tracy.g.young@nasa.gov

News release: 2011-257 August 18, 2011

NASA's GRAIL Moon Twins are Joined to Their Booster

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-257&cid=release_2011-257

CAPE CANAVERAL, Fla. -- NASA's lunar-bound GRAIL twins were mated to their Titan II
launch vehicle at the Cape Canaveral Air Force Station's Launch Complex 17 at 8:19 a.m. EDT
(5:19 a.m. PDT) yesterday. The 15-mile (25-kilometer) trip from Astrotech Space Operations in
Titusville, Fla., is the last move for GRAIL before it begins its journey to the moon. NASA's
dynamic duo will orbit the moon to determine the structure of the lunar interior from crust to
core and to advance understanding of the thermal evolution of the moon.

"We are about to finish one chapter in the GRAIL story and open another," said Maria Zuber,
GRAIL's principal investigator, based at the Massachusetts Institute of Technology in
Cambridge. "Let me assure you this one is a real page-turner. GRAIL will rewrite the book on
the formation of the moon and the beginning of us."

Now that the GRAIL spacecraft are atop their rocket, a final flurry of checks and tests can begin
to confirm that all is go for launch. The final series of checks begins tomorrow, Aug. 19, with an
on-pad functional test. The test is designed to confirm that the spacecraft is healthy after the
fueling and transport operations. Next week, among all the upcoming final tests, reviews and
closeout operations leading up to liftoff, the GRAIL team will install the launch vehicle fairing
around the spacecraft.

GRAIL's launch period opens Sept. 8, 2011, and extends through Oct. 19. For a Sept. 8 liftoff,
the launch window opens at 8:37 a.m. EDT (5:37 a.m. PDT) and remains open through 9:16 a.m.
EDT (6:16 a.m. PDT).

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the GRAIL mission. The
Massachusetts Institute of Technology, Cambridge, is home to the mission's principal
investigator, Maria Zuber. The GRAIL mission is part of the Discovery Program managed at
NASA's Marshall Space Flight Center in Huntsville, Ala. Lockheed Martin Space Systems,
Denver, built the spacecraft. Launch management for the mission is the responsibility of NASA's
Launch Services Program at the Kennedy Space Center in Florida. JPL is a division of the
California Institute of Technology in Pasadena.

More information about GRAIL is online at: http://www.nasa.gov/grail .

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Tuesday, August 16, 2011

Comet Elenin Poses No Threat to Earth

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

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

News Release: 2011-255 Aug. 16, 2011

Comet Elenin Poses No Threat to Earth

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-255&cid=release_2011-255

Often, comets are portrayed as harbingers of gloom and doom in movies and on
television, but most pose no threat to Earth. Comet Elenin, the latest comet to visit our
inner solar system, is no exception. Elenin will pass about 22 million miles (35 million
kilometers) from Earth during its closest approach on Oct. 16, 2011.

Also known by its astronomical name C/2010 X1, the comet was first detected on Dec.
10, 2010 by Leonid Elenin, an observer in Lyubertsy, Russia, who made the discovery
"remotely" using an observatory in New Mexico. At that time, Elenin was about 401
million miles (647 million kilometers) from Earth. Since its discovery, Comet Elenin
has – as all comets do – closed the distance to Earth's vicinity as it makes its way
closer to perihelion, its closest point to the sun.

NASA scientists have taken time over the last several months to answer your
questions. Compiled below are the some of the most popular questions, with answers
from Don Yeomans of NASA's Near-Earth Object Program Office at NASA's Jet
Propulsion Laboratory in Pasadena, Calif., and David Morrison of the NASA
Astrobiology Institute at the NASA Ames Research Center in Moffett Field, Calif.

Most Popular Questions About Comet Elenin

When will Comet Elenin come closest to the Earth and appear the brightest?

Comet Elenin should be at its brightest shortly before the time of its closest approach to
Earth on Oct. 16, 2011. At its closest point, it will be 22 million miles (35 million
kilometers) from us.

Will Comet Elenin come close to the Earth or between the Earth and the moon?

Comet Elenin will not come closer to Earth than 22 million miles (35 million
kilometers). That's more than 90 times the distance to the moon.

Can this comet influence us from where it is, or where it will be in the future? Can
this celestial object cause shifting of the tides or even tectonic plates here on
Earth?

There have been incorrect speculations on the Internet that alignments of comet
Elenin with other celestial bodies could cause consequences for Earth and external
forces could cause comet Elenin to come closer. "Any approximate alignments of
comet Elenin with other celestial bodies are meaningless, and the comet will not
encounter any dark bodies that could perturb its orbit, nor will it influence us in any
way here on Earth," said Don Yeomans, a scientist at NASA JPL.

"Comet Elenin will not only be far away, it is also on the small side for comets," said
Yeomans. "And comets are not the most densely-packed objects out there. They
usually have the density of something akin to loosely packed icy dirt.

"So you've got a modest-sized icy dirtball that is getting no closer than 35 million
kilometers [about 22 million miles)," said Yeomans. "It will have an immeasurably
miniscule influence on our planet. By comparison, my subcompact automobile exerts
a greater influence on the ocean's tides than comet Elenin ever will."

I've heard about three days of darkness because of Comet Elenin. Will Elenin
block out the sun for three days?

"As seen from the Earth, comet Elenin will not cross the sun's face," says Yeomans.

But even if it could cross the sun, which it can't, astrobiologist David Morrison notes
that comet Elenin is about 2-3 miles (3-5 kilometers) wide, while the sun is roughly
865,000 miles (1,392,082 kilometers) across. How could such a small object block the
sun, which is such a large object?

Let's think about an eclipse of the sun, which happens when the moon appears
between the Earth and the sun. The moon is about 2,500 miles (4,000 kilometers) in
diameter, and has the same apparent size as the sun when it is about 250,000 miles
(400,000 kilometers) away -- roughly 100 times its own diameter. For a comet with a
diameter of about 2-3 miles (3-5 kilometers) to cover the sun it would have to be within
250 miles (400 kilometers), roughly the orbital altitude of the International Space
Station. However, as stated above, this comet will come no closer to Earth than 22
million miles.

I've heard there is a "brown dwarf" theory about Comet Elenin. Would its mass be
enough to pull Comet Honda's trajectory a significant amount? Could this be used
to determine the mass of Elenin?

Morrison says that there is no 'brown dwarf theory' of this comet. "A comet is nothing
like a brown dwarf. You are correct that the way astronomers measure the mass of one
object is by its gravitational effect on another, but comets are far too small to have a
measureable influence on anything."

If we had a black or brown dwarf in our outer solar system, I guess no one could
see it, right?

"No, that's not correct," says Morrison. "If we had a brown dwarf star in the outer solar
system, we could see it, detect its infrared energy and measure its perturbing effect on
other objects. There is no brown dwarf in the solar system, otherwise we would have
detected it. And there is no such thing as a black dwarf."

Will Comet Elenin be visible to the naked eye when it's closer to us? I missed Hale-
Bopp's passing, so I want to know if we'll actually be able to see something in the
sky when Elenin passes.

We don't know yet if Comet Elenin will be visible to the naked eye. Morrison says, "At
the rate it is going, seeing the comet at its best in early October will require binoculars
and a very dark sky. Unfortunately, Elenin is no substitute for seeing comet Hale-Bopp,
which was the brightest comet of the past several decades."

"This comet may not put on a great show. Just as certainly, it will not cause any
disruptions here on Earth. But, there is a cause to marvel," said Yeomans. "This
intrepid little traveler will offer astronomers a chance to study a relatively young comet
that came here from well beyond our solar system's planetary region. After a short
while, it will be headed back out again, and we will not see or hear from Elenin for
thousands of years. That's pretty cool."

This comet has been called 'wimpy' by NASA scientists. Why?

"We're talking about how a comet looks as it safely flies past us," said Yeomans of
NASA's Near-Earth Object Program Office. "Some cometary visitors arriving from
beyond the planetary region – like Hale-Bopp in 1997 -- have really lit up the night sky
where you can see them easily with the naked eye as they safely transit the inner-solar
system. But Elenin is trending toward the other end of the spectrum. You'll probably
need a good pair of binoculars, clear skies and a dark, secluded location to see it even
on its brightest night."

Why aren't you talking more about Comet Elenin? If these things are small and
nothing to worry about, why has there been no public info on Comet Elenin?

Comet Elenin hasn't received much press precisely because it is small and faint.
Several new comets are discovered each year, and you don't normally hear about
them either. The truth is that Elenin has received much more attention than it deserves
due to a variety of Internet postings that are untrue. The information NASA has on
Elenin is readily available on the Internet. (See
http://www.jpl.nasa.gov/news/news.cfm?release=2011-135 ) If this comet were any
danger to anyone, you would certainly know about it. For more information, visit
NASA's AsteroidWatch site at http://www.jpl.nasa.gov/asteroidwatch/.

I've heard NASA has observed Elenin many times more than other comets. Is this
true, and is NASA playing this comet down?

NASA regularly detects, tracks and characterizes asteroids and comets passing
relatively 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 predicts their paths to determine if any
could be potentially hazardous to our planet. For more information, visit the NASA-JPL
Near Earth objects site at http://neo.jpl.nasa.gov/ .

However, neither NASA nor JPL is in the business of actively observing Elenin or any
other comet. Most of the posted observations are made by amateur astronomers
around the world. Since Elenin has had so much publicity, it naturally has attracted
more observers.

I was looking at the orbital diagram of Comet Elenin on the JPL website, and I was
wondering why the orbit shows some angles when zooming? If you pick any
other comet, you can see that there are no angles or bends.

Many people are trying to plot the orbit of the comet with the routine on the JPL
website, without realizing that this is just a simple visualization tool. While the tool has
been recently improved to show smoother trajectories near the sun, it is not a scientific
program to generate an accurate orbit. Yeomans explains that the orbit plotter on the
Near-Earth Object website is not meant to accurately depict the true motion of objects
over long time intervals, nor is it accurate during close planetary encounters. For more
accurate long-term plotting, Yeomans suggests using the JPL Horizons system
instead:
http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=sb&sstr=C/2010%20X1 .

#2011-255

DC Agle 818-393-9011
Jet Propulsion Laboratory, Pasadena, Calif.
agle@jpl.nasa.gov
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NASA Research Confirms it's a Small World, After All

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

Alan Buis/Whitney Clavin (818) 354-0474/354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
alan.d.buis@jpl.nasa.gov / whitney.clavin@jpl.nasa.gov

News Release: 2011-254 Aug. 16, 2011

NASA Research Confirms it's a Small World, After All

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-254&cid=release_2011-254

A NASA-led research team has confirmed what Walt Disney told us all along: Earth really is a small
world, after all.

Since Charles Darwin's time, scientists have speculated that the solid Earth might be expanding or
contracting. That was the prevailing belief, until scientists developed the theory of plate tectonics,
which explained the large-scale motions of Earth's lithosphere, or outermost shell. Even with the
acceptance of plate tectonics half a century ago, some Earth and space scientists have continued to
speculate on Earth's possible expansion or contraction on various scientific grounds.

Now a new NASA study, published recently in Geophysical Research Letters, has essentially laid
those speculations to rest. Using a cadre of space measurement tools and a new data calculation
technique, the team detected no statistically significant expansion of the solid Earth.

So why should we care if Mother Nature is growing? After all, Earth's shape is constantly changing.
Tectonic forces such as earthquakes and volcanoes push mountains higher, while erosion and
landslides wear them down. In addition, large-scale climate events like El Nino and La Nina
redistribute vast water masses among Earth's ocean, atmosphere and land.

Scientists care because, to put movements of Earth's crust into proper context, they need a frame of
reference to evaluate them against. Any significant change in Earth's radius will alter our
understanding of our planet's physical processes and is fundamental to the branch of science called
geodesy, which seeks to measure Earth's shape and gravity field, and how they change over time.

To make these measurements, the global science community established the International
Terrestrial Reference Frame. This reference frame is used for ground navigation and for tracking
spacecraft in Earth orbit. It is also used to monitor many aspects of global climate change, including
sea level rise and its sources; imbalances in ice mass at Earth's poles; and the continuing rebound
of Earth's surface following the retreat of the massive ice sheets that blanketed much of Earth during
the last Ice Age.

But measuring changes in Earth's size hasn't exactly been easy for scientists to quite literally "get
their arms around." After all, they can't just wrap a giant tape measure around Earth's belly to get a
definitive reading. Fortunately, the field of high-precision space geodesy gives scientists tools they
can use to estimate changes in Earth's radius. These include:

* Satellite laser ranging -- a global observation station network that measures, with millimeter-level
precision, the time it takes for ultrashort pulses of light to travel from the ground stations to
satellites specially equipped with retroreflectors and back again.
* Very-long baseline interferometry -- a radio astronomy technology that combines observations of
an object made simultaneously by many telescopes to simulate a telescope as big as the
maximum distance between the telescopes.
* Global Positioning System -- the U.S.-built space-based global navigation system that provides
users around the world with precise location and time information.
* Doppler Orbitography and Radiopositioning Integrated by Satellite -- a French satellite system
used to determine satellite orbits and positioning. Beacons on the ground emit radio signals that
are received by satellites. The movement of the satellites causes a frequency shift of the signal
that can be observed to determine ground positions and other information.

Scientists use all these techniques to calculate the International Terrestrial Reference Frame.
Central to the reference frame is its point of origin: the precise location of the average center of
mass of the total Earth system (the combination of the solid Earth and the fluid envelope of ocean,
ice and atmosphere that surrounds it, around which all Earth satellites orbit). Scientists currently
determine this origin point based on a quarter century of satellite laser ranging data, considered the
most accurate space geodetic tool for this purpose.

But the accuracy of the satellite laser ranging data and all existing space geodesy technologies is
contaminated, both by the effects of other major Earth processes, and limited ground measurement
sites. Think of it this way: if all of Earth's GPS stations were located in Norway, their data would
indicate that Earth is growing, because high-latitude countries like Norway are still rising in elevation
in response to the removal of the weight of Ice Age ice sheets. So how can scientists be sure the
reference frame is accurate?

Enter an international group of scientists led by Xiaoping Wu of NASA's Jet Propulsion Laboratory,
Pasadena, Calif., and including participants from the Institut Geographique National, Champs-sur-
Marne in France, and Delft University of Technology in The Netherlands. The team set out to
independently evaluate the accuracy of the International Terrestrial Reference Frame and shed new
light on the Earth expansion/contraction theory.

The team applied a new data calculation technique to estimate the rate of change in the solid Earth's
average radius over time, taking into account the effects of other geophysical processes. The
previously discussed geodetic techniques (satellite laser ranging, very-long baseline interferometry
and GPS) were used to obtain data on Earth surface movements from a global network of carefully
selected sites. These data were then combined with measurements of Earth's gravity from NASA's
Gravity Recovery and Climate Experiment (GRACE) spacecraft and models of ocean bottom
pressure, which help scientists interpret gravity change data over the ocean.

The result? The scientists estimated the average change in Earth's radius to be 0.004 inches (0.1
millimeters) per year, or about the thickness of a human hair, a rate considered statistically
insignificant.

"Our study provides an independent confirmation that the solid Earth is not getting larger at present,
within current measurement uncertainties," said Wu.

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Thursday, August 11, 2011

GRAIL Launch Less Than One Month Away

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

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

Feature: 2011-251 Aug. 11, 2011

GRAIL Launch Less Than One Month Away

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-251&cid=release_2011-251

NASA's twin lunar probes – GRAIL-A and GRAIL-B - completed their final inspections and were weighed one
final time at the Astrotech Space Operations facility in Titusville, Fla., on Tuesday. The two Gravity Recovery
and Interior Laboratory (GRAIL) spacecraft will orbit the moon in formation to determine the structure of the
lunar interior from crust to core and to advance understanding of the thermal evolution of the
moon. GRAIL's launch period opens Sept. 8, 2011, and extends through Oct. 19. For a Sept. 8 liftoff, the
launch window opens at 5:37 a.m. PDT (8:37 a.m. EDT) and remains open through 6:16 a.m. PDT (9:16 a.m.
EDT).

Later this week, the two spacecraft will be loaded side-by-side on a special adapter and packaged inside a
payload fairing that will protect them during their launch into space. Next week, GRAIL is expected to make
the trip from Astrotech to Launch Complex 17 at the Cape Canaveral Air Force Station where it will be mated
with its United Launch Alliance Delta II Heavy rocket.

GRAIL-A and GRAIL-B will fly in tandem orbits around the moon for several months to measure its gravity
field in unprecedented detail. The mission will answer longstanding questions about Earth's moon, and
provide scientists a better understanding of how Earth and other rocky planets in the solar system formed.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the GRAIL mission. The Massachusetts Institute
of Technology, Cambridge, is home to the mission's principal investigator, Maria Zuber. The GRAIL mission is
part of the Discovery Program managed at NASA's Marshall Space Flight Center in Huntsville, Ala. Lockheed
Martin Space Systems, Denver, built the spacecraft. Launch management for the mission is the responsibility
of NASA's Launch Services Program at the Kennedy Space Center in Florida. JPL is a division of the California
Institute of Technology in Pasadena.

More information about GRAIL is online at: http://grail.nasa.gov .

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NASA's Asteroid Photographer Beams Back Science Data

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

Feature Aug. 11, 2011

NASA's Asteroid Photographer Beams Back Science Data

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-250&cid=release_2011-250

The Dawn spacecraft has completed a graceful spiral into the first of four planned science
orbits during the spacecraft's yearlong visit to Vesta. The spacecraft started taking
detailed observations on Aug. 11 at 9:13 a.m. PDT (12:13 a.m. EDT), which marks the
official start of the first science-collecting orbit phase at Vesta, also known as the survey
orbit.

Survey orbit is the initial and highest orbit, at roughly 1700 miles (2700 kilometers) above
the surface, which will provide an overview or "big picture" perspective of the giant
asteroid.

The primary objective of survey orbit is to image the surface with near-global coverage in
visible and infrared wavelengths with the mapping spectrometer, also known as VIR.
Dawn also will be using its framing camera to collect image mosaics that complement the
VIR spectral data to produce geologic and compositional maps of Vesta's surface.
Ultrasensitive measurements of the spacecraft's motion using radio signals will allow
improved understanding of the giant asteroid's gravity field. Dawn's gamma ray and
neutron detector will continue to collect background data.

The survey phase is planned to last 20 days. Each orbit takes almost three days, which
will provide the spacecraft seven trips around Vesta. After survey orbit, Dawn will
resume thrusting, taking about a month to spiral down gently to its next science orbit for
an even closer view. That orbit, known as High Altitude Mapping Orbit, or HAMO,
begins in late September. Dawn will spend about a month in HAMO, circling around
Vesta in half a day, rather than three. Dawn will orbit more than 60 times during HAMO,
allowing the camera to fully map the illuminated portion of Vesta at even higher
resolution, and enable the science team to generate stereo images.

For more information about Dawn, visit: http://www.nasa.gov/dawn and
http://dawn.jpl.nasa.gov .

Dawn launched in September 2007 and arrived at Vesta in July 2011. Following a year at
Vesta, the spacecraft will depart in July 2012 for Ceres, where it will arrive in 2015.
Dawn's mission to Vesta and Ceres is managed by the Jet Propulsion Laboratory,
Pasadena, Ca., for NASA's Science Mission Directorate in Washington. JPL is a division
of the California Institute of Technology in Pasadena. Dawn is a project of the
directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in
Huntsville, Ala.?? UCLA is responsible for overall Dawn mission science. Orbital
Sciences Corp. in Dulles, Va., designed and built the spacecraft. The German Aerospace
Center, the Max Planck Institute for Solar System Research, the Italian Space Agency
and the Italian National Astrophysical Institute are international partners on the mission
team.

-end-

Priscilla Vega
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-1357
Priscilla.r.vega@jpl.nasa.gov
2011-250


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Wednesday, August 10, 2011

NASA Mars Rover Arrives at New Site on Martian Surface

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

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

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

News release: 2011-248 Aug. 10, 2011

NASA Mars Rover Arrives at New Site on Martian Surface

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-248&cid=release_2011-248

PASADENA, Calif. – After a journey of almost three years, NASA's Mars Exploration Rover
Opportunity has reached the Red Planet's Endeavour crater to study rocks never seen before.

On Aug. 9, the golf cart-sized rover relayed its arrival at a location named Spirit Point on the crater's
rim. Opportunity drove approximately 13 miles (21 kilometers) since climbing out of the Victoria
crater.

"NASA is continuing to write remarkable chapters in our nation's story of exploration with
discoveries on Mars and trips to an array of challenging new destinations," NASA Administrator
Charles Bolden said. "Opportunity's findings and data from the upcoming Mars Science Laboratory
will play a key role in making possible future human missions to Mars and other places where
humans have not yet been."

Endeavour crater, which is more than 25 times wider than Victoria crater, is 14 miles (22 kilometers)
in diameter. At Endeavour, scientists expect to see much older rocks and terrains than those examined
by Opportunity during its first seven years on Mars. Endeavour became a tantalizing destination after
NASA's Mars Reconnaissance Orbiter detected clay minerals that may have formed in an early
warmer and wetter period.

"We're soon going to get the opportunity to sample a rock type the rovers haven't seen yet," said
Matthew Golombek, Mars Exploration Rover science team member, at NASA's Jet Propulsion
Laboratory (JPL) in Pasadena, Calif. "Clay minerals form in wet conditions so we may learn about a
potentially habitable environment that appears to have been very different from those responsible for
the rocks comprising the plains."

The name Spirit Point informally commemorates Opportunity's twin rover, which stopped
communicating in March 2010. Spirit's mission officially concluded in May.

"Our arrival at this destination is a reminder that these rovers have continued far beyond the original
three-month mission," said John Callas, Mars Exploration Rover project manager at JPL.

NASA's Mars Reconnaissance Orbiter, which launched Aug. 12, 2005, is searching for evidence that
water persisted on the Martian surface for a long period of time. Other Mars missions have shown
water flowed across the surface in the planet's history, but scientists have not determined if water
remained long enough to provide a habitat for life.

NASA launched the Mars rovers Spirit and Opportunity in the summer of 2003. Both completed their
three-month prime missions in April 2004 and continued years of extended operations. They made
important discoveries about wet environments on ancient Mars that may have been favorable for
supporting microbial life.

JPL, a division of the California Institute of Technology in Pasadena, manages the Mars Exploration
Rover Project for NASA's Science Mission Directorate, Washington.

Imagery taken after Opportunity arrived at Endeavour will be released on NASA's website and
NASA Television as soon as available on Wednesday. For more information about the rover and a
color image as it approached the crater, visit: http://www.nasa.gov/rovers and
http://marsrovers.jpl.nasa.gov .

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

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Monday, August 8, 2011

NASA Teacher Workshop

NASA Teacher Workshop Aug. 08, 2011

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

NASA Teacher Workshop: Lunar and Meteorite Sample Certification

Date:Saturday, Aug. 13, 2011, 10 a.m. - 12 p.m.

Target audience:Teachers, grades K - 12 and pre-service teachers

Location: Columbia Memorial Space Center, 12400 Columbia Way Downey, Calif.

Overview:NASA makes actual lunar samples from the historic Apollo missions available to lend
to teachers. Attend this certification workshop to bring the excitement of real lunar rocks and
regolith samples to your students. RSVP required. Call the Columbia Memorial Space Center at
(562) 231-1200 to save your spot!

Also attend the Columbia Memorial Space Center's Teacher Open House on Aug, 13 from 12
p.m. to 4 p.m. for a look at the center and information on field trips. Free admission for teachers! (Family and friends of a teacher are also welcome to attend but must pay the $5 admission fee.) Learn more at http://www.columbiaspacescience.org/events/?event_id=50.

Please call the Columbia Memorial Space Center at (562) 231-1200 to register.

See a listing of upcoming workshops at http://www.columbiaspacescience.org/event-list/ .

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