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Tuesday, October 29, 2013

NASA Hosts Earth Science Social Media Event

JPL/NASA News
News release: 2013-315b                                                             Oct. 29, 2013

NASA Hosts Earth Science Social Media Event

NASA Hosts Earth Science Social Media Event

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-315b&cid=release_2013-315b

One-hundred people from 22 U.S. states and some foreign countries will attend a two-day NASA Social on Nov. 4 and 5 at the agency's Jet Propulsion Laboratory in Pasadena, Calif.

The attendees, who follow NASA and JPL on Twitter, Facebook, Google+ and other social networks, will tour JPL, participate in interactive events and hear from scientists and engineers about current and upcoming space- and Earth-observing missions. Attendees will share their experiences with their followers through the various social media platforms.

The Nov. 4 events will highlight NASA's role in studying Earth and its climate and will preview three Earth-observing missions JPL is preparing for launch in 2014: the Soil Moisture Active Passive (SMAP) spacecraft, which will measure soil moisture from space; ISS-RapidScat, which will measure ocean winds from the International Space Station; and the Orbiting Carbon Observatory-2 (OCO-2), which will study atmospheric carbon dioxide from space.

These presentations will air on NASA Television on Nov. 4 starting at 10 a.m. PST (1 p.m. EST) at http://www.nasa.gov/ntv and http://www.ustream.tv/nasajpl2 .

To join and track the conversation online during the NASA Social, follow the hashtag #NASASocial .

NASA Social attendees were selected from more than 475 people who registered online. Participants represent Canada, Croatia, Indonesia, Norway, Peru, the United States and the United Kingdom. Attendees from the U.S. come from 22 states: Alabama, Alaska, Arizona, Arkansas, California, Colorado, Georgia, Illinois, Maine, Maryland, Massachusetts, Nebraska, Nevada, New Jersey, New York, North Carolina, Oregon, Texas, Utah, Virginia, Washington and Wisconsin. More information about connecting and collaborating with NASA is at: http://www.nasa.gov/connect .

More information about SMAP is online at: http://smap.jpl.nasa.gov/ . More information about ISS-RapidScat is at: http://www.nasa.gov/mission_pages/station/research/experiments/ISSRapidScat.html and http://winds.jpl.nasa.gov/missions/RapidScat/ .

More information about OCO-2 is at: http://oco.jpl.nasa.gov/ .

The California Institute of Technology in Pasadena manages JPL for NASA.

Courtney O'Connor 818-354-2274
Jet Propulsion Laboratory, Pasadena, Calif.
oconnor@jpl.nasa.gov

John Yembrick / Jason Townsend 202-358-1584 / 202-358-0359
NASA Headquarters, Washington
john.yembrick@nasa.gov / jason.c.townsend@nasa.gov

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Upcoming Workshops, Giveaway Days at the NASA/JPL Educator Resource Center

JPL/NASA News

This is a feature of the NASA/JPL Education Office                                          Oct. 29, 2013


Educator Workshop: Lunar and Meteorite Sample Certification Program

Date: Saturday, Nov. 9, 2013, 10 a.m. to 12:30 p.m.

Target Audience: This workshop is for credentialed teachers, teaching grades K-12 in a classroom setting

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

Overview: NASA makes actual lunar samples from the historic Apollo missions available to lend to teachers. You must attend this certification workshop to bring the excitement of real lunar rocks and regolith samples to your students.

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

*Note: The NASA/JPL Educator Resource Center will be hosting a giveaway day featuring numerous items from its Pomona, Calif., location immediately following this workshop. See below for more information.


Educator Workshop: Marsbound! Mission to the Red Planet

Date: Saturday, Dec. 7, 2013, 10:00 a.m. to 12:30 p.m.

Target audience: Educators for grades 4 and above

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

Overview: Bring Marsbound! Mission to the Red Planet, an exciting hands-on lesson that addresses Common Core and Next Generation Science Standards, to your classroom! Build a mission to Mars using a mat and cards game, design and redesign, facing the same problems that real engineers and scientists face. Compare Earth and Mars geology and explore what it will take to create a Mars colony, socially, historically, physically and vocationally! This workshop is limited to 30 participants.

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

*Note: The NASA/JPL Educator Resource Center will be hosting a giveaway day featuring numerous items from its Pomona, Calif., location immediately following this workshop. See below for more information.


Giveaway Days:

After 15 years in its Pomona, Calif., location, the NASA Jet Propulsion Laboratory's Educator Resource Center will be moving. (A new arrangement for the center has not been determined. Continue to check the ERC page at http://www.jpl.nasa.gov/education/index.cfm?page=115 for future updates.)

To facilitate our move, we need your help giving some of our excess material a new home. Up for grabs are items such as historical reference books, posters, historical JPL annual reports, bookmarks, postcards, and other JPL and educational materials.

In the coming months, we will have two free yard-sale-type events during which you can visit the ERC at the Indian Hill Mall in Pomona and take whatever you can use: Saturday, Nov. 9 and Saturday, Dec. 7. The doors will open for each event at 12:30 p.m. and close at 2:30 p.m., no need to RSVP. We recommend arriving with boxes or bags to carry items home. No early birds please.


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Thursday, October 24, 2013

NASA's Great Observatories Begin Deepest-Ever Probe of the Universe

JPL/NASA News
News Release: 2013-306                                                             Oct. 24, 2013

NASA's Great Observatories Begin Deepest-Ever Probe of the Universe



The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-306

PASADENA, Calif. -- NASA's Hubble, Spitzer and Chandra space telescopes are teaming up to look deeper into the universe than ever before. With a boost from natural "zoom lenses" found in space, they should be able to uncover galaxies that are as much as 100 times fainter than what these three great observatories typically can see.

In an ambitious collaborative program called The Frontier Fields, astronomers will make observations during the next three years peering at six massive clusters of galaxies, exploiting a natural phenomenon known as gravitational lensing, to learn not only what is inside the clusters but also what is beyond them. The clusters are among the most massive assemblages of matter known, and their gravitational fields can be used to brighten and magnify more distant galaxies so they can be observed.

"The Frontier Fields program is exactly what NASA's Great Observatories were designed to do; working together to unravel the mysteries of the universe" said John Grunsfeld, associate administrator for NASA's Science Mission Directorate in Washington. "Each observatory collects images using different wavelengths of light with the result that we get a much deeper understanding of the underlying physics of these celestial objects."

The first object they will view is Abell 2744, commonly known as Pandora's Cluster. The giant galaxy cluster appears to be the result of a simultaneous pile-up of at least four separate, smaller galaxy clusters that took place over a span of 350 million years.

Astronomers anticipate these observations will reveal populations of galaxies that existed when the universe was only a few hundred million years old, but have not been seen before.

"The idea is to use nature's natural telescopes in combination with the great observatories to look much deeper than before and find the most distant and faint galaxies we can possibly see," said Jennifer Lotz, a principal investigator with the Space Telescope Science Institute in Baltimore, Md.

Data from the Hubble and Spitzer space telescopes will be combined to measure the galaxies' distances and masses more accurately than either observatory could measure alone, demonstrating their synergy for such studies.

"We want to understand when and how the first stars and galaxies formed in the universe, and each great observatory gives us a different piece of the puzzle," said Peter Capak, the Spitzer principal investigator for the Frontier Fields program at NASA's Spitzer Science Center at the California Institute of Technology, Pasadena. "Hubble tells you which galaxies to look at and how many stars are being born in those systems. Spitzer tells you how old the galaxy is and how many stars have formed."

The Chandra X-ray Observatory also will peer deep into the star fields. It will image the clusters at X-ray wavelengths to help determine their mass and measure their gravitational lensing power, and identify background galaxies hosting supermassive black holes.

High-resolution Hubble data from Frontier Fields will be used to trace the distribution of dark matter within the six massive foreground clusters. Accounting for the bulk of the universe's mass, dark matter is the underlying invisible scaffolding attached to galaxies.

Hubble and Spitzer have studied other deep fields with great success. The Frontier Fields researchers anticipate a challenge because the distortion and magnification caused by the gravitational lensing phenomenon will make it difficult for them to understand the true properties of the background galaxies.

For images and more information about The Frontier Fields, visit: http://hubblesite.org/news/2013/44 .

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at Caltech. Spacecraft operations are based at Lockheed Martin Space Systems Company, Littleton, Colorado. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech. Caltech manages JPL for NASA. For more information about Spitzer, visit http://spitzer.caltech.edu and http://www.nasa.gov/spitzer .

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

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

J.D. Harrington 202-358-5241
Headquarters, Washington
j.d.harrington@nasa.gov

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Friday, September 20, 2013

NASA's Deep Space Comet Hunter Mission Comes to an End

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

D.C. 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

Lee Tune 301-405-4679
University of Maryland, College Park, Md.
ltune@umd.edu

News release: 2013-287 Sept. 20, 2013

NASA's Deep Space Comet Hunter Mission Comes to an End

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-287&cid=release_2013-287

PASADENA, Calif. - After almost 9 years in space that included an unprecedented July 4th impact
and subsequent flyby of a comet, an additional comet flyby, and the return of approximately 500,000
images of celestial objects, NASA's Deep Impact mission has ended.

The project team at NASA's Jet Propulsion Laboratory in Pasadena, Calif., has reluctantly
pronounced the mission at an end after being unable to communicate with the spacecraft for over a
month. The last communication with the probe was Aug. 8. Deep Impact was history's most traveled
comet research mission, going about 4.7 billion miles (7.58 billion kilometers).

"Deep Impact has been a fantastic, long-lasting spacecraft that has produced far more data than we
had planned," said Mike A'Hearn, the Deep Impact principal investigator at the University of
Maryland in College Park. "It has revolutionized our understanding of comets and their activity."

Deep Impact successfully completed its original bold mission of six months in 2005 to investigate
both the surface and interior composition of a comet, and a subsequent extended mission of another
comet flyby and observations of planets around other stars that lasted from July 2007 to December
2010. Since then, the spacecraft has been continually used as a space-borne planetary observatory to
capture images and other scientific data on several targets of opportunity with its telescopes and
instrumentation.

Launched in January 2005, the spacecraft first traveled about 268 million miles (431 million
kilometers) to the vicinity of comet Tempel 1. On July 3, 2005, the spacecraft deployed an impactor
into the path of comet to essentially be run over by its nucleus on July 4. This caused material from
below the comet's surface to be blasted out into space where it could be examined by the telescopes
and instrumentation of the flyby spacecraft. Sixteen days after that comet encounter, the Deep Impact
team placed the spacecraft on a trajectory to fly back past Earth in late December 2007 to put it on
course to encounter another comet, Hartley 2 in November 2010.

"Six months after launch, this spacecraft had already completed its planned mission to study comet
Tempel 1," said Tim Larson, project manager of Deep Impact at JPL. "But the science team kept
finding interesting things to do, and through the ingenuity of our mission team and navigators and
support of NASA's Discovery Program, this spacecraft kept it up for more than eight years, producing
amazing results all along the way."

The spacecraft's extended mission culminated in the successful flyby of comet Hartley 2 on Nov. 4,
2010. Along the way, it also observed six different stars to confirm the motion of planets orbiting
them, and took images and data of Earth, the moon and Mars. These data helped to confirm the
existence of water on the moon, and attempted to confirm the methane signature in the atmosphere of
Mars. One sequence of images is a breathtaking view of the moon transiting across the face of Earth.

In January 2012, Deep Impact performed imaging and accessed the composition of distant comet
C/2009 P1 (Garradd). It took images of comet ISON this year and collected early images of ISON in
June.

After losing contact with the spacecraft last month, mission controllers spent several weeks trying to
uplink commands to reactivate its onboard systems. Although the exact cause of the loss is not
known, analysis has uncovered a potential problem with computer time tagging that could have led to
loss of control for Deep Impact's orientation. That would then affect the positioning of its radio
antennas, making communication difficult, as well as its solar arrays, which would in turn prevent the
spacecraft from getting power and allow cold temperatures to ruin onboard equipment, essentially
freezing its battery and propulsion systems.

"Despite this unexpected final curtain call, Deep Impact already achieved much more than ever was
envisioned," said Lindley Johnson, the Discovery Program Executive at NASA Headquarters, and the
Program Executive for the mission since a year before it launched. "Deep Impact has completely
overturned what we thought we knew about comets and also provided a treasure trove of additional
planetary science that will be the source data of research for years to come."

The mission is part of the Discovery Program managed at NASA's Marshall Space Flight Center in
Huntsville, Ala. JPL manages the Deep Impact mission for NASA's Science Mission Directorate in
Washington. Ball Aerospace & Technologies Corp. of Boulder, Colo., built the spacecraft. The
California Institute of Technology in Pasadena manages JPL for NASA.

To find out more about Deep Impact's scientific results, visit: http://go.nasa.gov/19ki9LG .
For more information about Deep Impact, visit: http://www.nasa.gov/deepimpact .

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Thursday, September 19, 2013

NASA Curiosity Rover Detects No Methane on 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

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: 2013-285 Sept. 19, 2013

NASA Curiosity Rover Detects No Methane on Mars

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-285&cid=release_2013-285

PASADENA, Calif. -- Data from NASA's Curiosity rover has revealed the Martian environment lacks methane. This is a surprise to researchers because previous data reported by U.S. and international scientists indicated positive detections.

The roving laboratory performed extensive tests to search for traces of Martian methane. Whether the Martian atmosphere contains traces of the gas has been a question of high interest for years because methane could be a potential sign of life, although it also can be produced without biology.

"This important result will help direct our efforts to examine the possibility of life on Mars," said Michael Meyer, NASA's lead scientist for Mars exploration. "It reduces the probability of current methane-producing Martian microbes, but this addresses only one type of microbial metabolism. As we know, there are many types of terrestrial microbes that don't generate methane."

Curiosity analyzed samples of the Martian atmosphere for methane six times from October 2012 through June and detected none. Given the sensitivity of the instrument used, the Tunable Laser Spectrometer, and not detecting the gas, scientists calculate the amount of methane in the Martian atmosphere today must be no more than 1.3 parts per billion. That is about one-sixth as much as some earlier estimates. Details of the findings appear in the Thursday edition of Science Express.

"It would have been exciting to find methane, but we have high confidence in our measurements, and the progress in expanding knowledge is what's really important," said the report's lead author, Chris Webster of NASA's Jet Propulsion Laboratory in Pasadena, Calif. "We measured repeatedly from Martian spring to late summer, but with no detection of methane."

Webster is the lead scientist for spectrometer, which is part of Curiosity's Sample Analysis at Mars (SAM) laboratory. It can be tuned specifically for detection of trace methane. The laboratory also can concentrate any methane to increase the gas' ability to be detected. The rover team will use this method to check for methane at concentrations well below 1 part per billion.

Methane, the most abundant hydrocarbon in our solar system, has one carbon atom bound to four hydrogen atoms in each molecule. Previous reports of localized methane concentrations up to 45 parts per billion on Mars, which sparked interest in the possibility of a biological source on Mars, were based on observations from Earth and from orbit around Mars. However, the measurements from Curiosity are not consistent with such concentrations, even if the methane had dispersed globally.

"There's no known way for methane to disappear quickly from the atmosphere," said one of the paper's co-authors, Sushil Atreya of the University of Michigan, Ann Arbor. "Methane is persistent. It would last for hundreds of years in the Martian atmosphere. Without a way to take it out of the atmosphere quicker, our measurements indicate there cannot be much methane being put into the atmosphere by any mechanism, whether biology, geology, or by ultraviolet degradation of organics delivered by the fall of meteorites or interplanetary dust particles."

The highest concentration of methane that could be present without being detected by Curiosity's measurements so far would amount to no more than 10 to 20 tons per year of methane entering the Martian atmosphere, Atreya estimated. That is about 50 million times less than the rate of methane entering Earth's atmosphere.

Curiosity landed inside Gale Crater on Mars in August 2012 and is investigating evidence about habitable environments there. JPL manages the mission and built the rover for NASA's Science Mission Directorate in Washington. The rover's Sample Analysis at Mars suite of instruments was developed at NASA's Goddard Space Flight Center in Greenbelt, Md., with instrument contributions from Goddard, JPL and the University of Paris in France.

For more information about the mission, visit http://www.nasa.gov/msl and http://mars.jpl.nasa.gov/msl . To learn more about the SAM instrument, visit:
http://ssed.gsfc.nasa.gov/sam/index.html .

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Wednesday, September 18, 2013

Long-stressed Europa Likely Off-kilter at One Time

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

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

Elizabeth Zubritsky/Nancy Neal-Jones 301-614-5438/301-286-0039
Goddard Space Flight Center, Greenbelt, Md.
elizabeth.a.zubritsky@nasa.gov/nancy.n.jones@nasa.gov

Long-stressed Europa Likely Off-kilter at One Time

News release: 2013-283 Sept. 18, 2013

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-283&cid=release_2013-283

By analyzing the distinctive cracks lining the icy face of Europa, NASA scientists found evidence that this moon of Jupiter likely spun around a tilted axis at some point.

Europa's tilt could influence calculations of how much of the moon's history is recorded in its frozen shell, how much heat is generated by tides in its ocean, and even how long the ocean has been liquid.

"One of the mysteries of Europa is why the orientations of the long, straight cracks called lineaments have changed over time. It turns out that a small tilt, or obliquity, in the spin axis, sometime in the past, can explain a lot of what we see," said Alyssa Rhoden, a postdoctoral fellow with Oak Ridge Associated Universities who is working at NASA's Goddard Space Flight Center in Greenbelt, Md. She is the lead author of a paper in the September–October issue of Icarus that describes the results.

Europa's network of crisscrossing cracks serves as a record of the stresses caused by massive tides in the moon's global ocean. These tides occur because Europa travels around Jupiter in a slightly oval-shaped orbit. When Europa comes closer to the planet, the moon gets stretched like a rubber band, with the ocean height at the long ends rising nearly 100 feet (30 meters). That's roughly as high as the 2004 tsunami in the Indian Ocean, but it happens on a body that measures only about one-quarter of Earth's diameter. When Europa moves farther from Jupiter, it relaxes back into the shape of a ball.

The moon's ice layer has to stretch and flex to accommodate these changes, but when the stresses become too great, it cracks. The puzzling part is why the cracks in Europa's icy layer point in different directions over time, even though the same side of Europa always faces Jupiter.

A leading explanation has been that Europa's frozen outer shell might rotate slightly faster than the moon orbits Jupiter. If this out-of-sync rotation does occur, the same part of the ice shell would not always face Jupiter.

Rhoden and her Goddard co-author Terry Hurford put that idea to the test using images taken by NASA's Galileo spacecraft during its nearly eight-year mission, which began in 1995. "Galileo produced many paradigm shifts in our understanding of Europa, one of which was the phenomena of out-of-sync rotation," said Claudia Alexander of NASA's Jet Propulsion Laboratory in Pasadena, Calif., who was the project manager when the Galileo mission ended.

Rhoden and Hurford compared the pattern of cracks in a key area near Europa's equator to predictions based on three different explanations. The first set of predictions was based on the rotation of the ice shell. The second set assumed that Europa was spinning around a tilted axis, which, in turn, made the orientation of the pole change over time. This effect, called precession, looks very much like what happens when a spinning toy top has started to slow down and wobble. The third explanation was that the cracks were laid out in random directions.

The researchers got the best performance when they assumed that precession had occurred, caused by a tilt of about one degree, and combined this effect with some random cracks, said Rhoden. Out-of-sync rotation was surprisingly unsuccessful, in part because Rhoden found an oversight in the original calculations for this model.

The results are compelling enough to satisfy Richard Greenberg, the professor from the University of Arizona, Tucson, who had earlier proposed the idea of out-of sync rotation.

"By extracting new information from the Galileo data, this work refines and improves our understanding of the very unusual geology of Europa," said Greenberg, who was Rhoden's undergraduate advisor and Hurford's graduate advisor.

The existence of tilt would not rule out the out-of-sync rotation, according to Rhoden and Greenberg. But it does suggest that Europa's cracks may be much more recent than previously thought. That's because the spin pole direction may change by as much as a few degrees per day, completing one precession period over several months. On the other hand, with the leading explanation, one full rotation of the ice sheet would take roughly 250,000 years. In either case, several rotations would be needed to explain the crack patterns.

A tilt also could affect the estimates of the age of Europa's ocean. Tidal forces are thought to generate the heat that keeps Europa's ocean liquid, and a tilt in the spin axis might suggest that more heat is generated by tidal forces. This heat might keep the ocean liquid longer.

The analysis does not specify when the tilt would have occurred. So far, measurements have not been made of the tilt of Europa's axis, and this is one goal scientists have for any future Europa mission.

"One of the fascinating open questions is how active Europa still is. If researchers pin down Europa's current spin axis, then our findings would allow us to assess whether the clues we are finding on the moon's surface are consistent with the present-day conditions," said Rhoden.

The Galileo mission was managed by NASA's Jet Propulsion Laboratory in Pasadena, Calif., for the agency's Science Mission Directorate. JPL is a division of the California Institute of Technology, Pasadena.

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

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Monday, September 16, 2013

NASA Invites Social Media Fans to Earth Science Event

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

Courtney O'Connor 818-354-2274
Jet Propulsion Laboratory, Pasadena, Calif.
oconnor@jpl.nasa.gov

John Yembrick/Jason Townsend 650-604-2065 / 202-358-0359
NASA Headquarters, Washington
john.yembrick@nasa.gov / jason.c.townsend@nasa.gov

News release: 2013-280 Sept. 16, 2013

NASA Invites Social Media Fans to Earth Science Event

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-280&cid=release_2013-280

PASADENA, Calif. – NASA is inviting its social media followers to apply for participation in a two-day NASA Social on Nov. 4 and 5 at the agency's Jet Propulsion Laboratory in Pasadena, Calif. The event will highlight NASA and JPL's role in studying Earth and its climate and will preview three Earth-observing missions JPL is preparing for launch in 2014.

The event will offer people who connect with NASA through Twitter, Facebook, Google+ and other social networks the opportunity to interact with scientists and engineers working on upcoming missions and participate in hands-on demonstrations. Participants will also interact with fellow tweeps, space enthusiasts and members of NASA's social media team. They will get a behind-the-scenes tour of JPL, including:

-- The Spacecraft Assembly Facility, where hardware for two upcoming Earth missions is currently under construction. This clean room is also where NASA's Voyager and Cassini spacecraft and the Curiosity, Opportunity and Spirit Mars rovers were built and tested.
-- The JPL Earth Science Center, where data from many of the agency's Earth-observing missions are showcased in interactive displays.
-- The Mission Control Center of NASA's Deep Space Network, where engineers "talk to" spacecraft across the solar system and in interstellar space.
-- The JPL Mars Yard, where engineers and scientists test engineering models of NASA's Curiosity rover in a sandy, Mars-like environment.

Registration for the NASA Social is open until noon PDT (3 p.m. EDT) on Wednesday, Sept. 18. NASA will randomly select at least 100 participants from online registrations.
More information on NASA Socials and the application for the Nov. 4/5 event are online at: http://www.nasa.gov/social .

The two NASA/JPL Earth-observing missions being assembled at JPL are the Soil Moisture Active Passive (SMAP) spacecraft and ISS-RapidScat. SMAP will produce global maps of soil moisture for tracking water availability around our planet. ISS-RapidScat is a scatterometer instrument that will be mounted outside the International Space Station to measure ocean surface wind speeds and directions. ISS-RapidScat is scheduled to launch first, in April 2014, with SMAP scheduled to launch in October 2014.

A third NASA/JPL Earth mission, the Orbiting Carbon Observatory-2 (OCO-2), scheduled to launch in July 2014, is in final assembly and testing at an Orbital Sciences Corp. facility in Gilbert, Ariz. The mission will be NASA's first dedicated Earth remote-sensing satellite to study atmospheric carbon dioxide from space.

To join and track the conversation online during the NASA Socials, follow the hashtag #NASASocial.

More information about connecting and collaborating with NASA is at: http://www.nasa.gov/connect .

For more on SMAP, visit: http://smap.jpl.nasa.gov/ .

For more on ISS-RapidScat, visit: http://www.nasa.gov/mission_pages/station/research/experiments/ISSRapidScat.html and http://winds.jpl.nasa.gov/missions/RapidScat/ .

For more on OCO-2, visit: http://oco.jpl.nasa.gov/ .

The California Institute of Technology in Pasadena manages JPL for NASA.

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Thursday, September 12, 2013

NASA Spacecraft Embarks on Historic Journey Into Interstellar Space

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

Jia-Rui C. Cook/D.C. Agle 818-354-0850/818-393-9011
Jet Propulsion Laboratory, Pasadena, Calif.
jccook@jpl.nasa.gov

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

News release: 2013-277 Sept. 12, 2013

NASA Spacecraft Embarks on Historic Journey Into Interstellar Space

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-277&cid=release_2013-277

PASADENA, Calif. -- NASA's Voyager 1 spacecraft officially is the first human-made object to venture into interstellar space. The 36-year-old probe is about 12 billion miles (19 billion kilometers) from our sun.

New and unexpected data indicate Voyager 1 has been traveling for about one year through plasma, or ionized gas, present in the space between stars. Voyager is in a transitional region immediately outside the solar bubble, where some effects from our sun are still evident. A report on the analysis of this new data, an effort led by Don Gurnett and the plasma wave science team at the University of Iowa, Iowa City, is published in Thursday's edition of the journal Science.

"Now that we have new, key data, we believe this is mankind's historic leap into interstellar space," said Ed Stone, Voyager project scientist based at the California Institute of Technology, Pasadena. "The Voyager team needed time to analyze those observations and make sense of them. But we can now answer the question we've all been asking -- 'Are we there yet?' Yes, we are."

Voyager 1 first detected the increased pressure of interstellar space on the heliosphere, the bubble of charged particles surrounding the sun that reaches far beyond the outer planets, in 2004. Scientists then ramped up their search for evidence of the spacecraft's interstellar arrival, knowing the data analysis and interpretation could take months or years.

Voyager 1 does not have a working plasma sensor, so scientists needed a different way to measure the spacecraft's plasma environment to make a definitive determination of its location. A coronal mass ejection, or a massive burst of solar wind and magnetic fields, that erupted from the sun in March 2012 provided scientists the data they needed. When this unexpected gift from the sun eventually arrived at Voyager 1's location 13 months later, in April 2013, the plasma around the spacecraft began to vibrate like a violin string. On April 9, Voyager 1's plasma wave instrument detected the movement. The pitch of the oscillations helped scientists determine the density of the plasma. The particular oscillations meant the spacecraft was bathed in plasma more than 40 times denser than what they had encountered in the outer layer of the heliosphere. Density of this sort is to be expected in interstellar space.

The plasma wave science team reviewed its data and found an earlier, fainter set of oscillations in October and November 2012. Through extrapolation of measured plasma densities from both events, the team determined Voyager 1 first entered interstellar space in August 2012.

"We literally jumped out of our seats when we saw these oscillations in our data -- they showed us the spacecraft was in an entirely new region, comparable to what was expected in interstellar space, and totally different than in the solar bubble," Gurnett said. "Clearly we had passed through the heliopause, which is the long-hypothesized boundary between the solar plasma and the interstellar plasma."

The new plasma data suggested a timeframe consistent with abrupt, durable changes in the density of energetic particles that were first detected on Aug. 25, 2012. The Voyager team generally accepts this date as the date of interstellar arrival. The charged particle and plasma changes were what would have been expected during a crossing of the heliopause.

"The team's hard work to build durable spacecraft and carefully manage the Voyager spacecraft's limited resources paid off in another first for NASA and humanity," said Suzanne Dodd, Voyager project manager, based at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "We expect the fields and particles science instruments on Voyager will continue to send back data through at least 2020. We can't wait to see what the Voyager instruments show us next about deep space."

Voyager 1 and its twin, Voyager 2, were launched 16 days apart in 1977. Both spacecraft flew by Jupiter and Saturn. Voyager 2 also flew by Uranus and Neptune. Voyager 2, launched before Voyager 1, is the longest continuously operated spacecraft. It is about 9.5 billion miles (15 billion kilometers) away from our sun.

Voyager mission controllers still talk to or receive data from Voyager 1 and Voyager 2 every day, though the emitted signals are currently very dim, at about 23 watts -- the power of a refrigerator light bulb. By the time the signals get to Earth, they are a fraction of a billion-billionth of a watt. Data from Voyager 1's instruments are transmitted to Earth typically at 160 bits per second, and captured by 34- and 70-meter NASA Deep Space Network stations. Traveling at the speed of light, a signal from Voyager 1 takes about 17 hours to travel to Earth. After the data are transmitted to JPL and processed by the science teams, Voyager data are made publicly available.

"Voyager has boldly gone where no probe has gone before, marking one of the most significant technological achievements in the annals of the history of science, and adding a new chapter in human scientific dreams and endeavors," said John Grunsfeld, NASA's associate administrator for science in Washington. "Perhaps some future deep space explorers will catch up with Voyager, our first interstellar envoy, and reflect on how this intrepid spacecraft helped enable their journey."

Scientists do not know when Voyager 1 will reach the undisturbed part of interstellar space where there is no influence from our sun. They also are not certain when Voyager 2 is expected to cross into interstellar space, but they believe it is not very far behind.

JPL built and operates the twin Voyager spacecraft. The Voyagers Interstellar Mission is a part of NASA's Heliophysics System Observatory, sponsored by the Heliophysics Division of NASA's Science Mission Directorate in Washington. NASA's Deep Space Network, managed by JPL, is an international network of antennas that supports interplanetary spacecraft missions and radio and radar astronomy observations for the exploration of the solar system and the universe. The network also supports selected Earth-orbiting missions.

The cost of the Voyager 1 and Voyager 2 missions -- including launch, mission operations and the spacecraft's nuclear batteries, which were provided by the Department of Energy -- is about $988 million through September.

For a sound file of the oscillations detected by Voyager in interstellar space, animations and other information, visit: http://www.nasa.gov/voyager .

For an image of the radio signal from Voyager 1 on Feb. 21 by the National Radio Astronomy Observatory's Very Long Baseline Array, which links telescopes from Hawaii to St. Croix, visit:
http://www.nrao.edu .

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NASA News Conference Today to Discuss Voyager Spacecraft

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/Jia-Rui Cook 818-393-9011/818-354-0850
Jet Propulsion Laboratory, Pasadena, Calif.
agle@jpl.nasa.gov/jccook@jpl.nasa.gov

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

News advisory: 2013-276b Sept. 12, 2013

NASA News Conference Today to Discuss Voyager Spacecraft

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-276&cid=release_2013-276

PASADENA, Calif. – NASA will host a news conference today at 11 a.m. PDT (2 p.m. EDT), to discuss NASA's Voyager mission. It is related to a paper to be published in the journal Science, which is embargoed until 11 a.m. PDT (2 p.m. EDT).

The briefing will be held at NASA Headquarters in Washington and air live on NASA Television and the agency's website.

During the news conference, the public may send questions via Twitter to #AskNASA.

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

The event will also be streamed live on Ustream at: http://www.ustream.tv/nasajpl2 .

For information about the Voyager mission, visit: http://www.nasa.gov/voyager .

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Monday, September 9, 2013

'La Nada' Climate Pattern Lingers in the Pacific

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

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

News feature: 2013-272 Sept. 9, 2013

'La Nada' Climate Pattern Lingers in the Pacific

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-272&cid=release_2013-272

New remote sensing data from NASA's Jason-2 satellite show near-normal sea-surface height conditions across the equatorial Pacific Ocean. This neutral, or "La Nada" event, has stubbornly persisted for 16 months, since spring 2012. Models suggest this pattern will continue through the spring of 2014, according to the National Weather Service's Climate Prediction Center.

"Without an El Niño or La Niña signal present, other, less predictable, climatic factors will govern fall, winter and spring weather conditions," said climatologist Bill Patzert of NASA's Jet Propulsion Laboratory, Pasadena, Calif. Long-range forecasts are most successful during El Niño and La Niña episodes. The "in between" ocean state, La Nada, is the dominant condition, and is frustrating for long-range forecasters. It's like driving without a decent road map -- it makes forecasting difficult."

The near-normal conditions are shown in a new image (as areas shaded in green), based on the average of 10 days of data centered on Aug. 27, 2013. The image is available at: http://www.jpl.nasa.gov/spaceimages/details.php?id=pia17454 .

For the past several decades, about half of all years have experienced La Nada conditions, compared to about 20 percent for El Niño and 30 percent for La Niña. 

Patzert noted that some of the wettest and driest winters occur during La Nada periods.
 
"Neutral infers something benign, but in fact if you look at these La Nada years when neither El Niño nor La Niña are present, they can be the most volatile and punishing. As an example, the continuing, deepening drought in the American West is far from 'neutral,'" he said.
 
The height of the sea water relates, in part, to its temperature, and thus is an indicator of the amount of heat stored in the ocean below. As the ocean warms, its level rises; as it cools, its level falls. Yellow and red areas indicate where the waters are relatively warmer and have expanded above normal sea level, while green (which dominates in this image) indicates near-normal sea level, and blue and purple areas show where the waters are relatively colder and sea level is lower than normal. Above-normal height variations along the equatorial Pacific indicate El Niño conditions, while below-normal height variations indicate La Niña conditions.The temperature of the upper ocean can have a significant influence on weather patterns and climate. For a more detailed explanation of what this type of image means, visit: http://sealevel.jpl.nasa.gov/science/elninopdo/latestdata/.

This latest image highlights the processes that occur on time scales of more than a year, but usually less than 10 years, such as El Niño and La Niña. These processes are known as the interannual ocean signal. To show that signal, scientists refined data for this image by removing trends over the past 20 years, seasonal variations and time-averaged signals of large-scale ocean circulation.

NASA scientists will continue to monitor this persistent La Nada event to see what the Pacific Ocean has in store next for the world's climate.
The comings and goings of El Niño, La Niña and La Nada are part of the long-term, evolving state of global climate, for which measurements of sea surface height are a key indicator. Jason-2 is a joint effort between NASA, the National Oceanic and Atmospheric Administration (NOAA), the French Space Agency Centre National d'Etudes Spatiales (CNES) and the European Organisation for the Exploitation of Meteorological Satellites (EUMETSAT). JPL manages the U.S. portion of Jason-2 for NASA's Science Mission Directorate, Washington, D.C.

In early 2015, NASA and its international partners CNES, NOAA and EUMETSAT will launch Jason-3, which will extend the timeline of ocean surface topography measurements begun by the Topex/Poseidon and Jason 1 and 2 satellites. Jason-3 will make highly detailed measurements of sea level on Earth to gain insight into ocean circulation and climate change.

For more on NASA's satellite altimetry programs, visit: http://sealevel.jpl.nasa.gov.

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