NASA Revises Cost and Schedule for Displaying Retired Shuttles

NASA has issued a follow-up Request for Information, or RFI, for ideas from education institutions, science museums and other appropriate organizations about the community's ability to acquire and publicly display orbiters after the conclusion of the Space Shuttle Program.

The original RFI in December 2008 noted that a potential shuttle recipient would have to pay an estimated $42 million for the cost of "safeing" an orbiter, preparing it for display and ferrying it to a U.S. destination airport. NASA has updated the requirements and tasks needed to make each orbiter safe for disposition. The agency will not ask recipients to provide the funds for this activity. Except for cost and scheduled delivery changes, the 2008 and 2010 RFIs are virtually the same. In this follow-up RFI, NASA revised the estimated display preparation and ferrying costs to $28.8 million.

The schedule for transferring the orbiters may be six months earlier than originally anticipated. NASA also desires to make selections a year before receipt of the orbiters, so recipient organizations will have sufficient time to conduct any fundraising activities necessary to support preparation and ferry costs.

RFI responses are due to NASA by 11:59 p.m. EST on Friday, Feb. 19, 2010. Organizations that responded to the original RFI do not need to resubmit a full response, but should clarify their positions with respect to these changes.

NASA is planning to transfer space shuttle Discovery to the National Air and Space Museum. Shuttle orbiters Endeavour and Atlantis will be available for placement no earlier than July, 2011.

For additional information and to view the RFI, visit:

http://www.nasa.gov/transition

For additional information about the shuttle program, visit:

http://www.nasa.gov/shuttle

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Fault Responsible for Haiti Quake Slices Island’s Topography

Port-au-Prince, Haiti
A magnitude 7.0 earthquake occurred on January 12, 2010, at Port-au-Prince, Haiti, with major impact to the region and its citizens.

› Full image and caption

The fault responsible for the Jan. 12 magnitude 7.0 earthquake that devastated Haiti is visible in images created using NASA radar topography data acquired in 2000.

This perspective view of the pre-earthquake topography of the area, created using data from the Shuttle Radar Topography Mission that flew aboard Space Shuttle Endeavour in February 2000, clearly shows the Enriquillo fault that is apparently responsible for the earthquake. The fault is visible as a prominent linear landform that forms a sharp diagonal line at the center of the image. The city of Port-au-Prince is immediately to the left (north) at the mountain front and shoreline.

Elevations in the image are color coded from dark green at low elevations to white at high elevations, and the topography is shaded with illumination from the left. The topography in this image is exaggerated by a factor of two.

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JPL Scientist Honored by President Obama With Early Career Award

JPL Oceanographer Josh Willis (center) receives the Presidential Early Career Award for Scientists and Engineers from White House Office of Science and Technology Policy Director John Holdren (left) and NASA Associate Administrator Lori Garver (right
JPL Oceanographer Josh Willis (center) receives the Presidential Early Career Award for Scientists and Engineers from White House Office of Science and Technology Policy Director John Holdren (left) and NASA Associate Administrator Lori Garver (right) Jan. 13 in Washington, D.C. › Enlarge image

JPL oceanographer Josh Willis was honored by President Obama at the White House on Wednesday, Jan. 13, as a recipient of this year's Presidential Early Career Award for Scientists and Engineers. The award is the highest honor bestowed by the U.S. government on scientists and engineers in the early stages of their independent research careers. It recognizes researchers whose early career accomplishments show the greatest promise for strengthening America's leadership in science and technology and contributing to the awarding agencies' missions.

John Holdren, President Obama's science advisor and director of the White House Office of Science and Technology Policy, presented the award to Willis at a ceremony at the Department of Commerce in Washington, along with NASA Associate Administrator Lori Garver. Willis was among 100 scientists and engineers selected for this year's award from among nine federal departments and agencies.

Following the ceremony, the recipients met with President Obama at the White House. President Obama said, "You have been selected for this honor not only because of your innovative research, but also for your demonstrated commitment to community service and public outreach. Your achievements as scientists, engineers, and engaged citizens are exemplary, and the value of your work is amplified by the inspiration you provide to others."

A researcher in JPL's Ocean Circulation Group, Willis uses data collected by satellites and at sea to study the impact of global warming on the ocean. His studies of ocean warming and sea level rise have been widely used by colleagues around the world and were cited in the 2007 report of the Intergovernmental Panel on Climate Change. That report shared the 2007 Nobel Peace prize with Vice President Al Gore. Willis frequently lectures to the public and works with students to educate them about climate change issues and human impacts on global warming.

Willis holds a bachelor of science degree in physics and mathematics from the University of Houston; a master of science degree in physics from the University of California, San Diego, in La Jolla, Calif.; and a doctorate in oceanography from the Scripps Institution of Oceanography, University of California, San Diego. He joined JPL in 2004. His previous honors include JPL's Charles K. Witham Environmental Stewardship Award.

More information is online at: http://www.ostp.gov/galleries/press_release_files/PECASE%20OSTP%20Press%20Release2%20revised.pdf and http://www.jpl.nasa.gov/news/news.cfm?release=2009-108 .

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Land Ho! Huygens Plunged to Titan Surface 5 Years Ago

Artist concept showing the descent and landing of HuygensThe Huygens probe parachuted down to the surface of Saturn's haze-shrouded moon Titan exactly five years ago on Jan. 14, 2005, providing data that scientists on NASA's Cassini mission to Saturn are still building upon today.

"Huygens has gathered critical on-the-scene data on the atmosphere and surface of Titan, providing valuable groundtruth to Cassini's ongoing investigations," said Bob Pappalardo, Cassini project scientist at NASA's Jet Propulsion Laboratory.

The Huygens probe, built and managed by the European Space Agency, was bolted to Cassini and rode along during its nearly seven-year journey to Saturn. Huygens' descent marked mankind's first and only attempt to land a probe on another world in the outer solar system.

Huygens transmitted data for more than four hours, as it plunged through Titan's hazy atmosphere and landed near a region now known as Adiri. Atmospheric density measurements from Huygens have helped engineers refine calculations for how low Cassini can fly through the moon's thick atmosphere.

Huygens captured the most attention for providing the first view from inside Titan's atmosphere and on its surface. The pictures of drainage channels and pebble-sized ice blocks surprised scientists with the extent of the moon's similarity to Earth. They showed evidence of erosion from methane and ethane rain.

"It was eerie," said Jonathan Lunine, an interdisciplinary Cassini scientist at the University of Rome, Tor Vergata, and University of Arizona, Tucson, and was with the Huygens camera team five years ago as they combed through the images coming down. "We saw bright hills above a dark plain, a weird combination of light and dark. It was like seeing a landscape out of Dante."

Combining these images with detections of methane and other gasses emanating from the surface, scientists came to believe Titan had a hydrologic cycle similar to Earth's, though Titan's cycle depends on methane and ethane rather than water. Titan is the only other body in the solar system other than Earth believed to have an active hydrologic cycle.

Huygens also gave scientists an opportunity to make electric field measurements from the atmosphere and surface, revealing a signature consistent with a water-and-ammonia ocean under an icy crust.

While the Huygens probe itself remains inactive on the Titan surface, insights inspired by the probe continue and ESA has convened a conference this week to extend the discussion, said Jean-Pierre Lebreton, Huygens Project Scientist for ESA.

"Huygens was a unique, once-in-a-lifetime mission," he said. "But we still have a lot to learn and I hope it will provide guidance for future missions to Titan."

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. JPL, a division of the California Institute of Technology in Pasadena, manages the Cassini mission for NASA's Science Mission Directorate, Washington, D.C. JPL designed, developed and assembled the Cassini orbiter. Huygens data was sent to NASA's Cassini spacecraft, and was recorded and relayed to Earth by NASA's Deep Space Network. JPL also manages the Deep Space Network.

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Dune Symmetry Inside Martian Crater

Dune symmetry inside Martian crater

Dunes of sand-sized materials have been trapped on the floors of many Martian craters. This is one example, from a crater in Noachis Terra, west of the giant Hellas impact basin.

The High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter captured this view on Dec. 28, 2009.

The dunes here are linear, thought to be due to shifting wind directions. In places, each dune is remarkably similar to adjacent dunes, including a reddish (or dust colored) band on northeast-facing slopes. Large angular boulders litter the floor between dunes.

The most extensive linear dune fields know in the solar system are on Saturn's large moon Titan. Titan has a very different environment and composition, so at meter-scale resolution they probably are very different from Martian dunes.

This image covers a swath of ground about 1.2 kilometers (three-fourth of a mile) wide, centered at 42.7 degrees south latitude, 38.0 degrees east longitude. It is one product from HiRISE observation ESP_016036_1370. The season on Mars is southern-hemisphere autumn. Other image products from this observation are available at http://hirise.lpl.arizona.edu/ESP_016036_1370.

The University of Arizona, Tucson, operates the HiRISE camera, which was built by Ball Aerospace & Technologies Corp., Boulder, Colo. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology, Pasadena, manages the Mars Reconnaissance Orbiter for the NASA Science Mission Directorate, Washington. Lockheed Martin Space Systems, Denver, is the prime contractor for the project and built the spacecraft.

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GOES-P Spacecraft Being Processed in Florida

On Cape Canaveral Air Force Station in Florida, the core stage of a Delta IV rocket arrives at Launch Complex 37During the first three weeks in January, the latest in the series of Geostationary Operational Environmental Satellites also known as GOES-P is being processed and prepped for launch. Meanwhile, the first and second stages of the Delta IV rocket that will carry it into orbit, are being assembled on the launch pad.

The GOES-P spacecraft is currently being processed at Astrotech Space Operations in Titusville, Florida. Prior to the holiday break the Payload Attached Fitting (PAF) fit check was successfully completed on December 18, 2009. Functional testing on the spacecraft bus (the satellite) was successfully completed on December 22, 2009.

The NASA Team at the Shuttle Landing Facility in Florida poses after GOES-P arrivesOver the last couple of weeks, the GOES-P spacecraft team commenced with instrument testing and cleaning on the Solar X-Ray Imager and the Imager and Sounder. Testing has completed on schedule and performance is as expected.

The first and second stage of the Delta IV rocket were mated in the United Launch Alliance (ULA) Horizontal Integrating Facility on Jan.6. Following the vehicle mate the rocket was transported to the launch pad (Pad 37B) at the Cape Canaveral Air Force Station on January 13th. The vehicle was successfully erected and stands ready for further processing and testing. The smaller solid rocket boosters are expected to be transported to the pad and integrated on January 14-15.

The GOES-P spacecraft being removed from the aircraft that transported it to NASA's Kennedy Space CenterAndre' Dress, GOES N-P Deputy Project Manager at NASA's Goddard Space Flight Center in Greenbelt, Md. said, "Our team has made incredible strides in the past few weeks. Just coming off the successful launch and check out of GOES O, everyone is ready to go again and we are anxious to see GOES P added to the NOAA constellation."

Launch is targeted for no earlier than March 1.

For information on GOES-P, visit

http://goespoes.gsfc.nasa.gov/goes/spacecraft/n_p_spacecraft.html.

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Head of NASA Space Operations Honored With National Space Trophy

NASA Associate Administrator for Space Operations Bill GerstenmaierNASA Associate Administrator for Space Operations Bill Gerstenmaier has been selected to receive the 2010 National Space Trophy The award is the highest honor bestowed by the Rotary National Award for Space Achievement (RNASA) Foundation. Each year, the foundation presents the trophy to an outstanding American who has made major contributions to our nation's space program. Previous awardees include former NASA Administrator Dan Goldin; NASA astronaut Neil Armstrong; Apollo 11 Flight Director Gene Kranz and President George H.W. Bush.

Since 2005, Gerstenmaier has been responsible for overseeing the International Space Station and Space Shuttle programs, space communications and space launch vehicles.

Lesa B. Roe, director of NASA Langley Research Center in Virginia, former NASA Administrator Mike Griffin, NASA Johnson Space Center Director Mike Coats, and RNASA Advisor and Apollo 17 Astronaut Harrison Schmitt nominated Gerstenmaier for the National Space Trophy.

"Gerstenmaier's career achievements and personal initiatives have had a direct impact on the current U.S. human space flight program, the international community, and residents of planet Earth," said Roe. "His efforts will continue to shape the future of space exploration for many years to come."

The National Space TrophyGriffin said, "It was my honor to work with Bill for four years. Quite simply, Bill Gerstenmaier is regarded as the ultimate authority on the space shuttle and International Space Station. When he says something, people listen, and they know that what he says is true."

Coats added, "Bill's impact in the space community is unparalleled. He has literally guided an international group of thousands of individuals in many countries in furthering human space flight and assuring a continued human presence in space. The partnerships we currently enjoy with our international partners for the ISS are largely due to Bill's tremendous efforts and diligence."

Gerstenmaier will formally be recognized at a RNASA gala on April 30. The seven-foot, 500-pound lead crystal trophy is on display at Space Center Houston.

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Infrared Hunt Begins: WISE Starts All-Sky Survey

Artist's concept of WISE mapping the infrared sky

NASA's Wide Field Infrared Survey Explorer (WISE) began its survey of the infrared sky today. The mission will spend nine months scanning the sky one-and-a-half times in infrared light, revealing all sorts of cosmic characters -- everything from near-Earth asteroids to young galaxies more than ten billion light-years away.

WISE, which launched Dec. 14, 2009, from Vandenberg Air Force Base in California, will uncover hundreds of thousands of asteroids, and hundreds of millions of stars and galaxies. Its vast catalog of data will provide astronomers and other missions with data for mine for decades to come.

NASA's Jet Propulsion Laboratory manages the Wide-field Infrared Survey Explorer for NASA's Science Mission Directorate, Washington. The principal investigator, Edward Wright, is at UCLA. The mission was competitively selected under NASA's Explorers Program managed by the Goddard Space Flight Center, Greenbelt, Md. The science instrument was built by the Space Dynamics Laboratory, Logan, Utah, and the spacecraft was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Science operations and data processing take place at the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena. Caltech manages JPL for NASA. More information is online at http://www.nasa.gov/wise, http://wise.astro.ucla.edu and http://www.jpl.nasa.gov/wise .

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NASA Satellite, Natural Hazard Networks Supporting Disaster Recovery

Haiti
An image of Port au Prince, Haiti, captured by NASA's Earth Observing-1 satellite on Jan. 15, 2010, shows damage to the city's pier, when compared with an image from Sept. 2008. Credit: NASA
› Full Story

NASA's considerable Earth-observing and data analysis and distribution capabilities have been mobilized to provide information to support disaster recovery efforts in Haiti after the devastating Jan. 12 earthquake.

NASA has tasked two of its space-based, high-resolution instruments to image areas hardest hit by the earthquake. Before-and-after scenes of Port-au-Prince, for example, will be used to aid with damage assessment and recovery.

The Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER), a Japanese-U.S. instrument with visible, infrared and thermal infrared sensors flying on the Terra spacecraft, took observations of the region on Jan. 14. The data are being processed and compared with pre-earthquake imagery. ASTER will again revisit the area on Jan. 19 and Jan. 21.

NASA's Earth Observing-1 (EO-1) satellite is scheduled to obtain multispectral images of the region on Jan. 15.

NASA and the NASA-funded SERVIR Rapid Response Mapping team at the Center for Water in the Humid Tropics in Latin America and the Caribbean are on standby to support the damage assessment efforts once EO-1 and ASTER data are available.

NASA is coordinating its efforts with international space agencies through the United Nations Platform for Space-based Information for Disaster Management and Emergency Response, as well as agreements with the Committee on Earth Observations and the Group on Earth Observations.

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STS-129 Crew Meets With Members of Congress

NASA Administrator Charles Bolden, the STS-129 space shuttle crew and members of the Congressional Black Caucus pose for a group photo at the Capitol Building, Wednesday, Jan. 13, 2010, in Washington. Back row from left to right: U.S. Rep Donna Edwards (D-MD), U.S. Rep Diane Watson (D-CA), NASA Administrator Charles Bolden, astronauts Leland Melvin, Mike Forman, Robert Satcher, Barry Wilmore, Randy Breznik, and U.S. Rep Mel Watt (D-NC). Front row from left to right: U.S. Rep Robert Scott (D-VA), U.S. Rep. Corrine Brown (D-Fla), U.S. Rep. Barbara Lee (D-CA), U.S. Rep. Donna Christensen (D-VI) and U.S. Rep. Donald Payne (D-NJ). The crew of STS-129 presented the CBC with a montage commemorating the shuttle mission.

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President Honors Outstanding Early-Career Scientists

Today at the White House, President Obama will honor more than 100 outstanding early career scientists–the latest winners of the Presidential Early Career Award for Scientists and Engineers, including NASA scientists Benjamin Smith and Joshua K. Willis. The award is the highest honor bestowed by the United States government on scientists and engineers in the early stages of their independent research careers. Annually, nine federal departments and agencies nominate the most meritorious young scientists and engineers--researchers whose early accomplishments show the greatest promise for strengthening America’s leadership in science and technology and contributing to the awarding agencies' missions.

"You have been selected for this honor not only because of your innovative research, but also for your demonstrated commitment to community service and public outreach," President Obama said in a letter to the winners. "Your achievements as scientists, engineers and engaged citizens are exemplary, and the value of your work is amplified by the inspiration you provide to others."

The awards, established by President Clinton in February 1996, are coordinated by the Office of Science and Technology Policy within the Executive Office of the President. Awardees are selected on the basis of two criteria: Pursuit of innovative research at the frontiers of science and technology and a commitment to community service as demonstrated through scientific leadership, public education or community outreach. Winning scientists and engineers receive up to a five-year research grant to further their study in support of critical government missions.

NASA recipient Joshua K. Willis' research focuses on the system of ocean currents called the Atlantic Meridional Overturning Circulation (AMOC). The AMOC helps to regulate the climate across much of Europe and throughout the North Atlantic. It has been theorized that this circulation could play a role in rapid climate change, causing cooling in some regions even as the planet warms overall. AMOC’s exact role in global warming, however, remains a mystery. Using data from several NASA satellites along with observations taken by thousands of Argo floats, which autonomously measure ocean properties and currents, Willis has developed a novel technique for estimating the strength of the AMOC and how it changes over time.

Benjamin Smith’s research is in the area of understanding changes in the Earth’s ice sheets and their contributions to sea level using satellite remote sensing. In particular, he has been a leader in the analysis of ICESat data and has been a key figure in the science definition activities of ICESat-ll. He has been instrumental in extracting elevation change information from ICESat in its compromised operations scenario (as a result of the premature failure of two of ICESat’s three lasers) and has published some of the most significant ICESat-based ice sheet change assessments to date.

Read the White House press release for more information.

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Is Antarctica Melting?

The continent of Antarctica has been losing more than 100 cubic kilometers (24 cubic miles) of ice per year since 2002There has been lots of talk lately about Antarctica and whether or not the continent's giant ice sheet is melting. One new paper 1, which states there’s less surface melting recently than in past years, has been cited as "proof" that there’s no global warming. Other evidence that the amount of sea ice around Antarctica seems to be increasing slightly 2-4 is being used in the same way. But both of these data points are misleading. Gravity data collected from space using NASA's Grace satellite show that Antarctica has been losing more than a hundred cubic kilometers (24 cubic miles) of ice each year since 2002. The latest data reveal that Antarctica is losing ice at an accelerating rate, too. How is it possible for surface melting to decrease, but for the continent to lose mass anyway? The answer boils down to the fact that ice can flow without melting.

Two-thirds of Antarctica is a high, cold desert. Known as East Antarctica, this section has an average altitude of about 2 kilometer (1.2 miles), higher than the American Colorado Plateau. There is a continent about the size of Australia underneath all this ice; the ice sheet sitting on top averages at a little over 2 kilometer (1.2 miles) thick. If all of this ice melted, it would raise global sea level by about 60 meter (197 feet). But little, if any, surface warming is occurring over East Antarctica. Radar and laser-based satellite data show a little mass loss at the edges of East Antarctica, which is being partly offset by accumulation of snow in the interior, although a very recent result from the NASA/German Aerospace Center's Gravity Recovery and Climate Experiment (Grace) suggests that since 2006 there has been more ice loss from East Antarctica than previously thought 5. Overall, not much is going on in East Antarctica -- yet.

A Frozen Hawaii

West Antarctica is very different. Instead of a single continent, it is a series of islands covered by ice -- think of it as a frozen Hawaii, with penguins. Because it's a group of islands, much of the West Antarctic Ice Sheet (WAIS, in the jargon) is actually sitting on the floor of the Southern Ocean, not on dry land. Parts of it are more than 1.7 kilometer (1 mile) below sea level. Pine Island is the largest of these islands and the largest ice stream in West Antarctica is called Pine Island Glacier. The WAIS, if it melted completely, would raise sea level by 5 to 7 meter (16 to 23 feet). And the Pine Island Glacier would contribute about 10 percent of that.

The Antarctic ice sheet. East Antarctica is much higher in elevation than West Antarctica

Since the early 1990s, European and Canadian satellites have been collecting radar data from West Antarctica. These radar data can reveal ice motion and, by the late 1990s, there was enough data for scientists to measure the annual motion of the Pine Island Glacier. Using radar information collected between 1992 and 1996, oceanographer Eric Rignot, based at NASA’s Jet Propulsion Laboratory (JPL), found that the Pine Island Glacier's "grounding line" -- the line between the glacier's floating section and the part of the glacier that rests on the sea floor -- had retreated rapidly towards the land. That meant that the glacier was losing mass. He attributed the retreat to the warming waters around West Antarctica 6. But with only a few years of data, he couldn't say whether the retreat was a temporary, natural anomaly or a longer-term trend from global warming.

Rignot's paper surprised many people. JPL scientist Ron Kwok saw it as demonstrating that "the old idea that glaciers move really slowly isn't true any more." One result was that a lot more people started to use the radar data to examine much more of Antarctica. A major review published in 2009 found that Rignot's Pine Island Glacier finding hadn't been a fluke 7: a large majority of the marine glaciers of the Antarctic Peninsula were retreating, and their retreat was speeding up. This summer, a British group revisited the Pine Island Glacier finding and found that its rate of retreat had quadrupled between 1995 and 2006 8.

How the Ice Shelf Crumbles

The retreat of West Antarctica's glaciers is being accelerated by ice shelf collapse. Ice shelves are the part of a glacier that extends past the grounding line towards the ocean they are the most vulnerable to warming seas. A longstanding theory in glaciology is that these ice shelves tend to buttress (support the end wall of) glaciers, with their mass slowing the ice movement towards the sea, and this was confirmed by the spectacular collapse of the Rhode Island-sized Larsen B shelf along the Eastern edge of the Antarctic Peninsula in 2002. The disintegration, which was caught on camera by NASA's Moderate Resolution Imaging Spectroradiometer (MODIS) imaging instruments on board its Terra and Aqua satellites, was dramatic: it took just three weeks to crumble a 12,000-year old ice shelf. Over the next few years, satellite radar data showed that some of the ice streams flowing behind Larsen B had accelerated significantly, while others, still supported by smaller ice shelves, had not 9. This dynamic process of ice flowing downhill to the sea is what enables Antarctica to continue losing mass even as surface melting declines.

Michael Schodlok, a JPL scientist who models the way ice shelves and the ocean interact, says melting of the underside of the shelf is a pre-requisite to these collapses. Thinning of the ice shelf reduces its buttressing effect on the glacier behind it, allowing glacier flow to speed up. The thinner shelf is also more likely to crack. In the summer, meltwater ponds on the surface can drain into the cracks. Since liquid water is denser than solid ice, enough meltwater on the surface can open the cracks up deeper down into the ice, leading to disintegration of the shelf. West Antarctica is a series of islands covered by ice. Think of it as a frozen Hawaii, with penguinsThe oceans surrounding Antarctica have been warming 10, so Schodlok doesn't doubt that the ice shelves are being undermined by warmer water being brought up from the depths. But he admits that it hasn't been proven rigorously, because satellites can’t measure underneath the ice.

Glaciologist Robert Bindschadler of NASA's Goddard Space Flight Center intends to show just that. He's leading an expedition scheduled to start in 2011 to drill through the Pine Island Glacier and place an automated buoy into the water below it. According to Bindschadler, Pine Island Glacier "is the place to go because that is where the changes are the largest. If we want to understand how the ocean is impacting the ice sheet, go to where it's hitting the ice sheet with a sledgehammer, not with a little tack hammer."

Meanwhile, measurements from the Grace satellites confirm that Antarctica is losing mass 11. Isabella Velicogna of JPL and the University of California, Irvine, uses Grace data to weigh the Antarctic ice sheet from space. Her work shows that the ice sheet is not only losing mass, but it is losing mass at an accelerating rate. "The important message is that it is not a linear trend. A linear trend means you have the same mass loss every year. The fact that it’s above linear, this is the important idea, that ice loss is increasing with time," she says. And she points out that it isn’t just the Grace data that show accelerating loss; the radar data do, too. "It isn't just one type of measurement. It's a series of independent measurements that are giving the same results, which makes it more robust."

For more information about this topic, visit NASA's Global Climate Change website.

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Asteroid To Fly By Earth Wednesday Is a Natural

Orbital diagram depicts the trajectory of asteroid 2010 AL30 during its flyby of Earth in the early morning hours of Jan. 13.
Asteroid 2010 AL30, discovered by the LINEAR survey of MIT's Lincoln Laboratories on Jan. 10, will make a close approach to the Earth's surface to within 76,000 miles on Jan. 13 at 12:46 pm Greenwich time (7:46 am EST, 4:46 am PST). Because its orbital period is nearly identical to the Earth's one year period, some have suggested it may be a manmade rocket stage in orbit about the sun. However, this object's orbit reaches the orbit of Venus at its closest point to the sun and nearly out to the orbit of Mars at its furthest point, crossing the Earth's orbit at a very steep angle. This makes it very unlikely that 2010 AL30 is a rocket stage. Furthermore, trajectory extrapolations show that this object cannot be associated with any recent launch and it has not made any close approaches to the Earth since well before the Space Age began.

It seems more likely that this is a near-Earth asteroid about 10-15 meters in size, one of approximately 2 million such objects in near-Earth space. One would expect a near-Earth asteroid of this size to pass within the moon's distance about once every week on average. The asteroid does not pose a risk, in fact, stony asteroids under 25 meters in diameter would be expected to burn up in our atmosphere, causing little or no ground damage.

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Solar Scientists Use ‘Magnetic Mirror Effect’ to Reproduce IBEX Observation

entire sky in the emission of neutral hydrogenEver since NASA's Interstellar Boundary Explorer, or IBEX, mission scientists released the first comprehensive sky map of our solar system's edge in particles, solar physicists have been busy revising their models to account for the discovery of a narrow "ribbon" of bright emission that was completely unexpected and not predicted by any model at the time.

Further study by a team of scientists funded through NASA's Heliophysics Guest Investigator program has produced a revised model that explains and closely reproduces the IBEX result by incorporating a single new effect into an existing model. The new effect, put forward by the IBEX team soon after sighting of the ribbon, is that the magnetic field surrounding our solar system—called the local galactic magnetic field—acts like a mirror for the particles that IBEX sees.

The results appear in the January 10 issue of the Astrophysical Journal Letters. Jacob Heerikhuisen, a solar physicist at the University of Alabama in Huntsville, is the lead author of the paper. Heerikhuisen and his colleagues believe the orientation of the local galactic magnetic field is closely related to the location of the ribbon in the sky.

Charged particles "orbit" magnetic field lines. When they suddenly lose their charge, they fly off in a straight line maintaining their current direction. Only particles that orbit the magnetic mirror, where it faces us directly, can flow back toward us and are captured by IBEX.

These particles originate in our magnetized solar system, or heliosphere—the region from the sun to where the solar wind meets the local interstellar medium (LISM). First these particles lose their charge and fly out of the heliosphere. At some distance they charge again and start “orbiting” a field line of the local interstellar magnetic field, where they get “recycled” by losing their charge again.

entire sky in the emission of neutral hydrogenSolar physicists did not expect this “mirror effect,” which is "somewhat analogous to exploring an unknown cave," says Arik Posner, IBEX program scientist at NASA Headquarters. "By activating IBEX, we suddenly see that the solar system has a lit candle and see its light reflected in the 'cave walls' shining back at us," says Posner. "What we find is that the 'cave wall' acts more like a faint mirror than like a normal wall," he adds.

What we saw with IBEX is that this “cave” we are exploring apparently has very straight and smooth magnetic walls, being shaped somewhat like a subway tunnel. IBEX can remotely observe the direction of the local interstellar magnetic field and may observe whether it stays the same or changes over time.

The sun’s presence affects the local interstellar magnetic field, bulging the field out to form something larger that is similar to a subway station. However, the “station” itself, our heliosphere, slowly moves along the tunnel, not subway cars.

Straight magnetic field lines are only found in plasmas where the magnetic field is strong and shapes the flow of particles, such as the smooth magnetic loops observed in the sun’s corona.

The IBEX results appear consistent with a recent finding by the Voyager mission that the surrounding galactic magnetic field in the LISM is much stronger than previously thought.

Assuming this "magnetic mirror effect" produces the narrow "ribbon" discovered by IBEX, then the orientation of the local galactic magnetic field is closely related to the location of the ribbon. With the help of global 3D models, this mechanism could help accurately determine the magnetic field's direction. The finding would also suggest that IBEX is detecting the particles from both inside and outside the heliopause, which is the boundary region between the outer solar system and the local interstellar medium.

"The IBEX mission has from the outset stressed both the criticality of new measurements and the collaboration between observations and theoretical research," explains Robert MacDowall, IBEX mission scientist at NASA Goddard. "The discovery by Heerikhuisen and colleagues demonstrates how successful this approach can be."

The IBEX spacecraft was launched in October 2008. Its science objective was to discover the nature of the interactions between the solar wind and the interstellar medium at the edge of our solar system. The Southwest Research Institute developed and leads the mission with a team of national and international partners. The spacecraft is the latest in NASA's series of low-cost, rapidly developed Small Explorers Program. NASA's Goddard Space Flight Center manages the program for the agency's Science Mission Directorate at NASA Headquarters in Washington.

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NASA’s New Museum Grant Allies Will Make the Universe Accessible to Families From Alaska to Florida

Interactive museum exhibits about climate change, Earth science, and missions beyond Earth are among the projects NASA has selected to receive agency funding. Nine informal education providers from Alaska to New York will share $6.2 million in grants through NASA's Competitive Program for Science Museums and Planetariums.

Participating organizations include museums, science centers, Challenger Centers and other institutions of informal education. Selected projects will partner with NASA's Museum Alliance, an Internet-based, nationwide network of more than 400 science centers, planetariums, museums, aquariums, zoos, observatory visitor centers, NASA visitor centers, nature centers and park visitor centers.

Projects in the program will engage learners of all ages as well as educators who work in formal or informal science education. The projects will provide NASA-inspired space, science, technology, engineering or mathematics educational opportunities, including planetarium shows and exhibits.

In conjunction with NASA's Museum Alliance, the grants focus on NASA-themed space exploration, aeronautics, space science, Earth science, microgravity or a combination of themes. Some projects will include partnerships with elementary and secondary schools, colleges and universities.

The projects are located in Alaska, Colorado, Florida, Illinois, New York, North Carolina, Oregon and South Dakota. The nine grants have a maximum five-year period of performance and range in value from approximately $120,000 to $1.5 million. Selected projects work with the NASA Shared Service Center in Mississippi to complete the business review necessary before a NASA award is issued.

Proposals were selected through a merit-based, external peer-review process. NASA's Office of Education and mission directorates collaborated to solicit and review the grant applications. This integrated approach distinguishes NASA's investment in informal education. NASA received 67 proposals from 32 states and the District of Columbia.

Congress initially funded the Competitive Program for Science Museums and Planetariums grants in 2008. The first group of projects began in fall 2009 in California, Colorado, Florida, Illinois, Iowa, Minnesota, Michigan, Montana, New York, North Carolina, Vermont and Washington. Congress has enacted funds to continue this program in 2010, and NASA anticipates selecting additional proposals to fund from those submitted in 2009.

For a list of selected organizations and projects descriptions, click on "Selected Proposals" and look for "Competitive Program for Science Museums and Planetariums (CP4SMP)" or solicitation NNH09ZNE005N at:

http://nspires.nasaprs.com

For information about NASA's Education programs, visit:

http://www.nasa.gov/education

NASA's Jet Propulsion Laboratory in Pasadena, Calif., leads the Museum Alliance. For information about the alliance, visit:

http://informal.jpl.nasa.gov/museum

For more information about NASA and agency programs, visit:

http://www.nasa.gov

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Meet the Next International Space Station Crew: NASA Holds Briefing and One-On-One Media Interviews on Jan. 21

NASA will hold a briefing for journalists with the next set of residents of the International Space Station at 1 p.m. CST Thursday, Jan. 21, from NASA's Johnson Space Center in Houston. The briefings will be broadcast live on NASA Television and the agency's Web site. Questions also will be taken from participating NASA locations.

The briefing participants are:
- Expedition 23 Flight Engineer and NASA astronaut Tracy Caldwell Dyson
- Expedition 23 Flight Engineer and Russian cosmonaut Alexander Skvortsov
- Expedition 23 Flight Engineer and Russian cosmonaut Mikhail Kornienko

Following the briefing, the crew members will be available for individual round-robin interviews, in person or by phone. There also will be a photo opportunity. To participate in the interviews, reporters should contact the Johnson newsroom at 281-483-5111, by 4 p.m. CST, Wednesday, Jan. 20. U.S. and foreign nationals planning to attend the news briefing must contact the Johnson newsroom by 4 p.m. Thursday, Jan. 14, to arrange credentials.

On April 2, Skvortsov, Kornienko, and Caldwell Dyson will launch to the station aboard a Russian Soyuz spacecraft. They will dock to the space station on April 4, joining Russian cosmonaut Oleg Kotov, NASA astronaut T.J. Creamer and Japan Aerospace Exploration Agency (JAXA) astronaut Soichi Noguchi, who arrived on the station in December as part of Expedition 22.

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

http://www.nasa.gov/ntv

For the latest information about Expedition 23 and its crew, visit:

http://www.nasa.gov/station

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Martian Landform Observations Fill Special Journal Issue

This view shows color variations in bright layered deposits on a plateau near Juventae Chasma in the Valles Marineris region of Mars.
This view shows color variations in bright layered deposits on a plateau near Juventae Chasma in the Valles Marineris region of Mars.
› Full image and caption

Martian landforms shaped by winds, water, lava flow, seasonal icing and other forces are analyzed in 21 journal reports based on data from a camera orbiting Mars.

The research in a January special issue of Icarus testifies to the diversity of the planet being examined by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter. Examples of the findings include:

-- Valleys associated with light-toned layered deposits in several locations along the plateaus adjacent to the largest canyon system on Mars suggest low-temperature alteration of volcanic rocks by acidic water both before and after formation of the canyons.

-- The youngest flood-lava flow on Mars, found in the Elysium Planitia region and covering an area the size of Oregon, is the product of a single eruption and was put in place turbulently over a span of several weeks at most.

-- New details are observed in how seasonal vanishing of carbon-dioxide ice sheets in far-southern latitudes imprints the ground with fan-shaped and spider-shaped patterns via venting of carbon-dioxide gas from the undersurface of the ice.

HiRISE is operated by the University of Arizona, Tucson, and was built by Ball Aerospace & Technologies Corp., Boulder, Colo. It is one of six instruments on NASA's Mars Reconnaissance Orbiter, which is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., and was built by Lockheed Martin Space Systems, Denver. The U.S. Geological Survey Astrogeology Science Center, Flagstaff, Ariz., played a special role in preparation of the special issue, providing two guest editors and authorship of multiple papers. For more information, see http://hirise.lpl.arizona.edu

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NASA Briefings to Preview Year’s First Space Shuttle Mission Rescheduled

The news briefings to preview the year's first space shuttle mission have been rescheduled to Friday, Jan. 29, at NASA's Johnson Space Center in Houston. NASA Television and the agency's Web site will broadcast the briefings live. Reporters may ask questions from participating NASA locations.

The series of briefings will focus on shuttle Endeavour's STS-130 mission to deliver the final module of the U.S. portion of the International Space Station. The briefings have been rescheduled to allow more analysis of engineering data from the test of high-pressure ammonia jumper hose assemblies that failed during a prelaunch test last week. The results will determine if there will be any impact to the shuttle mission. Teams continue to work toward a target launch of Feb. 7.

Previously submitted requests from reporters for credentials to attend the briefings, or to participate in round-robin interviews with an STS-130 astronaut, will be adjusted for the new date and do not need to be resubmitted. Reporters who have not requested credentials and are planning to attend the briefings in Houston must contact the Johnson newsroom at 281-483-5111 by 5 p.m. CST, on Jan. 21.

Endeavour's six astronauts will be available for interviews at Johnson. New requests to reserve an interview slot should be submitted to Gayle Frere at 281-483-8645 by Jan. 21.

The updated schedule of briefings (all times CST) is:
8 a.m. - STS-130 Video B-Roll feed
9 a.m. - STS-130 Mission Overview Briefing
10:30 a.m. - STS-130 Spacewalk Overview Briefing
11:30 a.m. - NASA TV Video File
1 p.m. - Crew News Conference

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

http://www.nasa.gov/ntv

For the latest information about the STS-130 mission and its crew, visit:

http://www.nasa.gov/shuttle

For the latest information on the space station, visit:

http://www.nasa.gov/station

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Cassini Returns to Southern Hemisphere of Titan

Artist's concept of Cassini's Jan. 12, 2010NASA'S Cassini spacecraft will return to Titan's southern hemisphere on a flyby tomorrow, Jan. 12, plunging to within about 1,050 kilometers (about 670 miles) of the hazy moon's surface. During this pass, the onboard radar instrument will scan Ontario Lacus, the largest lake in the southern hemisphere, in a quest to learn more about the liquid methane and ethane in the lake and obtain more detailed topographical information about the shoreline. Titan is the only other body in the solar system besides Earth that is known to have stable liquid on its surface.

This will also be the most southern pass in the mission for the ion and neutral mass spectrometer instrument, which will probe the composition and density of the atmosphere near Titan's south pole. The atmospheric data collected on this pass will be paired with a similar sampling mission near Titan's north pole during the most recent flyby, 16 days earlier.

Cassini last flew by Titan on Dec. 27, 2009 California time, or Dec. 28 Universal Time. Although this latest flyby is dubbed "T65," planning changes early in the orbital tour have made this the 66th targeted flyby of Titan. This flyby also comes two days before the fifth anniversary of the landing of the Huygens probe on the surface of Titan.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. JPL, a division of the California Institute of Technology in Pasadena, manages the Cassini mission for NASA's Science Mission Directorate, Washington, D.C. JPL designed, developed and assembled the Cassini orbiter. The Huygens probe, built and managed by the European Space Agency, was bolted to Cassini and rode along during its nearly seven-year journey to Saturn, before being released for its descent through Titan's atmosphere.

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