NASA Honors 2009 Centennial Challenges Winners

NASA will honor the achievements of the 2009 Centennial Challenges prize winners and competition hosts with a technical symposium Feb. 25 and a recognition ceremony Feb. 26. Centennial Challenges is NASA's program of technology prizes for the citizen-inventor. Nine prizes totaling $3.65 million were awarded in 2009. Both events will be held at the James E. Webb Memorial Auditorium at NASA Headquarters, 300 E Street, SW, Washington.

The Centennial Challenges Technical Symposium will take place from 9 a.m. to 4:30 p.m. EST Thursday, Feb. 25. Winners will discuss their accomplishments and future plans and answer questions from the audience. A one-hour panel discussion will be dedicated to each of the challenges, including the new Green Flight Challenge and ongoing Strong Tether and Power Beaming Challenges. The public is invited, and government, industry and media representatives interested in the technologies and incentive prize competitions are encouraged to attend.

The recognition ceremony will begin at 10 a.m. on Friday, Feb. 26. NASA Administrator Charles Bolden will participate, as will winners of the Regolith Excavation, Lunar Lander, Power Beaming and Astronaut Glove Challenges. Reporters will have an opportunity to talk with the winners during a reception in the NASA Headquarters West Lobby immediately following the one-hour ceremony.

The competitions address a range of technical challenges that support NASA's missions in aeronautics and space with a goal of encouraging novel solutions from non-traditional sources. The partner organizations that conducted the competitions are: California Space Education and Workforce Institute (Regolith Excavation), X Prize Foundation (Lunar Lander), Spaceward Foundation (Power Beaming and Strong Tether), Volanz Aerospace Inc. (Astronaut Glove) and Comparative Aircraft Flight Efficiency Foundation (Green Flight). NASA's Innovative Partnerships Program manages the Centennial Challenges.

NASA Television will broadcast the events. For NASA TV downlink, schedule and streaming video information, visit:

http://www.nasa.gov/ntv

For additional information about the Centennial Challenges, visit:

http://www.nasa.gov/challenges

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NASA Finds Warmer Ocean Speeding Greenland Glacier Melt

Calving front of Equp Sermia glacier, West Greenland
Calving front of Equp Sermia glacier, West Greenland, one of the four glaciers studied by Rignot and his team. Image credit: Michele Koppes, University of British Columbia
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Glaciers in west Greenland are melting 100 times faster at their end points beneath the ocean than they are at their surfaces, according to a new NASA/university study published online Feb. 14 in Nature Geoscience. The results suggest this undersea melting caused by warmer ocean waters is playing an important, if not dominant, role in the current evolution of Greenland's glaciers, a factor that had previously been overlooked.

Researchers Eric Rignot and Isabella Velicogna, both of NASA's Jet Propulsion Laboratory, Pasadena, Calif., and the University of California, Irvine; along with colleague Michele Koppes of the University of British Columbia, Vancouver, Canada, measured the undersea melting rates of four glaciers in central west Greenland in the summer of 2008. They deployed oceanographic equipment in the glacier fjords, sampling the water at various depths to measure ocean currents, temperature and salinity, along with the depth of the fjords. The researchers found the melt rates of the glaciers studied was 100 times larger under the ocean at their terminus points than that observed at the glacial surfaces.

Rignot said the new study complements other recent research on the effects of ocean conditions in Greenland fjords. A study in the same online issue of Nature Geoscience by researcher Fiammetta Straneo of the Woods Hole Oceanographic Institution, Woods Hole, Mass., and colleagues looked at changes in oceanographic conditions in fjords that may be conducive to changes in undersea melting. Another 2008 Nature Geoscience study by researcher David Holland of New York University, New York, found that Greenland glaciers sped up as warm waters intruded into their fjords.

"Our study fills the gap by actually looking at these submarine melt rates, something that had never been done before in Greenland," Rignot said. "The results indicate rather large values that have vast implications for the evolution of the glaciers if ocean waters within these fjords continue to warm."

In recent years, scientists have observed a widespread acceleration of Greenland's glaciers, associated with thinning of their lower reaches as they reach the sea. In the past decade, surface melting of glaciers around Greenland due to warm air temperatures has increased in both magnitude and area, while snowfall has increased just slightly. The result is a tripling in the amount of ice mass lost in Greenland between 1996 and 2007. Of this loss, between 50 and 60 percent is attributable to a speedup in the flow of outlet glaciers, with the remainder due to increased surface melting.

But the glaciers also melt along their submerged faces, where they come into contact with warm ocean waters. A warmer ocean erodes a glacier's submerged, grounded ice and causes its grounding line -- the point at which a tidewater glacier floats free of its bed -- to retreat. Little is known about these rates of undersea melting and how they may influence the glaciers. The only previous measurements of undersea glacier melting were in Alaska.

The melting of glaciers beneath the ocean surface causes deep, warm, salty water to be drawn up toward the glacier's face, where it mixes turbulently with the glacier's cold, fresh water. The water then rises along the glacier face, melting its ice along the way, then reaches the ocean surface and flows away from the glacier in a plume. An ocean temperature of 3 degrees Celsius (37.4 degrees Fahrenheit) can melt glacial ice at a rate of several meters per day, or hundreds of meters over the course of a summer.

Rignot said the study points to the need to include the ocean factor if scientists are to increase the reliability of models used to predict how Greenland will be affected by climate change.

"All major Greenland glaciers end up in the ocean, and tidewater glaciers control 90 percent of the ice discharged by Greenland into the sea," Rignot said. "Submarine melting may therefore have a large indirect impact on the ice mass budget of the entire Greenland Ice Sheet. If we are to determine the future of the Greenland Ice Sheet more reliably in a changing climate, more complete and detailed studies of the interactions between ice and ocean at the ice sheet's margins are essential."

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Get Set for a Possible Glimpse of an Asteroid

Asteroid Vesta as seen by NASA's Hubble Space Telescope

Asteroid Vesta as seen by NASA's Hubble Space Telescope.

The most prominent asteroid in the sky is currently yours for the perusing with b-- and perhaps even the naked eye.

Tomorrow night, Wednesday, Feb. 17, Vesta, the second most massive object in the asteroid belt, reaches what astronomers like to call "opposition." An asteroid (or planet or comet) is said to be "in opposition" when it is opposite to the sun as seen from Earth. In other words, if you were to stand outside with the sun directly above you at high noon, Vesta would be directly below your feet some 211,980,000 kilometers (131,700,000 miles) away. With Vesta at opposition, the asteroid is at its closest point to Earth in its orbit.

Wednesday night, the asteroid is expected to shine at magnitude 6.1. That brightness should make it visible to interested parties brandishing telescopes or binoculars, and even those blessed with excellent vision and little or no light pollution or clouds in their vicinity. Vesta will be visible in the eastern sky in the constellation Leo.

What makes this space rock so prominent these days? Along with its relative proximity at this point, a full half of the asteroid is being bathed by sunlight when seen from Earth, making it appear brighter. Another attribute working in the observer's favor is that Vesta has a unique surface material that is not as dark as most main belt asteroids - allowing more of the sun's rays to reflect off its surface.

If spotting Vesta in the night sky has whetted your appetite for mega-rocks, all we can say is, stay tuned. NASA's Dawn spacecraft, currently motoring its way through the asteroid belt, will begin its exploration of Vesta in the summer of 2011.

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

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Cassini Shoots New Close-Ups of Death Star-like Moon

Saturn's moon Mimas

Cassini captured this image of Mimas' giant Herschel Crater, which measures about 140 kilometers (88 miles) wide, during its Feb. 13, 2010, flyby of the Death Star-like Saturnian moon.

Blazing through its closest pass of the Saturnian moon Mimas on Feb. 13, Cassini sent back striking close-ups of the moon likened to the Death Star from "Star Wars" and the enormous crater scarring its surface. The flyby also yielded solid data on the moon's thermal signature and surface composition.

Some of the raw, unprocessed images sent back from the flyby show the bright, steep slopes of the giant Herschel Crater, which measures about 140 kilometers (88 miles) wide. The icy slopes appear to be pitched around 24 degrees, which would probably earn them a black- or double-black-diamond rating on Earth. Olympic downhill skiers could probably tear down these runs with ease, but it's clear Mimas is no place for bunny-slope beginners.

The images, which have the highest resolution so far, also show jumbled terrain inside the crater and many craters within the crater. These features hint at a long history, which scientists will be working diligently to analyze.

"This flyby has been like looking at a cell or an onion skin under the microscope for the first time," said Bonnie Buratti, one of the leads for the Satellite Orbiter Science Team. "We'd seen the large crater from afar since the early 1980s, but now its small bumps and blemishes are all clearly visible."

This encounter took the spacecraft as close as about 9,500 kilometers (5,900 miles) above Mimas. Cassini had to maneuver through a dusty region to get in position, but survived the trip unscathed, as expected.

The moon averages 396 kilometers (246 miles) in diameter. The walls of Herschel Crater are about 5 kilometers (3 miles) high, and parts of the floor are approximately 10 kilometers (6 miles) deep.

Unprocessed images of the flyby are available at http://saturn.jpl.nasa.gov/photos/raw/. More information about the Cassini mission is at http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov.

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Space Rocks! Moon and Mt. Everest Rocks Find a Home in Orbit

Former NASA astronaut Scott Parazynski (left) presents STS-130 Commander George Zamka (right) with a plaque containing moon rocks collected during the Apollo 11 mission and a rock from the summit of Mt. EverestMoon rocks, collected during the historic Apollo 11 mission, will find a new residence aboard the International Space Station alongside a piece of Mt. Everest.

On May 20, 2009, during his second attempt to reach the highest point on Earth’s continental crust, former NASA astronaut Scott Parazynski successfully carried the moon rocks with him to the summit of Mt. Everest. Part of the Himalaya range in Asia, Mt. Everest is located on the border between Sagarmatha Zone, Nepal and Tibet, China - a perilous journey for Parazynski and his team.

Parazynski collected a rock from the summit of Mt. Everest to accompany the lunar samples on their journey back to space.

Plaque containing rock collected from the summit of Mt. Everest (left) and moon rocks collected during the Apollo 11 mission (right)On Jan. 6, at Space Center Houston, Parazynski presented the rocks to NASA astronaut and STS-130 Commander George Zamka during a special ceremony. Zamka will deliver the rocks to the space station during Space Shuttle Endeavour's mission where they will reside in the Tranquility module, also being delivered to the station by the crew.

Fittingly, the moon rocks were originally collected by former NASA astronaut Neil Armstrong from the Sea of Tranquility on the lunar surface more than four decades ago.

After being presented with the moon and Earth rocks, Zamka expressed the significance of the event.

“These rocks have already done more than a human being can do in a lifetime,” Zamka said. “For 4 million years they were on the moon undisturbed. They got on a spaceship, traveled to Earth, went up to Mt. Everest. So in a way they have tremendous history, and now they’re going to travel 17,500 mph back to space, where they will reside in the cupola of the Tranquility node.”

Upon reaching the summit of Mt. Everest, former NASA astronaut Scott Parazynski stops for a photo with the Apollo 11 moon rocks he carried along for the trekZamka said the rocks will be a reminder to the astronauts on the space station about “what human beings can do and what our challenges are. So this is a tremendous opportunity.”

During the presentation, Parazynski gave a narration of his journey to the top of Mt. Everest. He explained that a part of his motivation to carry along the lunar samples was pride to have been “born in this great country of ours and growing up in the shadows of many heroes, such as John Glenn, Jacques Cousteau, Neil Armstrong and Buzz Aldrin,” among others.

“These are the folks who I really looked up to as a kid,” Parazynski said. “It’s great to grow up in a country where you can walk in the paths of these types of people. One of the things I like to do is to honor them and pay tribute to them, and that is why I took a sample of the moon with me to Mt. Everest.”

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NASA’s Fermi Closes on Source of Cosmic Rays

Fermi's Large Area Telescope resolved GeV gamma rays from supernova remnants of different ages and in different environments. W51C, W44 and IC 443 are middle-aged remnants between 4,000 and 30,000 years oldNew images from NASA's Fermi Gamma-ray Space Telescope show where supernova remnants emit radiation a billion times more energetic than visible light. The images bring astronomers a step closer to understanding the source of some of the universe's most energetic particles -- cosmic rays.

Cosmic rays consist mainly of protons that move through space at nearly the speed of light. In their journey across the galaxy, the particles are deflected by magnetic fields. This scrambles their paths and masks their origins.

"Understanding the sources of cosmic rays is one of Fermi's key goals," said Stefan Funk, an astrophysicist at the Kavli Institute for Particle Astrophysics and Cosmology (KIPAC), jointly located at SLAC National Accelerator Laboratory and Stanford University, Calif.

Cassiopeia A supernova remnant across the spectrumWhen cosmic rays collide with interstellar gas, they produce gamma rays.

"Fermi now allows us to compare emission from remnants of different ages and in different environments," Funk added. He presented the findings Monday at the American Physical Society meeting in Washington, D.C.

Fermi's Large Area Telescope (LAT) mapped billion-electron-volt (GeV) gamma-rays from three middle-aged supernova remnants -- known as W51C, W44 and IC 443 -- that were never before resolved at these energies. (The energy of visible light is between 2 and 3 electron volts.) Each remnant is the expanding debris of a massive star that blew up between 4,000 and 30,000 years ago.

In addition, Fermi's LAT also spied GeV gamma rays from Cassiopeia A (Cas A), a supernova remnant only 330 years old. Ground-based observatories, which detect gamma rays thousands of times more energetic than the LAT was designed to see, have previously detected Cas A.

Fermi mapped GeV-gamma-ray emission regions (magenta) in the W44 supernova remnant"Older remnants are extremely bright in GeV gamma rays, but relatively faint at higher energies. Younger remnants show a different behavior," explained Yasunobu Uchiyama, a Panofsky Fellow at SLAC. "Perhaps the highest-energy cosmic rays have left older remnants, and Fermi sees emission from trapped particles at lower energies."

In 1949, the Fermi telescope's namesake, physicist Enrico Fermi, suggested that the highest-energy cosmic rays were accelerated in the magnetic fields of gas clouds. In the decades that followed, astronomers showed that supernova remnants are the galaxy's best candidate sites for this process.

Young supernova remnants seem to possess both stronger magnetic fields and the highest-energy cosmic rays. Stronger fields can keep the highest-energy particles in the remnant's shock wave long enough to speed them to the energies observed.

The Fermi observations show GeV gamma rays coming from places where the remnants are known to be interacting with cold, dense gas clouds.

"We think that protons accelerated in the remnant are colliding with gas atoms, This animation shows the creation of a pion via the collision of a proton and a cosmic ray protoncausing the gamma-ray emission," Funk said. An alternative explanation is that fast-moving electrons emit gamma rays as they fly past the nuclei of gas atoms. "For now, we can't distinguish between these possibilities, but we expect that further observations with Fermi will help us to do so," he added.

Either way, these observations validate the notion that supernova remnants act as enormous accelerators for cosmic particles.

"How fitting it is that Fermi seems to be confirming the bold idea advanced over 60 years ago by the scientist after whom it was named," noted Roger Blandford, director of KIPAC.

Related Links:

› Additional information and resolutions of supernova remnant media
› Additional information and resolutions of pion creation media

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Installing a Room With a View

In the grasp of the Canadarm2, the cupola was relocated from the forward port to the Earth-facing port of the International Space Station's newly installed Tranquility node. The cupola is a robotic control station with six windows around its sides and another in the center that will provide a panoramic view of Earth, celestial objects and visiting spacecrafts. With the installation of Tranquility and cupola, the space station is about 90 percent complete.

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Installing Tranquility

NASA astronauts Robert Behnken and Nicholas Patrick conducted the STS-130 mission's first spacewalk on Thursday, Feb. 11, 2010. The spacewalking pair finished all their assigned work and some get-ahead tasks. The Tranquility node and cupola were robotically maneuvered from Endeavour's payload bay, and then installed onto the port side of the Unity node. This was the first of three planned spacewalks for the STS-130 mission.

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NASA Extends Johnson Aircraft Maintenance Contract

NASA will exercise a one-year extension option for a contract with Computer Science Corporation of Fort Worth, Texas, to provide aircraft maintenance and modification support. The extension is valued at $58 million.

The Aircraft Maintenance and Modification Program contract provides for the continuity of services for flight line; intermediate and depot level maintenance; repairs; and modifications and engineering support on aircraft.

The aircraft supported are operated at NASA's Johnson Space Center in Houston; NASA's Dryden Flight Research Center in Edwards, Calif.; and NASA's Langley Research Center in Hampton, Va. The aircraft are used for astronaut crew training and NASA flight research. Work under the contract is performed at Johnson, Dryden and Langley, as well as NASA facilities in El Paso, Texas.

The option exercised on the cost-plus-award-fee contract begins March 1, 2010, and will continue to Feb. 28, 2011. Qualified Technical Services, Inc. of Houston is a significant subcontractor for the work.

For information about NASA and other agency programs, visit:

http://www.nasa.gov

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NASA Sets Out of this World News Conference with Shuttle Endeavour and Space Station Crews

The 11 crew members aboard space shuttle Endeavour and the International Space Station will hold a news conference at 8:39 p.m. CST on Thursday, Feb. 18.

U.S. reporters may ask questions in person from NASA's Johnson Space Center in Houston, NASA's Kennedy Space Center in Florida and NASA Headquarters in Washington. A portion of the news conference will be set aside for Japanese reporters.

To participate in the news conference, U.S. journalists must call the public affairs office at their preferred NASA center by 5 p.m. Wednesday. Media must be in place at participating locations at least 20 minutes prior to the start of the news conference.

NASA Television will provide live coverage of the 40-minute news conference. For NASA TV downlink, schedule and streaming video information, visit:

http://www.nasa.gov/ntv

During Endeavour's STS-130 mission, astronauts installed the Tranquility node, a module that provides additional room for crew members and many of the space station's life support and environmental control systems. Attached to Tranquility is a cupola with seven windows that provide a panoramic view of Earth, celestial objects and visiting spacecraft. Tranquility and its cupola are the final major U.S. portions of the station. The orbiting laboratory now is approximately 90 percent complete in terms of mass.

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

http://www.nasa.gov/shuttle

For more information about the space station and its crew, visit:

http://www.nasa.gov/station

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NASA’s Next Shuttle Launch Now Targeted for April 5; Media Credentials Deadlines Updated

NASA is targeting Monday, April 5, for the launch of the next space shuttle from the agency's Kennedy Space Center in Florida. Shuttle Discovery's seven crew members had planned to lift off on March 18 to begin the STS-131 mission to the International Space Station. However, cold weather in Florida has delayed Discovery's move to the Vehicle Assembly Building to complete the shuttle's processing, which has delayed the rollout to the launch pad.

The Space Shuttle Program has specific rules against transporting the shuttle when temperatures are below a certain level for extended periods. The vehicle has thrusters with seals that could leak under cold temperatures. As a result of the new STS-131 target launch date, NASA has extended the media accreditation deadlines. Deadlines for journalists to apply for the shuttle rollout and Terminal Countdown Demonstration Test are as early as Feb. 23. To be accredited, reporters must work for verifiable news-gathering organizations. No substitutions of credentials are allowed at any NASA facility.

Additional time may be required to process accreditation requests by journalists from certain designated countries. Designated countries include those with which the United States has no diplomatic relations, countries on the State Department's list of state sponsors of terrorism, those under U.S. sanction or embargo, and countries associated with proliferation concerns. Please contact the accrediting NASA center for details. Journalists should confirm they have been accredited before they travel.

KENNEDY SPACE CENTER

Reporters applying for credentials at Kennedy should submit requests via the Web at:

https://media.ksc.nasa.gov

Reporters must use work e-mail addresses, not personal accounts, when applying. After accreditation is approved, applicants will receive confirmation via e-mail.

Accredited media representatives with mission badges will have access to Kennedy from launch through the end of the mission. The application deadline for mission badges is March 24 for all reporters requesting credentials.

Discovery's rollout from the Vehicle Assembly Building, or VAB, to Launch Pad 39A, planned for March 2, follows its rollover from Orbiter Processing Facility-3 to the VAB, which is targeted for Feb. 22. The launch countdown dress rehearsal, known as the Terminal Countdown Demonstration Test, is targeted for March 5. Media must apply by 5 p.m. EST, Tuesday, Feb. 23 to cover rollout and the Terminal Countdown Demonstration Test.

Reporters with special logistic requests for Kennedy, such as space for satellite trucks, trailers, electrical connections or work space, must contact Laurel Lichtenberger by March 11 at:

laurel.a.lichtenberger@nasa.gov

There is no longer free wireless Internet access provided at Kennedy's news center. Work space in the news center and the news center annex is provided on a first-come basis, limited to one space per organization. To set up temporary telephone, fax, ISDN or network lines, media representatives must make arrangements with BellSouth at 800-213-4988. Reporters must have an assigned seat in the Kennedy newsroom prior to setting up lines. To obtain an assigned seat, contact Patricia Christian at:

patricia.christian-1@nasa.gov

Journalists must have a public affairs escort to all other areas of Kennedy except the Launch Complex 39 cafeteria.

JOHNSON SPACE CENTER

Reporters may obtain credentials for NASA's Johnson Space Center in Houston by calling the Johnson newsroom at 281-483-5111 or by presenting STS-131 mission credentials from Kennedy. Media representatives planning to cover the mission only from Johnson need to apply for credentials only at Johnson. The application deadline for mission badges is March 19 for all reporters requesting credentials.

Journalists covering the mission from Johnson using Kennedy credentials must contact the Johnson newsroom by March 19 to arrange workspace, phone lines and other logistics. Johnson is responsible for credentialing media if the shuttle lands at NASA's White Sands Space Harbor, N.M. If a landing is imminent at White Sands, Johnson will arrange credentials.

DRYDEN FLIGHT RESEARCH CENTER

Notice for a space shuttle landing at NASA's Dryden Flight Research Center on Edwards Air Force Base in California could be short. Domestic media outlets should consider accrediting Los Angeles-based personnel who could travel quickly to Dryden. Deadlines for submitting Dryden accreditation requests are March 9 for non-U.S. media, regardless of citizenship, and April 12 for U.S. media who are U.S. citizens or who have permanent residency status.

For Dryden media credentials, U.S. citizens representing domestic media outlets must provide their full name, date of birth, place of birth, media organization, driver's license number with the name of the issuing state, and the last six digits of their social security number.

In addition to the above requirements, foreign media representatives, regardless of citizenship, must provide data including their citizenship, visa or passport number and its expiration date. Foreign nationals representing either domestic or foreign media who have permanent residency status must provide their alien registration number and expiration date.

Journalists should fax requests for credentials on company letterhead to 661-276-3566 or e-mail requests to:

DrydenPAO@nasa.gov

Requests must include a phone number and business e-mail address for follow-up contact. Journalists who previously requested credentials will not need to do so again.

NASA PUBLIC AFFAIRS CONTACTS:

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

Johnson Space Center: James Hartsfield, 281-483-5111, james.a.hartsfield@nasa.gov

Dryden Flight Research Center: Leslie Williams, 661-276-3893, leslie.a.williams@nasa.gov

For information about the STS-131 mission, visit:

http://www.nasa.gov/shuttle

Two STS-131 crew members, NASA astronaut Clay Anderson and Naoko Yamazaki of the Japan Aerospace Exploration Agency, are tweeting about preparing for their mission. They can be followed at:

http://www.twitter.com/Astro_Clay

and

http://www.twitter.com/Astro_Naoko

For information about the International Space Station, visit:

http://www.nasa.gov/station

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Firefly Mission to Study Terrestrial Gamma-ray Flashes

High-energy bursts of gamma rays typically occur far out in space, perhaps near black holes or other high-energy cosmic phenomena. So imagine scientists' surprise in the mid-1990s when they found these powerful gamma ray flashes happening right here on Earth, in the skies overhead.

They're called Terrestrial Gamma-ray Flashes, or TGFs, and very little is known about them. They seem to have a connection with lightning, but TGFs themselves are something entirely different.

Right: An artist's concept of TGFs. Credit: NASA/Robert Kilgore [more]

"In fact," says Doug Rowland of NASA's Goddard Space Flight Center, "before the 1990s nobody knew they even existed. And yet they're the most potent natural particle accelerators on Earth."

Individual particles in a TGF acquire a huge amount of energy, sometimes in excess of 20 mega-electron volts (MeV). In contrast, the colorful auroras that light up the skies at high latitudes are powered by particles with less than one thousandth as much energy.

At this stage, there are more questions about TGFs than answers. What causes these high-energy flashes? Do they help trigger lightning--or does lightning trigger them? Could they be responsible for some of the high-energy particles in the Van Allen radiation belts, which can damage satellites?

To investigate, Rowland and his colleagues at GSFC, Siena College, Universities Space Research Association, and the Hawk Institute for Space Sciences are planning to launch an NSF-funded* satellite called Firefly in 2010 or 2011. Because of its small size, similar to a football, Firefly will cost less than $1 million — about 100 times cheaper than what full-sized satellite missions normally cost. Part of the cost savings comes from launching Firefly under the National Science Foundation's CubeSat program, which launches small satellites as "stowaways" aboard rockets carrying larger satellites into space, rather than requiring dedicated rocket launches.

Below: An artist's concept of Firefly on the lookout for TGFs above a thunderstorm. Firefly will make simultaneous measurements of energetic electrons, gamma rays, and the radio and optical signatures of the lightning discharge. [more]

see caption

If successful, Firefly will return the first simultaneous measurements of TGFs and lightning. Most of what's known about TGFs to date has been learned from missions meant to observe gamma rays coming from deep space, such as NASA's Compton Gamma Ray Observatory, which discovered TGFs in 1994. As it stared out into space, Compton caught fleeting glimpses of gamma rays out of the corner of its eye, so to speak. The powerful flashes were coming--surprise!--from Earth's atmosphere.

Subsequent data from Compton and other space telescopes have provided a tantalizingly incomplete picture of how TGFs occur:

In the skies above a thunderstorm, powerful electric fields generated by the storm stretch upward for many miles into the upper atmosphere. These electric fields accelerate free electrons, whisking them to speeds approaching the speed of light. When these ultra-high speed electrons collide with molecules in the air, the collisions release high-energy gamma rays as well as more electrons, setting up a cascade of collisions and perhaps more TGFs.

Right: Doug Rowland, principal investigator for Firefly stands next to the a life-sized model of the tiny satellite. Credit: NASA/Pat Izzo

To the eye, a TGF probably wouldn't look like much. Unlike lightning, most of a TGF's energy is released as invisible gamma rays, not visible light. They don't produce colorful bursts of light like sprites and other lightning-related phenomena. Nevertheless, these unseen eruptions could help explain why brilliant lightning strikes occur.

A longstanding mystery about lightning is how a strike gets started. Scientists know that the turbulence inside a thundercloud separates electric charge, building up enormous voltages. But the voltage needed to ionize air and generate a spark is about 10 times greater than the voltage typically found inside storm clouds.

"We know how the clouds charge up," Rowland says, "we just don't know how they discharge. That is the mystery."

TGFs could provide that spark. By generating a quick burst of electron flow, TGFs might help lightning strikes get started, Rowland suggests. "Perhaps this phenomenon is why we have lightning," he says.

If so, there ought to be many more TGFs each day than currently known. Observations by Compton and other space telescopes indicate that there may be fewer than 100 TGFs worldwide each day. Lightning strikes millions of times per day worldwide. That's quite a gap.

Then again, Compton and other space telescopes before Firefly weren't actually looking for TGFs. So perhaps it's not surprising that they didn't find many. Firefly will specifically look for gamma ray flashes coming from the atmosphere, not space, conducting the first focused survey of TGF activity. Firefly's sensors will even be able to detect flashes that are mostly obscured by the intervening air, which is a strong absorber of gamma rays (a fact that protects people on the ground from the energy in these flashes). Firefly's survey will give scientists much better estimates of the number of TGFs worldwide and help determine if the link to lightning is real.

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UK plan to create £40bn space industry and 100,000 new jobs

Space Innovation and Growth Strategy launched

In July 2009, Minister for Science Lord Drayson tasked Government, industry and academia to develop a 20-year vision to grow the UK’s share of the global space market.

The Space Innovation and Growth Team’s (Space IGT) findings were announced at an event at the QEII centre entitled “The Space Innovation and Growth Strategy: A 20 year vision for the UK Space Sector

The event took place between 10:00 and 14:00 on 10th February 2010 and 250 delegates from industry, academia, government and press attended.

Speakers:

  • Ian Pearson, Economic Secretary of State to the Treasury
  • Lord Drayson, Minister for Science, Department of Innovation Business and Skills
  • Andy Green, CEO Logica and Chairman of the Space Innovation and Growth Team
For more information please visit the IGS website

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Shuttle blasts off to deliver 360º observation deck to the ISS

British born astronaut Dr Nicholas Patrick – a Cambridge graduate originally from Saltburn-by-sea, North Yorkshire - is part of a team that embarked on a 13-day mission to the International Space Station (ISS) on Monday 8 February 2010.

Dr Patrick, 45, will attach two new segments – each weighing around 15 tonnes – to the ISS with fellow spacewalker Robert Behnken as they circle the earth at 17,500 mph.

Space Shuttle Endeavour launched from the Kennedy Space Centre at 09:14 GMT on Monday 8th February, to deliver two new modules to the International Space Station but was delayed when cloud cover made the team miss their 10 minute launch window.

Cupola is an observation module featuring the largest and most complex window assembly ever launched into space. The dome-shaped module will provide a 360º view from a panoramic control tower - to enable astronauts to observe external operations such as spacewalks, robotics or visiting spacecraft and guide activity as providing psychological benefits for the crew.

Nodes are connecting elements between the various pressurised modules on the ISS. Node-3 will provide more space for equipment and the astronauts.

Learn more about the Node-3, Cupola and STS-130, with press releases, and mission information on the ESA (link opens in a new window) and NASA (link opens in a new window) Website.

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UK scientists find more evidence for water on moon of Saturn

UK scientists working on the Cassini mission to Saturn have found evidence of liquid water on the planet’s icy moon Enceladus, suggesting the possibility of life below its surface.

The findings come from the work of space scientists at Imperial College London, UCL, Open University, University of Oxford and Queen Mary’s University of London.

“While it’s no surprise that there is water there, these short-lived ions are extra evidence for sub-surface water and where there’s water, carbon and energy, some of the major ingredients for life are present,” said lead author Andrew Coates from University College London’s Mullard Space Science Laboratory.

These revelations add to our growing knowledge about the detailed chemistry of the atmospheres on Saturn’s moons Titan and Enceladus: giving new understanding of environments beyond Earth where life-sustaining environments might exist.

Early in its mission, Cassini discovered the plume of water, which jets water vapour and ice particles above Enceladus. Since then, scientists have found that these water products dominate Saturn’s magnetic environment and create Saturn’s huge E-ring.

The Cassini plasma spectrometer is operated by UK teams who gather and interpret surface data such as the density, flow velocity and temperature of ions and electrons that enter the instrument.

Cassini was launched in 1997 and reached Saturn in 2004. The study’s findings are based on analysis from data taken in fly-throughs in 2008.

The Cassini-Huygens mission is a joint project between NASA, the European Space Agency and the Italian Space Agency.

For more information on the Cassini Mission, please visit the Cassini mission page and NASA website (link opens in a new window).

For the full press release, please visit the STFC website

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NASA’s Solar Dynamics Observatory launches successfully

Scientists are celebrating as NASA successfully launched its high resolution Sun probe into space today, Thursday 11 February.

The Solar Dynamics Observatory will give space scientists the most detailed views ever of the Sun to help improve their understanding of the Sun’s disruptive influence on space weather and services such as telecommunications on Earth. The UK, including scientists and engineers from the Science and Technology Facility Council’s (STFC’s) Rutherford Appleton Laboratory (RAL), has provided essential expertise and technology to the mission.

RAL Scientists involved in the five year mission watched as SDO was launched from Florida's Cape Canaveral base at 15.23 (GMT).

For the full story, please visit the STFC website

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Shuttle Silhouette

Shuttle Silhouette
In a very unique setting over Earth's colorful horizon, the silhouette of the space shuttle Endeavour is featured in this photo by an Expedition 22 crew member on board the International Space Station, as the shuttle approached for its docking on Feb. 9 during the STS-130 mission.

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Voyager Celebrates 20-Year-Old Valentine to Solar System

six narrow-angle color images taken from Voyager 1
These six narrow-angle color images were made from the first ever 'portrait' of the solar system taken by Voyager 1, which was more than 4 billion miles from Earth and about 32 degrees above the ecliptic. › Full image and caption
Twenty years ago on February 14, NASA's Voyager 1 spacecraft had sailed beyond the outermost planet in our solar system and turned its camera inward to snap a series of final images that would be its parting valentine to the string of planets it called home.

Mercury was too close to the sun to see, Mars showed only a thin crescent of sunlight, and Pluto was too dim, but Voyager was able to capture cameos of Neptune, Uranus, Saturn, Jupiter, Earth and Venus from its unique vantage point. These images, later arranged in a large-scale mosaic, make up the only family portrait of our planets arrayed about the sun.

The Apollo missions in the 1960s and 70s had already altered our perspective of Earth by returning images of our home planet from the moon, but Voyager was providing a completely new perspective, said Ed Stone, Voyager project scientist at the California Institute of Technology in Pasadena.

"It captured the Earth as a speck of light in the vastness of the solar system, which is our local neighborhood in the Milky Way galaxy, in a universe replete with galaxies," Stone said.

In the years since the twin Voyager spacecraft were launched in 1977, they had already sent back breathtaking, groundbreaking pictures of the gas giants Jupiter, Saturn, Uranus and Neptune. It took Voyager 1 more than 12 years to reach the place where it took the group portrait, 6 billion kilometers (almost 4 billion miles) away from the sun. The imaging team started snapping images of the outer planets first because they were worried that pointing the camera near the sun would blind it and prevent more picture-taking.

Candy Hansen, a planetary scientist based at NASA's Jet Propulsion Laboratory in Pasadena, Calif., who worked with the Voyager imaging team at the time, remembers combing through the images and finally finding the image of Earth. She had seen so many pictures over the years that she could distinguish dust on the lens from the black dots imprinted on the lens for geometric correction.

There was our planet, a bright speck sitting in a kind of spotlight of sunlight scattered by the camera. Hansen still gets chills thinking about it.

"I was struck by how special Earth was, as I saw it shining in a ray of sunlight," she said. "It also made me think about how vulnerable our tiny planet is."

This was the image that inspired Carl Sagan, the the Voyager imaging team member who had suggested taking this portrait, to call our home planet "a pale blue dot."

As he wrote in a book by that name, "That's here. That's home. That's us. On it everyone you love, everyone you know, everyone you ever heard of, every human being who ever was, lived out their lives. … There is perhaps no better demonstration of the folly of human conceits than this distant image of our tiny world."

After these images were taken, mission managers started powering down the cameras. The spacecraft weren't going to fly near anything else, and other instruments that were still collecting data needed power for the long journey to interstellar space that was ahead.

The Voyagers are still transmitting data daily back to Earth. Voyager 1 is now nearly 17 billion kilometers (more than 10 billion miles) away from the sun. The spacecraft have continued on to the next leg of their interstellar mission, closing in on the boundary of the bubble created by the sun that envelops all the planets. Scientists eagerly await the time when the Voyagers will leave that bubble and enter interstellar space.

"We were marveling at the vastness of space when this portrait was taken, but 20 years later, we're still inside the bubble," Stone said. "Voyager 1 may leave the solar bubble in five more years, but the family portrait gives you a sense of the scale of our neighborhood and that there is a great deal beyond it yet to be discovered."

The Voyagers were built by JPL, which continues to operate both spacecraft. Caltech manages JPL for NASA.

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Cassini Set to Do Retinal Scan of Saturnian Eyeball

Saturn's moon Mimas
During its approach to Mimas on Aug. 2, 2005, the Cassini spacecraft narrow-angle camera obtained multi-spectral views of the moon from a range of 228,000 kilometers (142,500 miles).
On Feb. 13, 2010, NASA's Cassini spacecraft will make its closest examination yet of Mimas, an eyeball-shaped moon of Saturn that has also been likened to the Death Star of "Star Wars." The spacecraft will be returning the highest-resolution images yet of this battered satellite.

Mimas bears the mark of a violent, giant impact from the past - the 140-kilometer-wide (88-mile-wide) Herschel Crater - and scientists hope the encounter will help them explain why the moon was not blown to smithereens when the impact happened. They will also be trying to count smaller dings inside the basin of Herschel Crater so they can better estimate its age.

In addition, Cassini's composite infrared spectrometer will be working to determine the thermal signature of the moon, and other instruments will be making measurements to learn more about the surface composition.

The Mimas flyby involves a significant amount of skill because the spacecraft will be passing through a dusty region to get there. Mission managers have planned for the Cassini spacecraft to lead with its high-gain antenna to provide a barrier of protection. At closest approach, the spacecraft will be flying about 9,500 kilometers (5,900 miles) above the moon. Cassini will start taking images and measurements shortly after closest approach.

Mimas is an inner moon of Saturn that averages 396 kilometers (246 miles) in diameter. The diameter of Herschel Crater is about one-third that of the entire moon. The walls of the crater are about 5 kilometers (3 miles) high, and parts of the floor are approximately 10 kilometers (6 miles) deep.

More information is available at http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov.

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Endeavour Brings Tranquility

Backdropped by the blackness of space, space shuttle Endeavour was photographed by the Expedition 22 crew as the shuttle approached the International Space Station during STS-130 rendezvous and docking operations on Feb. 9, 2010. The Tranquility node can be seen in the shuttle's payload bay.

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