Eclipses Yield First Images of Elusive Iron Line in Solar Corona

Solar physicists attempting to unlock the mysteries of the solar corona have found another piece of the puzzle by observing the sun’s outer atmosphere during eclipses.

Ground-based observations reveal the first images of the solar corona in the near-infrared emission line of highly ionized iron, or Fe XI 789.2 nm. The observations were taken during total solar eclipses in 2006, 2008, and 2009 by astrophysicist Adrian Daw of NASA’s Goddard Space Flight Center in Greenbelt, Md., with an international team of scientists led by Shadia Habbal from the University of Hawaii’s Institute for Astronomy (IfA).
"The first image of the corona in Fe XI 789.2 nm was taken during the total solar eclipse of March 29, 2006," said Daw.

The images revealed some surprises. Most notably, that the emission extends out at least three solar radii -- that’s one-and-a-half times the sun’s width at its equator, or middle -- above the surface of the sun, and that there are localized regions of enhanced density for these iron ions.

Combined with observations of other iron charge states, the observations yield the two-dimensional distribution of electron temperature and charge-state measurements for the first time, and establish the first direct link between the distribution of charge states in the corona and in interplanetary space.

"These are the first such maps of the 2-D distribution of coronal electron temperature and ion charge state," said Daw.

Mapping the distribution of electron temperature and iron charge states in the corona with total solar eclipse observations represents an important step in understanding the solar corona and how space weather impacts Earth.

The scientists’ results will be presented at the American Astronomical Society meeting on January 4 in Washington and published in the January issue of the Astrophysical Journal.

Massive Black Hole Implicated in Stellar Destruction

New results from NASA's Chandra X-ray Observatory and the Magellan telescopes suggest that a dense stellar remnant has been ripped apart by a black hole a thousand times as massive as the Sun. If confirmed, this discovery would be a cosmic double play: it would be strong evidence for an intermediate mass black hole, which has been a hotly debated topic, and would mark the first time such a black hole has been caught tearing a star apart.

This scenario is based on Chandra observations, which revealed an unusually luminous source of X-rays in a dense cluster of old stars, and optical observations that showed a peculiar mix of elements associated with the X-ray emission. Taken together, a case can be made that the X-ray emission is produced by debris from a disrupted white dwarf star that is heated as it falls towards a massive black hole. The optical emission comes from debris further out that is illuminated by these X-rays.

The intensity of the X-ray emission places the source in the "ultraluminous X-ray source" or ULX category, meaning that it is more luminous than any known stellar X-ray source, but less luminous than the bright X-ray sources (active galactic nuclei) associated with supermassive black holes in the nuclei of galaxies. The nature of ULXs is a mystery, but one suggestion is that some ULXs are black holes with masses between about a hundred and several thousand times that of the Sun, a range intermediate between stellar-mass black holes and supermassive black holes located in the nuclei of galaxies.

This ULX is in a globular cluster, a very old and crowded conglomeration of stars. Astronomers have suspected that globular clusters could contain intermediate-mass black holes, but conclusive evidence for this has been elusive.

"Astronomers have made cases for stars being torn apart by supermassive black holes in the centers of galaxies before, but this is the first good evidence for such an event in a globular cluster," said Jimmy Irwin of the University of Alabama who led the study.

Irwin and his colleagues obtained optical spectra of the object using the Magellan I and II telescopes in Las Campanas, Chile. These data reveal emission from gas rich in oxygen and nitrogen but no hydrogen, a rare set of signals from globular clusters. The physical conditions deduced from the spectra suggest that the gas is orbiting a black hole of at least 1,000 solar masses. The abundant amount of oxygen and absence of hydrogen indicate that the destroyed star was a white dwarf, the end phase of a solar-type star that has burned its hydrogen leaving a high concentration of oxygen. The nitrogen seen in the optical spectrum remains an enigma.

"We think these unusual signatures can be explained by a white dwarf that strayed too close to a black hole and was torn apart by the extreme tidal forces," said coauthor Joel Bregman of the University of Michigan.

Theoretical work suggests that the tidal disruption-induced X-ray emission could stay bright for more than a century, but it should fade with time. So far, the team has observed there has been a 35 percent in X-ray emission from 2000 to 2008.

The ULX in this study is located in NGC 1399, an elliptical galaxy about 65 million light years from Earth.

Irwin presented these results at the 215th meeting of the American Astronomical Society in Washington, DC. NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory controls Chandra's science and flight operations from Cambridge, Mass.

More information, including images and other multimedia, can be found at:

http://chandra.harvard.edu

NASA Astronaut John Grunsfeld, Instrumental to Hubble Telescope Repair, Will Help Oversee its Science Operations

NASA astronaut John Grunsfeld, who participated in three spaceflights to service the Hubble Space Telescope, is leaving the agency to become the deputy director of the Space Telescope Science Institute in Baltimore. The institute is the science operations center for Hubble and the James Webb Space Telescope, which is planned for launch in 2014.

"During the past 18 years, John has been a true asset to the agency," said NASA Administrator Charles Bolden, a former astronaut who few on the STS-31 mission that deployed the Hubble. "Some have called him the chief Hubble repairman, but I call him a friend and wish him the best in his new endeavor."

In addition to Grunsfeld's flights to Hubble (STS-103 in Dec. 1999, STS-109 in March 2002, and STS-125 in May 2009), he also served on two other shuttle missions. He performed eight critical spacewalks and logged more than 835 hours in space.

During 2003 and 2004, he was NASA's Chief Scientist at the agency's headquarters in Washington. He helped develop the Vision for Space Exploration, which set NASA on the path for future exploration endeavors.

In accepting the institute position, Grunsfeld said, "This is an incredibly exciting opportunity for me to work at a focal point of top astronomers at the leading edge of scientific inquiry. The team at the Space Telescope Science Institute has a demonstrated record of meeting the high performance challenges of operating the Hubble Space Telescope and preparing for the James Webb Space Telescope. I look forward to working with this excellent team as we continue to explore the mysteries of the universe."

Related Site:

› John Grunsfeld's Official Biography
› Hubble Space Telescope Mission Section

NASA's Mars Rover has Uncertain Future as Sixth Anniversary Nears

NASA's Mars rover Spirit will mark six years of unprecedented science exploration and inspiration for the American public on Sunday. However, the upcoming Martian winter could end the roving career of the beloved, scrappy robot.

Spirit successfully landed on the Red Planet at 8:35 p.m. PST on Jan. 3, 2004, and its twin Opportunity arrived at 9:05 p.m. Jan. 24, 2004. The rovers began missions intended to last for three months but which have lasted six Earth years, or 3.2 Mars years. During this time, Spirit has found evidence of a steamy and violent environment on ancient Mars that was quite different from the wet and acidic past documented by Opportunity, which has been operating successfully as it explores halfway around the planet.

A sand trap and balky wheels are challenges to Spirit's mobility that could prevent NASA's rover team from using a key survival strategy for the rover. The team may not be able to position the robot's solar panels to tilt toward the sun to collect power for heat to survive the severe Martian winter.

Nine months ago, Spirit's wheels broke through a crusty surface layer into loose sand hidden underneath. Efforts to escape this sand trap barely have budged the rover. The rover's inability to use all six wheels for driving has worsened the predicament. Spirit's right-front wheel quit working in 2006, and its right-rear wheel stalled a month ago. Surprisingly, the right-front wheel resumed working, though intermittently. Drives with four or five operating wheels have produced little progress toward escaping the sand trap. The latest attempts resulted in the rover sinking deeper in the soil.

"The highest priority for this mission right now is to stay mobile, if that's possible," said Steve Squyres of Cornell University in Ithaca, N.Y. He is principal investigator for the rovers.

If mobility is not possible, the next priority is to improve the rover's tilt, while Spirit is able to generate enough electricity to turn its wheels. Spirit is in the southern hemisphere of Mars, where it is autumn, and the amount of daily sunshine available for the solar-powered rover is declining. This could result in ceasing extraction activities as early as January, depending on the amount of remaining power. Spirit's tilt, nearly five degrees toward the south, is unfavorable because the winter sun crosses low in the northern sky.

Unless the tilt can be improved or luck with winds affects the gradual buildup of dust on the solar panels, the amount of sunshine available will continue to decline until May 2010. During May, or perhaps earlier, Spirit may not have enough power to remain in operation.

"At the current rate of dust accumulation, solar arrays at zero tilt would provide barely enough energy to run the survival heaters through the Mars winter solstice," said Jennifer Herman, a rover power engineer at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

The team is evaluating strategies for improving the tilt even if Spirit cannot escape the sand trap, such as trying to dig in deeper with the wheels on the north side. In February, NASA will assess Mars missions, including Spirit, for their potential science versus costs to determine how to distribute limited resources. Meanwhile, the team is planning additional research about what a stationary Spirit could accomplish as power wanes.

"Spirit could continue significant research right where it is," said Ray Arvidson of Washington University in St. Louis, deputy principal investigator for the rovers. "We can study the interior of Mars, monitor the weather and continue examining the interesting deposits uncovered by Spirit's wheels."

A study of the planet's interior would use radio transmissions to measure wobble of the planet's axis of rotation, which is not feasible with a mobile rover. That experiment and others might provide more and different findings from a mission that has already far exceeded expectations.

"Long-term change in the spin direction could tell us about the diameter and density of the planet's core," said William Folkner of JPL. He has been developing plans for conducting this experiment with a future, stationary Mars lander. "Short-period changes could tell us whether the core is liquid or solid," he said.

In 2004, Opportunity discovered the first mineralogical evidence that Mars had liquid water. The rover recently finished a two-year investigation of a half-mile wide crater called Victoria and now is headed toward Endeavor crater, which is approximately seven miles from Victoria and nearly 14 miles across. Since landing, Opportunity has driven more than 11 miles and returned more than 132,000 images.

For more information about the rovers, visit:
http://www.nasa.gov/rovers

Read more: Road Trip Memories of Mars.

NASA Awards Contract For Fabrication Services To Hampton, Va., Firm

NASA has selected Science and Technology Corp. of Hampton, Va., to provide fabrication support services to NASA's Langley Research Center in Hampton.

The value of the indefinite delivery indefinite quantity contract is not to exceed $35 million. The period of performance is five years from the effective date, including a one-month phase-in period.

Science and Technology Corp. will provide technical support to fabricate research-oriented electronics circuitry, including circuit assemblies for ground support equipment, aircraft, spaceflight, laboratory, science and research facility instrumentation. Special fabrication operations, procedures and techniques may be required. Services will be performed at Langley, the contractor facility and other sites.

For information about NASA's Langley Research Center, visit:

http://www.nasa.gov/langley

New Moon Marvels

The Cassini orbiter has been working overtime during the holidays to deliver a cartload of gifts from Saturn and its moons. Highlights include fresh views of frost-spewing Enceladus and yam-shaped Prometheus, plus a "Nutcracker"-style ballet of Saturnian satellites.

The excitement began last week with the animated images of moonsimage advisory, the folks who process Cassini's pictures compared the interplay to the dance of the Sugar Plum Fairy from Tchaikovsky's "Nutcracker" ballet. passing back and forth with the giant planet and its rings as a backdrop. In an

My favorite movie is "Moon Jumble," which has Rhea in the starring role, joined by its siblings Janus, Mimas and Pandora. (That's the real Pandora, not the fictional "Avatar" moon). Make sure you stretch your browser window wide enough to take in the whole picture.

"As yet another year in Saturn orbit draws to a close, these wondrous movies of an alien place clear across the solar system remind us how fortunate we are to be engaged in this magnificent exploratory expedition," imaging team leader Carolyn Porco said. "So, from all of us on the Cassini Imaging Team to all of you, Happy Holidays!"

That might fool you into thinking the Cassini team was taking the holidays off. There's no way that was going to happen. On Christmas and the day after, the orbiter snapped pictures as it flew past Enceladus and Prometheus. Over the weekend, Cassini zoomed within 600 miles (960 kilometers) of Titan's north pole.

A sampling of the raw imagery released on Sunday includes a striking full-disk view of Enceladus and its geysers of water ice, spewing out from southern fissures that have been nicknamed "tiger stripes." Such geysers hint at the existence of a subsurface ocean beneath Enceladus' icy surface - an ocean that just might harbor alien life.

The latest picture was taken from a distance of 383,000 miles (617,000 kilometers), and it might make you wonder why those geysers hadn't been spotted decades ago when the Voyager spacecraft flew past. In a posting to the imaging team's Web site, Porco says it wouldn't have been that easy for Voyager to spot the frosty spray.

"We never got a good look at the southern hemisphere with Voyager; we even missed the tiger stripes back then," she wrote. Porco also said "some of the jets - and maybe all of them - are 'intermittent' in the sense that we expect they could turn on and off on a daily timescale (where 'daily' here means 1.3 Earth days)."

Another raw image provides the best view yet of Prometheus, a "shepherding" moon that along with Pandora helps keep Saturn's F ring in line. This view was captured from a distance of 36,000 miles (59,000 kilometers). A farther-out image from Cassini, released five years ago, shows Prometheus at work.

The Planetary Society's Emily Lakdawalla put together the raw imagery to produce a natural-color composite photo of the moon, which measures 74 miles long and as little as 38 miles wide (119 by 87 by 61 kilometers).

"This is one of the more elongated moons to be seen in the solar system, almost exactly twice as long as it is wide," Lakdawalla observes. "The word 'potato' is commonly used to describe the shape of small bodies in the solar system, but I think that Prometheus, with its pointy ends, looks more like a related vegetable, a yam."

The fact that candied yams are a traditional holiday dish makes Prometheus even more palatable as a year-end picture - and whets the appetite for more from Cassini in the year to come.

Passing of Stan Lebar

Stan Lebar, who led the Westinghouse Electric Corporation team that developed the lunar camera that brought the televised news images of Neil Armstrong stepping onto the moon to more than 500 million people on earth, died on Tuesday, Dec. 22, 2009.

During his long and distinguished career, other camera programs he managed for NASA included the Apollo Color TV Cameras, the Skylab series of TV cameras, and the TV cameras for the Apollo-Soyuz Test Program (ASTP).

From 1943 until the end of World War II, Lebar served in the Pacific Theater of Operations as an Air Force B-24 Ball Turret Gunner. After the war, he attended the University of Missouri and received a BS in Electrical Engineering in 1950. He joined Westinghouse Electric Corporation in 1953, and worked in the Aerospace Division, Baltimore, Maryland, until his retirement in 1986.

Undergraduate Students Fly High for Weightless Science

NASA has selected 28 undergraduate student teams to test their science experiments in simulated weightlessness. The teams were selected to fly in the summer of 2010 with NASA's Reduced Gravity Student Flight Opportunities and Systems Engineering Educational Discovery (SEED) programs.

Selected teams will test and evaluate their experiments aboard an aircraft modified to simulate a reduced-gravity environment. The aircraft will fly approximately 30 roller-coaster-like climbs and dips during experiment flights to produce periods of weightlessness and hyper-gravity ranging from 0 g to 2 g.

"Today's students will be the ones going to the moon and beyond to live, explore and work," said Douglas Goforth, the Reduced Gravity Education Flight Program manager at NASA's Johnson Space Center in Houston."This project gives them a head start in preparing for those future ventures by allowing them to conduct hands-on research and engineering today in a unique reduced-gravity laboratory."

The Reduced Gravity Student Flight Opportunities Program provides a rare academic experience for undergraduate students to propose, design, fabricate, fly and evaluate a reduced-gravity experiment. The overall experience includes scientific research, hands-on experimental design, test operations and outreach activities.

Teams selected to participate in the Reduced Gravity Student Flight Opportunities Program are from Utah State University, San Jacinto College North, the College of New Jersey, State University of New York at Buffalo, West Virginia University, Purdue University, Yale University, Austin Community College, the University of Washington, the University of Wisconsin at Madison, two teams from Embry-Riddle Aeronautical University, and two teams from the University of Michigan. Teams also may invite a full-time, accredited journalist to fly with them and document the team's experiment and experiences.

Teams selected to participate in the SEED program will work with NASA scientists, engineers and researchers on systems engineering projects that use a reduced gravity environment to test spaceflight hardware, spacecraft components and spaceflight procedures. Each team is assigned a NASA principal investigator to help prepare their experiment for flight. The SEED teams also will participate in at least two videoconferences through NASA's Digital Learning Network to work with other engineering and agency organizations.

The SEED teams for 2010 are from Washington University, Massachusetts Institute of Technology, the University of Wisconsin, Auburn University, the Ohio State University, the University of Nebraska, the University of Toledo, Carthage College, Yale University, the University of Kentucky, the University of Colorado, and Boise State University, from which two teams were selected.

Under these programs, NASA continues its investment in the nation's education programs. It is directly tied the agency's education goal of strengthening NASA and the nation's future workforce. Through this and other college and university programs, NASA will identify and develop the critical skills and capabilities needed to carry out its space exploration mission.

The flights are provided in cooperation with the Reduced Gravity Office at NASA's Johnson Space Center. For more information about the Reduced Gravity Education Flight Program or to view abstracts of the selected team's experiments visit:

http://microgravityuniversity.jsc.nasa.gov

For more information about SEED, visit:

http://microgravityuniversity.jsc.nasa.gov/se

For more information about NASA's education programs, visit:

http://www.nasa.gov/education

NASA Announces Information Technology Contract Extension

NASA has extended the Unified NASA Information Technology Services, or UNITeS, contract with Science Applications International Corporation (SAIC) of San Diego. The action is intended to allow for the completion of recompetition activities for NASA's Information Technology Infrastructure Integration Program, which encompasses agency-wide management, integration and delivery of information technology infrastructure services.

The contract extension provides NASA with agency-wide information services and integration support for NASA's Integrated Enterprise Management Program, or IEPM, administered by NASA's Marshall Space Flight Center in Huntsville, Ala. The contract also provides additional information technology services for the Marshall Center until such time as follow-on contracts are awarded for these efforts.

The contract modification extends the period of performance by 14 months, including an eight-month base period, valued at approximately $120 million, followed by six one-month options. The extension began Dec. 1 and ends Jan. 31, 2011, if all options are exercised.

The UNITeS contract began Jan. 1, 2004. The total value of the UNITeS contract, including this extension, is approximately $1.31 billion.

Marshall's responsibilities for information technology include managing software applications, Web/computer server systems, audio-visual information, telecommunications, information technology security, information technology procurement, documentation storage and protection hardware maintenance. Support provided under the UNITeS contract includes NASA-wide information technology security, encryption security systems, computer networking and digital imaging.

For more information about NASA's Information Technology Infrastructure Integration Program, visit:

http://i3p-acq.ksc.nasa.gov/i3p/default.cfm

For more information about NASA and agency programs, visit:

http://www.nasa.gov

Space Shuttle Crew Returns Home after 11-Day Mission

Space shuttle Atlantis and its crew of seven astronauts ended an 11-day journey of nearly 4.5 million miles with a 9:44 a.m. EST landing Friday at NASA's Kennedy Space Center in Florida.

The mission, designated STS-129, included three spacewalks and the installation of two platforms to the International Space Station's truss, or backbone. The platforms hold large spare parts to sustain station operations after the shuttles are retired. The shuttle crew delivered about 30,000 pounds of replacement parts for systems that provide power to the station, keep it from overheating, and maintain a proper orientation in space.

STS-129 Commander Charlie Hobaugh was joined on Atlantis' STS-129 mission by Pilot Barry Wilmore and Mission Specialists Leland Melvin, Randy Bresnik, Mike Foreman and Bobby Satcher. Atlantis returned with station resident Nicole Stott, who spent 91 days in space. This marks the final time the shuttle is expected to rotate station crew members.

A welcome ceremony for the astronauts will be held Monday, Nov. 30, in Houston. The public is invited to attend the 4 p.m. CST event at Ellington Field's NASA Hangar 990. Highlights from the ceremony will be broadcast on NASA Television's Video File. For NASA TV downlink information, schedules and links to streaming video, visit:

http://www.nasa.gov/ntv

With Atlantis and its crew safely home, the stage is set for launch of shuttle Endeavour on its STS-130 mission, targeted to begin in February. Endeavour will deliver a pressurized module, known as Tranquility, which will provide room for many of the space station's life support systems. Attached to the node is a cupola, a robotic control station with six windows around its sides and another in the center that provides a 360-degree view around the station.

For more about the STS-129 mission and the upcoming STS-130 flight, visit:

http://www.nasa.gov/shuttle

STS-129 crew members Melvin, Satcher and Stott are providing mission updates on Twitter. For their Twitter feeds and other NASA social media Web sites, visit:

http://www.nasa.gov/connect

For information about NASA and agency programs, visit:

http://www.nasa.gov

NASA Space Shuttle Atlantis Crew Set to Land in Florida Friday

Space shuttle Atlantis and its seven-member crew are expected to return to Earth on Friday, Nov. 27, after an 11-day mission. The two landing opportunities at NASA's Kennedy Space Center in Florida are at 9:44 a.m. and 11:19 a.m. EST.

NASA will evaluate weather conditions at Kennedy before permitting Atlantis and its crew to land. If bad weather prevents a return to Florida on Friday or Saturday, both Kennedy and the backup landing site at Edwards Air Force Base in California will be activated for consideration on Sunday. For recorded updates about the shuttle landing, call 321-867-2525.

Approximately two hours after landing, NASA officials will hold a briefing to discuss the mission. The participants will be:

- Bill Gerstenmaier, NASA associate administrator for Space Operations
- Mike Moses, space shuttle launch integration manager
- Mike Leinbach, NASA shuttle launch director

After touchdown in Florida, the astronauts will undergo physical examinations and meet with their families. They are expected to make brief remarks at the runway and hold a news conference approximately six hours after landing. The news events will be broadcast live on NASA Television and the agency's Web site.

The Kennedy news center will open for landing activities at 5 a.m. Friday and close at 5 p.m., or one hour after the last media event.

The STS-129 media badges are in effect through landing. The media accreditation building on State Road 3 will be open Friday from 6 a.m. to 8:30 a.m. The last bus will depart from the news center for the Shuttle Landing Facility one hour before landing.

If the landing is diverted to Edwards, reporters should call NASA's Dryden Flight Research Center public affairs office at 661-276-3449. Dryden has limited facilities available for previously accredited journalists.

The NASA News Twitter feed is updated throughout the shuttle mission and landing. To access the feed, visit:

http://www.twitter.com/nasa

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

http://www.nasa.gov/ntv

For the latest information about the STS-129 mission and accomplishments, visit:

http://www.nasa.gov/shuttle

The Big Thaw? NASA Satellites Detect Unexpected Ice Loss in East Antarctica

Using gravity measurement data from the NASA/German Aerospace Center's Gravity Recovery and Climate Experiment (Grace) mission, a team of scientists from the University of Texas at Austin has found that the East Antarctic ice sheet-home to about 90 percent of Earth's solid fresh water and previously considered stable-may have begun to lose ice.

The team used Grace data to estimate Antarctica's ice mass between 2002 and 2009. Their results, published Nov. 22 in the journal Nature Geoscience, found that the East Antarctic ice sheet is losing mass, mostly in coastal regions, at an estimated rate of 57 gigatonnes a year. A gigatonne is one billion metric tons, or more than 2.2 trillion pounds. The ice loss there may have begun as early as 2006. The study also confirmed previous results showing that West Antarctica is losing about 132 gigatonnes of ice per year.

"While we are seeing a trend of accelerating ice loss in Antarctica, we had considered East Antarctica to be inviolate," said lead author and Senior Research Scientist Jianli Chen of the university's Center for Space Research. "But if it is losing mass, as our data indicate, it may be an indication the state of East Antarctica has changed. Since it's the biggest ice sheet on Earth, ice loss there can have a large impact on global sea level rise in the future."

NASA's Jet Propulsion Laboratory, Pasadena, Calif., developed the twin Grace satellites. The University of Texas Center for Space Research in Austin has overall Grace mission responsibility. Grace was launched in 2002.

More information on Grace is online at http://www.csr.utexas.edu/grace/ and http://grace.jpl.nasa.gov/.

› Read the UTCSR news release

NASA Pushes Social Media Experience to New Heights

NASA launched a social media experience at the Kennedy Space Center in Florida that quickly turned into an unprecedented world-wide event as more than 100 Twitter users got a unique look inside America's space program and front row seats to the Nov. 16 liftoff of the space shuttle Atlantis.

People from as far away as New Zealand participated in Kennedy's first Tweetup, an event where bloggers meet face-to-face and share their experiences in 140 character online bursts. During the two-day event Twitter users, or Tweeps, took behind-the-scenes tours of Kennedy, spoke at length with NASA astronauts, technicians, engineers and managers, and saw a launch from the vantage point usually reserved for more traditional media.

"We were very excited by the extraordinary number of people from all over the world who participated," said Lori Garver, NASA's deputy administrator. "NASA will continue to evolve with the social media environment and look for new ways to engage the public and spread the word about the tremendous things we do."

The Tweetup, identified by the search term #nasatweetup, was the third highest trending topic Nov. 15 on the social networking service. The micro-blogs, or tweets, are text-based Internet posts that are delivered to the author's subscribers. The more than 100 people in attendance had over 150,000 followers. As people share and forward the information, the potential online reach could be in the millions.

People from 21 states and the District of Columbia attended, as did guests who flew from Canada, England, Morocco and New Zealand. Participants ranged in age from 18 to more than 60, with most being under age 40. NASA Television also streamed video of Tweetup events online where more than 7,500 viewers watched the events prior to launch.

"The way people are communicating and receiving information is undergoing a global revolution," said Morrie Goodman, NASA's assistant administrator for Public Affairs. "NASA is a recognized leader in adopting social media and this is another exciting 'first' for the agency."

NASA's Jet Propulsion Laboratory held the first NASA Tweetup on Jan. 21. NASA Headquarters held its first Tweetup on July 21, followed by another from Headquarters Sept. 24 that featured the STS-127 space shuttle crew. On Oct. 21, NASA held a smaller Tweetup, allowing 35 Tweeps to talk with Nicole Stott and Jeff Williams aboard the International Space Station via a live downlink.

In April, Mike Massimino (@Astro_Mike) became NASA's first astronaut to tweet. Astro_Mike reached 1 million Twitter followers on Sept. 23. He sent his first tweet from space while flying on the STS-125 Hubble servicing mission in May. Since then, 12 other NASA astronauts have set up Twitter accounts. You can follow them individually or through the NASA Astronauts Twitter account at:

http://twitter.com/NASA_Astronauts

To view the Nov. 15 portion of the Tweetup on YouTube, visit:

http://www.youtube.com/user/NASAtelevision#p/u/3/wl9zBgpmdjQ

To view photos from the STS-129 launch Tweetup, visit:

http://www.flickr.com/photos/nasahqphoto/sets/72157622806978124

For more information about NASA's Tweetup events, visit:

http://www.nasa.gov/tweetup

To view all NASA's Twitter and other social media accounts at:

http://www.nasa.gov/connect

For more information about space shuttle Atlantis' STS-129 mission, visit:

http://www.nasa.gov/shuttle

Space Shuttle Pilot Set to Talk With Tennessee Students from Orbit

Congressman Bart Gordon and Tennessee Technological University in Cookeville will host a live conversation between more than 120 students and NASA astronaut Barry E. Wilmore on Sunday, Nov. 22. Wilmore is the pilot of space shuttle Atlantis, which launched Nov. 16 on an 11-day mission to the International Space Station. Members of Wilmore's family also will attend the event.

The live call from orbit will take place between 11:08 a.m. and 11:28 a.m. CST. Twenty students, ranging from kindergarten to college age, will ask questions of Wilmore and fellow astronauts Nicole Stott and Leland Melvin. Stott has served as a flight engineer and member of the Expedition 21 crew living aboard the International Space Station for more than two months. She will return to Earth aboard Atlantis. Melvin is a mission specialist and crewmate of Wilmore's aboard Atlantis.

Reporters interested in attending the event should contact Monica Greppin at 931-372-3214.

Gordon is the chairman of the House Science and Technology Committee. Wilmore was born and raised in Gordon's district in Tennessee and earned bachelor's and master's degrees in electrical engineering from Tennessee Technological University.

The downlink is one in a series with educational organizations in the U.S. and abroad to improve teaching and learning in science, technology, engineering and mathematics. It is an integral component of NASAs Teaching From Space office. The office promotes learning opportunities and builds partnerships with the education community using the unique environment of human spaceflight.

Tennessee Tech University and WCTE, the local PBS affiliate, will carry a live feed of the event at:

http://www.tntech.edu

and

http://www.wcte.org

For more information about Wilmore, visit:

http://www.jsc.nasa.gov/Bios/htmlbios/wilmore-be.html

For information about NASAs education programs, visit:

http://www.nasa.gov/education

For information about the sts-129 space shuttle mission, visit:

http://www.nasa.gov/shuttle

NASA Provides Venerable Hubble Hardware to Smithsonian

NASA's Wide Field and Planetary 2 camera on display in the National Air and Space Museum's Space Hall.

Two key instruments from NASA's Hubble Space Telescope have a new home in the Smithsonian's National Air and Space Museum in Washington after being returned to Earth aboard space shuttle Atlantis last May.

Astronauts brought back the Wide Field and Planetary Camera 2, or WFPC-2, and the Corrective Optics Space Telescope Axial Replacement, or COSTAR, after more than 15 years in space. The camera returned the iconic images that now adorn posters, album covers, the Internet, classrooms and science text books worldwide.

"This was the camera that saved Hubble," said Ed Weiler, associate administrator for the Science Mission Directorate at NASA Headquarters in Washington. "I have looked forward for a long time to stand in front of this very instrument while on display to the public."

After Hubble's launch and deployment aboard the shuttle in 1990, scientists realized the telescope's primary mirror had a flaw, known as a spherical aberration. The outer edge of the mirror was ground too flat by a depth of 2.2 microns, roughly equal to one-fiftieth the thickness of a human hair. This tiny flaw resulted in fuzzy images because some of the light from the objects being studied was scattered.

Hubble's first servicing mission provided the telescope with hardware that basically acted as eye glasses. Launched in December 1993 aboard space shuttle Endeavour, the mission added the WFPC-2, about the size of a baby grand piano, and COSTAR, about the size of a telephone booth. The WFPC-2 had the optical fix built in, while the COSTAR provided the optical correction for other Hubble instruments.

The WFPC-2 made more than 135,000 observations of celestial objects from 1993 to 2009. The camera was the longest serving and most prolific instrument aboard Hubble.

"For years the Wide Field and Planetary Camera 2 has been taking pictures of the universe," said John Trauger of NASA's Jet Propulsion Laboratory in Pasadena, Calif. "Today, we are taking pictures of the WFPC-2 and I guess if there was ever a camera that deserves to have its picture taken, this is it."

The Hubble instruments will be on display in the National Air and Space Museum's Space Hall through mid-December. They then will travel to Southern California to go on temporary display at several venues. In March 2010, the instruments will return to the Smithsonian Air and Space Museum, where they will take up permanent residency.

NASA's Jet Propulsion Laboratory designed and built the WFPC-2. The COSTAR instrument was built by Ball Aerospace in Boulder, Colo. The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. The project is managed by NASA's Goddard Space Flight Center in Greenbelt, Md. The Space Telescope Science Institute in Baltimore conducts Hubble science operations. The institute is operated for NASA by the Association of Universities for Research in Astronomy Inc., in Washington.

For more information about the Hubble Space Telescope, visit: http://www.nasa.gov/hubble