NASA Chooses Three Finalists for Future Space Science Mission to Venus, an Asteroid or the Moon

NASA has selected three proposals as candidates for the agency's next space venture to another celestial body in our solar system. The final project selected in mid-2011 may provide a better understanding of Earth's formation or perhaps the origin of life on our planet.

The proposed missions would probe the atmosphere and crust of Venus; return a piece of a near-Earth asteroid for analysis; or drop a robotic lander into a basin at the moon's south pole to return lunar rocks back to Earth for study.

NASA will select one proposal for full development after detailed mission concept studies are completed and reviewed. The studies begin during 2010, and the selected mission must be ready for launch no later than Dec. 30, 2018. Mission cost, excluding the launch vehicle, is limited to $650 million.

"These are projects that inspire and excite young scientists, engineers and the public," said Ed Weiler, associate administrator for the Science Mission Directorate at NASA Headquarters in Washington. "These three proposals provide the best science value among eight submitted to NASA this year."

Each proposal team initially will receive approximately $3.3 million in 2010 to conduct a 12-month mission concept study that focuses on implementation feasibility, cost, management and technical plans. Studies also will include plans for educational outreach and small business opportunities.

Astronauts Aboard the Space Station Talk With Troops in Iraq

This is one of a series of images featuring the International Space Station photographed soon after the space shuttle Atlantis and the station began their post-undocking relative separation. Some scenes in the series show parts of the Mediterranean Sea and Africa and Spain in the background.

Some U.S. forces in Iraq will get the chance during the holidays to talk with two NASA astronauts aboard the International Space Station who also are far away from their families and friends. A 20-minute live video downlink will start at 9 a.m. EST on Dec. 29. The event will be carried live on NASA Television and streamed on the agency's Web site.

Station Commander Jeff Williams, a retired U.S. Army colonel, and Flight Engineer T.J. Creamer, an Army colonel, will talk with U.S. forces while orbiting 220 miles above Earth. Service members will have the chance to talk with the astronauts about life on the station, their military careers and what it is like to live in space for up to six months.

Technology developed for the space and Earth science programs at NASA is currently being repurposed for use to protect our soldiers in Iraq and across the globe. Examples include satellite-based communications and weather resources, GPS, and other NASA Spinoffs.

NASA Television will provide live coverage of the conversations, with video from aboard the station during the event. A video file will be available later in the day, with edited footage from both the station and the service members in Iraq.

Keck Telescopes Gaze into Young Star's "Life Zone"

The inner regions of young planet-forming disks offer information about how worlds like Earth form, but not a single telescope in the world can see them. Yet, for the first time, astronomers using the W. M. Keck Observatory in Hawaii have measured the properties of a young solar system at distances closer to the star than Venus is from our sun.

"When it comes to building rocky planets like our own, the innermost part of the disk is where the action is," said team member William Danchi at NASA's Goddard Space Flight Center in Greenbelt, Md. Planets forming in a star's inner disk may orbit within its "habitable zone," where conditions could potentially support the development of life.

To achieve the feat, the team used the Keck Interferometer to combine infrared light gathered by both of the observatory's twin 10-meter telescopes, which are separated by 85 meters. The double-barreled approach gives astronomers the effective resolution of a single 85-meter telescope -- several times larger than any now planned.

"Nothing else in the world provides us with the types of measurements the Keck Interferometer does," said Wesley Traub at Caltech's Jet Propulsion Laboratory in Pasadena, Calif. "In effect, it's a zoom lens for the Keck telescopes."

Off-Duty Day for New Expanded Crew

Following the arrival of the three new Expedition 22 crew members Tuesday, the crew aboard the International Space Station had an off-duty day Wednesday. The crew members spent most of the day sleeping due to the late finish of the docking activities.

NASA astronaut T.J. Creamer, Russian cosmonaut Oleg Kotov and Japan Aerospace Exploration Agency astronaut Soichi Noguchi docked with their new home at 5:48 p.m. EST Tuesday. The trio launched aboard the Soyuz TMA-17 spacecraft at 4:52 p.m. Sunday from the Baikonur Cosmodrome in Kazakhstan.

From inside the station, Commander Jeff Williams and Flight Engineer Maxim Suraev monitored the approach of the Russian spacecraft as it docked to the Earth-facing port of the Zarya module.

After completion of leak checks, the hatches between the two vehicles were opened at 7:30 p.m. Williams and Suraev, who arrived at the station Oct. 2 aboard the Soyuz TMA-16, welcomed the new Expedition 22 flight engineers aboard their orbital home for the next five months.

Creamer, 50, is making his first flight into space. Selected as an astronaut in 1998, Creamer was a support astronaut for the Expedition 3 crew and worked with hardware integration and robotics.

Kotov, 44, is making his second spaceflight, having previously served six months aboard the station as an Expedition 15 flight engineer in 2007. Kotov will be a flight engineer for Expedition 22 and assume the duties of Expedition 23 commander when Williams and Suraev depart in March 2010.

Noguchi is making his second spaceflight. He flew on the STS-114 return-to-flight mission of Discovery in 2005 and conducted three spacewalks totaling more than 20 hours.

Tropical Storm David Forms and Romps in the Southern Indian Ocean

Tropical Storm David formed over the weekend and as a depression, has been romping around the open waters of the Southern Indian Ocean and will continue to do just that. David is located approximately 580 nautical miles west-southwest of Diego Garcia, near 11.3 degrees South and 63.8 degrees East.

David has been tracking in a westward direction, but it now changing course and moving east-southeast near 7 mph. David's maximum sustained winds are near 46 mph, and the storm may strengthen over the next couple of days.



Animated infrared satellite imagery, such as that using NASA's Atmospheric Infrared Sounder (AIRS) instrument on the Aqua satellite, indicates slight improvement in organization over the past 12 hours despite moderate northwesterly vertical wind shear. AIRS captured an infrared and visible image of David on December 21 at 09:17 UTC (4:17 a.m. ET) and noticed that David had some high thunderstorm tops indicating strong convection and strong thunderstorms with heavy rainfall. The cloud tops were as cold or colder than minus 63 degrees Fahrenheit!

On December 21 at 1504 UTC (10:04 ET) the Tropical Rainfall Measuring Mission (TRMM) satellite, a satellite managed by NASA and the Japanese Space Agency, flew over David to analyze the storm's rainfall. The image showed convective banding, that is, bands of thunderstorms, wrapping from the north of the storm into the south of the storm. Microwave imagery, however, such as that from NASA's Aqua satellite showed that David's low-level circulation is partially exposed, opening the storm up to wind shear, which could weaken it.

Astronauts Test Glenn Exercise Harnesses

Imagine that you want to exercise on a treadmill. You step onto the machine and select your desired speed. As the belt starts moving, you start walking and eventually running. Your feet rhythmically hit the belt, and you get a nice workout.

In space, it isn't that simple.

For astronauts living in space, like those who reside on the International Space Station, getting a good workout is equally -- and in some ways even more important -- than for earthbound people.

"Crew members exercise for a host of important reasons. There's a psychological benefit to exercise, and crew members work out to combat spaceflight deconditioning -- to help fend off the bone loss that they experience in microgravity and to help maintain muscle strength and cardiovascular endurance. All of these things are adversely affected by long-duration space flight," says Gail Perusek, Manager for Exercise Physiology and Countermeasures Project at NASA's Glenn Research Center.

Hubble Finds Smallest Kuiper Belt Object Ever Seen

NASA's Hubble Space Telescope has discovered the smallest object ever seen in visible light in the Kuiper Belt, a vast ring of icy debris that is encircling the outer rim of the solar system just beyond Neptune.

The needle-in-a-haystack object found by Hubble is only 3,200 feet across and a whopping 4.2 billion miles away. The smallest Kuiper Belt Object (KBO) seen previously in reflected light is roughly 30 miles across, or 50 times larger.

This is the first observational evidence for a population of comet-sized bodies in the Kuiper Belt that are being ground down through collisions. The Kuiper Belt is therefore collisionally evolving, meaning that the region's icy content has been modified over the past 4.5 billion years.

The object detected by Hubble is so faint - at 35th magnitude -- it is 100 times dimmer than what the Hubble can see directly.

So then how did the space telescope uncover such a small body?

In a paper published in the December 17th issue of the journal Nature, Hilke Schlichting of the California Institute of Technology in Pasadena, Calif., and her collaborators are reporting that the telltale signature of the small vagabond was extracted from Hubble's pointing data, not by direct imaging.

Hubble has three optical instruments called Fine Guidance Sensors (FGS). The FGSs provide high-precision navigational information to the space observatory's attitude control systems by looking at select guide stars for pointing. The sensors exploit the wavelike nature of light to make precise measurement of the location of stars.

Schlichting and her co-investigators determined that the FGS instruments are so good that they can see the effects of a small object passing in front of a star. This would cause a brief occultation and diffraction signature in the FGS data as the light from the background guide star was bent around the intervening foreground KBO.

TMA-17 Arrives at Pad, Crew Prepares for Launch

Early Friday morning at the Baikonur Cosmodrome in Kazakhstan, the Soyuz TMA-17 spacecraft left its processing facility on a rail car then was vertically set up at its launch pad. On Sunday at 4:52 p.m. EST, three new crew members will launch aboard the TMA-17 to join the Expedition 22 crew after docking to the International Space Station. They dock to the International Space Station Tuesday.

Watch NASA TV for coverage of the launch, which begins Sunday at 4 p.m.

NASA astronaut T.J. Creamer, Russian cosmonaut Oleg Kotov and Japanese astronaut Soichi Noguchi will expand Expedition 22 to five crew members. Residing onboard the station since Oct. 2 are Commander Jeff Williams and Flight Engineer Maxim Suraev.

While they wait for the arrival of the rest of the crew, Williams and Suraev continue their normal science, maintenance and exercise activities.

The two orbiting crew members each performed different experiments that measure an astronaut’s performance of various tasks during long-term spaceflight. Williams performed an experiment that studies how the lack of gravity affects concentration, verbal working memory, attention, short-term memory, spatial processing and math skills. Suraev performed tests and games to assess the actual mental state, prediction and correction of quality of professional task performance in a space flight.

New Results from a Terra-ific Decade in Orbit

December 18, 2009, marks the tenth year since the launch of Terra, one of NASA's "flagship" Earth observing satellites. But the decade is more than just a mechanical milestone. With each additional day and year that the satellite monitors Earth, scientists achieve a lengthened record of Earth's vital signs. It's that record that helps scientists assess the health of Earth's ocean, land, and atmosphere, and determine how these systems are changing.



"Earth system science is a relatively young science," said Marc Imhoff, project scientist for the mission and a researcher at NASA's Goddard Space Flight Center in Greenbelt, Md. "Terra's sensors have provided the first coordinated set of observations allowing us to link Earth system processes across space and time so we can better understand how they function together and how we interact with them."

Since Terra's five instruments officially saw "first light" on Feb 24, 2000, after a post-launch checkout, the data have continued to advance Earth system science. Here's a sample of the latest developments to be presented by Terra researchers at the Fall Meeting of the American Geophysical Union in San Francisco.

NASA's AIM Satellite and Models are Unlocking the Secrets of Mysterious "Night-Shining" Clouds

This image of Polar Mesospheric Clouds (PMC) from the Aeronomy of Ice in the Mesosphere Cloud Imaging and Particle Size (AIM-CIPS) instrument on July 14, 2009 in the northern polar region. The North Pole (90N) is in the center. Latitude bands of 80N, 70N, and 60N are also indicated by the light blue circles.

NASA's Aeronomy of Ice in the Mesosphere (AIM) satellite has captured five complete polar seasons of noctilucent (NLC) or "night-shining" clouds with an unprecedented horizontal resolution of 3 miles by 3 miles. Results show that the cloud season turns on and off like a "geophysical light bulb" and they reveal evidence that high altitude mesospheric "weather" may follow similar patterns as our ever-changing weather near the Earth's surface. These findings were unveiled today at the Fall Meeting of the American Geophysical Union today in San Francisco.

The AIM measurements have provided the first comprehensive global-scale view of the complex life cycle of these clouds, also called Polar Mesospheric Clouds (PMCs), over three entire Northern Hemisphere and two Southern Hemisphere seasons revealing more about their formation, frequency and brightness and why they appear to be occurring at lower latitudes than ever before

NASA's WISE Eye on the Universe Begins All-Sky Survey Mission

NASA's Wide-field Infrared Survey Explorer, or WISE, lifted off over the Pacific Ocean this 14tht morning on its way to map the entire sky in infrared light.

A Delta II rocket carrying the spacecraft launched at 6:09 a.m. PST (9:09 a.m. EST) from Vandenberg Air Force Base in California. The rocket deposited WISE into a polar orbit 326 miles above Earth.

"WISE thundered overhead, lighting up the pre-dawn skies," said William Irace, the mission's project manager at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "All systems are looking good, and we are on our way to seeing the entire infrared sky better than ever before."

Engineers acquired a signal from the spacecraft via NASA's Tracking and Data Relay Satellite System just 10 seconds after the spacecraft separated from the rocket. Approximately three minutes later, WISE re-oriented itself with its solar panels facing the sun to generate its own power. The next major event occurred about 17 minutes later. Valves on the cryostat, a chamber of super-cold hydrogen ice that cools the WISE instrument, opened. Because the instrument sees the infrared, or heat, signatures of objects, it must be kept at chilly temperatures. Its coldest detectors are less than minus 447 degrees Fahrenheit.

"WISE needs to be colder than the objects it's observing," said Ned Wright of UCLA, the mission's principal investigator. "Now we're ready to see the infrared glow from hundreds of thousands of asteroids, and hundreds of millions of stars and galaxies."

With the spacecraft stable, cold and communicating with mission controllers at JPL, a month-long checkout and calibration is underway.

WISE will see the infrared colors of the whole sky with sensitivity and resolution far better than the last infrared sky survey, performed 26 years ago. The space telescope will spend nine months scanning the sky once, then one-half the sky a second time. The primary mission will end when WISE's frozen hydrogen runs out, about 10 months after launch.

WISE Launch Set for Monday, Dec. 14

Image tells: A Delta II rocket is set to launch with NASA's Wide-field Infrared Survey Explorer from Vandenberg Air Force Base, Calif.

From Vandenberg Air Force Base in Calif., all systems are “Go” for WISE’s launch attempt aboard a Delta II rocket on Monday morning, Dec. 14. Weather forecast remains at 80-percent favorable conditions at launch time. The rollback of the mobile service tower is scheduled for 8:30 p.m. PST Sunday evening.

The problem with the motion of a booster steering engine that occurred during pre-launch testing for Friday’s launch attempt resulted in a decision to remove and replace a suspect component. Work is now complete and all tests have been performed with good results.

The launch time is set for 6:09:33 a.m. PST (9:09 a.m. EST) at the opening of a 14-minute window. NASA TV and NASA's Launch Blog coverage start at 4 a.m. PST (7 a.m. EST).

The WISE spacecraft will circle Earth over the poles, scanning the entire sky one-and-a-half times in nine months. The mission will uncover hidden cosmic objects, including the coolest stars, dark asteroids and the most luminous galaxies.

Wide-field Infrared Survey Explorer Set for Dec. 14 Launch

NASA's Wide-field Infrared Survey Explorer has been wrapped in the outer nose cone, or "fairing," that will protect it during its scheduled Dec. 9 launch from Vandenberg Air Force Base, Calif. Image credit: NASA/VAFB

The launch of NASA’s Wide-field Infrared Survey Explorer (WISE) mission is now rescheduled for Dec. 14, with a launch window of 6:09-6:23 a.m. PST (9:09:33 - 9:23:51 a.m. EST). The first launch attempt scheduled for Dec. 11 was delayed due to an anomaly in the motion of a booster steering engine.

Mission managers have implemented a plan to completely resolve the anomaly. This plan includes removing and replacing a suspect component on Friday, Dec. 11 allowing the Delta II to be ready for Monday’s launch attempt. The current weather forecast calls for an 80 percent chance of acceptable weather during the launch window.

The WISE spacecraft will circle Earth over the poles, scanning the entire sky one-and-a-half times in nine months. The mission will uncover hidden cosmic objects, including the coolest stars, dark asteroids and the most luminous galaxies.

Chopper Drop Tests New Technology

How do you make a helicopter safer to fly? You crash one.

NASA aeronautics researchers recently dropped a small helicopter from a height of 35 feet (10.7 m) to see whether an expandable honeycomb cushion called a deployable energy absorber could lessen the destructive force of a crash.

On impact, the helicopter's skid landing gear bent outward, but the cushion attached to its belly kept the rotorcraft's bottom from touching the ground. Four crash test dummies along for the ride appeared only a little worse for the wear.


Researchers must analyze the test results before they can say for sure whether the deployable energy absorber worked as designed.

"I'd like to think the research we're doing is going to end up in airframes and will potentially save lives," said Karen Jackson, an aerospace engineer who oversaw the test at NASA's Langley Research Center in Hampton, Va.

According to the National Transportation Safety Board, more than 200 people are injured in helicopter accidents in the United States each year, in part because helicopters fly in riskier conditions than most other aircraft. They fly close to the ground, not far from power lines and other obstacles, and often are used for emergencies, including search and rescue and medical evacuations.

Version 1.1 of the NASA App Is Now Available!

The first official NASA App invites you to discover a wealth of NASA information right on your iPhone or iPod Touch. The NASA App collects, customizes and delivers an extensive selection of dynamically updated information, images and videos from various online NASA sources in a convenient mobile package. Come explore with us.

Features:

• NASA Mission Information


• Launch Information & Countdown clocks


• Sighting Opportunities (Visible Passes for ISS, Space Shuttle)


• Mission Orbit Trackers


• NASA Image of the Day


• Astronomy Picture of the Day


• NASA Videos


• NASA Twitter Feeds/Mission Updates

What's New In This Version:

• Visible sighting opportunities listed for the International Space Station (ISS) and Space Shuttle, by home location and through search for location


• Richer Mission details and more content


• Enhancements to Videos and Updates panels


• High-resolution image option (configured in device settings)


• Status updates on upcoming launches


• Prevent sleep mode setting for tracking launches (configured in device settings)

NASA Uses Twin Processes to Develop New Tank Dome Technology

NASA has partnered with Lockheed Martin Space Systems in Denver, Colo., and MT Aerospace in Augsburg, Germany, to successfully manufacture the first full-scale friction stir welded and spun formed tank dome designed for use in large liquid propellant tanks.

The NASA and Lockheed Martin team traveled to Germany to witness the first successful aerospace application of two separate manufacturing processes: friction stir welding, a solid-state joining process, and spin forming, a metal working process used to form symmetric parts.

The twin processes were used by MT Aerospace to produce an 18-foot-diameter tank dome using high-strength 2195 aluminum-lithium. The diameter of this development dome matches the tank dimensions of the upper stage of the ARES I launch vehicle under development by NASA, as well as the central stage of the European Ariane V launcher.

"This new manufacturing technology allows us to use a thinner, high-strength alloy that will reduce the weight of future liquid propellant tanks by 25 percent, compared to current tank designs that use a lower-strength aluminum alloy that weighs more," said Louis Lollar, project lead for the Friction Stir Weld Spun Form Dome Project at NASA's Marshall Space Flight Center in Huntsville, Ala.

The concave net shape spin forming process, patented by MT Aerospace, drastically simplifies the manufacturing of large tank domes and reduces cost by eliminating manufacturing steps, such as machining and assembly welding, that are required when manufacturing traditional gore panel - a pie-shaped section of the tank dome --construction domes.

WISE Snug in Its Nose Cone

NASA's Wide-field Infrared Survey Explorer has been wrapped in the outer nose cone, or "fairing," that will protect it during its scheduled Dec. 9 launch from Vandenberg Air Force Base, Calif.

The fairing will split open like a clamshell about five minutes after launch. The spacecraft will circle Earth over the poles, scanning the entire sky one-and-a-half times in nine months. The mission will uncover hidden cosmic objects, including the coolest stars, dark asteroids and the most luminous galaxies.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages WISE 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.

Fermi Telescope Peers Deep into Microquasar

NASA's Fermi Gamma-ray Space Telescope has made the first unambiguous detection of high-energy gamma-rays from an enigmatic binary system known as Cygnus X-3. The system pairs a hot, massive star with a compact object -- either a neutron star or a black hole -- that blasts twin radio-emitting jets of matter into space at more than half the speed of light.

Astronomers call these systems microquasars. Their properties -- strong emission across a broad range of wavelengths, rapid brightness changes, and radio jets -- resemble miniature versions of distant galaxies (called quasars and blazars) whose emissions are thought to be powered by enormous black holes.

"Cygnus X-3 is a genuine microquasar and it's the first for which we can prove high-energy gamma-ray emission," said Stéphane Corbel at Paris Diderot University in France.

The system, first detected in 1966 as among the sky's strongest X-ray sources, was also one of the earliest claimed gamma-ray sources. Efforts to confirm those observations helped spur the development of improved gamma-ray detectors, a legacy culminating in the Large Area Telescope (LAT) aboard Fermi.

At the center of Cygnus X-3 lies a massive Wolf-Rayet star. With a surface temperature of 180,000 degrees F, or about 17 times hotter than the sun, the star is so hot that its mass bleeds into space in the form of a powerful outflow called a stellar wind. "In just 100,000 years, this fast, dense wind removes as much mass from the Wolf-Rayet star as our sun contains," said Robin Corbet at the University of Maryland, Baltimore County.

Every 4.8 hours, a compact companion embedded in a disk of hot gas wheels around the star. "This object is most likely a black hole, but we can't yet rule out a neutron star," Corbet noted.

Fermi's LAT detects changes in Cygnus X-3's gamma-ray output related to the companion's 4.8-hour orbital motion. The brightest gamma-ray emission occurs when the disk is on the far side of its orbit. "This suggests that the gamma rays arise from interactions between rapidly moving electrons above and below the disk and the star's ultraviolet light," Corbel explained.

When ultraviolet photons strike particles moving at an appreciable fraction of the speed of light, the photons gain energy and become gamma rays. "The process works best when an energetic electron already heading toward Earth suffers a head-on collision with an ultraviolet photon," added Guillaume Dubus at the Laboratory for Astrophysics in Grenoble, France. "And this occurs most often when the disk is on the far side of its orbit."

Through processes not fully understood, some of the gas falling toward Cygnus X-3's compact object instead rushes outward in a pair of narrow, oppositely directed jets. Radio observations clock gas motion within these jets at more than half the speed of light.

Between Oct. 11 and Dec. 20, 2008, and again between June 8 and Aug. 2, 2009, Cygnus X-3 was unusually active. The team found that outbursts in the system's gamma-ray emission preceded flaring in the radio jet by roughly five days, strongly suggesting a relationship between the two.

NASA Provides Venerable Hubble Hardware to Smithsonian

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.

Inventors Answer Call for New Glove Designs

Two independent inventors answered NASA's call for innovative new designs for the next generation of astronaut gloves. Today's spacewalkers have to contend with bulky gloves that stiffen when pressurized, making it tough to grip and flex while completing tasks in the vacuum of space.

Peter Homer and Ted Southern put their prototypes to the test during NASA's 2009 Astronaut Glove Challenge, held Nov. 19 at the Astronaut Hall of Fame in Titusville, Fla., near NASA's Kennedy Space Center.

Homer, an engineer from Southwest Harbor, Maine, was awarded $250,000 after placing first. Southern, a sculpture major at New York's Pratt Institute, earned second place and $100,000.

The ultimate goal of the Astronaut Glove Challenge is to improve the current design, resulting in a stronger and more flexible glove that will reduce the hand fatigue experienced by astronauts working in space.

For the first Astronaut Glove Challenge held in 2007, competitors supplied only the inner pressure-restraining layer. The outer layer, which provides protection against extreme temperatures and micrometeoroids, was an added requirement this year. Representatives from NASA and the agency's spacesuit contractor, ILC Dover, observed and noted the gloves' performances in a series of three tests.

The competitor inserted his gloved arm and hand into a depressurized glove box for the dexterity and flexibility test, completing cycles of movements and tasks, such as gripping a handle, using tools, flexing the hand and wrist, and touching the tip of the thumb to the tip of each finger.

In the joint force test, test operators from ILC Dover sealed and pressurized each glove to 4.3 pounds per square inch (psi) of internal pressure, then tugged it through its full range of motion while measuring the amount of force each movement required.

Finally, the gloves' strength capabilities were measured in the burst test. The room quieted as test operators sealed the glove and filled it with water, slowly increasing the pressure. Competitors, judges and other spectators leaned forward, watching the glove for signs of weakness or rupture.

NASA's Wise Gets Ready to Survey the Whole Sky

NASA's Wide-field Infrared Survey Explorer, or Wise, is chilled out, sporting a sunshade and getting ready to roll. NASA's newest spacecraft is scheduled to roll to the pad on Friday, Nov. 20, its last stop before launching into space to survey the entire sky in infrared light.

Wise is scheduled to launch no earlier than 6:09 a.m. PST (9:09 a.m. EST) on Dec. 9 from Vandenberg Air Force Base in California. It will circle Earth over the poles, scanning the entire sky one-and-a-half times in nine months. The mission will uncover hidden cosmic objects, including the coolest stars, dark asteroids and the most luminous galaxies.


"The eyes of Wise are a vast improvement over those of past infrared surveys," said Edward "Ned" Wright, the principal investigator for the mission at UCLA. "We will find millions of objects that have never been seen before."

The mission will map the entire sky at four infrared wavelengths with sensitivity hundreds to hundreds of thousands of times greater than its predecessors, cataloging hundreds of millions of objects. The data will serve as navigation charts for other missions, pointing them to the most interesting targets. NASA's Hubble and Spitzer Space Telescopes, the European Space Agency's Herschel Space Observatory, and NASA's upcoming Sofia and James Webb Space Telescope will follow up on Wise finds.

"This is an exciting time for space telescopes," said Jon Morse, NASA's Astrophysics Division director at NASA Headquarters in Washington. "Many of the telescopes will work together, each contributing different pieces to some of the most intriguing puzzles in our universe."

COBE Satellite Marks 20th Anniversary

NASA's Cosmic Background Explorer (COBE) satellite rocketed into Earth orbit on Nov. 18, 1989, and quickly revolutionized our understanding of the early cosmos. Developed and built at Goddard Space Flight Center in Greenbelt, Md., COBE precisely measured and mapped the oldest light in the universe -- the cosmic microwave background.

COBE showed that the radiation's spectrum agrees exactly with predictions based on the Big Bang theory. And COBE's map of slight hot and cold spots within this background let scientists glimpse the roots of cosmic structure we see around us today. In essence, COBE produced the first "baby picture" of the universe.

For these results, COBE scientists John Mather, at Goddard, and George Smoot, at the University of California, Berkeley, shared the 2006 Nobel Prize in physics. The mission ushered cosmologists into a new era of precision measurements, paving the way for deeper exploration of the microwave background by NASA's ongoing WMAP mission and the European Space Agency's new Planck satellite.

The cosmic microwave background radiation is a remnant of the Big Bang. These minute temperature variations (depicted here as varying shades of blue and purple) are linked to slight density variations in the early universe. These variations are believed to have given rise to the structures that populate the universe today: clusters of galaxies, as well as vast, empty regions. This image, representing data collected between 1990 and 1992, received much publicity at the time. It was later superseded by a more accurate four-year COBE map.

NASA EDGE Nominated for ‘Best Video Podcast’ in the 5th Annual Podcast Awards! ›› Vote Now for NASA EDGE!

NASA EDGE continues their unprecedented, unscripted journey through the world of video podcasting with their very first award nomination. This is no small accomplishment considering that only two and half years ago, they weren’t sure that they would find an audience.

Well, they have. Almost three years and 3.2 million downloads later, NASA EDGE is now recognized in the company of such internet greats and fellow nominees as “Buzz out Loud,” “Diggnation” and “Filmriot” just to name a few.

In fact, the 5th Annual Podcast Awards, managed by Podcast Connect Inc., mentioned on their Web site that this year’s competition received more than 321,000 nominations for over 3,500 different shows.

What is NASA EDGE?

NASA EDGE is different. Unscripted and unpredictable, NASA EDGE takes a unique look in and around the greatest space program on the planet. They have hosted the Great Moonbuggy Race, examined NASA spinoff technology at the X Games, followed the Desert-RATS with an unconventional set of duct tape boots, coined the term Magnetospherence and even made an appearance on ESPN’s nationally syndicated "Mike & Mike in the Morning" show.

Check out their latest Vodcast, which added a new wrinkle. In October they covered NASA’s historic Ares I-X Flight Demonstration live on the Web. That show featured the entire broadcast team and an attempt at defining and redefining 'triboelectrification.'

Of course, NASA EDGE isn’t just a video podcast. If you have questions, comments or thoughts about NASA or NASA EDGE, you can friend them on facebook and ask questions, chat or check out some exclusive facebook videos.

Or if you just want to keep up with their latest shows or activities you can follow them on twitter (@NASA_EDGE).

If all goes well, you’ll hear from them the second they win their very first award!

NASA Technology Spinoffs Art Contest Winner Presentation at the Statue of Liberty

NASA Goddard Space Flight Center in Greenbelt, Md. is recognizing award-winning artwork honoring NASA Spinoff technology that was used to restore the Statue of Liberty National Monument, a unit of the National Park Service.

Students are recognizing NASA Goddard's 50th anniversary by reflecting on science, technology, engineering and the fine arts. NASA Goddard was opened in 1959.

NASA's Innovative Partnerships Program (IPP) Office sponsored "Goddard Celebrates 50 Years of Technology Spinoffs Art Contest" last winter. The purpose of the contest was to allow middle and high school students across the country to demonstrate through art, their knowledge of how NASA Goddard scientific technological achievements have made impacts on the quality of life. Some of the reference or source material the students were to use was the IPP Office annual publication, NASA Spinoff magazine, and the IPP Office website.

After receiving and reviewing contest submissions, Ja Hyun "Ashely" Lim was chosen as the winner. At the time of contest submission, she was a ninth grader at North County High School in Glen Burnie, Md. Lim’s eloquent rendering of a paint brush stroke from the Space Shuttle’s lift off pad launch gantries to the Statute of Liberty monument plainly demonstrates "movement" of NASA technology from one application of a technology to another external to NASA.

The connection between the Statue of Liberty and NASA is in a NASA Goddard-developed technology. When the Statue of Liberty was being restored in the early 1980s, the bars that help to support the copper skin of the Statue of Liberty were covered with a corrosion-resistant coating developed by NASA Goddard engineers. The coating is known as IC531, and is an aerospace Spinoff product manufactured by Inorganic Coatings, Inc. of Malvern, Penn.

IC531 was used as an interior structure primer coating for Miss Liberty. The coating was developed by NASA Goddard to protect gantries and other structures at NASA's Kennedy Space Center, Fla. launch site.

The high-ratio silicate formulation in IC531 bonds to steel and in just 30 minutes and creates a very hard ceramic finish with superior adhesion and abrasion resistance.

Lim was honored at the NASA Goddard Celebrates 50 Years of Technology Spinoffs Event this past summer. In the spirit of cooperation, the NASA Goddard IPP will be presenting a framed copy of Lim’s artwork to the National Park Service at the Statue of Liberty on Nov. 13 at 9:30 a.m. EST at Ellis Island, N.Y.

NASA's Great Observatories Celebrate International Year of Astronomy

In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The entire image width covers about one-half a degree, about the same angular width as the full moon. Credit: NASA, ESA, SSC, CXC, and STScI

A never-before-seen view of the turbulent heart of our Milky Way galaxy is being unveiled by NASA on Nov. 10. This event will commemorate the 400 years since Galileo first turned his telescope to the heavens in 1609.

In celebration of this International Year of Astronomy, NASA is releasing images of the galactic center region as seen by its Great Observatories to more than 150 planetariums, museums, nature centers, libraries and schools across the country.

The sites will unveil a giant, 6-foot-by-3-foot print of the bustling hub of our galaxy that combines a near-infrared view from the Hubble Space Telescope, an infrared view from the Spitzer Space Telescope and an X-ray view from the Chandra X-ray Observatory into one multi-wavelength picture. Experts from all three observatories carefully assembled the final image from large mosaic photo surveys taken by each telescope. This composite image provides one of the most detailed views ever of our galaxy's mysterious core.

Participating institutions also will display a matched trio of Hubble, Spitzer and Chandra images of the Milky Way's center on a second large panel measuring 3 feet by 4 feet. Each image shows the telescope's different wavelength view of the galactic center region, illustrating not only the unique science each observatory conducts, but also how far astronomy has come since Galileo.

Each telescope's contribution is presented in a different color:
Yellow represents the near-infrared observations of Hubble. They outline the energetic regions where stars are being born as well as reveal hundreds of thousands of stars.

Red represents the infrared observations of Spitzer. The radiation and winds from stars create glowing dust clouds that exhibit complex structures from compact, spherical globules to long, stringy filaments.

Blue and violet represent the X-ray observations of Chandra. X-rays are emitted by gas heated to millions of degrees by stellar explosions and by outflows from the supermassive black hole in the galaxy's center. The bright blue blob on the left side is emission from a double star system containing either a neutron star or a black hole.

NASA Reproduces a Building Block of Life in Laboratory

NASA scientists studying the origin of life have reproduced uracil, a key component of our hereditary material, in the laboratory. They discovered that an ice sample containing pyrimidine exposed to ultraviolet radiation under space-like conditions produces this essential ingredient of life.

Pyrimidine is a ring-shaped molecule made up of carbon and nitrogen and is the basic structure for uracil, part of a genetic code found in ribonucleic acid (RNA). RNA is central to protein synthesis, but has many other roles.

"We have demonstrated for the first time that we can make uracil, a component of RNA, non-biologically in a laboratory under conditions found in space," said Michel Nuevo, research scientist at NASA's Ames Research Center, Moffett Field, Calif. "We are showing that these laboratory processes, which simulate occurrences in outer space, can make a fundamental building block used by living organisms on Earth."

Nuevo is the lead author of a research paper titled “Formation of Uracil from the Ultraviolet Photo-Irradiation of Pyrimidine in Pure Water Ices,” Astrobiology vol. 9 no. 7, published Oct. 1, 2009.

NASA Ames scientists have been simulating the environments found in interstellar space and the outer solar system for years. During this time, they have studied a class of carbon-rich compounds, called polycyclic aromatic hydrocarbons (PAHs), which have been identified in meteorites, and are the most common carbon-rich compound observed in the universe. PAHs typically are six-carbon ringed structures that resemble fused hexagons, or a piece of chicken wire.

Pyrimidine also is found in meteorites, although scientists still do not know its origin. It may be similar to the carbon-rich PAHs, in that it may be produced in the final outbursts of dying, giant red stars, or formed in dense clouds of interstellar gas and dust.

“Molecules like pyrimidine have nitrogen atoms in their ring structures, which makes them somewhat whimpy. As a less stable molecule, it is more susceptible to destruction by radiation, compared to its counterparts that don’t have nitrogen,” said Scott Sandford, a space science researcher at Ames. “We wanted to test whether pyrimidine can survive in space, and whether it can undergo reactions that turn it into more complicated organic species, such as the nucleobase uracil.”

Spitzer Observes a Chaotic Planetary System

Before our planets found their way to the stable orbits they circle in today, they wiggled and jostled about like unsettled children. Now, NASA's Spitzer Space Telescope has found a young star with evidence for the same kind of orbital hyperactivity. Young planets circling the star are thought to be disturbing smaller comet-like bodies, causing them to collide and kick up a huge halo of dust.

The star, called HR 8799, was in the news last November 2008, for being one of the first of two stars with imaged planets. Ground-based telescopes at the W.M. Keck Observatory and the Gemini Observatory, both in Hawaii, took images of three planets orbiting in the far reaches of the system, all three being roughly 10 times the mass of Jupiter. Another imaged planet was also announced at the same time around the star Fomalhaut, as seen by NASA's Hubble Space Telescope. Both HR 8799 and Fomalhaut are younger and more massive than our sun.

Astronomers had previously used both Spitzer and Hubble to image a rotating disk of planetary debris around Fomalhaut, which is 25 light-years from Earth. HR 8799 is about five times farther away, so scientists weren't sure if Spitzer would be able to capture a picture of its disk. To their amazement and delight, Spitzer succeeded. The picture can be seen online at http://spitzer.caltech.edu/images/2781 .

The Spitzer team, led by Kate Su of the University of Arizona, Tucson, says the giant cloud of fine dust around the disk is very unusual. They say this dust must be coming from collisions among small bodies similar to the comets or icy bodies that make up today's Kuiper Belt objects in our solar system. The gravity of the three large planets is throwing the smaller bodies off course, causing them to migrate around and collide with each other. Astronomers think the three planets might have yet to reach their final stable orbits, so more violence could be in store.

"The system is very chaotic and collisions are spraying up a huge cloud of fine dust," said Su. "What's exciting is that we have a direct link between a planetary disk and imaged planets. We've been studying disks for a long time, but this star and Fomalhaut are the only two examples of systems where we can study the relationships between the locations of planets and the disks."

When our solar system was young, it went through similar planet migrations. Jupiter and Saturn moved around quite a bit, throwing comets around, sometimes into Earth. Some say the most extreme part of this phase, called the late heavy bombardment, explains how our planet got water. Wet, snowball-like comets are thought to have crashed into Earth, delivering life's favorite liquid.

New Science Findings From Messenger's Third Mercury Flyby

A MESSENGER color observation of Mercury obtained as the spacecraft approached the planet for its third and final flyby on 29 September 2009. The 1000, 700, and 430 nm filters were combined in red, green, and blue to create this color image (approximately 5 km/pixel resolution), the last that will be acquired until MESSENGER goes into orbit around Mercury in March of 2011. Only 6% of Mercury's surface in this image had not been viewed previously by spacecraft, and most of the measurements made by MESSENGER's other instruments during this flyby were made prior to closest approach. The observations nonetheless revealed fresh surprises.

NASA Innovation Partnerships Program (IPP), Technology Infusion

Much of what we gain from our space exploration is in the scientific and technological progress that comes in the process of doing it. Many of those technologies are the direct result of NASA supported funding for both internal R&D projects performed at NASA centers and external research from the small business community. As a result of these expanding needs for new capabilities to explore space, NASA missions often result in technologies which have applications beyond aerospace. These technologies while targeted for integration into the mainstream NASA flight programs, can also be commercialized creating new marketplace products and provide opportunities for improving the quality of life for the American public right here on earth.

For NASA, Technology infusion is the process of strategically binding technical needs and potential solutions. These innovative solutions, be they hardware or software; enhancing or enabling; near-term or far-term; low Technology Readiness Level (TRL) or High TRL, NASA internally or externally developed; must all be managed through some aspect of transition from their originating source to the targeted challenges within NASA's programs and projects.

The IPP, Technology Infusion Element includes the Small Business Innovative Research (SBIR), the Small Business Technology Transfer (STTR) and the IPP Seed Fund. Together these programs provide pathways from these originating sources to IPPs' technology portfolio, and provide enabling infrastructures that enhance the infusion of these technologies in NASA missions and programs. These programs allow the agency to implement successful technology infusion and receive benefits in the following ways:

• Leverage limited program funds for technology development


• Leverage partners' funds/investments to achieve NASA's research and development (R&D) goals


• Avoid additional program cost by providing a portfolio of technology solutions


• Accelerate technology maturation through concurrent Research and Development


• Make informed decisions when selecting technologies for programs/projects/missions (i.e., better trade space information)


• Increase the return on its R&D investment with additional marketplace applications of technologies (benefits for both NASA and the public.

NASA issues annual program solicitations that set forth a substantial number of R/R&D topics and subtopic areas consistent with stated agency needs or missions. Both the list of topics and the description of the topics and subtopics are sufficiently comprehensive to provide a wide range of opportunity for Small Business Concerns (SBC) to participate in NASA research or R&D programs. Topics and subtopics emphasize the need for proposals with advanced concepts to meet specific agency R/R&D needs.

New Celestial Map Gives Directions for GPS

Many of us have been rescued from unfamiliar territory by directions from a Global Positioning System (GPS) navigator. GPS satellites send signals to a receiver in your GPS navigator, which calculates your position based on the location of the satellites and your distance from them. The distance is determined by how long it took the signals from various satellites to reach your receiver.

The system works well, and millions rely on it every day, but what tells the GPS satellites where they are in the first place?

"For GPS to work, the orbital position, or ephemeris, of the satellites has to be known very precisely," said Dr. Chopo Ma of NASA's Goddard Space Flight Center in Greenbelt, Md. "In order to know where the satellites are, you have to know the orientation of the Earth very precisely."

This is not as obvious as simply looking at the Earth – space is not conveniently marked with lines to determine our planet's position. Even worse, "everything is always moving," says Ma. Earth wobbles as it rotates due to the gravitational pull (tides) from the moon and the sun. Even apparently minor things like shifts in air and ocean currents and motions in Earth's molten core all influence our planet's orientation.

Just as you can use landmarks to find your place in a strange city, astronomers use landmarks in space to position the Earth. Stars seem the obvious candidate, and they were used throughout history to navigate on Earth. "However, for the extremely precise measurements needed for things like GPS, stars won't work, because they are moving too," says Ma.

What is needed are objects so remote that their motion is not detectable. Only a couple classes of objects fit the bill, because they also need to be bright enough to be seen over incredible distances. Things like quasars, which are typically brighter than a billion suns, can be used. Many scientists believe these objects are powered by giant black holes feeding on nearby gas. Gas trapped in the black hole's powerful gravity is compressed and heated to millions of degrees, giving off intense light and/or radio energy.

Most quasars lurk in the outer reaches of the cosmos, over a billion light years away, and are therefore distant enough to appear stationary to us. For comparison, a light year, the distance light travels in a year, is almost six trillion miles. Our entire galaxy, consisting of hundreds of billions of stars, is about 100,000 light years across.

Fermi Telescope Caps First Year With Glimpse of Space-Time

During its first year of operations, NASA's Fermi Gamma Ray Space Telescope mapped the extreme sky with unprecedented resolution and sensitivity.

It captured more than 1,000 discrete sources of gamma rays -- the highest-energy form of light. Capping these achievements was a measurement that provided rare experimental evidence about the very structure of space and time, unified as space-time in Einstein's theories.

"Physicists would like to replace Einstein's vision of gravity -- as expressed in his relativity theories -- with something that handles all fundamental forces," said Peter Michelson, principal investigator of Fermi's Large Area Telescope, or LAT, at Stanford University in Palo Alto, Calif. "There are many ideas, but few ways to test them."

Many approaches to new theories of gravity picture space-time as having a shifting, frothy structure at physical scales trillions of times smaller than an electron. Some models predict that the foamy aspect of space-time will cause higher-energy gamma rays to move slightly more slowly than photons at lower energy.

Such a model would violate Einstein's edict that all electromagnetic radiation -- radio waves, infrared, visible light, X-rays and gamma rays -- travels through a vacuum at the same speed.

On May 10, 2009, Fermi and other satellites detected a so-called short gamma ray burst, designated GRB 090510. Astronomers think this type of explosion happens when neutron stars collide. Ground-based studies show the event took place in a galaxy 7.3 billion light-years away. Of the many gamma ray photons Fermi's LAT detected from the 2.1-second burst, two possessed energies differing by a million times. Yet after traveling some seven billion years, the pair arrived just nine-tenths of a second apart.

"This measurement eliminates any approach to a new theory of gravity that predicts a strong energy dependent change in the speed of light," Michelson said. "To one part in 100 million billion, these two photons traveled at the same speed. Einstein still rules."

Fermi's secondary instrument, the Gamma ray Burst Monitor, has observed low-energy gamma rays from more than 250 bursts. The LAT observed 12 of these bursts at higher energy, revealing three record setting blasts.

GRB 090510 displayed the fastest observed motions, with ejected matter moving at 99.99995 percent of light speed. The highest energy gamma ray yet seen from a burst -- 33.4 billion electron volts or about 13 billion times the energy of visible light -- came from September's GRB 090902B. Last year's GRB 080916C produced the greatest total energy, equivalent to 9,000 typical supernovae.

Scanning the entire sky every three hours, the LAT is giving Fermi scientists an increasingly detailed look at the extreme universe. "We've discovered more than a thousand persistent gamma ray sources -- five times the number previously known," said project scientist Julie McEnery at NASA's Goddard Space Flight Center in Greenbelt, Md. "And we've associated nearly half of them with objects known at other wavelengths."

Blazars -- distant galaxies whose massive black holes emit fast-moving jets of matter toward us -- are by far the most prevalent source, now numbering more than 500. In our own galaxy, gamma ray sources include 46 pulsars and two binary systems where a neutron star rapidly orbits a hot, young star.

"The Fermi team did a great job commissioning the spacecraft and starting its science observations," said Jon Morse, Astrophysics Division director at NASA Headquarters in Washington. "And now Fermi is more than fulfilling its unique scientific promise for making novel, high-impact discoveries about the extreme universe and the fabric of space-time."‪

NASA Ice Campaign Takes Flight in Antarctica

Early in the 20th century, a succession of adventurers and scientists pioneered the exploration of Antarctica. A century later, they're still at it, albeit with a different set of tools. This fall, a team of modern explorers will fly over Earth's southern ice-covered regions to study changes to its sea ice, ice sheets, and glaciers as part of NASA's Operation Ice Bridge.

Starting next month, NASA will fly its DC-8, a 157-foot-long airborne laboratory that can accommodate many instruments. The fall 2009 campaign is one of few excursions to the remote continent made by the DC-8, the largest aircraft in NASA's airborne science fleet.

The plane is scheduled to leave NASA's Dryden Flight Research Center in Edwards, Calif., on October 12 and fly to Punta Arenas, Chile, where the plane, crew and researchers will be based for through mid-November. For six weeks, the Ice Bridge team will traverse the Southern Ocean for up to 17 flights over West Antarctica, the Antarctic Peninsula, and coastal areas where sea ice is prevalent. Each round-trip flight lasts about 11 hours, two-thirds of that time devoted to getting to and from Antarctica.

Operation Ice Bridge is a six-year campaign of annual flights to each of Earth's polar regions. The first flights in March and April carried researchers over Greenland and the Arctic Ocean. This fall's Antarctic campaign, led by principal investigator Seelye Martin of the University of Washington, will begin the first sustained airborne research effort of its kind over the continent. Data collected by researchers will help scientists bridge the gap between NASA's Ice, Cloud and Land Elevation Satellite (ICESat) -- which is operating the last of its three lasers -- and ICESat-II, scheduled to launch in 2014.

The Ice Bridge flights will help scientists maintain the record of changes to sea ice and ice sheets that have been collected since 2003 by ICESat. The flights will lack the continent-wide coverage that can be achieved by satellite, so researchers carefully select key target locations. But the flights will also turn up new information not possible from orbit, such as the shape of the terrain below the ice.

"Space-based instruments like the ICESat lasers are the only way to find out where change is occurring in remote, continent-sized ice sheets like Antarctica," said Tom Wagner, cryosphere program scientist at NASA Headquarters in Washington, D.C. "But aircraft missions like Ice Bridge allow us to follow up with more detailed studies and make other measurements critical to modeling sea level rise."

STS-128 Outfits Station for New Science

Space shuttle Discovery launched atop brilliant pillars of fire into a midnight sky over NASA’s Kennedy Space Center in Florida on Aug. 28, 2009, to begin a textbook outfitting and supply mission to the International Space Station.

With the Leonardo cargo module bolted tight into the payload bay and astronaut Rick “C.J.” Sturckow in the commander’s seat, Discovery pursued the space station for two days before linking up with the orbiting laboratory.

Pilot Kevin Ford and Mission Specialists Jose Hernandez and Nicole Stott marked their first days in space during STS-128. Along with veteran commander Sturckow, Mission Specialists Patrick Forrester, Danny Olivas and Christer Fuglesang brought a wealth of spaceflight experience to the flight.

The first task of STS-128’s extensive mission manifest wrapped up soon after docking as Stott joined the station’s Expedition 20 crew and station resident Tim Kopra took Stott’s slot on the shuttle.

Crews on the shuttle and station numbered 13 in all and included astronauts from the U.S., Canada, Sweden, and Belgium and cosmonauts from Russia.

Leonardo, one of the multi-purpose logistics modules NASA uses to carry large racks to and from the station, was the star of Discovery’s fourth day in orbit. Ford and Michael Barratt used the robotic arm from the space station to lift the 21-foot-long Leonardo from its cradle inside Discovery and connect it directly to the station, clearing the way for about a week of moving work for the crew members.

Spacewalker Olivas stepped outside the station along with Stott for the first of three spacewalks slated for STS-128. With crew members outfitting the inside of the station, the two spacewalkers set out for some upkeep tasks on the outside. Assisted by the station’s robotic arm, known as Canadarm 2, Olivas and Stott removed an empty ammonia tank from the truss. The station uses ammonia to cool its sophisticated system of equipment. The astronauts also took two experiments off the outside of the European Space Agency’s Columbus laboratory module.

Inside the station, the Colbert treadmill was moved into its new home in space. The treadmill is a new exercise machine that station residents will use to stay fit while in the weightlessness of space. It gained notoriety when NASA named it after Comedy Central comedian and faux newscaster Stephen Colbert following an online NASA poll to name a new station module. The exercise equipment is more advanced than the treadmill already on the station. For example, it allows astronauts to run as fast as an Olympic sprinter. The treadmill is mounted on a system to prevent the vibrations from shaking the station as it floats through space.

The treadmill was far from the only thing moved into the station. Leonardo was loaded with nine racks and eight platforms. The racks are the basic structure for holding space station systems inside the laboratory. Each one is a shell about the size of a refrigerator and is outfitted with connectors that attach to the station on the back and the specialized equipment inside. The hatches from Leonardo to the station are large enough to allow the racks to pass through easily, and even though a full rack can only be moved with a forklift on Earth, a single astronaut can push them around in the microgravity of the station.

The racks are big enough to house a crew quarters or bedroom for a station astronaut, and one of the racks Leonardo carried up became a private room right away for Canadian station resident Robert Thirsk.

Two of the racks were set up for research in space: the Fluids Integrated Rack to study liquid in weightlessness, and the Materials Science Research Rack, which is to conduct experiments on different materials to find new ways to use them. A second freezer for completed experiments also was carried into orbit inside Discovery, along with an air filtration system destined for the Tranquility node, which will be added to the station in 2010.

Olivas led the second spacewalk on the seventh day of the STS-128 mission. He was joined by Sweden’s Fuglesang, another veteran spacewalker. Their work centered on the ammonia tanks. They fastened the old tank inside Discovery so it could be returned to Earth, refilled and launched again on a future mission. The new tank went into place easily for the astronauts.

After getting most of the equipment out of Leonardo, the astronauts on Discovery and the station changed focus a bit to move items into the cargo module. Completed experiments and expired equipment were some of the items to be taken back to Earth.

The mission’s third spacewalk began Sept. 6, again performed by Olivas and Fuglesang. It set up the station for future missions and the Tranquility module. When it finished, Discovery’s spacewalkers had added more than 20 hours to the spacewalk log for space station assembly. Astronauts have completed more than 830 hours of spacewalks to build the space station to this point.

The transfers between the station and Leonardo also wrapped up Sept. 6. Leonardo was repositioned inside Discovery the next day and the crews split up into their shuttle and station contingents before the hatches between the two craft were closed.

Sept. 8 saw Discovery back away from the station, pushed along by springs so the shuttle wouldn’t have to fire its steering jets close to the orbital complex. Minutes later, Ford took the controls to maneuver the shuttle in a circle around the station from about 650 feet away. He then steered the spacecraft away from the station, putting it on a path to move further away as the crew looked ahead to going back to Earth.

That return was delayed by a day, however, after poor weather conditions materialized over the primary landing site at Kennedy. The bad weather stayed over Florida the following day and mission controllers opted to send Sturckow and his team of astronauts to Edwards Air Force Base in California instead.

Sturckow and Ford guided Discovery through Earth’s atmosphere Sept. 11. The spacecraft glided over the Pacific Ocean and soared over Greater Los Angeles on its way to Edwards and its home in the high desert. Discovery’s wheels touched down at 8:53 p.m. EDT and the shuttle rolled to a stop about a minute later to end the flight.

While the astronauts returned to their training base at NASA’s Johnson Space Center in Houston, the mission was just beginning for the team of technicians and specialists who spent the next week getting Discovery set up and mounted on a modified 747 for the ride back to Kennedy. Discovery faced more weather concerns during that flight, too, but a break in the storms allowed the 747 and Discovery to land at Kennedy on Sept. 21.

Climate Simulation Computer Becomes More Powerful

Remember the day you got a brand-new computer? Applications snapped open, processes that once took minutes finished in seconds, and graphics and animation flowed as smoothly as TV video. But several months and many new applications later, the bloom fell off the rose.

Your lightning-fast computer no longer was fast. You needed more memory and faster processors to handle the gigabytes of new files now embedded in your machine.

Climate scientists can relate.

They, too, need more powerful computers to process the sophisticated computer models used in climate forecasts. Such an expanded capability is now being developed at NASA’s Goddard Space Flight Center in Greenbelt, Md.

High-End Computing System Installed

In August, Goddard added 4,128 new-generation Intel "Nehalem" processors to its Discover high-end computing system. The upgraded Discover will serve as the centerpiece of a new climate simulation capability at Goddard. Discover will host NASA’s modeling contributions to the Intergovernmental Panel on Climate Change (IPCC), the leading scientific organization for assessing climate change, and other national and international climate initiatives.

To further enhance Discover’s capabilities, Goddard will install another 4,128 Nehalem processors in the fall, bringing Discover to 15,160 processors.

"We are the first high-end computing site in the United States to install Nehalem processors dedicated to climate research," said Phil Webster, chief of Goddard’s Computational and Information Sciences and Technology Office (CISTO). "This new computing system represents a dramatic step forward in performance for climate simulations."

Well-Suited for Climate Studies

According to CISTO lead architect Dan Duffy, the Nehalem architecture is especially well-suited to climate studies. "Speed is an inherent advantage for solving complex problems, but climate models also require large memory and fast access to memory," he said. Each processor has 3 gigabytes of memory, among the highest available today. In addition, memory access is three to four times faster than Discover’s previous-generation processors.

In preliminary testing of Discover’s Nehalem processors, NASA climate simulations performed up to twice as fast per processor compared with other nationally recognized high-end computing systems. The new computational capabilities also allowed NASA climate scientists to run high-resolution simulations that reproduced atmospheric features not previously seen in their models.

For instance, "features such as well-defined hurricane eyewalls and convective cloud clusters appeared for the first time," said William Putman, acting lead of the Advanced Software Technology Group in Goddard’s Software Integration and Visualization Office. "At these cloud-permitting resolutions, the differences are stunning."

IPCC Simulations

For the IPCC studies, scientists will run both longer-term and shorter-term climate projections using different computer models. A climate model from the Goddard Institute for Space Studies will perform simulations going back a full millennium and forward to 2100. Goddard’s Global Modeling and Assimilation Office will use a climate model for projections of the next 30 years and an atmospheric chemistry-climate model for short-term simulations of chemistry-climate feedbacks. The IPCC will use information from climate simulations such as these in its Fifth Assessment Report, which IPCC expects to publish in 2014.

NASA climate simulation efforts also contribute to the U.S. Global Change Research Program, the U.S. Integrated Earth Observation System, and the U.S. Weather Research Program. Supported international programs include UNESCO’s Intergovernmental Oceanographic Commission, the United Nations Environment Programme, the World Climate Research Programme, the World Meteorological Organization, and the World Weather Research Programme.