Cryogenic Testing Completed for NASA's Webb Telescope Mirrors

Cryogenic testing is complete for the final six primary mirror segments and a secondary mirror that will fly on NASA's James Webb Space Telescope. The milestone represents the successful culmination of a process that took years and broke new ground in manufacturing and testing large mirrors.

"The mirror completion means we can build a large, deployable telescope for space," said Scott Willoughby, vice president and Webb program manager at Northrop Grumman Aerospace Systems. "We have proven real hardware will perform to the requirements of the mission."

The Webb telescope has 21 mirrors, with 18 mirror segments working together as a large 21.3-foot (6.5-meter) primary mirror. Each individual mirror segment now has been successfully tested to operate at 40 Kelvin (-387 Fahrenheit or -233 Celsius).

"Mirrors need to be cold so their own heat does not drown out the very faint infrared images," said Lee Feinberg, NASA Optical Telescope Element manager for the Webb telescope at the agency's Goddard Space Flight Center in Greenbelt, Md. "With the completion of all mirror cryogenic testing, the toughest challenge since the beginning of the program is now completely behind us."

For more info, visit : http://www.nasa.gov/topics/technology/features/webb-mirror-cryo.html

NASA Tests New Smart Card Access to Google Apps

NASA recently began a pilot using Google Apps, a suite of applications that brings services such as Gmail, Google Docs and other products together to help workers in today's business environment. NASA IT Labs, a part of the Office of the Chief Information Officer (CIO), sponsored the pilot to meet the growing demand from workers to access resources on any device.

About 600 IT staff from 11 NASA centers and facilities are participating in the pilot, which offers cost savings by managing user's identities, credentials and access via cloud computing using on-demand software. Cloud computing refers to resources and applications that are available on the Internet from nearly any Internet-connected device. No sensitive NASA data is being placed in the cloud.

Under the pilot, NASA users can connect to Google Apps for Government using an existing NASA work ID, which also functions as a smart card in the card reader of compatible computers. The card was created as a common identification standard for federal employees and contractors to increase security and reduce opportunities for identify fraud.

The pilot complies with the Federal Information Security Management Act of 2002, which is designed to protect the nation's critical information infrastructure. Because no new ID or credential is needed, NASA complies with the law and workers can access secure materials from any smart device.

NASA also accepts and electronically verifies personal identity verification (PIV) credentials issued by other federal agencies through a credential registration process. With this capability, any authorized federal PIV card, which includes the DoD Common Access Card, may be used today for authentication to the Google Apps for Government NASA site.

For more info, visit : http://www.nasa.gov/topics/technology/features/google_apps.html

SOFIA Completes First Flight of German Science Instrument

The Stratospheric Observatory for Infrared Astronomy, or SOFIA, completed its first science flight Wednesday, April 6, using the German Receiver for Astronomy at Terahertz Frequencies (GREAT) scientific instrument. GREAT is a high-resolution far-infrared spectrometer that finely divides and sorts light into component colors for detailed analysis.

SOFIA is the only operational airborne observatory. It is a joint program between NASA and the German Aerospace Center (DLR). The observatory is a heavily modified Boeing 747SP aircraft carrying a reflecting telescope with an effective diameter of 100 inches. Flying at altitudes between 39,000 and 45,000 feet, above the water vapor in Earth's lower atmosphere that blocks most infrared radiation from celestial sources, SOFIA conducts astronomy research not possible with ground-based telescopes.

"SOFIA's onboard crew seamlessly combined scientists, engineers and technicians from the U.S. and Germany, working together on an observatory developed in the U.S., using a telescope and instrument built in Germany, to gather data of great interest to the entire world's scientific community," said Bob Meyer, NASA's SOFIA Program manager at the agency's Dryden Flight Research Center in Edwards, Calif.

GREAT Principal Investigator Rolf Guesten of the Max Planck Institute for Radio Astronomy in Bonn, Germany, and his team conducted observations high above the central and western United States beginning the night of April 5 with their instrument installed on SOFIA's telescope.

Among their targets were IC 342, a spiral galaxy located 11 million light-years from Earth in the constellation Camelopardalis ("The Giraffe"), and the Omega Nebula (known as M17), 5,000 light-years away in Sagittarius. The team captured and analyzed radiation from ionized carbon atoms and carbon monoxide molecules to probe the chemical reactions, motions of matter and flows of energy occurring in interstellar clouds. Astronomers have evidence such clouds in both IC 342 and M17 are forming numerous massive stars.

For more information, visit:
http://www.nasa.gov/centers/dryden/news/NewsReleases/2011/11-10.html

NASA's Kepler Mission Confirms Its First Planet in Habitable Zone of Sun-like Star

NASA's Kepler mission has confirmed its first planet in the "habitable zone," the region where liquid water could exist on a planet’s surface. Kepler also has discovered more than 1,000 new planet candidates, nearly doubling its previously known count. Ten of these candidates are near-Earth-size and orbit in the habitable zone of their host star. Candidates require follow-up observations to verify they are actual planets.

The newly confirmed planet, Kepler-22b, is the smallest yet found to orbit in the middle of the habitable zone of a star similar to our sun. The planet is about 2.4 times the radius of Earth. Scientists don't yet know if Kepler-22b has a predominantly rocky, gaseous or liquid composition, but its discovery is a step closer to finding Earth-like planets.

Previous research hinted at the existence of near-Earth-size planets in habitable zones, but clear confirmation proved elusive. Two other small planets orbiting stars smaller and cooler than our sun recently were confirmed on the very edges of the habitable zone, with orbits more closely resembling those of Venus and Mars.

"This is a major milestone on the road to finding Earth's twin," said Douglas Hudgins, Kepler program scientist at NASA Headquarters in Washington. "Kepler's results continue to demonstrate the importance of NASA's science missions, which aim to answer some of the biggest questions about our place in the universe."

Kepler discovers planets and planet candidates by measuring dips in the brightness of more than 150,000 stars to search for planets that cross in front, or "transit," the stars. Kepler requires at least three transits to verify a signal as a planet.

F-15D Chase Aircraft

Dryden currently flies an F-15D Eagle aircraft for research support and pilot proficiency. The F-15D has a two-seat cockpit and like the 2 seat Support Aircraft F-18, it is normally used for photo or video chase. It will be transmitting live video from the air back to Dryden so engineers can visually monitor the mission as it is being flown. This feature greatly enhances flight safety.

NASA research support aircraft are commonly called chase planes and fill the role of escort aircraft during research missions. Chase pilots are in constant radio contact with research pilots and serve as an "extra set of eyes" to help maintain total flight safety during specific tests and maneuvers. They monitor certain events for the research pilot and are an important safety feature on all research missions.

Chase aircraft also are used as camera platforms for research missions that must be photographed or videotaped. Aeronautical engineers use this pictorial coverage (photos, motion pictures, and videotape) extensively to monitor and verify various aspects of research projects.

NASA Quiet Sonic Boom Research Effort Ends With a Whisper

NASA's Dryden Flight Research Center recently completed NASA’s latest quiet sonic boom research study at Edwards Air Force Base.

The Waveforms and Sonic boom Perception and Response, or WSPR, project gathered data from a select group of more than 100 volunteer Edwards Air Force Base residents on their individual attitudes toward sonic booms produced by aircraft in supersonic flight over Edwards.

NASA and industry are studying technology that will reduce the noise and annoyance associated with sonic booms to the point where aircraft flying over populated areas at supersonic speeds do not disturb the peace, and aviation and governmental authorities may consider lifting prohibitions. But before the current restrictions on supersonic flight over land can be changed, much research is needed to understand how individuals and communities react to low-noise sonic booms.

WSPR's primary purpose is to develop data collection methods and test protocols for future public perception studies in communities that do not usually experience sonic booms. The base's unique flight-test airspace puts Edwards residents in a position to experience loud booms regularly, so their reactions to low-noise booms will be a valuable guide for future work in sonic boom perception and response.

For more info, read:
http://www.nasa.gov/centers/dryden/Features/WSPR_research_complete.html

NASA Launches Most Capable and Robust Rover to Mars

NASA began a historic voyage to Mars with the Nov. 26 launch of the Mars Science Laboratory, which carries a car-sized rover named Curiosity. Liftoff from Cape Canaveral Air Force Station aboard an Atlas V rocket occurred at 10:02 a.m. EST (7:02 a.m. PST).

"We are very excited about sending the world's most advanced scientific laboratory to Mars," NASA Administrator Charles Bolden said. "MSL will tell us critical things we need to know about Mars, and while it advances science, we'll be working on the capabilities for a human mission to the Red Planet and to other destinations where we've never been."

The mission will pioneer precision landing technology and a sky-crane touchdown to place Curiosity near the foot of a mountain inside Gale Crater on Aug. 6, 2012. During a nearly two-year prime mission after landing, the rover will investigate whether the region has ever offered conditions favorable for microbial life, including the chemical ingredients for life.

"The launch vehicle has given us a great injection into our trajectory, and we're on our way to Mars," said Mars Science Laboratory Project Manager Peter Theisinger of NASA's Jet Propulsion Laboratory in Pasadena, Calif. "The spacecraft is in communication, thermally stable and power positive."

The Atlas V initially lofted the spacecraft into Earth orbit and then, with a second burst from the vehicle's upper stage, pushed it out of Earth orbit into a 352-million-mile (567-million-kilometer) journey to Mars.

"Our first trajectory correction maneuver will be in about two weeks," Theisinger said. "We'll do instrument checkouts in the next several weeks and continue with thorough preparations for the landing on Mars and operations on the surface."

For more info, read http://www.nasa.gov/mission_pages/msl/news/msl20111126.html

Mars Science Laboratory En Route to Mars

NASA's Mars Science Laboratory (MSL) spacecraft - which includes the newest Red Planet rover, the car-sized Curiosity - began its mission with an on-time launch aboard a United Launch Alliance Atlas V rocket Nov. 26, 2011 at 10:02 a.m. EST.

The Atlas V lifted off with MSL on the first opportunity, rising from Space Launch Complex 41 on Cape Canaveral Air Force Station in Florida following a smooth countdown throughout the morning. Although clouds occasionally drifted through the launch area during fueling operations, conditions were favorable at launch time, as forecasters had predicted.

MSL separated from the Centaur upper stage about 44 minutes into the mission and sent a signal to officials on the ground six minutes later. The spacecraft is in excellent health as it begins its journey to Mars.

All Systems Go For Next Communication Spacecraft

The most recent evaluations of NASA’s Tracking and Data Relay Satellite (TDRS) project confirmed all systems go for a third generation upgrade of the orbiting communications network. TDRS-K is scheduled for launch aboard an Atlas V rocket from Cape Canaveral, Florida in the fall of 2012.

Approval to move forward came during a recent Agency Project Management Council (APMC) meeting at NASA Headquarters. "I am very proud of the entire TDRS civil servant and contractor team for successfully completing this milestone and demonstrating that the TDRS project is ready to proceed into the integration phase,” said Jeff Gramling, TDRS Project Manager. “I am excited to see the TDRS-K satellite enter the thermal vacuum chamber and begin environmental testing." Testing will occur within the Boeing Space Systems Facility in El Segundo, California.

APMC approval allows the project to enter Phase D that will include spacecraft integration and testing. During this phase the spacecraft reflectors will be mounted, the thermal panels and batteries will be installed before the spacecraft will have to endure the rigors of the vibration and acoustic testing. Finally, the spacecraft must pass a pre-ship review prior to being transported to Florida for launch.
For more info, visit:http://www.nasa.gov/topics/technology/features/tdrs-go.html

Nasa Technology Innovation

NASA seeks to create partnerships and cooperative activities with U.S. enterprises to develop technology that is applicable to NASA's mission technology needs and contributes to commercial competitiveness in global markets. Technology Innovation provides information about NASA's technology needs and opportunities, as well as interesting facts and feature articles about our successes.

For more info, read
http://www.nasa.gov/offices/oct/communications/products/product_innovation.html

MSL Entry, Descent and Landing Instrumentation (MEDLI)

NASA's Mars Science Laboratory, which is set to launch Nov. 25, is expected to improve not only our knowledge of Mars, but also the science of hypersonic flight - more than five times the speed of sound - within an out-of-this-world atmosphere. That's something of great interest to NASA researchers who study flight through all atmospheres so they can help design better air and spacecraft.

The Mars Science Laboratory (MSL) Curiosity rover is protected by an encapsulating aeroshell made up of a heat shield and back shell. Embedded in the MSL heat shield is a set of sensors designed to record the heat and atmospheric pressure experienced during the spacecraft's high-speed, extremely hot entry into the Martian atmosphere. The sensor suite is called MEDLI, which stands for MSL Entry, Descent and Landing Instrumentation.

"This is the first time we've ever had sensors that will collect accurate, high fidelity data of atmospheric entry at another planet," said Jim Pittman, head of the Hypersonics Project, which is part of the Fundamental Aeronautics Program in NASA's Aeronautics Research Mission Directorate (ARMD). "Having that knowledge is of great interest to the hypersonics community - especially when it comes to being able to design future Mars entry systems that are safer, more reliable and lighter weight."

NASA's ARMD is one of the sponsors of the $28 million MEDLI system research, development and data analysis. It also has support from NASA's Science and Human Exploration and Operations Mission Directorates, and is the first Technology Demonstration Mission from NASA's Space Technology Program to go into space.

For more info, visit http://www.nasa.gov/mission_pages/msl/news/msl-medli.html

NASA Develops New Game-Changing Technology

Two NASA California centers have been selected to develop new space-aged technologies that could be game-changers in the way we look at planets from above and how we safely transport robots or humans through space and bring them safely back to Earth.

NASA's Jet Propulsion Laboratory in Pasadena, Calif., will use advanced compound semiconductor materials to develop new technologies for the High Operating Temperature Infrared Sensor Demonstration. The higher the temperature at which an infrared detector can operate, the less power is required to cool it. Reduced power needs can translate into operational cost and system weight savings. If successful, this sensor technology could be used in many future NASA Earth and planetary science instruments, as well as for U.S. commercial and defense applications.

"The technology demonstration effort is different in the fact that we're focused on affordability concurrently with performance," said Sarath Gunapala of JPL, who is project manager for the High Operating Temperature Infrared Sensor Demonstration. "This technology has excellent potential for transitioning from laboratory demonstration to NASA and commercial product lines."

The overall goal for this technology development effort is to achieve 100 percent cost savings as compared with traditional cryogenically cooled infrared sensors. The weight and volume savings allow for more compact instruments -- an important consideration for a spacecraft's payload size and cost. This state-of-the-art technology also will have spinoff applications for commercial instrument manufacturers.

Seeking to radically change the way heat shields protect spacecraft during atmospheric entry, NASA's Ames Research Center at Moffett Field, Calif., is developing the Woven Thermal Protection System. The project is a revolutionary approach to thermal protection system design and manufacturing for extreme environments. Ames is the lead center for the project, partnering with NASA's Langley Research Center in Hampton, Va.

Partnering with the U.S. textile industry, NASA is employing an advanced, three-dimensional weaving approach in the design and manufacture of thermal protection systems. Today, lightweight aircraft parts are being manufactured using similar weaving technologies. This will be expanded to include spacecraft heatshield applications. The system will enhance performance using advanced design tools with cost savings from a shortened product development and testing cycle.

NASA Announces 2011 NASA OPTIMUS PRIME Spinoff Video Contest

NASA is kicking off its second annual NASA OPTIMUS PRIME Spinoff Video Contest to raise student awareness of how NASA technologies provide benefits to the public. Registration for the contest is open until January 3, 2012.

The NASA OPTIMUS PRIME Spinoff Video Contest emphasizes the similarities between the popular OPTIMUS PRIME character from Hasbro's TRANSFORMERS brand and NASA technologies now being used back on Earth.

Last year’s contest brought video submissions from over 190 students in grades 3–8, from 31 states, describing their favorite story from NASA's 2009 Spinoff publication. This year’s contest will feature stories from NASA's 2010 Spinoff publication and will be expanded to allow students in grades 9–12 to participate.

"The level of skill, effort and comprehension demonstrated by last year’s contestants was truly amazing," said Nona Cheeks, head of the Goddard Space Flight Center's Innovative Partnerships Office, which administers the contest for the Agency. "However, this year we are opening the contest up to include high school students, and we fully expect the videos sent in by that group to take the contest to a whole new level." Additional changes for the 2011 contest include transitioning the awards ceremony to the Kennedy Space Center in Florida and some exciting new prizes to be announced in December.

NASA-Sponsored Robotics Teams Gear Up for 2012

The CalGames robot contests have begun! NASA Ames Research Center, Moffett Field, Calif. is supporting two competitive high school robotics teams: Space Cookies Team 1868, and Cheesy Poofs Teams 252 and 254. All three teams recently won top ranking positions in the CalGames Western Region Robotics Forum (Wrrf) At Archbishop Mitty High School, San Jose, Calif.

Each year, FIRST, or For Inspiration and Recognition of Science and Technology, challenges high school students to design, build, test and compete robots that can outperform their opponents. To help students compete, regional competitions are held to hone their skills for the national FIRST Robotics Competition (FRC) that starts this year in January. In addition, NASA engineers and scientists are encouraged to share their expertise and experiences by mentoring teams in an engineering laboratory with machinery and tools at NASA Ames.

“We couldn’t be more proud of our teams and their commitment to ‘rise to the challenge’ and produce outstanding software and technology, building and operating robots each year,” said Mark Leon, manager of NASA Robotics Alliance Project at NASA Ames.

No matter which is the favorite robot at these competitions, the stands generally are filled full of cheering fans watching 120-pound robots swivel, scoop and travel speeds up to nearly 20 feet per second to score a point. The outcome of the multiple two- minute-15-second matches is dependent upon both robot and human performances.

For more info, visit: http://www.nasa.gov/topics/technology/features/FIRST_2012.html

Canadian Robot Repairs Components on the Space Station

Dextre, the Canadian Space Agency’s robotic handyman aboard the International Space Station (ISS), has successfully replaced a faulty circuit-breaker box on the orbiting lab. The robot swapped the failed component for a fresh one, thereby restoring part of the orbiting lab’s backup electrical systems. The maneuver marks the first time Dextre replaces defective equipment on the Station.

"This week's successful replacement of an electrical circuit breaker on the space station's truss is an important operational milestone," said Lead Expedition 28 Flight Director, Ed Van Cise. "In the past, we've only had the option of sending humans outside the station on a spacewalk to perform such repairs.

Having a dexterous robot outside the station capable of doing this while controlled from the ground is a big advance in capability that will free up crew time for important research inside the station. Our Flight Control Teams in Houston and in Canada have outdone themselves, and we're looking forward to stretching Dextre's arms on other tasks that will continue to help pave the way for future exploration."

Known by the technical term “Remote Power Control Modules,” (RPCMs) circuit-breaker boxes control the flow of electricity through the ISS’s secondary power distribution system, and tend to fail occasionally. Up to now, exchanging the boxes was done by spacewalkers, which always carries a certain level of risk. Dextre was designed to reduce the need for astronauts to conduct spacewalks for routine maintenance, therefore freeing up the crew’s time for more important activities, like conducting science.

Canadarm2 supported Dextre during the entire operation, which took place on August 28-29. Dextre was operated from the ground by robotics flight controllers at NASA’s Johnson Space Center in Houston, Texas, and supported by several teams of engineers both in Houston and at the Canadian Space Agency’s headquarters in Saint-Hubert, Quebec.

Atlantis’ Final Mission Included: Kennedy-Developed Plant Experiment

Atlantis carried many science and research experiments in its middeck during NASA’s last shuttle flight, STS-135, in July. Among these was a plant experiment developed at Kennedy Space Center’s Space Life Sciences Laboratory (SLSL) that could have an impact on long duration missions to the moon or Mars.

Principal Investigators Dr. Gary Stutte and Dr. Michael Roberts with QinetiQ NA, and NASA Project Scientist Dr. Howard Levine created the Biological Research in Canisters-Symbiotic Nodulation in a Reduced Gravity Environment (BRIC-SyNRGE). A first of its kind to fly on a space shuttle, the purpose of the experiment was to study the symbiotic relationship between plants similar to alfalfa, which is in the legume family, and specific nitrogen-reacting bacteria in microgravity.

"It’s a distinct honor to have had an experiment onboard Atlantis, the final space shuttle mission, and I am indebted to everyone who worked so hard to make it possible to be a part of this historic mission," Stutte said.

About four hours after Atlantis landed at Kennedy’s Shuttle Landing Facility, the BRIC-SyNRGE experiment was retrieved and returned to the SLS Laboratory. Stutte said that initial reviews show that there was 100 percent germination of the plant seeds and excellent growth was observed.

The alfalfa-like plant, Medicago truncatula, was grown in a plant chamber at the SLSL. The day before Atlantis’ launch, several laboratory rooms were abuzz with activity. In one lab, samples were carefully harvested and inserted into Petri dish units. In another lab, technicians added the nitrogen-fixing bacteria and a liquid preservative to the dishes.

Green Flight Challenge Competition

At the CAFE Green Flight Challenge, sponsored by Google, the competing electric aircraft are completing battery recharging today in preparation for their speed challenge tomorrow. Many of the team members are away from the CAFE campus, doing some sightseeing and catching up on other business. Everything is much more relaxed today here in Santa Rosa, Calif., at the site of this NASA Centennial Challenges event.

CAFE has more than 80 volunteers helping out with the competition. They can be seen around the campus, wearing Green Flight Challenge shirts. They've been quite the local heroes.

The daily briefing was at 11 a.m. EDT. A big concern for tomorrow's challenge is the weather, which looks to be a bit questionable when the speed test is planned, so CAFE wants to get the planes off as soon as they can tomorrow morning. A suggestion was made to have the pilots' briefing at 10:30 a.m. EDT in order to expedite the planes taking off.

Safety and security measures were reviewed and particular emphasis was placed on the no-smoking requirement. (This is fire season in California and the area is quite dry and a fire would be a bad thing to deal with.)

Everyone was also cautioned about the poisonous black widow and brown recluse spiders in the area - adding another note of excitement as the next competition nears.

SLS task schedule improving – Crewed Moon task moving to 2019

Nasa - Only one long term visible for the SLS had been listed in recent months, showing the debut of the Heavy Lift Launch Vehicle (HLV) in 2017 – an unmanned task around the moon – prior to a four year gap until the crewed version was to be launched.

That visible showed that it would take until SLS-13 for the debut of the fully evolved 130mt version of the SLS, planned for 2032.

The schedule was rightly criticized. However, it was always characterize as a worst case scenario manifest – not least because the full mission outline for the SLS launches was yet to be formed. This work is currently ongoing under the leadership of former Space Shuttle Program (SSP) manager John Shannon.


The expected realization of an improved manifest is now starting to be satisfied, just weeks after the SLS was officially announced, in turn allowing for a full test plan effort to be worked.

SLS-1, a 70mt version of the SLS, is still expected to debut in 2017, with a “crew capable” Orion (Multi-Purpose Crew Vehicle) being sent on a test trip around the Moon. The 2021 debut of SLS/Orion for the crewed version of this mission is now being pressed to the left by two years, with a launch date of 2019.

The news came via notes linked with a meeting between SLS and Orion managers, which discussed the future Planning, Programming, Budgeting and Execution (PPBE) process, in turn providing “high level guidance” to schedule planning.

“MOD (Mission Operations Directorate) is to prepare bottoms up budget for a 2017 un-crewed circum lunar mission. MPCV (Orion) wants that vehicle to be crew capable. In addition MPCV wants to pull the planned 2021 manned mission to the left to 2019,” added the notes on L2, dated September 26. “MOD is also to prepare a budget for a 2019 crewed High Lunar Orbit mission.”

This realigned schedule effort slips the Orion Flight Test (OFT-1) – involving the MPCV being sent on a multi-orbit mission around the Earth via a Delta IV-H – to December, 2013. This slip of around six months had been likely for some time, and the test may yet slip into 2014.

The AA2 test – which involves an unmanned ascent abort test of Orion at MaxQ velocities – will follow the OFT-1 mission, although no date has yet been scheduled.

“The (new) schedule is OFT-1, Dec 2013. AA2 following that mission, then the 2017 and 2019 flight. direction from (managers) will be forth coming, as there is open work on procedure, displays, training, etc to support the purposed schedule.”

Unlike the Constellation Program (CxP) – which appeared to start with an indefensible schedule, prior to almost yearly slips being noted during Program Milestone Reviews (PMRs) – sources note that all SLS mission schedules are being worked with large amounts of margin.

It has been noted that the crewed mission around the moon may even be higher to 2018, one year after the debut SLS-1 launch, should funding projections remain stable over the coming years. Even with the two year advance to SLS-2, the downstream manifest is predictable to improve to the point the evolved SLS may be ready “many years” ahead of the earlier schedule.

Airplane add Heat add Ice Equals Mystery

It's difficult to believe that an airplane flying in the tropics in the summer could have an engine fill up with ice, freeze, and shut down. But the phenomenon, known as engine core ice accretion, has happened more than 150 times since 1988 — frequently enough to attract the attention of NASA aviation safety experts, who are preparing a flight campaign in northern Australia to learn more about this occasional hazard and what can be done to prevent it.

"It's not happening in one particular type of engine and it's not happening on one particular type of airframe," said Tom Ratvasky, an icing flight research engineer at NASA's Glenn Research Center in Cleveland. "The problem can be found on aircraft as big as large commercial airliners, all the way down to business-sized jet aircraft." And it has happened at altitudes up to 41,000 feet.

No accident has been attributed to the phenomenon in the 23 years since it was identified, but there have been some harrowing moments in the air. In most of the known cases, pilots have managed to restore engine power and reach their destinations without further problems. According to the Federal Aviation Administration, there have been two forced landings. For example, in 2005, both engines of a Beechcraft business jet failed at 38,000 feet above Jacksonville, Fla. The pilot glided the aircraft to an airport, dodging thunderstorms and ominous clouds on the way down. Engine core ice accretion was to blame.

Little is understood about ice crystal properties at high altitude and how ice accumulates inside engines. The engines may be toasty warm inside at such heights, but the air outside is frosty cold. The prevailing theory holds the trouble occurs around tropical storms in which strong convection currents move moist air from low altitudes to high altitudes where the local temperatures are very cold, creating high concentrations of ice crystals. But the properties of the ice crystals, such as their size and how many of them are in a given volume of air, are a mystery — one that an international research team led by NASA aims to solve.

Researchers point how a Distant Black Hole overcome a Star

Two studies appearing in the Aug. 25 issue of the journal Nature provide new insights into a cosmic accident that has been streaming X-rays toward Earth since late March. NASA's Swift satellite first alerted astronomers to intense and unusual high-energy flares from the new source in the constellation Draco.

"Incredibly, this source is still producing X-rays and may remain bright enough for Swift to observe into next year," said David Burrows, professor of astronomy at Penn State University and lead scientist for the mission's X-Ray Telescope instrument. "It behaves unlike anything we've seen before."

Astronomers soon realized the source, known as Swift J1644+57, was the result of a truly extraordinary event -- the awakening of a distant galaxy's dormant black hole as it shredded and consumed a star. The galaxy is so far away, it took the light from the event approximately 3.9 billion years to reach Earth.

Burrows' study included NASA scientists. It highlights the X- and gamma-ray observations from Swift and other detectors, including the Japan-led Monitor of All-sky X-ray Image (MAXI) instrument aboard the International Space Station.

The second study was led by Ashley Zauderer, a post-doctoral fellow at the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass. It examines the unprecedented outburst through observations from numerous ground-based radio observatories, including the National Radio Astronomy Observatory's Expanded Very Large Array (EVLA) near Socorro, N.M.

Most galaxies, including our own, possess a central supersized black hole weighing millions of times the sun's mass. According to the new studies, the black hole in the galaxy hosting Swift J1644+57 may be twice the mass of the four-million-solar-mass black hole in the center of the Milky Way galaxy. As a star falls toward a black hole, it is ripped apart by intense tides. The gas is corralled into a disk that swirls around the black hole and becomes rapidly heated to temperatures of millions of degrees.

The innermost gas in the disk spirals toward the black hole, where rapid motion and magnetism create dual, oppositely directed "funnels" through which some particles may escape. Jets driving matter at velocities greater than 90 percent the speed of light form along the black hole's spin axis. In the case of Swift J1644+57, one of these jets happened to point straight at Earth.

"The radio emission occurs when the outgoing jet slams into the interstellar environment," Zauderer explained. "By contrast, the X-rays arise much closer to the black hole, likely near the base of the jet."

NASA's WISE Mission Finds First Trojan Asteroid Sharing Earth's Orbit

Astronomers studying observations taken by NASA's Wide-field Infrared Survey Explorer (WISE) mission have discovered the first known "Trojan" asteroid orbiting the sun along with Earth.

Trojans are asteroids that share an orbit with a planet near stable points in front of or behind the planet. Because they constantly lead or follow in the same orbit as the planet, they never can collide with it. In our solar system, Trojans also share orbits with Neptune, Mars and Jupiter. Two of Saturn's moons share orbits with Trojans.

Scientists had predicted Earth should have Trojans, but they have been difficult to find because they are relatively small and appear near the sun from Earth's point of view.

"These asteroids dwell mostly in the daylight, making them very hard to see," said Martin Connors of Athabasca University in Canada, lead author of a new paper on the discovery in the July 28 issue of the journal Nature. "But we finally found one, because the object has an unusual orbit that takes it farther away from the sun than what is typical for Trojans. WISE was a game-changer, giving us a point of view difficult to have at Earth's surface."

The WISE telescope scanned the entire sky in infrared light from January 2010 to February 2011. Connors and his team began their search for an Earth Trojan using data from NEOWISE, an addition to the WISE mission that focused in part on near-Earth objects, or NEOs, such as asteroids and comets. NEOs are bodies that pass within 28 million miles (45 million kilometers) of Earth's path around the sun. The NEOWISE project observed more than 155,000 asteroids in the main belt between Mars and Jupiter, and more than 500 NEOs, discovering 132 that were previously unknown.

The team's hunt resulted in two Trojan candidates. One called 2010 TK7 was confirmed as an Earth Trojan after follow-up observations with the Canada-France-Hawaii Telescope on Mauna Kea in Hawaii.

What's Next For NASA?

"As a former astronaut and the current NASA Administrator, I'm here to tell you that American leadership in space will continue for at least the next half-century because we have laid the foundation for success -- and failure is not an option." Charles Bolden, NASA Administrator

Exploration
NASA is designing and building the capabilities to send humans to explore the solar system, working toward a goal of landing humans on Mars. We will build the Multi-Purpose Crew Vehicle, based on the design for the Orion capsule, with a capacity to take four astronauts on 21-day missions.

We will soon announce the design for the heavy-lift Space Launch System that will carry us out of low Earth orbit. We are developing the technologies we will need for human exploration of the solar system, including solar electric propulsion, refueling depots in orbit, radiation protection and high-reliability life support systems.
International Space Station
The International Space Station is the centerpiece of our human spaceflight activities in low Earth orbit. The ISS is fully staffed with a crew of six, and American astronauts will continue to live and work there in space 24 hours a day, 365 days a year. Part of the U.S. portion of the station has been designated as a national laboratory, and NASA is committed to using this unique resource for scientific research.

The ISS is a test bed for exploration technologies such as autonomous refueling of spacecraft, advanced life support systems and human/robotic interfaces. Commercial companies are well on their way to providing cargo and crew flights to the ISS, allowing NASA to focus its attention on the next steps into our solar system.

Aeronautics
NASA is researching ways to design and build aircraft that are safer, more fuel-efficient, quieter, and environmentally responsible. We are also working to create traffic management systems that are safer, more efficient and more flexible. We are developing technologies that improve routing during flights and enable aircraft to climb to and descend from their cruising altitude without interruption.

We believe it is possible to build an aircraft that uses less fuel, gives off fewer emissions, and is quieter, and we are working on the technologies to create that aircraft. NASA is also part of the government team that is working to develop the Next Generation Air Transportation System, or NextGen, to be in place by the year 2025. We will continue to validate new, complex aircraft and air traffic control systems to ensure that they meet extremely high safety levels.

Science
NASA is conducting an unprecedented array of missions that will seek new knowledge and understanding of Earth, the solar system and the universe. On July 16, the Dawn spacecraft begins a year-long visit to the large asteroid Vesta to help us understand the earliest chapter of our solar system's history. In August, the Juno spacecraft will launch to investigate Jupiter's origins, structure, and atmosphere. The September launch of the National Polar-orbiting Operational Environmental Satellite System Preparatory Project is a critical first step in building a next-generation Earth-monitoring satellite system.

NASA returns to the moon to study the moon's gravity field and determine the structure of the lunar interior with the October launch of GRAIL. In November, we launch the Mars Science Laboratory named Curiosity on its journey to Mars to look for evidence of microbial life on the red planet. And in February 2012, we will launch the Nuclear Spectroscopic Telescope Array to search for black holes, map supernova explosions, and study the most extreme active galaxies.

Ultraviolet Spotlight on Plump Stars in Tiny Galaxies

Astronomers using NASA's Galaxy Evolution Explorer may be closer to knowing why some of the most massive stellar explosions ever observed occur in the tiniest of galaxies.

"It's like finding a sumo wrestler in a little 'Smart Car,'" said Don Neill, a member of NASA's Galaxy Evolution Explorer team at the California Institute of Technology in Pasadena, and lead author of a new study published in the Astrophysical Journal.

"The most powerful explosions of massive stars are happening in extremely low-mass galaxies. New data are revealing that the stars that start out massive in these little galaxies stay massive until they explode, while in larger galaxies they are whittled away as they age, and are less massive when they explode," said Neill.

Over the past few years, astronomers using data from the Palomar Transient Factory, a sky survey based at the ground-based Palomar Observatory near San Diego, have discovered a surprising number of exceptionally bright stellar explosions in so-called dwarf galaxies up to 1,000 times smaller than our Milky Way galaxy. Stellar explosions, called supernovae, occur when massive stars -- some up to 100 times the mass of our sun -- end their lives.

The Palomar observations may explain a mystery first pointed out by Neil deGrasse Tyson and John Scalo when they were at the University of Austin Texas (Tyson is now the director of the Hayden Planetarium in New York, N.Y.). They noted that supernovae were occurring where there seemed to be no galaxies at all, and they even proposed that dwarf galaxies were the culprits, as the Palomar data now indicate.

Now, astronomers are using ultraviolet data from the Galaxy Evolution Explorer to further examine the dwarf galaxies. Newly formed stars tend to radiate copious amounts of ultraviolet light, so the Galaxy Evolution Explorer, which has scanned much of the sky in ultraviolet light, is the ideal tool for measuring the rate of star birth in galaxies.

The results show that the little galaxies are low in mass, as suspected, and have low rates of star formation. In other words, the petite galaxies are not producing that many huge stars.

"Even in these little galaxies where the explosions are happening, the big guys are rare," said co-author Michael Rich of UCLA, who is a member of the mission team.

In addition, the new study helps explain why massive stars in little galaxies undergo even more powerful explosions than stars of a similar heft in larger galaxies like our Milky Way. The reason is that low-mass galaxies tend to have fewer heavy atoms, such as carbon and oxygen, than their larger counterparts. These small galaxies are younger, and thus their stars have had less time to enrich the environment with heavy atoms.

Every Day is Earth Day at NASA

Earth Day, April 22, is the annual celebration of the environment and a time to assess the work still needed to protect the natural gifts of our planet. It affirms that environmental awareness is part of our consciousness and that the idea of protecting the environment has moved into the mainstream.

NASA's Earth Science Mission seeks to understand Earth's systems and their responses to natural and anthropogenic (human-made) changes. A fleet of satellites in NASA's Earth Observing System gives scientists the global, long-term measurements they need to connect the atmosphere (air), lithosphere (land), hydrosphere (water), cryosphere (snow/ice), and biosphere (life) as a single system.

NASA works with many other partners from government, industry, academia, and international space agencies on the 17 satellite missions that make up the EOS series. Each of these satellites gathers a unique set of measurements for studying Earth. These measurements are used to improve weather forecasts, understand natural disasters, manage agriculture and forests, and predict how climate will change.

Geomagnetic wind in evolution

A G1-class geomagnetic storm is in progress, flashed by a high-speed solar wind river which is buffeting Earth's magnetic field. Lofty latitude sky watchers should be attentive for auroras.

What is a geomagnetic wind?

The Earth's magnetosphere is created by our attractive field and protects us from most of the particles the sun emits. When a CME or high-speed stream arrives at Earth it buffets the magnetosphere. If the new solar magnetic field is directed southward it interacts strongly with the oppositely leaning magnetic field of the Earth. The Earth's magnetic field is then peeled open like an onion allowing energetic solar wind particles to stream down the field lines to hit the atmosphere over the poles. At the Earth's surface a magnetic storm is seen as a fast drop in the Earth's magnetic ground strength. This decrease lasts about 6 to 12 hours, after which the attractive field gradually recovers over a period of several days.

What's causing the poles to warm faster than the rest of Earth?

The poles are warming faster than other parts of the Earth – a fact that has been widely accepted for years. But what is causing the accelerated warming?

Research aimed at answering that question has been done before, but a recent study by Patrick Taylor, a scientist at NASA's Langley Research Center in Hampton, Va., suggests a new reason.

Taylor's research shows the Earth's poles are warming faster than the rest of the planet because of energy in the atmosphere that is carried to the poles through large weather systems.


Decades of NASA data show the Earth is warming. According to NASA's Goddard Institute for Space Studies in Manhattan, the Earth has warmed about 1.44 degrees Fahrenheit during the last 40 years. But the poles are warming even faster; the Arctic has warmed by more than 3.5 degrees Fahrenheit during the same time period.

"It was previously thought that amplified polar warming was caused by melting ice, lowering surface albedo," Taylor said.

Albedo is the amount of sun’s energy that is reflected off the Earth’s surface and back into space, rather than absorbed. The more reflective the surface – such as ice – the more energy is reflected and the cooler the temperature. When ice melts, less energy is reflected and temperature increases.

"Surface albedo at the poles, however, is lowest in the summer, which is when we see the weakest temperature response. More recent research suggests that other atmospheric processes are at work," Taylor said.

For this study, Taylor used Clouds and the Earth's Radiant Energy System (CERES) satellite data, and a climate model that assumes carbon emissions will be reduced slightly below "business as usual."

His results suggest that summertime changes in clouds reflect a lot of the sun's energy, offsetting the low surface albedo, and that it must be something else that determines the amount of warming.

"The total warming at the poles is due to changes in clouds, water vapor, surface albedo and atmospheric temperature," he said. "But there is greater warming in the winter than in the summer and that is caused by energy transport," he said.

Taylor's research shows that the seasonality of the polar warming is largely a result of energy in the atmosphere that is being transported to the poles through large weather systems.

The importance of energy transport in the warming of the poles suggests more study is needed on the interactions between large weather systems and more local changes, involving clouds, water vapor, surface albedo and atmospheric temperature, in order to better understand climate sensitivity.

"We hope to learn more about the processes involved in atmospheric processes in order to better understand what climate models are telling us," Taylor said.

Pretty in Pink

Inside the Plasma Spray-Physical Vapor Deposition, or PS-PVD, ceramic powder is introduced into the plasma flame, which vaporizes it and then condenses it to form the ceramic coating.

The PS-PVD rig at NASA's Glenn Research Center uses new technology to create super thin ceramic coatings, which are being developed to protect high efficiency engines. The coatings created in the PS-PVD rig are thinner and more complex than those previously available.

The PS-PVD rig uses a system of vacuum pumps and a blower to remove air from the chamber, reducing the pressure inside to fraction of normal atmospheric pressure. The plasma flame is extremely hot and reaches 10,000 degrees Celsius. Ceramic powder is introduced from the torch into the plasma flame. The plasma vaporizes the ceramic powder, which then condenses 5 feet away from the torch onto the component to form the ceramic coating.

Plasma--not a gas, liquid or solid--is the fourth state of matter and often behaves like a gas, except that it conducts electricity and is affected by magnetic fields. On an astronomical scale, plasma is common. The sun is composed of plasma, fire is plasma, fluorescent and neon lights contain plasma. NASA’s PS-PVD rig is one of only two such facilities in the country and one of four in the world.

NASA Stardust Spacecraft Officially Ends Operations

NASA's Stardust spacecraft sent its last transmission to Earth at 4:33 p.m. PDT (7:33 p.m. EDT) Thursday, March 24, shortly after depleting fuel and ceasing operations. During a 12-year period, the venerable spacecraft collected and returned comet material to Earth and was reused after the end of its prime mission in 2006 to observe and study another comet during February 2011.

The Stardust team performed the burn to depletion because the comet hunter was literally running on fumes. The depletion maneuver command was sent from the Stardust-NExT mission control area at Lockheed Martin Space Systems in Denver. The operation was designed to fire Stardust's rockets until no fuel remained in the tank or fuel lines. The spacecraft sent acknowledgment of its last command from approximately 312 million kilometers (194 million miles) away in space.



"This is the end of the spacecraft's operations, but really just the beginnings of what this spacecraft's accomplishments will give to planetary science," said Lindley Johnson, Stardust-NExT and Discovery program executive at NASA Headquarters in Washington. "The treasure-trove of science data and engineering information collected and returned by Stardust is invaluable for planning future deep space planetary missions."

After completion of the burn, mission personnel began comparing the computed amount of fuel consumed during the engine firing with the anticipated amount based on consumption models. The models are required to track fuel levels, because there are no fully reliable fuel gauges for spacecraft in the weightless environment of space. Mission planners use approximate fuel usage by reviewing the history of the vehicle's flight, how many times and how long its rocket motors fired.

"Stardust's motors burned for 146 seconds," said Allan Cheuvront, Lockheed Martin Space Systems Company program manager for Stardust-NExT in Denver. "We'll crunch the numbers and see how close the reality matches up with our projections. That will be a great data set to have in our back pocket when we plan for future missions."

Cassini Finds Saturn Sends Mixed Signals

Recent data from NASA's Cassini spacecraft show that the variation in radio waves controlled by the planet's rotation is different in the northern and southern hemispheres. Moreover, the northern and southern rotational variations also appear to change with the Saturnian seasons, and the hemispheres have actually swapped rates. These two radio waves, converted to the human audio range, can be heard in a new video available online at: http://www.nasa.gov/multimedia/videogallery/index.html?media_id=74390781

"These data just go to show how weird Saturn is," said Don Gurnett, Cassini's radio and plasma wave science instrument team lead and professor of physics at the University of Iowa, Iowa City. "We thought we understood these radio wave patterns at gas giants, since Jupiter was so straightforward. Without Cassini's long stay, scientists wouldn't have understood that the radio emissions from Saturn are so different."

Saturn emits radio waves known as Saturn Kilometric Radiation, or SKR for short. To Cassini, they sound a bit like bursts of a spinning air raid siren, since the radio waves vary with each rotation of the planet. This kind of radio wave pattern had been previously used at Jupiter to measure the planet's rotation rate, but at Saturn, as is the case with teenagers, the situation turned out to be much more complicated.

When NASA's Voyager spacecraft visited Saturn in the early 1980s, the radiation emissions indicated the length of Saturn's day was about 10.66 hours. But as its clocking continued by a flyby of the joint ESA-NASA Ulysses spacecraft and Cassini, the radio burst varied by seconds to minutes. A paper in Geophysical Research Letters in 2009 analyzing Cassini data showed that the Saturn Kilometric Radiation was not even a solo, but a duet, with two singers out of sync. Radio waves emanating from near the north pole had a period of around 10.6 hours; radio waves near the south pole had a period of around 10.8 hours.

NASA's Aqua Satellite Spies a "3-leaf Clover" View of Ireland for St. Patrick's Day

Typical clovers have three leaves, unless you happen to be lucky, and NASA's Aqua satellite has provided three different views of Ireland to mark Saint Patrick's Day on March 17, 2011. With the luck o’ the Irish, NASA's Aqua satellite was fortunate to capturemostly clear views of the Emerald Isle in these near-infrared/visible, infrared and microwave light views acquired by Aqua’s Atmospheric Infrared Sounder (AIRS) instrument on March 3, 2011, at 13:11 UTC.

Ireland, located in the Atlantic Ocean, is the third-largest island in Europe, and originated the St. Patrick's Day holiday. Located west of Great Britain and separated from it by the Irish Sea, it is surrounded by hundreds of islands and islets. In March, Ireland's average daytime high temperature is near 9.4 degrees Celsius (49 degrees Fahrenheit) and its average nighttime low temperature is near 3.3 degrees Celsius (38 degrees Fahrenheit).

The AIRS instrument measures temperatures of land, sea and air to provide a better understanding of what is happening in those environments. The March 3 images reveal temperatures near the surface that were near normal for this time of year.

NASA's Aqua satellite circles Earth pole-to-pole 15 times a day in a sun-synchronous orbit to provide data and images to researchers in Earth, ocean and atmospheric sciences. When Aqua passed over Ireland on March 3, it captured visible, infrared and microwave images: a clover of images from one instrument.

Japan Quake May Have Shortened Earth Days, Moved Axis

The March 11, magnitude 9.0 earthquake in Japan may have shortened the length of each Earth day and shifted its axis. But don't worry—you won't notice the difference.

Using a United States Geological Survey estimate for how the fault responsible for the earthquake slipped, research scientist Richard Gross of NASA's Jet Propulsion Laboratory, Pasadena, Calif., applied a complex model to perform a preliminary theoretical calculation of how the Japan earthquake—the fifth largest since 1900—affected Earth's rotation. His calculations indicate that by changing the distribution of Earth's mass, the Japanese earthquake should have caused Earth to rotate a bit faster, shortening the length of the day by about 1.8 microseconds (a microsecond is one millionth of a second).

The calculations also show the Japan quake should have shifted the position of Earth's figure axis (the axis about which Earth's mass is balanced) by about 17 centimeters (6.5 inches), towards 133 degrees east longitude. Earth's figure axis should not be confused with its north-south axis; they are offset by about 10 meters (about 33 feet). This shift in Earth's figure axis will cause Earth to wobble a bit differently as it rotates, but it will not cause a shift of Earth's axis in space—only external forces such as the gravitational attraction of the sun, moon and planets can do that.

Both calculations will likely change as data on the quake are further refined.

In comparison, following last year's magnitude 8.8 earthquake in Chile, Gross estimated the Chile quake should have shortened the length of day by about 1.26 microseconds and shifted Earth's figure axis by about 8 centimeters (3 inches). A similar calculation performed after the 2004 magnitude 9.1 Sumatran earthquake revealed it should have shortened the length of day by 6.8 microseconds and shifted Earth's figure axis by about 7 centimeters, or 2.76 inches. How an individual earthquake affects Earth's rotation depends on its size (magnitude), location and the details of how the fault slipped.

Gross said that, in theory, anything that redistributes Earth's mass will change Earth's rotation.

NASA Light Technology Successfully Reduces Cancer Patients Painful Side Effects from Radiation

A NASA technology originally developed for plant growth experiments on space shuttle missions has successfully reduced the painful side effects resulting from chemotherapy and radiation treatment in bone marrow and stem cell transplant patients.


In a two-year clinical trial, cancer patients undergoing bone marrow or stem cell transplants were given a far red/near infrared Light Emitting Diode treatment called High Emissivity Aluminiferous Luminescent Substrate, or HEALS, to treat oral mucositis -- a common and extremely painful side effect of chemotherapy and radiation treatment. The trial concluded that there is a 96 percent chance that the improvement in pain of those in the high-risk patient group was the result of the HEALS treatment.

"Using this technology as a healing agent was phenomenal," said Dr. Donna Salzman, clinical trial principal investigator and director of clinical services and education at the Bone Marrow Transplant and Cellular Therapy Unit at the University of Alabama at Birmingham Hospital. "The HEALS device was well tolerated with no adverse affects to our bone marrow and stem cell transplant patients."

The HEALS device, known as the WARP 75 light delivery system, can provide a cost-effective therapy since the device itself is less expensive than a day at the hospital and a proactive therapy for symptoms of mucositis that are currently difficult to treat without additional, negative side effects.

Launching Balloons in Antarctica

They nicknamed it the "Little Balloon That Could." Launched in December of 2010 from McMurdo Station in Antarctica, the research balloon was a test run and it bobbed lower every day like it had some kind of leak. But every day for five days it rose back up in the sky to some 112,000 feet in the air.


Down on Earth, physicist Robyn Millan was cheering it on, hoping the test launch would bode well for the success of her grand idea: launches in 2013 and 2014 of 20 such balloons to float in the circular wind patterns above the South Pole. Each balloon will help track electrons from space that get swept up in Earth's magnetic field and slide down into our atmosphere. Such electrons are an integral part of the turbulent magnetic space weather system that extends from the sun to Earth.

A professor at Dartmouth College, Millan is the principal investigator for a project called BARREL, or Balloon Array for RBSP Relativistic Electron Losses. Millan's proposal will work hand in hand with NASA's Radiation Belt Space Probes (RBSP) mission, two NASA spacecraft due to launch in 2012 to study a mysterious part of Earth's magnetic environs called the Van Allen radiation belts. The radiation belts are made up of two regions, each one a gigantic donut of protons and electrons that surrounds Earth.

"We're both looking at the loss of particles from the radiation belts," says Millan. "RBSP sits in space near the equatorial plane and looks at the particles along magnetic field lines there. These particles come into our atmosphere – following magnetic field lines to their base at the Poles – and produce X-rays. BARREL measures those X-rays. Together we can combine measurements of the same set of particles."

Figuring out what causes this rain of electrons will do more than simply improve understanding of the physics behind what drives such high-energy particles. The charged particles within the radiation belts can damage sensitive electronics on spacecraft like those used for global positioning systems and communications, and can injure humans in space. (The electrons don't make it all the way to Earth, so pose no danger to those of us on the ground.) Experiments like BARREL and RBSP help us understand the processes and mitigate those risks.

The International Space Station video update

A Race Against Time to Find Apollo 14's Lost Voyager

In communities all across the U.S., travelers that went to the moon and back with the Apollo 14 mission are living out their quiet lives. The whereabouts of more than 50 are known. Many, now aging, reside in prime retirement locales: Florida, Arizona and California. A few are in the Washington, D.C., area. Hundreds more are out there -- or at least, they were. And Dave Williams of NASA's Goddard Space Flight Center in Greenbelt, Md., wants to find them before it's too late.

The voyagers in question are not astronauts. They're "moon trees" -- redwood, loblolly pine, sycamore, Douglas fir, and sweetgum trees sprouted from seeds that astronaut Stuart Roosa took to the moon and back 40 years ago.

"Hundreds of moon trees were distributed as seedlings," says Williams, "but we don't have systematic records showing where they all went."

And though some of the trees are long-lived species expected to live hundreds or thousands of years, others have started to succumb to the pressures of old age, severe weather and disease. At least a dozen have died, including the loblolly pine at the White House and a New Orleans pine that was damaged by Hurricane Katrina and later removed.

To capture the vanishing historical record, Williams, a curator at the National Space Science Data Center, has been tracking down the trees, dead or alive.