Nasa Technology

NASA's James Webb Space Telescope: A Year of Achievement and Success

2012-01-28T01:05:00.000-08:00

The James Webb Space Telescope marked a year of significant progress in 2011 as it continues to come together as NASA's next generation space telescope. The year brought forth a pathfinder backplane to support the large primary mirror structure, mirror cryotesting, creation of mirror support structures, several successful sunshield layer tests and the creation of an assembly station within NASA Goddard Space Flight Center's cleanroom. Achievements were also made in the areas of flight and communications software and the propulsion system.

In December, manufacturing and testing of all flight mirrors was completed in a final test at the X-ray and Calibration Facility at Marshall Space Flight Center, Huntsville, Ala. During these tests mirror segments were chilled to temperatures similar to those Webb will see in space, around minus 400 degrees Fahrenheit.

It was the culmination of work started in 2003. Heeding lessons learned from the Hubble Space Telescope, the program adopted the strategy of tackling the most difficult technical challenges first. That decision proved to be the right one. In June, all 18 flight primary mirror segments, plus the secondary, tertiary and fine steering mirrors, were polished and coated yielding exquisite surfaces that will enable Webb to image the most distant galaxies.

Two of Webb’s supporting and pathfinder structures were also completed. To assemble the flight telescope on the ground, a 139,000 pound structure will install the flight mirrors using an overhead track system supporting a robotic arm. The huge platform has been completed and assembled in the ultra-clean room used for telescope assembly at Goddard.

For more info, visit:
http://www.nasa.gov/topics/technology/features/webb-2011progress.html

Supersonic Research Fleet Grows at Kennedy

2012-01-24T01:15:00.000-08:00

The final pieces of a unique squadron of supersonic fighters arrived at NASA's Kennedy Space Center in Florida on Thursday, Jan. 19, where they will be reassembled and put to work with a private company aiming to use them for research and microgravity training.

The new planes were part of a group of five F-104 fighters bought by Starfighters Inc. from the Italian Air Force. The company already had four of the aircraft, but that wasn't enough for the company to pursue a number of different opportunities.

With nine aircraft at his disposal, Starfighters owner Rick Svetkoff said there will always be aircraft available to fly missions for a variety of customers. As importantly, the company will have what it needs to fly two aircraft on a single mission, with one serving as a chase plane to photograph experiments.

"Now we're in a position where we can really start operations," Svetkoff said. "Before, we couldn't do a lot of things we wanted to do."

Starfighters operates out of a hangar at the Shuttle Landing Facility at Kennedy under an agreement with Kennedy. Svetkoff's main goal is to fly research and development missions, ranging from experiments flown for universities to evaluating rocket and spacecraft components in high-stress environments including high-acceleration and microgravity.

Space Florida and Embry-Riddle University already have partnerships with the company.

Because the aircraft can soar to some 70,000 feet and speed past Mach 2, it can be used to launch small satellites into space. The 19-foot-long, 900-pound rocket, about the size of a Sparrow missile, has already been tested in a series of taxi runs hanging from an F-104's wings.

For more info, read http://www.nasa.gov/centers/kennedy/news/starfightersnewplanes.html

NASA Helps Kick Off 2012 FIRST Robotics Competition

2012-01-12T02:58:00.000-08:00

An international robotics competition aimed at developing a new generation of technology leaders kicks off at 10:30 a.m. EST Saturday, Jan. 7. NASA, the largest sponsor of the FIRST Robotics Competition, and its centers across the nation will join local technology firms to launch the event. The main competition kickoff will take place at Southern New Hampshire University in Manchester and will air live on NASA Television.

FIRST -- or For Inspiration and Recognition of Science and Technology -- is a long-standing challenge to inspire curiosity and create interest in science, technology, engineering and mathematics (STEM) among high school students. Encouraging students to pursue STEM studies and careers is the focus of NASA's education programs.

"NASA's Science Mission Directorate is proud to have sponsored this technology revolution for the past 19 years," said John Grunsfeld, NASA's associate administrator for the agency's Science Mission Directorate in Washington. "This program has given tens of thousands of students a crucial mentoring experience if they choose to be a part of future exploration endeavors in space. FIRST Robotics is fun and exciting and will sustain an unprecedented positive educational impact on our nation's youth."

The FIRST Robotics Competition gives students the opportunity to design, build and test a robot that can perform specific functions. The competition also gives students the opportunity to be mentored by NASA professionals, who help them to explore potential solutions to robotics problems and understand the real-world challenges faced by engineers and researchers.

"FIRST Robotics has had a tremendous impact on students' interest in robotics and invention since its inception," said Leland Melvin, NASA's associate administrator for Education. "In fact, it was a mutual interest in FIRST Robotics that led the agency to a recently announced collaboration with entertainer will.i.am. We are excited to work together to help inspire the next generation to pursue STEM and robotics studies."

For more info, visit :

http://www.nasa.gov/home/hqnews/2012/jan/HQ_12-004_FIRST_Robotics.html

NASA 'Smart SPHERES' Tested Successfully on International Space Station

2012-01-11T01:08:00.000-08:00

In November, a free-flying robot on the International Space Station successfully gathered and delivered motion data to its astronaut handler via a new smartphone controller.

The Human Exploration Telerobotics project, one of NASA's new, high-value Technology Demonstration Missions, equipped the compact, free-flying satellites - known as Synchronized Position Hold, Engage, Reorient Experimental Satellites, or SPHERES - with a Samsung Nexus S handset that features Google’s open-source Android platform.

Each volleyball-sized SPHERES has its own onboard power, propulsion, computing and navigational software. Adding the smartphone transforms the satellite into a free-flying robot, or "Smart SPHERES" -- complete with a compact, low-power, low-cost embedded computer and built-in cameras and sensors to enhance and expand robotic operations.

Minor modifications were made to the smartphones, including removing the GSM cellular communications chip to avoid interference with station electronics, and replacing the standard lithium-ion battery with AA alkaline batteries. Otherwise, the smartphone is identical to the off-the-shelf consumer device.

The ongoing experiment demonstrates how the Smart SPHERES can serve as remotely operated assistants for astronauts in space. In coming months, these compact assistants will conduct interior station surveys and inspections, capturing mobile camera images and video. NASA also plans to simulate external free-flight excursions and in time will test whether the robots can handle other, more challenging tasks.

For more info, Visit : http://www.nasa.gov/mission_pages/tdm/telerobotics/11-160.html

Cryogenic Testing Completed for NASA's Webb Telescope Mirrors

2011-12-27T02:43:00.000-08:00

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

2011-12-16T04:08:00.000-08:00

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

2011-12-13T04:04:00.000-08:00

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

2011-12-08T04:28:00.000-08:00

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

2011-12-06T02:49:00.000-08:00

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

2011-12-02T04:42:00.000-08:00

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

2011-11-29T00:58:00.000-08:00

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

2011-11-28T03:03:00.000-08:00

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

2011-11-24T02:04:00.000-08:00

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

2011-11-23T01:46:00.000-08:00

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)

2011-11-19T01:21:00.000-08:00

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

2011-11-18T00:36:00.000-08:00

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

2011-11-16T01:34:00.000-08:00

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

2011-11-09T00:38:00.000-08:00

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

2011-11-04T00:41:00.000-07:00

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

2011-11-03T01:35:00.000-07:00

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

2011-11-01T02:44:00.000-07:00

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

2011-10-01T00:05:00.000-07:00

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

2011-09-05T23:31:00.000-07:00

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

2011-08-24T22:56:00.000-07:00

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

2011-08-03T00:47:00.000-07:00

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?

2011-07-20T06:37:00.000-07:00

"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

2011-04-27T04:50:00.000-07:00

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

2011-04-22T06:40:00.000-07:00

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

2011-04-12T22:54:00.001-07:00

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?

2011-04-07T07:05:00.000-07:00

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

2011-04-04T01:48:00.000-07:00

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

2011-03-28T23:30:00.000-07:00

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

2011-03-23T03:18:00.000-07:00

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

2011-03-21T06:46:00.000-07:00

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

2011-03-16T02:10:00.000-07:00

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

2011-03-06T22:55:00.000-08:00

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

2011-02-22T21:03:00.000-08:00

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

2011-02-21T02:51:00.000-08:00

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

2011-02-18T00:44:00.000-08:00

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.

Five Things About NASA's Valentine's Day Comet

2011-02-13T23:44:00.000-08:00

Here are five facts you should know about NASA's Stardust-Next spacecraft as it prepares for a Valentine's "date" with comet Tempel 1. Feel free to sing along!

1. "The Way You Look Tonight" – The spacecraft is on a course to fly by comet Tempel 1 on Feb. 14 at about 8:37 p.m. PST (11:37 p.m. EST) -- Valentine's Day. Time of closest approach to Tempel 1 is significant because of the comet's rotation. We won't know until images are returned which face the comet has shown to the camera.

2. "It's All Coming Back To Me Now" – In 2004, Stardust became the first mission to collect particles directly from a comet, Wild 2, as well as samples of interstellar dust. The samples were returned in 2006 via a capsule that detached from the spacecraft and parachuted to the ground at a targeted area in Utah. Mission controllers then placed the still-viable Stardust spacecraft on a flight path that could reuse the flight system, if a target of opportunity presented itself. Tempel 1 became that target of opportunity.

3. "The First Time Ever I Saw Your Face" – The Stardust-NExT mission will allow scientists for the first time to look for changes on a comet's surface that occurred after one orbit around the sun. Tempel 1 was observed in 2005 by NASA's Deep Impact mission, which put an impactor on a collision course with the comet. Stardust-NExT might get a glimpse of the crater left behind, but if not, the comet would provide scientists with previously unseen areas for study. In addition, the Stardust-NExT encounter might reveal changes to Tempel 1 between Deep Impact and Stardust-Next, since the comet has completed an orbit around the sun.

4. "The Wind Beneath My Wings" – This Tempel 1 flyby will write the final chapter of the spacecraft's success story. The aging spacecraft approached 12 years of space travel on Feb. 7, logging almost 6 billion kilometers (3.5 billion miles) since launch. The spacecraft is nearly out of fuel. The Tempel 1 flyby and return of images are expected to consume the remaining fuel.

5. "Love is Now the Stardust of Yesterday" – Although the spacecraft itself will no longer be active after the flyby, the data collected by the Stardust-NExT mission will provide comet scientists with years of data to study how comets formed and evolved.

NASA Releases First 360-Degree View of Entire Sun

2011-02-07T22:03:00.000-08:00

On Feb. 6th, NASA's twin STEREO probes moved into position on opposite sides of the sun, and they are now beaming back uninterrupted images of the entire star—front and back.

"For the first time ever, we can watch solar activity in its full 3-dimensional glory," says Angelos Vourlidas, a member of the STEREO science team at the Naval Research Lab in Washington, DC.

NASA released a 'first light' 3D movie on, naturally, Super Bowl Sunday:

Scientists particularly want to better predict space weather and the violent eruptions that can spout from the sun's surface. These eruptions can damage satellites, disrupt communications and disable power systems on Earth.

"Solar missions such as STEREO and SDO not only give us more information about star formation and evolution throughout our universe, but are of vital importance in our quest to further understand the sun's processes and the effect they can have on our planet and way of life," said David Parker, director of space science and exploration for the U.K. Space Agency. "This spectacular 360-degree view is another triumph for the STEREO mission, which continues to obtain some of the best images yet of the sun."

The two identical spacecraft of the NASA STEREO mission were launched in October 2006. They are offset from one another, one flying ahead of the Earth and the other behind.

SDO is the first mission in NASA's Living with a Star program and was launched in February 2010. SDO's unique orbit allows high-resolution images of the sun to be recorded every three-quarters of a second.

Surprise Hidden in Titan's Smog: Cirrus-Like Clouds

2011-02-04T03:28:00.000-08:00

Every day is a bad-air day on Saturn's largest moon, Titan. Blanketed by haze far worse than any smog belched out in Los Angeles, Beijing or even Sherlock Holmes's London, the moon looks like a dirty orange ball. Described once as crude oil without the sulfur, the haze is made of tiny droplets of hydrocarbons with other, more noxious chemicals mixed in. Gunk.

Icky as it may sound, Titan is really the rarest of gems: the only moon in our solar system with an atmosphere worthy of a planet. This atmosphere comes complete with lightning, drizzle and occasionally a big, summer-downpour style of cloud made of methane or ethane -- hydrocarbons that are best known for their role in natural gas.

Now, thin, wispy clouds of ice particles, similar to Earth's cirrus clouds, are being reported by Carrie Anderson and Robert Samuelson at NASA's Goddard Space Flight Center in Greenbelt, Md. The findings, published February 1 in Icarus, were made using the Composite Infrared Spectrometer (CIRS) on NASA's Cassini spacecraft.

Unlike Titan's brownish haze, the ice clouds have the pearly white appearance of freshly fallen snow. Their existence is the latest clue to the workings of Titan's intriguing atmosphere and its one-way "cycle" that delivers hydrocarbons and other organic compounds to the ground as precipitation. Those compounds don't evaporate to replenish the atmosphere, but somehow the supply has not run out (yet?).

"This is the first time we have been able to get details about these clouds," says Samuelson, an emeritus scientist at Goddard and the co-author of the paper. "Previously, we had a lot of information about the gases in Titan's atmosphere but not much about the [high-altitude] clouds."

First Solar Sail organize in Low-Earth Orbit

2011-01-26T22:37:00.000-08:00

NASA is now one step nearer to sailing among the stars! In a famous milestone on Jan. 21, 2011, NASA engineers established that the NanoSail-D nanosatellite deployed its 100-square-foot polymer sail in low-Earth orbit and is working as planned. The deployment was complete with beacon packets data received from NanoSail-D and extra ground-based satellite tracking assets.

NASA hopes to one day use thin membranes to de-orbit satellites and space trash. While NanoSail-D's relatively low altitude means drag from Earth's atmosphere may lead any force from the sun, the nanosatellite remains a small first step towards finally deploying solar sails at higher altitudes.

Mars Sliding last Sun After drifter Anniversary

2011-01-24T05:18:00.000-08:00

The team operating NASA's Mars rover Opportunity will temporarily suspend commanding for 16 days after the rover's seventh anniversary next week, but the rover will stay busy.

For the fourth time since Opportunity landed on Mars on Jan. 25, 2004, Universal Time (Jan. 24, Pacific Time), the planets' orbits will put Mars almost directly behind the sun from Earth's perspective.

During the days surrounding such an alignment, called a solar conjunction, the sun can disrupt radio transmissions between Earth and Mars. To avoid the chance of a command being corrupted by the sun and harming a spacecraft, NASA temporarily refrains from sending commands from Earth to Mars spacecraft in orbit and on the surface. This year, the commanding moratorium will be Jan. 27 to Feb. 11 for Opportunity, with similar periods for the Mars Reconnaissance Orbiter and Mars Odyssey orbiter.

Downlinks from Mars spacecraft will continue during the conjunction period, though at a much reduced rate. Mars-to-Earth communication does not present risk to spacecraft safety, even if transmissions are corrupted by the sun.

NASA's Mars Reconnaissance Orbiter will scale back its observations of Mars during the conjunction period due to reduced capability to download data to Earth and a limit on how much can be stored onboard.

NASA & OPTIMUS PRIME team up to Educate Youth

2011-01-20T22:20:00.000-08:00

NASA has opened online voting for the agency's OPTIMUS PRIME Spin-off Award student video challenge. The public is invited to vote for its favorite videos, made by students in grades three through eight, developed to help educate America's youth about the profit of NASA's technologies.

NASA is using the union between Hasbro's TRANSFORMERS property and commercialized agency " Spinoffs" to help students know how technology developed for space and aeronautics "transforms" into what is old on Earth.

More than 190 children from 31 states have submitted creative videos describing their favorite agency technology from NASA's 2009 Spinoff publication. The students also documented why their video should be selected to win the NASA OPTIMUS PRIME trophy.

The top five submissions from each of two groups (third through fifth and sixth through eighth grades) will proceed for final judging. The voting course is open until Feb. 6.

A panel of NASA judges will select the winners in each of the two grade categories. The winning students, associated Spinoff companies and NASA innovators will be announced in February.

In addition to the trophy, the winners will travel to Colorado Springs, Colo., for an award service during the 27th National Space Symposium on April 12.

NASA intends to make this an annual competition. Students can begin thinking about next year's competition by deciding which Spinoffs they like best from NASA's recently-published Spin-off 2010.

Andromeda is So Hot 'n' Cold

2011-01-06T00:59:00.000-08:00

This mosaic of the Andromeda spiral galaxy highlights explosive stars in its interior, and cooler, dusty stars forming in its many rings. The image is a combination of observations from the Herschel Space Observatory taken in infrared light (seen in orange hues), and the XMM-Newton telescope captured in X-rays (seen in blues). NASA plays a role in both of these European Space Agency-led missions.

Herschel provides a detailed look at the cool clouds of star birth that line the galaxy's five concentric rings. Massive young stars are heating blankets of dust that surround them, causing them to glow in the longer-wavelength infrared light, known as far-infrared, that Herschel sees.

In contrast, XMM-Newton is capturing what happens at the end of the lives of massive stars. It shows the high-energy X-rays that come from, among other objects, supernova explosions and massive dead stars rotating around companions. These X-ray sources are clustered in the center of the galaxy, where the most massive stars tend to form.

Andromeda is our Milky Way galaxy's nearest large neighbor. It is located about 2.5 million light-years away and holds up to an estimated trillion stars. Our Milky Way is thought to contain about 200 billion to 400 billion stars.

Webb Telescope Sunshield Passes Launch Depressurization Tests to Verify Flight Design

2010-10-20T05:22:00.000-07:00

NASA's James Webb Space Telescope continues to make significant progress, successfully completing a series of sunshield vent tests that validate the telescope's sunshield design.

"While adequate venting is a design consideration for all spaceflight hardware, this was a particularly unique challenge for the sunshield given the large volume of trapped air in the membrane system at launch," said Keith Parrish, Webb telescope sunshield manager at NASA's Goddard Space Flight Center in Greenbelt, Md. "From the beginning of its development venting features have been a critical part of the overall sunshield design. Since we cannot vent test the actual flight article these test have shown the design works and the sunshield will vent safely on its way to orbit."

The sunshield on the Webb telescope will block the heat of the Sun and Earth from reaching the cold section of the Observatory. That's a critical function because the telescope and instruments must be cooled below 50 Kelvin (~-369.7 Fahrenheit) to allow them to see faint infrared emissions from astronomical objects. The sunshield consists of five layers of Kapton ®E with aluminum and doped-silicon coatings to reflect the sun's heat back into space.

Using flight-like sunshield membranes, the tests are designed to mimic the rapid change in air pressure the folded sunshield will experience the first minutes of launch. Several different folding configurations each underwent a series of 90-second depressurization tests and proved that the stowed sunshield will retain its shape during launch and allow trapped air to escape safely, both critical to sunshield deployment and performance.

Goddard Team attains the 'Unobtainium' for NASA's Next Space Observatory

2010-10-08T04:40:00.000-07:00

Imagine building a car chassis without a blueprint or even a list of recommended construction materials.

In a sense, that's precisely what a team of engineers at the NASA Goddard Space Flight Center in Greenbelt, Md., did when they designed a one-of-a-kind structure that is one of 9 key new technology systems of the Integrated Science Instrument Module (ISIM). Just as a chassis supports the engine and other components in a car, the ISIM will hold four highly sensitive instruments, electronics, and other shared instrument systems flying on the James Webb Space Telescope, NASA's next flagship observatory.

From scratch — without past experience to help guide them — the engineers designed the ISIM made of a never-before-manufactured composite material and proved through testing that it could withstand the super-cold temperatures it would encounter when the observatory reached its orbit 1.5-million kilometers (930,000 miles) from Earth. In fact, the ISIM structure survived temperatures that plunged as low as 27 Kelvin (-411 degrees Fahrenheit), colder than the surface of Pluto.

"It is the first large, bonded composite spacecraft structure to be exposed to such a severe environment," said Jim Pontius, ISIM lead mechanical engineer.

The 26-day test was specifically carried out to test whether the car-sized structure contracted and distorted as predicted when it cooled from room temperature to the frigid — very important since the science instruments must maintain a specific location on the structure to receive light gathered by the telescope's 6.5-meter (21.3-feet) primary mirror. If the structure shrunk or distorted in an unpredictable way due to the cold, the instruments no longer would be in position to gather data about everything from the first luminous glows following the big bang to the formation of star systems capable of supporting life.

"The tolerances are much looser on the Hubble Space Telescope," said Ray Ohl, a Goddard optical engineer who leads ISIM's optical integration and test. "The optical requirements for Webb are even more difficult to meet than those on Hubble."

NASA's Webb Telescope MIRI device Takes One Step quicker To Space

2010-10-05T05:07:00.000-07:00

A major instrument due to fly aboard NASA's James Webb Space Telescope is getting its first taste of space in the test facilities at the Rutherford Appleton Laboratory (RAL) in the United Kingdom. The Mid-InfraRed Instrument (MIRI) has been designed to contribute to areas of investigation as diverse as the first light in the early Universe and the formation of planets around other stars.

"The start of space simulation testing of the MIRI is the last major engineering activity needed to enable its delivery to NASA. It represents the culmination of 8 years of work by the MIRI consortium, and is a major progress milestone for the Webb telescope project," said Matt Greenhouse, NASA Project Scientist for the Webb telescope Integrated Science Instrument Module, at NASA's Goddard Space Flight Center, Greenbelt, Md.

The James Webb Space Telescope represents the next generation of space telescope and, unlike its predecessor Hubble, it will have to journey far from home. Its ultimate destination is L2, a gravitational pivot point located 1.5 million kilometers (930,000 miles) away, on the opposite side of the Earth from the Sun. Here it is cool enough for the MIRI to obtain exquisite measurements that astronomers will use to help decipher the Universe. "At L2 we are at an environmentally stable point where we can be permanently shaded from light from the Sun and Earth. That allows us to reach the very low temperatures - as low as 7K (- 447.1 Fahrenheit) in the case of MIRI – that are necessary to measure in the mid-infrared," says Jose Lorenzo Alvarez, MIRI Instrument Manager for European Space Agency (ESA).

The MIRI provides imaging, coronagraphy and integral field spectroscopy over the 5-28 micron wavelength range. It is being developed as a partnership between Europe and the U.S. The MIRI is one of four instruments flying aboard the Webb telescope. The other instruments include: NIRSpec (a near-infrared spectrograph), NIRCam (a near-infrared camera), and TFI (a tunable filter imager).

One of the jewels in the MIRI's crown is the potential to observe star formation that has been triggered by an interaction between galaxies. This phenomena has been difficult to study with Hubble or ground-based telescopes since the optical and near-infrared light from these newly formed stars is hidden from view by clouds of dust that typically surround newly formed stars This will not be a problem for MIRI, as it is sensitive to longer wavelengths of light in the range 5 to 28 microns, which can penetrate the dust.

However, keeping the MIRI at a colder temperature than on Pluto, for a sustained period of time, was one of the biggest engineering challenges facing those charged with constructing the instrument. "A critical aspect, to achieving the right sensitivity, is to ensure stable operation at 7 Kelvin (- 447.1 Fahrenheit) that will last for the five years of the mission," explains Alvarez.

Emerging Technologies May Fuel Revolutionary Launcher

2010-09-22T04:14:00.000-07:00

As NASA studies possibilities for the next launcher to the stars, a team of engineers from Kennedy Space Center and several other field centers are looking for a system that turns a host of existing cutting-edge technologies into the next giant leap spaceward.

An early proposal has emerged that calls for a wedge-shaped aircraft with scramjets to be launched horizontally on an electrified track or gas-powered sled. The aircraft would fly up to Mach 10, using the scramjets and wings to lift it to the upper reaches of the atmosphere where a small payload canister or capsule similar to a rocket's second stage would fire off the back of the aircraft and into orbit. The aircraft would come back and land on a runway by the launch site.

Engineers also contend the system, with its advanced technologies, will benefit the nation's high-tech industry by perfecting technologies that would make more efficient commuter rail systems, better batteries for cars and trucks, and numerous other spinoffs.

It might read as the latest in a series of science fiction articles, but NASA's Stan Starr, branch chief of the Applied Physics Laboratory at Kennedy, points out that nothing in the design calls for brand-new technology to be developed. However, the system counts on a number of existing technologies to be pushed forward.

'Mindshift' Biofeedback Gaming Technology

2010-09-07T04:14:00.000-07:00

Nasa - The gamer's quest is for reality, but there are limits when an animated, armored man is shooting at a banshee flying at him at simulated warp speed on a video screen; or a caricature of an athlete is trying to hit a light that represents a ball that can curve in ways that defy physics.

And logic.

This is the world in which NASA's Langley Research Center scientists Alan Pope and Chad Stephens worked with Langley Volunteer Service Program high school intern Nina Blanson until she decamped to become a freshman at Yale.

They have invented technology to inject stress levels into the games' controls so that the nervous or stressed shooter is aiming a moving gun at a moving target. The technology has a long, somewhat descriptive, acronym-defying name, but the inventors are just calling it "Mindshift" and are inviting representatives of the gaming industry to a demonstration on September 22 in Raleigh, N.C.

It includes a sensor attached to the player's earlobe, checking the pulse and wired into the control. Or sensors attached to the forehead, seeking the facial muscle strain that is a sign of stress.

Or even sensors attached to the player's partner to inject a social variable into game play, requiring teamwork between the two players. At issue is understanding that video games are with us, so why not involve them in the monitoring and treatment of stress?

"You don't have to do everything in a disciplined way," said Pope, whose field of expertise is engineering psychophysiology and biomedical feedback. "You can also do it recreationally.

"There are some people who claim that playing video games contributes to attention deficit, that it rewires our brains. Well, if that's the case then let's decide how we want video games rewiring our brain."

NASA Art challenger Lasso Their Imaginations to the Moon

2010-08-10T04:01:00.000-07:00

NASA - On your way home, you find it a little hard to breathe. Your breathing becomes shorter as your heart rate gets faster. Come to find out, your personal oxygen tank is low, so you stop at the oxygen station to get a refill, just to be on the safe side. As you are filling your oxygen tank, you talk with the person next to you about the craters around your home, meteor showers and the latest gossip of life on earth.

Once you fill your tank, your heart rate and breathing return to normal. You get home, call it a day, and buckle up in your bed near the ceiling to get a good night's rest.

Scenarios like this are what more than 200 college and high school students thought of when creating art and design entries to submit to NASA's "2010 Life and Work on the Moon Art and Design Contest." This may seem like a simple theme to apply when creating original artwork, but it was not as easy as one would think for these talented students.

Not only did they need to imagine and create original art related to life and work on the Moon, but the art needed to portray life that could survive the Moon's harsh conditions. Students needed to ask themselves, what would fuel a spacecraft, what types of food would people eat, how would there be enough oxygen, and many more questions like these.

Students expressed their creativity and innovation pertaining to life and work on the Moon through many categories, including two-dimensional, three-dimensional, digital art, music, literature and video.

"Offering students the opportunity to express themselves through art allows us to reach out to people who otherwise might not be able to participate in our program of exploration," said Jerry Hartman, Education Lead for the Exploration Systems Mission Directorate at NASA Headquarters. "Plus, the young people come up with a lot of cool stuff!"

A panel of scientists, professional artists and educators from the U.S. and other nations reviewed and judged the students' artwork. Judges based their reviews on three elements. The first was an artist statement that described what inspired the student, what artistic media they chose and why. Second was creativity and artistic expression. The third category and the hardest to judge was the validity of a realistic situation for the Moon's harsh conditions.

Jim Plaxco, third year NASA art contest judge, with his own digital art gallery website, Artsnova, describes how judging validity is the most difficult. "In the case of a painting that consists only of a space-suited astronaut walking on the surface of the Moon - does the person really understand that environment?" said Plaxco. "For example, people without spacesuits on the Moon is kind of a dead giveaway."

NASA Chief Technology Officer for IT Honored by CIO Magazine

2010-06-16T22:51:00.000-07:00

Nasa Technology - Chris C. Kemp, NASA’s chief technology officer for Information Technology and ‘super star’ of IT innovation for the agency, has been recognized with CIO Magazine’s “CIO 100” award for his work done while he was chief information officer for NASA’s Ames Research Center in Moffett Field, Calif., in 2009. Every year, CIO Magazine identifies and honors 100 organizations that have distinguished themselves through the effective and innovative use of information technology.

“I am honored to be recognized by CIO Magazine and to be the first honoree from Ames is truly humbling. The work that I did there in 2009 was meaningful to me and makes me extremely proud. I am inspired by NASA’s mission, and it’s been an honor to be a member of the team ” said Kemp.

The combination of Kemps’ enthusiasm for NASA and information technology has made him extremely successful at his job.

"This year's CIO 100 awards draws well-deserved attention to companies that are not only innovating with IT but creating genuine business value as well," said Maryfran Johnson, editor in chief of CIO Magazine. "These winning companies and their IT organizations are an inspiration to businesses everywhere."

Kemp is not afraid to venture into unchartered territory. In 2008, he began the Nebula Cloud Computing project (now a NASA-wide program) which uses open source software components to create a robust cloud environment where scientists can process and share data. Kemp also implemented an agency-wide IT Security Operations Center at Ames.

“The Nebula Platform allows scientists to focus on their research and spend less time and money on IT infrastructure. These researchers are doing amazing things, and it’s rewarding to create a platform that enables this innovation,” said Kemp.

Kemp is NASA’s first chief technology officer for IT, a new position established to lead IT innovation across the agency. "This move will leverage Chris’ creative talents and energies," said NASA Chief Information Officer Linda Cureton.

“I’m extremely excited about my new position. I’m thrilled to be involved in supporting many of the ground-breaking IT innovations happening here” Kemp said.

Kemp joined Ames as a successful entrepreneur, having helped create several companies including the third largest online community, Classmates.com. He also helped create the leading web-based vacation rental platform Escapia, and the first online grocery shopping platform for Kroger, the world’s largest grocery store chain.

Backwards Black Holes Might Make Bigger Jets

2010-06-08T06:12:00.000-07:00

Going against the grain may turn out to be a powerful move for black holes. New research suggests supermassive black holes that spin backwards might produce more ferocious jets of gas. The results have broad implications for how galaxies change over time.

"A lot of what happens in an entire galaxy depends on what's going on in the miniscule central region where the black hole lies," said theoretical astrophysicist David Garofalo of NASA's Jet Propulsion Laboratory in Pasadena, Calif. Garofalo is lead author of a new paper that appeared online May 27 in the Monthly Notices of the Royal Astronomical Society. Other authors are Daniel A. Evans of the Massachusetts Institute of Technology, Cambridge, Mass., and Rita M. Sambruna of NASA Goddard Space Flight Center, Greenbelt, Md.

Black holes are immense distortions of space and time with gravity that is so great, even light itself cannot escape. Astronomers have known for more than a decade that all galaxies, including our own Milky Way, are anchored by tremendous, so-called supermassive black holes, containing billions of suns' worth of mass. The black holes are surrounded and nourished by disks of gas and dust, called accretion disks. Powerful jets stream out from below and above the disks like lasers, and fierce winds blow off from the disks themselves.

The black holes can spin either in the same direction as the disks, called prograde black holes, or against the flow - the retrograde black holes. For decades, astronomers thought that the faster the spin of the black hole, the more powerful the jet. But there were problems with this "spin paradigm" model. For example, some prograde black holes had been found with no jets.

Garofalo and his colleagues have been busy flipping the model on its head. In previous papers, they proposed that the backward, or retrograde, black holes spew the most powerful jets, while the prograde black holes have weaker or no jets.

The new study links the researchers' theory with observations of galaxies across time, or at varying distances from Earth. They looked at both "radio-loud" galaxies with jets, and "radio-quiet" ones with weak or no jets. The term "radio" comes from the fact that these particular jets shoot out beams of light mostly in the form of radio waves.

The results showed that more distant radio-loud galaxies are powered by retrograde black holes, while relatively closer radio-quiet objects have prograde black holes. According to the team, the supermassive black holes evolve over time from a retrograde to a prograde state.

"This new model also solves a paradox in the old spin paradigm," said David Meier, a theoretical astrophysicist at JPL not involved in the study. "Everything now fits nicely into place."

The scientists say that the backward black holes shoot more powerful jets because there's more space between the black hole and the inner edge of the orbiting disk. This gap provides more room for the build-up of magnetic fields, which fuel the jets, an idea known as the Reynold's conjecture after the theoretical astrophysicist Chris Reynolds of the University of Maryland, College Park.

"If you picture yourself trying to get closer to a fan, you can imagine that moving in the same rotational direction as the fan would make things easier," said Garofalo. "The same principle applies to these black holes. The material orbiting around them in a disk will get closer to the ones that are spinning in the same direction versus the ones spinning the opposite way."

Jets and winds play key roles in shaping the fate of galaxies. Some research shows that jets can slow and even prevent the formation of stars not just in a host galaxy itself, but also in other nearby galaxies.

"Jets transport huge amounts of energy to the outskirts of galaxies, displace large volumes of the intergalactic gas, and act as feedback agents between the galaxy's very center and the large-scale environment," said Sambruna. "Understanding their origin is of paramount interest in modern astrophysics."

Sailor Reflects on NASA Technology That Saved His Life

2010-05-24T23:35:00.000-07:00

Just seven days after setting sail for a tiny island off the eastern tip of Puerto Rico on Dec. 26, 2009, Missourian Dennis Clements thought his life was over; his crippled 34-foot Fiberglas sailboat -- buffeted for four days by gale-force winds and high seas -- had capsized, tossing him into the frigid waters of the North Atlantic Ocean.

"At one point, I saw the mast pointed straight down to the bottom of sea, and the boat continued to roll," he said. "I was shaken loose somewhere underwater and when I reached the surface, I could see my boat about 30 feet away... I could see her stand up... She righted herself. She was heavily flooded. There was still a piece of sail and I saw it catch the wind. I saw her sail away and leave me there. And I was alone in the dark, and in the storm, 250 miles from the shore... As I floated there, I knew this was the end. This was how it would end for me."

Today, Clements considers himself fortunate.

Thanks to NASA technology, the Search and Rescue Satellite-Aided Tracking (SARSAT) program managed by the National Oceanic and Atmospheric Administration (NOAA), and the bravery of military rescuers, Clements was ultimately plucked to safety by a Navy seaman who had been dispatched from the U.S.S. Dwight D. Eisenhower. It was the only vessel within a hundred miles of Clements' location able to respond to the Coast Guard's call for help and attempt the rescue, which took only four minutes once the Navy helicopter arrived on the scene. "It was the bravest thing I've ever seen," Clements said.

In a sense, Clements dramatic rescue began years earlier when he bought a 406 MHz Emergency Position Indicating Radio Beacon (EPIRB), designed for maritime use. When his sailboat, "Gloria Adios" had taken on water, the beacon activated, transmitting an emergency distress signal that NOAA weather satellites equipped with NASA-developed repeaters then relayed back to NOAA-operated ground stations. While Clements battled the storm, which was slowly but surely overwhelming his sailboat, a chain reaction had already been set in place before the rogue wave had even capsized his boat.

Sometime after the beacon began transmitting the emergency alert, SARSAT equipment located hundreds of miles away received the signal and had begun processing it to determine its precise location. The U.S. Coast Guard, which is responsible for at-sea rescues, received the alert and searched the NOAA Registration Database to determine whether the beacon had been registered. Luckily for Clements, he had done so, providing emergency contact numbers and other information that the Coast Guard used to contact Clements' family.

The database is a vital part of the SARSAT program. "We use the database to provide critical information to help expedite the search process, especially if the location of the beacon is not immediately known," said Mickey Fitzmaurice, a space systems engineer for the SARSAT program, the organization that operates the U.S. component of the COSPAS-SARSAT system now comprised of 40 nations.

The beacon on Clements' boat was an older model and did not encode GPS location data, with its signal. However, the ground-station equipment used the Doppler effect from its low-Earth-orbiting weather satellites to help pinpoint the location of the signal. This can take a little time depending on where the satellites are located at the time of the incident. While the SARSAT system calculated the location of the signal, a Coast Guard search and rescue controller was on the phone calling to find out if Clements had gone to sea and where he was headed. From this information, a more precise location could be provided to the rescuers.

Given the harrowing weather conditions the night Clements was rescued, Fitzmaurice said it fortuitous that Clements had registered his beacon. The U.S. Coast Guard was able to confirm the validity of Clements’s distress signal. Therefore, the U.S. Coast Guard and U.S. Navy personnel involved in his rescue were not unnecessarily exposed to life-threatening conditions due to a false alert.

"The beacon registration information can help save lives, not only the person in distress, but also the rescuers," said LCDR Kathy Niles, U.S. Coast Guard SARSAT Liaison Officer. "NOAA's database currently contains about 275,000 registrations which, unfortunately, are only about 75 percent of the beacons out there."

Since his rescue on Jan. 2, 2010, Clements has had time to reflect on the technology and people who saved his life. "I'm very glad I had that beacon," he said. "I knew it was a satellite system and somewhere there were people monitoring it, but I didn't know it was a weather satellite. It really is a wonderful system that they have come up with," he said. "It speaks volumes about the United States of America in the things that matter to us as a nation, that we would invest time, resources, and manpower (into technologies) that save people's lives."

Now, NOAA, NASA, the U.S. Coast Guard, and U.S. Air Force officials say they are working together to develop and new and improved search and rescue system, called the Distress Alerting Satellite System (DASS).

Engineers at the NASA Goddard Space Flight Center in Greenbelt, Md., are developing next-generation search and rescue technologies that will more quickly detect and locate distress signals generated by 406 MHz beacons installed on aircraft and vessels or carried by individuals. That's because NASA plans to install the repeaters on Global Position System (GPS), a constellation of 24 spacecraft operating in mid-Earth orbit, and not weather satellites.

For more information visit - nasa.gov

Beauty of upcoming Airplanes is extra than Skin Deep

2010-05-18T22:32:00.000-07:00

An 18-month NASA research effort to visualize the passenger airplanes of the future has produced some ideas that at first glance may appear to be old fashioned. Instead of exotic new designs seemingly borrowed from science fiction, familiar shapes dominate the pages of advanced concept studies which four industry teams completed for NASA's Fundamental Aeronautics Program in April 2010.

Look more closely at these concepts for airplanes that may enter service 20 to 25 years from now and you'll see things that are quite different from the aircraft of today.

Just beneath the skin of these concepts lie breakthrough airframe and propulsion technologies designed to help the commercial aircraft of tomorrow fly significantly quieter, cleaner, and more fuel-efficiently, with more passenger comfort, and to more of America's airports.

You may see ultramodern shape memory alloys, ceramic or fiber composites, carbon nanotube or fiber optic cabling, self-healing skin, hybrid electric engines, folding wings, double fuselages and virtual reality windows.

"Standing next to the airplane, you may not be able to tell the difference, but the improvements will be revolutionary," said Richard Wahls, project scientist for the Fundamental Aeronautics Program's Subsonic Fixed Wing Project at NASA's Langley Research Center in Hampton, Va. "Technological beauty is more than skin deep."

In October 2008, NASA asked industry and academia to imagine what the future might bring and develop advanced concepts for aircraft that can satisfy anticipated commercial air transportation needs while meeting specific energy efficiency, environmental and operational goals in 2030 and beyond. The studies were intended to identify key technology development needs to enable the envisioned advanced airframes and propulsion systems.

NASA's goals for a 2030-era aircraft, compared with an aircraft entering service today, are:

* A 71-decibel reduction below current Federal Aviation Administration noise standards, which aim to contain objectionable noise within airport boundaries.
* A greater than 75 percent reduction on the International Civil Aviation Organization's Committee on Aviation Environmental Protection Sixth Meeting, or CAEP/6, standard for nitrogen oxide emissions, which aims to improve air quality around airports.
* A greater than 70 percent reduction in fuel burn performance, which could reduce greenhouse gas emissions and the cost of air travel.
* The ability to exploit metroplex concepts that enable optimal use of runways at multiple airports within metropolitan areas, as a means of reducing air traffic congestion and delays.

The teams were led by General Electric, Massachusetts Institute of Technology, Northrop Grumman and The Boeing Company. Here are some highlights from their final reports:

* The GE Aviation team conceptualizes a 20-passenger aircraft that could reduce congestion at major metropolitan hubs by using community airports for point-to-point travel. The aircraft has an oval-shaped fuselage that seats four across in full-sized seats. Other features include an aircraft shape that smoothes the flow of air over all surfaces, and electricity-generating fuel cells to power advanced electrical systems. The aircraft's advanced turboprop engines sport low-noise propellers and further mitigate noise by providing thrust sufficient for short takeoffs and quick climbs.
* With its 180-passenger D8 "double bubble" configuration, the Massachusetts Institute of Technology team strays farthest from the familiar, fusing two aircraft bodies together lengthwise and mounting three turbofan jet engines on the tail. Important components of the MIT concept are the use of composite materials for lower weight and turbofan engines with an ultra high bypass ratio (meaning air flow through the core of the engine is even smaller, while air flow through the duct surrounding the core is substantially larger, than in a conventional engine) for more efficient thrust. In a reversal of current design trends the MIT concept increases the bypass ratio by minimizing expansion of the overall diameter of the engine and shrinking the diameter of the jet exhaust instead. The team said it designed the D8 to do the same work as a Boeing 737-800. The D8's unusual shape gives it a roomier coach cabin than the 737.
* The Northrop Grumman team foresees the greatest need for a smaller 120-passenger aircraft that is tailored for shorter runways in order to help expand capacity and reduce delays. The team describes its Silent Efficient Low Emissions Commercial Transport, or SELECT, concept as "revolutionary in its performance, if not in its appearance." Ceramic composites, nanotechnology and shape memory alloys figure prominently in the airframe and ultra high bypass ratio propulsion system construction. The aircraft delivers on environmental and operational goals in large part by using smaller airports, with runways as short as 5,000 feet, for a wider geographic distribution of air traffic.
* The Boeing Company's Subsonic Ultra Green Aircraft Research, or SUGAR, team examined five concepts. The team's preferred concept, the SUGAR Volt, is a twin-engine aircraft with hybrid propulsion technology, a tube-shaped body and a truss-braced wing mounted to the top. Compared to the typical wing used today, the SUGAR Volt wing is longer from tip to tip, shorter from leading edge to trailing edge, and has less sweep. It also may include hinges to fold the wings while parked close together at airport gates. Projected advances in battery technology enable a unique, hybrid turbo-electric propulsion system. The aircraft's engines could use both fuel to burn in the engine's core, and electricity to turn the turbofan when the core is powered down.

NASA did not specify future commercial air transportation needs as domestic or global. All four teams focused on aircraft sized for travel within a single continent because their business cases showed that small- and medium-sized planes will continue to account for the largest percentage of the overall fleet in the future. One team, however, did present a large hybrid wing concept for intercontinental transport.

All of the teams provided "clear paths" for future technology research and development, said Ruben Del Rosario, principal investigator for the Subsonic Fixed Wing Project at NASA's Glenn Research Center in Cleveland. "Their reports will make a difference in planning our research portfolio. We will identify the common themes in these studies and use them to build a more effective strategy for the future," Del Rosario said.

These are some of the common themes from the four reports:

* Slower cruising -- at about Mach 0.7, or seven-tenths the speed of sound, which is 5 percent to 10 percent slower than today's aircraft -- and at higher altitudes, to save fuel.
* Engines that require less power on takeoff, for quieter flight.
* Shorter runways -- about 5,000 feet long, on average -- to increase operating capacity and efficiency.
* Smaller aircraft – in the medium-size class of a Boeing 737, with cabin accommodations for no more than 180 passengers – flying shorter and more direct routes, for cost-efficiency.
* Reliance on promised advancements in air traffic management such as the use of automated decision-making tools for merging and spacing enroute and during departure climbs and arrival descents.

The teams recommended a variety of improvements in lightweight composite structures, heat- and stress-tolerant engine materials, and aerodynamic modeling that can help bring their ideas to reality. NASA is weighing the recommendations against its objective of developing aeronautics technologies that can be applied to a broad range of aircraft and operating scenarios for the greatest public benefit.

"This input from our customers has provided us with well thought-out scenarios for our vision of the future, and it will help us place our research investment decisions squarely in the mainstream," said Jaiwon Shin, associate administrator for aeronautics research at NASA Headquarters in Washington.

"Identifying those necessary technologies will help us establish a research roadmap to follow in bringing these innovations to life during the coming years," Shin said.

The next step in NASA's effort to design the aircraft of 2030 is a second phase of studies to begin developing the new technologies that will be necessary to meet the national goals related to an improved air transportation system with increased energy efficiency and reduced environmental impact. The agency received proposals from the four teams in late April and expects to award one or two research contracts for work starting in 2011.

NASA managers also will reassess the goals for 2030 aircraft to determine whether some of the crucial technologies will need additional time to move from laboratory and field testing into operational use. The four teams managed to meet either the fuel burn or the noise goal with their concepts, not both.

A companion research effort looked at concepts for a new generation of supersonic transport aircraft capable of meeting NASA's noise, emissions and fuel efficiency goals for 2030. NASA envisions a broader market for supersonic travel, with aircraft carrying more passengers to improve economic viability while meeting increasingly stringent environmental requirements.

Pad Abort-1 Set for May 6 Launch

2010-05-05T23:41:00.000-07:00

Nasa - With hundreds of tests and verifications officially complete, members of the Flight Test Readiness Review board unanimously agreed that Pad Abort 1 (PA-1) is ready for launch May 6 at White Sands Missile Range, N.M.

Often in a readiness review prior to any launch, there are open items that need to be closed before a mission gets the “go-ahead.” If there is an issue with hardware or software, the launch date could be delayed until it is fixed. However, on April 22, the PA-1 team concluded that all flight and support hardware and software are flight ready, launch facilities and range assets are in place and that the flight test team is prepared to execute PA-1 efficiently, effectively, and safely.

PA-1 is the first fully integrated flight test of the launch abort system being developed for the Orion crew exploration vehicle. The test is part of an ongoing mission to develop safer vehicles for human spaceflight applications.

The only question mark for the launch is the weather with the major constraint being wind. The flight test team will monitor the weather closely on test day, leading up to the targeted 9 a.m. EDT launch.

Scientists Say Ice Lurks in Asteroid's Cold Heart

2010-04-28T23:13:00.000-07:00

Scientists using a NASA funded telescope have detected water-ice and carbon-based organic compounds on the surface of an asteroid. The cold hard facts of the discovery of the frosty mixture on one of the asteroid belt's largest occupants, suggests that some asteroids, along with their celestial brethren, comets, were the water carriers for a primordial Earth. The research is published in today's issue of the journal Nature.

"For a long time the thinking was that you couldn't find a cup's worth of water in the entire asteroid belt," said Don Yeomans, manager of NASA's Near-Earth Object Program Office at the Jet Propulsion Laboratory in Pasadena, Calif. "Today we know you not only could quench your thirst, but you just might be able to fill up every pool on Earth – and then some."

The discovery is a result of six years of observing asteroid 24 Themis by astronomer Andrew Rivkin of the Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland. Rivkin, along with Joshua Emery, of the University of Tennessee in Knoxville, employed the NASA Infrared Telescope Facility to take measurements of the asteroid on seven separate occasions beginning in 2002. Buried in their compiled data was the consistent infrared signature of water ice and carbon-based organic materials.

The study's findings are particularly surprising because it was believed that Themis, orbiting the sun at "only" 479 million kilometers (297 million miles), was too close to the solar system's fiery heat source to carry water ice left over from the solar system's origin 4.6 billion years ago.

Now, the astronomical community knows better. The research could help re-write the book on the solar system's formation and the nature of asteroids.

"This is exciting because it provides us a better understanding about our past – and our possible future," said Yeomans. "This research indicates that not only could asteroids be possible sources of raw materials, but they could be the fueling stations and watering holes for future interplanetary exploration."

Rivkin and Emory's findings were independently confirmed by a team led by Humberto Campins at the University of Central Florida in Orlando.

NASA detects, tracks and characterizes asteroids and comets passing close to Earth using both ground- and space-based telescopes. The Near-Earth Object Observations Program, commonly called "Spaceguard," discovers these objects, characterizes a subset of them, and plots their orbits to determine if any could be potentially hazardous to our planet.

Starry-Eyed Hubble Celebrates 20 Years of Awe and Discovery

2010-04-26T04:40:00.000-07:00

Over the years, Hubble has suffered broken equipment, a bleary-eyed primary mirror, and the cancellation of a planned shuttle servicing mission. But the ingenuity and dedication of Hubble scientists, engineers and NASA astronauts allowed the observatory to rebound and thrive. The telescope's crisp vision continues to challenge scientists and the public with new discoveries and evocative images.

"Hubble is undoubtedly one of the most recognized and successful scientific projects in history," said Ed Weiler, associate administrator for the Science Mission Directorate at NASA Headquarters in Washington. "Last year's space shuttle servicing mission left the observatory operating at peak capacity, giving it a new beginning for scientific achievements that impact our society."

Hubble fans worldwide are being invited to take an interactive journey with Hubble. They can also visit Hubble Site to share the ways the telescope has affected them. Follow the “Messages to Hubble” link to send an e-mail, post a Facebook message, or send a cell phone text message. Fan messages will be stored in the Hubble data archive along with the telescope’s science data. For those who use Twitter, you can follow @HubbleTelescope or post tweets using the Twitter hashtag #hst20.

The public also will have an opportunity to become at-home scientists by helping astronomers sort out the thousands of galaxies seen in a Hubble deep field observation. STScI is partnering with the Galaxy Zoo consortium of scientists to launch an Internet-based astronomy project where amateur astronomers can peruse and sort galaxies from Hubble’s deepest view of the universe into their classic shapes: spiral, elliptical, and irregular. Dividing the galaxies into categories will allow astronomers to study how they relate to each other and provide clues that might help scientists understand how they formed.

To visit the Galaxy Zoo page, go to http://www.hubble.galaxyzoo.org.

For educators and students, STScI is creating an educational website called “Celebrating Hubble’s 20th Anniversary." It offers links to facts and trivia about Hubble, a news story that chronicles the observatory’s life and discoveries, and the IMAX “Hubble 3D” educator's guide. An anniversary poster containing Hubble’s “hall-of-fame” images, including the Eagle Nebula and Saturn, also is being offered with downloadable classroom activity information.

Visit the website at http://amazing-space.stsci.edu/hubble_20.

To date, Hubble has observed more than 30,000 celestial targets and amassed more than a half-million pictures in its archive. The last astronaut servicing mission to Hubble in May 2009 made the telescope 100 times more powerful than when it was launched.

Testing Future Engine Technology is a Work of Art

2010-04-21T02:22:00.000-07:00

An engine nozzle turns a dramatic array of colors during a recent hot-fire test at NASA's White Sands Test Facility near Las Cruces, N.M. A team of engineers from Glenn Research Center in Cleveland, Ohio, Marshall Space Flight Center in Huntsville, Ala., and Johnson Space Center in Houston conducted tests on a cryogenic liquid oxygen and liquid methane engine to measure the engine’s performance for future use with in-space vehicles.

Last month, eight altitude chamber tests were performed using an Aerojet workhorse engine to gather design data for future lander and in-space engines. Using the altitude chamber, which simulates the space-type vacuum environment, engineers were able to attach a larger nozzle and vary the propellant mixture ratios to test the engine's overall operating capability. This technology could be selected for future use with vehicles designed for transport, descent, or ascent to another planetary body or asteroid.

The nozzle, or large bell-shaped hardware, directs the flow of the combustion products from the liquid methane fuel and liquid oxygen oxidizer mixture and accelerates the exhaust gasses to generate thrust. The nozzle material is made of columbium and heats up during the test causing the color change. The nozzle is radiatively cooled and once the engine shuts down, the nozzle returns to its previous color.

Another test objective was to look at the specific impulse, or gas mileage, this engine could provide to a space vehicle. Specific impulse is simply a measurement of the amount of thrust that can be attained per mass of rocket propellant consumed. The higher specific impulse attained improves the overall rocket performance and reduces the weight of propellants that need to be carried on the vehicle.

Overall, the test series was successful and valuable performance data was obtained. Data received from the tests is currently being reviewed to ensure the engine performed as expected on a continual basis with each individual test.

Engineers will continue to vary and refine the engine test parameters to evaluate the technology further. Developing technology is a test-rich process to ensure as many unknowns are worked out on the ground before this technology is put into application in a space environment.

STS-131 Landing Blog

2010-04-19T04:30:00.000-07:00

Space shuttle Discovery and the seven-person STS-131 crew are set to wrap up their mission to the International Space Station with a landing at Kennedy Space Center's Shuttle Landing Facility. Join blogger Steven Siceloff for landing-day updates from the runway's air traffic control tower.

During the two-week mission, Discovery brought the Leonardo multi-purpose logistics module and transferred its payload of science racks to the space station's laboratories. The flight was highlighted by three spacewalks.

President Outlines Exploration Goals, Promise

2010-04-16T05:05:00.000-07:00

Astronauts will soar spaceward in commercial spacecraft while NASA develops technology so humans can venture to Mars and out into the solar system, President Barack Obama told a space conference Thursday at NASA's Kennedy Space Center in Florida.

Laying out his plans, President Obama committed NASA to a series of development milestones he said would lead to new spacecraft for astronauts to ride to the International Space Station, a modified Orion capsule developed as an emergency return spacecraft, and a powerful new rocket. He also promised a host of new technologies that would protect space travelers from radiation and other unique hazards.

"Early in the next decade, a set of crewed flights will test and prove the systems required for exploration beyond low Earth orbit," the president said. "And by 2025, we expect new spacecraft designed for long journeys to allow us to begin the first-ever crewed missions beyond the moon into deep space. We’ll start by sending astronauts to an asteroid for the first time in history. By the mid-2030s, I believe we can send humans to orbit Mars and return them safely to Earth. And a landing on Mars will follow. And I expect to be around to see it."

The president spoke to 200 senior officials, space and industry leaders, and academic experts inside the Operations and Checkout Building at Kennedy in the same area that was used to process Apollo spacecraft for the missions to the moon in the 1960s and 70s.

Standing in front of one of the space shuttle main engines that launched former U.S. Senator and astronaut John Glenn into orbit, President Obama said, "It was from here that men and women, propelled by sheer nerve and talent, set about pushing the boundaries of humanity's reach.

"The question for us now is whether that was the beginning of something, or the end of something. I prefer to believe it was the beginning of something."

The president's fiscal year 2011 budget proposal increases NASA's budget by $6 billion throughout the next five years to fund the plans.

Noting "the sense that folks in Washington -- driven less by vision than by politics -- have for years neglected NASA’s mission and undermined the work of the professionals who fulfill it," the president said the budget increase changes that.

The president's address comes at a critical juncture for NASA because the space shuttle fleet is scheduled to be retired after three more missions. The president said it will be quicker and less costly to let private companies develop new spacecraft for astronauts rather than continue with NASA's Constellation Program, which was deemed too expensive and behind schedule.

"Pursuing this new strategy will require that we revise the old strategy. In part, this is because the old strategy -- including the Constellation Program -- was not fulfilling its promise in many ways," the president said. "That’s not just my assessment; that’s also the assessment of a panel of respected non-partisan experts charged with looking at these issues closely."

President Obama's plan largely mirrors the "flexible path" option offered by a blue-ribbon panel established by the president last year to help decide the best map for future space exploration.

The outline does not do away with all the research and development from Constellation . Noting the success of the agency's development of the Orion crew capsule, Obama called on NASA to develop a version of that spacecraft so it can be launched without a crew to the International Space Station. It will be based there as an emergency craft for astronauts living on the orbiting laboratory.

The speech kicked off the Conference on the American Space Program for the 21st Century.

Norm Augustine, chairman of the blue-ribbon panel called the Review of U.S. Human Space Flight Plans Committee, that evaluated Constellation and came up with the "flexible path" option, endorsed the presidential strategy as the conference got under way.

Saying NASA is largely "trapped" in low Earth orbit, Augustine said industry, with NASA's guidance, can do its part for the plan.

The president acknowledged the need to get the decision right.

"Now, the challenges facing our space program are different, and our imperatives for this program are different than in decades past," the president said. "But while the measure of our achievements has changed a great deal over the past fifty years, what we do -- or fail to do -- in seeking new frontiers is no less consequential for our future in space and here on Earth."

The plan, the president said, would free NASA's designers and engineers to develop spacecraft, large rockets and new technologies that can extend the frontier of human space exploration to asteroids and even Mars.

About $3.1 billion of the additional funding would go into research and development for a heavy-lift rocket. A design for a large booster would be chosen in 2015 with the goal of launching the spacecraft a few years later. The bigger rocket could be used to loft payloads too large for most boosters, including giant fuel depots that would be parked in distant orbits so spacecraft could refuel on their way to asteroids, the moons of Mars and eventually Mars itself.

In addition to more funding, President Obama said his initiative brings more jobs than previous schedules.

"My plan will add more than 2,500 jobs along the Space Coast in the next two years compared to the plan under the previous administration," he said. "I’m proposing a $40 million initiative led by a high-level team from the White House, NASA, and other agencies to develop a plan for regional economic growth and job creation. And I expect this plan to reach my desk by Aug. 15. It’s an effort that will help prepare this already skilled work force for new opportunities in the space industry and beyond."

Students take Fresh Outlook and latest Technology to Webb Telescope

2010-04-12T04:34:00.000-07:00

Deep inside Building 5 at NASA's Goddard Space Flight Center in Greenbelt, Md., graduate students are on the front lines of technology development adjusting lasers and mirrors and spending long hours at a computer terminals. University partnerships are playing key roles in developing new and innovative technologies for NASA missions while creating a pathway for future NASA scientists and engineers.

"Investments in students today help us build what comes after the Webb telescope," said Lee Feinberg, Webb telescope Optical Telescope Element Manager at NASA Goddard. "University professors serve on our advisory boards. It allows us to tap the brightest minds in the country."

Past experience bears out Feinberg's observations.

Six years ago, Matthew Bolcar was a graduate student from the University of Rochester, N.Y. when he started working at NASA Goddard. He has been exploring interesting problems and developing risk-reduction techniques related to aligning segmented mirrors on the Webb telescope.

The Webb telescope primary mirror is composed of 18 segments that will unfold to create a single 6.5-meter (21-foot) mirror system once the observatory reaches orbit and begins operations. To work properly, the mirrors must be perfectly aligned. "If there were a problem, the telescope's operators could adjust the mirrors from the ground to correct for any possible misalignments," said Bruce Dean, group leader of the Wavefront Sensing and Control (WFSC) group at NASA Goddard.

Dean's group was charged with developing the software to compute the optimum position of each of the 18 mirrors, and then adjusting and aligning them, if necessary. The work was funded by the Webb telescope technology development program and was patented by Goddard in 2009. Goddard worked together with Ball Aerospace & Technologies Corp. in 2005, to develop this flight software for the Webb Space Telescope.

In 2006-2007, a team of engineers from both Goddard and Ball Aerospace & Technologies Corp., successfully tested the WFSC algorithms on a laboratory model of the Webb Telescope, proving they are ready to work in space.

Today, Bolcar is a full-time optical engineer for the Goddard WFSC group. Currently, he is working on the Thermal InfraRed Sensor (TIRS) instrument that will fly on the Landsat Data Continuity Mission (LDCM), the next in a series of satellites that have remotely sensed Earth’s continental surfaces for more than 30 years. He's also working on an experimental instrument, called the Visible Nulling Coronagraph (VNC) that would be used for exoplanet detection.

The graduate fellowship and co-op programs give NASA time to train students for optical engineering. "It takes four to five years to really train someone in wavefront-sensing technology," Dean added.

University partnerships are a great way to get young engineers and scientists interested in NASA, Bolcar agreed. "When you're a graduate student, wherever the funding is, you are going to develop partnerships and relationships," he added. "There is a potential to go beyond graduate school. It's good for the university and its good for attracting young talent to NASA."

Alex Maldonado, a University of Arizona graduate student in optical engineering, is following in Bolcar's footsteps. He spends half his time working at Goddard as a co-op student and the other half taking classes at the university in Tucson, Ariz. When at Goddard, he researches new techniques for polishing optical lenses to prevent light scattering.

Astronomers need bigger and smoother mirrors that will collect more light to allow scientists to see faint objects farther into the distant universe. A common and effective technique for shaping optical lenses is called diamond-turning, where a diamond tip cuts away the lens material. However, this technique also introduces flaws that can deflect light. Maldonado spends much of his time designing and executing testing procedures to see if new polishing techniques reduce this effect -- efforts that will be applied to the Near Infrared Camera (NIRCam), a Webb telescope imager.

The University of Arizona is providing the Near Infrared Camera (NIRCam) to the Webb Space Telescope, an imager with a large field of view and high angular resolution. Prof. Marcia Rieke at the University is the lead for that instrument.

The James Webb Space Telescope is the next-generation premier space observatory, exploring deep space phenomena from distant galaxies to nearby planets and stars. The Webb Telescope will give scientists clues about the formation of the universe and the evolution of our own solar system, from the first light after the Big Bang to the formation of star systems capable of supporting life on planets like Earth.

"In addition to the students, we work with the professors," according to Dean. Bolcar's graduate professor, James R. Fienup, is a world-renowned expert in optics. "We asked him to help us cover high-risk areas on the Webb telescope," said Dean.

"This is a win-win for the schools and NASA," said Feinberg. "We fund their graduate students, and in return, we get really bright, fresh minds working on NASA's most challenging missions.

Expected to launch in 2014, the telescope is a joint project of NASA, the European Space Agency and the Canadian Space Agency.

Flying Across the Moon

2010-04-07T05:33:00.000-07:00

The International Space Station flew across the face of the moon over NASA's Kennedy Space Center in Florida approximately 15 minutes before the launch of space shuttle Discovery on the STS-131 mission. Discovery successfully launched on April 5 and is now docked with the station. STS-131 will deliver the multi-purpose logistics module Leonardo, filled with supplies, a new crew sleeping quarters and science racks that will be transferred to the International Space Station's laboratories. The crew also will switch out a gyroscope on the station’s truss, install a spare ammonia storage tank and retrieve a Japanese experiment from the station’s exterior.

IV Water Filter May Open Medical Options for Astronauts

2010-04-02T21:27:00.000-07:00

Technology for a water filtration system initially developed at NASA's Kennedy Space Center in Florida is going to get a major test during the STS-131 mission as it is called on to create water clean enough to be used intravenously, commonly referred to as an IV. If it works, the system could prove critical to future astronauts if they have a medical emergency while traveling far from Earth. It could also find earthbound uses by the military, in remote locations or in humanitarian relief efforts.

Dr. Philip Scarpa’s team at Kennedy partnered with NASA’s Glenn Research Center in Ohio to develop a device that filters microscopic contaminants, including heavy metals and toxins, out of drinking water to produce fluid as sterile as any made on Earth.

"On every space mission, there's a potential of getting sick or getting hurt," Scarpa said. As Kennedy's medical operations manager, Scarpa helps provide medical support to the astronauts before they launch into space and after they land.

On Earth, several medical conditions require IV fluids, usually for rehydration or for delivering medicines. The NASA International Space Station Patient Condition Database identified 115 medical conditions that could occur on the space station and would require IV fluids to be administered.

For example, an astronaut with severe burns can require about 100 liters of IV fluids for weeks, with 30 liters needed in the first three days. One recent NASA study reported that a mission to Mars may need as much as 248 liters of IV fluids on board. Currently there are 12 liters of fluid stored on the space station. Even less severe conditions, such as broken bones or motion sickness, can deplete the stock quickly, especially if more than one astronaut is sick or injured.

At more than two pounds of weight per liter, IV fluids are very costly to take into space. It also takes up a lot of volume, and due to its need for sterility, IV fluids have a limited shelf life.

“On board or ‘in-situ’ production of IV fluids needed for medical treatments, could greatly reduce these costs and storage limitations, and would give NASA much more flexibility in how it can use the water it already has on the spacecraft,” Scarpa said.

Prior to partnering with Glenn in 2007, Scarpa teamed up with researchers from the United Kingdom and Canada to develop the technology. Called “Project Clearwater,” the team started its research in 2005 with a grant from the Florida Space Research Institute. "When we started looking into this, we thought we would quickly find out that someone had done this already," Scarpa said. "After our background research, we were surprised that no one had been successful with this before. It's not easy. The requirements for medical-grade water for injection are very strict and difficult to meet without large factory-based processes."

Devising a workable filter system for space also presents more hurdles than just removing contaminants successfully.

Without gravity, water can channel by adherence to its container and bypass a filter entirely. Mixing of the final salt water solution also could be incomplete, and launch vibrations could cause the device to release small particulates into the lines. Also, without gravity, the air in the system doesn't separate out from the fluid. This may form bubbles in critical areas, such as blocking off filters. If the filters are blocked, the water will not be screened.

"Bubbles are probably the biggest concern," Scarpa said. “Bubbles in IV fluids are dangerous for a patient as well. If entered into the veins, they could cause a stroke by blocking the brain’s blood flow.”

Scarpa’s team devised the use of micron-sized filters to trap and squeeze out the bubbles from the system.

By 2006, the team had developed a suitcase-sized device that filtered both drinking and dirty water, producing ultra-pure sterile water that meets all U.S. Pharmacopeia standards.

Based on that initial success, the team from Kennedy and Glenn developed a flight-ready system. Dubbed “IVGEN” for IntraVenous Fluid Generation, it will seek to produce IV-grade water from available space station drinking water.

The device will be hooked up to an Iodine Crew Water Container on the station and water will be transferred into an accumulator, which is a plastic bag inside a hard container. Nitrogen from the station will pressurize the bag to push the water out of the accumulator and through several micron filters, a deionized packed resin filter, then another set of micron filters and into an IV collection bag similar to the kind used in hospitals.

The strength of Pete Conrad Lives on at improvement Summit

2010-03-30T04:58:00.000-07:00

A lunar habitat module, paper that captures sound as energy and a drug delivery system for use in space. What do these inventions have in common? They’re all concepts being developed for commercialization by high school students competing in the Conrad Foundation’s Innovation Summit.

The summit is being held April 8-10, 2010 at NASA’s Ames Research Center, Moffett Field, Calif. The "Spirit of Innovation" award is in honor of the late Charles 'Pete' Conrad, a highly decorated naval aviator and astronaut who flew Gemini V, Gemini XI, commanded Apollo XII and was the third person to walk on the moon. Conrad went on to fly Skylab, our first space station. He received a Congressional Space Medal of Honor for his work on Skylab.

Nancy Conrad, wife of the late Pete Conrad, serves as chairman of the Conrad Foundation. She formed the program to provide high school students with an understanding of science and technology and give them an opportunity to solve real world problems through innovation and entrepreneurship.

During the three-day event, 25 teams from all over the U.S. present their ideas to a panel of experts similar to the way start-up entrepreneurs "pitch" to potential investors. The teams create an online portfolio (videos, blog and "company" logo) to present to venture capitalists, entrepreneurs and scientists.

Winning teams receive an opportunity to commercialize the technology and $5,000 in seed money to further develop the product.

"Our goal is to excite students about science, technology and innovation by connecting them with top entrepreneurs, scientists and industry leaders," said Joshua Neubert, executive director for the Conrad Foundation.

Niveditha Jayasekar, a student from Monta Vista High School in Cupertino, Calif., said she became fascinated with nanotechnology as early as the sixth grade. Jayasekar and her four teammates are using a patented nanotechnology developed by NASA scientist Dr. David Loftus to deliver pharmaceuticals in microgravity. The team hopes the product could lead to future breakthroughs in the field of space medicine.

NASA Astrobiology Institute ‘Removes Walls’ for Virtual Conference

2010-03-25T06:17:00.000-07:00

A virtual "Workshop Without Walls" conference hosted last week by the NASA Astrobiology Institute (NAI) drew more than 170 registrants from 21 states and 16 foreign countries.

Entitled "The Organic Continuum from the Interstellar Medium to the Early Earth," the two-day workshop held March 11-12, 2010 was organized by George Cody, leader of the NAI's Carnegie Institution of Washington team and Doug Whittet, leader of the NAI’s team at the Rensselaer Polytechnic Institute, Troy, New York.

Among the countries represented at the workshop were Canada, Mexico, six western European nations, Ukraine, India, South Korea, Japan, Australia, Brazil, Colombia, and Uruguay.

"The Workshop was in many ways a realization of the original vision of the virtual institute,"said Carl Pilcher, director of the NAI. "When the NAI began 12 years ago, we envisioned scientists interacting seamlessly at a distance. But the technology and the culture weren't ready. Today the technology works beautifully, and people have come to see this as the wave of the future. This workshop demonstrated that the future has arrived."

A total of 33 scientific talks were presented during the workshop, with interactive question and answer capability provided for the participants at eight sites equipped with high definition video and audio, and streaming with real-time question submission through the Adobe Connect web interface.

"The advances in technology that made this meeting possible have been paralleled by remarkable developments in the research that drives the science," Whittet said. "The benefit in terms of scientific knowledge gained and dollars expended by participants is likely unprecedented," added Cody.

According to Cody, the conference was "an experiment." Most participants categorized their experience level with remote collaborative technologies as beginner or intermediate, and a few had no prior experience at all.

Despite this, participants reported the experiment was a great success. "I was not expecting to have the same intellectual experience as I normally do at conferences…but after this conference, I do have that same sense of having been to a "real" conference,” adding, "this was very fulfilling for me professionally," said one participant.

Locations of participants ranged from a conference room in a major city with high-speed connectivity and professional videoconferencing equipment, to a home office in a small town with a laptop and home-based Internet connection.

"Over the course of the conference, I actually came to be unaware of the conference as being at multiple venues,"Cody said, "…the difference that high definition, high band-width videoconferencing makes is remarkable. Clear face-to-face contact with no time lag in either visual or audio was the essential part. Evidently the difference between 100 feet and 3000 miles is not all that great."

NASA's Spitzer Unearths Primitive Black Holes

2010-03-24T02:33:00.000-07:00

Astronomers have come across what appear to be two of the earliest and most primitive supermassive black holes known. The discovery, based largely on observations from NASA's Spitzer Space Telescope, will provide a better understanding of the roots of our universe, and how the very first black holes, galaxies and stars came to be.

"We have found what are likely first-generation quasars, born in a dust-free medium and at the earliest stages of evolution," said Linhua Jiang of the University of Arizona, Tucson. Jiang is the lead author of a paper announcing the findings in the March 18 issue of Nature.

Black holes are beastly distortions of space and time. The most massive and active ones lurk at the cores of galaxies, and are usually surrounded by doughnut-shaped structures of dust and gas that feed and sustain the growing black holes. These hungry, supermassive black holes are called quasars.

As grimy and unkempt as our present-day universe is today, scientists believe the very early universe didn't have any dust -- which tells them that the most primitive quasars should also be dust-free. But nobody had seen such immaculate quasars -- until now. Spitzer has identified two -- the smallest on record -- about 13 billion light-years away from Earth.

The quasars, called J0005-0006 and J0303-0019, were first unveiled in visible light using data from the Sloan Digital Sky Survey. That discovery team, which included Jiang, was led by Xiaohui Fan, a coauthor of the recent paper at the University of Arizona. NASA's Chandra X-ray Observatory had also observed X-rays from one of the objects. X-rays, ultraviolet and optical light stream out from quasars as the gas surrounding them is swallowed.

"Quasars emit an enormous amount of light, making them detectable literally at the edge of the observable universe," said Fan.

When Jiang and his colleagues set out to observe J0005-0006 and J0303-0019 with Spitzer between 2006 and 2009, their targets didn't stand out much from the usual quasar bunch. Spitzer measured infrared light from the objects along with 19 others, all belonging to a class of the most distant quasars known. Each quasar is anchored by a supermassive black hole weighing more than 100 million suns.

Shuttle Detector at Heart of Volcano Alert System

2010-03-23T05:29:00.000-07:00

As Tim Griffin and his team were working on better ways to detect hazardous gases on the shuttle launch pad, they found out they also could build something to find hazardous gases venting from a volcano.

That means they may be only a short time away from building an early warning system for volcano eruptions -- a system that could give those near an active cone days or more to evacuate to safety.

"There are all kinds of volcano eruptions, some have all kinds of gases and some don't have any gases," Griffin said. "The long-term idea for this is that we'd be able to characterize the volcanoes. Then if the volcano becomes more active, we can get a better idea of what's going on, how active it is, (and) do we think it's going to be a violent eruption or mainly gases coming out?"

Griffin, who is the chief of NASA Kennedy Space Center's Chemical Analysis Branch and holds a Ph.D. in chemistry, never studied volcanoes. Instead, his group's goal was to shrink the leak detection system at the launch pad from the size of three refrigerators to something that could be carried by hand, in a car or perhaps inside a spacecraft.

"This project started off as a way to push the boundaries with our shuttle system," said Richard Arkin of ASRC Aerospace, the detector's co-designer. "We wanted to make it smaller, more powerful and lighter while still maintaining operational abilities and maintenance."

Parts of the miniaturization work were easy, such as going from numerous sampling ports required at the pad to a single port for the smaller machine. Other aspects, such as building smaller pumps and other components, required innovation and invention. In both, a mass spectrometer is used to find out what chemicals are present in the air.

They also set out to make the unit relatively autonomous, but still reliable and hearty.

At this point, the detector weighs in at 75 pounds. It stands about 9 inches tall and its footprint is a bit larger than a backpack. In fact, one of the goals of the project is to make it small enough to be carried in a backpack.

Griffin was talking about some of the work involved in chemical analysis at a conference when officials from Costa Rica's scientific program asked about applying the technology to the volcanic studies. It started to look like a natural fit.

Costa Rica proved a good testing ground for the equipment because most of the population lives around or near four active volcanoes. They don't worry only about sudden eruptions, but also high concentrations of carbon dioxide the volcanoes vent. The gas tends to kill all vegetation and livestock near the venting areas, but people can't see the carbon dioxide.

The detector showed a way to find out where the gas pockets are and how they change. The team flew the detector on three different kinds of airplanes, where it modeled the chemicals in volcanic plumes in three dimensions, a level of precision that astonished Arkin.

"That was something that I never thought about doing," Arkin said.

The team also put the detector in the backseat of a car and drove it through Costa Rican cities to sample the air and also carried it into the volcanoes by hand. In the future, Griffin wants to load it inside drones so the detection system can fly directly into the plumes of erupting mountains without endangering a pilot.

The results are expected to provide more information to help researchers pinpoint what volcanoes are doing at any given time, and when or if they might be about to spew.

Winds of Change: How Black Holes May Shape Galaxies

2010-03-17T11:36:00.000-07:00

New observations from NASA's Chandra X-ray Observatory provide evidence for powerful winds blowing away from the vicinity of a supermassive black hole in a nearby galaxy. This discovery indicates that "average" supermassive black holes may play an important role in the evolution of the galaxies in which they reside.

For years, astronomers have known that a supermassive black hole grow in parallel with its host galaxy. And, it has long been suspected that material blown away from a black hole -- as opposed to the fraction of material that falls into it -- alters the evolution of its host galaxy.

A key question is whether such "black hole blowback" typically delivers enough power to have a significant impact. Powerful relativistic jets shot away from the biggest supermassive black holes in large, central galaxies in clusters like Perseus are seen to shape their host galaxies, but these are rare. What about less powerful, less focused galaxy-scale winds that should be much more common?

"We're more interested here in seeing what an "average"-sized supermassive black hole can do to its galaxy, not the few, really big ones in the biggest galaxies," said Dan Evans of the Massachusetts Institute of Technology who presented these results at the High Energy Astrophysics Division of the American Astronomical Society meeting in Kona, Hawaii.

Evans and his colleagues used Chandra for five days to observe NGC 1068, one of the nearest and brightest galaxies containing a rapidly growing supermassive black hole. This black hole is only about twice as massive as the one in the center of our Galaxy, which is considered to be a rather ordinary size.

The X-ray images and spectra obtained using Chandra's High Energy Transmission Grating Spectrometer showed that a strong wind is being driven away from the center of NGC 1068 at a rate of about a million miles per hour. This wind is likely generated as surrounding gas is accelerated and heated as it swirls toward the black hole. A portion of the gas is pulled into the black hole, but some of it is blown away. High energy X-rays produced by the gas near the black hole heat the ouflowing gas, causing it to glow at lower X-ray energies.

Crew Members Prep for Undocking, Future Arrivals

2010-03-16T12:04:00.000-07:00

NASA - Soaring high over the Earth in the International Space Station, the astronauts and cosmonauts of the Expedition 22 crew began a new week Monday, the final week in space for two of their number.

Commander Jeff Williams and Flight Engineer Maxim Suraev will depart the station Thursday aboard the Soyuz TMA-16 spacecraft. They will undock from the orbiting complex and take a three-and-a-half-hour ride that will culminate in a parachute-assisted landing on the steppe of Kazakhstan early that morning.

Williams and Suraev began their final week in orbit by testing the Soyuz spacecraft’s motion control system and recharging the satellite telephone they will carry with them in the unlikely event that they land off course in the barren landing region and need to contact search and recovery forces. They also spent three hours going over procedures for their homeward flight with specialists on the ground.

As members of the Expedition 21 and 22 crews, Williams and Suraev will have spent 169 days in space. Including his time on the Expedition 13 and STS-101 crews, this will give Williams a total of 362 days in space, placing him fourth on the all-time U.S. list of space travelers behind Peggy Whitson with 377 days, Mike Foale with 374 and Mike Fincke with 366. Williams will be 26th on the all-time endurance list for all space travelers.

Expedition 22 Flight Engineers Soichi Noguchi, T.J. Creamer and Oleg Kotov will continue their stay on the station becoming the new Expedition 23 crew. Kotov will become the new station commander when the departing Williams enters the Soyuz vehicle and closes the hatch.

On April 4, Expedition 23 will expand to a six-member crew. Arriving in the Soyuz TMA-18 spacecraft will be new station crew members Alexander Skvortsov, Tracy Caldwell Dyson and Mikhail Kornienko.

On April 7, space shuttle Discovery is scheduled to arrive for a thirteen day mission to supply the station with new science racks and ammonia tanks. STS-131 will feature three spacewalks and the delivery of the Leonardo Multi-Purpose Logistics Module.

In preparation for the joint spacewalks to be performed during STS-131, Creamer and Noguchi packed up equipment for Discovery to return to Earth and Noguchi performed maintenance on the cooling loops in the U.S. spacesuits housed in the station’s Quest airlock.

Controllers on the ground operated Canadarm2, the station’s robotic arm, to remove the Special Purpose Dextrous Manipulator, known as Dextre, from the Mobile Base System (MBS) on the complex’s truss structure. Tuesday they will move it to the outside of the Destiny laboratory in order to make the MBS available for use during STS-131.

Bursting at the Seams

2010-03-12T10:58:00.000-08:00

Dramatic plumes, both large and small, spray water ice out from many locations along the famed 'tiger stripes' near the south pole of Saturn's moon Enceladus. The tiger stripes are fissures that spray icy particles, water vapor and organic compounds.

This mosaic was created from two high-resolution images that were captured by the narrow-angle camera when NASA's Cassini spacecraft flew past Enceladus and through the jets on Nov. 21, 2009. Imaging the jets over time will allow Cassini scientists to study the consistency of their activity.

Go into a NASA Clean Room Daily with the Webb Telescope via NASA's 'Webb-cam'

2010-03-10T23:36:00.000-08:00

How often can you say that you've seen the components of a space telescope being worked on at NASA? The answer is probably "rarely, if ever." However, thanks to NASA's Goddard Space Flight Center in Greenbelt, Md., that has now changed.

Web cameras in Goddard's largest clean room are now providing daily, live coverage of work being done on components of the upcoming James Webb Space Telescope. You could say they're "Webb-cams" and they provide one image per minute so people can see what happens behind the scenes. Of course, the work happens during regular working hours, so there may not be action on screen all the time.

John Decker, Webb telescope Deputy Project Manager at NASA Goddard was the motivator in getting the "Webb-cam" up and running. "I thought it would be a great way for everyone to see what happens behind the scenes as components of this exciting new space telescope are being tested and coming together here at NASA Goddard," Decker said.

The Webb telescope project is managed at Goddard, and several components of this next generation space telescope are already in a clean room here.

The James Webb Space Telescope is the next-generation premier space observatory, exploring deep space phenomena from distant galaxies to nearby planets and stars. The Webb telescope will give scientists clues about the formation of the universe and the evolution of our own solar system, from the first light after the Big Bang to the formation of star systems capable of supporting life on planets like Earth. The telescope is a joint project of NASA, the European Space Agency, and the Canadian Space Agency and is expected to launch in 2014.

Clean rooms are like operating rooms in hospitals. They are pristine areas kept as free as possible of contaminants that could interfere with delicate technology. There are several clean rooms at NASA Goddard.

Anyone that works in a clean room, such as engineers and scientists, have to wear sterile bodysuits, head covers, gloves, boots, and face masks. It takes about 10 to 15 minutes to get dressed before entering, and it's important because even one speck of dust or a fingerprint could severely damage the sensitive telescope components and instruments. Clean rooms act to filter out these harmful contaminants through a unique ventilation system and an entire wall of air filters.

The clean room ventilation system circulates almost one million cubic feet of air every minute through 9,000 square feet of HEPA filters located along one wall. The HEPA filters are specially designed to last several decades. All of these features provide the largest Goddard clean room with a Class-10,000 rating. That means any cubic foot of air in the clean room has no more than 10,000 particles floating around in it larger than 0.5 microns. A micron is one-millionth of a meter, and typical “outside” air has millions of such particles. A human hair is between 20 and 200 microns wide.

Alternative Energy Crops in Space

2010-03-08T22:01:00.000-08:00

What if space held the key to producing alternative energy crops on Earth? That's what researchers are hoping to find in a new experiment on the International Space Station.

NASA - The experiment, National Lab Pathfinder-Cells 3, is aimed at learning whether microgravity can help jatropha curcas plant cells grow faster to produce biofuel, or renewable fuel derived from biological matter. Jatropha is known to produce high quality oil that can be converted into an alternative energy fuel, or biofuel.

By studying the effects of microgravity on jatropha cells, researchers hope to accelerate the cultivation of the plant for commercial use by improving characteristics such as cell structure, growth and development. This is the first study to assess the effects of microgravity on cells of a biofuel plant.

"As the search for alternate energy sources has become a top priority, the results from this study could add value for commercialization of a new product,” said Wagner Vendrame, principal investigator for the experiment at the University of Florida in Homestead. "Our goal is to verify if microgravity will induce any significant changes in the cells that could affect plant growth and development back on Earth."

Launched on space shuttle Endeavour’s STS-130 mission in February, cell cultures of jatropha were sent to the space station in special flasks containing nutrients and vitamins. The cells will be exposed to microgravity until they return to Earth aboard space shuttle Discovery's STS-131 mission targeted for April.

For comparison studies of how fast the cultures grow, a replicated set of samples are being maintained at the University of Florida's Tropical Research and Education Center in Homestead.

"Watching the space shuttle go up carrying a little piece of my work is an indescribable experience," said Vendrame. "Knowing that my experiment could contribute to creating a sustainable means for biofuel production on Earth, and therefore making this a better world adds special value to the work."

NASA’s International Space Station Program Wins Collier Trophy

2010-03-07T21:54:00.000-08:00

The International Space Station Program has won the 2009 Collier Trophy, which is considered the top award in aviation. The National Aeronautic Association bestows the award annually to recognize the greatest achievement in aeronautics or astronautics in America.

“We are honored to receive this prestigious award,” said Bill Gerstenmaier, associate administrator for NASA’s Space Operations Mission Directorate. “We're proud of our past achievements to build and operate the space station, and we're excited about the future- there's a new era ahead of potential groundbreaking scientific research aboard the station."

The International Space Station is a joint project of five space agencies and 15 countries that is nearing completion and will mark the 10th anniversary of a continuous human presence in orbit later this year. The largest and most complicated spacecraft ever built, the space station is an international, technological and political achievement that represents the latest step in humankind’s quest to explore and live in space.

Designated as a national laboratory by Congress in the 2005 NASA Authorization Act, the space station provides a research platform that takes advantage of the microgravity conditions 220 miles above the Earth’s surface across a wide variety of fields, including human life sciences, biological science, human physiology, physical and materials science, and Earth and space science.

Upon completion of assembly later this year, the station’s crew and its U.S., European, Japanese and Russian laboratory facilities will expand the pace of space-based research to unprecedented levels. Nearly 150 experiments are currently under way on the station, and more than 400 experiments have been conducted since research began nine years ago. These experiments already are leading to advances in the fight against food poisoning, new methods for delivering medicine to cancer cells and the development of more capable engines and materials for use on Earth and in space.

The international partner agencies – NASA, the Canadian Space Agency, the European Space Agency, the Japan Aerospace Exploration Agency and the Russian Federal Space Agency – provide control centers and support teams that train and launch crews to the station, provide support for systems operations and coordinate the on-orbit research 24 hours a day, 7 days a week, 365 days a year.

Now supporting a multicultural crew of six, the station has a mass of almost 800,000 pounds and a habitable volume of more than 12,000 cubic feet – approximately the size of a five-bedroom home, and uses state-of-the-art systems to generate solar electricity, recycle nearly 85 percent of its water and generate much of its own oxygen supply. Nearly 190 humans have visited the space station, which is now supporting its 22nd resident crew.

Former NASA Ames Employee Wants Energy to Bloom Throughout the World

2010-02-28T21:32:00.000-08:00

K.R. Sridhar used to spend his time as a researcher at NASA Ames Research Center, Moffett Field, Calif., looking at the sky and dreaming of ways to sustain life on Mars. Now, CEO of Bloom Energy, Sridhar heads a company that just unveiled new technology that could make energy cleaner, cheaper, more reliable and accessible to everyone in the world.

The journey from NASA to Bloom Energy started with Sridhar and a small team of university researchers working to build a fuel cell powered module to go to Mars. When their NASA project ended, the team left academic life, opened a research and development office in NASA Research Park, and began working to commercialize the fuel cell technology with a new company, ION America, which became Bloom Energy.

"NASA is a tremendous environment for encouraging innovation - it's all about solving problems that are seemingly unsolvable. After realizing that we could make oxygen on Mars, making electrons on Earth seemed far less daunting. We're grateful to NASA for giving us a challenge with serendipitous impact for mankind," said Sridhar.

Invented over a century ago, fuel cells have been used in practically every NASA mission since the 1960s. However, they have not gained widespread acceptance because of their inherently high cost. Traditional fuel cell technology used precious metals but this technology uses sand. Sand is inexpensive, which Sridhar asserts makes the Bloom Energy technology affordable and easy to mass produce.

As more people consume more energy, Sridhar became aware that the world was heading in the wrong direction. “We would be handing our children and their children a broken planet," ventured Sridhar. “I didn’t want to sit on the sidelines and do nothing." Sridhar believed that conservation alone was not enough and that there was a “calling to our generation to find a different way to create energy."

"To make clean reliable energy affordable for everyone in the world," is the mission of Bloom Energy. "One in three humans lives without power," Sridhar asserted. "Energy demand exceeds supply. Global population is growing quickly." Keeping these three facts in mind, Sridhar is working to bring energy to parts of the world that don’t have power.

A Stellar, Metal-Free Way to Make Carbon Nanotubes

2010-02-22T21:23:00.000-08:00

Nanotubes can grow on graphite (top) in an unruly mass (middle) according to "space's recipe." The overlapping segments on a single nanotube (bottom) are a telltale sign of the cup-stacked structure. (Image on bottom reproduced from Astrophysical Journal Letters.)

Space apparently has its own recipe for making carbon nanotubes, one of the most intriguing contributions of nanotechnology here on Earth, and metals are conspicuously missing from the list of ingredients.

The finding is the surprising by-product of lab experiments designed by Joseph Nuth at NASA’s Goddard Space Flight Center, Greenbelt, Md. and his colleagues to address the astronomical question of how carbon gets recycled in the regions of space that spawn stars and planets. The work also could help researchers understand puzzling observations about some supernovas.

In a recent paper in Astrophysical Journal Letters, Nuth’s team describes the modest chemical reaction. Unlike current methods for producing carbon nanotubes—tiny yet strong structures with a range of applications in electronics and, ultimately, perhaps even medicine—the new approach does not need the aid of a metal catalyst. "Instead, nanotubes were produced when graphite dust particles were exposed to a mixture of carbon monoxide and hydrogen gases," explains Nuth.

"I am amazed at the implications of this paper, not only for astrophysics but also for materials science," says Dick Zare, the chair of the chemistry department at Stanford University, Stanford, Calif. "Could Nature know a new chemistry for making carbon nanotubes that we have yet to discover?"

One indication of that possibility came in 2008, when the long, thin carbon structures known as graphite whiskers—essentially, bigger cousins of carbon nanotubes—were identified in three meteorites. That finding offered the tantalizing prospect that a haze of graphite whiskers in space could explain why some supernovas appear dimmer, and therefore farther away, than they should be, according to current models. Yet, "very little is known about graphite whisker formation, and so it is difficult to adequately interpret their discovery," says Marc Fries of NASA’s Jet Propulsion Laboratory, Pasadena, Calif.

The Puffin: A Passion for Personal Flight

2010-02-22T05:24:00.000-08:00

Meet the Puffin. It's an airplane concept conjured up by the mind of aerospace engineer Mark Moore. The unusual looking, vertical take-off and landing tailsitter is only an idea, but you'd never know that from the attention the Puffin has gotten on the Internet.

Moore came up with the design for the electric powered, 12-foot (3.7 m) long, 14.5-foot (4.4 m) wingspan personal air vehicle as part of the coursework for his doctoral degree. Then Langley's creativity and innovation and revolutionary technical challenges funds paid for much of the research. How the Puffin rocketed from esoteric erudition to web sensation is a classic case study in the power of the viral nature of the web.

"The animation of the Puffin on YouTube has gotten more 648,000 hits in a week," said Moore. "Until the concept was mentioned in the media Jan. 19, the video had only been clicked on a couple of thousand times since it was uploaded to the NASAPAV channel last November."

It all started with an email from a reporter who was pursuing a story on electric aircraft propulsion for "a couple of websites associated with space.com." As the former manager of the former Vehicle System program's Personal Air Vehicle sector. Moore is a nationally recognized expert on that and other small aircraft systems.

NASA, GM Take Giant Leap in Robotic Technology

2010-02-16T04:46:00.000-08:00

Robonaut is evolving.

NASA and General Motors are working together to accelerate development of the next generation of robots and related technologies for use in the automotive and aerospace industries.

Engineers and scientists from NASA and GM worked together through a Space Act Agreement at the agency's Johnson Space Center in Houston to build a new humanoid robot capable of working side by side with people. Using leading edge control, sensor and vision technologies, future robots could assist astronauts during hazardous space missions and help GM build safer cars and plants.

The two organizations, with the help of engineers from Oceaneering Space Systems of Houston, developed and built the next iteration of Robonaut. Robonaut 2, or R2, is a faster, more dexterous and more technologically advanced robot. This new generation robot can use its hands to do work beyond the scope of prior humanoid machines. R2 can work safely alongside people, a necessity both on Earth and in space.

"This cutting-edge robotics technology holds great promise, not only for NASA, but also for the nation," said Doug Cooke, associate administrator for the Exploration Systems Mission Directorate at NASA Headquarters in Washington. "I'm very excited about the new opportunities for human and robotic exploration these versatile robots provide across a wide range of applications."

NASA Airborne Radar to Study Quake Faults in Haiti, Dominican Republic

2010-01-29T03:35:00.000-08:00

In response to the disaster in Haiti on Jan. 12, NASA has added a series of science overflights of earthquake faults in Haiti and the Dominican Republic on the island of Hispaniola to a previously scheduled three-week airborne radar campaign to Central America.

NASA's Uninhabited Aerial Vehicle Synthetic Aperture Radar, or UAVSAR, left NASA's Dryden Flight Research Center in Edwards, Calif., on Jan. 25 aboard a modified NASA Gulfstream III aircraft.

During its trek to Central America, which will run through mid-February, the repeat-pass L-band wavelength radar, developed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., will study the structure of tropical forests; monitor volcanic deformation and volcano processes; and examine Mayan archeology sites. After the Haitian earthquake, NASA managers added additional science objectives that will allow UAVSAR's unique observational capabilities to study geologic processes in Hispaniola following the earthquake. UAVSAR's ability to provide rapid access to regions of interest, short repeat flight intervals, high resolution and its variable viewing geometry make it a powerful tool for studying ongoing Earth processes.

"UAVSAR will allow us to image deformations of Earth's surface and other changes associated with post-Haiti earthquake geologic processes, such as aftershocks, earthquakes that might be triggered by the main earthquake farther down the fault line, and the potential for landslides," said JPL's Paul Lundgren, the principal investigator for the Hispaniola overflights. "Because of Hispaniola's complex tectonic setting, there is an interest in determining if the earthquake in Haiti might trigger other earthquakes at some unknown point in the future, either along adjacent sections of the Enriquillo-Plantain Garden fault that was responsible for the main earthquake, or on other faults in northern Hispaniola, such as the Septentrional fault."

NASA Adds Extensive Data to Open Government Initiative Web Site

2010-01-25T04:29:00.000-08:00

NASA has contributed a wide range of scientific data to the new publicly accessible Web site "Data.gov" in accordance with the administration's Open Government Directive issued in Dec. 2009.

The purpose of Data.gov is to increase public access to high value datasets generated by the Executive Branch of the federal government. Public users may search for information by topic or by accessing the data contributed by any of the 24 participating major government departments and agencies.

NASA's input includes timely, extensive, accurate and relevant data about, Earth science and observation research, global change, agency missions, projects and instruments. Data.gov is a searchable Web site providing access to government information through the Raw Data, Tool and GeoData Catalogs.

The data may be read on line or downloaded to improve public knowledge of the agency and its operations; potentially create economic opportunities; or respond to need and demand as identified through public or industry consultation.

NASA products are in the Tool and GeoData Catalogs. Tool Catalog products include planet counter and climate change widgets and various Earth observation and other analysis utilities. In the GeoData Catalog, the agency posted more than 600 datasets across a wide range of imagery, maps, atmospheric, climate, geological and geophysical data. NASA will continuously update and add new data sets as they become available.

NASA's submission of an additional 18 catalogs released today is the first milestone within the Open Government Directive. Over the coming weeks, NASA will release a new Web site and provide a platform for public participation and engagement becoming a more transparent, participatory and collaborative agency.

JPL Scientist Receives American Meteorological Society Honor

2010-01-21T03:15:00.000-08:00

JPL senior research scientist Tim Liu has received the 2010 Verner E. Suomi Award from the American Meteorological Society, the nation's leading professional society for scientists in atmospheric and related sciences.

Liu is being recognized for his "research in space-borne measurements of air-sea interactions and the water cycle, and for inspiring progress through interdisciplinary science team leadership." The Suomi Award is given to individuals in recognition of highly significant technological achievement in the atmospheric or related oceanic and hydrologic sciences. The award is being presented today at the American Meteorological Society's 90th Annual Meeting in Atlanta.

Liu, a JPL research scientist since 1979, developed the first credible method of using satellite data to estimate evaporation and latent heat flux in the 1980s, and was one of the first scientists to use a combination of satellite sensors to study the global relationship between surface thermal forcing and ocean temperature response. He has served in scientific leadership positions on a number of NASA missions, including QuikScat, the NASA Scatterometer, Topex/Poseidon, Jason-1, the Tropical Rainfall Measurement Mission, Aqua and Aquarius. He has served on NASA's Earth Science and Application Division Advisory Subcommittee and various NASA science working groups. He has also served on numerous science working groups and advisory panels of the World Climate Research Program, and on the editorial boards of scientific journals.

Among Liu's other honors are a NASA Medal for Exceptional Scientific Achievement, a NASA Exceptional Achievement Medal and numerous NASA group achievement awards and certificates of recognition. He is a fellow of both the American Association for the Advancement of Science and the American Meteorological Society. A native of Hong Kong, Liu earned his bachelor's degree (Summa Cum Laude) at Ohio University in Athens, Ohio, and completed his master's degree and doctorate at the University of Washington, Seattle, where he also began his career as a research associate.

Locating Landslide Risks in Post-Quake Haiti

2010-01-19T04:30:00.000-08:00

Landslides are a potential threat for Haiti following the Jan. 12 earthquake. Mountainous areas surrounding Port-au-Prince may be subject to landslides after the quake shatters the rock substrate and exposes areas to severe erosion. The risk of further erosion and slope failure increases with the subsequent loss of vegetation combined with intense rainfall events that are typical of Haiti’s tropical environment.

Analysis of NASA satellite images showing areas of landslide risk have been shared with regional and international humanitarian assistance groups to assist those agencies with pinpointing their disaster relief efforts and anticipating further damages due to landslides.

The NASA satellite image analysis (see below) was produced by CATHALAC, the Spanish acronym for the Water Center for Humid Tropics of Latin America and the Caribbean. From its regional headquarters in Panama City, Panama, CATHALAC is one of the main implementing agencies for SERVIR, the Regional Visualization & Monitoring System for Mesoamerica and the Dominican Republic. SERVIR is supported by NASA and the U.S. Agency for International Development. Since SERVIR’s establishment in Mesoamerica in 2005, the system has served as a virtual observatory of the region’s atmosphere and terrestrial and marine environment. For more information, visit www.servir.net.

NASA’s Earth Observing-1 satellite with the Advanced Land Imager captured images of Haiti on Jan. 15, three days after the devastating 7.0 earthquake rocked Port-au-Prince and the surrounding area. The locations of possible landslide areas (left panel, purple) were identified by comparing this new image with archived imagery. The 7.0 epicenter of the quake is located to the southwest of Port-au-Prince near the town of Henry. Nearby aftershocks ranging from 4.1 to 6.0 are also shown in this image. Regions subject to severe erosion are in indicated in green in the right panel.

A close-up view of the area around Henry, Haiti, showing possible landslide areas (purple outlines) identified in analyses of images from NASA’s EO-1 satellite . This information has been shared with national authorities as well as regional and international humanitarian assistance groups.

Land Ho! Huygens Plunged to Titan Surface 5 Years Ago

2010-01-17T23:01:00.000-08:00

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

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

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

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

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

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

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

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

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

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

Solar Scientists Use 'Magnetic Mirror Effect' to Reproduce IBEX Observation

2010-01-13T02:19:00.000-08:00

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

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

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

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

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

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

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

Martian Landform Observations Fill Special Journal Issue

2010-01-12T04:52:00.000-08:00

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

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

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

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

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

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

Suzaku Finds "Fossil" Fireballs from Supernovae

2010-01-11T04:32:00.000-08:00

Studies of two supernova remnants using the Japan-U.S. Suzaku observatory have revealed never-before-seen embers of the high-temperature fireballs that immediately followed the explosions. Even after thousands of years, gas within these stellar wrecks retain the imprint of temperatures 10,000 times hotter than the sun's surface.

"This is the first evidence of a new type of supernova remnant -- one that was heated right after the explosion," said Hiroya Yamaguchi at the Institute of Physical and Chemical Research in Japan.

A supernova remnant usually cools quickly due to rapid expansion following the explosion. Then, as it sweeps up tenuous interstellar gas over thousands of years, the remnant gradually heats up again.

Capitalizing on the sensitivity of the Suzaku satellite, a team led by Yamaguchi and Midori Ozawa, a graduate student at Kyoto University, detected unusual features in the X-ray spectrum of IC 443, better known to amateur astronomers as the Jellyfish Nebula.

The remnant, which lies some 5,000 light-years away in the constellation Gemini, formed about 4,000 years ago. The X-ray emission forms a roughly circular patch in the northern part of the visible nebulosity.

Suzaku's X-ray Imaging Spectrometers (XISs) separate X-rays by energy in much the same way as a prism separates light into a rainbow of colors. This allows astronomers to tease out the types of processes responsible for the radiation.

Some of the X-ray emission in the Jellyfish Nebula arises as fast-moving free electrons sweep near the nuclei of atoms. Their mutual attraction deflects the electrons, which then emit X-rays as they change course. The electrons have energies corresponding to a temperature of about 12 million degrees Fahrenheit (7 million degrees Celsius).

Several bumps in the Suzaku spectrum were more puzzling. "These structures indicate the presence of a large amount of silicon and sulfur atoms from which all electrons have been stripped away," Yamaguchi said. These "naked" nuclei produce X-rays as they recapture their lost electrons.

But removing all electrons from a silicon atom requires temperatures higher than about 30 million degrees F (17 million C); hotter still for sulfur atoms. "These ions cannot form in the present-day remnant," Yamaguchi explained. "Instead, we're seeing ions created by the enormous temperatures that immediately followed the supernova."

NASA Supports the President's Educate To Innovate Campaign With Summer Of Innovation To Bring Students The Universe

2010-01-07T22:27:00.000-08:00

NASA has launched an initiative to use its out-of-this-world missions and technology programs to boost summer learning, particularly for underrepresented students across the nation. NASA's Summer of Innovation supports President Obama's Educate to Innovate campaign for excellence in science, technology, engineering and mathematics, or STEM, education.

The Summer of Innovation program will work with thousands of middle school teachers and students during multi-week programs in the summer of 2010 to engage students in stimulating math and science-based education programs. NASA's goal is to increase the number of future scientists, mathematicians, and engineers, with an emphasis on broadening participation of low-income, minority students.

"This is an incredible opportunity for our administration to come together to address our nation's critical science, technology, engineering and math education needs," said NASA Administrator and former astronaut Charles F. Bolden. "Through Summer of Innovation, NASA is calling on our financial and human resources to align with federal, state, and local governments, nonprofit partners, universities and teachers to expand the opportunity for more of our young people to aspire to and engage in the future prosperity of our nation."

Through competitive cooperative agreements to states, and partnerships with companies and nonprofits, NASA will use its substantial STEM assets -- including the agency's scientists and engineers -- to create multi-week summer learning programs.

"NASA's Summer of Innovation will increase the scope and scale of the agency's commitment to a robust program of STEM education opportunities," said Joyce Winterton, assistant administrator for education at NASA Headquarters in Washington.

The Summer of Innovation pilot will infuse NASA content and products into existing, evidence-based summer learning programs at the state level coupled with design competitions and events open to students and teachers nationwide. The program will culminate in a national event, in partnership with other departments and agencies.

NASA will use the Summer of Innovation as a catalyst to expand, align, and strengthen existing state-based networks. Awardees will be expected to implement the Summer of Innovation program and services during 2010 through the strategic infusion of NASA content and products into existing, evidence-based summer learning programs. The pilot program will seek to improve STEM performance for a diverse population of students, placing them on a trajectory to pursue further studies in STEM fields throughout their education.

Contingent upon the availability of funding, NASA intends to competitively select district partnerships in up to seven states to pilot the Summer of Innovation during 2010. Awards will have a period of performance of 36 months. Local programs will be required to develop ways to keep students and teachers engaged during the school year and to track student participants' performance through 2012. Awardees will be encouraged to leverage the unique capabilities and resources of program partners to ensure a sustainable effort following the period of performance.

Nature's Most Precise Clocks May Make "Galactic GPS" Possible

2010-01-06T03:45:00.000-08:00

Radio astronomers have uncovered 17 millisecond pulsars in our galaxy by studying unknown high-energy sources detected by NASA's Fermi Gamma-ray Space Telescope. The astronomers made the discovery in less than three months. Such a jump in the pace of locating these hard-to-find objects holds the promise of using them as a kind of "galactic GPS" to detect gravitational waves passing near Earth.

A pulsar is the rapidly spinning and highly magnetized core left behind when a massive star explodes. Because only rotation powers their intense gamma-ray, radio and particle emissions, pulsars gradually slow as they age. But the oldest pulsars spin hundreds of times per second -- faster than a kitchen blender. These millisecond pulsars have been spun up and rejuvenated by accreting matter from a companion star.

"Radio astronomers discovered the first millisecond pulsar 28 years ago," said Paul Ray at the Naval Research Laboratory in Washington. "Locating them with all-sky radio surveys requires immense time and effort, and we've only found a total of about 60 in the disk of our galaxy since then. Fermi points us to specific targets. It's like having a treasure map."

Millisecond pulsars are nature's most precise clocks, with long-term, sub-microsecond stability that rivals human-made atomic clocks. Precise monitoring of timing changes in an all-sky array of millisecond pulsars may allow the first direct detection of gravitational waves -- a long-sought consequence of Einstein's relativity theory.

"The Global Positioning System uses time-delay measurements among satellite clocks to determine where you are on Earth," explained Scott Ransom of the National Radio Astronomy Observatory in Charlottesville, Va. "Similarly, by monitoring timing changes in a constellation of suitable millisecond pulsars spread all over the sky, we may be able to detect the cumulative background of passing gravitational waves."

The sources Fermi detected are not associated with any known gamma-ray emitting objects and did not show evidence of pulsing behavior. However, scientists considered it likely that many of the unidentified sources would turn out to be pulsars.

NASA’s Kepler Space Telescope Discovers its First Five Exoplanets

2010-01-05T04:36:00.000-08:00

NASA's Kepler space telescope, designed to find Earth-size planets in the habitable zone of sun-like stars, has discovered its first five new exoplanets, or planets beyond our solar system.

Kepler's high sensitivity to both small and large planets enabled the discovery of the exoplanets, named Kepler 4b, 5b, 6b, 7b and 8b. The discoveries were announced Monday, Jan. 4, by the members of the Kepler science team during a news briefing at the American Astronomical Society meeting in Washington.

"These observations contribute to our understanding of how planetary systems form and evolve from the gas and dust disks that give rise to both the stars and their planets," said William Borucki of NASA's Ames Research Center in Moffett Field, Calif. Borucki is the mission's science principal investigator. "The discoveries also show that our science instrument is working well. Indications are that Kepler will meet all its science goals."

Known as "hot Jupiters" because of their high masses and extreme temperatures, the new exoplanets range in size from similar to Neptune to larger than Jupiter. They have orbits ranging from 3.3 to 4.9 days. Estimated temperatures of the planets range from 2,200 to 3,000 degrees Fahrenheit, hotter than molten lava and much too hot for life as we know it. All five of the exoplanets orbit stars hotter and larger than Earth's sun.

"It's gratifying to see the first Kepler discoveries rolling off the assembly line," said Jon Morse, director of the Astrophysics Division at NASA Headquarters in Washington. "We expected Jupiter-size planets in short orbits to be the first planets Kepler could detect. It's only a matter of time before more Kepler observations lead to smaller planets with longer period orbits, coming closer and closer to the discovery of the first Earth analog."

New Video Reveals Secrets of Webb Telescope's MIRI

2010-01-04T05:46:00.000-08:00

It's going to take infrared eyes to see farther back in time than even the Hubble Space Telescope, and that's what the James Webb Space Telescope's MIRI or Mid-Infrared Instrument detectors will do. Now there's a new short movie that shows what the MIRI detectors are all about and what they can do.

"The MIRI is one of four science instruments aboard the Webb telescope that is designed to record images and spectra at the longest wavelengths that the Webb telescope can observe," said Matt Greenhouse, Project Scientist for the science instrument payload. "The mid-infrared spectrum covers wavelengths in the range of 5 to 28 micrometers or microns (about 10 to 50 times longer than our eyes can see). Light in this portion of the spectrum is invisible to our eyes but is produced by all room-temperature objects and carries key information about the local and early universe," Greenhouse said. Light at these wavelengths is blocked by water vapor in the earth’s atmosphere and can only be efficiently observed using a telescope in space.

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

2009-12-30T00:58:00.000-08:00

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

2009-12-28T21:00:00.001-08:00

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"

2009-12-28T05:17:00.000-08:00

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

2009-12-24T01:34:00.000-08:00

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

2009-12-22T21:45:00.000-08:00

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

2009-12-22T05:53:00.000-08:00

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

2009-12-21T00:59:00.000-08:00

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

2009-12-18T20:15:00.000-08:00

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

2009-12-16T21:38:00.000-08:00

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.