Friday, March 18, 2011

Kennedy Employees Form Human Shuttle


Thousands of NASA Kennedy Space Center employees stand side-by-side to form a full-scale outline of a space shuttle orbiter outside the Vehicle Assembly Building. The unique photo opportunity was designed to honor the Space Shuttle Program's 30-year legacy and the people who contribute to safely processing, launching and landing the vehicle.

For more information visit http://www.nasa.gov/multimedia/imagegallery/image_feature_1899.html

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Thursday, March 17, 2011

Madrid Event Marks Spain's Role in Next Mars Mission


Spain is providing a key science instrument and the high-gain antenna communication subsystem for NASA's Mars Science Laboratory mission, on track for launch this year.

At a small ceremony held March 17, 2011, in Madrid, representatives of the United States and Spain signed an agreement for cooperation on the mission. Signers included Alan D. Solomont, U.S. ambassador to Spain; Arturo Azcorra, director general of Spain's Center for the Development of Industrial Technology; and Jaime Denis, director general of Spain's National Institute for Aerospace Technology. Spain's Minister of Defense Carme Chacon Piqueras and Minister of Science and Innovation Cristina Garmendia Mendizabal were also present.

The Mars Science Laboratory instrument provided by Spain is the Remote Environmental Monitoring Station, which will measure daily and seasonal changes in weather using sensors on the mast, on the deck and inside the mission's rover. The rover's high-gain antenna will send and receive communications directly between the rover and Earth, using X-band radio transmissions.

The mission's rover, named Curiosity, is currently in vacuum-chamber testing at NASA's Jet Propulsion Laboratory, Pasadena, Calif., where it is being built and tested. This is part of preparation for launch during the period Nov. 25 to Dec. 18, 2011, and landing on Mars in August 2012. Its 10 science investigations will assess the modern environment of the landing area and clues about environments billions of years ago.

JPL, a division of the California Institute of Technology in Pasadena, manages the Mars Science Laboratory mission for the NASA Science Mission Directorate, Washington.

For more information visit http://www.nasa.gov/mission_pages/msl/news/msl20110317.html

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Wednesday, March 16, 2011

NASA Picks a Festive Clover of Ireland Images


March 17 marks St. Patrick's Day —a day when shamrocks, Ireland and "wearing of the green" are especially en vogue. To celebrate this festive occasion, NASA's Aqua satellite has picked a clover of different views of the Emerald Isle, Ireland.

The collection of images acquired by Aqua's Atmospheric Infrared Sounder (AIRS) instrument on March 3, 2011, includes near-infrared/visible, infrared and microwave light views of the land where St. Patrick's Day originated.

The AIRS instrument measures temperatures of land, sea and air to provide a better understanding of what is happening in those environments.

The clover of AIRS images reveal temperatures near Earth's surface that were near normal for this time of year. The visible image showed a mostly cloud-free country blanketed by an approaching cold front. The infrared image showed low western clouds associated with a cold front moving east. The microwave brightness temperature data are a bit colder than the infrared temperature data, 273 Kelvin, which is just at the freezing point of water (0 degrees Celsius, or 32 degrees Fahrenheit).

AIRS observes and records the global daily distribution of temperature, water vapor, clouds and several atmospheric gases, including ozone, methane and carbon monoxide.

For more information visit http://www.jpl.nasa.gov/news/news.cfm?release=2011-083

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Tuesday, March 15, 2011

Chasma Boreale, Mars


Chasma Boreale, a long, flat-floored valley, cuts deep into Mars' north polar icecap. Its walls rise about 4,600 feet, or 1,400 meters, above the floor. Where the edge of the ice cap has retreated, sheets of sand are emerging that accumulated during earlier ice-free climatic cycles. Winds blowing off the ice have pushed loose sand into dunes and driven them down-canyon in a westward direction.

This scene combines images taken during the period from December 2002 to February 2005 by the Thermal Emission Imaging System instrument on NASA's Mars Odyssey was part of a special series of images marking the orbiter as the longest-working Mars spacecraft in history.

For more information visit http://www.nasa.gov/multimedia/imagegallery/image_feature_1894.html

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Monday, March 14, 2011

Legendary Fire Trainer Retires After 42 Years

George Hoggard had an extraordinary career by most standards, so it wasn't easy for him to say goodbye to the fire department at NASA's Kennedy Space Center.

"People who don't know anything about the space program cannot imagine how exciting it is to work out here," Hoggard said. "The very idea of it lasting 30 years never dawned on me and I never did have any retirement plans because working out here is so much fun. Quite frankly, I'm thinking, 'Why would I want to leave this?'"

As the chief of fire training, Hoggard and his crew worked closely with astronauts to teach them how to handle emergencies on the launch pad or on the ground following a problem. He showed them where to go once they left the shuttle cockpit, such as when to take the elevator and when to go straight to the slidewire basket. He and then-astronaut Charlie Bolden took a ride in one of the baskets in the late 1980s to prove they were safe.

It might look like it would be a thrill ride, sitting inside a basket riding a cable from 195 feet above the launch pad, but Hoggard said it was a very straightforward event.

"Back in those days," Hoggard said, "if you went to Disney World you had to pay a little bit more money for the e-tickets because they were the more exciting rides and when they asked me how the basket ride was, I said, 'If I went to Disney World with my granddaughter and took that ride and had to use an e-ticket, I'd ask for my money back because it wasn't that exciting, it was kind of dull."

Bolden, returning as NASA administrator, gave Hoggard a commemorative medallion during his retirement party the day before space shuttle Discovery lifted off on its final flight, the STS-133 mission.

Hoggard's skill and dedication came across to the astronauts very easily and made the firefighter a true legend at Kennedy, Shuttle Launch Director Mike Leinbach said.

"The astronauts know they can trust him with their lives, and that says an enormous amount about his experience, heart and wisdom," Leinbach said.

It's a far different existence than Hoggard thought he would have. After getting out of the Marines, Hoggard thought he'd go into the family business: law enforcement. His father and brother were both policemen, and Hoggard joined the force. He was assigned to the vice squad and during the next year had some close calls, including getting stabbed and shot at.

"At the end of the year I told my dad, 'Hey, I know you wanted me to be a cop, but I've got to go find a safer job, I don't like being a cop,'" Hoggard said. "Luckily for me he was friends with a fire chief and got me a job on a really good department and he said, 'This is the safest job I can get you,' and I've been a fireman ever since."

Working as a firefighter in southeastern Virginia, Hoggard's career turned again after a friend of his told him about the construction under way on NASA's Kennedy Space Center.

"Quite frankly, I had been on the department up there for eight or nine years and I was tired of freezing on the tail board of a fire engine on Chesapeake Bay in the winter time with the sleet blowing in my face," Hoggard said. "I said, 'If I'm going to continue in this job, I'm going to a warmer climate.'"

Hoggard's firefighting career at Kennedy began with a level of excitement that would become the norm.

"I was really new out here and got to go out to the fire training area and they said three astronauts were going to show up and I didn't know who they were," Hoggard said. "They did everything we asked them to do with extinguishers and the hose and the masks and stuff, part of the training. And they left and I had no idea who they were and six months later they stepped on the moon . . . it was the Apollo 11 crew."

"When the shuttle started up we kind of had to sort of reinvent everything because there wasn't going to be just three astronauts, there were going to be as many as seven astronauts in there," Hoggard said. "It was going to be a completely different ball game so the preparation and planning and training for that was real exciting."

Hoggard and his team taught the astronauts before each launch how to drive the yellow M113 armored personnel carriers. The lessons would be critical if there was an emergency and the crew had to drive out of harm's way.

"I tell the astronauts the shuttle cockpit's got over 2,000 switches, this one's only got two, on and off, and it's easy as it can be," Hoggard said. "If you can drive a tractor and plow a field, you can drive an M113."

Hoggard still has a rule, though: "They said is there a pass/fail to this driving test and I said, 'Yeah, if you hurt the old guy, you're going to fail the test, that's the bottom line, don't hurt the old guy.' "

That approach also was on display when Hoggard was training Leinbach years ago when he and other NASA test directors were learning about rescue procedures.

"One day we went out to their fire training area for rappelling training," Leinbach said. "During my first rappel, George was on the belay line. About halfway down the side of the 50-foot building he cinched up on the rope and I slammed into the concrete wall and hung there until he let up on the rope. I’ll never forget it. I was hanging there and he was on the ground laughing. After what seemed like an eternity, he let me down and we just laughed and laughed until we almost cried."

Hoggard saw different perspectives of NASA when he conducted training classes at the agency's other field centers.

"They ask, 'Have you seen a launch?' And I'm like, 'Yeah, I don't close my eyes,'" he said. "Then they asked, 'Well, what's that like?' Then it dawned on me, there are thousands of people who work for NASA and NASA contractors who have never seen a launch and I've seen many of them and that's just kind of amazing. It's a shame that everybody can't be in the position that I am here at Kennedy."

For more information visit http://www.nasa.gov/mission_pages/shuttle/behindscenes/hoggardprofile.html

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Sunday, March 13, 2011

NASA Images Tsunami's Effects on Northeastern Japan


The extent of inundation from the destructive and deadly tsunami triggered by the March 11, 2011, magnitude 8.9 earthquake centered off Japan's northeastern coast about 130 kilometers (82 miles) east of the city of Sendai is revealed in this before-and-after image pair from the Multi-angle Imaging SpectroRadiometer (MISR) instrument on NASA's Terra spacecraft.

The image comparison is online at http://photojournal.jpl.nasa.gov/catalog/PIA13913 . For optimum viewing, click the link to open the full-resolution TIFF image.

The new image, shown on the right, was acquired at 10:30 a.m. local time (01:30 UTC) on March 12, 2011. For comparison, shown on the left is a MISR image from about 10 years ago, on March 16, 2001, acquired under nearly identical illumination conditions. Flooding extending more than 4 kilometers (2.5 miles) inland from the eastern shoreline is visible in the post-earthquake image. The white sand beaches visible in the pre-earthquake view are now covered by water and can no longer be seen. Among the locations where severe flooding is visible is the area around Matsukawa-ura Bay, located just north and east of the image center.

From top to bottom, each image extends from just north of the Abukuma River (about 21 kilometers, or 13 miles, south of Sendai) to south of the town of Minamisoma (population 71,000, located in Japan's Fukushima Prefecture about 70 kilometers, or 44 miles, south of Sendai). The images cover an area of 78 kilometers (48 miles) by 104 kilometers (65 miles).

These unique images enhance the presence of water in two ways. First, their near-infrared observations cause vegetated areas to appear red, which contrasts strongly with the blue shades of the water. Second, by combining nadir (vertical-viewing) imagery with observations acquired at a view angle of 26 degrees, reflected sunglint enhances the brightness of water, which is shown in shades of blue. This use of different view-angle observations causes a stereoscopic effect, where elevated clouds have a yellow tinge at their top edges and blue tinge at their bottom edges.

For more information visit http://www.nasa.gov/topics/earth/features/japanquake/misr20110312.html

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Thursday, March 10, 2011

MESSENGER Poised for Mercury Orbit Insertion


After more than a dozen laps through the inner solar system, NASA's MESSENGER spacecraft will move into orbit around Mercury on March 17, 2011. The durable spacecraft--carrying seven science instruments and fortified against the blistering environs near the sun--will be the first to orbit the innermost planet.

At 8:45 p.m. EDT, MESSENGER--having pointed its largest thruster very close to the direction of travel--will fire that thruster for nearly 14 minutes, with other thrusters firing for an additional minute, slowing the spacecraft by 862 meters per second (1,929 mph) and consuming 31 percent of the propellant that the spacecraft carried at launch. Less than 9.5 percent of the usable propellant at the start of the mission will remain after completing the orbit insertion maneuver, but the spacecraft will still have plenty of propellant for future orbit correction maneuvers.

The orbit insertion will place the spacecraft into a 12-hour orbit about Mercury with a 200 kilometer (124 mile) minimum altitude. At the time of orbit insertion, MESSENGER will be 46.14 million kilometers (28.67 million miles) from the sun and 155.06 million kilometers (96.35 million miles) from Earth.

MESSENGER has been on a six-year mission to become the first spacecraft to orbit Mercury. The spacecraft followed a path through the inner solar system, including one flyby of Earth, two flybys of Venus, and three flybys of Mercury. This impressive journey is returning the first new spacecraft data from Mercury since the Mariner 10 mission over 30 years ago.

On March 7, antennas from each of the three Deep Space Network (DSN) ground stations began continuous monitoring, allowing flight control engineers at the Johns Hopkins University Applied Physics Laboratory to observe MESSENGER on its final approach to Mercury. The spacecraft also began executing the last cruise command sequence of the mission, when the command sequence containing the orbit-insertion burn will start.

"This is a milestone event for our small, but highly experienced, operations team, marking the end of six and one half years of successfully shepherding the spacecraft through six planetary flybys, five major propulsive maneuvers, and sixteen trajectory-correction maneuvers, all while simultaneously preparing for orbit injection and primary mission operations," said MESSENGER Systems Engineer Eric Finnegan. "Whatever the future holds, this team of highly dedicated engineers (http://messenger.jhuapl.edu/moc/index.html) has done a phenomenal job methodically generating, testing, and verifying commands to the spacecraft, getting MESSENGER where it is today."

"The cruise phase of the MESSENGER mission has reached the end game," adds MESSENGER Principal investigator Sean Solomon, of the Carnegie Institution of Washington. "Orbit insertion is the last hurdle to a new game level, operation of the first spacecraft in orbit about the solar system's innermost planet. The MESSENGER team is ready and eager for orbital operations to begin."

For more information visit http://www.nasa.gov/mission_pages/messenger/media/MESSENGERPoisedInsertion.html

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Wednesday, March 9, 2011

Color View from Orbit Shows Mars Rover Beside Crater


NASA's Mars Exploration Rover Opportunity has nearly completed its three-month examination of a crater informally named "Santa Maria," but before the rover resumes its overland trek, an orbiting camera has provided a color image of Opportunity beside Santa Maria.

The High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter acquired the image on March 1, while Opportunity was extending its robotic arm to take close-up photos of a rock called "Ruiz Garcia." From orbit, the tracks Opportunity made as it approached the crater from the west are clearly visible. Santa Maria crater is about 90 meters (295 feet) in diameter.

Opportunity completed its three-month prime mission on Mars in April 2004 and has been working in bonus extended missions since then. The Mars Reconnaissance Orbiter, which arrived at Mars on March 10, 2006, has also completed its prime mission and is operating in an extended mission.

The High Resolution Imaging Science Experiment is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter and the Mars Exploration Rover projects for NASA's Science Mission Directorate, Washington, and built Opportunity and its twin rover, Spirit. Lockheed Martin Space Systems, Denver, is NASA's industry partner for the Mars Reconnaissance Orbiter project and built that spacecraft.

For more information visit http://www.nasa.gov/mission_pages/MRO/news/mro20110309.html

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Tuesday, March 8, 2011

James Webb Space Telescope's "Chassis" Gets Taken Out for a Spin at NASA


The Integrated Science Instrument Module, or ISIM, is the structural heart of the James Webb Space Telescope, what engineers call the main payload. It will house the four main scientific instruments of the telescope. The ISIM is like a chassis in a car providing support for the engine and other components.

Webb will undergo significant shaking when it is launched on the large Ariane V rocket. To be sure the telescope's "chassis" is ready for this "bumpy road," the ISIM is subjected to some extreme testing. During the testing process, the ISIM is spun and shaken while many measurements are taken. Afterwards, engineers compare the measurements with their models of the ISIM. If there are discrepancies, then the engineers track down why, and make corrections.

Webb will be the first next-generation large space observatory and will serve thousands of astronomers worldwide. Designed to detect light from as far away as approximately 14 billion light years, Webb will study every phase in the history of our Universe, ranging from the first luminous glows after the Big Bang, to the formation of planetary systems capable of supporting life on planets like Earth, to the evolution of our own Solar System. The Webb telescope is a joint mission of NASA, the European Space Agency and Canadian Space Agency.

For more information visit http://www.nasa.gov/topics/technology/features/isim-spin.html

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Monday, March 7, 2011

NASA Creates Glory Satellite Mishap Investigation Board

NASA's Glory mission ended Friday after the spacecraft failed to reach orbit following its launch from Vandenberg Air Force Base in California.

NASA has begun the process of creating a Mishap Investigation Board to evaluate the cause of the failure. Telemetry indicated the fairing, a protective shell atop the satellite's Taurus XL rocket, did not separate as expected.

The launch proceeded as planned from its liftoff at 5:09 a.m. EST through the ignition of the Taurus XL's second stage. However, the fairing failure occurred during the second stage engine burn. It is likely the spacecraft fell into the South Pacific, although the exact location is not yet known.

NASA's previous launch attempt of an Earth science spacecraft, the Orbiting Carbon Observatory onboard a Taurus XL on Feb. 24, 2009, also failed to reach orbit when the fairing did not separate.

NASA's Orbiting Carbon Observatory Mishap Investigation Board reviewed launch data and the fairing separation system design, and developed a corrective action plan. The plan was implemented by Taurus XL manufacturer Orbital Sciences Corporation. In October 2010, NASA's Flight Planning Board confirmed the successful closure of the corrective actions.

The Glory Earth-observing satellite was intended to improve our understanding of how the sun and tiny atmospheric particles called aerosols affect Earth's climate.

For more information visit http://www.nasa.gov/home/hqnews/2011/mar/HQ_11-065_Glory_Board.html

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Sunday, March 6, 2011

Anchored


Anchored to a Canadarm2 mobile foot restraint, NASA astronaut Steve Bowen participates in the STS-133 mission's second spacewalk as construction and maintenance continue on the International Space Station. During the six-hour, 14-minute spacewalk, Bowen and fellow astronaut Alvin Drew tackled a variety of tasks, including venting into space some remaining ammonia from a failed pump module they moved during the mission's first spacewalk.

For more information visit http://www.nasa.gov/multimedia/imagegallery/image_feature_1886.html

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Friday, March 4, 2011

NASA Develops Light Microscope For International Space Station

NASA began testing a new multi-capability microscope this week on the International Space Station. It will help scientists study the effects of the space environment on physics and biology aboard the orbiting laboratory. The microscope is isolated from vibrations on the station, allowing it to obtain clear, high-resolution images. Using high-resolution magnification, scientists can examine microorganisms and individual cells of plants and animals, including humans.

The microscope will allow real-time study of the effects of the space environment without the need to return samples to Earth. Any living specimens returned to Earth must endure the effects of re-entry through the atmosphere. The ability to use the Light Microscopy Module (LMM) on station will enable scientists to study data unaffected by re-entry.

"We really need to maximize life science investigations conducted on the International Space Station," said Jacob Cohen, principal investigator of the technology demonstration and a researcher at NASA's Ames Research Center, Moffett Field, Calif. "It's really amazing to be able to remotely manage, optimize and troubleshoot experiments observed with a microscope in space without the need to return the samples back to Earth. This microscope is helping fulfill the vision of a true laboratory in space."

The biological samples for the LMM launched on space shuttle Discovery's STS-133 mission on Feb. 24. They include eight fixed slides containing yeast; bacteria; a leaf; a fly; a butterfly wing; tissue sections and blood; six containers of live C. elegans worms, an organism biologists commonly study; a typed letter "r" and a piece of fluorescent plastic. The wing is from a previous study, Butterflies in Space, involving students from around the country, and flown on STS-129 in 2009. Some of the worms are descendants of those that survived the space shuttle Columbia (STS-107) accident; and others are modified to fluoresce. Scientists commonly attach green, yellow and red florescent proteins to study gene expression.

"Operating the LMM on the space station has been a goal of NASA's Life and Physical Sciences Program for many years," said Ron Sicker, LMM project manager at NASA's Glenn Research Center in Cleveland. "Scientists and engineers at Glenn modified the commercial microscope in the LMM with 23 micro motors and cameras to allow remote control operations."

Cohen and Sicker expect the LMM to perform the same as a microscope on Earth. In the future, the microscope could be used to assist in maintenance of station crew health, advance our knowledge of the effects of space on biology and contribute to the development of applications for space exploration and on Earth. This technology demonstration was developed by Ames and Glenn, which developed and manages the LMM. The Advanced Capabilities Division in the Exploration Systems Mission Directorate at NASA Headquarters in Washington, funds the project.

"This is a facility to support research in both physical and life sciences by NASA-funded and National Laboratory users," said Julie Robinson, International Space Station Program scientist at NASA's Johnson Space Center in Houston. "It gives us a capability not available before that allows more types of research to be done."

For more information visit http://www.nasa.gov/home/hqnews/2011/mar/HQ_11-063_Light_Scope.html

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Thursday, March 3, 2011

National Inventors Hall of Fame Taps Former JPL Engineer


The National Inventors Hall of Fame is inducting former JPL physicist and engineer Eric Fossum, who led a team that invented a semiconductor active pixel image sensor that is widely used in cell phone cameras, webcams, digital still cameras, medical imaging and other applications. Fossum is now an engineering professor at Dartmouth College, Hanover, N.H.

The image sensor chip was created at JPL in the early 1990s. Fossum and his team discovered it while researching ways to drastically reduce the size of cameras on interplanetary spacecraft while maintaining the scientific image quality.

The result was the invention of the CMOS active-pixel sensor (CMOS-APS), which consolidates various functions of the prevalent image sensor of the time, but with one-hundredth of the power of its predecessors and with the ability to make its own conversion from analog to digital for output on computer monitors. Fossum soon realized that the CMOS-APS technology would be useful not only for space exploration, but here on Earth as well.

In 1995, Fossum and a group of JPL engineers founded Photobit, in Pasadena. Photobit exclusively licensed the CMOS-APS technology from JPL, becoming the first company to commercialize CMOS image sensors.

NASA's Jet Propulsion Laboratory is managed by the California Institute of Technology in Pasadena.

For more information visit http://www.jpl.nasa.gov/news/news.cfm?release=2011-065

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Wednesday, March 2, 2011

NASA Nanosatellite Celebrates 100 Days In Space Studying Life


More than one hundred days ago, on Nov. 19, 2010, NASA sent a small satellite about the size of a loaf of bread on an important mission to answer astrobiology’s fundamental questions about the origin, evolution and distribution of life in the universe.

Since then, the nanosatellite, known as Organism/Organic Exposure to Orbital Stresses (O/OREOS) continues on its quest, which has taken it just about everywhere between the Arctic and Antarctic Circles more than 400 miles above Earth's surface.

O/OREOS weighs approximately 12 pounds and is NASA’s first CubeSat to demonstrate the capability to have two distinct, completely independent science experiments on a single autonomous satellite. O/OREOS is using NASA’s first propellant-less mechanism on a scientific satellite to ensure it de-orbits and burns up as it re-enters Earth’s atmosphere, less than 25 years after completing its mission. It's also the first nanosatellite to not only operate, but also conduct autonomous biological and chemical measurements, in the region of space known as the exosphere.

"The fact that we're getting consistently good science data in such a challenging environment tells us that secondary payload nanosatellites like O/OREOS can be made rugged enough to enhance our opportunities to conduct research in low Earth orbit," said Antonio Ricco, instrument scientist for O/OREOS and a researcher at NASA's Ames Research Center, Moffett Field, Calif. "This is enabling us to study organics, microorganisms, and astrobiology in the space environment in real time."

O/OREOS was a secondary payload aboard a U.S. Air Force four-stage Minotaur IV rocket launched from the Alaska Aerospace Corporation’s Kodiak Launch Complex on Kodiak Island, Alaska. After O/OREOS separated from the rocket and successfully entered low Earth orbit, it activated and began transmitting radio signals to ground control stations and spacecraft operators in the mission control center at Santa Clara University, Santa Clara, Calif. Nearly daily two-way communications with the spacecraft provided valuable information about its health, status and science data, and have given scientists the ability to fine tune the science payloads’ operating parameters.

On Dec. 3, 2010, two weeks after O/OREOS deployed, the first of three biological experiments began operating automatically within the Space Environment Survivability of Living Organisms (SESLO) payload; and was successfully completed just 24 hours later. On Feb. 18, 2011, the second part of the SESLO biological experiment began and also was successfully finished in one day. The experiment is designed to characterize the growth, activity, health and ability of microorganisms commonly found in soil and salt ponds in a dried and dormant state - Bacillus subtilis and Halorubrum chaoviatoris – to adapt to the stresses of outer space by rehydrating, or “feeding,” and growing them using dyed liquid nutrients. Scientists will compare the microbes' population density and change in color at three different times during the mission to determine how and if their behavior changes with longer exposure to radiation and weightless conditions in space.

"Days before the second part of the SESLO experiment began, a large solar flare sent radiation, including energetic protons and X-rays, hurtling towards O/OREOS and Earth, yet O/OREOS still successfully completed the experiment and got some promising results that we're now evaluating," said Ricco.

Hours after reaching orbit, O/OREOS activated its other science experiment payload, called the Space Environment Viability of Organics (SEVO), which monitors the stability and changes in four classes of biologically important organic molecules as they are exposed to space conditions, most notably sunlight completely unfiltered by Earth’s atmosphere. For the SEVO experiment, scientists selected organic molecules distributed throughout our galaxy, as well as organic “biomarkers” of life as we know it on Earth. O/OREOS houses the organic samples in “micro-environments” relevant to space and planetary conditions. The experiment exposes the organic compounds to solar ultraviolet (UV) light, visible light, trapped-particle and cosmic radiation. Scientists will determine the stability of the molecules by studying changes in UV, visible, and near-infrared light absorption.

"Using the sun as its light source, O/OREOS has made nearly 500 periodic spectral measurements of the organic materials, and 200 of those have been transmitted to us so far," said Pascale Ehrenfreund, O/OREOS project scientist at George Washington University, Washington, D.C. "We are excited to see the payload's miniature spectrometer and sample positioning systems working so well and are grateful to our operations team at Santa Clara University."

The Small Spacecraft Division at Ames manages the O/OREOS payload and mission operations with the professional support of staff and students from Santa Clara University.

As with NASA's previous small satellite missions, such as the GeneSat-1 and PharmaSat, Santa Clara University invites amateur radio operators around the world to tune in to the satellite's broadcast. To date, more than 70,000 beacon data packets have been collected and provided via the Internet to the O/OREOS mission operations team by HAM operators in 19 nations.

For more information visit http://www.nasa.gov/centers/ames/news/features/2011/o-oreos_100_days.html

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NASA has announced program office assignments at three NASA field centers to align the president's fiscal year 2012 budget request and the NASA Authorization Act of 2010. The agency also has released three Space Technology Program solicitations.
NASA will create new program offices to manage human spaceflight activities associated with the development of the Space Launch System, the heavy-lift rocket that will carry humans beyond low Earth orbit; the Multi-Purpose Crew Vehicle, the next human exploration spacecraft; and commercial spaceflight vehicles.

"NASA is moving forward to aggressively implement the bi-partisan direction the President and Congress have given us, and these program offices will help us carry out this important mission," NASA Administrator Charles Bolden said. "The United States continues its leadership role in human spaceflight and these moves will ensure this continues for many years to come."

NASA's Johnson Space Center in Houston will host a program office responsible for developing the Multi-Purpose Crew Vehicle. Johnson also will continue to lead the way in human research to enable exploration beyond low Earth orbit. This research heavily leverages the International Space Station. In addition, the center will be critical to efforts to facilitate commercial access to low Earth orbit.

NASA's Kennedy Space Center in Florida will lead the way in enabling commercial human spaceflight capabilities and host a program office dedicated to that work. Kennedy will continue to provide launch services to both science missions and commercial crew providers.
The Marshall Space Flight Center in Huntsville, Ala., will lead NASA's efforts on a heavy- lift rocket that will carry humans beyond low Earth orbit. The center will house the program office for the Space Launch System and continue to support station operations.

NASA also released three Space Technology Program solicitations Tuesday as part of the agency's efforts to develop innovative solutions to enable future exploration and science missions and lower the cost of other government and commercial space activities.

"These solicitations for innovative research and technology development, from their earliest stages through maturation and testing in flight, will provide new knowledge and capabilities for our future missions," NASA Deputy Administrator Lori Garver said. "Technological leadership is how the United States is going to out-innovate, out-educate and out-build the rest of the world."

The NASA Innovative Advanced Concepts program seeks transformative ideas to enable new aeronautics and space systems capabilities. NASA's Game Changing Development Program is soliciting proposals for research and technology development for revolutionary improvements in America's space capabilities. NASA also is seeking Technology Demonstration Mission proposals in four areas: high-bandwidth deep space communication, navigation and timing; orbital debris mitigation or removal systems; advanced in-space propulsion systems; and autonomous rendezvous, docking, close proximity operations and formation flying.

The programs are managed by NASA's Office of the Chief Technologist consistent with provisions of the Authorization Act of 2010. NASA seeks proposals for all three solicitations that align with the agency's Space Technology Roadmaps and NASA's Grand Challenges. Awards are contingent on availability of fiscal year 2011 appropriations.

For more information visit http://www.nasa.gov/home/hqnews/2011/mar/HQ_11-057_Program_Offices.html

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