Friday, October 31, 2008

NASA to Hold Small Business Symposium

NASA will host the inaugural Small Business Symposium and Awards Ceremony Nov. 17-18 in Washington at the Hilton Washington, 1919 Connecticut Ave., NW. Participation in this symposium is open to industry, academia and domestic small businesses. The deadline to register for the symposium is Nov. 3.

The Business Opportunities Office at NASA's Jet Propulsion Laboratory in Pasadena, Calif., and NASA's Office of Small Business Programs at NASA Headquarters in Washington are hosting the event.

Attendees will have the opportunity to network with NASA and its prime contractors and learn how to do business with the agency. NASA representatives will discuss plans for future Earth and space missions as well as other agency programs, initiatives, and business opportunities. NASA will provide information about the skills, resources and technologies needed to achieve NASA's missions, programs and research.

Topics at this two-day event include information about NASA's Mentor-Protege Program, how NASA's Small Business Program works, how to reach NASA's prime contractors for subcontracting opportunities, and how small businesses can build a high-tech industrial base.

NASA's Small Business Industry and Advocate awards will be presented on the symposium's second day. The awards recognize outstanding contributions made by NASA employees and industry representatives to support the agency's small business program.

To register for the symposium, visit http://acquisition.jpl.nasa.gov/boo/2008sbsym/index.asp . For more information about the NASA-JPL Small Business Symposium, contact Andrea Acosta at andrea.e.acosta@jpl.nasa.gov or 818-354-7531.

More information about NASA's Office of Small Business Programs is at: http://www.osbp.nasa.gov . More information about JPL's Business Opportunities Office is at: http://acquisition.jpl.nasa.gov/boo .

JPL is managed for NASA by the California Institute of Technology in Pasadena.

Spooky Creatures on the Prowl

The Cassini-Huygens team sends "best witches" for a happy, healthy and fun Halloween. Cassini's first four years at Saturn have bedazzled with stunning images and exciting results. With the start of the Equinox mission, the team promises to scare up many more treats as they continue studying the eerie glow of Saturn's rings, the spine-tingling thunder on the planet, the hair-raising jets on Enceladus, and the murky brew on Titan. A full view of their ghostly Saturn can be seen at
http://saturn.jpl.nasa.gov/multimedia/images/image-details.cfm?imageID=3293

Closer to home, ghoulish phantoms appear to haunt Earth's middle atmosphere in this enhanced depiction of water vapor derived from an animation of NASA Aqua Atmospheric Infrared Sounder data. To watch the animation, go to
http://airs.jpl.nasa.gov/story_archive/Ghostly_Images_in_Earths_Water_Vapor/

For some eerie sounds, visit our spooky sounds from space at
http://www.jpl.nasa.gov/multimedia/sounds2/index-flash.html .

Thursday, October 30, 2008

NASA Phoenix Mission Status Report

NASA'S Phoenix Mars Lander entered safe mode late yesterday in response to a low-power fault brought on by deteriorating weather conditions. While engineers anticipated that a fault could occur due to the diminishing power supply, the lander also unexpectedly switched to the "B" side of its redundant electronics and shut down one of its two batteries.

During safe mode, the lander stops non-critical activities and awaits further instructions from the mission team. Within hours of receiving information of the safing event, mission engineers at NASA's Jet Propulsion Laboratory, Pasadena, Calif., and at Lockheed Martin in Denver, were able to send commands to restart battery charging. It is not likely that any energy was lost.

Weather conditions at the landing site in the north polar region of Mars have deteriorated in recent days, with overnight temperatures falling to -141F (-96C), and daytime temperatures only as high as -50F (-45C), the lowest temperatures experienced so far in the mission. A mild dust storm blowing through the area, along with water-ice clouds, further complicated the situation by reducing the amount of sunlight reaching the lander's solar arrays, thereby reducing the amount of power it could generate. Low temperatures caused the lander's battery heaters to turn on Tuesday for the first time, creating another drain on precious power supplies.

Science activities will remain on hold for the next several days to allow the spacecraft to recharge and conserve power. Attempts to resume normal operations will not take place before the weekend.

"This is a precarious time for Phoenix," said Phoenix Project Manager Barry Goldstein of JPL. "We're in the bonus round of the extended mission, and we're aware that the end could come at any time. The engineering team is doing all it can to keep the spacecraft alive and collecting science, but at this point survivability depends on some factors out of our control, such as the weather and temperatures on Mars."

The ability to communicate with the spacecraft has not been impacted. However, the team decided to cancel communication sessions Wednesday morning in order to conserve spacecraft power. The next communication pass is anticipated at 9:30 p.m. PDT Wednesday.

Yesterday, the mission announced plans to turn off four heaters, one at a time, in an effort to preserve power. The faults experienced late Tuesday prompted engineers to command the lander to shut down two heaters instead of one as originally planned. One of those heaters warmed electronics for Phoenix's robotic arm, robotic-arm camera, and thermal and evolved-gas analyzer (TEGA), an instrument that bakes and sniffs Martian soil to assess volatile ingredients. The second heater served the lander's pyrotechnic initiation unit, which hasn't been used since landing. By turning off selected heaters, the mission hopes to preserve power and prolong the use of the lander's camera and meteorological instruments.

Originally scheduled to last 90 days, Phoenix has completed a fifth month of exploration in the Martian arctic. As the Martian northern hemisphere shifts from summer to autumn, the lander was expected to generate less power due to fewer hours of sunlight reaching its solar panels. "It could be a matter of days, or weeks, before the daily power generated by Phoenix is less than needed to operate the spacecraft," said JPL mission manager Chris Lewicki. "We have only a few options left to reduce the energy usage."

The Phoenix mission is led by Peter Smith of the University of Arizona, Tucson, with project management at the Jet Propulsion Laboratory and development partnership at Lockheed Martin, Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus in Denmark; the Max Planck Institute in Germany; and the Finnish Meteorological Institute. The California Institute of Technology in Pasadena manages JPL for NASA.

NASA TV PROVIDES HD FEED OF DOCUMENTARY ON NASA'S FIRST 50 YEARS

NASA Television will provide a high definition feed of the documentary "50 Years of Exploration: The Golden Anniversary of NASA" on Thursday, Oct. 30, at 1 and 8 p.m. EDT.

Hosted by Neil Armstrong, the 90-minute documentary features film and video highlights of the agency's first half-century, as well as the insights and perspectives of astronauts, scientists, engineers and others whose contributions have helped shepherd America's space program.

Among the interviewees are former NASA astronaut and U.S. Senator John Glenn, Apollo Flight Director Gene Kranz, author Ray Bradbury, NASA scientist and Nobel Prize winner John Mather, and presidents George H.W. Bush and Bill Clinton.

"50 Years of Exploration: The Golden Anniversary of NASA" is a production of NASA Television. It will be re-fed on Friday, Oct. 31, at 10 a.m. and 2 p.m.

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

http://www.nasa.gov/ntv

NASA TO DISCUSS STATUS OF HUBBLE SERVICING MISSION THURSDAY

NASA will host a media teleconference at 5 p.m. EDT on Thursday, Oct. 30, to discuss the status of the upcoming shuttle servicing mission to the Hubble Space Telescope. The fifth and final "house call" by astronauts to the telescope originally was planned for Oct. 10 but was postponed due to an onboard computer anomaly.

The briefing participants are:
- Jon Morse, director of the Astrophysics Division in NASA's Science Mission Directorate at NASA Headquarters in Washington
- Preston Burch, Hubble Space Telescope manager at NASA's Goddard Space Flight Center in Greenbelt, Md.

To participate in the teleconference, reporters in the U.S. should call 1-888-469-0494 and use the passcode "Hubble." International reporters should call 1-415-228-3905.

Approximately one hour after the briefing concludes, a recorded replay of the conference will be available by calling 1-888-458-8114. International callers can hear the replay by calling 1-402-998-1352.

Audio of the teleconference will be streamed live on the Internet at:

http://www.nasa.gov/newsaudio

MESSENGER SPACECRAFT REVEALS MORE HIDDEN TERRITORY ON MERCURY

A NASA spacecraft gliding over the battered surface of Mercury for the second time this year has revealed more previously unseen real estate on the innermost planet. The probe also has produced several science firsts and is returning hundreds of new photos and measurements of the planet's surface, atmosphere and magnetic field.

The MErcury Surface, Space ENvironment, GEochemistry, and Ranging, or MESSENGER, spacecraft flew by Mercury shortly after 4:40 a.m. EDT, on Oct. 6. It completed a critical gravity assist to keep it on course to orbit Mercury in 2011 and unveiled 30 percent of Mercury's surface never before seen by a spacecraft.

"The region of Mercury's surface that we viewed at close range for the first time this month is bigger than the land area of South America," said Sean Solomon, principal investigator and director of the Department of Terrestrial Magnetism at the Carnegie Institution of Washington. "When combined with data from our first flyby and from Mariner 10, our latest coverage means that we have now seen about 95 percent of the planet."

The spacecraft's science instruments operated throughout the flyby. Cameras snapped more than 1,200 pictures of the surface, while topography beneath the spacecraft was profiled with a laser altimeter. The comparison of magnetosphere observations from the spacecraft's first flyby in January with data from the probe's second pass has provided key new insight into the nature of Mercury's internal magnetic field and revealed new features of its magnetosphere. The magnetosphere is the volume surrounding Mercury that is controlled by the planet's magnetic field.

"The previous flybys by MESSENGER and Mariner 10 provided data only about Mercury's eastern hemisphere," explains Brian Anderson of the Johns Hopkins University Applied Physics Laboratory, known as APL, in Laurel, Md. "The most recent flyby gave us our first measurements on Mercury's western hemisphere, and with them we discovered that the
planet's magnetic field is highly symmetric."

The probe's Mercury Laser Altimeter, or MLA, measured the planet's topography, allowing scientists, for the first time, to correlate high-resolution topography measurements with high-resolution images.

"The MLA collected altimetry in regions where images from MESSENGER and Mariner 10 data are available, and new images were obtained of the region sampled by the altimeter in January," said Maria Zuber, co-investigator and head of the Department of Earth, Atmospheric, and Planetary Sciences at the Massachusetts Institute of Technology. "These topographic measurements now improve considerably the ability to interpret surface geology."

The Mercury Atmospheric and Surface Composition Spectrometer observed Mercury's thin atmosphere, known as an exosphere. The instrument searched for emissions from sodium, calcium, magnesium, and hydrogen atoms. Observations of magnesium are the first detection of this chemical in Mercury's exosphere. Preliminary analysis suggests that the spatial distributions of sodium, calcium, and magnesium are different. Simultaneous observations of these spatial distributions, also a first for the spacecraft, have opened an unprecedented window into the interaction of Mercury's surface and exosphere.

Spacecraft images also are revealing for the first time vast geologic differences on the surface.

"Now that MESSENGER's cameras have imaged more than 80 percent of Mercury, it is clear that, unlike the moon and Mars, Mercury's surface is more homogeneously ancient and heavily cratered, with large extents of younger volcanic plains lying within and between giant impact basins," said co-investigator Mark Robinson of Arizona State University in Tempe.

The project is the seventh in NASA's Discovery Program of lower-cost, scientifically focused missions. APL designed, built and operates the spacecraft and manages the mission for NASA's Science Mission Directorate in Washington. Science instruments were built by APL; NASA's Goddard Space Flight Center in Greenbelt, Md.; the University of Michigan, Ann Arbor; and the University of Colorado, Boulder. GenCorp Aerojet of Sacramento, Calif., and Composite Optics Inc. of San Diego, provided the propulsion system and composite structure.

For more information about the Mercury mission, visit:

www.nasa.gov/messenger

NASA MEASUREMENTS SHOW GREENHOUSE GAS METHANE ON THE RISE AGAIN

The amount of methane in Earth's atmosphere shot up in 2007, bringing to an end approximately a decade in which atmospheric levels of the potent greenhouse gas were essentially stable. The new study is based on data from a worldwide NASA-funded measurement network.

Methane levels in the atmosphere have more than tripled since pre-industrial times, accounting for around one-fifth of the human contribution to greenhouse gas-driven global warming. Until recently, the leveling off of methane levels had suggested that the rate of its emission from Earth's surface was being approximately balanced by the rate of its destruction in the atmosphere.

However, the balance has been upset since early 2007, according to research published this week in the American Geophysical Union's "Geophysical Review Letters." The paper's lead authors, Matthew Rigby and Ronald Prinn of the Massachusetts Institute of Technology, say this imbalance has resulted in several million metric tons of additional methane in the atmosphere.

Methane is produced by wetlands, rice paddies, cattle, and the gas and coal industries. It is destroyed in the atmosphere by reaction with the hydroxyl free radical, often referred to as the atmosphere's "cleanser."

"This increase in methane is worrisome because the recent stability of methane levels was helping to compensate for the unexpectedly fast growth of carbon dioxide emissions," said climate modeler Drew Shindell at NASA's Goddard Institute for Space Studies in New York.

"If methane continues to increase rapidly, we'll lose that offsetting effect. We will use NASA's climate modeling capability to improve our understanding of what is causing the increase and project future methane levels."

One surprising feature of this recent growth is that it occurred almost simultaneously at all measurement locations across the globe. However, the majority of methane emissions are in the Northern Hemisphere, and it takes more than one year for gases to be mixed between the hemispheres. Theoretical analysis of the measurements shows that if an increase in emissions is solely responsible, these emissions must have risen by a similar amount in both hemispheres at the same time.

The scientists analyzed air samples collected by the NASA-funded Advanced Global Atmospheric Gases Experiment ground network from 1997 through April 2008. The network was created in the 1970s in response to international concerns about chemicals depleting the ozone layer. It is supported by NASA as part of its congressional mandate to monitor ozone-depleting trace gases, many of which also are greenhouse gases. Air samples are collected and analyzed at several stations around the world.

According to the researchers, a rise in Northern Hemispheric emissions may be a result of very warm conditions over Siberia throughout 2007, potentially leading to increased bacterial emissions from wetland areas. However, a potential cause for an increase in Southern
Hemispheric emissions is less clear.

An alternative explanation for the rise may lie, at least in part, with a drop in the concentrations of the methane-destroying hydroxyl free radical. Theoretical studies show that if this has happened, the required global methane emissions rise would have been smaller and more strongly biased to the Northern Hemisphere. At present, however, it is uncertain whether such a drop in hydroxyl free radical concentrations did occur.

"The next step to pin down the cause of the methane increase will be to study this using a very high-resolution atmospheric circulation model and additional measurements from other networks," Prinn said. "The key is to determine more precisely the relative roles of increased methane emission versus a decrease in the rate of removal. Apparently we have a mix of the two, but we want to know how much of each is responsible for the overall increase."

It is too early to tell whether this increase represents a return to sustained methane growth, or the beginning of a relatively short-lived anomaly, according to Rigby and Prinn. Given that methane is about 25 times stronger as a greenhouse gas per metric ton of emissions than carbon dioxide, the situation will require careful monitoring in the near future to better understand methane's impact on future climate change.

For information about NASA and agency programs, visit:

http://www.nasa.gov

Wednesday, October 29, 2008

NASA Tests Rover Concepts in Arizona

NASA's newest lunar rover prototype has now gone farther than it ever has before.

A collection of engineers, astronauts and geologists have spent the past week testing out the Small Pressurized Rover in the 11th annual Desert RATS – or Research and Technology Studies -- field tests. Two teams of one astronaut and one geologist each have been driving the rover through the Arizona desert, trying it out in two different configurations.

One configuration leaves the crew members free to get on and off the rover whenever they like, but they must wear spacesuits at all times to protect them from the lunar environment. The second configuration -- called the Small Pressurized Rover, or SPR -- adds a module on top of the rover’s chassis that the crew can sit inside as they drive the vehicle, donning spacesuits whenever they want to get out.

For the first week of tests, the rover has been driven on day-long trips to determine how each configuration performed. These have been some of the longest drives the prototype has ever made, but next week the group will step it up another notch or two, by going on a three-day drive through the desert in the SPR to determine how it performs and whether it's comfortable enough for long-duration trips.

› NASA Edge Blog
› Download Analogs Fact Sheet (2.2 MB PDF)
› Download Small Pressurized Rover Fact Sheet (3.7 MB PDF)
› More on Analog Field Tests

NASA's Phoenix Mission Faces Survival Challenges

In a race against time and the elements, engineers with NASA's Phoenix Mars Lander mission hope to extend the lander's survival by gradually shutting down some of its instruments and heaters, starting today.

Originally scheduled to last 90 days, Phoenix has completed a fifth month of exploration in the Martian arctic. As expected, with the Martian northern hemisphere shifting from summer to fall, the lander is generating less power due to shorter days and fewer hours of sunlight reaching its solar panels. At the same time, the spacecraft requires more power to run several survival heaters that allow it to operate even as temperatures decline.

"If we did nothing, it wouldn't be long before the power needed to operate the spacecraft would exceed the amount of power it generates on a daily basis," said Phoenix Project Manager Barry Goldstein of NASA's Jet Propulsion Laboratory, Pasadena, Calif. "By turning off some heaters and instruments, we can extend the life of the lander by several weeks and still conduct some science."

Over the next several weeks, four survival heaters will be shut down, one at a time, in an effort to conserve power. The heaters serve the purpose of keeping the electronics within tested survivable limits. As each heater is disabled, some of the instruments are also expected to cease operations. The energy saved is intended to power the lander's main camera and meteorological instruments until the very end of the mission.

Later today, engineers will send commands to disable the first heater. That heater warms Phoenix's robotic arm, robotic-arm camera, and thermal and evolved-gas analyzer (TEGA), an instrument that bakes and sniffs Martian soil to assess volatile ingredients. Shutting down this heater is expected to save 250 watt-hours of power per Martian day.

The Phoenix team has parked the robotic arm on a representative patch of Martian soil. No additional soil samples will be gathered. The thermal and electrical-conductivity probe (TECP), located on the wrist of the arm, has been inserted into the soil and will continue to measure soil temperature and conductivity, along with atmospheric humidity near the surface. The probe does not need a heater to operate and should continue to send back data for weeks.

Throughout the mission, the lander's robotic arm successfully dug and scraped Martian soil and delivered it to the onboard laboratories. "We turn off this workhorse with the knowledge that it has far exceeded expectations and conducted every operation asked of it," said Ray Arvidson, the robotic arm's co-investigator, and a professor at Washington University, St. Louis.

When power levels necessitate further action, Phoenix engineers will disable a second heater, which serves the lander's pyrotechnic initiation unit. The unit hasn't been used since landing, and disabling its heater is expected to add four to five days to the mission's lifetime. Following that step, engineers would disable a third heater, which warms Phoenix's main camera -- the Surface Stereo Imager –and the meteorological suite of instruments. Electronics that operate the meteorological instruments should generate enough heat on their own to keep most of those instruments and the camera functioning.

In the final step, Phoenix engineers may turn off a fourth heater -- one of two survival heaters that warm the spacecraft and its batteries. This would leave one remaining survival heater to run out on its own.

"At that point, Phoenix will be at the mercy of Mars," said Chris Lewicki of JPL, lead mission manger.

Engineers are also preparing for solar conjunction, when the sun is directly between Earth and Mars. Between Nov. 28 and Dec. 13, Mars and the sun will be within two degrees of each other as seen from Earth, blocking radio transmission between the spacecraft and Earth. During that time, no commands will be sent to Phoenix, but daily downlinks from Phoenix will continue through NASA's Odyssey and Mars Reconnaissance orbiters. At this time, controllers can't predict whether the fourth heater would be disabled before or after conjunction.

The Phoenix mission is led by Peter Smith of the University of Arizona, Tucson, with project management at the Jet Propulsion Laboratory and development partnership at Lockheed Martin, Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus in Denmark; the Max Planck Institute in Germany; and the Finnish Meteorological Institute. The California Institute of Technology in Pasadena manages JPL for NASA.

Closest Planetary System Hosts Two Asteroid Belts

New observations from NASA's Spitzer Space Telescope indicate that the nearest planetary system to our own has two asteroid belts. Our own solar system has just one.

The star at the center of the nearby system, called Epsilon Eridani, is a younger, slightly cooler and fainter version of the sun. Previously, astronomers had uncovered evidence for two possible planets in the system, and for a broad, outer ring of icy comets similar to our own Kuiper Belt.

Now, Spitzer has discovered that the system also has dual asteroid belts. One sits at approximately the same position as the one in our solar system. The second, denser belt, most likely also populated by asteroids, lies between the first belt and the comet ring. The presence of the asteroid belts implies additional planets in the Epsilon Eridani system.

"This system probably looks a lot like ours did when life first took root on Earth," said Dana Backman, an astronomer at the SETI Institute, in Mountain View, Calif., and outreach director for NASA's Sofia mission. "The main difference we know of so far is that it has an additional ring of leftover planet construction material." Backman is lead author of a paper about the findings to appear Jan. 10 in the Astrophysical Journal.

Asteroid belts are rocky and metallic debris left over from the early stages of planet formation. Their presence around other stars signals that rocky planets like Earth could be orbiting in the system's inner regions, with massive gas planets circling near the belts' rims. In our own solar system, for example, there is evidence that Jupiter, which lies just beyond our asteroid belt, caused the asteroid belt to form long ago by stirring up material that would have otherwise coalesced into a planet. Nowadays, Jupiter helps keep our asteroid belt confined to a ring.

Astronomers have detected stars with signs of multiple belts of material before, but Epsilon Eridani is closer to Earth and more like our sun overall. It is 10 light-years away, slightly less massive than the sun, and roughly 800 million years old, or one-fifth the age of the sun.

Because the star is so close and similar to the sun, it is a popular locale in science fiction. The television series Star Trek and Babylon 5 referenced Epsilon Eridani, and it has been featured in novels by Issac Asimov and Frank Herbert, among others.

The popular star was also one of the first to be searched for signs of advanced alien civilizations using radio telescopes in 1960. At that time, astronomers did not know of the star's young age.

Spitzer observed Epsilon Eridani with both of its infrared cameras and its infrared spectrometer. When asteroid and comets collide or evaporate, they release tiny particles of dust that give off heat, which Spitzer can see. "Because the system is so close to us, Spitzer can really pick out details in the dust, giving us a good look at the system's architecture," said co-author Karl Stapelfeldt of NASA's Jet Propulsion Laboratory, Pasadena, Calif.

The asteroid belts detected by Spitzer orbit at distances of approximately 3 and 20 astronomical units from the star (an astronomical unit is the average distance between Earth and the sun). For reference, our own asteroid belt lies at about 3 astronomical units from the sun, and Uranus is roughly 19 astronomical units away.

One of the two possible planets previously identified around Epsilon Eridani, called Epsilon Eridani b, was discovered in 2000. The planet is thought to orbit at an average distance of 3.4 astronomical units from the star -- just outside the innermost asteroid belt identified by Spitzer. This is the first time that an asteroid belt and a planet beyond our solar system have been found in a similar arrangement as our asteroid belt and Jupiter.

Some researchers had reported that Epsilon Eridani b orbits in an exaggerated ellipse ranging between 1 and 5 astronomical units, but this means the planet would cross, and quickly disrupt, the newfound asteroid belt. Instead, Backman and colleagues argue that this planet must have a more circular orbit that keeps it just outside the belt.

The other candidate planet was first proposed in 1998 to explain lumpiness observed in the star's outer comet ring. It is thought to lie near the inner edge of the ring, which orbits between 35 and 90 astronomical units from Epsilon Eridani.

The intermediate belt detected by Spitzer suggests that a third planet could be responsible for creating and shepherding its material. This planet would orbit at approximately 20 astronomical units and lie between the other two planets. "Detailed studies of the dust belts in other planetary systems are telling us a great deal about their complex structure," said Michael Werner, co-author of the study and project scientist for Spitzer at JPL. "It seems that no two planetary systems are alike."

JPL manages the Spitzer mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology in Pasadena. Caltech manages JPL for NASA. More information about Spitzer is at http://www.spitzer.caltech.edu/spitzer and http://www.nasa.gov/spitzer . More information about extrasolar planets and NASA's planet-finding program is at http://planetquest.jpl.nasa.gov .

NASA Orbiter Reveals Details of a Wetter Mars

NASA's Mars Reconnaissance Orbiter has observed a new category of minerals spread across large regions of Mars. This discovery suggests that liquid water remained on the planet's surface a billion years later than scientists believed, and it played an important role in shaping the planet's surface and possibly hosting life.

Researchers examining data from the orbiter's Compact Reconnaissance Imaging Spectrometer for Mars have found evidence of hydrated silica, commonly known as opal. The hydrated, or water-containing, mineral deposits are telltale signs of where and when water was present on ancient Mars.

"This is an exciting discovery because it extends the time range for liquid water on Mars, and the places where it might have supported life," said Scott Murchie, the spectrometer's principal investigator at the Johns Hopkins University Applied Physics Laboratory in Laurel, Md. "The identification of opaline silica tells us that water may have existed as recently as 2 billion years ago."

Until now, only two major groups of hydrated minerals, phyllosilicates and hydrated sulfates, had been observed by spacecraft orbiting Mars. Clay-like phyllosilicates formed more than 3.5 billion years ago where igneous rock came into long-term contact with water. During the next several hundred million years, until approximately 3 billion years ago, hydrated sulfates formed from the evaporation of salty and sometimes acidic water.

The newly discovered opaline silicates are the youngest of the three types of hydrated minerals. They formed where liquid water altered materials created by volcanic activity or meteorite impact on the Martian surface. One such location noted by scientists is the large Martian canyon system called Valles Marineris.

"We see numerous outcrops of opal-like minerals, commonly in thin layers extending for very long distances around the rim of Valles Marineris and sometimes within the canyon system itself," said Ralph Milliken of NASA's Jet Propulsion Laboratory in Pasadena, Calif.

Milliken is lead author of an article in the November issue of "Geology" that describes the identification of opaline silica. The study reveals that the minerals, which also were recently found in Gusev Crater by NASA's Mars rover Spirit, are widespread and occur in relatively young terrains.

In some locations, the orbiter's spectrometer observed opaline silica with iron sulfate minerals, either in or around dry river channels. This indicates the acidic water remained on the Martian surface for an extended period of time. Milliken and his colleagues believe that in these areas, low-temperature acidic water was involved in forming the opal. In areas where there is no clear evidence that the water was acidic, deposits may have formed under a wide range of conditions.

"What's important is that the longer liquid water existed on Mars, the longer the window during which Mars may have supported life," says Milliken. "The opaline silica deposits would be good places to explore to assess the potential for habitability on Mars, especially in these younger terrains."

The spectrometer collects 544 colors, or wavelengths, of reflected sunlight to detect minerals on the surface of Mars. Its highest resolution is about 20 times sharper than any previous look at the planet in near-infrared wavelengths.

NASA's Jet Propulsion Laboratory manages the Mars Reconnaissance Orbiter mission for NASA's Science Mission Directorate in Washington. Lockheed Martin Space Systems, Denver, is the prime contractor for the project and built the spacecraft. The Applied Physics Laboratory led the effort to build the spectrometer and operates the instrument in coordination with an international team of researchers from universities, government and the private sector.

More information about the Mars Reconnaissance Orbiter is at http://www.nasa.gov/mro

Monday, October 27, 2008

Space Science News in Modern World

Space Science News is the study of everything above and beyond the surface of the Earth, from Earth's atmosphere to the very edges of the universe. Space Science News Technology refers to the technology in Space Science satellites and ground systems used by Space Science scientists to study the universe (looking up) and the earth (looking down), or to deliver services to users on the ground. The vast majority of Space Science satellites are launched into space to provide services to people on Earth.

Space Science Satellite is an object which has been placed into orbit by human endeavor. Such objects are sometimes called artificial Space satellites to distinguish them from natural Space Science satellites such as the Moon. Space Science News Technology is the property of the universe, in which matter is physically extended and objects have positions relative to one another.

In classical mechanics, Space Science was treated as being separate from time and is thought of as one of the few fundamental physical quantities. In Isaac Newton's view Space Science was absolute, and held that it exists permanently and independently of whether there is any matter in the Space Science or moving through it.

Space Science Exploration and Space Science News is the use of Space Science astronomy and Space Science technology to explore outer Space Science. Physical exploration of Space Science is conducted both by human spaceflights and by robotic Space Science Spacecraft. Space Science exploration and Space Science News has often been used as a proxy competition for geopolitical rivalries such as the Cold War.

The first human spaceflight was Vostok 1 (East 1), carrying 27 year old cosmonaut Yuri Gagarin on April 12, 1961. The Space Science spacecraft completed one orbit around the globe, lasting about 1 hour and 48 minutes. Gagarin's flight resonated around the world; it was a demonstration of the advanced Soviet Space Science News program and it opened an entirely new era in space exploration — human spaceflight.

Space Shuttle Discovery and Space Science News Technology (Orbiter Vehicle Designation: OV-103) is one of the three currently operational orbiters in the Space Shuttle Science fleet of NASA, the Space Science agency of the United States. (The other two are Atlantis and Endeavour.) When first flown in 1984, Space Science Discovery became the third operational orbiter, and is now the oldest orbiter in service. Space Science Discovery has performed both research and International Space Station (ISS) assembly Space Science missions.

Space Science Technology News is technology that is related to entering space science and news, maintaining and using systems during Space Science spaceflight and returning people and things from Space Science.

Space Science Technology News has a huge impact on the everyday lives of people; and something as simple as checking the weather or watching Space Science Satellite television or receiving a parcel guided by Space Science Satellite, it touches most people's lives on any given day.

Friday, October 24, 2008

NASA's Phoenix Mars Team Wins National Space Club Award

The National Space Club presented NASA's Phoenix Mars Lander mission team with its Astronautics Engineer Award last night in Huntsville, Ala. Phoenix Project Manager Barry Goldstein of NASA's Jet Propulsion Laboratory, Pasadena, Calif., accepted the award on behalf of the team at the Space Club's 20th Annual Dr. Wernher von Braun Memorial Dinner.

The nonprofit National Space Club established the Astronautics Engineer Award in 1991. It is given to scientists and engineers in the United States who have led and made significant contributions in rocketry and astronautics. Past recipients include NASA's Return to Flight Team and Alan Stern, former associate administrator for NASA's Science Mission Directorate.

The dinner honors the memory of von Braun, the first director of NASA's Marshall Space Flight Center and one of the most important rocket developers and champions of space exploration in the 20th century.

"This award recognizes that our team really met the ideals of the von Braun legacy," said Goldstein. "Being recognized at a ceremony named for one of the seminal engineers in our industry is a true honor for our teams at JPL, Lockheed Martin, the University of Arizona, and the many other organizations responsible for our success."

The Phoenix Mars Lander reached the northern plains of Mars on May 25, 2008. The lander has been studying the Martian arctic for evidence of past liquid water and habitability. It is also learning about the Red Planet's current climate and atmosphere. Robotic laboratory instruments have sniffed, baked and tasted the Martian soil and ice for their chemical and mineral properties. Phoenix's cameras have returned more than 25,000 images of Mars.

Earlier this month, the Phoenix mission received a 2008 Popular Mechanics Breakthrough Award for innovation. In November, Phoenix will also be presented the 2008 Civil Space Award from the California Space Authority. The mission previously received the 2007 Arizona Governor's Innovation Award in the academia category.

The Astronautics Engineer award was one of five presented at the Space Club event. The other four awards are the Aerospace Educator Award, the Media Award, the Community Service Award, and the Dr. Wernher von Braun Space Flight Trophy. The Space Club's Huntsville chapter sponsored the event, which was held at the Davidson Center for Space Exploration.

The Phoenix mission is led by Principal Investigator Peter Smith of the University of Arizona, with project management at the Jet Propulsion Laboratory and development partnership at Lockheed Martin, located in Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel; the universities of Copenhagen and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute.

Expedition 17 Crew Lands in Kazakhstan

Commander Sergei Volkov and Flight Engineer Oleg Kononenko of the 17th International Space Station crew landed on the steppes of Kazakhstan at 11:37 p.m. EDT Thursday after more than six months days in space.

All three people aboard the Soyuz TMA-12 spacecraft were reported to be in good condition after their re-entry and landing.

A Russian recovery team and NASA personnel reached the landing site by helicopter shortly after the Soyuz touched down. They helped the crew members into reclining chairs for medical tests and set up a medical tent nearby.

With Volkov and Kononenko was spaceflight participant Richard Garriott. He launched to the station Oct. 12 with the Expedition 18 crew, Commander Mike Fincke and Flight Engineer Yury Lonchakov, under contract with the Russian Federal Space Agency.

Astronaut Gregory Chamitoff came to the station aboard Discovery on its STS-124 mission, launched May 31. He served for the last part of Expedition 17 as a flight engineer. He remains aboard the station as a member of the Expedition 18 crew.
Expedition 17 crew members undocked their Soyuz spacecraft from the station at 8:16 p.m. Thursday. The deorbit burn to slow the Soyuz and begin its descent toward the Earth took place at 10:45 a.m.

When they landed, Volkov and Kononenko had spent 199 days in space on their Expedition 17 flight, 197 of them on the station.

Volkov, 35, a lieutenant in the Russian air force, returned from his first spaceflight. Kononenko, a spacecraft design engineer, also completed his first spaceflight.

+ Read more about Expedition 18
+ Read more about Expedition 17 + View crew timelines
+ View crew timelines

Next Moon Mission Begins Thermal Vacuum Test

NASA's Lunar Reconnaissance Orbiter, or LRO, has begun environmental testing in a thermal vacuum that simulates the harsh rigors of space.

The spacecraft, built at NASA's Goddard Space Flight Center in Greenbelt, Md., has been lifted into a four-story thermal vacuum chamber there for a test that will last approximately five weeks. Once sealed in the chamber, the satellite will undergo a series of tests that simulate the space environment it will encounter when it orbits the moon.

During the tests, NASA engineers will operate the spacecraft to ensure it is performing as planned. The project also will conduct mission simulations to further train and develop the team that will operate the spacecraft.

"This is an exciting time for our project" said Cathy Peddie, LRO deputy project manager at Goddard. "Thermal vacuum testing is one of our major milestones. Not only are we checking out LRO in a test facility that most closely matches its final destination, but we are getting more 'hands-on' time operating LRO as we will see it next year at the moon."

The orbiter will carry seven instruments to provide scientists with detailed maps of the lunar surface and enhance our understanding of the moon's topography, lighting conditions, mineralogical composition and natural resources. Information gleaned from LRO will be used to select safe landing sites, determine locations for future lunar outposts and help to mitigate radiation dangers to astronauts.

The orbiter will be shipped to NASA's Kennedy Space Center in Florida early next year to be prepared for its April 24 launch aboard an Atlas V rocket. Accompanying the spacecraft will be the Lunar Crater Observation and Sensing Satellite, a mission that will impact the moon's surface in its search for water ice.

POTENT GREENHOUSE GAS MORE COMMON IN ATMOSPHERE THAN ESTIMATED

New research indicates a powerful greenhouse gas is at least four times more prevalent in the atmosphere than previously estimated. The research, based on data from a NASA-funded measurement network, examined nitrogen trifluoride, which is thousands of times more effective at warming the atmosphere than an equal mass of carbon dioxide.

Using new analytical techniques, Ray Weiss of the Scripps Institution of Oceanography in La Jolla, Calif., led a team of researchers in making the first atmospheric measurements of nitrogen trifluoride. The amount of the gas in the atmosphere, which could not be detected using previous techniques, had been estimated at less than 1,200 metric tons in 2006. The new research shows the actual amount was 4,200 metric tons. In 2008, about 5,400 metric tons of the gas are in the atmosphere, a quantity that is increasing at a rate of about 11 percent per year.

"Accurately measuring small amounts of nitrogen trifluoride in air has proven to be a very difficult experimental problem, and we are very pleased to have succeeded in this effort," Weiss said. The research will be published Oct. 31 in the American Geophysical Union's Geophysical Research Letters.

Emissions of nitrogen trifluoride were thought to be so low that the gas was not considered a significant potential contributor to global warming. It was not covered by the Kyoto Protocol, the 1997 agreement to reduce greenhouse gas emissions signed by 182 countries. The gas is 17,000 times more potent as a global warming agent than a similar mass of carbon dioxide. It survives in the atmosphere about five times longer than carbon dioxide. However, current nitrogen trifluoride emissions contribute only about 0.15 percent of the total global warming effect caused by current human-produced carbon dioxide emissions.

Nitrogen trifluoride is one of several gases used during the manufacture of liquid crystal flat-panel displays, thin-film solar cells and microcircuits. Many industries have used the gas in recent years as an alternative to perfluorocarbons, which also are potent greenhouse gases, because it was believed that no more than two percent of the nitrogen trifluoride used in these processes escaped into the atmosphere.

The Scripps team analyzed air samples gathered during the past 30 years, including samples from the NASA-funded Advanced Global Atmospheric Gases Experiment network of ground-based space stations. The network was created in the 1970s in response to international concerns about chemicals depleting the ozone layer. It is supported by NASA as part of its congressional mandate to monitor ozone-depleting trace gases, many of which also are greenhouse gases. Air samples are collected at several stations around the world. The Scripps team analyzed samples from coastal clean-air stations in California and Tasmania for this research.

The researchers found concentrations of the gas rose from about 0.02 parts per trillion in 1978 to 0.454 parts per trillion in 2008. The samples also showed significantly higher concentrations of nitrogen trifluoride in the Northern Hemisphere than in the Southern Hemisphere, which the researchers said is consistent with its use predominantly in that hemisphere. The current observed rate of increase of nitrogen trifluoride in the atmosphere corresponds to emissions of about 16 percent of the amount of the gas produced globally.

In response to the growing use of the gas and concerns that its emissions are not well known, Space Station Scientists recently have recommended adding it to the list of greenhouse gases regulated by Kyoto.

"As is often the case in studying atmospheric emissions, this study shows a significant disagreement between 'bottom-up' emissions estimates and the actual emissions as determined by measuring their accumulation in the atmosphere," Weiss said.

For more information about NASA and agency programs, visit:

http://www.nasa.gov

People's Republic of China joins WorldWideScience Alliance

WorldWideScienceThe People’s Republic of China has joined the WorldWideScience Alliance – the multilateral governance structure for the global science gateway, WorldWideScience.org. WorldWideScience.org is intended to accelerate international scientific progress by serving as a single, sophisticated point of access for diverse scientific resources and expertise from nations around the world. The addition of China is a notable milestone, as it is a major global contributor to scientific knowledge. Read the press release.


Thursday, October 23, 2008

2008 Nobel Prize in Physics Is Awarded to Researcher Supported by U.S. Department of Energy

A researcher supported by the U.S. Department of Energy has been named co-winner of the 2008 Nobel Prize in Physics. The Royal Swedish Academy of Sciences awarded Dr. Yoichiro Nambu of the United States half of the prize "for the discovery of the mechanism of spontaneous broken symmetry in subatomic physics." Dr. Makoto Kobayashi and Dr. Tohihide Maskawa received a quarter of the 2008 prize "for the discovery of the origin of the broken symmetry which predicts the existence of at least three quarks in nature" (see DOE press release). See OSTI’s Science Showcase on Dr. Nambu and view and download Dr. Nambu’s research from OSTI R&D collections.

Join the discussion on important DOE research

Information BridgeJoin the discussion! A new social networking feature, Document Discussion, has been added to the DOE Information Bridge to provide a forum for moderated, substantive commentary on important DOE research and development. Users may perform a search at the Information Bridge site and then begin a discussion or add to a discussion about any of the documents in the results list returned. Authors of the documents will be notified so that they may view and contribute to the discussion. The Information Bridge is a core OSTI product featuring approximately 190,000 fully searchable DOE technical reports. Information Bridge serves over 3 million user transactions per month.

NASA AND THE CHALLENGER CENTER ANNOUNCE NAMING CONTEST

NASA and the Challenger Center for Space Education have partnered to engage students in ongoing activities for one of NASA's concepts for astronaut housing on the moon through a contest to name a habitat in Antarctica. NASA currently is conducting a test of a lightweight, durable, inflatable habitat on the cold, harsh landscape of the National Science Foundation's McMurdo Station.

The Challenger Center is organizing and conducting the "Name that Habitat" competition for students in kindergarten through twelfth grades from Oct 21 to Nov. 20, 2008. The Challenger Center will recruit subject matter experts to serve as judges for the contest and will provide prizes and other items for the winner and participants. The winning name will be selected later this year and announced by scientists in Antarctica in January 2009. Student, teachers and the public will be able to follow the progress of inflatable habitat activities throughout the project.

The habitat was funded through NASA's Innovative Partnership Program's Seed Fund initiative, with in-kind resource contributions by the National Science Foundation and ILC Dover of Frederica, Del., the manufacturer of the structure. An inflatable habitat is one of several concepts being considered for astronaut housing on the moon.

The structure looks something like an inflatable backyard bounce house for children, but it is far more sophisticated. It is insulated, heated and is pressurized, and has power. It offers 384 square feet of living space and has, at its highest point, an 8-foot ceiling. During the test period, sensors will allow engineers to monitor the habitat's performance.

The contest helps NASA fulfill its mission to promote an interest in science, technology, engineering and mathematics education. The Challenger Center is an international, nonprofit educational organization founded in 1986 by the families of the astronauts lost during the last flight of the space shuttle Challenger. The goal of the organization is to foster student interest in careers in science, technology, engineering and mathematics.

For more information about entering the Name that Habitat contest, visit:

http://www.challenger.org/hab

The inflatable habitat is being developed under NASA's Innovative Partnerships Program. For more information about the program, visit:

http://www.ipp.nasa.gov

For more information about NASA and agency programs, visit:

http://www.nasa.gov

NASA INVITES REPORTERS TO TESTS OF MOON TOOLS IN HAWAII NOV. 13

Media are invited to observe tests of NASA equipment and rover concepts that will demonstrate how astronauts might prospect for lunar resources and make their own oxygen for survival on the moon. The tests will take place Thursday, Nov. 13, starting at 9 a.m. HST outside Hilo, Hawaii.

NASA's In Situ Resource Utilization project focuses on developing methods for astronauts to take advantage of lunar resources at landing sites on the moon. During two weeks of field tests, NASA will demonstrate prototype systems that could enable a sustainable and affordable lunar outpost by minimizing the amount of water and oxygen that must be supplied from Earth. The Pacific International Center for Exploration Systems, or PISCES, headquartered at the University of Hawaii, Hilo, will host the tests.

Reporters will be able to observe and photograph various tests of a prototype moon rover designed to prospect for ice in lunar craters, and two systems to manufacture oxygen from the lunar soil. Engineers involved in the development of these systems will be available for interviews.

Reporters must contact Kimberly Land at 757-746-4749, or Grey Hautaluoma at 202-358-0668 by Friday, Oct. 31, to R.S.V.P. to attend the event. Access to the test site is restricted and requires a letter of assignment on company letterhead for credentials.

For more information about NASA's plans to return to the moon, visit:

http://www.nasa.gov/exploration

For more information about PISCES, visit:

http://www.pisces.uhh.hawaii.edu

NASA'S SHUTTLE ENDEAVOUR MOVES TO LAUNCH PAD, PRACTICE LIFTOFF SET

Space shuttle Endeavour is scheduled to move from Launch Pad 39B to Pad 39A at NASA's Kennedy Space Center, Fla., as early as 8 a.m., Thursday, Oct. 23, as preparations for the STS-126 mission move forward. Endeavour is targeted to lift off Nov. 14 to the International Space Station.

Early Thursday morning, NASA managers will decide when to move the shuttle based on the progress of removing the payload canister from the pad following installation into the pad's changeout room.

The payload was delivered to Pad A early Wednesday morning. Endeavour had been scheduled to move Saturday, Oct. 25, but possibly severe weather now is forecast for the area.

The latest information about the rollaround will be available by calling 321-867-2525.

NASA Television will provide live video of Endeavour's rollaround beginning at 8 a.m. Video highlights of the rollout will air on the NASA TV Video File.

Reporters with Kennedy credentials for this event are invited to a photo opportunity of the move and interview availability with Endeavour Flow Director Ken Tenbusch at 1:30 p.m. For the photo opportunity, media need to be at Kennedy's News Center by 7 a.m. for transportation to the viewing site. For the Tenbusch interview, media need to be at the News Center at 12:30 p.m. for transportation to the launch pad.

The move will take approximately seven hours. After reaching its launch pad, Endeavour will await its next major milestone. A launch dress rehearsal, known as the Terminal Countdown Demonstration Test, is scheduled to take place at Kennedy from Oct. 27 to 29.

During Endeavour's 15-day mission, the shuttle's seven crew members will deliver supplies and equipment necessary to double the station crew size from three to six members and during four spacewalks, service the station's two Solar Alpha Rotary Joints, which allow its solar arrays to track the sun. The shuttle also will deliver Expedition 18 crew member Sandra Magnus and return Expedition 17 flight engineer Greg Chamitoff, who has been aboard the station for more than five months.

Chris Ferguson will command Endeavour. Eric Boe is the pilot. Mission specialists are Steve Bowen, Shane Kimbrough, Heidemarie Stefanyshyn-Piper, Donald Pettit and Magnus.

The Terminal Countdown Demonstration Test provides each shuttle crew with an opportunity to participate in various simulated countdown activities, including equipment familiarization and emergency training.

The following media events are associated with the test. All times are Eastern.

- Oct. 26: STS-126 crew arrival. The crew will arrive between 2:45 p.m. and 4 p.m. at the Shuttle Landing Facility and make a statement. Arrival will be broadcast live on NASA TV.

- Oct. 28: STS-126 crew media availability. The astronauts will take questions from reporters at Launch Pad 39A at 8:30 a.m. The session will be carried live on NASA TV.

- Oct. 29: STS-126 crew walkout photo opportunity. The astronauts will depart from the Operations and Checkout Building at 7:45 a.m. in their flight entry suits in preparation for the countdown demonstration test at the launch pad. The walkout will not be broadcast live but will be part of the NASA TV Video File.

Schedule updates are available by calling 321-867-2525.

To attend crew arrival, reporters must pick up badges before 4 p.m. Friday, Oct. 24, at the Kennedy Badging Facility on State Road 405. For information about covering these events, including proper attire and meeting locations, credentialed media should visit:

http://www.nasa.gov/centers/kennedy/news/media.html

Video b-roll of the Terminal Countdown Demonstration Test will be available on the NASA TV Video File. For NASA TV downlink information, schedules and links to streaming video, visit:

http://www.nasa.gov/ntv

For more information about the STS-126 mission and crew, visit:

http://www.nasa.gov/shuttle

NEXT HUBBLE TELESCOPE MEDIA TELECONFERENCE THURSDAY, OCT. 23

NASA will provide an update to reporters on the current efforts to restore Hubble Space Telescope science observations during a media teleconference on Thursday, Oct. 23, at 2 p.m. EDT.

The briefing participants are:
- Jon Morse, director of the Astrophysics Division in the Science Mission Directorate at NASA Headquarters in Washington
- Art Whipple, manager of the Hubble Systems Management Office at NASA's Goddard Space Flight Center in Greenbelt, Md.

To participate in the conference, reporters in the U.S. should call 1-888-469-0494 and use the pass code "Hubble." International reporters should call 1-415-228-3905.

A recorded replay of the teleconference will be available approximately one hour after the conclusion of the call by dialing 1-888-566-0499. International callers can hear the replay by calling 1-203-369-3057.

Audio of the teleconference will be streamed live at:

http://www.nasa.gov/newsaudio

Wednesday, October 22, 2008

STS-126 Mission Moves Forward!

The Space Shuttle Program's two-day Flight Readiness Review, or FRR, for Endeavour's STS-126 mission will wrap up Wednesday.

From this week's FRR discussions, decisions about preparedness for launch will be taken to the agency-level Flight Readiness Review that will be held Oct. 30-31 at NASA's Kennedy Space Center in Florida.

At that time the launch date will be set and shuttle processing will continue toward the projected liftoff date.

A news conference broadcast on NASA TV will follow the FRR to announce the official launch date.

Back at Kennedy's Space Station Processing Facility, the STS-126 Multi-Purpose Logistics Module is scheduled to be transferred to Launch Pad 39A on Wednesday.

Workers are now turning their attention to Endeavour's move off of Launch Pad 39B.

The crawler-transporter will glide under the shuttle, stacked on the mobile launcher platform, for Endeavour's Saturday roll around to Pad A.

At Johnson Space Center's Neutral Buoyancy Laboratory today, STS-126 mission astronauts Heidemarie Stefanyshyn-Piper and Steve Bowen are rehearsing spacewalking techniques.

Endeavour is targeted to lift off at 7:55 p.m. EST, Nov. 14 on the 27th shuttle mission to the International Space Station.

Climate change seeps into the sea

The ocean has helped slow global warming by absorbing much of the excess heat and heat-trapping carbon dioxide that has been going into the atmosphere since the start of the Industrial Revolution.

All that extra carbon dioxide, however, has been a bitter pill for the ocean to swallow. It's changing the chemistry of seawater, making it more acidic and otherwise inhospitable, threatening many important marine organisms.

Scientists call ocean acidification "the other carbon dioxide problem." They warn that because it causes such fundamental changes in the ocean, it could impact millions of people who depend on the ocean for food and resources. "The growing amount of carbon dioxide in the ocean could have a bigger effect on life on Earth than carbon dioxide in the atmosphere," says JPL's Charles Miller, deputy principal investigator for NASA's new Orbiting Carbon Observatory, scheduled to launch next January.

The ocean takes in and stores most of the heat from the sun that is deposited at Earth's surface -- heat that would otherwise be melting land ice and warming the atmosphere. The ocean also absorbs about one third of the carbon dioxide that humans now put into the air. The rest is taken up by terrestrial vegetation and soils or remains in the atmosphere, increasing the greenhouse effect.

"The ocean surface acts like a sponge to soak up excess carbon dioxide from the atmosphere," says Scott Doney, a senior scientist in marine chemistry at the Woods Hole Oceanographic Institution in Woods Hole, Mass. Much of the extra dissolved carbon is in the ocean’s upper few thousand feet. However, at high latitudes, surface water quickly cools, becomes saltier and denser and sinks, carrying the dissolved carbon to some of the deepest parts of the ocean.

Mix carbon dioxide with water and the result is carbonic acid. After that first simple chemical reaction comes a slightly more complicated series of changes in seawater chemistry. The final outcome is a lowering of the ocean's pH -- meaning the ocean is more acidic, and, ironically, a reduction in a particular form of carbon -- carbonate ion -- that many marine organisms need to make shells and skeletal material. The lower pH and lack of carbonate ion have serious consequences for life in the ocean.

Carbon, carbon everywhere, but not the right kind to use

Closest to the atmospheric source of excess carbon dioxide, the ocean’s surface waters are the first to show the effects of acidification. Since the beginning of the industrial era, the pH of surface waters has decreased slightly but significantly from 8.2 to 8.1, and it continues to decrease. Scientists project the pH of surface water will decrease by the year 2100 to a level not seen on Earth over the past 20 million years, if not longer.

Likely casualties of ocean acidification are the marine plants and animals that use carbonate to form hard shells or other structures. These include mollusks like clams and oysters, and reef-building corals. Not only does ocean acidification limit their access to the carbonate they need for building material, it could become severe enough to dissolve existing coral structures and the shells of living organisms.

Since most corals live in shallow waters, coral reefs, some of the most biologically diverse places on Earth, are particularly vulnerable. "They are already under assault from warming water, over-fishing and habitat degradation," says Doney. "Environmental stress is leading to more incidents of 'coral bleaching,' which occurs when the symbiotic algae that lives inside the coral leaves or dies, and from which reefs often do not recover. Ocean acidification may push corals over the edge."

Other sensitive areas are the Southern Ocean and the subpolar North Pacific, where acidification threatens to unravel important food chains by making life difficult for a small marine snail called a pteropod. It’s a favorite food of small fishes, which, in turn, support larger fishes, penguins, whales and seabirds. Ocean acidification strips seawater of the carbonate ion that pteropods need to build new shells, and it also damages their existing ones.

There will be some winners and losers, says Doney, as the effects of growing ocean acidification are felt. "Although we don’t know exactly how many species depend on pteropods, clams, oysters, mussels or other shelled organisms for food, or on coral reefs for critical habitat, it’s clear that ocean acidification will cause a wholesale alteration of some marine ecosystems in ways we can’t predict," he explains.

History isn't much of a guide. While there have been times in Earth's past when the ocean was more acidic than now, most environmental changes occurred at a considerably slower pace than today. "At the rates of climate change and ocean acidification we’re seeing now, many organisms may be not able to keep up," Doney says.

That sinking feeling

Much of the carbon now in the air will find its way into the ocean with predictable results. "Even if we stopped adding carbon dioxide to the atmosphere today, ocean acidification will continue to increase," says Doney. "What marine fisheries and coral reefs will look like 100 years from now is a big question. We need to know how much carbon dioxide is being taken up, more about the gas exchange between the ocean and the atmosphere, and how this mechanism is affected by climate change."

NASA’s new Orbiting Carbon Observatory will help provide some of the answers after it is launched in January 2009. A NASA Earth System Science Pathfinder mission, it will make precise measurements of atmospheric carbon dioxide on a global scale.

The Orbiting Carbon Observatory will help identify carbon dioxide sources and sinks -- things that absorb and store carbon -- on land and in the ocean and show how they vary over time. Researchers will be able to combine mission data with numerical models to estimate global patterns of the exchange of carbon dioxide from the ocean and atmosphere.

"We’ll have a much better idea about what’s going on over the ocean where measurements have been sparse," explains Miller. "This is especially true in the Southern Ocean, which we believe is a big sink for carbon dioxide based on existing models."

While the Orbiting Carbon Observatory may be the newest NASA mission to help address the issue of ocean acidification, NASA has many other projects and missions that provide important information about ocean biology and chemistry that relates directly to this problem. These include NASA's Moderate Resolution Imaging Spectroradiometer (MODIS), flying on the Terra and Aqua satellites, and the Sea-Viewing Wide Field-of-View Sensor (SeaWiFS). These instruments collect data on ocean color -- a key component of many studies of ocean ecology, plankton and coral reefs. Another example is the recent National Oceanic and Atmospheric Administration and NASA-sponsored Southern Gas Exchange Experiment. During this six-week research cruise, scientists investigated how gases, including carbon dioxide, move between the ocean and the atmosphere in high winds and rough seas.

The really big question is how much longer the ocean can continue to be a sink for atmospheric carbon dioxide before becoming saturated -- a process that may already be underway. The implications for our future climate -- and the ocean -- are immense.

Scientists Seek Climate Clues From Atop Hawaiian Volcano

JPL scientists, satellites and ground-based instruments are contributing to a month-long, university-led experiment on Hawaii's Mauna Loa volcano to track water vapor in Earth's sub-tropics, which affects global temperatures, and rainfall in North America.

For the full story, go to the University of Colorado release at http://www.colorado.edu/news/reports/watervapor/

Phoenix Lander Finishes Soil Delivery to Onboard Labs

NASA's Phoenix Mars Lander has finished scooping soil samples to deliver to its onboard laboratories, and is now preparing to analyze samples already obtained. Scientists are anxious to analyze the samples as the power Phoenix generates continues to drop. The amount of sunlight is waning on Mars' northern plains as late-summer turns to fall.

The spacecraft's robotic arm is digging into the lower portion of the "Upper Cupboard" and "Stone Soup" areas of the Phoenix worksite. Its Surface Stereoscopic Imager is taking photos of this trenching so scientists can better map out the geology of the Red Planet's ice table.

"We're basically trying to understand the depth and extent of the ice table to tie together how geology and climate control its formation," said Phoenix mission scientist Diana Blaney of NASA's Jet Propulsion Laboratory, Pasadena, Calif.

Later this week, Phoenix engineers and scientists will use the robotic arm to attempt to push a soil sample piled in a funnel on top of the lander's Wet Chemistry Laboratory into a cell for analysis. They will take images of soil captured in its Optical Microscope, as well as take digital-elevation models of a rock called "Sandman" with Phoenix's Robotic Arm Camera.

Phoenix has operated nearly five months on Mars since landing on May 25, 2008.

NASA's Phoenix mission is led by Principal Investigator Peter Smith of the University of Arizona, Tucson, with project management at JPL, and development partnership at Lockheed Martin, Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel; the universities of Copenhagen and Aarhus, Denmark; the Max Planck Institute, Germany; and the Finnish Meteorological Institute.

Tuesday, October 21, 2008

NASA RETURNS TO THE MOON WITH INSTRUMENTS ON INDIAN SPACECRAFT

Two NASA instruments to map the lunar surface will launch on India's maiden moon voyage. The Moon Mineralogy Mapper will assess mineral resources, and the Miniature Synthetic Aperture Radar, or Mini-SAR, will map the polar regions and look for ice deposits. The Indian Space Research Organization, or ISRO, is scheduled to launch its robotic Chandrayaan-1 on Oct. 22 from Sriharikota, India.

Data from the two instruments will contribute to NASA's increased understanding of the lunar environment as it implements the nation's space exploration policy, which calls for robotic and human missions to the moon.

"The opportunity to fly NASA instruments on Chandrayaan-1 undoubtedly will lead to important scientific discoveries," NASA Administrator Michael Griffin said. "This exciting collaboration represents an important next step in what we hope to be a long and mutually beneficial relationship with India in future civil space exploration."

The Moon Mineralogy Mapper is a state-of-the-art imaging spectrometer that will provide the first map of the entire lunar surface at high spatial and spectral resolution, revealing the minerals that make up the moon's surface. Scientists will use this information to answer questions about the moon's origin and geological development, as well as the evolution of terrestrial planets in the early solar system. The map also may be used by astronauts to locate resources, possibly including water, that can support exploration of the moon and beyond.

The Mini-SAR is a small imaging radar that will map the permanently shadowed lunar polar regions, including large areas never visible from Earth. The Mini-SAR data will be used to determine the location and distribution of water ice deposits on the moon. Data from the instrument will help scientists learn about the history and nature of objects hitting the moon, and the processes that throw material from the outer solar system into the inner planets.

The spacecraft also will carry four instruments and a small lunar impactor provided by ISRO, and four instruments from Europe. ISRO will launch the vehicle into a lunar polar orbit for a two-year mission.

In addition to the two science instruments, NASA will provide space communications support to Chandrayaan-1. The primary location for the NASA ground tracking station will be at the Johns Hopkins University Applied Physics Laboratory in Laurel, Md.

For more information about Chandrayaan-1, visit:

http://www.isro.org/Chandrayaan

For more information about the Moon Mineralogy Mapper, visit:

http://m3.jpl.nasa.gov

For more information about the Mini-SAR, visit:

http://www.nasa.gov/mission_pages/Mini-RF/main/index.html

For information about NASA's space exploration program, visit:

Monday, October 20, 2008

NASA LAUNCHES IBEX MISSION TO OUTER SOLAR SYSTEM

NASA's Interstellar Boundary Explorer mission, or IBEX, successfully launched from the Kwajalein Atoll in the Pacific Ocean at 1:47 p.m. EDT, Sunday. IBEX will be the first spacecraft to image and map dynamic interactions taking place in the outer solar system.

The spacecraft separated from the third stage of its Pegasus launch vehicle at 1:53 p.m. and immediately began powering up components necessary to control onboard systems. The operations team is continuing to check out spacecraft subsystems.

"After a 45-day orbit raising and spacecraft checkout period, the spacecraft will start its exciting science mission," said IBEX mission manager Greg Frazier of NASA's Goddard Space Flight Center in Greenbelt, Md.

Just as an impressionist artist makes an image from countless tiny strokes of paint, IBEX will build an image of the outer boundary of the solar system from impacts on the spacecraft by high-speed particles called energetic neutral atoms. These particles are created in the boundary region when the 1-million mph solar wind blows out in all directions from the sun and plows into the gas of interstellar space. This region is important to study because it shields many of the dangerous cosmic rays that would flood the space around Earth.

"No one has seen an image of the interaction at the edge of our solar system where the solar wind collides with interstellar space," said IBEX Principal Investigator David McComas of the Southwest Research Institute in San Antonio. "We know we're going to be surprised. It's a little like getting the first weather satellite images. Prior to that, you had to infer the global weather patterns from a limited number of local weather stations. But with the weather satellite images, you could see the hurricanes forming and the fronts developing and moving across the country."

IBEX is the latest in NASA's series of low-cost, rapidly developed Small Explorers spacecraft. The Southwest Research Institute developed the IBEX mission with a team of national and international partners. Goddard manages the Explorers Program for the Science Mission Directorate in Washington.

For more information about the IBEX mission, visit:

http://www.nasa.gov/ibex

Doomed Moon of Mars

This moon is doomed. Mars, named for the Roman god of war, has two tiny moons--Phobos and Deimos--whose names are derived from the Greek for fear and panic. These Martian moons may well be captured asteroids originating in the main asteroid belt between Mars and Jupiter or perhaps from even more distant reaches of the solar system.

The larger moon, Phobos, is a cratered, asteroid-like object in this stunning color image from the Mars Reconnaissance Orbiter. Phobos orbits so close to Mars that gravitational tidal forces are dragging it down. In 100 million years or so, Phobos likely will be shattered by stress caused by the relentless tidal forces, the debris forming a decaying ring around Mars.

Friday, October 17, 2008

LUNAR LANDER TEAMS TO COMPETE FOR $2 MILLION NASA PRIZE

Nine teams with rocket-powered vehicles will compete for $2 million in NASA prize money during the 2008 Northrop Grumman Lunar Lander Challenge, Oct. 24-25, at Las Cruces International Airport in New Mexico.

Teams must fly their vehicle, simulating a takeoff and landing on the moon, and repeat the task in a limited period of time. The competition provides a demanding test of navigation and control for the vehicles, as well as a demonstration of reusable rocket engine technology.

NASA provides the prize money for the competition as part of the Centennial Challenges Program. The X PRIZE Foundation manages the competition at no cost to NASA, receiving financial support from sponsors such as the Northrop Grumman Corp. and the state of New
Mexico.

Media planning to cover the event should contact Becky Ramsey at 202-349-1125 by 5 p.m. EDT, Oct. 20. Attendance at the competition is limited. The competition will webcast live at:

http://space.xprize.org/webcast

The Lunar Lander Challenge is one of seven NASA technology prize competitions. The Centennial Challenge prizes are offered to independent inventors who work without government support, including small businesses, student groups and individuals.

NASA's Innovative Partnerships Program Office manages the Centennial Challenges program. For more information about Centennial Challenges, visit:

http://ipp.nasa.gov/cc

NASA UPDATES TIME FOR SPACE SHUTTLE ATLANTIS' ROLL FROM LAUNCH PAD

NASA managers have adjusted the time for space shuttle Atlantis' rollback from Launch Pad 39A to the Vehicle Assembly Building at NASA's Kennedy Space Center in Florida on Monday, Oct. 20, to 7 a.m. EDT. Atlantis is expected to be in the Vehicle Assembly Building by about 2 p.m.

NASA Television will provide live coverage of Atlantis' move off the pad beginning Monday at 6:30 a.m. Video highlights of the rollback will air on NASA TV Video File.

Media are invited to a photo opportunity of the shuttle's move from the pad at 7 a.m. Monday, and must arrive at Kennedy's News Center by 6 a.m. for transportation to the viewing area. Because dates and times of this event are subject to change, updates are available by calling 321-867-2525.

Media badges may be picked up Friday, Oct. 17, at the Kennedy Badging Office on State Road 405, west of Gate 3, just past the Kennedy Visitor Complex.

The next space shuttle flight will be shuttle Endeavour's STS-126 mission to the International Space Station, targeted for launch Nov. 14. Endeavour is scheduled to move from Launch Pad 39B to pad 39A on Oct. 25.

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

http://www.nasa.gov/ntv

For more information about upcoming shuttle missions, visit:

http://www.nasa.gov/shuttle

NASA INCREASES VALUE OF ENGINEERING AND TECHNOLOGY CONTRACT

NASA has increased the maximum ordering value of a contract with Stinger Ghaffarian Technologies (SGT) Inc., by $49.2 million to support the Applied Engineering and Technology Directorate at NASA's Goddard Space Flight Center in Greenbelt, Md.

Under the Multidisciplinary Engineering and Technology Support services (METS) indefinite-delivery, indefinite-quantity contract, SGT Inc. performs tasks necessary for the design, testing, verification and operations of space flight and ground system hardware and software.

Tasks include development and validation of new technologies to enable future space and science missions in support of the directorate's five engineering divisions: Mechanical Services, Information Systems, Instrument Systems and Technology, Electrical Engineering, and Mission Engineering and Systems Analysis.

Work under the contract provides critical support to a wide range of Goddard's missions and projects, including the Lunar Reconnaissance Orbiter, the Solar Dynamics Observatory, the Hubble Space Telescope, the James Webb Space Telescope, the Geostationary Environmental Operational Satellites-R, the Polar Operational Environmental Satellites, the Magnetospheric MultiScale Satellites, the Global Precipitation Measurement Observatory and the Glory Observatory.

For information about NASA and agency programs, visit:

http://www.nasa.gov

Two Black Holes Teach Astronomers a Lesson

Observations of two different systems -- both containing stellar-mass black holes -- are showing astronomers how much they have yet to learn. Coordinated observations of these systems using the European Southern Observatory's Very Large Telescope and NASA's Rossi X-ray Timing Explorer reveal surprising dips in optical brightness moments before high-energy flares erupt.

The systems are Swift J1753.5-0127 -- discovered by NASA's Swift satellite -- and GX 339-4. In them, a black hole and a normal star orbit a few million miles apart. That's less than 10 percent of the distance between Mercury and our sun.

Because the normal stars in these systems have evolved into bloated giants, a stream of matter spills toward the black hole and forms a disk of hot gas around it. As matter collides in this so-called accretion disk, it heats up to millions of degrees. Near the black hole, intense magnetic fields in the disk accelerate material into tight jets that flow in opposite directions away from the hole.

If that sounds familiar, it should. A similar process occurs in active galaxies and quasars, where black holes weighing millions of suns gobble up matter. Jets from active galaxies may extend tens of thousands of light-years. Because the process is thought to be the same despite the black hole's size, astronomers class systems like Swift J1753.5-0127 and GX 339-4 as "microquasars." Astronomers don't fully understand how black holes create these jets, so they study nearby microquasars for a detailed look at the process in miniature. "Microquasars are not only closer, but they change more rapidly," says Richard Mushotzky at NASA's Goddard Space Flight Center in Greenbelt, Md. "Changes that may take a year to see in a quasar occur in these systems over a minute or less."

"The orbital period of Swift J1753.5-0127 -- just 3.2 hours -- is the fastest found for a likely black hole," says team member Martin Durant at the Institute of Astrophysics of the Canary Islands. The orbital period of GX 339-4, by contrast, is about 1.7 days. "Yet the two systems are similar in their X-ray properties," he notes.
Astronomers had thought that the cooler visible-light emission comes from so far out in a black hole's accretion disk that it reflects little of the main action. "We were wrong, and these systems prove it," Durant says. "The optical and X-ray emissions are intrinsically linked, probably by the same immense magnetic fields that can hurl material into light-years-long jets."

To study the systems, an international team led by Poshak Gandhi of Japan's RIKEN Institute of Physical and Chemical Research watched them simultaneously using two different instruments, one on the ground and one in space. A high-speed camera called ULTRACAM on the European Southern Observatory's Very Large telescope captured visible light changes. ULTRACAM recorded up to 20 images a second.

NASA's Rossi X-ray Timing Explorer captured the X-ray variations. The satellite can record changes in X-ray output that occur in millionths of a second. "Being able to take readings at high speed and coordinate between NASA's satellite and the ESO's biggest telescopes gives us a unique opportunity to seeing what's going on in the systems," Durant says.

The data show that the light output typically drops just before the X-ray output undergoes a large spike, which mean the two emissions are strongly connected. "The rapid variations in the X-ray and visible light output must have some common origin, and one very close to the black hole itself," Gandhi concludes. "The cool thing about discovering such patterns that stand out amidst chaotic fluctuations of light is that they give us a new handle on understanding the underlying physics."

“Strong magnetic fields represent the best candidate for the dominant physical process,” says team member Jon Miller at the University of Michigan. Magnetic fields can soak up energy liberated close to the black hole and store it. This energy is released either as multi-million-degree, X-ray-emitting gas or as streams of charged particles traveling near the speed of light. How the black holes divide the energy between these two forms determines the characteristic pattern of X-ray and optical changes astronomers observe.

"These kinds of studies are mapping the accretion disks around black holes," says Mushotzky. "Right now, astronomers aren't sure what's happening where."

Phoenix Gets Bonus Soil Sample

The Mars Phoenix Lander's robotic arm successfully delivered soil into oven six of the lander's thermal and evolved-gas analyzer (TEGA) on Monday, Oct. 13, or Martian day (sol) 137 of the mission.

The delivery to oven six is a "bonus round" for Phoenix, as the mission goal requirement of filling and analyzing soil in at least three of the ovens has already been satisfied. Six of eight ovens have been used to date.

TEGA's tiny ovens heat the soil to as high as 1,800 degrees Fahrenheit (1,000 degrees Celsius). The lab's "nose," or mass spectrometer, then "smells" and analyzes the gases derived from heating the soil. Mission scientists will continue to research and analyze the soil samples in the coming months, long after Phoenix stops operating on the surface.

Now in Martian late-summer, Phoenix is gradually getting less power as the sun drops below the horizon.

"My entire team is working very hard to make use of the power we have before it disappears," said William Boynton of the University of Arizona, Tucson, the lead scientist for TEGA. "Every time we fill an oven, we potentially learn more about Mars' geochemistry."

NASA's Phoenix mission is led by Peter Smith of the University of Arizona, with project management at NASA's Jet Propulsion Laboratory, Pasadena, Calif., and development partnership at Lockheed Martin, Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel; the universities of Copenhagen and Aarhus, Denmark; the Max Planck Institute, Germany; and the Finnish Meteorological Institute.

NASA's Spitzer Gets Sneak Peak Inside Comet Holmes

When comet Holmes unexpectedly erupted in 2007, professional and amateur astronomers around the world turned their telescopes toward the spectacular event. Their quest was to find out why the comet had suddenly exploded.

Observations taken of the comet after the explosion by NASA's Spitzer Space Telescope deepen the mystery, showing oddly behaving streamers in the shell of dust surrounding the nucleus of the comet. The data also offer a rare look at the material liberated from within the nucleus, and confirm previous findings from NASA's Stardust and Deep Impact missions.

"The data we got from Spitzer do not look like anything we typically see when looking at comets," said Bill Reach of NASA's Spitzer Science Center at the California Institute of Technology, Pasadena, Calif. Reach is lead investigator of the Spitzer observations. "The comet Holmes explosion gave us a rare glimpse at the inside of a comet nucleus." The findings were presented at the 40th meeting of the Division of Planetary Sciences in Ithaca, N.Y.

Every six years, comet 17P/Holmes speeds away from Jupiter and heads inward toward the sun, traveling the same route typically without incident. However, twice in the last 116 years, in November 1892 and October 2007, comet Holmes exploded as it approached the asteroid belt, and brightened a million-fold overnight.

In an attempt to understand these odd occurrences, astronomers pointed NASA's Spitzer Space Telescope at the comet in November 2007 and March 2008. By using Spitzer's infrared spectrograph instrument, Reach was able to gain valuable insights into the composition of Holmes' solid interior. Like a prism spreading visible-light into a rainbow, the spectrograph breaks up infrared light from the comet into its component parts, revealing the fingerprints of various chemicals.

In November of 2007, Reach noticed a lot of fine silicate dust, or crystallized grains smaller than sand, like crushed gems. He noted that this particular observation revealed materials similar to those seen around other comets where grains have been treated violently, including NASA's Deep Impact mission, which smashed a projectile into comet Tempel 1; NASA's Stardust mission, which swept particles from comet Wild 2 into a collector at 13,000 miles per hour (21,000 kilometers per hour), and the outburst of comet Hale-Bopp in 1995.

"Comet dust is very sensitive, meaning that the grains are very easily destroyed, said Reach. "We think the fine silicates are produced in these violent events by the destruction of larger particles originating inside the comet nucleus."

When Spitzer observed the same portion of the comet again in March 2008, the fine-grained silicate dust was gone and only larger particles were present. "The March observation tells us that there is a very small window for studying composition of comet dust after a violent event like comet Holmes' outburst," said Reach.

Comet Holmes not only has unusual dusty components, it also does not look like a typical comet. According to Jeremie Vaubaillon, a colleague of Reach's at Caltech, pictures snapped from the ground shortly after the outburst revealed streamers in the shell of dust surrounding the comet. Scientists suspect they were produced after the explosion by fragments escaping the comet's nucleus.

In November 2007, the streamers pointed away from the sun, which seemed natural because scientists believed that radiation from the sun was pushing these fragments straight back. However, when Spitzer imaged the same streamers in March 2008, they were surprised to find them still pointing in the same direction as five months before, even though the comet had moved and sunlight was arriving from a different location. "We have never seen anything like this in a comet before. The extended shape still needs to be fully understood," said Vaubaillon.

He notes that the shell surrounding the comet also acts peculiarly. The shape of the shell did not change as expected from November 2007 to March 2008. Vaubaillon said this is because the dust grains seen in March 2008 are relatively large, approximately one millimeter in size, and thus harder to move.

"If the shell was comprised of smaller dust grains, it would have changed as the orientation of the sun changes with time," said Vaubaillon. "This Spitzer image is very unique. No other telescope has seen comet Holmes in this much detail, five months after the explosion."

"Like people, all comets are a little different. We've been studying comets for hundreds of years – 116 years in the case of comet Holmes - but still do not really understand them," said Reach. "However, with the Spitzer observations and data from other telescopes, we are getting closer."

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology, also in Pasadena. Caltech manages JPL for NASA.

For more information about Spitzer, visit http://www.spitzer.caltech.edu/spitzer and http://www.nasa.gov/spitzer .

NASA'S Fermi Telescope Discovers First Gamma-Ray-Only Pulsar

About three times a second, a 10,000-year-old stellar corpse sweeps a beam of gamma-rays toward Earth. Discovered by NASA's Fermi Gamma-ray Space Telescope, the object, called a pulsar, is the first one known that only "blinks" in gamma rays.

"This is the first example of a new class of pulsars that will give us fundamental insights into how these collapsed stars work," said Stanford University's Peter Michelson, principal investigator for Fermi's Large Area Telescope in Palo Alto, Calif.

The gamma-ray-only pulsar lies within a supernova remnant known as CTA 1, which is located about 4,600 light-years away in the constellation Cepheus. Its lighthouse-like beam sweeps Earth's way every 316.86 milliseconds. The pulsar, which formed about 10,000 years ago, emits 1,000 times the energy of our sun.

A pulsar is a rapidly spinning neutron star, the crushed core left behind when a massive sun explodes. Astronomers have cataloged nearly 1,800 pulsars. Although most were found through their pulses at radio wavelengths, some of these objects also beam energy in other forms, including visible light and X-rays. However, the source in CTA 1 only pulses at gamma-ray energies.

"We think the region that emits the pulsed gamma rays is broader than that responsible for pulses of lower-energy radiation," explained team member Alice Harding at NASA's Goddard Space Flight Center in Greenbelt, Md. "The radio beam probably never swings toward Earth, so we never see it. But the wider gamma-ray beam does sweep our way."

Scientists think CTA 1 is only the first of a large population of similar objects.

"The Large Area Telescope provides us with a unique probe of the galaxy's pulsar population, revealing objects we would not otherwise even know exist," says Fermi project scientist Steve Ritz, also at Goddard.

The pulsar in CTA 1 is not located at the center of the remnant's expanding gaseous shell. Supernova explosions can be asymmetrical, often imparting a "kick" that sends the neutron star careening through space. Based on the remnant's age and the pulsar's distance from its center, astronomers believe the neutron star is moving at about a million miles per hour -- a typical speed.

Fermi's Large Area Telescope scans the entire sky every three hours and detects photons with energies ranging from 20 million to more than 300 billion times the energy of visible light. The instrument sees about one gamma ray every minute from CTA 1, enough for scientists to piece together the neutron star's pulsing behavior, its rotation period, and the rate at which it is slowing down.

A pulsar's beams arise because neutron stars possess intense magnetic fields and rotate rapidly. Charged particles stream outward from the star's magnetic poles at nearly the speed of light to create the gamma-ray beams Fermi sees. Because the beams are powered by the neutron star's rotation, they gradually slow the pulsar's spin. In the case of CTA 1, the rotation period is increasing by about one second every 87,000 years.

"This observation shows the power of the Large Area Telescope," Michelson said. "It is so sensitive that we can now discover new types of objects just by observing their gamma-ray emissions."

NASA's Fermi Gamma-ray Space Telescope is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S.

A paper about the new pulsar appears in the Oct. 16 edition of Science Express. For images and animations associated with this release, visit:

http://www.nasa.gov/mission_pages/GLAST/news/gr_pulsar.html

Hubble Status Update: Oct. 16, 2008

During the night of Oct. 15, Space Telescope Operations Control Center engineers at NASA’s Goddard Space Flight Center turned on and checked out Side ‘B’ of Hubble’s Science Instrument Control and Data Handling (SIC&DH) system.

Subsequently, the Advanced Camera for Surveys (ACS), Wide Field Planetary Camera 2 (WFPC2) and Near Infrared Camera and Multi-Object Spectrometer (NICMOS) instruments were retrieved from safe mode to establish that each has a working interface to the Side B SIC&DH. The instruments were then commanded back into safe mode, and will remain in that state until the SI C&DH begins issuing commands to them later today.

Around noon today commands to recover Hubble’s science instruments from their safe modes will begin and internal exposures and calibrations of the telescope’s science instruments will occur before midnight Thursday.

Scientists at the Space Telescope Science Institute in Baltimore should complete their review of the internal exposures by noon on Friday, October 17. This procedure involves collecting and comparing baseline exposures previously supported by Side A of the SI C&DH to new exposures supported by Side B. This review will be one last check of the “transparency” (non-impact) of switching to the redundant spacecraft electronics the Hubble team activated on Wednesday.

A full schedule of science observations with the WFPC2 camera, ACS’ Solar Blind Channel camera, and the Fine Guidance Sensors will resume early Friday morning.

SCHMITT COMPLETES NASA ADVISORY COUNCIL SERVICE; FORD NAMED CHAIRMAN

NASA Advisory Council Chairman Harrison "Jack" H. Schmitt announced Thursday he was leaving the council. Fellow council member Kenneth Ford will succeed him as chairman effective immediately. The NASA Advisory Council provides advice to the NASA administrator on important program and policy matters related to the U.S. space program.

"My service as chairman of Administrator Mike Griffin's advisory council has been one of my most rewarding professional experiences," Schmitt said. "The members of the council represent the finest and most diverse group of advisors that could be assembled, and I am greatly indebted to them for the stimulating interaction and productive deliberations we have had during the last three years. The administrator, NASA and the nation have been well served by their dedication and hard work, and I am certain that even more productive activity will take place under the guidance of the new chairman, Ken Ford."

The council consists of experts from various fields offering knowledge of the multitude of functions within the agency. Council recommendations and advice are critical to the agency's timely strategic and tactical decisions about NASA's mission.

"Sen. Schmitt has provided invaluable advice and leadership for over three years as Chair of the NASA Advisory Council," Griffin said. "He was instrumental in reformulating the NAC to fulfill its proper role as NASA's primary external advisory group. The experience he has brought to the NAC as a scientist, astronaut and former U.S. senator has been of tremendous value to me in helping to manage the agency. I am deeply grateful for both his long friendship and his commitment of service to NASA and the nation."

Schmitt has served as chair of the NASA Advisory Council since November 2005. Under his leadership, the council developed and submitted more than 100 recommendations to the NASA administrator in the areas of aeronautics, audit and finance, exploration, human capital, science, and space operations. These recommendations significantly contributed to NASA's implementation of the agency's new space exploration plans.

Schmitt also was the primary advocate behind the council's February 2007 workshop that produced 35 recommendations covering exploration science, lunar science, lunar-based science, and other research enabled by the emerging exploration architecture for returning humans to the moon by 2020. The workshop was a key part of the council's obligation to advise the administrator about science associated with the nation's return to the moon while making its findings directly available to NASA's exploration and science directorates. Schmitt also led the council's initiative to build a strong relationship with the National Institute of Health and other entities for the utilization of the International Space Station as a national laboratory.

Schmitt is a geologist, former NASA astronaut and former U.S. senator. He and his Apollo 17 crewmate, Eugene Cernan, were the last two people to walk on the moon.

Kenneth Ford has been a member of the NASA Advisory Council since June 2007, serving on the Exploration Committee. He is founder and director of the Florida Institute for Human and Machine Cognition, a statewide not-for-profit research institute of the state university system of Florida. The institute features world-class scientists and engineers investigating a broad range of topics related to building technological systems that are aimed at amplifying and extending
human cognitive and perceptual capacities.

In January 1997, NASA asked Ford to develop and direct its new Center of Excellence in Information Technology at NASA's Ames Research Center at Moffett Field, Calif. He served as both associate center director and director of the Center of Excellence. Ford was awarded the NASA Outstanding Leadership Medal in July 1999.

Ford is the author of hundreds of scientific papers and six books. His research interests include artificial intelligence, cognitive science, human-centered computing, and entrepreneurship in government and academia. He earned a Ph.D. in computer science from Tulane University. Ford is a fellow of the Association for the Advancement of Artificial Intelligence and was the 2008 recipient of the Robert S. Englemore Memorial Award for his work in artificial intelligence.

In 2005, Ford was appointed to the Air Force Science Advisory Board. President George W. Bush nominated Ford to serve a six-year term on the National Science Board in October 2002.

For more information about the NASA Advisory Council, visit:

http://www.hq.nasa.gov/office/oer/nac

For more information about NASA and agency programs, visit:

http://www.nasa.gov

ADMINISTRATOR'S STATEMENT ON SIGNING OF THE NASA AUTHORIZATION ACT

The following is a statement by NASA Administrator Michael Griffin after the signing by the president of the NASA Authorization Act of 2008:

"I'm grateful to the president for his signature on the NASA Authorization Act of 2008. The major provisions of this authorization bill affirm Congress' support for the broad goals of the president's space exploration policy, including the return of American astronauts to the moon, exploration of Mars and other destinations."

For more information about NASA and agency programs, visit:

http://www.nasa.gov

Thursday, October 16, 2008

A Robot to Find Water and Oxygen on the Moon

A robot rover designed for prospecting within lunar craters has to operate in continual darkness at extremely cold temperatures with little power. The moon has one-sixth the gravity of Earth, so a lightweight rover will have a difficult job resisting drilling forces and remaining stable. Lunar soil, known as regolith, is abrasive and compact, so if a drill strikes ice, it likely will have the consistency of concrete. Meeting these challenges in one system requires ingenuity and teamwork.

Engineers used this lunar rover to demonstrate a drill capable of digging samples of regolith. The demonstration used a laser light camera to select a site for drilling then commanded the four-wheeled rover to lower the drill and collect three-foot samples of soil and rock.

Image at Top: This robot shares some features with the lunar truck, but is equipped with a drill designed to find water and oxygen-rich soil on the moon. Credit: Carnegie Mellon University.

For more information about NASA's plans for a lunar outpost, visit:

http://www.nasa.gov/exploration

NASA INVITES REPORTERS TO OBSERVE LUNAR ROVER TESTS IN ARIZONA

NASA is practicing for future lunar road trips, and reporters are invited to observe the activities. The annual Desert RATS, or Research and Technology Studies, field test will be held in Arizona during October, and NASA will host a media day on Oct. 24. The tests help NASA engineers identify transportation and spacewalking needs for NASA's return to the moon by 2020 and preparation for human journeys to Mars.

This year's tests will demonstrate an enclosed configuration for a lunar rover NASA has been developing since 2007. The rover has six independent wheels that can each turn a full 360 degrees and lift off the ground for maneuvering around and over obstacles. The addition of the pressurized module to the rover allows the crew to drive in shirtsleeves, only donning spacesuits to leave the vehicle for scientific observations or exploration tasks.

For this year's tests, two teams of one astronaut and one geologist will conduct one-day and three-day drives of the rover with and without the pressurized cabin. Without the cabin, the crew operates the rover from rotating driving turrets while wearing spacesuits to protect them from the moon's dusty, airless environment.

Reporters will be able to observe and photograph the small pressurized rover and interview engineers involved with its development. For more information, including an agenda, and to R.S.V.P., reporters must contact Ashley Edwards at 202-358-1756 no later than Wednesday, Oct. 22. Reporters with reservations will meet at the U.S. Geological Survey office in Flagstaff, Ariz., by 7 a.m. MST for a NASA escort to the test site, where access is restricted. NASA requires a letter of assignment on company letterhead for credentials.

Organizations involved in the test are NASA's Johnson Space Center in Houston; NASA's Kennedy Space Center in Florida; the Smithsonian Institution of Washington, the U.S. Geological Survey, in Flagstaff; Arizona State University of Tempe; the Mars Institute in Moffett Field, Calif.; and the Lunar Planetary Institute in Houston.

For more information about the lunar rover, visit:

http://www.nasa.gov/mission_pages/constellation/main/lunar_truck.html

For more information about NASA's plans to return to the moon, visit:

http://www.nasa.gov/exploration

NASA TO DISCUSS MISSION TO STUDY SUN'S WEAKENING PROTECTIVE BUBBLE

NASA will hold a media teleconference on Friday, Oct. 17, at 1 p.m. EDT, to preview the Interstellar Boundary Explorer, or IBEX, mission. The spacecraft may confirm if the sun's protective bubble surrounding our solar system, called the heliosphere, is about to shrink and weaken. IBEX also will be the first spacecraft to image and map the dynamic interactions taking place where the hot solar wind slams into the cold expanse of space.

The heliosphere acts as a shield for our solar system, warding off most of the galactic cosmic rays. Recent data indicate the solar wind's global pressure is the lowest seen since the beginning of the space age.

IBEX is set to launch Oct. 19 from the Kwajalein Atoll, a part of the Marshall Islands in the Pacific Ocean.

Panelists will be:
- David McComas, IBEX principal investigator at Southwest Research Institute in San Antonio
- Nathan Schwadron, co-investigator and IBEX Science Operations Center lead at Boston University
- Stephen Fuselier, co-investigator and IBEX-Lo Sensor lead at Lockheed-Martin Advanced Technology Center in Palo Alto, Calif.
- Eric Christian, program scientist at NASA Headquarters in Washington

Reporters should call 1-888-323-5257 and use the passcode "IBEX" to participate in the teleconference. International media should call 1-415-228-4881. Supporting information for the briefing will be available at the start of the teleconference on the Web at:

http://www.nasa.gov/ibex

NASA SETS MEDIA BRIEFING FOR CREWS ON INTERNATIONAL SPACE STATION

The astronauts, cosmonauts and spaceflight participant aboard the International Space Station will participate in a news conference at 12:20 p.m. CDT, Monday, Oct. 20. Reporters at participating NASA centers may ask questions.

Expedition 17 Commander Sergei Volkov and Flight Engineer Oleg Kononenko, who have been on the station since April, are scheduled to return to Earth with spaceflight participant Richard Garriott, a U.S. citizen, in the Soyuz TMA-12 spacecraft Oct. 23, landing in central Kazakhstan. Garriott, who flew under an agreement with the Russian Federal Space Agency, arrived at the station with Fincke and Lonchakov.

Expedition 17 Commander Sergei Volkov and Flight Engineer Oleg Kononenko, who have been on the station since April, are scheduled to return to Earth with U.S. spaceflight participant Richard Garriott in the Soyuz TMA-12 spacecraft Oct. 23, landing in central Kazakhstan. Garriott arrived at the station with Fincke and Lonchakov.

A change of command ceremony between the two crews will be broadcast on NASA Television at 12:40 p.m. Wednesday, Oct. 22.

For NASA TV streaming video, downlink and scheduling information, visit:

http://www.nasa.gov/ntv

For more information about the International Space Station, visit:

http://www.nasa.gov/station

NASA TO WEBCAST IBEX SPACECRAFT LAUNCH ON PEGASUS ROCKET OCT. 19

The first NASA spacecraft to image and map the dynamic interactions taking place where the hot solar wind slams into the cold expanse of space will be launched on Sunday, Oct. 19, at 1:48 p.m. EDT, during a launch window that extends from 1:44 p.m. to 1:52 p.m. The two-year mission will begin from the U.S. Army's Reagan test site at Kwajalein Atoll, a part of the Marshall Islands in the south Pacific Ocean.

Called the Interstellar Boundary Explorer, or IBEX, the spacecraft will conduct extremely high-altitude orbits above Earth to investigate and capture images of processes taking place at the farthest reaches of the solar system. Known as the interstellar boundary, this region marks where the solar system meets interstellar space.

Carrying the IBEX spacecraft into orbit will be a Pegasus XL rocket built by Orbital Sciences Corporation of Dulles, Va. The Pegasus will be deployed from the Orbital Sciences L-1011 aircraft over the Pacific Ocean about 125 miles north of Kwajalein. The spacecraft also was built by Orbital Sciences.

Live coverage of the IBEX launch will be provided via the Web. No live NASA Television coverage is planned. The live streaming video of the countdown and launch will be available on the NASA home page at:

http://www.nasa.gov

Audio coverage of the launch will be available at 321-867-1220, 1240, 1260, and 7135. Streaming video and audio coverage will begin at 12:15 p.m. on Oct. 19. It will conclude after spacecraft separation from the Pegasus, approximately 12 minutes after launch.

For more information about IBEX, including a launch blog, visit:

http://www.nasa.gov/ibex

NASA RELEASES DOCUMENTARY CELEBRATING AGENCY'S FIRST 50 YEARS

In celebration of its 50th anniversary, NASA will premiere the documentary "50 Years of Exploration: The Golden Anniversary of NASA" on NASA Television's Public and Education channels Wednesday, Oct. 15, at 9 p.m. EDT.

Neil Armstrong hosts the 90-minute documentary that features film and video highlights of the agency's first half-century. Included are insights and perspectives from astronauts, scientists, engineers and others whose contributions have helped shepherd America's space program.

Interviews include former NASA astronaut and U.S. Senator John Glenn, Apollo Flight Director Gene Kranz, author Ray Bradbury, NASA scientist and Nobel Prize winner John Mather, and presidents George H.W. Bush and Bill Clinton.

"50 Years of Exploration: The Golden Anniversary of NASA" is a production of NASA Television. It will be re-broadcast on NASA TV's Public and Education channels at 1, 5 and 9 p.m. EDT on both Thursday, Oct. 16, and Friday, Oct. 17.

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

http://www.nasa.gov/ntv

For information about NASA's 50th Anniversary, visit:

http://www.nasa.gov/50th

For more information about NASA, visit:

http://www.nasa.gov

NASA'S SPACE SHUTTLE ATLANTIS ROLLS OFF LAUNCH PAD MONDAY

Space shuttle Atlantis is scheduled to roll back from Launch Pad 39A to the Vehicle Assembly Building at NASA's Kennedy Space Center in Florida on Monday, Oct. 20, to await launch on its mission to repair the Hubble Space Telescope. First motion of the shuttle is scheduled for 12:01 a.m. EDT.

Atlantis' targeted launch on Oct. 10 was delayed when a system that transfers science data from the orbiting observatory to Earth malfunctioned on Sept. 27. The new target launch date is under review.

The fully assembled space shuttle Atlantis, consisting of the orbiter, external tank and twin solid rocket boosters, is mounted on a Mobile Launcher Platform and will be delivered to the Vehicle Assembly Building atop a crawler transporter. The crawler will travel slower than 1 mph during the 3.4-mile journey, which is expected to take approximately six hours.

NASA Television will provide live coverage of Atlantis' rollback beginning Monday at 6:30 a.m. Video highlights of the rollback will air on NASA TV Video File.

Media are invited to a photo opportunity of the shuttle's move from the pad at 6 a.m. Monday. As dates and times of this event are subject to change, updates are available by calling 321-867-2525.

Media must arrive at Kennedy's News Center by 5 a.m. for transportation to the viewing area. Foreign news media accreditation for this event is closed. U.S. media without permanent Kennedy Space Center credentials must apply for accreditation online by 3 p.m. Thursday, Oct. 16, at:

https://media.ksc.nasa.gov

Badges may be picked up between 10 a.m. and 4 p.m. Friday, Oct. 17 at the Kennedy Badging Office on State Road 405, west of Gate 3, just past the Kennedy Visitor's Complex.

The next space shuttle flight will be shuttle Endeavour's STS-126 mission to the International Space Station, targeted for launch Nov. 14. Endeavour is scheduled to move from Launch Pad 39B to Pad 39A on Oct. 25.

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

http://www.nasa.gov/ntv

For more information about upcoming shuttle missions, visit:

http://www.nasa.gov/shuttle

JPL's Jon Giorgini Honored With Masursky Award

Jon Giorgini, an engineer at NASA's Jet Propulsion Laboratory, Pasadena, Calif., has received the prestigious Harold Masursky Award, presented by the American Astronomical Society's Division for Planetary Sciences.

The Masursky Award recognizes individuals for outstanding service to planetary science and exploration through engineering, managerial, programmatic or public service activities. Giorgini runs JPL's Horizons system, an online database that can generate locations and orbits for the almost half-million known celestial bodies in our solar system.

The award citation states in part: A specialist at the NASA Jet Propulsion Laboratory, Jon developed and implemented the on-line Horizons system that is used by the international scientific community to generate accurate ephemeris information for the 450,000 currently known objects in the solar system. This includes the sun, planets, their moons, asteroids, comets, and many spacecraft... This system is used by observers, researchers, and mission planners to plan observations and track the targets of space and ground-based telescopes, as well as spacecraft. Since its inception in October 1996, the Horizons system has responded to more than ten million requests (on average, more than 2200 per day) received from 300,000 unique locations.

Giorgini, a senior engineer in JPL's Solar System Dynamics Group, was a navigator for the Magellan spacecraft during its mapping of Venus (1991-1993), developing and implementing the new navigation methodology for the first interplanetary aerobrake. He created JPL's "On-Site Orbit Determination" system -- software used at the Goldstone and Arecibo planetary radar sites to track and update the orbits of radar targets. He then returned to navigation for the Mars Global Surveyor aerobrake planning and interplanetary phases (1995-1997), followed by the Near-Earth Asteroid Rendezvous mission navigation and radio science teams (1997-2001). As a member of the asteroid radar observing team (1994-present), he is responsible for orbit analysis and predictions used to operate radar tracking systems at Goldstone and Arecibo. He has worked on more than 290 asteroid radar targets since 1994 and is co-discoverer of 27 asteroid satellites. He discovered the potential Earth impact hazard posed by the asteroid 1950 DA, and developed methods to assess dynamics and impact potential over centuries. Giorgini is author or co-author of 99 research papers and four book chapters.

Giorgini's outside activities have included climbs of Mount Kilimanjaro and Vinson Massif, the highest mountains in Africa and Antarctica. He has practiced martial arts and kickboxing for the last 22 years.

Giorgini's previous awards include the JPL 2007 Ed Stone Outstanding Research Paper Award, a NASA Space Act Award and a NASA Exceptional Service Medal. The International Astronomical Union named asteroid "6775 Giorgini" in his honor in 1996.

Giorgini has a Bachelor of Science degree in aerospace engineering from Iowa State University, Ames; and a Master of Science degree in aerospace engineering, specializing in celestial mechanics, from the University of Texas, Austin. He has worked at JPL for 17 years.

For more information on JPL, visit: http://www.jpl.nasa.gov .

NASA's Mars Odyssey Shifting Orbit for Extended Mission

The longest-serving of six spacecraft now studying Mars is up to new tricks for a third two-year extension of its mission to examine the most Earthlike of known foreign planets.

NASA's Mars Odyssey is altering its orbit to gain even better sensitivity for its infrared mapping of Martian minerals. During the mission extension through September 2010, it will also point its camera with more flexibility than it has ever used before. Odyssey reached Mars in 2001.

The orbit adjustment will allow Odyssey's Thermal Emission Imaging System to look down at sites when it's mid-afternoon, rather than late afternoon. The multipurpose camera will take advantage of the infrared radiation emitted by the warmer rocks to provide clues to the rocks' identities.

"This will allow us to do much more sensitive detection and mapping of minerals," said Odyssey Project Scientist Jeffrey Plaut of NASA's Jet Propulsion Laboratory, Pasadena, Calif.

The mission's orbit design before now used a compromise between what works best for the Thermal Emission Imaging System and what works best for another instrument, the Gamma Ray Spectrometer.

On commands from its operations team at JPL and at Denver-based Lockheed Martin Space Systems, Odyssey fired thrusters for nearly 6 minutes on Sept. 30, the final day of the mission's second two-year extension.

"This was our biggest maneuver since 2002, and it went well," said JPL's Gaylon McSmith, Odyssey mission manager. "The spacecraft is in good health. The propellant supply is adequate for operating through at least 2015."

Odyssey's orbit is synchronized with the sun. The local solar time has been about 5 p.m. at whatever spot on Mars Odyssey flew over as it made its dozen daily passes from between the north pole region to the south pole region for the past five years. (Likewise, the local time has been about 5 a.m. under the track of the spacecraft during the south-to-north leg of each orbit.)

The push imparted by the Sept. 30 maneuver will gradually change that synchronization over the next year or so. Its effect is that the time of day on the ground when Odyssey is overhead is now getting earlier by about 20 seconds per day. A follow-up maneuver, probably in late 2009 when the overpass time is between 2:30 and 3:00 p.m., will end the progression toward earlier times.

While aiding performance of the Thermal Emission Imaging System, the shift to mid-afternoon is expected to stop the use of one of three instruments in Odyssey's Gamma Ray Spectrometer suite. The suite's gamma ray detector needs a later-hour orbit to avoid overheating of a critical component. The suite's neutron spectrometer and high-energy neutron detector are expected to keep operating.

The Gamma Ray Spectrometer provided dramatic discoveries of water-ice near the surface throughout much of high-latitude Mars, the impetus for NASA's Phoenix Mars Lander mission. The gamma ray detector has also mapped global distribution of many elements, such as iron, silicon and potassium, a high science priority for the first and second extensions of the Odyssey mission. A panel of planetary scientists assembled by NASA recommended this year that Odyssey make the orbit adjustment to get the best science return from the mission in coming years.

Increased sensitivity for identifying surface minerals is a key science goal for the mission extension beginning this month. Also, the Odyssey team plans to begin occasionally aiming the camera away from the straight-down pointing that has been used throughout the mission. This will allow the team to fill in some gaps in earlier mapping and also create some stereo, three-dimensional imaging.

Odyssey will continue providing crucial support for Mars surface missions as well as conducting its own investigations. It has relayed to Earth nearly all data returned from NASA rovers Spirit and Opportunity. It shares with NASA's Mars Reconnaissance Orbiter the relay role for Phoenix. It has made targeted observations for evaluating candidate landing sites.

Mars Odyssey, launched in 2001, is managed by JPL, a division of the California Institute of Technology, Pasadena, for NASA's Science Mission Directorate, Washington. Lockheed Martin Space Systems, Denver, is the prime contractor for the project and built the spacecraft. Investigators at Arizona State University, Tempe, operate the Thermal Emission Imaging System. Investigators at the University of Arizona, Tucson, head operation of the Gamma Ray Spectrometer. Additional science partners are located at the Russian Aviation and Space Agency, which provided the high-energy neutron detector, and at Los Alamos National Laboratories, New Mexico, which provided the neutron spectrometer.

For more about the Mars Odyssey mission, visit: http://mars.jpl.nasa.gov/odyssey .

NEW CREW BLASTS OFF FOR INTERNATIONAL SPACE STATION

A new crew that will live and work aboard the International Space Station rocketed into orbit early Sunday aboard a Soyuz spacecraft. U.S. astronaut E. Michael Fincke, Russian cosmonaut Yury Lonchakov and Richard Garriott, a U.S. computer game developer, lifted off from the Baikonur Cosmodrome in Kazakhstan at 2:01 a.m. CDT.

Fincke, the only American to launch twice on a Soyuz, will serve as commander of the six-month Expedition 18 mission. The mission's main focus will be preparing the station to house six crew members on long-duration missions.

The Expedition 18 crew is scheduled to arrive at the station Tuesday, with docking to the Zarya module scheduled for 3:33 a.m. After the hatches are opened, Expedition 17 Commander Sergey Volkov and spaceflight participant Garriott will become the first children of previous space fliers to greet each other in orbit. Garriott is the son of former NASA astronaut Owen Garriott, who was a member of the Skylab-3 crew in 1973. Volkov is the son of veteran cosmonaut Alexander Volkov, who flew three Soyuz missions.

Garriott will spend nine days on the station under a commercial agreement with the Russian Federal Space Agency. He will return to Earth on Oct. 23 with Volkov and Expedition 17 Flight Engineer Oleg Kononenko, who have worked aboard the station since April 10.

Expedition 17 Flight Engineer Greg Chamitoff, who arrived at the station in June, will be replaced in November by NASA astronaut Sandra Magnus. Space shuttle Endeavour will deliver Magnus and return Chamitoff to Earth.

Endeavour's November STS-126 mission also will deliver equipment to the station necessary for supporting a six-member crew, including a water recycling system, sleeping quarters, a new kitchen, a second toilet, and an advanced exercise device.

Although they will be in space on Election Day, Chamitoff and Fincke have arranged for the chance to cast their ballots from the station.

For more information about the space station and how to view it from Earth, visit:

http://www.nasa.gov/station

For more information about upcoming space shuttle missions and their crews, visit:

http://www.nasa.gov/shuttle

NASA TO PROVIDE UPDATE TO HUBBLE ANOMALY STATUS

NASA will host a media teleconference at 12:30 p.m. EDT, Tuesday, Oct. 14, to brief reporters about the status of efforts to revive the data handling unit that failed on the Hubble Space Telescope in late-September. The failure halted almost all science operations on the orbiting observatory.

A meeting will be held at NASA Headquarters on Tuesday morning to review plans for transitioning operations to the redundant "B" side of Hubble's data handling unit. This equipment has not been used or tested since Hubble's launch in 1990. If approved, ground controllers could begin the process of sending commands to Hubble as early as Wednesday, Oct. 15, to begin the transition. The process could take as long as 48 hours to complete.

The briefing participants are:
- Jon Morse, Astrophysics Division director in the Science Mission Directorate at NASA Headquarters in Washington.
- Art Whipple, manager of the Hubble Space Telescope Systems Management Office at NASA's Goddard Space Flight Center in Greenbelt, Md.

To participate in the teleconference, reporters in the U.S. should call 1-866-556-1095 and use the pass code "Hubble." International reporters should call 1-212-547-0420.

Audio of the teleconference will be streamed live at:

http://www.nasa.gov/newsaudio

Friday, October 10, 2008

NASA TO PROVIDE MARS SCIENCE LABORATORY LAUNCH UPDATE

NASA will host a media teleconference at 3 p.m. EDT, Friday, Oct. 10, to brief reporters after a meeting held by the agency's administrator concerning the Mars Science Laboratory, or MSL. The meeting is to discuss technical and budget issues.

The mission, scheduled to launch in 2009, will assess a variety of scientific objectives, including whether Mars had, or has today, an environment able to support microbial life. The rover will carry the largest, most advanced suite of instruments for scientific studies ever sent to the Martian surface.

The briefing participants are:
- James Green, director of the Planetary Division in the Science Mission Directorate at NASA Headquarters in Washington
- Doug McCuistion, director of the Mars Exploration Program at NASA Headquarters
- Michael Meyer, Mars Program lead scientist at NASA Headquarters

To participate in the teleconference, reporters in the U.S. should call 1-866-398-6118 and use the pass code "MSL." International reporters should call 1-517-308-9407.

Audio of the teleconference will be streamed live at:

http://www.nasa.gov/newsaudio

For more information about MSL, visit:

http://mars.jpl.nasa.gov/msl

NASA SETS BRIEFINGS FOR NEXT SHUTTLE MISSION TO THE SPACE STATION

NASA will hold a series of news briefings on Monday, Nov. 3, to preview the upcoming space shuttle Endeavour mission that will outfit the International Space Station for six-person crews.

NASA Television and the agency's Web site will provide live coverage of the briefings from NASA's Johnson Space Center in Houston. News media questions also will be taken from other participating NASA locations.

Endeavour's 15-day flight, designated STS-126, is targeted for launch Nov. 14. The flight will deliver supplies and equipment to prepare the station for six-person crews starting next spring. The mission also includes four spacewalks to service the two Solar Array Rotary Joints that allow the arrays to track the sun.

U.S. reporters planning to attend the briefings in Houston must contact the Johnson newsroom at 281-483-5111 by Oct. 29 to arrange for credentials. Journalists who are foreign nationals must contact the Johnson newsroom by Oct. 16.

Also on Nov. 3, Endeavour's seven astronauts will be available for round-robin interviews at Johnson. Reporters must contact Gayle Frere at 281-483-8645 by Oct. 29 to reserve an interview opportunity.

Chris Ferguson will command Endeavour's crew, which includes Pilot Eric Boe, and Mission Specialists Donald Pettit, Steve Bowen, Heidemarie Stefanyshyn-Piper, Shane Kimbrough, and Sandra Magnus. The spacewalkers will be Stefanyshyn-Piper, Bowen and Kimbrough. Magnus will remain on the station as flight engineer and science officer of the Expedition 18 crew. Expedition 17 Flight Engineer Greg Chamitoff will return to Earth on Endeavour to conclude six months on the station.

Briefing times (all times CST):

7 a.m.: Video B-roll feed on NASA TV

8 - 9:30 a.m.: Program Overview Space Shuttle Program Manager John Shannon International Space Station Program Manager Mike Suffredini

9:30 - 11 a.m.: Mission Overview STS-126 Lead Flight Director Mike Sarafin International Space Station Lead Flight Director Ginger Kerrick Launch Package Manager Kevin Engelbert

11 a.m.: NASA TV Video File

11:30 a.m.-1 p.m.: Spacewalk Overview Briefing Lead Extravehicular Activity Officer John Ray

1 - 2 p.m.: STS-126 Crew News Conference

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

http://www.nasa.gov/ntv

For the latest information about the STS-126 mission and its crew, visit:

http://www.nasa.gov/shuttle

For the latest information on the International Space Station, visit:

http://www.nasa.gov/station

Thursday, October 9, 2008

NASA ASTRONAUT TALKS WITH STUDENT CHESS OPPONENTS THURSDAY

NASA astronaut Greg Chamitoff will meet his opponents in the ongoing Earth vs. space chess match Thursday, Oct. 9. At 1:05 p.m. CDT, NASA Television will broadcast the live linkup with Chamitoff, who lives aboard the International Space Station, and his competitors from the Stevenson Elementary School in Bellevue, Wash.

Reporters may attend the event in the Bellevue Community College's Carlson Theater, where the kindergarten through third grade members of the U.S. Chess Championship Team and its chess club teammates will gather.

The students are key players in the Earth vs. space match, proposing moves that are voted on by the public via the Internet. The match began Sept. 29.

The U.S. Chess Federation is facilitating the match on its Web site at:

http://www.uschess.org/nasa2008

Chamitoff, a space station flight engineer orbiting 210 miles above Earth at five miles a second, is a chess aficionado. He brought a chess set with him when he arrived at the complex last June. Chamitoff has added Velcro to the chess pieces to keep them from floating away in the weightlessness of space. He has been playing long-distance chess with station control centers around the world. So far, he is undefeated.

For more information about the U.S. Chess Federation, visit:

http://www.uschess.org

For more about Chamitoff and the space station, visit:

http://www.nasa.gov/station

For NASA TV schedule updates, downlinks, and streaming video information, visit:

http://www.nasa.gov/ntv

Spinoff 2008 lists, NASA innovations

The 2008 edition of NASA's annual Spinoff publication celebrates the agency's 50th anniversary and highlights 50 new examples of how NASA technology is being put to use in everyday life.
This anniversary edition features a 50-year timeline of NASA-derived technologies from historical programs and projects, and a summary of award-winning NASA technologies included in Spinoff over the years.

Spinoff 2008 lists many of the latest NASA innovations now in the commercial marketplace. These innovations have resulted in healthcare advances, transportation breakthroughs, public safety benefits, new consumer goods, environmental protection, computer technology and
industrial productivity.

"The results of NASA research and technology are all around us, providing benefits to many aspects of our daily lives and well-being," said NASA's Deputy Administrator Shana Dale.

Several examples of these benefits are described in Spinoff 2008, including:
- Advanced polymer coatings for implantable devices to help avert heart failure
- Robotic technology used for minimally invasive knee surgery
- Space suit-derived textiles to help protect firefighters and race car drivers
- Drag reduction research applied to record-breaking swimsuit development
- Astronaut food supplements in worldwide use to improve baby formula
- Carbon nanomesh technology applied to filtering safe drinking water
- Rocket engine valve technology reducing emissions for power generation.

Spinoff 2008 also profiles NASA research and development activities, education efforts, and partnership successes. The publication provides reference information and resources available through the agency's Innovative Partnerships Program.

NASA's Innovative Partnerships Program produces the NASA Spinoff series. The program fosters technology partnerships, commercialization and innovation in support of NASA's overall mission and national priorities. For more information about the program, visit:

http://www.ipp.nasa.gov

To request a free copy of Spinoff 2008, call 301-286-0561. To access Spinoff 2008 on the Web, and view a searchable database of more than 1,600 NASA-derived technologies that have been featured in previous Spinoff editions, visit:

http://www.sti.nasa.gov/tto/

For information about NASA and agency programs, visit:

http://www.nasa.gov

MESSENGER Returns Images from Oct. 6 Mercury Fly-By

MESSENGER is the first mission sent to orbit the planet closest to the sun. On Oct. 6, 2008, at roughly 4:40 a.m. ET, MESSENGER flew by Mercury for the second time this year. During the encounter, the probe swung just 125 miles (200 kilometers) above the cratered surface of Mercury, snapping hundreds of pictures and collecting a variety of other data from the planet as it gains a critical gravity assist that keeps the probe on track to become the first spacecraft ever to orbit the innermost planet beginning in March 2011.

At roughly 1:50 a.m. ET on October 7, MESSENGER's most recent images began to be received back on Earth. The spectacular image shown here is one of the first to be returned. It shows Mercury about 90 minutes after the spacecraft’s closest approach. The bright crater just south of the center of the image is Kuiper, identified on images from the Mariner 10 mission in the 1970s.

For most of the terrain east of Kuiper, toward the limb (edge) of the planet, the departing images are the first spacecraft views of that portion of Mercury’s surface. A striking characteristic of this newly imaged area is the large pattern of rays that extend from the northern region of Mercury to regions south of Kuiper.

Splashy Portrait Helps Explain How Stars Form

Different wavelengths of light swirl together like watercolors in a new, ethereal portrait of a bright, star-forming region.

The multi-wavelength picture combines infrared, visible and X-ray light from NASA's Spitzer Space Telescope, the European Southern Observatory's New Technology Telescope, and the European Space Agency's XMM-Newton orbiting X-Ray telescope, respectively.

The colorful image offers a fresh look at the history of the star-studded region, called NGC 346, revealing new information about how stars form in the universe. NGC 346 is the brightest star-forming region in the Small Magellanic Cloud, a so-called irregular dwarf galaxy that orbits our Milky Way galaxy, 210,000 light-years away.

"NGC 346 is an astronomical zoo," said Dimitrios Gouliermis of the Max Planck Institute for Astronomy in Germany, lead author of a new paper describing the observations in an upcoming issue of the Astrophysical Journal. "When we combined data at various wavelengths, we were able to tease apart what's going on in different parts of the cloud."

The new picture is available online at: http://www.nasa.gov/mission_pages/spitzer/multimedia/20081008.html .

Small stars are scattered throughout the NGC 346 region, while massive stars populate its center. The massive stars and most of the small stars formed at the same time out of one dense cloud, while other small stars were created later through a process called triggered star formation. Intense radiation from massive stars ate away at the surrounding dusty cloud, triggering gas to expand and create shock waves that compressed nearby cold dust and gas into new stars. The red-orange filaments surrounding the center of the image show where this process has occurred.

But a set of even younger small stars in the region, seen as a pinkish blob at the top of the image, couldn't be explained by this mechanism. Scientists were scratching their heads over what caused this seemingly isolated group of stars to form.

By combining multi-wavelength data of NGC 346, Gouliermis says he and his team were able to pinpoint the trigger as a very massive star that blasted apart in a supernova explosion about 50,000 years ago. According to the astronomers, this very massive star spurred the isolated young stars into existence before it died, but through a different type of triggered star formation than that which occurred near the center of the region. Fierce winds from the massive star, and not radiation, pushed dust and gas together, compressing it into new stars.

The finding demonstrates that both wind- and radiation-induced triggered star formation are at play in the same cloud. According to Gouliermis, "The result shows us that star formation is a far more complicated process than we used to believe, comprising different competitive or collaborative mechanisms."

The new image also reveals a bubble, seen as a blue halo to the left, caused by the supernova explosion that happened 50,000 years ago. Further analysis shows that this bubble is located within a large expanding gaseous shell, possibly powered by the explosion and the winds of other bright stars in its vicinity.

Infrared light (red) shows cold dust; visible light (green) denotes glowing gas; and X-rays (blue) represent very warm gas. Ordinary stars appear as blue spots with white centers, while young stars enshrouded in dust appear as red spots with white centers.

Other authors of this paper include Thomas Henning and Wolfgang Brandner of the Max Planck Institute for Astronomy, and You-Hua Chu and Robert Gruendl of the University of Illinois at Urbana-Champaign.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology, also in Pasadena. Caltech manages JPL for NASA.

More information about Spitzer is at http://www.spitzer.caltech.edu/spitzer and http://www.nasa.gov/spitzer .

NASA ISSUES SPACE SHUTTLE TO CONSTELLATION WORKFORCE TRANSITION REPORT

NASA is releasing an updated version of the Workforce Transition Strategy Report, which was delivered to Congress on Wednesday. The report details the agency's plan to minimize job losses while transitioning from the Space Shuttle Program to the Constellation Program.

The report will be available online Wednesday at 3 p.m. EDT at:

http://www.nasa.gov/transition

The initial report was submitted to Congress on March 31, 2008. The next update will be submitted to Congress in spring 2009.

NASA SELECTS ITT FOR SPACE COMMUNICATIONS NETWORK SERVICES

NASA has selected ITT Corporation, Advanced Engineering and Sciences of Herndon, Va., to perform telemetry, tracking and command services for near-Earth missions under the Space
Communications Network Services contract.

The contract, with an estimated maximum value of $1.26 billion, will support NASA's Space and Near Earth Networks, which provide most of the communications for a wide range of NASA's science-based Earth-orbiting spacecraft, including the International Space Station, the space shuttle, the Hubble Space Telescope and the Earth Observing System satellites.

This cost-plus-award-fee core and indefinite-delivery/indefinite-quantity contract has a basic period of performance of five years and three months, including the phase-in period. The contract also includes two one-year options.

The core portion of the contract provides for the operation and maintenance of NASA's Space Network, comprised of the Tracking and Data Relay Satellites and associated ground systems located primarily at White Sands, N.M., and Guam. The contract also provides support to ancillary Space Network sites located in American Samoa, Ascension Island and Australia.

The indefinite-delivery/indefinite-quantity portion of the contract provides for operation and maintenance of NASA's Near Earth Network, including operations at Wallops Flight Facility at Wallops Island, Va.; the White Sands Complex in Las Cruces, N.M.; the Merritt Island Launch Annex in Florida; and McMurdo Station in Antarctica. It also includes commercial tracking and data-acquisition operations worldwide, and the Electronics Systems Test Laboratory at NASA's Johnson Space Center in Houston. This portion of the contract also includes support for the Satellite Laser Ranging network and the global Very Long Baseline Interferometry Network. Support in the areas of systems and sustaining engineering, logistics, facilities management and hardware and software development for the Space Network and the Near Earth Network also will be provided.

For more information about NASA and agency programs, visit:

http://www.nasa.gov

Phoenix Lander Digs and Analyzes Soil as Darkness Gathers

As fall approaches Mars' northern plains, NASA's Phoenix Lander is busy digging into the Red Planet's soil and scooping it into its onboard science laboratories for analysis.

Over the past two weeks, Phoenix's nearly 2.4-meter-long (8 feet) arm moved a rock, nicknamed "Headless," about 0.4 meters (16 inches), and snapped an image of the rock with its camera. Then, the robotic arm scraped the soil underneath the rock and delivered a few teaspoonfuls of soil onto the lander's optical and atomic-force microscopes. These microscopes are part of Phoenix's Microscopy, Electrochemistry and Conductivity Analyzer (MECA).

Scientists are conducting preliminary analysis of this soil, nicknamed "Galloping Hessian." The soil piqued their interest because it may contain a high concentration of salts, said Diana Blaney, a scientist on the Phoenix mission with NASA's Jet Propulsion Laboratory, Pasadena, Calif.

As water evaporates in arctic and arid environments on Earth, it leaves behind salt, which can be found under or around rocks, Blaney said. "That's why we wanted to look under 'Headless,' to see if there's a higher concentration of salts there."

More digging is underway. Phoenix scientists want to analyze a hard, icy layer beneath the Martian soil surface, and excavating to that icy layer underneath a rock might give scientists clues about processes affecting the ice.

So the robotic arm has dug into a trench called "La Mancha," in part to see how deep the Martian ice table is. The Phoenix team also plans to dig a trench laterally across some of the existing trenches in hopes of revealing a cross section, or profile, of the soil's icy layer.

"We'd like to see how the ice table varies around the workspace with the different topography and varying surface characteristics such as different rocks and soils," said Phoenix co-investigator Mike Mellon of the University of Colorado, Boulder. "We hope to learn more about how the ice depth is controlled by physical processes, and by looking at how the ice depth varies, we can pin down how it got there."

Over the weekend, on the 128th Martian day, or sol, Phoenix engineers successfully directed the robotic arm to dig in a trench called "Snow White" in the eastern portion of the lander's digging area. The robotic arm then delivered the material to an oven screen on Phoenix's Thermal and Evolved-Gas Analyzer.

The Phoenix team will try to shake the oven screen so the soil can break into smaller lumps and fall through for analysis.

The Phoenix lander, originally planned for a three-month mission on Mars, is now in its fifth month. As fall approaches, the lander's weather instruments detect diffuse clouds above northern Mars, and temperatures are getting colder as the daylight hours wane.

Consequently, Phoenix faces an increasing drop in solar energy as the sun falls below the Martian horizon. Mission engineers and scientists expect this power decline to curtail activities in the coming weeks. As darkness deepens, Phoenix will primarily become a weather station and will likely cease all activity by the end of the year.

The Phoenix mission is led by Principal Investigator Peter Smith at the University of Arizona. Project management is the responsibility of JPL, with development partnership by Lockheed Martin in Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus, Denmark; the Max Planck Institute, Germany; and the Finnish Meteorological Institute.

More information about Phoenix is at: www.nasa.gov/phoenix .

Artists and Astronomers 'Observe' the Universe Together

Our current view of the universe, to quote Albert Einstein, is "not weirder than we do imagine, but weirder than we can imagine." That said, we have no choice but to observe the universe through human eyes and brains. How can we even start to make sense of it?

One answer might be to call in the artists. For thousands of years, people have used art to explore ideas that humble, confuse or even frighten us. A new exhibition opening in Pasadena continues this tradition, bringing artists and astronomers together to create original pieces of art.

Called "Observe," the exhibition is the culmination of a yearlong collaboration between two Pasadena institutions -- the Art Center College of Design and NASA's Spitzer Science Center at the California Institute of Technology. Beginning Oct. 10, visitors to the Art Center's Williamson Gallery will be challenged to stretch their imaginations as infrared observations from NASA's Spitzer Space Telescope are visualized through the minds of five contemporary Southern California artists.

"Science is bringing us spectacular discoveries that torque our everyday perception of reality. Things like black holes, multiple universes and time distortions challenge our human-centered culture and beliefs," said Stephen Nowlin, director of the Williamson Gallery. "This is an exhibition about the newly unknown."

Dan Goods, an Observe artist and a visual strategist at NASA's Jet Propulsion Laboratory in Pasadena, was fascinated by the idea that light from distant stars and galaxies travels for years before reaching us. "Some of those stars died thousands of years ago, and they only exist in the light that is still on its way to our eyes," he pointed out.

Goods built a clock that spans a large room. Spheres throughout the room represent the hours. The spheres all look the same at the entrance, but like stars in the sky, they are actually different sizes and distances away. Speakers on the spheres play back sounds from people in the room, distorted and delayed by random time increments. This distortion represents a phenomenon called "redshift" in astronomy, in which light is stretched to longer wavelengths as it travels through space. "It's like the stars are talking to you," Goods explained.

Other projects include an interactive video installation by Daniel Wheeler, which invites visitors to "send" data all over the world to create an abstract collage of images; and a planetarium-like room filled with changing projections of the stars by Lita Albuquerque. George Legrady used a projected laser to make patterns representing all the pointing commands that have been sent up to Spitzer in space. And Lynn Aldrich created a fake-fur wormhole -- a theoretical tunnel through space and time -- that people can crawl through.

"I was amazed by the serendipities that cropped up," said Michelle Thaller, outreach manager at the Spitzer Science Center. "Lynn Aldrich's furry wormhole is a great way to represent the weird, almost chaotic nature of other dimensions!"

"I've always thought that Spitzer's images were spectacular, but working with the artists has made me look at scientific data in a whole new way," she added. "Data out of context can become art."

Observe opens to the public on Oct. 10 as part of ArtNight Pasadena, a weekend of art around town sponsored by the Pasadena Arts and Culture Commission. Opening-night hours are 6 to 10 p.m. The exhibition will run though Jan. 9, 2009, ushering in the International Year of Astronomy, a yearlong celebration of the 400th anniversary of Galileo and the first telescope.

JPL manages the Spitzer mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center. Caltech manages JPL for NASA.

More information about Spitzer is at www.spitzer.caltech.edu . More information about the Art Center College of Design is at www.artcenter.edu . More information about Pasadena ArtNight is at www.artcenter.edu/artnight .

Tuesday, October 7, 2008

NASA AWARDS FUTURE VEHICLE AIRCRAFT RESEARCH CONTRACTS

NASA has awarded research contracts worth a total of $12.4 million to six industry teams to study advanced concepts for subsonic and supersonic commercial transport aircraft that could
enter service in 25 to 30 years.

NASA's Aeronautics Research Mission Directorate selected teams led by The Boeing Company, GE Aviation, Lockheed Martin Corporation, Massachusetts Institute of Technology and Northrop Grumman to receive separate 18-month study contracts valued at approximately $2 million each.

The focus of the studies is on commercial transports that can overcome significant performance and environmental challenges for the benefit of the general public. The work is intended to identify key technology development needs, such as advanced airframes and propulsion systems, as well as breakthroughs that will enable such vehicles to enter service in 2030-2035. The vehicles represent a research and development generation known as "N+3," denoting three generations beyond the current commercial transport fleet.

"The future of air transportation is all about protecting the environment and responding to increasing energy costs in a balanced way," said Juan Alonso, director of NASA's Fundamental Aeronautics Program at NASA's Headquarters in Washington. "We will need airplanes that are quieter and more fuel efficient, and cleaner-burning fuels to power them. We are challenging industry to introduce these new technologies without impairing the convenience, safety and security of commercial air transportation."

The studies constitute the first phase of a two-phase acquisition involving a competitive down-selection process. Participants who successfully complete the first phase will be asked to submit proposals for Phase 2, which provides additional funds for initial research on the enabling technologies identified in Phase 1.

The Phase 1 research projects are listed below, including team members and award amounts.

Development of Subsonic Ultra Green Aircraft Research: The Boeing Company, Georgia Institute of Technology, GE Global Research and GE Aviation; $1.9 million.

Small Commercial Efficient and Quiet Air Transportation for 2030-2035: GE Aviation, GE Global Research, Georgia Institute of Technology and Cessna Aircraft Company; $1.97 million.

Aircraft and Technology Concepts for an N+3 Subsonic Transport: Massachusetts Institute of Technology, Aurora Flight Sciences, Aerodyne Research Inc., Pratt and Whitney and Boeing Phantom Works; $2.13 million.

Advanced Concept Studies for Subsonic Commercial Transport Aircraft Entering Service in the 2030-2035 Time Period: Northrop Grumman Systems Corporation, Tufts University, Sensis Corporation, Spirit Aerosystems Corp. and Rolls-Royce North America Inc.; $1.97 million.

Advanced Concepts Studies for Supersonic Commercial Transport Aircraft Entering Service in the 2030-2035 Time Period: The Boeing Company, Boeing Phantom Works, GE Global Research, Georgia Institute of Technology, M4 Engineering Inc., Pratt and Whitney, Rolls Royce and Wyle Labs; $2.28 million.

NASA N+3 Supersonic, Three Generations Forward in Aviation Technology: Lockheed Martin Corporation, GE Global Research, Purdue University and Wyle Laboratories; $1.96 million.

For more information about NASA's Aeronautics Research Mission Directorate, visit:

http://aeronautics.nasa.gov

NASA SPACECRAFT READY TO EXPLORE OUTER SOLAR SYSTEM

The first NASA spacecraft to image and map the dynamic interactions taking place where the hot solar wind slams into the cold expanse of space is ready for launch Oct. 19. The two-year mission will begin from the Kwajalein Atoll, a part of the Marshall Islands in the Pacific Ocean.

Called the Interstellar Boundary Explorer or IBEX, the spacecraft will conduct extremely high-altitude orbits above Earth to investigate and capture images of processes taking place at the farthest reaches of the solar system. Known as the interstellar boundary, this region marks where the solar system meets interstellar space.

"The interstellar boundary regions are critical because they shield us from the vast majority of dangerous galactic cosmic rays, which otherwise would penetrate into Earth's orbit and make human spaceflight much more dangerous," said David J. McComas, IBEX principal investigator and senior executive director of the Space Science and Engineering Division at the Southwest Research Institute in San Antonio.

The story of the outer solar system began to unfold when the Voyager 1 and Voyager 2 spacecrafts left the inner solar system and headed out toward the boundary between our solar system and interstellar space.

"The Voyager spacecraft are making fascinating observations of the local conditions at two points beyond the termination shock that show totally unexpected results and challenge many of our notions about this important region," said McComas.

Other spacecraft have continued the exploration of the interstellar boundary region. Recently, a pair of NASA sun-focused satellites, the Solar Terrestrial Relations Observatory mission, detected a higher-energy version of the particles IBEX will observe in the heliosphere. The heliosphere is an area that contains the solar wind. It stretches from the sun to a distance several times the orbit of Pluto.

IBEX is poised to thoroughly map this interstellar boundary region of the solar system. The images will allow scientists to understand the global interaction between our sun and the galaxy for the very first time.

IBEX will be launched aboard a Pegasus rocket dropped from under the wing of an L-1011 aircraft flying over the Pacific Ocean. The Pegasus will carry the spacecraft approximately 130 miles above Earth and place it in orbit.

"What makes the IBEX mission unique is that it has an extra kick during launch," said Willis Jenkins, IBEX program executive at NASA Headquarters in Washington. "An extra solid-state motor pushes the spacecraft further out of low-Earth orbit where the Pegasus launch vehicle leaves it."

The IBEX mission is the next in NASA's series of low-cost, rapidly developed Small Explorers spacecraft. NASA's Goddard Space Flight Center in Greenbelt, Md., manages the Explorers Program for NASA's Science Mission Directorate in Washington. The mission was developed by Southwest Research Institute with national and international partner participation.

For more information about IBEX, visit:

http://www.nasa.gov/ibex

NASA AND THE ADLER PLANETARIUM HOST NASA FUTURE FORUM IN CHICAGO

NASA Deputy Administrator Shana Dale will deliver a keynote address on Friday, Oct. 10, at the Adler Planetarium to kick off NASA's Future Forum in Chicago. The 8:45 a.m. CDT event marks the final Future Forum and is part of a year-long series celebrating the agency's 50th anniversary. The forum will focus on how space exploration benefits Chicago's economic and academic sectors.

During the forum, astronauts Robert Satcher, Jr., and Kenneth Ham will discuss upcoming space shuttle missions. Carl Walz, director of NASA's Advanced Capabilities Division at the agency's headquarters in Washington, will provide an overview of the agency's plans to return astronauts to the moon and travel beyond. Other NASA participants include Woodrow Whitlow, Jr., director of NASA's Glenn Research Center in Cleveland, and senior officials, engineers and scientists.

NASA astronauts and senior officials will be available to answer questions from news media. Reporters who would like to attend should contact Sonja Alexander at sonja.r.alexander@nasa.gov or 202-358-1761.

Event schedule for the NASA Chicago Future Forum: (All times CDT, subject to minor changes)

- 8:30 a.m. - Welcome by Paul H. Knappenberger, Jr., PhD, president, Adler Planetarium, Chicago
- 8:45 a.m. - Remarks by NASA Deputy Administrator Shana Dale
- 9 a.m. - Overview of the NASA Exploration Program by Carl Walz
- 10 a.m. - Innovation Panel: "Unleashing the power of technology and creativity"
- 11:15 a.m. -Discovery Panel: "Pushing the limits of knowledge to inspire new generations"
- 12:30 p.m. -Luncheon speaker: Mr. John W. Rowe, Chairman, President and CEO, Exelon Corporation
- 1:45 p.m. - Inspiration Panel: "Building idea factories for the future"

For more information on NASA's 50th Anniversary Future Forums, visit:

http://www.nasa.gov/50th/future_forums

For complete biographical information about Dale, visit:

http://www.nasa.gov/about/highlights/dale_bio.html

For more information about the Adler Planetarium, visit:

http://www.adlerplanetarium.org

Cassini Plans Doubleheader Flybys of Saturn's Geyser Moon

As major league baseball readies for the World Series, NASA's Cassini team will come to bat twice this month when the spacecraft flies by Saturn's geyser moon, Enceladus.

The Oct. 9 flyby is an inside pitch -- the closest flyby yet of any moon of Saturn, at only 25 kilometers (16 miles) from the surface. The Oct. 31 flyby is farther out, at 196 kilometers (122 miles).

Scientists are intrigued by the possibility that liquid water, perhaps even an ocean, may exist beneath the surface of Enceladus. Trace amounts of organics have also been detected, raising tantalizing possibilities about the moon's habitability.

While Cassini's cameras and other optical instruments were the focus of an Aug. 11 flyby, during Cassini's Oct. 9 flyby, the spacecraft's fields and particles instruments will venture deeper into the plume than ever before, directly sampling the particles and gases. The emphasis here is on the composition of the plume rather than imaging the surface.

"We know that Enceladus produces a few hundred kilograms per second of gas and dust and that this material is mainly water vapor and water ice," said Tamas Gambosi, Cassini scientist at the University of Michigan, Ann Arbor. "The water vapor and the evaporation from the ice grains contribute most of the mass found in Saturn's magnetosphere.

"One of the overarching scientific puzzles we are trying to understand is what happens to the gas and dust released from Enceladus, including how some of the gas is transformed to ionized plasma and is disseminated throughout the magnetosphere," said Gambosi.

On Oct. 31, the cameras and other optical remote sensing instruments will be front and center, imaging the fractures that slash across the moon's south polar region like stripes on a tiger.

These two flybys might augment findings from the most recent Enceladus flyby, which hint at possible changes associated with the icy moon. Cassini's Aug. 11 encounter with Enceladus showed temperatures over one of the tiger-stripe fractures were lower than those measured in earlier flybys. The fracture, called Damascus Sulcus, was about 160 to 167 Kelvin (minus 171 to minus 159 degrees Fahrenheit), below the 180 Kelvin (minus 136 degrees Fahrenheit) reported from a flyby in March of this year.

"We don't know yet if this is due to a real cooling of this tiger stripe, or to the fact that we were looking much closer, at a relatively small area, and might have missed the warmest spot," said John Spencer, Cassini scientist on the composite infrared spectrometer, at the Southwest Research Institute, Boulder, Colo.

Results from Cassini's magnetometer instrument during the August flyby suggest a difference in the intensity of the plume compared to earlier encounters. Information from the next two flybys will help scientists understand these observations.

Four more Enceladus flybys are planned in the next two years, bringing the total number to seven during Cassini's extended mission, called the Cassini Equinox Mission. The next Enceladus doubleheader will be November 2 and 21, 2009.

The Enceladus geysers were discovered by Cassini in 2005. Since then, scientists have been intrigued about what powers them, because the moon is so tiny, roughly the width of Arizona at only 500 kilometers (310 miles) in diameter.

"The October doubleheader gives Cassini two more opportunities to hit the ball out of the park," said Bob Pappalardo, Cassini project scientist at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "With high scores in geology, surface heat, watery plumes and magnetospheric effects, Enceladus could win the 'world championship' title this year!"

Scientists anticipate reporting results from the two flybys in November and early December.

Cassini has been orbiting Saturn since 2004. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. JPL manages the Cassini-Huygens mission for NASA's Science Mission Directorate. The Cassini orbiter was designed, developed and assembled at JPL.

For images, videos and a mission blog on the flyby, visit: http://www.nasa.gov/cassini . More information on the Cassini mission is also available at http://saturn.jpl.nasa.gov .

SMALL ASTEROID TO LIGHT UP SKY OVER AFRICA

An asteroid measuring several feet in diameter is expected to enter the atmosphere over northern Sudan before dawn Tuesday, setting off a potentially brilliant natural fireworks display.

It is unlikely any sizable fragments will survive the fiery passage through Earth's atmosphere. The event is expected to occur at 5:46 a.m. local time (10:46 p.m. EDT Monday).

"We estimate objects this size enter Earth's atmosphere once every few months," said Don Yeomans of the Near-Earth Object Office at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "The unique aspect of this event is that it is the first time we have observed an impacting object during its final approach."

The small space rock, designated 2008 TC3, will be traveling on an eastward trajectory that will carry it toward the Red Sea.

"Observers in the region could be in for quite a show," Yeomans said. "When the object enters the atmosphere, it could become an extremely bright fireball."

The small space rock first was observed by the Mount Lemon telescope of the NASA-funded Catalina Sky Survey early Monday. NASA detects and tracks asteroids and comets passing close to Earth. The Near Earth Object Observation Program, commonly called "Spaceguard," plots the orbits of these objects to determine if any could be potentially hazardous to our planet.

For more information, visit:

http://neo.jpl.nasa.gov/

Monday, October 6, 2008

NASA Spacecraft Finds the Sun is Not a Perfect Sphere

Scientists using NASA’s RHESSI spacecraft have measured the roundness of the sun with unprecedented precision. They find that it is not a perfect sphere. During years of high solar activity the sun develops a thin “cantaloupe skin” that significantly increases its apparent oblateness: the sun’s equatorial radius becomes slightly larger than its polar radius. Their results appear the Oct. 2nd edition of Science Express.

“The sun is the biggest and therefore smoothest object in the solar system, perfect at the 0.001% level because of its extremely strong gravity,” says study co-author Hugh Hudson of UC Berkeley. “Measuring its exact shape is no easy task.”

The team accomplished the task by analyzing data from the Reuven Ramaty High-Energy Solar Spectroscopic Imager, RHESSI for short, an x-ray/gamma-ray space telescope launched in 2002 on a mission to study solar flares. Although RHESSI was never intended to measure the roundness of the sun, it has turned out ideal for the purpose. RHESSI observes the solar disk through a narrow slit and spins at 15 rpm. The spacecraft’s rapid rotation and high data sampling rate (necessary to catch fast solar flares) make it possible for investigators to trace the shape of the sun with systematic errors much less than any previous study. Their technique is particularly sensitive to small differences in polar vs. equatorial radius or “oblateness.”

“We have found that the surface of the sun has rough structure: bright ridges arranged in a network pattern, as on the surface of a cantaloupe but much more subtle,” describes Hudson. During active phases of the solar cycle, these ridges emerge around the sun’s equator, brightening and fattening the “stellar waist.” At the time of RHESSI’s measurements in 2004, ridges increased the sun’s apparent equatorial radius by an angle of 10.77 +- 0.44 milli-arcseconds, or about the same as the width of a human hair viewed one mile away.

“That may sound like a very small angle, but it is in fact significant,” says Alexei Pevtsov, RHESSI Program Scientist at NASA Headquarters. Tiny departures from perfect roundness can, for example, affect the sun’s gravitational pull on Mercury and skew tests of Einstein’s theory of relativity that depend on careful measurements of the inner planet’s orbit. Small bulges are also telltale signs of hidden motions inside the sun. For instance, if the sun had a rapidly rotating core left over from early stages of star formation, and if that core were tilted with respect to its outer layers, the result would be surface bulging. “RHESSI’s precision measurements place severe constraints on any such models.”

The “cantaloupe ridges” are magnetic in nature. They outline giant, bubbling convection cells on the surface of the sun called “supergranules.” Supergranules are like bubbles in a pot of boiling water amplified to the scale of a star; on the sun they measure some 30,000 km across (twice as wide as Earth) and are made of seething hot magnetized plasma. Magnetic fields at the center of these bubbles are swept out to the edge where they form ridges of magnetism. The ridges are most prominent during years around Solar Max when the sun’s inner dynamo “revs up” to produce the strongest magnetic fields. Solar physicists have known about supergranules and the magnetic network they produce for many years, but only now has RHESSI revealed their unexpected connection to the sun’s oblateness.

“When we subtract the effect of the magnetic network, we get a ‘true’ measure of the sun’s shape resulting from gravitational forces and motions alone,” says Hudson. “The corrected oblateness of the non-magnetic sun is 8.01 +- 0.14 milli arcseconds, near the value expected from simple rotation.”

Further analysis of RHESSI oblateness data may help researchers detect a long-sought type of seismic wave echoing through the interior of the sun: the gravitational oscillation or “g-mode.” Detecting g-modes would open a new frontier in solar physics—the study of the sun’s internal core.

A Celestial Landscape in Celebration of 10 Years of Stunning Hubble Heritage Images

The landmark 10th anniversary of the Hubble Space Telescope's Hubble Heritage Project is being celebrated with a "landscape" image from the cosmos. Cutting across a nearby star-forming region are the "hills and valleys" of gas and dust displayed in intricate detail. Set amid a backdrop of soft, glowing blue light are wispy tendrils of gas as well as dark trunks of dust that are light-years in height.

The Hubble Heritage Project, which began in October 1998, has released nearly 130 images mined from the Hubble data archive as well as a number of observations taken specifically for the project. By releasing a new, previously unseen Hubble image every month, the team's intent was to showcase some of the most attractive images ever taken by the Hubble telescope, and share them with a wide audience. The Heritage team continues to create aesthetic images that present the universe from an artistic perspective.

This month's three-dimensional-looking Hubble image shows the edge of the giant gaseous cavity within the star-forming region called NGC 3324. The glowing nebula has been carved out by intense ultraviolet radiation and stellar winds from several hot, young stars. A cluster of extremely massive stars, located well outside this image in the center of the nebula, is responsible for the ionization of the nebula and excavation of the cavity.

The image also reveals dramatic dark towers of cool gas and dust that rise above the glowing wall of gas. The dense gas at the top resists the blistering ultraviolet radiation from the central stars, and creates a tower that points in the direction of the energy flow. The high-energy radiation blazing out from the hot, young stars in NGC 3324 is sculpting the wall of the nebula by slowly eroding it away.

Located in the Southern Hemisphere, NGC 3324 is at the northwest corner of the Carina Nebula (NGC 3372), home of the Keyhole Nebula and the active, outbursting star Eta Carinae. The entire Carina Nebula complex is located at a distance of roughly 7,200 light-years, and lies in the constellation Carina.

This image is a composite of data taken with two of Hubble's science instruments. Data taken with the Advanced Camera for Surveys (ACS) in 2006 isolated light emitted by hydrogen. More recent data, taken in 2008 with the Wide Field Planetary Camera 2 (WFPC2), isolated light emitted by sulfur and oxygen gas. To create a color composite, the data from the sulfur filter are represented by red, from the oxygen filter by blue, and from the hydrogen filter by green.

The Heritage project has released images using several of Hubble's optical cameras: the Wide Field Planetary Camera (WF/PC), which was installed when the telescope was first deployed in 1990; WFPC2, which replaced WFPC in 1993 and is still in service today; and ACS, which was added in 2002. After the Hubble Servicing Mission, which is scheduled for 2009, the Hubble Heritage team hopes to continue using ACS as well as the newest of the optical cameras, Wide Field Camera 3.

Infrared Echoes Give NASA's Spitzer a Supernova Flashback

Hot spots near the shattered remains of an exploded star are echoing the blast's first moments, say scientists using data from NASA's Spitzer Space Telescope.

Eli Dwek of NASA's Goddard Space Flight Center in Greenbelt, Md. and Richard Arendt of the University of Maryland, Baltimore County, say these echoes are powered by radiation from Cassiopeia A supernova shock wave that blew the star apart some 11,000 years ago.

"We're seeing the supernova's first flash," Dwek said.

Previously, other Spitzer researchers discovered hot spots near the Cassiopeia A supernova remnant and recognized the spots' importance as light echoes of the original blast. Dwek and Arendt used Spitzer data to probe this hot dust and pin down the cause of the echoes more precisely.

Six knots of silicate dust near the remnant show temperatures between -173 and -123 degrees Celsius (-280 and -190 degrees Fahrenheit). Although this might seem frigid by earthly standards, such temperatures are downright hot compared to typical interstellar dust.

Writing in the October 1 issue of The Astrophysical Journal, the scientists show that the only event that could make the grains this hot is the powerful and short-lived pulse of ultraviolet radiation and X-rays that heralded the death of the star. The flash was a hundred billion times brighter than the sun, but lasted only a day or so.

"They've identified the precise event during the demolition of the star that produces the echo we see," said Michael Werner, the project scientist for Spitzer at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

Light from the explosion reached Earth in the 17th century, but no one noticed. The Spitzer find gives astronomers a second chance to study the supernova as it unfolds.

Although the explosion originally escaped detection, its aftermath -- a hot, expanding gas cloud known as Cassiopeia A (Cas A, for short) -- is one of the best-studied supernova remnants. The blast zone lies 11,000 light-years away in the constellation Cassiopeia.

When a massive star runs out of nuclear fuel, its core collapses into a superdense, city-sized object called a neutron star. As the neutron star forms, it stiffens and rebounds. This triggers a mammoth shock wave that blows the star's outer layers to smithereens. The exiting shock creates a high-energy flash that precedes the supernova's rise in visible light.

Evidence for a flash associated with this "shock breakout" existed only in computer simulations until January 9, 2008. That's when NASA's Swift satellite detected a 5-minute-long X-ray pulse from galaxy NGC 2770. A few days later, a new supernova -- designated SN 2008D -- appeared in the galaxy.

The infrared echoes from Cas A arise from dust clouds about 160 light-years farther away than the remnant. The supernova's initial radiation pulse expands through space at the speed of light, then encounters the clouds and heats their dust grains. The dust, in turn, re-radiates the energy at infrared wavelengths.

The breakout radiation took 160 years to reach the clouds and, once heated, the dust's infrared energy had to make up the same distance. This extra travel time results in a 320-year offset between the supernova's initial outward-moving flash and arrival of the dust's infrared echo at Earth. The researchers plan to use the echoes to paint an intimate portrait of the explosion, the star and the immediate environment.

When light from the Cas A supernova first reached Earth in the late 1600s, no one reported seeing a new star. On August 16, 1680, the English astronomer John Flamsteed might have seen the supernova without recognizing it. He recorded a faint naked-eye star near the position of Cas A, but none exists there now.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology, also in Pasadena. Caltech manages JPL for NASA.

More information about Spitzer is at http://www.spitzer.caltech.edu/spitzer and http://www.nasa.gov/spitzer .

NASA Selects Science Teams for Astrobiology Institute

NASA has awarded five-year grants, averaging $7 million each, to 10 research teams from across the country, including two from NASA's Jet Propulsion Laboratory in Pasadena, to study the origins, evolution, distribution and future of life in the universe.

The interdisciplinary teams will become new members of the NASA Astrobiology Institute, located at NASA's Ames Research Center at Moffett Field, Calif. Teams from the University of Hawaii in Honolulu; Arizona State University in Tempe; the Carnegie Institution of Washington; Pennsylvania State University in University Park, Pa.; the Georgia Institute of Technology in Atlanta; and Rensselaer Polytechnic Institute in Troy, N.Y., have been selected as members. Teams from Ames and NASA's Goddard Space Flight Center in Greenbelt, Md., also have been selected.

"The research of these new teams reflects the increasing maturity of astrobiology," said NASA Astrobiology Institute Director Carl Pilcher of Ames. "They are focused on fundamental questions of life in the universe, but their work has implications for all of science. The research of these teams, together with that of the four continuing institute teams, will bridge the basic science of astrobiology to NASA's current and planned space exploration missions."

The first of two JPL teams will be devoted to an interdisciplinary investigation of chemistry on Saturn's moon Titan. The team will focus on Titan's physical environment to provide a basis for understanding the chemistry of early Earth, which was the precursor for life. The second JPL team will investigate the habitability of icy worlds, such as Saturn's moons Titan and Enceladus, and Jupiter's moon Europa. They also will investigate how life could be detected in such environments and begin to define related instrumentation for future missions.

The University of Hawaii will investigate the origin, history, and distribution of water and its relation to life in the universe.

Arizona State University will develop new, more refined criteria to guide the search for life by characterizing life's elemental requirements. This will be developed by a "follow the elements" strategy for investigating habitability in extraterrestrial environments.

Carnegie Institution of Washington will conduct a wide range of research. They will focus on life's chemical and physical evolution, from the interstellar medium, through planetary systems, to the emergence and detection of life.

Rensselaer Polytechnic Institute will conduct a multifaceted, highly integrated, program of interdisciplinary research on setting the stage for life. This will focus on the origins of relevant molecules and habitable environments, and on the processes by which chemical evolution leads to life.

Pennsylvania State University will develop novel approaches to detecting and characterizing life. Investigations will include indicators or signatures of life in mission-relevant ecosystems and ancient rocks, and evaluating the potential for these signatures in extraterrestrial settings.

The Georgia Institute of Technology will pursue the scientific goal of rewinding the tape of life to before the last universal common ancestor of all living organisms. This could shed light on the nature of protein synthesis by the earliest living systems.

Ames will conduct a program of integrative, mission-enabling research to investigate the creation and distribution of early habitable environments in emerging planetary systems. Goddard will evaluate the possible role of organic material from space in the origin of life on Earth, and advance understanding of organics on other worlds.

"The new teams provide a superb foundation for the institute as it enters its second decade," said Jim Green, Planetary Science Division director at NASA Headquarters in Washington. "They bring together the many disciplines necessary for a comprehensive interdisciplinary approach to studying life in the universe."

The new members join four continuing teams led by Montana State University in Bozeman, the Massachusetts Institute of Technology in Cambridge, the University of Washington in Seattle, and the University of Wisconsin in Madison.

For more information about the NASA Astrobiology Institute, its new teams, and NASA's astrobiology program, visit http://astrobiology.nasa.gov .

Thursday, October 2, 2008

When it Comes to Galaxies, Diversity is Everywhere

There's an old saying in astronomy: "Galaxies are like people. They're only normal until you get to know them." That view is supported by a group of astronomers after using NASA's Hubble Space Telescope to study a large number of galaxies in our cosmic backyard.

The detailed survey, called the ACS Nearby Galaxy Survey Treasury (ANGST) program, observed roughly 14 million stars in 69 galaxies. The survey explored a region called the "Local Volume," and the galaxy distances ranged from 6.5 million light-years to 13 million light-years from Earth. The Local Volume resides beyond the Local Group of galaxies, an even nearer collection of a few dozen galaxies within about 3 million light-years of our Milky Way Galaxy.

A typical galaxy contains billions of stars but looks "smooth" when viewed through a telescope, because the stars are blurred together. In contrast, the galaxies in the new survey are close enough to Earth that the sharp "eyes" of Hubble's Advanced Camera for Surveys and Wide Field Planetary Camera 2 can resolve their brightest individual stars. By measuring the brightness and colors of these stars, scientists can derive the local history of star formation within a galaxy and can tease out subtle features in a galaxy's shape.

"Past Hubble observations of the local neighborhood have provided dramatic insights into the star-formation histories of individual galaxies, but the number of galaxies studied in detail has been rather small," said Julianne Dalcanton of the University of Washington in Seattle and leader of the ANGST survey. The survey's results were submitted to The Astrophysical Journal Supplement Series. Another paper that details the star-formation history in galaxy M81 has been submitted to The Astronomical Journal.

"Instead of picking and choosing particular galaxies to study, our survey will be complete by virtue of looking at 'all' the galaxies in the region. This gives us a multi-color picture of when and where all the stars in the local universe formed."

Many stars in nearby galaxies are the fossil equivalents of the active star formation seen in galaxies in the distant universe. "When we look back in time at distant, young galaxies, we see lots of vigorous star formation. However, we can only guess as to what those galaxies might eventually turn into," Dalcanton explained. "Using the galaxies in the nearby universe as a 'fossil record,' we can compare them with young galaxies far away. This comparison gives us a history of star formation and provides a better understanding of the masses, structures, and environments of the galaxies."

Early results of the ANGST survey show the rich diversity of galaxies. Some galaxies are made up entirely of ancient stars, while others have been forming stars nearly continuously during their whole lives. There are even a few examples of galaxies that have only started forming stars in the recent past.

"With these images, we can see what makes each galaxy unique," said team member Benjamin Williams of the University of Washington. "When we look at the distribution and development of stars in each survey galaxy, we can learn how differences in the galaxies' histories have produced the diversity of galaxy shapes and colors."

The ANGST survey also includes maps of many large galaxies, including M81. "With these maps, we can track when the different parts of the galaxy formed," explained Evan Skillman of the University of Minnesota, describing work by students Dan Weisz of the University of Minnesota and Stephanie Gogarten of the University of Washington.

In a separate paper describing the star-formation history in M81, astronomers confirmed that massive spiral galaxies formed most of their stars in the early universe. Analyzing M81's outer disk, the astronomers found that most of the stars formed more than 7 billion years ago, when the universe was half its present age. M81 and other mammoth galaxies also experienced rapid enrichment of heavy elements, such as carbon, through the deaths of massive stars in supernova explosions. "We were surprised by how quickly the elements formed and how the subsequent star-formation rate for the bulk of the stars in M81 changed after that," said Williams, the paper's lead author.

"This rich survey will add to Hubble's legacy, providing a foundation for future studies," Dalcanton said. "The ANGST sample offers superb targets for future multi-wavelength surveys, which will allow us to combine the star-formation maps with the properties of gas and dust in the galaxies. With this information, we will be able to trace the complete cycle of star formation in detail."

NASA TV COVERAGE SET FOR SPACE STATION CREW EXCHANGE

NASA Television will broadcast the launch of the next International Space Station crew Oct. 12 and the landing of the current crew Oct. 23.

NASA's Expedition 18 Commander and Science Officer Mike Fincke, Soyuz Commander and Flight Engineer Yury Lonchakov and spaceflight participant Richard Garriott, a U.S. citizen, are scheduled to launch Sunday, Oct. 12, at 3:01 a.m. EDT from the Baikonur Cosmodrome in Kazakhstan. Their Soyuz TMA-13 craft will dock to the station on Thursday, Oct. 14. Garriot will fly to the station under an agreement with the Russian Federal Space Agency.

NASA Flight Engineer Greg Chamitoff, who has been on the station since June, will remain with Fincke and Lonchakov until the arrival of space shuttle Endeavour on its STS-126 mission, targeted to launch in November. NASA astronaut Sandy Magnus will arrive on that flight to replace Chamitoff, who will come home on Endeavour.

Expedition 17 and Soyuz Commander Sergei Volkov, Flight Engineer Oleg Kononenko and Garriott will return to Earth Thursday, Oct. 23, at about 11:46 p.m. in their Soyuz TMA-12 spacecraft now docked to the station. Volkov and Kononenko have been aboard the complex since April.

From Oct. 8-11, NASA TV will broadcast video b-roll of crew rotation activities, including training, pre-launch events in Baikonur, the Oct. 10 rollout of the Soyuz TMA-13 spacecraft to the launch pad, and the final pre-launch news conference Oct. 11 at noon.

A joint crew news conference with all six crewmembers is scheduled Monday, Oct. 20 with a multi-center question and answer capability for media at NASA centers. A time for the news conference will be set in the near future. A change of command ceremony for the two crews will be broadcast on NASA TV. The time for that event also will be set soon.

The events to be broadcast on NASA TV's public and media channels include (all times approximate, EDT):

Oct. 12,
Sunday 1:15 a.m. - Expedition 18 / spaceflight participant video b-roll of prelaunch activities
2:00 a.m. - Expedition 18 / spaceflight participant live launch coverage (launch scheduled at 3:01 a.m.)
6 a.m. - Expedition 18 / spaceflight participant postlaunch video file

October 14, Tuesday
4 a.m. - Expedition 18 / spaceflight participant Soyuz docking to station and post-docking news conference live coverage (docking scheduled for 4:38 a.m.)
5:30 a.m. - Expedition 17 / spaceflight participant hatch opening to station live coverage (hatch opening scheduled for 6 a.m.)
9 a.m. - Expedition 17 / spaceflight participant docking & hatch opening video file feed

October 23, Thursday
4:45 p.m. - 5:30 p.m. - Expedition 17 / spaceflight participant farewell & Soyuz hatch closure live coverage (hatch closure scheduled for 5:15 p.m.)
8 p.m. - 8:45 p.m. - Expedition 17 / spaceflight participant Soyuz undocking from the station live coverage (undocking scheduled for 8:20 p.m.)
10:30 p.m. - 1:00 a.m. - Expedition 17 / spaceflight participant Soyuz deorbit burn and landing in Kazakhstan live coverage (deorbit burn scheduled for 10:56 p.m.; landing scheduled for 11:46 p.m.)

October 24, Friday
3 a.m. - Expedition 17 / spaceflight participant Soyuz post-landing video file feed

For NASA TV streaming video, downlink and schedule information, visit:

http://www.nasa.gov/ntv

NASA'S MESSENGER SPACECRAFT RETURNS TO MERCURY

A NASA spacecraft will conduct the second of three flybys of Mercury on Oct. 6 to photograph most of its remaining unseen surface and collect science data.

The MErcury Surface, Space ENvironment, GEochemistry, and Ranging, or MESSENGER, spacecraft will pass 125 miles above the planet's cratered surface, taking more than 1200 pictures. The flyby also will provide a critical gravity assist needed for the probe to become, in March 2011, the first spacecraft to orbit Mercury.

"The results from MESSENGER's first flyby of Mercury resolved debates that are more than 30 years old," said Sean C. Solomon, the mission's principal investigator from the Carnegie Institution of Washington. "This second encounter will uncover even more information about the
planet."

During the spacecraft's first flyby on Jan. 14, its cameras returned images of approximately 20 percent of Mercury's surface never before seen by space probes. Images showed that volcanic eruptions produced many of Mercury's plains, its magnetic field appears to be actively generated in a molten iron core, and the planet has contracted more than previously thought.

"This second flyby will show us a completely new area of Mercury's surface, opposite from the side of the planet we saw during the first," said Louise M. Prockter, instrument scientist for the
spacecraft's Mercury Dual Imaging System at the Johns Hopkins University Applied Physics Laboratory, or APL, in Laurel, Md.

The second flyby is expected to yield more surprises about the unique physical processes governing Mercury's atmosphere, as well as additional information about the charged particles located in and around Mercury's dynamic magnetic field. An altimeter on the spacecraft will measure the planet's topography, allowing scientists, for the first time, to correlate high-resolution topography measurements with high-resolution images.

A major goal of the orbital phase of the mission is to determine the composition of Mercury's surface. Instruments designed to make those measurements will get another peek at Mercury during this flyby.

"We will be able to do the first test of differences in the chemical compositions between the two hemispheres viewed in the two flybys," said Ralph McNutt, the mission's project scientist at APL. "Instruments also will provide information about portions of Mercury's surface in unprecedented detail."

The spacecraft is more than halfway through a 4.9-billion-mile journey to enter orbit around Mercury that includes more than 15 trips around the sun. In addition to flying by Mercury, the spacecraft flew past Earth in August 2005 and past Venus in October 2006 and June 2007. The project is the seventh in NASA's Discovery Program of low-cost, scientifically focused space missions. The spacecraft was designed and built by APL. The mission also is managed and operated by APL for NASA's Science Mission Directorate in Washington.

For more information about the mission, visit:

www.nasa.gov/messenger

NASA EXTENDS INTERNATIONAL SPACE STATION CONTRACT

NASA has awarded a two-year, $650 million contract extension to The Boeing Co. to continue engineering support of the International Space Station to Sept. 30, 2010.

The action extends the U.S. On-Orbit Segment Acceptance and Vehicle Sustaining Engineering contract, awarded in January 1995. Work under the contract extension will include completion of delivery and on-orbit acceptance of the U.S. segment of the station, sustaining engineering of station hardware and software, support of U.S. hardware and software provided to international partners and participants in the station program, and end-to-end subsystem management for the majority of station systems.

The work will be performed at NASA's Johnson Space Center in Houston, Kennedy Space Center in Florida, Marshall Space Flight Center in Huntsville, Ala., and at other domestic and international locations.

For information about NASA and its programs, visit:

http://www.nasa.gov

Wednesday, October 1, 2008

NASA UPDATES AVIATION SAFETY DATA WEB SITE

NASA will update its National Aviation Operations Monitoring Service, or NAOMS, Web site Tuesday to add more information from pilot survey responses.

The data files are essentially the same files posted to the Web site in late 2007 and early 2008. However, the files are packaged differently and contain fewer redactions than the original postings. Therefore, they provide more information from the NAOMS aviation safety surveys. The surveys were conducted from 2001 through 2004.

This release, in Microsoft Excel format, fulfills NASA's commitment to provide as much information as possible without compromising the anonymity and confidentiality promised to survey participants or the commercial confidentiality of the airlines and organizations involved. It also ensures that aviation safety researchers and the public have access to additional information that may be used to develop future models for safety systems to monitor the National Airspace System. NASA has no plans to post any additional NAOMS information after Sept. 30.

Additional information and the survey responses from the NAOMS project are available at:

http://www.nasa.gov/news/reports/NAOMS.html

NASA MARS LANDER SEES FALLING SNOW, SOIL DATA SUGGEST LIQUID PAST

NASA's Phoenix Mars Lander has detected snow falling from Martian clouds. Spacecraft soil tests experiments also have provided evidence of past interaction between minerals and liquid water, processes that occur on Earth.

A laser instrument designed to gather knowledge of how the atmosphere and surface interact on Mars, detected snow from clouds about 2.5 miles above the spacecraft's landing site. Data show the snow vaporizing before reaching the ground.

"Nothing like this view has ever been seen on Mars," said Jim Whiteway, of York University, Toronto, lead scientist for the Canadian-supplied Meteorological Station on Phoenix. "We'll be looking for signs that the snow may even reach the ground." Phoenix experiments also yielded clues pointing to calcium carbonate, the main composition of chalk, and particles that could be clay. Most carbonates and clays on Earth form only in the presence of liquid water.

"We are still collecting data and have lots of analysis ahead, but we are making good progress on the big questions we set out for ourselves," said Phoenix Principal Investigator Peter Smith of the University of Arizona, Tucson.

Since landing on May 25, Phoenix already has confirmed that a hard subsurface layer at its far-northern site contains water-ice. Determining whether that ice ever thaws would help answer whether the environment there has been favorable for life, a key aim of the mission.

The evidence for calcium carbonate in soil samples from trenches dug by the Phoenix robotic arm comes from two laboratory instruments called the Thermal and Evolved Gas Analyzer, or TEGA, and the wet chemistry laboratory of the Microscopy, Electrochemistry and Conductivity Analyzer, or MECA.

"We have found carbonate," said William Boynton of the University of Arizona, lead scientist for the TEGA. "This points toward episodes of interaction with water in the past."

The TEGA evidence for calcium carbonate came from a high-temperature release of carbon dioxide from soil samples. The temperature of the release matches a temperature known to decompose calcium carbonate and release carbon dioxide gas, which was identified by the
instrument's mass spectrometer.

The MECA evidence came from a buffering effect characteristic of calcium carbonate assessed in wet chemistry analysis of the soil. The measured concentration of calcium was exactly what would be expected for a solution buffered by calcium carbonate.

Both TEGA, and the microscopy part of MECA have turned up hints of a clay-like substance. "We are seeing smooth-surfaced, platy particles with the atomic-force microscope, not inconsistent with the appearance of clay particles," said Michael Hecht, MECA lead scientist at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

The Phoenix mission, originally planned for three months on Mars, now is in its fifth month. However, it faces a decline in solar energy that is expected to curtail and then end the lander's activities before the end of the year. Before power ceases, the Phoenix team will attempt to activate a microphone on the lander to possibly capture sounds on Mars.

"For nearly three months after landing, the sun never went below the horizon at our landing site." said Barry Goldstein, JPL Phoenix project manager. "Now it is gone for more than four hours each night, and the output from our solar panels is dropping each week. Before the end of October, there won't be enough energy to keep using the robotic arm."

The Phoenix mission is led by Smith at the University of Arizona. Project management is the responsibility of JPL with development partnership by Lockheed Martin in Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute.

For more about Phoenix, visit:

http://www.nasa.gov/phoenix

NASA TO DISCUSS HUBBLE ANOMALY AND SERVICING MISSION LAUNCH DELAY

NASA will host a media teleconference at 6 p.m. EDT today to discuss a significant Hubble Space Telescope anomaly that occurred this weekend affecting the storage and transmittal of science data to Earth. Fixing the problem will delay next month's space shuttle Atlantis' Hubble servicing mission.

The briefing participants are:
- Ed Weiler, associate administrator of the Science Mission Directorate at NASA Headquarters in Washington
- John Shannon, Shuttle Program manager at NASA's Johnson Space Center in Houston
- Preston Burch, Hubble manager at NASA's Goddard Space Flight Center in Greenbelt, Md.

To participate in the teleconference, reporters in the U.S. should call 1-800-369-6087 and use the pass code Hubble. International reporters should call 1-773-756-0843.

As a result of the launch delay, NASA has postponed the planned Oct. 3 Flight Readiness Review and subsequent news conference. The review will occur at a later date.

The malfunctioning system is Hubble's Control Unit/Science Data Formatter - Side A. Shortly after 8 p.m. on Saturday, Sept. 27, the telescope's spacecraft computer issued commands to safe the payload computer and science instruments when errors were detected within the Science Data Formatter. An attempt to reset the formatter and obtain a dump of the payload computer's memory was unsuccessful.

Additional testing demonstrates Side A no longer supports the transfer of science data to the ground. A transition to the redundant Side B should restore full functionality to the science instruments and operations.

The transition to Side B operations is complex. It requires that five other modules used in managing data also be switched to their B-side systems. The B-sides of these modules last were activated during ground tests in the late 1980's and/or early 1990, prior to launch. The Hubble operations team has begun work on the Side B transition and believes it will be ready to reconfigure Hubble later this week. The transition will happen after the team completes a readiness review.

Hubble could return to science operations in the immediate future if the reconfiguration is successful. Even so, the agency is investigating the possibility of flying a back-up replacement system, which could be installed during the servicing mission.

Audio of the teleconference will be streamed live at:

http://www.nasa.gov/newsaudio

Related images for the briefing will be available at:

http://www.nasa.gov/hubble

For more information about the Space Shuttle Program, visit:

http://www.nasa.gov/shuttle

NASA TO PREVIEW SECOND MERCURY FLYBY

NASA will host a media teleconference at 1 p.m. EDT on Wednesday, Oct. 1, to preview the Oct. 6 flyby of Mercury by the MErcury Surface, Space ENvironment, GEochemistry, and Ranging, or MESSENGER, spacecraft.

This second of three planned flybys will photograph most of the planet's remaining unseen surface. The spacecraft will pass 125 miles above Mercury's cratered surface, taking more than 1,200 pictures and collecting a variety of data. The flyby also will provide a critical gravity assist needed for the probe to become, in March 2011, the first spacecraft to orbit Mercury.

Briefing participants are:
- Marilyn M. Lindstrom, program scientist, NASA Headquarters in Washington
- Daniel J. O'Shaughnessy, lead for guidance and control subsystem, Johns Hopkins University Applied Physics Laboratory in Laurel, Md.
- Scott L. Murchie, co-investigator, Johns Hopkins University Applied Physics Laboratory
- Sean C. Solomon, principal investigator, Carnegie Institution of Washington

To participate in the teleconference, reporters in the United States should call 1-888-398-6118 and use the pass code Mercury. International reporters should call 1-312-470-7417.

Audio of the teleconference will be streamed live at:

http://www.nasa.gov/newsaudio

Related images for the briefing will be available at:

http://messenger.jhuapl.edu/news_room/index.html

CABANA TO SUCCEED PARSONS AS KENNEDY SPACE CENTER DIRECTOR

NASA announced Tuesday that William Parsons, director of the John F. Kennedy Space Center in Florida, is leaving the agency in mid-October to pursue opportunities in the private sector. Parsons will be succeeded by former astronaut Robert Cabana, currently director of NASA's John C. Stennis Space Center in Mississippi.

Gene Goldman, Stennis' deputy director, will become the acting center director.

Parsons, who joined NASA in 1990, also has served as director of Stennis. His other NASA assignments have included launch site support manager, manager of the Space Station Hardware Integration Office, chief of operations of the Propulsion Test Directorate, Space Shuttle Program manager and deputy director of the Johnson Space Center in Houston.

"It has been my distinct privilege to have gotten to know and work with Bill Parsons since joining NASA as the administrator," NASA Administrator Michael Griffin said. "In managing both centers and programs for NASA, Bill has demonstrated unswerving dedication to the mission and unshakable loyalty to his teammates. I have learned to expect that from marines, and Bill's early training is always in evidence. While wishing him well in his new endeavors, I will miss him greatly."

His successor, Cabana, is a native of Minnesota. He graduated from the U.S. Naval Academy in 1971 with a bachelor of science degree in mathematics and was commissioned as an officer in the U.S. Marine Corps. Cabana is a distinguished graduate of the U.S. Naval Test Pilot School and has logged over 7,000 hours in 36 different aircraft.

After his selection as an astronaut candidate in June of 1985, Cabana completed his training in 1986. He has flown four space shuttle missions, serving as the pilot of Discovery missions STS-41 in October 1990 and STS-53 in December 1992, commander of Columbia on STS-65 in July 1994, and commander of Endeavour on STS-88 - the first International Space Station assembly mission - in December 1998.

Before being named the director at Stennis in October 2007, Cabana served as deputy director of Johnson. In addition, Cabana has worked as chief of NASA's Astronaut Office; manager of international operations of the International Space Station Program; director of NASA's Human Space Flight Program in Russia; deputy director of the International Space Station Program; and director of Flight Crew Operations.

"Bob Cabana is long-time colleague, and another whose marine training has redounded to NASA's benefit," Griffin said. "Bob has seen it all and done it all in human spaceflight, and done it with an open, collaborative style. There is just no better teammate. He will be a terrific successor to Bill Parsons as Director of KSC."

For more information about NASA and agency programs, visit:

http://www.nasa.gov

NASA CHALLENGES STUDENTS TO DESIGN TOOLS FOR MOON ROVERS

A new NASA contest challenges college-level students to design tools or instrument packages that could be used on the next generation of human-driven moon rovers. Student will have the
opportunity to engage in NASA's return to the moon by designing equipment that will help astronauts accomplish tasks on the lunar surface.

Moon explorers will need to navigate in darkness around the moon's south pole and collect lunar regolith, or moon dust, for on-site analysis and radiation detection. They will need to communicate with Earth, a lunar outpost and spacecraft orbiting the moon. Moon inhabitants also will conduct video surveys of the moon's surface for transmission back to Earth, and practice rescue and the safe return of astronauts to their outpost from sorties.

Moon dust has the potential to serve as an on-site resource for building materials, water and oxygen. However, because of its structure, the dust can damage space suits, rovers and other
equipment. The particles have sharp, jagged edges and contain microscopic shards of glass. Tool or instrument designs that can withstand the sharp-edged particles could help future astronauts and might earn students an internship at a NASA facility.

The contest is open to full-time students enrolled in accredited post-secondary institution such as universities, colleges, trade schools, community colleges and professional schools in the United
States or its territories. Individuals or teams may apply, and interdisciplinary teams from across departments and institutions are encouraged.

NASA plans to invite contest winners to the next set of lunar technology mission tests planned for the summer or fall of 2009. Paid internships also are planned as student awards. The contest continues NASA's tradition of investing in the nation's education programs and ties into the agency's goal of strengthening NASA and America's future workforce.

To participate in the contest, students must submit a notice of intent to NASA by Dec. 15, 2008, with final papers due May 15, 2009. Specific details about how participation in the NASA University Design Contest in Exploration Systems, including submission requirements, can be found on the Web at:

http://moontasks.larc.nasa.gov

The contest is sponsored by NASA's Exploration Systems Mission Directorate. For more information about the directorate, visit:

http://www.nasa.gov/exploration

NASA ASSIGNS CREW FOR SPACE SHUTTLE DISCOVERY'S STS-129 MISSION

NASA has assigned the crew for space shuttle Discovery's STS-129 mission. The flight will deliver two experiment racks to the International Space Station.

Marine Col. Charlie Hobaugh will command the mission, which is targeted to launch in October 2009. Navy Capt. Barry Wilmore will serve as the pilot. Mission Specialists are Robert Satcher, Navy Capt. Michael Foreman, Marine Lt. Col. Randy Bresnik and Leland Melvin. Wilmore, Satcher and Bresnik will be making their first trips to space.

The mission will return Canadian Space Agency astronaut and station crew member Robert Thirsk to Earth. This is slated to be the final space shuttle crew rotation flight to or from the space station.

Discovery will deliver parts to the space station, including two spare gyroscopes. The mission will feature four spacewalks. Hobaugh flew as the pilot on STS-104 in 2001 and STS-118 in 2007. He was born in Bar Harbor, Maine. Hobaugh earned a bachelor's degree in aerospace engineering from the U.S. Naval Academy. He was selected as an astronaut in 1996.

Wilmore was born in Murfreesboro, Tenn., and grew up in Mt. Juliet. He has bachelor's and master's degrees in electrical engineering from Tennessee Technological University, and a master's degree in aviation systems from University of Tennessee. He was selected as an astronaut in 2000.

Foreman was born in Columbus, Ohio, but considers Wadsworth his hometown. He earned a bachelor's degree in aerospace engineering from the U.S. Naval Academy and a master's degree in aeronautical engineering from the U.S. Naval Postgraduate School. Foreman flew as a mission specialist on STS-123 in 2008 and performed three spacewalks. He was selected as an astronaut in 1998.

Satcher was selected as an astronaut in 2004. He earned a doctorate in chemical engineering from the Massachusetts Institute of Technology. He also is a graduate of Harvard Medical School. He was born in Hampton, Va.

Bresnik, also selected as an astronaut in 2004. He was born in Fort Knox, Ky., but considers Santa Monica, Calif., his hometown. Bresnik earned a bachelor's degree in mathematics from The Citadel and a master's degree in aviation systems from the University of Tennessee.

Melvin flew as a mission specialist on the STS-122 mission in 2008. He was born in Lynchburg, Va. Melvin earned a bachelor's degree in chemistry from the University of Richmond and a master's degree in materials science engineering from the University of Virginia. He was selected as an astronaut in 1998.

Thirsk will be concluding his long-duration stay on the station when STS-129 launches. He is scheduled to arrive at the complex in May 2009 aboard a Soyuz spacecraft and serve as a flight engineer during parts of Expeditions 20 and 21.

Video of the STS-129 crew members will air on NASA Television's Video File. For downlink and scheduling information and links to streaming video, visit:

http://www.nasa.gov/ntv

For complete astronaut biographical information, visit:

http://www.jsc.nasa.gov/Bios

For more information about NASA's Space Shuttle Program, visit:

http://www.nasa.gov/shuttle

'SMOG BLOG' FOR CENTRAL AMERICA AND CARIBBEAN DEBUTS

NASA and its partners today unveiled a new way to connect satellite air quality data with communities in Central America and the Caribbean. The MesoAmerican and Caribbean Smog Blog, a Web site interpreting local and regional air quality, was introduced at a news conference in Panama City in conjunction with a Global Earth Observation System of Systems (GEOSS) in the Americas symposium.

The Smog Blog provides timely information about air pollution and its sources in the region, helping the public, governments, and health officials monitor air quality and mitigate negative health impacts. The blog is written by faculty and students at the University of Panama and staff from the Water Center for the Humid Tropics of Latin America and the Caribbean (CATHALAC). It is the newest addition to SERVIR (Spanish for "to serve"), a regional environmental monitoring system that leverages the satellite resources of the United States
and other countries to put Earth observation data and other tools into action in Central America.

"CATHALAC has truly taken a leadership role in understanding how NASA atmospheric research information can benefit the citizens of Mesoamerica," said Teresa Fryberger, associate director of Applied Sciences in NASA's Earth Science Division in Washington and co-chair of the U.S. Group on Earth Observations. "With Smog Blog, Central American environmental and health officials will be able to better communicate warnings about hazardous air conditions so the public can take appropriate precautions."

Posts are made at least three times a week by trained personnel using information from satellites, air quality forecast models and soon-to-be-operational ground-based monitors. Satellites from NASA and the National Oceanic and Atmospheric Administration (NOAA) provide air quality information of use to the region. Data from NASA's Terra and Aqua satellites provide a variety of atmospheric measurements. The NASA-French Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation (CALIPSO) satellite mission provides bloggers with data about regional airborne particles. NOAA's Geostationary Operational Environmental Satellites provides continuous monitoring of Earth necessary for timely, intensive data analysis. Another NOAA data asset providing material is a Hazard Mapping System that detects wildfires from space and tracks the smoke they produce.

"The Smog Blog and other activities reflect the work of many partners in supporting the realization of GEOSS in the Western Hemisphere," said Emilio Sempris, director of CATHALAC. "In our region, this exciting initiative is going to improve the quality of life in vital sectors, including public health, energy, weather, climate, and agriculture."

A U.S. Smog Blog has been operated for five years by a team at the University of Maryland Baltimore County. The site draws 35,000 visits a month, mainly state and local air quality forecasters. It is a daily resource for "big picture" analysis of nationwide air quality and insights into how national trends may affect communities locally. Through a NASA cooperative agreement, the U.S. Smog Blog team is working with the SERVIR collaboration to bring this communications tool to Central America.

"The Smog Blog has been a powerful communications tool here in the United States," said Erica Zell, co-developer of the Smog Blog and research scientist for Battelle Memorial Institute. "We hope through sharing real-time air quality information in this region we will make an impact in preventing future harm. Pollution and acid rain have damaged ancient Mayan ruins and air quality has immense public health impacts in this region."

Support for the new Smog Blog is provided by CATHALAC, the University of Panama, the University of Maryland Baltimore County, Panama's national environmental authority, the World Bank and Battelle Memorial Institute. NASA, the U.S. Environmental Protection Agency and the U.S. Agency for International Development fund this initiative.

The Group on Earth Observations is coordinating intergovernmental efforts to build GEOSS, a network designed to better understand, monitor and forecast changes in the global environment. Driven by the 75-government Group on Earth Observations, GEOSS in the Americas is working as a catalyst for regional initiatives by advancing the use of Earth observations, encouraging shared use of data, and leveraging regional assets.

The SERVIR system, developed by researchers at NASA's Marshall Space Flight Center, Huntsville, Ala., was introduced in 2005 in Panama at CATHALAC. SERVIR takes a global approach to environmental challenges by pooling Earth observation tools and data.

To read the MesoAmerican and Caribbean Smog Blog, visit:

http://www.nasa.gov/servir