Monday, September 29, 2008

NASA ASTRONAUT IN SPACE CHALLENGES EARTHLINGS IN CHESS MATCH

It will be Earth vs. space in a unique chess match, and you can help Earth win. NASA and the U.S. Chess Federation (USCF) are teaming up to host the first public chess match between International Space Station astronaut Greg Chamitoff and the inhabitants of the Earth, beginning Monday, Sept. 29.

Key players in the game will be the kindergarten through third grade U.S. Chess Championship Team and its chess club teammates from Stevenson Elementary School in Bellevue, Wash. The K-3 champions will select up to four possible moves on Earth's turn. The public then will vote on the move transmitted to orbit. The USCF will facilitate the match on its Web site at:

http://www.uschess.org/nasa2008

"For the past 10 years, the International Space Station has been an important platform to learn about living in space. We're excited to have the opportunity to engage not only young students, but the public at large in this unique chess match," said Heather Rarick, lead flight director for the current space station mission at NASA's Johnson Space Center in Houston.

"We hope the excitement and interest this game generates will inspire students to become interested in chess," said USCF Executive Director Bill Hall. "Chess is a valuable tool to lead students to become interested in math and to develop critical thinking skills, objectives we focus on in our work with schools nationwide."

Chamitoff, a space station flight engineer speeding about 210 miles above the Earth at five miles a second, is a chess aficionado. He brought a chess set with him when he arrived at the complex on the STS-124 space shuttle mission in June. Chamitoff has added Velcro to the chess pieces to keep them from floating away in weightlessness. He has been playing long-distance chess during his mission in his off time with station control centers around the world. So far, he is undefeated.

The game against the public will move at a pace of one move per day on weekdays only. Play may be slower, however, because Chamitoff only makes moves when his workload permits.

For more information about the USCF, visit:

http://www.uschess.org

For more about Chamitoff and the space station, visit:

http://www.nasa.gov/station

NASA AMES AWARDS CONTRACT FOR INTELLIGENT SYSTEMS SUPPORT

NASA's Ames Research Center Friday awarded a contract with a maximum value of $300 million to Stinger Ghaffarian Technologies Inc. (SGT Inc.), of Greenbelt, Md., for intelligent systems research and development support.

Under the terms of the contract, SGT Inc. will provide support to the Intelligent Systems Division at Ames. The division conducts scientific research, develops technologies, builds applications and deploys advanced information systems technology into NASA missions and other federal government projects. Project areas include autonomous systems and robotics, collaborative and assistant systems, discovery and systems health, robust software engineering, and software systems engineering and software project management. Work will be performed at Ames.

The contract is a cost plus fixed-fee indefinite delivery, indefinite quantity, single award task order with a two-year base performance period, followed by three one-year options.

For more information about NASA's Ames Research Center, visit:

http://www.nasa.gov/ames

For more information about NASA and agency programs, visit:

http://www.nasa.gov

Thursday, September 25, 2008

NASA DISCUSSES LUNAR EXPLORATION CONCEPTS AND PLANS

NASA managers briefed industry representatives, members of academia and reporters Thursday about the agency's initial plans for the Ares V heavy-lift rocket and Altair lunar lander. The Ares V and Altair are part of a fleet of vehicles NASA is developing for a new space transportation system designed to travel beyond low Earth orbit and return humans to the moon by 2020.

Interested participants from throughout the aerospace community attended the forum to discuss the outcomes of a nine-month lunar transportation capabilities study, conceptual designs for the rocket and lunar lander, and near-term business opportunities. NASA is planning to release a Request for Proposals for Altair and Ares V in early 2009, and make awards in spring 2009.

Participants from NASA's Exploration Systems Mission Directorate included Doug Cooke, deputy associate administrator for the directorate, Jeff Hanley, manager of NASA's Constellation Program, and Geoff Yoder, director of the Constellation Systems Division.

Briefing charts from the event are available online at:

http://www.nasa.gov/directorates/esmd/home/lunar_id.html

NASA Television will rebroadcast the forum on its public channel Thursday at 4 and 9 p.m. EDT. For NASA TV downlink, schedule and streaming video information, visit:

http://www.nasa.gov/ntv

NASA's Constellation fleet also includes the Orion crew exploration vehicle and the Ares I launch vehicle. NASA plans to establish a human outpost on the moon through a successive series of lunar missions. For more information about NASA's Constellation Program, visit:

http://www.nasa.gov/constellation

NASA ORBITER REVEALS ROCK FRACTURE PLUMBING ON MARS

NASA's Mars Reconnaissance Orbiter has revealed hundreds of small fractures exposed on the Martian surface that billions of years ago directed flows of water through underground Martian sandstone.

Researchers used images from the spacecraft's High Resolution Imaging Science Experiment, or HiRISE, camera. Images of layered rock deposits at equatorial Martian sites show the clusters of fractures to be a type called deformation bands, caused by stresses below the surface in granular or porous bedrock.

"Groundwater often flows along fractures such as these, and knowing that these are deformation bands helps us understand how the underground plumbing may have worked within these layered deposits," said Chris Okubo of the U.S. Geological Survey in Flagstaff, Ariz.

Visible effects of water on the color and texture of rock along the fractures provide evidence that groundwater flowed extensively along the fractures.

"These structures are important sites for future exploration and investigations into the geological history of water and water-related processes on Mars," Okubo and co-authors state in a report published online this month in the Geological Society of America Bulletin.

Deformation band clusters in Utah sandstones, as on Mars, are a few yards wide and up to a few miles long. They form from either compression or stretching of underground layers, and can be
precursors to faults. The ones visible at the surface have become exposed as overlying layers erode away. Deformation bands and faults can strongly influence the movement of groundwater on Earth and appear to have been similarly important on Mars, according to this study.

"This study provides a picture of not just surface water erosion but true groundwater effects widely distributed over the planet," said Suzanne Smrekar, deputy project scientist for the Mars Reconnaissance Orbiter at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "Ground water movement has important implications for how the temperature and chemistry of the crust have changed over time, which in turn affects the potential for habitats for past life."

The recent study focuses on layered deposits in Mars' Capen crater, approximately 43 miles in diameter and 7 degrees north of the equator. This formerly unnamed crater became notable due to this discovery of deformation bands within it and was recently assigned a formal name. The crater was named for the late Charles Capen, who studied Mars and other objects as an astronomer at JPL's Table Mountain Observatory in southern California and at Lowell
Observatory, Flagstaff, Ariz.

The HiRISE camera is one of six science instruments on the orbiter. It can reveal smaller details on the surface than any previous camera to orbit Mars. The orbiter reached Mars in March 2006 and has returned more data than all other current and past missions to Mars combined.

The mission is managed by JPL for NASA's Science Mission Directorate. Lockheed Martin Space Systems of Denver built the spacecraft. The University of Arizona operates the HiRISE camera, built by Ball Aerospace and Technology Corp. of Boulder, Colo.

Images of the deformation band clusters and additional information about the mission are on the Internet at:

http://www.nasa.gov/mro

For more information about NASA and agency programs, visit:

http://www.nasa.gov

LIVE SPACE TALK NOW AVAILABLE 24/7 ON NASA WEB SITE

Conversations between astronauts aboard the International Space Station and flight controllers on the ground now are available for the public to hear live, 24 hours a day, seven days a week on NASA's Web site, www.nasa.gov .

The streaming audio of space-to-ground communications includes NASA commentary during specific station mission events and regularly scheduled space station commentary on NASA Television Monday through Friday at 10 a.m. Central time. NASA already provides this space-to-ground communication with commentary during space shuttle missions.

The streaming station and shuttle mission audio is available on the following NASA sites:

- Under the NASA TV (Live) tab at:

http://www.nasa.gov

- Under the left navigation at:

http://www.nasa.gov/station and http://www.nasa.gov/shuttle

- In the list of channels at:

http://www.nasa.gov/ntv

SEND YOUR NAME AROUND THE EARTH ON NASA'S GLORY MISSION

Members of the public can send their names around Earth on NASA's Glory satellite, the first mission dedicated to understanding the effects of particles in the atmosphere and the sun's variability on our climate.

The "Send Your Name Around the Earth" Web site enables everyone to take part in the science mission and place their names in orbit for years to come. The Web site, where participants can submit their information, is located at:

http://polls.nasa.gov/utilities/sendtospace/jsp/sendName.jsp

Participants will receive a printable certificate from NASA and have their name recorded on a microchip that will become part of the spacecraft. The deadline for submitting names is Nov. 1, 2008.

The Glory satellite will allow scientists to measure airborne particles more accurately from space than ever before. The particles, known as "aerosols," are tiny bits of material found in Earth's atmosphere, like dust and smog.

"Undoubtedly, greenhouse gases cause the biggest climatic effect," said Michael Mishchenko, the Glory project scientist at NASA's Goddard Institute for Space Studies in New York. "But the uncertainty in the aerosol effect is the biggest uncertainty in climate at the present."

Glory will carry two scientific instruments, the Aerosol Polarimetry Sensor, or APS, and the Total Irradiance Monitor, or TIM, and two cameras for cloud identification. The APS instrument will help quantify the role of aerosols as natural and human-produced agents of climate change more accurately than existing measurement tools. The TIM instrument will continue 30 years of measuring total solar irradiance, the amount of energy radiating from the sun to Earth, with improved accuracy and stability. Understanding the sun's energy is an important key to understanding climate change on Earth.

Glory is scheduled for launch in June 2009 from Vandenberg Air Force Base in California. Glory will orbit as part of the Afternoon Constellation, or "A-Train," a series of Earth-observing satellites. The A-Train spacecraft follow each other in close formation, crossing the equator a few minutes apart shortly after 1:30 p.m. local time each day. The A-Train orbits Earth once every 100 minutes.
NASA's Goddard Space Flight Center in Greenbelt, Md., is responsible for Glory project management. Orbital Sciences Corporation in Dulles, Va., is responsible for development, integration and operations of the spacecraft. Raytheon in El Segundo, Calif., is responsible for development of the APS. The Laboratory for Atmospheric and Space Physics in Boulder, Colo., is responsible for the development of the TIM. Glory's cloud cameras were built by Ball Aerospace and Technologies of Boulder.

For more information on Glory, visit:

http://glory.gsfc.nasa.gov

NASA STARDUST CAPSULE TO GO ON DISPLAY AT SMITHSONIAN


Having returned the world's first particles from a comet, NASA's Stardust sample return capsule will join the collection of flight icons in the Smithsonian's National Air and Space Museum in Washington. The capsule will go on public display in the museum's Milestones of Flight Gallery on Oct. 1, the 50th anniversary of NASA.

Stardust, comprising a spacecraft and capsule, completed a seven-year, 3-billion-mile journey in 2006. A tennis racket-like, aerogel-lined collector was extended to capture particles as the spacecraft flew within 150 miles of comet Wild 2 in January 2004. Carrying the collected particles, the capsule returned to Earth Jan. 15, 2006, landing in Utah. Two days later, it was transported to a curatorial facility at NASA's Johnson Space Center in Houston.

"Very few people get to build something, launch it into space, see it be successful and then get it back in their hands," said Karen McNamara, Johnson recovery lead for the Stardust mission. "To be able to share this with the public is phenomenal."

The capsule joins the Wright brothers' 1903 Flyer, Charles Lindbergh's Spirit of St. Louis and the Apollo 11 command module Columbia that carried the first men to walk on the moon.

"The Smithsonian Institution's National Air and Space Museum is delighted to add to the National Collection the Stardust return capsule," said Roger Launius, senior curator of the Division of Space History at the museum. "As one of the premier space science missions of the recent past, Stardust will take its place alongside other iconic objects from the history of air and spaceflight. I look forward to helping to impart more knowledge to our visitors about the
makeup of the universe using this significant and path breaking object."

Hardware provided to the Smithsonian includes actual flight components. Elements relevant to the science goals of the mission remain with NASA.

After successfully completing its mission, Stardust will use its flight-proven hardware to perform a new, previously unplanned investigation. The mission, called Stardust-NExT, will revisit comet 9P/Tempel 1. This investigation will provide the first look at the changes to a comet nucleus produced after a close approach to the sun. It also will mark the first time a comet ever has been revisited.

"Usually, when a piece of your spacecraft goes into the Smithsonian that means the mission's over," said Stardust-NExT project manager Rick Grammier, of NASA's Jet Propulsion Laboratory in Pasadena, Calif. "But the Stardust spacecraft is still doing the job for NASA and in February 2011, it will fly within 120 miles of the comet."

Stardust is a low-cost, Discovery Program mission for NASA's Science Mission Directorate. The Jet Propulsion Laboratory manages the project. Joseph Veverka of Cornell University in Ithaca, N.Y., is the mission's principal investigator. Lockheed Martin Space Systems of Denver manages mission operations.

For information about the Stardust mission on the Web, visit:

http://www.nasa.gov/stardust

Images of the Stardust capsule being prepared for shipment can be found at:

http://www.nasa.gov/centers/johnson/home/stardust.html

NASA Television will air Video File material to illustrate this story. For NASA TV downlink, schedule and streaming video information, visit:

http://www.nasa.gov/ntv

NASA TO DISCUSS PHOENIX MARS MISSION SCIENCE DATA


NASA will hold a media briefing Monday, Sept. 29, at 2 p.m. EDT, to discuss the latest developments, findings and upcoming science opportunities of the Phoenix Mars Lander. The briefing will take place in the NASA Headquarters' James E. Webb Auditorium, 300 E St., S.W., Washington. It will be carried live on NASA Television and on the Web.

Phoenix landed on Mars May 25, and officially ended its prime mission Aug. 26. Now in extended operations, the lander is continuing to study a northern arctic site and investigating if the environment there has ever been favorable for microbial life.

Participants will be:
- Doug McCuistion, director of Mars Exploration Program, NASA Headquarters, Washington
- Barry Goldstein, Phoenix project manager, Jet Propulsion Laboratory, Pasadena, Calif. - William Boynton, lead scientist, Thermal and Evolved-Gas Analyzer, University of Arizona, Tucson
- Michael Hecht, lead scientist, Microscopy, Electrochemistry and Conductivity Analyzer, JPL
- Leslie Tamppari, Phoenix project scientist, JPL
- Jim Whiteway, lead scientist, Phoenix Meteorological Station, York University, Toronto
- Peter Smith, Phoenix principal investigator, University of Arizona

Journalists may ask questions from participating NASA centers. Reporters also may listen or ask questions via phone. To reserve phone lines contact Steve Cole on 202-358-0918.

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

http://www.nasa.gov/ntv

For more information about the Phoenix mission, visit:

http://www.nasa.gov/phoenix

Wednesday, September 24, 2008

NASA ANNOUNCES NEW TARGET LAUNCH DATES, STATUS NEWS CONFERENCE

The target launch date for space shuttle Atlantis' STS-125 mission to service the Hubble Space Telescope has been reset to Oct. 14 at 10:19 p.m. EDT. A news conference is scheduled for Friday, Oct. 3, at NASA's Kennedy Space Center in Florida to announce an official launch date.

With the delay of Atlantis' launch from Oct. 10 to Oct. 14, shuttle Endeavour's STS-126 supply mission to the International Space Station, also will move from Nov. 12 to Nov. 16 at 7:07 p.m. EST. The target launch date adjustments were made Wednesday during the Space Shuttle Program's Flight Readiness Review, which concludes Thursday.

Detailed assessments were presented Wednesday by Mission Operations, Flight Crew Operations, and training divisions affected by the closure of the NASA's Johnson Space Center in Houston, as a result of Hurricane Ike. While vehicle processing at Kennedy continues on schedule, the lost week of training and mission preparation due to the impacts of the storm led to the decision to slip the dates.

The Oct. 3 news conference will follow the Flight Readiness Review, a meeting to assess preparations for the STS-125 mission to Hubble, and will begin no earlier than 4 p.m. EDT.

The briefing participants are:
- Associate Administrator for Space Operations Bill Gerstenmaier
- Deputy Associate Administrator for Programs, Science Mission Directorate Mike Luther
- Space Shuttle Program Manager John Shannon
- STS-125 Launch Director Ed Mango

NASA Television and the agency's Web site will broadcast the briefing live. Media may ask questions from participating NASA locations. Reporters should contact their preferred NASA center to confirm its participation.

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

http://www.nasa.gov/ntv

For more about the two remaining shuttle missions of 2008, visit:

http://www.nasa.gov/shuttle

NASA AND THE LEVINE SCHOOL COMBINE SPACE AND MUSIC

NASA and the Levine School of Music in Washington will host astronaut Leland Melvin, legendary music producer Quincy Jones and musician-producer Pharrell Williams on Thursday, Sept. 25, at 10 a.m. EDT. The school's address is 1901 Mississippi Ave. SE.

More than 300 students from area schools will hear a presentation from Melvin as he discusses being an astronaut and the importance of education. Melvin is a former pro football star who was injured early in his career, but refocused his life as a scientist and became a NASA astronaut.

During Melvin's last mission in space, he took a CD by one of his favorite musicians, Quincy Jones. He will present the flown CD to Jones during the event. Pharrell Williams also will address the students about the importance of music and education.

Since 1976, the Levine School of Music has dedicated itself to bringing the highest quality music education to everyone in the Washington region - regardless of age or ability. Jones and Williams
are models of success in general and music education, as well as role models for the students Levine hopes to reach.

The Town Hall Education Arts and Recreation Campus, also known as THEARC, opened in 2005 and represents a partnership of nine community organizations, including the Levine School of Music, Children's National Medical Center, and the Boys and Girls Club of Greater Washington.

Levine teaches more than 200 students at THEARC each year. Nearly all receive scholarship and outreach support. Overall, the Levine School serves more than 900 students though scholarship and outreach programs.

For more information about NASA, visit:

http://www.nasa.gov

For information about the Levine School of Music, visit:

http://www.levineschool.org

For information about THEARC Center, visit:

http://thearcdc.org

NASA TO PREVIEW NEXT SPACE STATION EXPEDITION

The work of the next International Space Station residents will be previewed in a briefing broadcast on NASA Television at 1 p.m. CDT Thursday, Sept. 25, from NASA's Johnson Space Center. Reporters at participating NASA centers may ask questions.

Expedition 18 Commander Mike Fincke, Flight Engineer and Soyuz Commander Yuri Lonchakov and U.S. spaceflight participant Richard Garriott are scheduled to launch in a Soyuz spacecraft Oct. 12 from the Baikonur Cosmodrome in Kazakhstan. They will arrive at the station Oct. 14. Garriott will return home with the two Russian members of the Expedition 17 crew on Oct. 24. Fincke and Lonchakov will join NASA astronaut Greg Chamitoff, who has been on board the orbiting complex since June.

The briefers who will preview Expedition 18 are:

-- Michael Suffredini, International Space Station Program manager
-- Susan Brand, Expedition 18 increment manager
-- Ron Spencer, Expedition 18 lead flight director
-- Julie Robinson, International Space Station Program scientist

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

http://www.nasa.gov/ntv

For more information about the International Space Station and its crews, visit:

http://www.nasa.gov/station

ULYSSES REVEALS GLOBAL SOLAR WIND PLASMA OUTPUT AT 50-YEAR LOW

Data from the Ulysses spacecraft, a joint NASA-European Space Agency mission, show the sun has reduced its output of solar wind to the lowest levels since accurate readings became available. The sun's current state could reduce the natural shielding that envelops our solar system.

"The sun's million mile-per-hour solar wind inflates a protective bubble, or heliosphere, around the solar system. It influences how things work here on Earth and even out at the boundary of our solar system where it meets the galaxy," said Dave McComas, Ulysses' solar wind instrument principal investigator and senior executive director at the Southwest Research Institute in San Antonio. "Ulysses data indicate the solar wind's global pressure is the lowest we have seen since the beginning of the space age."

The sun's solar wind plasma is a stream of charged particles ejected from the sun's upper atmosphere. The solar wind interacts with every planet in our solar system. It also defines the border between our solar system and interstellar space. This border, called the heliopause, surrounds our solar system where the solar wind's strength is no longer great enough to push back the wind of other stars. The region around the heliopause also acts as a shield for our solar system, warding off a significant portion of the cosmic rays outside the galaxy.

"Galactic cosmic rays carry with them radiation from other parts of our galaxy," said Ed Smith, NASA's Ulysses project scientist at the Jet Propulsion Laboratory in Pasadena, Calif. "With the solar wind at an all-time low, there is an excellent chance the heliosphere will diminish in size and strength. If that occurs, more galactic cosmic rays will make it into the inner part of our solar system."

Galactic cosmic rays are of great interest to NASA. Cosmic rays are linked to engineering decisions for unmanned interplanetary spacecraft and exposure limits for astronauts traveling beyond low-Earth orbit.

In 2007, Ulysses made its third rapid scan of the solar wind and magnetic field from the sun's south to north pole. When the results were compared with observations from the previous solar cycle, the strength of the solar wind pressure and the magnetic field embedded in the solar wind were found to have decreased by 20 percent. The field strength near the spacecraft has decreased by 36 percent. "The sun cycles between periods of great activity and lesser activity," Smith said. "Right now, we are in a period of minimal activity that has stretched on longer than anyone anticipated."

Ulysses was the first mission to survey the space environment over the sun's poles. Data Ulysses has returned have forever changed the way scientists view our star and its effects. The venerable spacecraft has lasted more than 18 years, or almost four times its expected mission lifetime. The Ulysses solar wind findings were published in a recent edition of Geophysical Research Letters.

The Ulysses spacecraft was carried into Earth orbit aboard space shuttle Discovery on Oct. 6, 1990. From Earth orbit it was propelled toward Jupiter, passing the planet on Feb. 8, 1992. Jupiter's immense gravity bent the spacecraft's flight path downward and away from the plane of the planets' orbits. This placed Ulysses into a final orbit around the sun that would take it over its north and south poles.

The Ulysses spacecraft was provided by ESA, having been built by Astrium GmbH (formerly Dornier Systems) of Friedrichshafen, Germany. NASA provided the launch vehicle and the upper stage boosters. The U.S. Department of Energy supplied a radioisotope thermoelectric generator to power the spacecraft. Science instruments were provided by U.S. and European investigators. The spacecraft is operated from JPL by a joint NASA-ESA team.

More information about the Ulysses mission is available on the Web at:

http://ulysses.jpl.nasa.gov

50TH ANNIVERSARY GALA EVENT CARRIED LIVE ON NASA TV AND INTERNET

NASA Television and www.nasa.gov will broadcast a gala event commemorating the agency's Golden Anniversary on Wednesday, Sept. 24, at 8 p.m. EDT.

The invitation-only celebration, organized by the American Institute of Aeronautics and Astronautics (AIAA), is being held at the Smithsonian's National Air and Space Museum Steven F. Udvar-Hazy Center in Chantilly, Va.

The program honors NASA's 50th Anniversary and celebrates the power of innovation and discovery, and recognizes the agency's challenges and achievements over the past five decades. Award-winning journalist and WJLA-TV news anchor Leon Harris will serve as master of ceremonies. Event participants include:

- George Muellner, AIAA president
- U.S. Sen. John Glenn, former Mercury and space shuttle astronaut
- Neil Armstrong, former Gemini and Apollo astronaut
- Michael Griffin, NASA administrator

The event also will feature a video presentation hosted by Gemini and Apollo veteran Jim Lovell and a message from the Expedition 17 crew aboard the International Space Station. The televised program will end with a special performance of "Fly Me to the Moon," directed by
music impresario Quincy Jones and the Space Philharmonic, and performed by Frank Sinatra, Jr.

NASA TV will serve as the video distributor and pool source for the media and general public. For technical information about NASA TV streaming video, downlink and scheduling information, visit:

http://www.nasa.gov/ntv

For more information about the 50th anniversary gala and the AIAA, visit:

http://www.aiaa.org/nasa50

For more information on NASA's Golden Anniversary, visit:

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

Tuesday, September 23, 2008

NASA's Phoenix Lander Might Peek Under a Rock

If the robotic arm on NASA's Phoenix Mars Lander can nudge a rock aside today, scientists on the Phoenix team would like to see what's underneath.

Engineers who develop commands for the robotic arm have prepared a plan to try displacing a rock on the north side of the lander. This rock, roughly the size and shape of a VHS videotape, is informally named "Headless."

"We don't know whether we can do this until we try," said Ashitey Trebi Ollennu, a robotics engineer at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "The idea is to move the rock with minimum disturbance to the surface beneath it. You have to get under it enough to lift it as you push it and it doesn't just slip off the scoop."

The lander receives commands for the whole day in the morning, so there's no way to adjust in mid-move if the rock starts slipping. Phoenix took stereo-pair images of Headless to provide a detailed three-dimensional map of it for planning the arm's motions. On Saturday, Sept. 20, the arm enlarged a trench close to Headless. Commands sent to Phoenix Sunday evening, Sept. 21, included a sequence of arm motions for today, intended to slide the rock into the trench.

Moving rocks is not among the many tasks Phoenix's robotic arm was designed to do. If the technique works, the move would expose enough area for digging into the soil that had been beneath Headless.

"The appeal of studying what's underneath is so strong we have to give this a try," said Michael Mellon, a Phoenix science team member at the University of Colorado, Boulder.

The scientific motive is related to a hard, icy layer found beneath the surface in trenches that the robotic arm has dug near the lander. Excavating down to that hard layer underneath a rock might provide clues about processes affecting the ice.

"The rocks are darker than the material around them, and they hold heat," Mellon said. "In theory, the ice table should deflect downward under each rock. If we checked and saw this deflection, that would be evidence the ice is probably in equilibrium with the water vapor in the atmosphere."

An alternative possibility, if the icy layer were found closer to the surface under a rock, could be the rock collecting moisture from the atmosphere, with the moisture becoming part of the icy layer.

The Phoenix mission is led by Smith at the University of Arizona with project management at NASA's Jet Propulsion Laboratory in Pasadena, Calif., and development partnership at Lockheed Martin in 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.

For more about Phoenix, visit: http://www.nasa.gov/phoenix or http://phoenix.lpl.arizona.edu

Monday, September 22, 2008

NASA AND AIR FORCE WORK TO ESTABLISH HYPERSONIC SCIENCE CENTERS

NASA and the United States Air Force are looking for university and industry partners as they work to advance hypersonic research.

NASA's Aeronautics Research Mission Directorate in Washington and the Air Force Research Laboratory's Office of Science Research at Wright-Patterson Air Force Base in Dayton, Ohio, have released a broad agency announcement describing their intent to establish three national hypersonic science centers. Hypersonic speed is defined as Mach 5, or five times the speed of sound, and faster.

NASA's Fundamental Aeronautics Program and the Air Force Office of Science Research plan to set aside as much as $30 million to fund the centers over five years. The maximum grant will be approximately $2 million a year. The jointly funded program will support university-level basic science or engineering research that provides improved understanding of hypersonic flight.

"We have identified three critical research areas: air-breathing propulsion, materials and structures, and boundary layer control," said James Pittman, principal investigator for NASA's Fundamental Aeronautics Program's Hypersonics Project at NASA's Langley Research Center in Hampton, Va. "These three areas are the biggest hurdles to successful hypersonic flight and low-cost space access using an air-breathing engine."

Details about the announcement and the process for submitting proposals are available at:

http://www.grants.gov

For more information about NASA's aeronautics research, visit:

http://aeronautics.nasa.gov

For more information about NASA and agency programs, visit:

http://www.nasa.gov

NASA's Mars Rover to Head Toward Bigger Crater

NASA's Mars Rover Opportunity is setting its sights on a crater more than 20 times larger than its home for the past two years.

To reach the crater the rover team calls Endeavour, Opportunity would need to drive approximately 12 kilometers (7 miles) to the southeast, matching the total distance it has traveled since landing on Mars in early 2004. The rover climbed out of Victoria Crater earlier this month.

"We may not get there, but it is scientifically the right direction to go anyway," said Steve Squyres of Cornell University, principal investigator for the science instruments on Opportunity and its twin rover, Spirit. "This crater is staggeringly large compared to anything we've seen before."

Getting there would yield a look inside a bowl 22 kilometers (13.7 miles) across. Scientists expect to see a much deeper stack of rock layers than those examined by Opportunity in Victoria Crater.

"I would love to see that view from the rim," Squyres said. "But even if we never get there, as we move southward we expect to be getting to younger and younger layers of rock on the surface. Also, there are large craters to the south that we think are sources of cobbles that we want to examine out on the plain. Some of the cobbles are samples of layers deeper than Opportunity will ever see, and we expect to find more cobbles as we head toward the south."

Opportunity will have to pick up the pace to get there. The rover team estimates Opportunity may be able to travel about 110 yards each day it is driven toward the Endeavour crater. Even at that pace, the journey could take two years.

"This is a bolder, more aggressive objective than we have had before," said John Callas, the project manager for both Mars rovers at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "It's tremendously exciting. It's new science. It's the next great challenge for these robotic explorers."

Opportunity, like Spirit, is well past its expected lifetime on Mars, and might not keep working long enough to reach the crater. However, two new resources not available during the 4-mile drive toward Victoria Crater in 2005 and 2006 are expected to aid in this new trek.

One is imaging from orbit of details smaller than the rover itself, using the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter, which arrived at the Red Planet in 2006.

"HiRISE allows us to identify drive paths and potential hazards on the scale of the rover along the route," Callas said. "This is a great example of how different parts of NASA's Mars Exploration Program reinforce each other."

Other advantages come from a new version of flight software uplinked to Opportunity and Spirit in 2006, boosting their ability to autonomously choose routes and avoid hazards such as sand dunes.

During its first year on Mars, Opportunity found geological evidence that the area where it landed had surface and underground water in the distant past. The rover's explorations since have added information about how that environment changed over time. Finding rock layers above or below the layers already examined adds windows into later or earlier periods of time.

NASA's JPL built and manage the rovers and the Mars Reconnaissance Orbiter for NASA's Science Mission Directorate, Washington.

For images and information about Spirit and Opportunity, visit:

http://www.nasa.gov/rovers

Taback: Godfather to Viking and a Fair Number of Engineers

Project scientist Gerry Soffen called Israel Taback the "father of the Mars Viking Lander," parentage that Taback rejected with his usual wry wit.

"He thought I was because I was responsible for most of the atmosphere surrounding the lander," Taback said. "Remember, there were over 150 Martin (Marietta) people and over 150 Langley people involved -- all talented, outstanding people. It didn't need a father.

"More of a godfather."

That was a role Taback – who passed away on August 30 -- could play naturally and did, from days when Langley was the National Advisory Committee for Aeronautics laboratory and he helped shepherd the X-15's instrumentation through its supersonic flights.

He carried the role through the transition into NASA, when he was chief engineer of one of the first of the new agency's projects, the Lunar Orbiter, which still ranks among NASA's most successful missions. Five Lunar Orbiters circled the moon, three taking pictures of places where Apollo could land, two mapping 99 percent of the lunar surface.

Then Taback went on to become deputy project manager for Mars Viking, in charge of building the lander that provided information that has been used for more than 30 years and will be used when NASA sends astronauts there, scheduled 22 years hence.

"I had the extraordinary opportunity to work under Iz's leadership for more than a decade," said Tom Young, who eventually became director at Goddard Space Flight Center before becoming an aerospace industry executive. "It's hard to imagine what a special thing it is for a young engineer to have that opportunity. Iz is clearly the best systems engineer I've ever known."

Said Fil Cuddihy, who assisted Taback on the technical side of Mars Viking: "I think Iz was just a wise mentor to everybody who had the privilege of working with him. He taught us all."

Small and slight of stature, Taback could teach so well because he had a natural curiosity and the kind of amazing intellect that made him challenge himself by doing things like working out the value of "pi" to 19 decimal places – in his head. For the curious, it's 3.1415926535897932385.

"I never spent a day in eight years without learning something after talking to Iz," said Gus Guastaferro, who worked on the business side of Mars Viking before leaving Langley for private business. "It was like going to school.

"He would ask the question I wouldn't ask. He would say, 'Fundamentally, that doesn't make sense to me. Explain it to me again,' and I would say, 'I'm glad he asked that because I didn't have the courage to ask it.' I wouldn't want my group to think I didn't know."

As much as anything, it was Taback issuing a Socratic challenge.

"He knew the answer," Guastaferro said. "He wanted to see what you were made of. He was testing you, not in a cruel sense and not in an aggressive sense, but in a way of letting you pass muster so he could gain confidence in what you were trying to sell him."

If it was "no sale," well, Taback had ways of dealing with that, too.

"I hadn't been working with NASA long and we had an outside contractor come in and make a presentation to Iz," Cuddihy said. "Iz gently poked and probed, and the guy didn't pay any attention. He had an agenda that he was going to sell.

"Finally, Iz said, 'well, you may be right,' and the guy went on with his presentation. What he didn't know was 'well, you may be right' was Iz saying, 'I'm done with you.' "

No sale.

Norm Crabill, who worked with Taback on Lunar Orbiter and Mars Viking, talked of a Taback technique that disarmed some.

"When you had a product and you gave it to an engineer and they went off and did all of these big computer programs, Iz would say, 'let's see if this is right,' " Crabill remembered. "He would go to a blackboard, even without a slide rule, and he would get an approximate answer. 'Yeah, that's right,' he would say, because the engineer's answer agrees with his approximate answer."

Young remembers sessions with Taback and a blackboard.

"Iz taught us that when you have a difficult technical problem, you don't solve it with meetings," Young said. "You don't solve it with consultants. You solve it by going back to basic principles. When Iz Taback would pick up a piece of chalk and go to a blackboard and say, 'let's go back to basic principles,' it was like watching a great master at work."

What the engineers came to realize was that Taback could do some of the quick calculations because he had already queried them about their methods. It was part of his management style.

"It was 'management by walking around,' " Guastaferro said. "He would walk around the Viking office and say, 'what are you doing?' He'd look at your in-basket and see it piling up because that was the days before e-mail. He would grab it and throw it in the garbage. He would say, 'you don't need that. Get around and talk to the people.' "

The young engineers would, of course, retrieve the contents of their in-basket, but then they would walk over to somebody else, to talk through problems.

There was some question as to whether Taback ever became comfortable with a computer. A chalkboard or a pencil and paper was more to his liking.

When Taback passed away, he was working on a car rack for his new adult tricycle. Two pages of penciled notes, sketches and engineering formulas were worked out, an 88-year-old man seeming to punctuate a 66-year career of engineering with one more design.

Sunday, September 21, 2008

NASA SPACE SHUTTLE ENDEAVOUR MOVES TO LAUNCH PAD 39B

For the first time since July 2001, two shuttles are on the launch pads at the same time at NASA's Kennedy Space Center. Space shuttle Endeavour completed a 4.2-mile journey to
Launch Pad 39B on Friday, Sept. 19, at 6:59 a.m. EDT.

Endeavour left Kennedy's Vehicle Assembly Building at 11:15 p.m. Thursday, traveling at less than 1 mph atop a massive crawler-transporter.

Endeavour will stand by at pad B in the unlikely event that a rescue mission is necessary during space shuttle Atlantis' upcoming mission to repair NASA's Hubble Space Telescope, targeted to launch Oct. 10. After Endeavour is cleared from its duty as a rescue spacecraft, it will be moved to Launch Pad 39A for the STS-126 mission to the International Space Station. That flight is targeted for launch Nov. 12.

Video file of rollout will be available on NASA Television. For NASA TV downlink information, schedules and links to streaming video, visit:

http://www.nasa.gov/ntv

For information about the upcoming shuttle missions, visit:

http://www.nasa.gov/shuttle

NASA'S SWIFT CATCHES FARTHEST-EVER GAMMA-RAY BURST

NASA's Swift satellite has found the most distant gamma-ray burst ever detected. The blast, designated GRB 080913, arose from an exploding star 12.8 billion light-years away.

"This is the most amazing burst Swift has seen," said the mission's lead scientist Neil Gehrels at NASA's Goddard Space Flight Center in Greenbelt, Md. "It's coming to us from near the edge of the visible universe."

Because light moves at finite speed, looking farther into the universe means looking back in time. GRB 080913's "lookback time" reveals that the burst occurred less than 825 million years after the universe began.

The star that caused this "shot seen across the cosmos" died when the universe was less than one-seventh its present age. "This burst accompanies the death of a star from one of the universe's early generations," says Patricia Schady of the Mullard Space Science Laboratory at University College London, who is organizing Swift observations of the event.

Gamma rays from the far-off explosion triggered Swift's Burst Alert Telescope at 1:47 a.m. EDT on Sept. 13. The spacecraft established the event's location in the constellation Eridanus and quickly turned to examine the spot. Less than two minutes after the alert, Swift's X-Ray Telescope began observing the position. There, it found a fading, previously unknown X-ray source.

Astronomers on the ground followed up as well. Using a 2.2-meter telescope at the European Southern Observatory in La Silla, Chile, a group led by Jochen Greiner at the Max Planck Institute for Extraterrestrial Physics in Garching, Germany, captured the bursts fading afterglow.

The telescope's software listens for alerts from Swift and automatically slewed to the burst position. Then, the team's Gamma-Ray Burst Optical/Near-Infrared Detector, or GROND,
simultaneously captured the waning light in seven wavelengths. "Our first exposure began just one minute after the X-Ray Telescope started observing," Greiner says.

In certain colors, the brightness of a distant object shows a characteristic drop caused by intervening gas clouds. The farther away the object is, the longer the wavelength where this fade-out begins. GROND exploits this effect and gives astronomers a quick estimate of an explosion's shift toward the less energetic red end of the electromagnetic spectrum, or "redshift," which suggests its record-setting distance.

An hour and a half later, as part of Greiner's research, the Very Large Telescope at Paranal, Chile, targeted the afterglow. Analysis of the spectrum with Johan Fynbo of the University of Copenhagen established the blasts redshift at 6.7 -- among the most distant objects known.

Gamma-ray bursts are the universe's most luminous explosions. Most occur when massive stars run out of nuclear fuel. As their cores collapse into a black hole or neutron star, gas jets -- driven by processes not fully understood -- punch through the star and blast into space. There, they strike gas previously shed by the star and heat it, which generates bright afterglows.

The previous record holder was a burst with a redshift of 6.29, which placed it 70 million light-years closer than GRB 080913.

Swift, launched in November 2004, has had a banner year. In March, the satellite detected the brightest gamma-ray burst, which was visible to the human eye despite occurring billions of light-years away. And in January, the spacecraft's instruments caught the first X-rays from a new supernova days before optical astronomers saw the exploding star.

Swift is managed by Goddard. It was built and is being operated in collaboration with Penn State University, University Park, Pa., the Los Alamos National Laboratory in New Mexico, and General Dynamics of Gilbert, Ariz., in the U.S. International collaborators include the University of Leicester and Mullard Space Sciences Laboratory in the United Kingdom, Brera Observatory and the Italian Space Agency in Italy, and additional partners in Germany and Japan.

For related images to this release, please visit:

http://www.nasa.gov/mission_pages/swift/bursts/farthest_grb.html

NASA'S KENNEDY SPACE CENTER HOLDS UNIQUE MEDIA EVENT, TCDT

For the first time since July 2001, two space shuttles are on the launch pads at the same time at NASA's Kennedy Space Center.

On Saturday, Sept. 20, media are invited to capture a unique opportunity with both shuttles Atlantis and Endeavour on their respective pads with the rotating service structures rolled back from the vehicles. The structures provide protection from the element and access to the shuttles.

A photo opportunity will be available from 8 to 9:30 a.m. EDT, allowing media to take imagery from several locations near Atlantis on Launch Pad 39A and Endeavour on Launch Pad 39B.

A live static shot of the two shuttles will be available on NASA Television from 6:30 to 9:30 a.m. Video b-roll of the shuttles, including aerial shots, 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

Still images, including aerial shots, will be posted online in Kennedy's media gallery at:

http://mediaarchive.ksc.nasa.gov/index.cfm

New media accreditation is closed for this event. Reporters with Kennedy credentials planning to attend should arrive at Kennedy's news center by 7 a.m. All participants must dress in full-length pants, flat shoes that entirely cover the feet and shirts with sleeves.

The next major milestone for Atlantis' upcoming STS-125 mission will begin when the crew arrives at Kennedy on Sunday, Sept. 21. A full launch dress rehearsal, known as the terminal countdown demonstration test, or TCDT, is scheduled to take place from Sept. 22 to 24.

The seven astronauts and ground crews will participate in various simulated countdown activities, including equipment familiarization and emergency training for the fifth and final shuttle flight to service NASA's Hubble Space Telescope.

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

- Sept. 21 -- STS-125 crew arrival: The astronauts are expected arrive between 5:45 and 7 p.m. at the Shuttle Landing Facility and will make a brief statement. The arrival will be broadcast live on NASA TV.

- Sept. 23 -- STS-125 crew availability: The crew will take news media questions at Launch Pad 39A at 9:40 a.m. The event will be carried live on NASA TV.

- Sept. 24 -- STS-125 crew walkout photo opportunity: The astronauts will depart from the Operations and Checkout Building at 7:45 a.m. wearing their launch and entry suits in preparation for the countdown demonstration test at the launch pad. The walkout will not be
broadcast live, but will be included in the NASA TV Video File.

Dates and times of events are subject to change. Schedule updates are available at 321-867-2525.

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

Media accreditation for TCDT is closed.

Video b-roll of the TCDT activities will be available on the NASA TV Video File.

For information about the STS-125 mission and crew, visit:

http://www.nasa.gov/shuttle

Thursday, September 18, 2008

NASA'S JOHNSON SPACE CENTER TO REOPEN MONDAY AFTER IKE

NASA's Johnson Space Center in Houston is scheduled to reopen Monday, Sept. 22, ending its closure related to Hurricane Ike. Johnson shut down Sept. 11 as Ike approached the Texas coast.

International Space Station flight control is scheduled to resume from Mission Control in Houston during the morning of Friday, Sept. 19. Station flight control was transferred to a backup facility near Austin, Texas, and later, to another facility at the Marshall Space Flight Center in Huntsville, Ala.

The Mission Control Center and other key Johnson facilities are largely unscathed, partly because of extensive preparations and the work of a hurricane rideout team of more than 60 people. However, some center buildings suffered roof, window and facade damage. Several light poles were downed, as were a number of trees. The damage assessment and cleanup continues.

Johnson employees should check the center's Employee Information Line for status updates at 281-483-3351, and are encouraged to contact their supervisors if they have not already done so. NASA has a public Web site to distribute important information for NASA employees and
contractors impacted by Hurricane Ike at:

http://www.nasa.gov/eoc

NASA TO DISCUSS CONDITIONS ON AND SURROUNDING THE SUN

NASA will hold a media teleconference Tuesday, Sept. 23, at 12:30 p.m. EDT, to discuss data from the joint NASA and European Space Agency Ulysses mission that reveals the sun's solar wind is at a 50-year low. The sun's current state could result in changing conditions in the solar system.

Ulysses was the first mission to survey the space environment above and below the poles of the sun. The reams of data Ulysses returned have changed forever the way scientists view our star and its effects. The venerable spacecraft has lasted more than 17 years - almost four times its expected mission lifetime.

The panelists are:
-- Ed Smith, NASA Ulysses project scientist and magnetic field instrument investigator, Jet Propulsion Laboratory, Pasadena, Calif.
-- Dave McComas, Ulysses solar wind instrument principal investigator, Southwest Research Institute, San Antonio
-- Karine Issautier, Ulysses radio wave lead investigator, Observatoire de Paris, Meudon, France
-- Nancy Crooker, Research Professor, Boston University, Boston, Mass.

Reporters should call 866-617-1526 and use the pass code "sun" to participate in the teleconference. International media should call 1-210-795-0624.

To access visuals that will the accompany presentations, go to:

http://www.nasa.gov/topics/solarsystem/features/ulysses-20080923.html

Audio of the teleconference will be streamed live at:

http://www.nasa.gov/newsaudio

NASA ANNOUNCES INFORMATION TECHNOLOGY CONTRACT EXTENSION

NASA has extended the Unified NASA Information Technology Services, or UNITeS, contract with Science Applications International Corporation (SAIC) of San Diego. This extension allows for the completion of an information technology infrastructure realignment and implementation through competition of various NASA agency-wide contracts.

The $214,470,324 contract extension provides NASA with agency-wide information services, information technology services to NASA's Marshall Space Flight Center in Huntsville, Ala., and support for Marshall's Integrated Enterprise Management Program, which combines agency financial resources and travel office information.

The modification provides additional support from Jan. 1, 2009, through Nov. 30, 2009. With this extension, the value of the contract, including options, is approximately $1.1 billion. The UNITeS contact was awarded to SAIC in January 2004.

Marshall's responsibilities for information technology include managing software applications, Web/computer server systems, audiovisual information, telecommunications, information technology security, information technology procurement, documentation storage and protection hardware maintenance. Support under the UNITeS contract includes NASA-wide information technology security, encryption security systems, computer networking and digital imaging.


For more information about NASA and agency programs, visit:

http://www.nasa.gov

NASA ECLIPS: A NEW APPROACH TO LEARNING

NASA is making available a free Web-based educational product to learners of all ages across the country. NASA eClips consists of more than 55 short, 5-10 minute video segments, which are available on-demand via the Internet for the 2008 -2009 school year.

NASA eClips features many of the agency's missions and engages students in the excitement of science and engineering. From the deepest regions of space to hurricanes here on Earth, the goal of NASA eClips is to inspire students to learn more about science and math concepts.

"This new product was designed to respond to the needs of today's educators, and highlights NASA's commitment to providing science, math, technology and engineering resources in a way that is relevant to tomorrow's explorers," said Joyce Winterton, NASA's assistant administrator for education.

Additionally, the NASA eClips program is separated into grade-appropriate topics and designed as a resource for classroom teachers. Accompanying the collection of NASA eClips will be educator guides to provide teachers with examples of how to effectively use the products as instructional tools.

Students, teachers and the general public can look forward to new video and educational content highlighting current research and innovations each week throughout the school year. The number of video clips is expected to grow to more than 220 by next year. The clips are available at:

http://www.nasa.gov/education/nasaeclips

and

http://www.youtube.com/nasaeclips

Partnering with the National Institute of Aerospace in Hampton, Va., CaptionMax of Minneapolis, Internet Archive of San Francisco and YouTube in San Bruno, Calif., allows for the widest distribution of eClips at the lowest cost.

NASA eClips will be featured during Thursday's Future Forum at Boston's Museum of Science. NASA leadership, including astronauts, scientists, and engineers, will discuss the role of space exploration in advancing science, engineering, technology, education and the economy.

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

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

For more information on the National Institute of Aerospace, visit:

http://www.NIAnet.org

Wednesday, September 17, 2008

Space Shuttle Discovery, lighted against the night sky

NASA Selects 'MAVEN' Mission to Study Mars Atmosphere

NASA has selected a Mars robotic mission that will provide information about the Red Planet's atmosphere, climate history and potential habitability in greater detail than ever before.

Called the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft, the $485 million mission is scheduled for launch in late 2013. The selection was evaluated to have the best science value and lowest implementation risk from 20 mission investigation proposals submitted in response to a NASA Announcement of Opportunity in August 2006.

"This mission will provide the first direct measurements ever taken to address key scientific questions about Mars' evolution," said Doug McCuistion, director of the Mars Exploration Program at NASA Headquarters in Washington.

Mars once had a denser atmosphere that supported the presence of liquid water on the surface. As part of a dramatic climate change, most of the Martian atmosphere was lost. MAVEN will make definitive scientific measurements of present-day atmospheric loss that will offer clues about the planet's history.

"The loss of Mars' atmosphere has been an ongoing mystery," McCuistion said. "MAVEN will help us solve it."

The principal investigator for the mission is Bruce Jakosky of the Laboratory for Atmospheric and Space Physics at the University of Colorado at Boulder. The university will receive $6 million to fund mission planning and technology development during the next year. NASA's Goddard Space Flight Center in Greenbelt, Md., will manage the project. Lockheed Martin of Littleton, Colo., will build the spacecraft based on designs from NASA's Mars Reconnaissance Orbiter and 2001 Mars Odyssey missions. The team will begin mission design and implementation in the fall of 2009.

Launched in August 2005, the Mars Reconnaissance Orbiter is a multipurpose spacecraft that carries the most powerful telescopic camera ever flown to another planet. The camera can show Martian landscape features as small as a kitchen table from low orbital altitudes. The mission is examining potential landing sites for future surface missions and providing a communications relay for other Mars spacecraft.

The 2001 Mars Odyssey, launched in April of that year, is determining the composition of the Red Planet's surface by searching for water and shallow buried ice. The spacecraft also is studying the planet's radiation environment.

After arriving at Mars in the fall of 2014, MAVEN will use its propulsion system to enter an elliptical orbit ranging 90 to 3,870 miles above the planet. The spacecraft's eight science instruments will take measurements during a full Earth year, which is roughly equivalent to half of a Martian year. MAVEN also will dip to an altitude 80 miles above the planet to sample Mars' entire upper atmosphere. During and after its primary science mission, the spacecraft may be used to provide communications relay support for robotic missions on the Martian surface.

"MAVEN will obtain critical measurements that the National Academy of Science listed as being of high priority in their 2003 decadal survey on planetary exploration," said Michael Meyer, the Mars chief scientist at NASA Headquarters. "This field of study also was highlighted in the 2005 NASA Roadmap for New Science of the Sun-Earth System Connection."

The Mars Scout Program is designed to send a series of small, low-cost, principal investigator-led missions to the Red Planet. The Phoenix Mars Lander was the first spacecraft selected. Phoenix landed on the icy northern polar region of Mars on May 25, 2008. The spacecraft completed its prime science mission on Aug. 25, 2008. The mission has been extended through Sept. 30.
NASA's Mars Exploration Program seeks to characterize and understand Mars as a dynamic system, including its present and past environment, climate cycles, geology and biological potential.

NASA USES COMMERCIAL MICROGRAVITY FLIGHT SERVICES FOR FIRST TIME

NASA for the first time last week used microgravity research flights aboard commercially-owned aircraft to test hardware and technologies. These flights, on an airplane operated by the Zero Gravity Corporation, simulated the weightless conditions of space.

In addition to numerous NASA experiments, five companies sponsored by the agency's Innovative Partnerships Program flew experiments aboard the reduced-gravity aircraft flights from Ellington Field in Houston. The flights were the first in NASA's Facilitated Access to the Space Environment for Technology Development and Training program, called FAST.

The companies, which are participating in the Small Business Innovation Research program, tested five new technologies Sept. 9-10:

- Pneumatic mining under lunar gravity conditions (Honeybee Robotics of New York)
- Aircraft sensor-logger operations (Metis Design Corporation of Cambridge, Mass.)
- Microgravity flight testing of self-deploying shells (Mevicon Inc. of Sunnyvale, Calif.)
- Virtual sensor test instrumentation operations (Mobitrum Corporation of Silver Spring, Md.)
- Nanofluid coolant testing (nanoComposix, Inc. of San Diego, Calif.)

Representatives of the companies were aboard the aircraft to operate and evaluate their technologies during the flights, which created zero-gravity and lunar-gravity conditions. The technologies will improve air and space vehicle capabilities and support the design of systems for the exploration of the moon and operations there.

NASA's contract with the Zero Gravity Corporation of Las Vegas, which is managed by NASA's Glenn Research Center in Cleveland, is part of an effort to expand the agency's use of commercial services. The flights were conducted from Ellington Field with the nearby Johnson Space Center in Houston providing technical support to the participating experimenters

Weightless conditions are achieved by flying an airplane on a parabolic trajectory. A typical flight lasting two hours consists of 50 parabolas, generating up to 25 seconds of microgravity during each parabola.

Four days of flights originally were scheduled in September, but the approach of Hurricane Ike caused those scheduled Sept. 11-12 to be suspended. An effort will be made to reschedule the flights in the future. NASA's first flights with the Zero Gravity Corporation occurred the week of Aug. 25. More flights are planned in October, November and January.

A call for new proposals for FAST program flights in 2009 will be issued later this month. It will be open to any companies or organizations working on technologies of value to NASA.

For more information about FAST, visit:

http://www.ipp.nasa.gov/ii_fast.htm

For more information about NASA and agency programs, visit:

http://www.nasa.gov

Arctic Sea Ice Reaches Lowest Coverage for 2008

Arctic sea ice coverage appears to have reached its lowest extent for the year and the second-lowest amount recorded since the dawn of the satellite era, according to observations from the NASA-supported National Snow and Ice Data Center at the University of Colorado in Boulder.

While slightly above the record-low minimum set Sept. 16, 2007, this season further reinforces the strong negative trend in summer sea ice extent observed during the past 30 years. Before last year, the previous record low for September was 2005.

In March, when the Arctic reached its annual maximum sea ice coverage during the winter, scientists from NASA and the data center reported that thick, older sea ice was continuing to decline. According to NASA-processed satellite microwave data, this perennial ice used to cover 50-60 percent of the Arctic, but this winter it covered less than 30 percent. Perennial sea ice is the long-lived layer of ice that remains even when the surrounding short-lived seasonal sea ice melts to its minimum extent during the summer.

NASA scientists have been observing Arctic sea ice cover since 1979. NASA developed the capability to observe the extent and concentration of sea ice from space using passive microwave sensors.

The National Snow and Ice Data Center will issue an analysis of the possible causes behind this year's Arctic sea ice conditions during the first week of October. For updates, visit http://nsidc.org/arcticseaicenews.

Friday, September 12, 2008

NASA CONDUCTS FIRST TEST ON NEW MOTOR FOR THE ARES I ROCKET

Engineers at NASA's Marshall Space Flight Center in Huntsville, Ala., have completed first-round testing of a critical motor for NASA's new Ares I rocket. The Ares I is a two-stage rocket that will launch astronauts aboard the Orion crew capsule on missions to the International Space Station and to the moon by 2020.

The ullage settling motor is a small, solid rocket motor that serves two key roles during the launch of the Ares I rocket. During first stage separation, which occurs 125.8 seconds into flight, the motor will fire for four seconds, producing the forward thrust needed to push the second, or upper, stage away from the first stage. This forward thrust also ensures the rocket's liquid fuel is properly pushed to the bottom of the upper stage fuel tank prior to ignition of the J-2X engine that powers the upper stage.

The successful hot-fire test of this new development motor -- the first test in this series -- was conducted Sept. 11 at Marshall. All test objectives were achieved, bringing NASA one step closer to developing America's new space transportation system. This first series of early development testing will consist of four motors. It is scheduled to run through 2009. The second test series is planned for February 2009.

"We are extremely excited about the success of this test that proves we are headed down the correct development path for this program," said Danny Davis, upper stage manager for Ares Projects at Marshall. "We have the right team in place, and we are working a design that will secure America's future in space."

The word "ullage" is taken from the French term "ouillage," which is used in winemaking to describe the space between wine and the top of a storage container, such as a barrel or bottle. In this case, it refers to the space at the top of the first stage fuel tank and the need to push the fuel, or settle it, to the bottom of the tank.

The ullage motor, 9 inches in diameter and 47 inches in length, is similar in design to the booster separation motor used on the space shuttle's reusable solid rocket motor. Eight ullage motors will be arranged in four pairs on the Ares I upper stage aft skirt, which also houses the reaction control system. The aft skirt is located between the upper stage core, which contains the liquid hydrogen and oxygen fuel tanks, and the interstage, which houses the rocket's roll control system.

"We are very excited about this opportunity for our team to practice the basic principles of solid rocket motor design for the Ares I," said Steve Harvison, ullage settling motor design lead at Marshall. "It has been especially beneficial to newer team members who are fresh out of college and eager for this challenge. We are working every engineering aspect of these motors, from technical analysis, modeling and simulations to propellant tailoring work and hands-on developmental testing."

The first Ares I test flight, called Ares I-X, is scheduled for 2009.

NASA's Johnson Space Center in Houston manages the Constellation Program, which includes the Ares I rocket, the Ares V heavy-lift launch vehicle, the Orion crew capsule and the Altair lunar lander. Marshall manages the Ares Projects.

Video of the ullage motor test will be available Friday, Sept. 12, on NASA Television's Video File. For NASA TV downlink, schedule and streaming video information, visit:

http://www.nasa.gov/ntv

For a photo of the test and more information about Ares, visit:

http://www.nasa.gov/mission_pages/constellation/multimedia/ullage_ares.html

HURRICANE IKE IMPACT FELT IN SPACE

Hurricane Ike has delayed the scheduled Friday arrival of a Russian Progress cargo ship at the International Space Station 220 miles above Earth.

The Progress docking was postponed when the space station's control room at NASA's Johnson Space Center in Houston was closed Thursday because of the approaching storm.

Control of the space station was handed to flight controllers at backup facilities near Austin, Texas, and Huntsville, Ala. Because the Mission Control Center in Houston is responsible for commanding many of the station's systems, U.S. and Russian officials agreed to delay the docking.

Russian flight controllers will execute a maneuver to place the Progress spacecraft into a safe orbit away from the station until docking, which is planned for Wednesday, Sept. 17. If Johnson's
control center is not restored to full capability for docking, one of the backup facilities may be used to command the station's systems.

Station Commander Sergei Volkov and Flight Engineers Oleg Kononenko and Greg Chamitoff are awaiting the arrival of the cargo ship. The spacecraft is carrying more than 2 tons of supplies, including food and fuel.

NASA Television may offer coverage of the Progress' arrival. For NASA TV schedule updates, downlinks, and streaming video information, visit:

http://www.nasa.gov/ntv

For more about the crew's activities and station sighting opportunities, visit:

http://www.nasa.gov/station

NASA'S SPACE SHUTTLE ENDEAVOUR TO MOVE TO LAUNCH PAD SEPT. 18

Space shuttle Endeavour is scheduled to roll out to Launch Pad 39B at NASA's Space shuttle Kennedy Space Center on Thursday, Sept. 18, in preparation for Space shuttle Atlantis' Space shuttle mission to repair the Hubble Space shuttle Telescope. Space shuttle Endeavour will stand by in the unlikely event a rescue Space shuttle mission is necessary following Space shuttle Atlantis' launch, which is targeted for Oct. 10.

After Endeavour is cleared from its duty as a rescue vehicle, it will move to Launch Pad 39A for the upcoming STS-126 Space shuttle mission to the International Space Station. That flight is targeted for launch Nov. 12.

On Thursday, Endeavour rolled over from Kennedy's Space shuttle Orbiter Processing Facility to the Vehicle Assembly Building. There, Endeavour will be attached to its external fuel tank and twin solid rocket boosters to prepare for its move to the pad.

The first motion of the Space shuttle toward the launch pad Sept. 18 is scheduled for 12:01 a.m. EDT. The fully assembled space shuttle, consisting of the orbiter, external tank and twin solid rocket boosters, will be delivered to the pad atop a crawler-transporter. The crawler will travel slower than 1 mph during the 4.2-mile journey. The process is expected to take approximately seven hours.

NASA Space shuttle Television will provide live coverage of Endeavour's rollout to the launch pad beginning at 6:30 a.m. Sept. 18. Video highlights of the rollout will air on the NASA Space shuttle TV Video File.

Space shuttle Media are invited to a photo opportunity of the Space shuttle move to the pad and interview availability with Endeavour Vehicle Manager Shelley Ford at 8 a.m. Thursday. Because dates and times of this event are subject to change, updates are available by calling 321-867-2525.

Space shuttle Media must arrive at Kennedy's news center by 6 a.m. Thursday for transportation to the viewing area. Foreign media with credentials must arrive at the Pass and ID Building on State Road 3 by 6 a.m. for transportation to the news center. The accreditation deadline for this event has passed for members of foreign news media. U.S. reporters without permanent Kennedy Space shuttle Center credentials must apply for accreditation online by 4 p.m. Monday, Sept. 15, at:

https://media.ksc.nasa.gov

Badges must be picked up by 4 p.m. Wednesday, Sept. 17 at the new Kennedy Space shuttle Center Badging Office on State Road 405, west of Gate 3 (just past the Kennedy Visitor's Complex).

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

http://www.nasa.gov/ntv

NASA ASTRONAUTS CONNECT WITH LUCKY LAS VEGAS SCHOOL KIDS

Space Station Mission Journalists are invited to join a group of Las Vegas students who have "struck it rich" on Wednesday, Sept. 17. These lucky students will chat with NASA's Space Station Mission Expedition 17 Space Station Mission astronauts aboard the International Space Station from 11:15 a.m. to 11:35 a.m. PDT at the Jim Bridger Middle School. The Space Station Mission school is located at 2505 North Bruce Street in Las Vegas.

A live educational downlink will connect an auditorium filled with hundreds of middle school Space Station Mission students and teachers with space station crewmembers. The Space Station Mission goal is to learn more about what life is like in space and how gravity affects people on Earth. Space Station Mission Reporters interested in attending the event must contact Terry Wood at 414-573-1700 or by e-mail at: tmwood@interact.ccsd.net .

Jim Bridger Middle School is a participant in the NASA Space Station Mission Explorer Schools Program. The program offers a three-year partnership between NASA Space Station Mission and school teams, which consist of teachers and education administrators from diverse communities across the country. Space Station Mission Focusing on underserved populations, the program is designed for education communities at the grade 4-9 levels to help middle schools improve teaching and learning in Space Station Mission, science, technology, engineering and math.

The Space Station Mission downlink event is one in a series with educational organizations in the U.S. and abroad. It is an integral component of NASA's Space Station Mission Teaching from Space Program. The program promotes learning opportunities and builds partnerships with the education community using the unique environment of human Space Station Mission flight.

The downlink will air live on NASA Space Station Mission Television and be streamed on the NASA Web site at:

http://www.nasa.gov/ntv

For information about NASA's Space Station Mission education programs on the Web, visit:

www.nasa.gov/education

For more information about Space Station Mission Jim Bridger Middle School, visit:

http://ccsd.net/schools/bridger

NASA'S JOHNSON SPACE CENTER CLOSES FOR IKE

NASA's Johnson Space Shuttle Station Center will close at noon CDT Thursday and remain closed until the threat of Space Station Hurricane Ike has passed. Ike, a category 2 hurricane in the western Gulf of Mexico, is expected to cross the Texas coast early Saturday as a category 3 storm.

The International Space Station Flight Control Room at Space Shuttle Station Mission Control in Houston was shut down Thursday morning. Space Discovery Station flight control continued through backup teams located near Austin, Texas and Huntsville, Ala.

Most NASA Space Shuttle Station aircraft at Ellington Field, located just north of Johnson, have been flown to a facility in El Paso, Texas. That includes 19 of 26 T-38s, a WB-57 and three of four Space Technology shuttle training aircraft. Nine other Space Shuttle Station aircraft are undergoing maintenance and have been secured in hangars at Ellington.

Space Shuttle Station Johnson employees and journalists should call the Employee Information Line for updated news on the center's status. The local telephone number is 281-483-3351. If local communications are disrupted, employees can call a toll-free information line at 877-283-1947.

NASA Space Shuttle Station has a Web site to convey important information to NASA Space Shuttle Station employees and contractors impacted by Hurricane Ike at:

http://www.nasa.gov/eoc

NASA Video: What's Up for September

NASA AWARDS EDUCATION RESEARCH GRANTS TO MINORITY UNIVERSITIES

NASA's Office of Education is awarding research grants totaling nearly $35 million to seven minority institutions.

The goal of NASA's Minority University Research and Education Program is to establish significant, multi-disciplinary scientific, engineering and commercial research centers at the host universities that contribute substantially to NASA programs. The awards will help to achieve a broad based, competitive aerospace research and technology development capability among the nation's Historically Black Colleges and Universities and Other Minority Universities.

The grants also will help increase participation by faculty and students of selected colleges and universities in the research programs of NASA's mission directorates, and increase the number of underrepresented minorities who obtain advanced degrees in NASA-related fields. Each university will receive up to $1 million per year for a maximum of five years based on performance and availability of funds. NASA's Office of Education intends to issue a cooperative agreement notice for the University Research Center project in the coming fiscal year.

The university organizations selected to receive awards are:

NASA University Research Center SPACE Center, California State University, Los Angeles

WaterSCAPES: Science of Coupled Aquatic Processes in Ecosystems from Space, Florida International University, Miami

Howard University Beltsville Center for Climate System Observation, Howard University, Washington

Center of Excellence in Systems Engineering for Space Exploration Technologies, Morgan State University, Baltimore

The Center for Radiation Engineering and Science for Space Exploration, Prairie View A & M University, Prairie View, Texas

Center for Bio-Nanotechnology and Environmental Research, Texas Southern University, Houston

Center for Advanced Nanoscale Materials II, University of Puerto Rico, Rio Piedras Campus, San Juan

For more information about the awards, visit:

http://mured.nasaprs.com

Next Mars Soil Scoop Slated for Last of Lander's Wet Lab Cells

The next soil sample that NASA's Phoenix Mars Lander will deliver to its deck instruments will go to the fourth of the four cells of Phoenix's wet chemistry laboratory, according to the Phoenix team's current plans.

The chosen source for that sample is from the "Snow White" trench on the eastern end of the work area reachable with Phoenix's robotic arm. In July that trench yielded a sample in which another analytical instrument, the Thermal and Evolved Gas Analyzer (or TEGA), confirmed the presence of water ice. One of the three cells previously used on the wet chemistry laboratory also analyzed a sample from Snow White.

The wet chemistry laboratory mixes Martian soil with purified water brought from Earth as part of its process for identifying soluble nutrients and other chemicals in the soil. Scientists have used it to determine that the soil beside the lander is alkaline and to identify magnesium, sodium, potassium, chloride and perchlorate in the soil.

The Phoenix team plans to fill the last four of eight single-use ovens on the TEGA instrument without waiting for the analysis of each sample to be completed before delivering the next. The strategy is to get as many samples as possible delivered while there is still enough energy available for digging. The northern Martian summer is nearly half over. The amount of sunshine reaching Phoenix's solar panels, and consequently the amount of electricity produced by the panels, is declining.

"Now that the sun is not constantly above the horizon at our landing site we are generating less power every sol," said Phoenix Project Manager Barry Goldstein of NASA's Jet Propulsion Laboratory, Pasadena, Calif. "When we landed in late May, and through much of our mission, we generated about 3,500 watt-hours every sol. We are currently at about 2,500 watt-hours, and sinking daily. With the remaining sols we need to scurry to squeeze the last bit of science out of the mission."

One hundred watt-hours is equivalent to what is needed to illuminate a 100-watt bulb for one hour.

As TEGA bakes samples, it identifies the temperatures at which volatile ingredients in the soil are vaporized. It also has a mass spectrometer to identify the vapors. A valve that controls the flow of a carrier gas for transporting the vapors to the mass spectrometer is no longer reliable, but researchers anticipate that the remaining samples will yield enough vaporized water and carbon dioxide to carry any scarcer vapors to the spectrometer. The team is also examining possible operational workarounds for unanticipated opening of a valve controlling flow of calibration gas.

The Snow White trench is the chosen source for the next sample to go into a TEGA oven, as well as the next sample for the wet chemistry laboratory. For the TEGA sample, the team plans to use a rasp on the robotic arm to churn up ice-rich material from the hard floor of the trench. Ice-rich samples stuck inside the scoop during two attempts in July to deliver them to a TEGA oven. However, a test run on Aug. 30 verified that an ice-rich sample can be delivered using methods that minimize the time the sample is in the scoop and the exposure of the scoop to direct sunlight.

The Phoenix mission is led by Smith at the University of Arizona with project management at NASA's Jet Propulsion Laboratory in Pasadena, Calif., and development partnership at Lockheed Martin in 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.

For more about Phoenix, visit: http://www.nasa.gov/phoenix or http://phoenix.lpl.arizona.edu.

Tuesday, September 9, 2008

NASA TO HOLD BRIEFING ABOUT LUNAR EXPLORATION CONCEPTS AND PLANS

NASA is inviting interested industry representatives, academics and reporters to learn more about the Ares V heavy lift-launch vehicle, the Altair lunar lander, and the roles they will play in returning humans to the moon by 2020.

The Exploration Systems Mission Directorate forum will take place Thursday, Sept. 25, from 8:30 to 11:30 a.m. EDT, at the U.S. Chamber of Commerce, 1615 H Street NW, Washington. The forum will focus on the first phase conceptual designs for the Ares V heavy lift-launch vehicle, the Altair lunar lander and lunar exploration scenarios. Forum attendees will discuss the outcomes of a nine-month lunar transportation capabilities study and near-term business
opportunities.

Participants from NASA's Exploration Systems Mission Directorate include Doug Cooke, deputy associate administrator for the directorate, Geoff Yoder, director of the Directorate Integration
Office, and Jeff Hanley, manager of NASA's Constellation Program.

Representatives of industry and academia interested in attending the forum must register online. Attendance is limited and registration will close at 5 p.m. EDT, Sept. 23. Registration and additional information, including an agenda, are available at:

http://www.nasa.gov/directorates/esmd/home/lunar_id.html

Reporters planning to attend must contact Stephanie Schierholz at 202-358-4997 or Grey Hautaluoma at 202-358-0688 by 5 p.m., Sept. 24.

The Ares V rocket and Altair lunar lander are part of a fleet of vehicles that NASA's Constellation Program is developing for a new space transportation system designed to travel beyond low Earth orbit. The Constellation fleet also includes the Orion crew exploration vehicle and the Ares I launch vehicle. NASA plans to establish a human outpost on the moon through a successive series of lunar missions beginning in 2020.

For more information about NASA's Constellation Program, visit:

http://www.nasa.gov/constellation

NASA DEBUTS 50TH ANNIVERSARY ART BOOK

To celebrate NASA's 50th anniversary in October, the agency is releasing the book "NASA/ART - 50 Years of Exploration," a historic collection of almost a half-century of space-inspired artwork.

In 1962, four years after NASA was founded, Administrator James E. Webb recognized space exploration would make a profound cultural impact, in addition to advancing science and technology. He established the NASA Art Program to commission pieces from prominent artists that would illustrate and interpret the space agency's missions.

Since that time, the art program has enjoyed the participation of such luminaries as Robert Rauschenberg, Norman Rockwell, James Wyeth, Nam June Paik, Patti LaBelle, William Wegman, Mike and Doug Starn, and Annie Leibovitz.

"Through the NASA Art Program, artists have been given an inside glimpse into the missions and programs which make up the space agency," said Bert Ulrich, the program's curator at NASA headquarters in Washington. "Through their imaginations, artists have shared an entirely new interpretation of the NASA story with the public."

In "NASA/ART - 50 Years of Exploration," co-authors James Dean and Ulrich present 150 full color illustrations with essays by astronaut Michael Collins, curator Tom D. Crouch and novelist Ray Bradbury. The book, published by Harry N. Abrams, Inc., New York, will be available in October. It is a companion to the Smithsonian traveling art exhibition drawn from the collections of NASA and the National Air and Space Museum, which features 73 works by some of America's
leading artists.

For more information about the book, "NASA/ART - 50 Years of Exploration, " visit:

http://www.nasa.gov/externalflash/NASAart_book/


Exhibition descriptions and tour schedules are available at:

http://www.sites.si.edu/exhibitions/exhibits/nasa_art/main.htm

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

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

NASA Hometown Heroes 2008: Col. Bob Cabana Visits the Minneapolis Twins

Sporting a flight jacket covered with enough mission patches to make almost any astronaut jealous, Col. Bob Cabana launched out of his childhood Minneapolis home at 5 a.m. and headed for the first of several early morning media interviews.

Cabana’s Aug. 11 visit to his hometown of Minneapolis was the fourth stop on NASA’s Hometown Heroes 2008 campaign. Throughout the summer, astronauts have been traveling back to their hometowns and home regions to throw out the first pitch at Major League Baseball games as part of NASA’s celebration of the International Space Station’s 10th year in orbit. In December 1998, Cabana served as shuttle commander for the first station assembly mission. During that mission, the first U.S. segment of the station, the Unity node, was mated with Zarya, the first Russian segment that was launched a month earlier. “It was great being on the first assembly mission,” Cabana shared with KMSP-TV morning news anchor Tom Butler. “We got to power up the space station and turn on the lights and go inside for the first time.”

Cabana has flown on four shuttle missions during his career with NASA. He was the pilot for STS-41 and STS-53 and the commander for STS-65 and STS-88. Earlier this year he had the distinctive honor of being inducted into the Astronaut Hall of Fame. He currently serves as Director of the NASA Stennis Space Center in Mississippi.

Cabana loves to talk about space and was asked a variety of space-related questions throughout his interviews. Questions that ranged from what it is like to fly the shuttle to what type of research is done on the station to what’s the future of NASA. By the end of the morning he had appeared on three television stations, one radio station and been interviewed by an online newspaper.

That evening, Cabana headed to the Metrodome in downtown Minneapolis where the Minnesota Twins were hosting the New York Yankees. Prior to the game, fans had the opportunity to meet the former shuttle commander during an autograph session in the main concourse.

After throwing out the honorary first pitch of the game, this hometown hero presented the Twins with a photo of Minneapolis taken from the station. Cabana spent the top of the third inning chatting live on-air with the Fox Sports Net broadcast team. Then it was back to the main concourse where he spent the rest of the game signing autographs and taking photographs with enthusiastic space fans.

“It was a great time meeting him,” said Minnesota Twins event marketing director Heidi Sammon. “I think the fans enjoyed him being here and meeting him and we’re thankful that he visited with us.”

The next morning, Cabana started his day at the Minneapolis Central Library. He gave two presentations about the space program and answered questions from the audience. The first presentation was to elementary school students and the second to a group of adults. An autograph session and photo opportunity followed each presentation.

“I like that he was motivating the kids to set goals,” said parent Carol Rettmann. “And we walked away with more questions than answers and I think that’s good. So we’re going to go do more research ourselves.”

By lunchtime Cabana was on the road and heading to a Lockheed Martin research and design facility in nearby Eagan, Minn. He presented an overview of the current state of NASA’s space exploration program and answered questions from the audience. He ended his presentation by thanking the crowd for the support they provide NASA and reminding them they are all important members of America’s space exploration team.

A tour of an onsite aeronautics test lab followed by a short autograph session wrapped up Cabana’s afternoon.

“I think it’s been terrific,” said Frank Parisi, the director of strategic partnerships for the city of Minneapolis. “We forget that we have some talented people like Cabana who have done remarkable things in their lives. And for a large measure of our population I think there was great joy last night. He threw out the first pitch at the Twins game and they beat the Yankees four to nothing! So who could ask for anything more than that?”

Underneath Phoenix Lander 97 Sols After Touchdown

The Robotic Arm Camera on NASA's Phoenix Mars Lander took this image on Sept. 1, 2008, at about 4 a.m. local solar time during the 97th Martian day, or sol, since landing. The view underneath the lander shows growth of the clumps adhering to leg strut (upper left) compared with what was present when a similar image was taken about three months earlier (see http://photojournal.jpl.nasa.gov/catalog/PIA10759).

The view in this Sol 97 image is southward. Illumination is from the early morning sun above the northeastern horizon. This is quite different from the illumination in the Sol 8 image, which was taken in mid-afternoon.

The science team has discussed various possible explanations for these clumps. One suggestion is that they may have started from a splash of mud if Phoenix's descent engines melted icy soil during the landing. Another is that specks of salt may have landed on the strut and began attracting atmospheric moisture that freezes and accumulates. The clumps are concentrated on the north side of the strut, usually in the shade, so their accumulation could be a consequence of the fact that condensation favors colder surfaces.

In this image, compared with the one from three months earlier, the flat, smooth patches of ice exposed underneath the lander seem to be partly covered by darker material left behind as ice vaporizes away. The flat patch in the center of the image has the informal name "Holy Cow," based on researchers' reaction when they saw the initial image of it.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Secret NASA Tape Found Today

Monday, September 8, 2008

REPORT EXPLORES USE OF EARTH DATA TO SUPPORT NATIONAL PRIORITIES

The nation faces challenges in utilizing Earth Space Station Shuttle science information to manage resources and protect public health, according to a NASA Space Station Shuttle sponsored report issued Monday by the U.S. Climate Change Space Station Shuttle Science Program.

The Space Station Shuttle report examines the computer-based decision support tools that many government agencies use to make predictions and forecasts in areas such as agricultural productivity, air quality, renewable energy resources, water management, and the prevention of vector-borne disease.

The authors of "Uses and Limitations of Observations, Data, Forecasts, and Other Projections in Decision Support for Selected Sectors and Regions" found that while these tools have successfully incorporated Earth science information to address a number of issues, they are not yet widely used to investigate the implications of future climate change.

The Space Station Shuttle report is the latest in a series of "synthesis and assessment products" by the U.S. Climate Change Space Station Shuttle Science Program to address various aspects of the country's highest priority research, observation and decision support needs. The Space Station Shuttle study's authors include experts from government, universities and non-governmental organizations.

New sources of Space Station Shuttle Earth information and advances in computing, modeling and analysis systems provide government agencies with new capabilities to enhance the way they manage resources and evaluate policy alternatives that affect local, national and international actions.

"All of the information we have now about Earth's Space Station Shuttle climate, water, air, land, and other dynamic processes is essential for understanding humankind's relationship to natural resources and our environment," said Molly Macauley of Resources for the Future in Washington, one of the report's lead authors. "We hope this report will give decision-makers a greater understanding of the valuable information resources available to them."

The Space Station Shuttle study examines a broad range of decision support tools that have the potential to address climate change impacts. The authors selected five for in-depth review. The tools are currently in use at the Department of Agriculture, the Environmental Protection Agency, the Department of Energy, the Centers for Disease Control and Prevention, the Department of Interior, and the Army Corps of Engineers.

Four of the tools examined - in the areas of agricultural efficiency, air quality, water management, and energy management - are well-established as a basis for public policy decision making, according to the report. However, the use of Earth information in public health decisions, such as the system developed to prevent the spread of Lyme disease in the United States, is a relatively new application area.

One of the major challenges facing increased use of Earth information for decision making is accounting for the degree of uncertainty in the results of these Space Station Shuttle systems. Like all computer models and data, there are many sources of uncertainty, including the accuracy of the data as well as assumptions in the modeling that underlie the decision-support tools. The report found that with all the tools investigated, the agencies are using various methods to understand the effects of uncertainty and clearly communicate the confidence levels of the information they produce.

The availability of data is also a limitation. For example, a challenge for the Department of Energy's model - used to decide where to build renewable energy technologies - is the lack of direct measurements of wind and solar radiation in specific locations. Incorporation of more satellite-based Earth data in all of the decision-support Space Station Shuttle systems is hampered by the fact much of the data is from short-term research missions that do not guarantee the type of long-term delivery of data to users as operational systems.

The Space Station Shuttle report concludes the value of these tools for forecasting impacts of a changing climate is largely unexplored. "Most of the agencies in this report have not yet made extensive use of climate change information, or used their decision tools to study the effect of a changing climate on the resources they manage," Macauley said.

Of the five systems evaluated, only the U.S. Centers for Space Station Shuttle Disease Control and Space Station Shuttle Prevention's Lyme disease prevention system has explicitly evaluated the potential impact of climate change scenarios. None of the other systems are directly integrated with climate change measurements, but all can and may in the future take this step, according to the study.

Federal agencies contributing to the report Space Station Shuttle include the Department of Energy, the Environmental Protection Agency, the National Oceanic and Atmospheric Administration, the U.S. Agency for International Space Station Shuttle Development, and the U.S. Space Station Shuttle Geological Survey.

The complete report is available on the Web at:

http://www.climatescience.gov/Library/sap/sap5-1/final-report/default.htm

NASA TO BRIEF MEDIA ABOUT COMPLETION OF ARES I ROCKET DESIGN REVIEW

NASA Space Station Shuttle will host a teleconference Wednesday, Sept. 10, no earlier than 6 p.m. EDT, to discuss the conclusion of the Nasa Space Station Shuttle Ares I rocket preliminary design review.

The review, conducted at NASA's Space Station Shuttle Marshall Center Space Flight Center in Huntsville, Ala., examines the current design for the Space Station Shuttle Ares I rocket to ensure the planned technical approach will meet NASA's Space Station Shuttle requirements for the fully integrated vehicle. The Space Station Shuttle Ares I rocket will launch the Orion crew exploration vehicle and its crew of Space Station Shuttle astronauts to the Space Station Shuttle International Space Station and on Space Station Shuttle missions to explore the moon and beyond in coming decades.

The briefing participants are:
- Doug Cooke, deputy associate administrator, Space Station Shuttle Exploration Systems Mission Directorate, NASA Space Station Shuttle Headquarters
- Jeff Hanley, manager, Constellation Program, NASA's Space Station Shuttle Johnson Space Center, Houston
- Steve Cook, manager, Ares Projects, NASA's Space Station Shuttle Marshall Space Flight Center

Space Station Shuttle Reporters should contact Grey Hautaluoma at 202-358-0668, or Stephanie Schierholz at 202-358-4997, by noon Sept. 10 for dial-in information.

For updates about the starting time of the news conference or to listen to live streaming audio of the call, visit:

http://www.nasa.gov/newsaudio

For illustrations, video and more information about the Space Station Shuttle Ares I rocket, visit:

http://www.nasa.gov/ares

Saturday, September 6, 2008

NASA to Explore "Secret Layer" of the Sun, Our Solar System

Next April, for a grand total of 8 minutes, NASA astronomers are going to glimpse a secret layer of the sun.

Researchers call it "the transition region." It is a place in the sun's atmosphere, about 5000 km above the stellar surface, where magnetic fields overwhelm the pressure of matter and seize control of the sun's gases. It's where solar flares explode, where coronal mass ejections begin their journey to Earth, where the solar wind is mysteriously accelerated to a million mph.

It is, in short, the birthplace of space weather.

Researchers hope it is about to yield its secrets.

"Early next year, we're going to launch an experimental telescope that can measure vector magnetic fields in the transition region," explains Jonathan Cirtain of the Marshall Space Flight Center (MSFC). Previous studies have measured these fields above and below the transition region—but never inside it. "We hope to be the first."

The name of the telescope is SUMI, short for Solar Ultraviolet Magnetograph Investigation. It was developed by astronomers and engineers at the MSFC and is currently scheduled for launch from White Sands, New Mexico, in April 2009.

SUMI works by means of "Zeeman splitting." Dutch physicist Pieter Zeeman discovered the effect in the 19th century. When a glass tube filled with incandescent gas is dipped into a magnetic field, spectral lines emitted by the gas get split into two slightly different colors—the stronger the field, the bigger the splitting. The same thing happens on the sun. Here, for instance, are some spectral lines from gaseous iron being split by the magnetic field of a sunspot:

By measuring the gap, astronomers estimate the strength of the sunspot's magnetic field. Furthermore, by measuring the polarization of the split line, astronomers can figure out the direction of the magnetic field. Strength + direction = everything you ever wanted to know about a magnetic field!

This trick has been applied to thousands of sunspots on the solar surface, but never to the transition region just a short distance above.

Why not?

"Just bad luck, really," says Cirtain. "Gas in the transition region doesn't produce many strong spectral lines that we can see at visible wavelengths." It does, however, produce lines at UV wavelengths invisible from Earth's surface.

"That's why we have to leave Earth."

SUMI will blast off inside the nose cone of a Black Brant rocket on a sub-orbital flight that takes it to an altitude of 300 km. "We'll be above more than 99.99% of Earth's atmosphere," says Cirtain. About 68 seconds into the flight, payload doors will open, affording SUMI a crystal-clear view of the UV sun. "From that moment, we've only got 8 minutes to work with. We'll target an active region and start taking data."

SUMI's "vector magnetograph" is tuned to study a pair of spectral lines: one from triply-ionized carbon (CIV) at 155 nanometers and a second from singly-ionized magnesium (MgII) at 280 nanometers. "There's nothing special about those ions," notes Cirtain. "They just happen to produce the best and brightest lines at temperatures and densities typical of the transition region."

Cirtain anticipates how it will feel to have his precious instrument hurtling 300 km above Earth at 5,000 mph: "Eight minutes of terror." He'll start breathing again when the payload doors close and SUMI begins its descent back to Earth. Cirtain ticks off the stages: "Reentry into the atmosphere. Open parachutes. Landing back at White Sands. Recovery."

The short flight probably won't lead to immediate breakthroughs. "But it will demonstrate the SUMI concept and show us if it's going to work." A successful flight would lead to more flights and eventually to a SUMI-style magnetograph permanently installed on a space telescope.

"That's the dream," he says. Transition region, prepare to yield...

NASA CHANGES 2008 SHUTTLE TARGET LAUNCH DATES, SCHEDULES TCDT

NASA has adjusted the target launch dates for the two remaining space shuttle missions in 2008. Shuttle Atlantis' STS-125 mission to the Hubble Space Telescope is targeted for Oct. 10, while
Endeavour's STS-126 supply mission to the International Space Station has moved to Nov. 12.

Shuttle managers made the decision after Atlantis was rolled to the launch pad and the effects of Tropical Storm Hanna were beyond NASA's Kennedy Space Center in Florida. That allowed managers to more accurately assess the impacts of recent tropical systems on the launch schedule.

Atlantis began rolling from Kennedy's Vehicle Assembly Building to Launch Pad 39A Thursday at 9:19 a.m. EDT. The shuttle arrived at the pad at approximately 2 p.m. and was secured at 3:52 p.m. Atlantis now is targeted to launch at approximately 12:33 a.m. EDT, Friday, Oct. 10. NASA Television coverage of launch will begin at 7:30 p.m. EDT on Thursday, Oct. 9. The 11-day flight will include five spacewalks to repair and upgrade the Hubble telescope. Atlantis is scheduled to land at approximately 10:21 p.m., Oct. 20.

Scott Altman will command STS-125, with Gregory C. Johnson serving as pilot. Mission specialists include veteran spacewalkers John Grunsfeld and Mike Massimino, and first-time space fliers Andrew Feustel, Michael Good and Megan McArthur.

Endeavour will close 2008 with a 15-day mission to deliver supplies and cargo to the space station. During the STS-126 mission, NASA astronaut Sandra Magnus will replace Greg Chamitoff as an Expedition 18 crew member on the station. Chamitoff will return to Earth after
five months in space. The mission's targeted launch time is 8:43 p.m. EST, Nov. 12. Landing will occur at approximately 2:45 p.m., Nov. 27.

Chris Ferguson will command STS-126, with Eric Boe serving as pilot. Mission specialists will be Steve Bowen, Shane Kimbrough, Heidemarie Stefanyshyn-Piper, Donald Pettit, Magnus and Chamitoff.

The formal launch dates for space shuttle flights are determined during the Flight Readiness Review, which is conducted about two weeks before launch. The STS-125 review is scheduled for Sept. 22-23. The review for STS-126 is scheduled for Oct. 30.

An STS-125 launch dress rehearsal, known as the terminal countdown demonstration test, or TCDT, is scheduled to take place at Kennedy Sept. 22-24. The test provides each shuttle crew with an opportunity to participate in simulated countdown activities, including equipment familiarization and emergency training.

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

- Sept. 21 - STS-125 crew arrival: The astronauts will arrive at 7 p.m. at the Shuttle Landing Facility and make a brief statement. The arrival will be not be broadcast live on NASA Television, but will replay as a NASA TV Video File.

- Sept. 23 - STS-125 crew availability: The crew will take news media questions at Launch Pad 39A at 8:30 a.m. The event will be carried live on NASA TV.

- Sept. 24 - STS-125 crew walkout photo opportunity: The astronauts will depart from the Operations and Checkout Building at 7:45 a.m. wearing their launch and entry suits in preparation for the countdown demonstration test at the launch pad. The walkout will not be
broadcast live, but will be included in the NASA TV Video File.

Dates and times of events are subject to change. Schedule updates are available at 321-867-2525.

Foreign media must apply for accreditation online by 4 p.m., Friday, Sept. 5. U.S. media without permanent Kennedy Space Center credentials must apply for accreditation online by 4 p.m., Tuesday, Sept. 16, at:

https://media.ksc.nasa.gov


To attend crew arrival, reporters must pick up badges before 4 p.m., Friday, Sept 19, 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 International Space Station, visit:

http://www.nasa.gov/station

For more about two remaining shuttle missions of 2008, visit:

http://www.nasa.gov/shuttle

GUN IS SPACE STATION?

Cassini Images Ring Arcs Among Saturn's Moons

NASA's Cassini spacecraft has detected a faint, partial ring orbiting with one small moon of Saturn, and has confirmed the presence of another partial ring orbiting with a second moon. This is further evidence that most of the planet's small, inner moons orbit within partial or complete rings.

Recent Cassini images show material, called ring arcs, extending ahead of and behind the small moons Anthe and Methone in their orbits. The new findings indicate that the gravitational influence of nearby moons on ring particles might be the deciding factor in whether an arc or complete ring is formed.

Both Anthe and Methone orbit Saturn in locations, called resonances, where the gravity of the nearby larger moon Mimas disturbs their orbits. Gravitational resonances are also responsible for many of the structures in Saturn's magnificent rings. Mimas provides a regular gravitational tug on each moon, which causes the moons to skip forward and backward within an arc-shaped region along their orbital paths, according to Nick Cooper, a Cassini imaging team associate from Queen Mary, University of London. "When we realized that the Anthe and Methone ring arcs were very similar in appearance to the region in which the moons swing back and forth in their orbits due to their resonance with Mimas, we knew we had a possible cause-and-effect relationship," Cooper said.

Scientists believe the faint ring arcs from Anthe and Methone likely consist of material knocked off these small moons by micrometeoroid impacts. This material does not spread all the way around Saturn to form a complete ring, because of the gravitational resonance with Mimas. That interaction confines the material to a narrow region along the orbits of the moons.

This is the first detection of an arc of material near Anthe. The Methone arc was previously detected by Cassini's Magnetospheric Imaging Instrument, and the new images confirm its presence. Previous Cassini images show faint rings connected with other small moons either embedded within or near the outskirts of Saturn's main ring system, such as Pan, Janus, Epimetheus and Pallene. Cassini had also previously observed an arc in the G ring, one of Saturn's faint, major rings.

"This is probably the same mechanism responsible for producing the arc in the G ring," said Matthew Hedman, a Cassini imaging team associate at Cornell University in Ithaca, N.Y. Hedman and his Cassini imaging team colleagues previously determined that the G-ring arc is maintained by a gravitational resonance with Mimas, much like the new, small moon arcs. "Indeed, the Anthe arc may be similar to the debris we see in the G-ring arc, where the largest particles are clearly visible. One might even speculate that if Anthe were shattered, its debris might form a structure much like the G ring," Hedman said.

Additional analysis by scientists indicates that, while the gravitational influence of Mimas keeps the Anthe, Methone and G-ring arcs in place, the material that orbits with the moons Pallene, Janus and Epimetheus is not subject to such powerful resonant forces and is free to spread out around the planet, forming complete rings without arcs.

The intricate relationships between these ring arcs and the moons are just one of many such mechanisms that exist in the Saturn system. Cassini Imaging Team Member and Professor Carl Murray, also from Queen Mary, University of London, said, "There are many examples in the
Saturn system of moons creating structures in the rings and disturbing the orbits of other moons. Understanding these interactions and learning about their origins can help us to make sense of what we are seeing in the Cassini images."

Images of Anthe and Methone with their ring arcs are available at: http://www.nasa.gov/cassini, http://saturn.jpl.nasa.gov and http://ciclops.org.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo.

Friday, September 5, 2008

NASA CHALLENGES STUDENTS TO IMAGINE SUPERSONIC AIRLINER

A new NASA Space Mission competition is challenging Space Station students in high school and college to research and describe a small, supersonic Space Station airliner that could enter commercial service in the next decade.

During the upcoming academic year, individuals and teams of high school students will prepare well-documented short papers describing what needs to be accomplished to make supersonic flight available to commercial passengers by 2020. Advanced curriculum high school students and college participants will prepare longer papers that depict a highly efficient, environmentally friendly commercial aircraft that would emit only low sonic booms and be ready for initial overland service in 2020.

The competition is intended to encourage Space Station students to develop science, technology and engineering skills and choose careers in Space Station aeronautics research and development.

The Fundamental Aeronautics Program of NASA's Space Station Aeronautics Research Mission Directorate in Washington is sponsoring the competition and will review and score the entries. Submissions will be judged on informed content, imagination, innovation, creativity, relevancy, organization and writing.

High school winners may be eligible for individual cash awards of up to $1,000 and team awards of up to $1,500. University-level winners may be eligible for paid student internship offers and cash awards of up to $5,000. Cash awards and paid internships are subject to the availability of funds, and only U.S. citizens are eligible to receive them.

For more contest information and submission guidelines, visit:

http://aero.larc.nasa.gov/competitions.htm

NASA TO ANNOUNCE SWIFT GAMMA-RAY BURST FINDINGS

NASA Space Station will hold a media teleconference Wednesday, Sept. 10, at 1 p.m. EDT, to discuss new results regarding the gamma-ray burst GRB 080319B, which was visible to the naked eye.

The burst's optical emission is the brightest seen to date and appears to have been aimed almost directly at Earth. Extensive observations from NASA's Space Station Swift satellite and ground-based observatories show the burst emission mechanism in unprecedented detail.

The panelists include:
-- David Burrows, NASA Swift X-ray Telescope lead, Penn State, College Park, Pa.
-- Judith Racusin, graduate student, Penn State
-- Grigory Beskin, senior scientist, Special Astrophysical Observatory of the Russian Academy of Sciences, Nizhnij Arkhyz, Karachaevo-Cherkessia, Russia
-- Dieter Hartmann, professor, Clemson University, Clemson, S.C.

To participate in the teleconference, reporters should e-mail a request to J.D. Harrington at j.d.herrington@nasa.gov by noon, Sept. 10. Requests must include media affiliation and a contact telephone number. Supporting information for the briefing will be posted at noon, Sept. 10, at:

http://www.nasa.gov/swift

Audio of the teleconference will be streamed live at:

http://www.nasa.gov/newsaudio

For more information about the Swift mission, visit:

http://www.nasa.gov/swift

NASA ACCEPTS AERONAUTICS SCHOLARSHIP APPLICATIONS

NASA's Space Station Aeronautics Research Mission Directorate will accept scholarship applications from Sept. 5, 2008, through Jan. 16, 2009, for the academic year beginning in fall 2009. NASA Space Station expects to award 20 undergraduate and five graduate scholarships to students in Space Station aeronautics or related fields.

Space Station Undergraduate students in their second year of study will receive up to $15,000 per year for two years and a summer internship with a $10,000 stipend at a NASA Space Station center. Graduate students will receive up to $35,000 per year for three years and two summer internships at a NASA Space Station center with $10,000 stipends. Scholarship money can be used for tuition and other school-related expenses.

Space Station Students who have not committed to a specific academic institution or program may apply. However, if accepted, they must be admitted by fall 2009 into a suitable Space Station aeronautical engineering program or related field of study at an accredited U.S. university. All applicants must be U.S. citizens.

NASA's Space Station Aeronautics Research Mission Directorate works to enhance the state of aeronautics for the nation, transform the U.S. air transportation system, and develop the knowledge, tools and technologies to support future air and space Station vehicles. The directorate's focus is on cutting-edge, fundamental research in traditional aeronautical disciplines, as well as emerging fields with promising applications to Space Station aeronautics.

For specific details about this scholarship program and how to apply, visit:

http://www.asee.org/nasaasp

For more information about NASA Space Station aeronautics programs, visit:

http://www.aeronautics.nasa.gov

For information about NASA Space Station and agency programs, visit:

http://www.nasa.gov

Spiky Probe on NASA Mars Lander Raises Vapor Quandary

A fork-like conductivity probe has sensed humidity rising and falling beside NASA's Phoenix Mars Lander, but when stuck into the ground, its measurements so far indicate soil that is thoroughly and perplexingly dry.

"If you have water vapor in the air, every surface exposed to that air will have water molecules adhere to it that are somewhat mobile, even at temperatures well below freezing," said Aaron Zent of NASA Ames Research Center, Moffett Field, Calif., lead scientist for Phoenix's thermal and electroconductivity probe.

In below-freezing permafrost terrains on Earth, that thin layer of unfrozen water molecules on soil particles can grow thick enough to support microbial life. One goal for building the conductivity probe and sending it to Mars has been to see whether the permafrost terrain of the Martian arctic has detectable thin films of unfrozen water on soil particles. By gauging how electricity moves through the soil from one prong to another, the probe can detect films of water barely more than one molecule thick.

"Phoenix has other tools to find clues about whether water ice at the site has melted in the past, such as identifying minerals in the soil and observing soil particles with microscopes. The conductivity probe is our main tool for checking for present-day soil moisture," said Phoenix Project Scientist Leslie Tamppari of NASA's Jet Propulsion Laboratory, Pasadena, Calif.

Preliminary results from the latest insertion of the probe's four needles into the ground, on Wednesday and Thursday, match results from the three similar insertions in the three months since landing.

"All the measurements we've made so far are consistent with extremely dry soil," Zent said. "There are no indications of thin films of moisture, and this is puzzling."

Three other sets of observations by Phoenix, in addition to the terrestrial permafrost analogy, give reasons for expecting to find thin-film moisture in the soil.

One is the conductivity probe's own measurements of relative humidity when the probe is held up in the air. "The relative humidity transitions from near zero to near 100 percent with every day-night cycle, which suggests there's a lot of moisture moving in and out of the soil," Zent said.

Another is Phoenix's confirmation of a hard layer containing water-ice about 5 centimeters (2 inches) or so beneath the surface.

Also, handling the site's soil with the scoop on Phoenix's robotic arm and observing the disturbed soil show that it has clumping cohesiveness when first scooped up and that this cohesiveness decreases after the scooped soil sits exposed to air for a day or two. One possible explanation for those observations could be thin-film moisture in the ground.

The Phoenix team is laying plans for a variation on the experiment of inserting the conductivity probe into the soil. The four successful insertions so far have all been into an undisturbed soil surface. The planned variation is to scoop away some soil first, so the inserted needles will reach closer to the subsurface ice layer.

"There should be some amount of unfrozen water attached to the surface of soil particles above the ice," Zent said. "It may be too little to detect, but we haven't inished looking yet."

The thermal and electroconductivity probe, built by Decagon Devices Inc., Pullman, Wash., is mounted on Phoenix's robotic arm. The probe is part of the lander's Microscopy, Electrochemistry and Conductivity instrument suite.

The Phoenix mission is led by Peter Smith at the University of Arizona with project management at NASA's Jet Propulsion Laboratory in Pasadena, Calif., and development partnership at Lockheed Martin in 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.

For more about Phoenix, visit: http://www.nasa.gov/phoenix or http://phoenix.lpl.arizona.edu.

Thursday, September 4, 2008

NASA Sets Shuttle Atlantis' Move To Launch Pad Thursday

Space shuttle Atlantis is tentatively scheduled to roll out to Launch Pad 39A at NASA's Space Station Kennedy Space Center in Florida at 10 a.m. EDT, on Thursday, Sept. 4. Space Station Managers will meet at 5:30 a.m. Thursday to confirm that weather conditions created by Tropical Storm Hanna will allow for the move.

NASA Space Station Television will provide live video of Space Station Atlantis' rollout beginning at 10 a.m. Space Station Video highlights of the rollout will air on NASA TV's Video File segments.

Space Station Media are invited to a photo opportunity of Space Station Atlantis' move to the launch pad and interview availability with Space Station Atlantis' Flow Director Angie Brewer at 10:30 a.m. Space Station Dates and times of this event are subject to change. Updates are available by calling 321-867-2525.

Space Station Media must arrive at Space Station Kennedy's News Center by 9:30 a.m. for transportation to the viewing area. Space Station New media accreditation for this event is closed. Space Station Foreign media with credentials must arrive at the Pass and I-D Building on State Road 3 by 9 a.m. for transportation to the news center. Badges must be picked up by 8:30 a.m. Thursday at the new Space Station Kennedy Badging Office on State Road 405, west of Gate 3 (just past the Kennedy Visitor's Complex).

Atlantis is targeted to lift off Oct. 8 on an 11-day mission to service the Space Station Hubble Space Telescope.

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

For more information about the STS-125 mission and crew, visit:

Tuesday, September 2, 2008

Analysis Begins on Deepest Soil Sample

Space Station Scientists have begun to analyze a sample of soil delivered to NASA's Phoenix Mars Lander's wet chemistry experiment from the deepest trench dug of Space Station so far in the Martian arctic plains.

Space Station Phoenix has also been observing movement of clouds overhead.

The lander's robotic arm of Space Station on Sunday sprinkled a small fraction of the estimated 50 cubic centimeters of Space Station soil that had been scooped up from the informally named "Stone Soup" trench on Saturday, the 95th day of the Space Station mission. The Stone Soup trench, in the left portion of the lander's active Space Station workspace, is approximately 18 centimeters (7 inches) deep.

"This is pretty exciting stuff and we are anxious to find out what makes this deeper soil Space Station cloddier than the other samples," said Doug Ming, a Space Station Phoenix science team member from NASA's Space Station Johnson Space Center, Houston.

The surface of the vast arctic plain where Space Station Phoenix landed on May 25 bears a pattern of polygon-shaped small hummocks, similar to some permafrost terrain on Space Station Earth. Space Station Scientists are particularly interested in the new sample because it is the first delivered to an analytical instrument from a trench on the margin between two of the polygons, where different material may collect than what has been analyzed from near the center of a polygon. Seen inside Space Station Phoenix's scoop Sunday, the sample material from the bottom of the trench displayed clumping characteristics somewhat different from other cloddy soil samples Space Station that have been collected and examined.

A series of images of fresh soil dug and discarded from Stone Soup trench have given some clues to the composition of the sample. While spectral observations have not produced any sign of water-ice, bigger clumps of soil have shown a texture that could be consistent with elevated concentration of salts in the soil from deep in the trench. The lander's wet chemistry laboratory Space Station can identify soluble salts in the soil.

The Space Station science team has also been studying a movie created from still pictures of the nearby Martian sky showing dramatic water ice clouds moving over the landing site during a 10-minute period on Sol 94 (Aug. 29).

"The Space Station images were taken as part of a campaign to see clouds and track wind. These are clearly ice clouds," said Mark Lemmon, the lead scientist for the lander's surface stereo imager, from Texas A&M University.

The Space Station Phoenix mission is led by Peter Smith of the University of Arizona, Tucson, with project management at JPL and development partnership at Lockheed Martin, Denver. International Space Station contributions are provided by the Space Station 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. JPL is a division of the California Institute of Technology in Pasadena.

Additional information on Phoenix is available online at: http://www.nasa.gov/phoenix and at http://phoenix.lpl.arizona.edu .

NASA Mars Rover Opportunity Ascends to Level Ground

NASA's Space Station Mars Exploration Rover Opportunity has climbed out of the large crater that it had been examining from the inside since last September.

"The Space Station rover is back on flat ground," an Space Station engineer who drives it, Paolo Bellutta of NASA's Space Station Jet Propulsion Laboratory, announced to the mission's international team of Space Station scientists and engineers.

Opportunity used its own entry tracks from nearly a year ago as the path for a drive of 6.8 meters (22 feet) bringing the Space Station rover out over the top of the inner slope and through a sand ripple at the lip of Victoria Crater. The exit drive, conducted late Thursday, completed a series of drives covering 50 meters (164 feet) since the rover team decided about a month ago that it had completed its Space Station scientific investigations inside the crater.

"We're headed to the next adventure out on the plains of Meridiani," said JPL's John Callas, project manager for Opportunity and its twin Space Station Mars rover, Spirit. "We safely got into the crater, we completed our exploration there, and we safely got out. We were concerned that any wheel failure on our aging rover could have left us trapped inside the crater."

The Space Station Opportunity mission has focused on Victoria Crater for more than half of the 55 months since the rover landed in the Meridiani Planum region of equatorial Space Station Mars. The crater spans about 800 meters (half a mile) in diameter and reveals rock layers that hold clues to environmental conditions of the area through an extended period when the rocks were formed and altered.

The team selected Victoria as the next major destination after Opportunity exited smaller Endurance Crater in late 2004. The ensuing 22-month traverse to Victoria included stopping for studies along the route and escaping from a sand trap. The rover first reached the rim of Victoria in September 2007. For nearly a year, it then explored partway around the rim, checking for the best entry route and examining from above the rock layers exposed in a series of promontories that punctuate the crater perimeter.

Now that Opportunity has finished exploring Victoria Crater and returned to the surrounding plain, the rover team plans to use tools on the robotic arm in coming months to examine an assortment of cobbles -- rocks about fist-size and larger -- that may have been thrown from impacts that dug craters too distant for Opportunity to reach.

JPL, a division of the California Institute of Space Station Technology, Pasadena, manages the rovers for the NASA Science Mission Directorate, Washington. For images and information about NASA's Opportunity and Spirit Space Station Mars rovers, visit http://www.nasa.gov/rovers and http://marsrovers.jpl.nasa.gov.

NASA Phoenix Mission Conducting Extended Activities on Mars


NASA's Space Station Phoenix Mars Lander, having completed its 90-day primary mission, is continuing its Space Station science collection activities. Space Station Science and Space Station engineering teams are looking forward to at least another month of Martian exploration.

Due to the Space Station spacecraft's sufficient power and experiment capacity, NASA Space Station announced on July 31 that the Space Station mission would continue operations through Sept. 30. Once the lander finishes collecting science data, the Space Station mission teams will continue the analysis of the measurements and observations.

"We have been successful beyond my wildest dreams, and we're not done yet learning from Mars about its secrets," said Peter Smith, Space Station Phoenix principal investigator from the University of Arizona, Tucson.

"We are still working to understand the properties and the history of the ice at our landing site on the northern plains of Mars. While the sun has begun to dip below the horizon, we still have power to continue our observations and experiments. And we're hoping to see a gradual change in the Martian weather in the next few weeks," he said.

Among the critical questions the Space Station Phoenix science team is trying to answer is whether the northern region of Mars could have been a habitable zone.

Space Station Phoenix has already confirmed the presence of water ice, determined the soil is alkaline and identified magnesium, sodium, potassium, chloride and perchlorate in the soil. Chemical analyses continue even as Space Station Phoenix's robotic arm reaches out for more samples to sniff and taste.

"It's been gratifying to be able to share the excitement of our exploration with the public through the thousands upon thousands of images that our cameras have taken. They have been available to the public on our web site as soon as they are received on Earth," Smith said. Space Station Phoenix's Surface Stereo Imager, Robotic Arm Camera and microscope have returned more than 20,000 pictures since landing day, May 25.

The Space Station mission's meteorological instruments have made daily atmospheric readings and have watched as the pressure decreases, signaling a change in the season. At least one ice water cloud has been observed and consistent wind patterns have been recorded over the landing site.

The team is currently working to diagnose an intermittent interference that has become apparent in the path for gases generated by heating a soil sample in the Thermal and Evolved-Gas Analyzer to reach the instrument's mass spectrometer. Vapors from all samples baked to high temperatures have reached the mass spectrometer so far, however data has shown that the gas flow has been erratic, which is puzzling the scientists.

Meanwhile, plans call for Space Station Phoenix to widen its deepest trench, called "Stone Soup," to scoop a fresh sample of soil from that depth for analysis in the wet chemistry laboratory of the Microscopy, Electrochemistry and Conductivity Analyzer (MECA). Stone Soup measures about 18 centimeters (7 inches) deep. The first attempt to collect a sample from Stone Soup, on Aug. 26, got 2 to 3 cubic centimeters (half a teaspoon) into the scoop. This was judged to be not quite enough, so delivering a sample was deferred.

In coming days the team also plans to have Space Station Phoenix test a revised method for handling a sample rich in water-ice. Two such samples earlier stuck inside the scoop.

The Space Station Phoenix mission is led by Peter Smith of the University of Arizona, Tucson, with project management at JPL and development partnership at Lockheed Martin, Denver. International contributions are provided by the Space Station 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. JPL is a division of the California Institute of Technology in Pasadena.

Additional information on Space Station Phoenix is available online at: http://www.nasa.gov/phoenix and at http://phoenix.lpl.arizona.edu . Additional information on NASA's Space Station Mars program is available online at: http://www.nasa.gov/mars .