NASA to Discuss Supernova and Dark Energy Research at Feb. 17 Teleconference

NASA will hold a teleconference with reporters at 1 p.m. EST on Wednesday, Feb. 17, to discuss the latest Chandra X-ray Observatory findings that advance our understanding of certain supernovae. This research is critical for studying dark energy, which astronomers believe pervades the universe.

The panelists are:
- Marat Gilfanov, astrophysicist, Max Planck Institute for Astrophysics, Garching, Germany
- Akos Bogdan, astrophysicist, Max Planck Institute for Astrophysics
- Mario Livio, astrophysicist, Space Telescope Science Institute, Baltimore

To reserve a telephone line, journalists should e-mail their name, media affiliation and telephone number to J.D. Harrington at:

j.d.harrington@nasa.gov

Audio of the teleconference will be streamed live on NASA's Web site at:

http://www.nasa.gov/newsaudio

For more information about NASA's Chandra X-ray Observatory, visit:

http://www.nasa.gov/chandra

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Are TGFs Hazardous to Air Travelers?

Instruments scanning outer space for cataclysmic explosions called gamma-ray bursts are detecting intense flashes of gamma-ray energy right here in the friendly skies of Earth. These terrestrial gamma-ray flashes, or TGFs, blast through thunderstorms close to the altitude where commercial airliners fly.

In fact, they could be too close for comfort.

In a recent study,* scientists estimated that airline passengers could be exposed to 400 chest X-rays worth of radiation by being near the origin of a single millisecond blast. Joe Dwyer of the Florida Institute of Technology took part in that research, which used observations from NASA's Reuven Ramaty High Energy Solar Spectroscopic Imager, or RHESSI, to estimate the danger TGFs pose.

see caption"We believe the risk of encountering a TGF in an airplane is very small," says Dwyer. "I wouldn't hesitate to take a flight. Pilots already avoid thunderstorms because of turbulence, hail, and lightning, and we may just have to add TGFs to the list of reasons to steer clear of those storms."

But, he stresses, "it's worth looking into."

Right: Lightning might not be the only reason to avoid thunderstorms. TGFs sometimes come blasting out of these clouds, too. Image credit: NOAA.

NASA's Gamma-ray Burst Monitor (GBM) on the Fermi Gamma-ray Telescope will help evaluate the hazards.

"GBM provides the best TGF data we have so far," says Dwyer. "It gets better measurements of their spectra than any previous instrument, giving us a more accurate idea of just how energetic they are."

Although TGFs are quite brief (1-2 milliseconds), they appear to be the most energetic events on Earth. They belch destructive gamma-rays packing over ten million times the energy of visible light photons – enough punch to penetrate several inches of lead.

"It's amazing," says Jerry Fishman, a co-investigator for the Gamma-ray Burst Monitor. "They come blasting right through the whole Fermi spacecraft and light up all of our detectors. Very few cosmic gamma-ray bursts manage to do this!"

The origin of TGFs is still a mystery, but researchers know this much: TGFs are associated with thunderstorms and lightning. "We think the electric field in a thunderstorm may get so strong that the storm itself turns into a gamma-ray factory," says Dwyer. "But we don't know exactly how or why or where inside the storm this happens."

So no one yet knows how often, if ever, planes end up in the wrong place at the wrong time.

see caption

Above: A cartoon sketch of electric and magnetic fields in a thunderstorm and some of the phenomena they produce. TGFs may be just one aspect of thunderstorm activity in addition to elves, sprites, blue jets and ordinary lightning. Credit: Stanford University. [more]

It's possible that lightning bolts trigger TGFs. Or maybe TGFs trigger lightning bolts. Researchers aren't sure which comes first. GBM's excellent timing accuracy – to within 2 microseconds – will help solve this riddle.

"For some of the TGFs, we've pinpointed the associated lightning," says Dwyer. "This information along with the spectrum should help us figure out how deep in the atmosphere a TGF source is and how many gamma-rays it's emitting. Then we can determine the altitude and location they're coming from in the thunderstorm."

Fishman offers some good news: "If TGFs originate near the tops of thunderstorms and propagate upward from there, airline passengers would be safe."

By looking closely at a TGF's life cycle, that is, how quickly it turns on and off, GBM may also help researchers calculate how large and concentrated the gamma-ray source is. If the gamma-rays are emitted over a large region, the radiation dose would be diluted and much less harmful.

see caption"But if the source is compact and the gamma-rays originate close to an aircraft, then that could be a problem," says Fishman.

Right: The radiation dose from an ordinary lightning leader vs. the dose from a TGF. Both phenomena are associated with electron beams. Tighter, more compact beams deliver a greater effective dose. Details of this model may be found in an upcoming issue of the Journal of Geophysical Research (Atmospheres). Look for "Estimation of the fluence of high-energy electron bursts produced by thunderclouds and the resulting radiation doses received in aircraft" by J. Dwyer et al. (in press).

"Of course the smaller the source the lower the odds of a plane ending up close to it," adds Dwyer.

GBM wasn't designed to look for TGFs, but GBM co-investigator Michael Briggs has greatly enhanced its sensitivity to them by writing new software.

"TGFs have really been an afterthought for missions so far," says Dwyer. RHESSI, for example, points at the sun, but the RHESSI team figured out a way to measure TGFs by detecting gamma-rays coming in through the satellite's backside. "All these instruments have been pointing across the universe, while right over our heads these monsters are going off!"

"Now the whole field of TGFs is on fire," says Fishman. "People are jumping on the bandwagon to try to figure them out."

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NASA Sets Media Credentials Deadlines for Next Space Shuttle Flight

NASA has set media accreditation deadlines for the March space shuttle flight to the International Space Station. Shuttle Discovery and seven crew members are targeted to launch the STS-131 mission on March 18 from NASA's Kennedy Space Center in Florida. Deadlines for international journalists to apply for the shuttle rollout and Terminal Countdown Demonstration Test are as early as 5 p.m. EST Feb. 11.

During the 13-day flight, the crew will deliver a multipurpose logistics module with science racks to the space station. Among the shuttle crew is Dottie Metcalf-Lindenburger, a former high school science teacher who is now a fully trained astronaut.

Reporters must apply for credentials to attend the launch or cover the mission from other NASA centers. To be accredited, reporters must work for verifiable news-gathering organizations. No substitutions of credentials are allowed at any NASA facility.

Additional time may be required to process accreditation requests by journalists from certain designated countries. Designated countries include those with which the United States has no diplomatic relations, countries on the State Department's list of state sponsors of terrorism, those under U.S. sanction or embargo, and countries associated with proliferation concerns. Please contact the accrediting NASA center for details. Journalists should confirm they have been accredited before they travel.

KENNEDY SPACE CENTER

Reporters applying for credentials at Kennedy should submit requests via the Web at:

http://media.ksc.nasa.gov

Reporters must use work e-mail addresses, not personal accounts, when applying. After accreditation is approved, applicants will receive confirmation via e-mail.

Accredited media representatives with mission badges will have access to Kennedy from launch through the end of the mission. The application deadline for mission badges is March 8 for all reporters requesting credentials.

Discovery's move from the Vehicle Assembly Building, or VAB, to Launch Pad 39A, planned for Feb. 19, follows its rollover from Orbiter Processing Facility-3 to the VAB, which is targeted for Feb. 12. Launch dress rehearsal activities, known as the Terminal Countdown Demonstration Test, and related training are scheduled for Feb. 22-24. International journalists must apply by 5 p.m. EST Feb. 11 to allow time for processing, and U.S. media representatives must apply by Feb. 17. Media badges will be valid for both rollout and the Terminal Countdown Demonstration Test.

Reporters with special logistic requests for Kennedy, such as space for satellite trucks, trailers, electrical connections or work space, must contact Laurel Lichtenberger by March 11 at:

laurel.a.lichtenberger@nasa.gov

There is no longer free wireless Internet access provided at Kennedy's news center. Work space in the news center and the news center annex is provided on a first-come basis, limited to one space per organization. To set up temporary telephone, fax, ISDN or network lines, media representatives must make arrangements with BellSouth at 800-213-4988. Reporters must have an assigned seat in the Kennedy newsroom prior to setting up lines. To obtain an assigned seat, contact Patricia Christian at:

patricia.christian-1@nasa.gov

Journalists must have a public affairs escort to all other areas of Kennedy except the Launch Complex 39 cafeteria.

JOHNSON SPACE CENTER

Reporters may obtain credentials for NASA's Johnson Space Center in Houston by calling the Johnson newsroom at 281-483-5111 or by presenting STS-131 mission credentials from Kennedy. Media representatives planning to cover the mission only from Johnson need to apply for credentials only at Johnson. The application deadline for mission badges is March 9 for all reporters requesting credentials.

Journalists covering the mission from Johnson using Kennedy credentials must contact the Johnson newsroom by March 9 to arrange workspace, phone lines and other logistics. Johnson is responsible for credentialing media if the shuttle lands at NASA's White Sands Space Harbor, N.M. If a landing is imminent at White Sands, Johnson will arrange credentials.

DRYDEN FLIGHT RESEARCH CENTER

Notice for a space shuttle landing at NASA's Dryden Flight Research Center on Edwards Air Force Base in California could be short. Domestic media outlets should consider accrediting Los Angeles-based personnel who could travel quickly to Dryden. Deadlines for submitting Dryden accreditation requests are Feb. 19 for non-U.S. media, regardless of citizenship, and March 24 for U.S. media who are U.S. citizens or who have permanent residency status.

For Dryden media credentials, U.S. citizens representing domestic media outlets must provide their full name, date of birth, place of birth, media organization, driver's license number with the name of the issuing state, and the last six digits of their social security number.

In addition to the above requirements, foreign media representatives, regardless of citizenship, must provide data including their citizenship, visa or passport number and its expiration date. Foreign nationals representing either domestic or foreign media who have permanent residency status must provide their alien registration number and expiration date.

Journalists should fax requests for credentials on company letterhead to 661-276-3566 or e-mail requests to:

DrydenPAO@nasa.gov

Requests must include a phone number and business e-mail address for follow-up contact. Journalists who previously requested credentials will not need to do so again.

NASA PUBLIC AFFAIRS CONTACTS:

Kennedy Space Center: Allard Beutel, 321-867-2468, allard.beutel@nasa.gov

Johnson Space Center: James Hartsfield, 281-483-5111, james.a.hartsfield@nasa.gov

Dryden Flight Research Center: Leslie Williams, 661-276-3893, leslie.a.williams@nasa.gov

For information about the STS-131 mission, visit:

http://www.nasa.gov/shuttle

Two STS-131 crew members, NASA astronaut Clay Anderson and Naoko Yamazaki of the Japan Aerospace Exploration Agency, are tweeting about preparing for their mission. They can be followed at:

http://www.twitter.com/Astro_Clay

and

http://www.twitter.com/Astro_Naoko

For information about the International Space Station, visit:

http://www.nasa.gov/station

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NASA Announces Winners of George M. Low Award for Quality and Performance

NASA presented its highest honor for quality and performance, the George M. Low Award, to two companies that share a commitment to teamwork, safety, customer service, technical and managerial excellence.

The Low award demonstrates the agency's commitment to promote excellence and continual improvement by challenging NASA's contractor community to be a global benchmark of quality management practices. The 2009 awards were presented Wednesday, Feb. 10, at NASA's seventh annual Project Management Challenge in Galveston, Texas, to:

  • United Space Alliance, or USA, of Houston. USA provides ground operations, vehicle processing and logistics at NASA's Kennedy Space Center in Florida.; delivers specialty engineering and technical services at NASA's Marshall Space Flight Center in Huntsville, Ala.; and designs and plans missions, trains astronauts, develops and verifies software, and executes mission operations at NASA's Johnson Space Center in Houston. USA received the award in the large business service category.
  • Applied Geo Technologies, or AGT, of Choctaw, Miss. Tribally owned AGT is a small, disadvantaged provider of aerospace and defense services. It provides scientific, laboratory and geographic analysis services; maintains measurement standards; and calibrates and repairs instrumentation at NASA's Stennis Space Center in Bay St. Louis, Miss. AGT received the award in the small business service category.
The award was established in 1985 as NASA's Excellence Award for Quality and Productivity. It was renamed in 1990 in memory of George M. Low, an outstanding leader during his 27-year tenure at the agency. Low was NASA's deputy administrator from 1969 to1976 and a leader in the early development of space programs.

For more information about the George M. Low Award, visit:

http://www.hq.nasa.gov/office/codeq/gml

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NASA and Texas Instruments Use Human Spaceflight to Bring Math and Science Topics into High School Classrooms

NASA and Texas Instruments are using the theme of human space exploration to develop digital libraries of math and science problems for high school students. The goal is to bring real-world topics in science, technology, engineering and mathematics, or STEM, into classrooms to spark students' excitement and interest in these critical career fields.

The collaboration will produce two digital libraries. One, called Exploring Space Through Math: Applications in High School Mathematics, will provide problems based on NASA data that are set in the context of space exploration. The project material will cover almost the entire high school math curriculum, with applications in Algebra 1, Geometry, Algebra 2, and Pre-Calculus.

The other digital library, named Science at Work: Exploring Space with NASA-AP, will contain questions for Advanced Placement classes. This program seeks to develop and test problems in calculus, statistics, physics, chemistry and biology.

"As students solve real problems NASA faces in space exploration, they will practice during high school and college the skills necessary to pursue a career in a STEM field," said Charles Lloyd, NASA's lead for the effort and program manager for Human Research Program Education and Outreach at NASA's Johnson Space Center in Houston. "NASA and Texas Instruments are passionate about motivating the next generation's interest in science and math subjects and equipping these students to take us farther into space and improve our lives here on Earth."

The libraries of questions will use NASA applications and data while incorporating Texas Instruments' math learning technology. Each problem includes student and teacher editions to help the teacher link content to higher concepts.

"Our goal is to make STEM subjects more fun and interactive," said Werner Garciano, director of Professional Development for Texas Instruments' Education Technology. "Working with NASA is a great opportunity to bring exciting, real-world math experiences into the classroom. Our collaboration will expand the digital content and professional development that Texas Instruments provides teachers, and will help engage students more deeply in math. Together, we believe these activities will break through to students who have never considered a STEM career path."

Both projects will be available in the fall of 2010 on NASA's Web site. With this program, NASA continues its investment in engaging and retaining students in STEM disciplines critical to the agency's future engineering, scientific, and technical missions. For more information about NASA's education programs, visit:

http://www.nasa.gov/education

For more information about NASA's Human Research Program Education and Outreach, visit:

http://humanresearch.jsc.nasa.gov/education.asp

The digital libraries also will be available through Texas Instruments' Teachers Teaching with Technology workshops and online at the Texas Instruments' Activities Exchange at:

http://education.ti.com/educationportal/activityexchange/activity_list.do?cid=us

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SDO Launches

SDO LaunchesNASA's Solar Dynamics Observatory, SDO, launched aboard a United Launch Alliance Atlas V from Space Launch Complex-41 at 10:23 a.m. EST on Thursday, Feb. 11, 2010. SDO is the first satellite of NASA's Living with a Star (LWS) program.

From its geosynchronous orbit, SDO will point its instruments at the sun, conducting groundbreaking research that is expected to reveal the sun's inner workings by constantly taking high resolution images, collecting readings from inside the sun and measuring its magnetic field activity. This data is expected to give researchers the insight they need to eventually predict solar storms and other activity on the sun that can affect spacecraft in orbit, astronauts on the International Space Station and electronic and other systems on Earth.

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Mission That Mapped Earth Marks 10th Anniversary

3-D perspective view of Russia’s volcanically active Kamchatka Peninsula, created using SRTM topographic data and an enhanced true-color image from the Landsat 7 satelliteOn Feb. 11, 2000, two radar antennas built by JPL launched aboard Space Shuttle Endeavour on an 11-day mission to create the first-ever near-global high-resolution database of Earth's topography. The international Shuttle Radar Topography Mission collected topographic data over nearly 80 percent of Earth's land surfaces, revealing for the first time large, detailed swaths of Earth's topography previously obscured by persistent cloudiness. The data benefit scientists, engineers, government agencies and the public alike, with applications that range from land-use planning to virtual Earth exploration.

mission that mapped the worldNASA is currently using Shuttle Radar Topography Mission data to create an even better global topographic map by combining it with the more complete Advanced Spaceborne Thermal Emission and Reflection Radiometer global digital elevation model of Earth released last year by NASA and Japan's Ministry of Economy, Trade and Industry.

Hop aboard as we take you on a virtual tour of some of the more "uplifting" topographic features of our home planet: http://www.nasa.gov/topics/earth/features/srtm/srtm20100211.html.

For more information on the Shuttle Radar Topography Mission, visit: http://www.jpl.nasa.gov/srtm.

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On Approach

On Approach
This view of space shuttle Endeavour's aft section includes the three main engines and was taken by the Expedition 22 crew during the shuttle's approach vehicle prior to docking with the International Space Station. As part of the survey and part of every mission's activities, Endeavour performed a back-flip for the rendezvous pitch maneuver (RPM). The image was photographed with a digital still camera, using a 400mm lens at a distance of about 600 feet (180 meters).

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Riding out the Snow Storm Inside Goddard to Carry on the Mission

Hundreds of ground crew workers at NASA Goddard Space Flight Center in Greenbelt, Md. have been working since Friday afternoon to keep buildings safe and ensure essential employees are there to support the Space Shuttle Endeavour (STS-130) mission and the launch and operation of the Solar Dynamics Observatory (SDO). Crews continue to work very hard to make sure the Center is ready to return to normal operations once this storm is over.

Civil servants, contractors, and subcontractors are working together using hundreds of front loaders, Bobcats®, snow plows, dump trucks, and shovels to clear roads and sidewalks on Center.

The biggest challenge to handling this storm is finding a place to put all the snow, according to Eric Holmes, Goddard Facility Manager. “We hauled over 2,000 thousand truckloads of snow and dumped it behind Building 28,” said Holmes. “We’ve built ‘Mount Goddard’.”

Emergency planning began last Wednesday, February 3, when Holmes received a weather report from AccuWeather about the storm. “We made sure we had enough fuel, rock salt, and magnesium chloride,” said Holmes. “About 250 tons of rock salt was delivered to the Center on Thursday. We also made sure contractors and Government personal were prepared.”

Crews will live inside Building 4 for the duration of the storm. There is a full kitchen and hundreds of cots and air mattresses set up.

We were prepared to open the Center this week," says Holmes. "However, because of the surrounding county roads, Center management thought it would be safer for employees to stay home."

Space Shuttle and Solar Dynamics Observatory Mission Support

“Employees have staffed the Network Integration Center (NIC) 24 hours a day since last Friday,” says Jim Bangerter, Network Director for Human Space Flight at Goddard Space Flight Center.

Goddard provides critical communications for human spaceflight missions. The Goddard team provides data to Johnson Space Center’s Mission Control Center that allows them to monitor the performance of thousands of systems on the Shuttle, send flight commands and navigational instructions, relay science data, support voice communications between the astronauts and mission control along with video and live television feeds.

In addition to the Shuttle, Goddard also provides critical mission support to the Solar Dynamics Observatory through its entire mission from Building 14’s Mission Operation Center. The Center is fully staffed and ready to monitor and control the spacecraft through its initial orbits, using the orbital data provided to them by the Flight Dynamics Facility (FDF).

Pre-storm planning for Shuttle and SDO mission support began early last week. Contractors secured rooms at the Greenbelt Holiday Inn and Greenbelt Marriott hotels. They also made sure they had 4-wheel-drive vehicles. Employees packed extra food, water, and shovels. “Several people who did not have to work over the weekend volunteered to drive people between the hotels and Goddard during the storm,” said Melissa Blizzard, Human Space Flight Operations Center Manager. Blizzard works in the NIC. “I was amazed by how people pulled together to help one another during this storm.”

“We could not say enough about the work the ground crew is doing at Goddard,” said Joan Dunham, Flight Dynamics Support Services Operations Domain Lead with a.i. solutions, a contractor at the FDF. “Crews spent a lot of time clearing snow from parking lots and sidewalks from behind Building 28. It’s like plowing an ocean,” said Dunham, “They cleared one area and more snow fills in.”

Dunham adds that on Friday night, February 5, about a dozen dump trucks, bulldozers, and Bobcats® worked to clear the Building’s parking lot. They also kept a backup generator clear of snow. Building 28 houses the Flight Dynamics Facility and NASA Television operations. Both facilities are critical to mission operations.

Bangerter stayed in the NIC from Friday afternoon to Monday morning. Bangerter lives in Annapolis, Md. and didn’t want to take a chance on the roads. He slept on a couch in the Mission Management Area. “It was kind of like the old days, before some our operations were moved to White Sands, NM a few years ago,” said Bangerter. “We used to camp out at Goddard during storms like this.”

NASA Goddard contractors did a great job planning for this storm. “Nobody missed a shift,” Bangerter said. “Everyone was able to focus on the Space Shuttle launch. I am deeply grateful for those who put themselves in harm’s way to make sure our crews were able to get to work safely.”

Friday and Saturday night snow removal crews made it possible to access the Building. There were several cars in the parking lot and crews cleared snow around everyone’s cars. Crews helped Bangerter dig his car out of the snow Monday morning.

“The streets and sidewalks inside Goddard are pretty good compared to the streets outside Goddard,” said Melissa Blizzard. “Crews are plowing continuously.”

Many mission support personal were able to take a break after the Space Shuttle launch. Several dozen, however, were right back at Goddard for the Solar Dynamics Observatory launch.

Meanwhile, ground crews continue to clear snow from sidewalks and roads around Goddard. They will be working through the storm until Goddard is able to open again. “We are a very big team here,” said Holmes. “Everyone is goal-oriented here. We recognize we are part of history.”

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Layers Piled in a Mars Crater Record a History of Changes

Perspective view of layered mound in Gale Crater, Mars
Near the center of a Martian crater about the size of Connecticut, hundreds of exposed rock layers form a mound as tall as the Rockies and reveal a record of major environmental changes on Mars billions of years ago.

The history told by this tall parfait of layers inside Gale Crater matches what has been proposed in recent years as the dominant planet-wide pattern for early Mars, according to a new report by geologists using instruments on NASA's Mars Reconnaissance Orbiter.

"Looking at the layers from the bottom to the top, from the oldest to the youngest, you see a sequence of changing rocks that resulted from changes in environmental conditions through time," said Ralph Milliken of NASA's Jet Propulsion Laboratory, Pasadena, Calif. "This thick sequence of rocks appears to be showing different steps in the drying-out of Mars."

Using geological layers to understand stages in the evolution of a planet's climate has a precedent on Earth. A change about 1.8 billion years ago in the types of rock layers formed on Earth became a key to understanding a dramatic change in Earth's ancient atmosphere.

Milliken and two co-authors report in Geophysical Research Letters that clay minerals, which form under very wet conditions, are concentrated in layers near the bottom of the Gale stack. Above that, sulfate minerals are intermixed with the clays. Sulfates form in wet conditions and can be deposited when the water in which they are dissolved evaporates. Higher still are sulfate-containing layers without detectable clays. And at the top is a thick formation of regularly spaced layers bearing no detectable water-related minerals.

Rock exposures with compositions like various layers of the Gale stack have been mapped elsewhere on Mars, and researchers, including Jean-Pierre Bibring of the University of Paris, have proposed a Martian planetary chronology of clay-producing conditions followed by sulfate-producing conditions followed by dry conditions. However, Gale is the first location where a single series of layers has been found to contain these clues in a clearly defined sequence from older rocks to younger rocks.

"If you could stand there, you would see this beautiful formation of Martian sediments laid down in the past, a stratigraphic section that's more than twice the height of the Grand Canyon, though not as steep," said Bradley Thomson of the Johns Hopkins University Applied Physics Laboratory, Laurel, Md. He and John Grotzinger of the California Institute of Technology in Pasadena are Milliken's co-authors.

NASA selected Gale Crater in 2008 as one of four finalist sites for the Mars Science Laboratory rover, Curiosity, which has a planned launch in 2011. The finalist sites all have exposures of water-related minerals, and each has attributes that distinguish it from the others. This new report is an example of how observations made for evaluating the landing-site candidates are providing valuable science results even before the rover mission launches.

Three instruments on NASA's Mars Reconnaissance Orbiter have provided key data about the layered mound in Gale Crater. Images from the High Resolution Imaging Science Experiment camera reveal details used to map hundreds of layers. Using stereo pairs of the images, the U.S. Geological Survey has generated three-dimensional models used to discern elevation differences as small as a meter (about a yard). Observations by the Compact Reconnaissance Imaging Spectrometer for Mars yielded information about minerals on the surface. The Context Camera provided broader-scale images showing how the layers fit geologically into their surroundings.

Thomson said, "This work demonstrates the synergy of the instruments on the Mars Reconnaissance Orbiter. We wouldn't have as complete a picture if we were missing any of the components."

The mission has been studying Mars since 2006. It has returned more data from the planet than all other Mars missions combined. More information about this mission is at http://www.nasa.gov/mro.

Malin Space Science Systems, San Diego, provided and operates the Context Camera. Johns Hopkins University Applied Physics Laboratory provided and operates the Compact Reconnaissance Imaging Spectrometer. The University of Arizona Lunar and Planetary Laboratory, Tucson, operates the High Resolution Imaging Science Experiment, which was built by Ball Aerospace & Technologies Corp., Boulder, Colo.

JPL, a division of Caltech, manages the Mars Reconnaissance Orbiter for NASA's Science Mission Directorate, Washington. Lockheed Martin Space Systems, Denver, is the prime contractor for the project and built the spacecraft.

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Spirit’s Rear View After Parking for Fourth Winter

NASA's Mars Exploration Rover Spirit recorded this fisheye view with its rear hazard-avoidance camera
NASA's Mars Exploration Rover Spirit recorded this fisheye view with its rear hazard-avoidance camera after completing a drive during the 2,169th Martian day, or sol, of Spirit's mission on Mars (Feb. 8, 2010). The drive left Spirit in the position where the rover will stay parked during the upcoming Mars southern-hemisphere winter.

Spirit moved about 34 centimeters (13 inches) toward the south southeast in a series of drives beginning on Sol 2145 (Jan. 15, 2010). The left-rear wheel (on the right in this rear-facing view) moved out of a rut that it had dug in soft soil in April 2009. The drive motor for the right-rear wheel (on the left in this view) stopped working in late 2009, leaving the six-wheeled rover with only four functioning wheels. The top of the image shows the underside of Spirit's solar array.

The rover's solar array is tilted 9 degrees toward the south for the winter. In the three previous winters that Spirit has spent on Mars, its parked positions tilted toward northward, a better attitude for drawing energy from the sun in the northern sky. Engineers anticipate that, due to the unfavorable tilt for this fourth winter, Spirit will soon be out of communication with Earth for several months. A low-power hibernation mode will shut down almost all functions except keeping a master clock running and checking periodically on Spirit's power status until it has enough power to reawaken.

› Full resolution jpeg (536 Kb)

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WISE Spies a Comet with its Powerful Infrared Eye

WISE's first comet
NASA's Wide-field Infrared Survey Explorer, or WISE, has discovered its first comet, one of many the mission is expected to find among millions of other objects during its ongoing survey of the whole sky in infrared light.

Officially named "P/2010 B2 (WISE)," but known simply as WISE, the comet is a dusty mass of ice more than 2 kilometers (1.2 miles) in diameter. It probably formed around the same time as our solar system, about 4.5 billion years ago. Comet WISE started out in the cold, dark reaches of our solar system, but after a long history of getting knocked around by the gravitational forces of Jupiter, it settled into an orbit much closer to the sun. Right now, the comet is heading away from the sun and is about 175 million kilometers (109 million miles) from Earth.

"Comets are ancient reservoirs of water. They are one of the few places besides Earth in the inner solar system where water is known to exist," said Amy Mainzer of NASA's Jet Propulsion Laboratory in Pasadena, Calif. Mainzer is the principal investigator of NEOWISE, a project to find and catalog new asteroids and comets spotted by WISE (the acronym combines WISE with NEO, the shorthand for near-Earth object).

"With WISE, we have a powerful tool to find new comets and learn more about the population as a whole. Water is necessary for life as we know it, and comets can tell us more about how much there is in our solar system."

The WISE telescope, which launched into a polar orbit around Earth on Dec. 14, 2009, is expected to discover anywhere from a few to dozens of new comets, in addition to hundreds of thousands of asteroids. Comets are harder to find than asteroids because they are much more rare in the inner solar system. Whereas asteroids tour around in the "main belt" between the orbits of Mars and Jupiter, large numbers of comets orbit farther away, in the icy outer reaches of our solar system.

Both asteroids and comets can fall into orbits that bring them close to Earth's path around the sun. Most of these "near-Earth objects" are asteroids but some are comets. WISE is expected to find new near-Earth comets, and this will give us a better idea of how threatening they might be to Earth.

"It is very unlikely that a comet will hit Earth," said James Bauer, a scientist at JPL working on the WISE project, "But, in the rare chance that one did, it could be dangerous. The new discoveries from WISE will give us more precise statistics about the probability of such an event, and how powerful an impact it might yield."

The space telescope spotted the comet during its routine scan of the sky on January 22. Sophisticated software plucked the comet out from the stream of images pouring down from space by looking for objects that move quickly relative to background stars. The comet discovery was followed up by a combination of professional and amateur astronomers using telescopes across the United States.

A teacher also teamed up with an observer to measure comet WISE using a home-built telescope next to a cornfield in Illinois. Their research is part of the International Astronomical Search Collaboration, an education program that helps teachers and students observe comets and asteroids (more information is online at http://iasc.hsutx.edu/ ).

All the data are catalogued at the Minor Planet Center, in Cambridge, Mass., the worldwide clearinghouse for all observations and orbits of minor planets and comets.

Comet WISE takes 4.7 years to circle the sun, with its farthest point being about 4 astronomical units away, and its closest point being 1.6 astronomical units (near the orbit of Mars). An astronomical unit is the distance between Earth and the sun. Heat from the sun causes gas and dust to blow off the comet, resulting in a dusty coma, or shell, and a tail.

Though this particular body is actively shedding dust, WISE is also expected to find dark, dead comets. Once a comet has taken many trips around the sun, its icy components erode away, leaving only a dark, rocky core. Not much is known about these objects because they are hard to see in visible light. WISE's infrared sight should be able to pick up the feeble glow of some of these dark comets, answering questions about precisely how and where they form.

"Dead comets can be darker than coal," said Mainzer. "But in infrared light, they will pop into view. One question we want to answer with WISE is how many dead comets make up the near-Earth object population."

The mission will spend the next eight months mapping the sky one-and-a-half times. A first batch of data will be available to the public in the spring of 2011, and the final catalog a year later. Selected images and findings will be released throughout the mission.

JPL manages the Wide-field Infrared Survey Explorer for NASA's Science Mission Directorate, Washington. The principal investigator, Edward Wright, is at UCLA. The mission was competitively selected under NASA's Explorers Program managed by the Goddard Space Flight Center, Greenbelt, Md. The science instrument was built by the Space Dynamics Laboratory, Logan, Utah, and the spacecraft was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Science operations and data processing take place at the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena. Caltech manages JPL for NASA. The ground-based observations are partly supported by the National Science Foundation. The Minor Planet Center is funded by NASA. More information is online at http://www.nasa.gov/wise and http://wise.astro.ucla.edu.

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NASA Successfully Launches a New Eye on the Sun

NASA's Solar Dynamics Observatory, or SDO, lifted off Thursday from Cape Canaveral Air Force Station's Launch Complex 41 on a first-of-a-kind mission to reveal the sun's inner workings in unprecedented detail. The launch aboard an Atlas V rocket occurred at 10:23 a.m. EST.

The most technologically advanced of NASA's heliophysics spacecraft, SDO will take images of the sun every 0.75 seconds and daily send back about 1.5 terabytes of data to Earth -- the equivalent of streaming 380 full-length movies.

"This is going to be sensational," said Richard R. Fisher, director of the Heliophysics Division at NASA Headquarters in Washington. "SDO is going to make a huge step forward in our understanding of the sun and its effects on life and society."

The sun's dynamic processes affect everyone and everything on Earth. SDO will explore activity on the sun that can disable satellites, cause power grid failures, and disrupt GPS communications. SDO also will provide a better understanding of the role the sun plays in Earth's atmospheric chemistry and climate.

SDO is the crown jewel in a fleet of NASA missions to study our sun. The mission is the cornerstone of a NASA science program called Living With A Star. This program will provide new understanding and information concerning the sun and solar system that directly affect Earth, its inhabitants and technology.

The SDO project is managed at NASA's Goddard Space Flight Center in Greenbelt, Md. NASA's Launch Services Program at Kennedy Space Center managed the payload integration and launch.

For launch coverage, briefing materials, and multimedia, visit:

http://www.nasa.gov/mission_pages/sdo/news/briefing-materials-20100209.html

For more information about the SDO mission, visit:

http://sdo.gsfc.nasa.gov

and

http://www.nasa.gov/sdo

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Orbiting Space Shuttle Astronauts Answer Questions from Students Nationwide

Students in elementary and middle schools nationwide will have their questions about space answered live on Feb. 14 by space shuttle astronauts orbiting 220 miles above Earth.

The students, who attend nine NASA Explorer Schools nationwide, submitted their questions to NASA via video. Space shuttle Pilot Terry Virts and Mission Specialist Kathryn Hire will answer the students' questions on NASA TV. The call is targeted for 10:34 p.m. to 10:54 p.m. EST on Sunday, Feb. 14, but could take place five to 15 minutes earlier or later. Viewers should consult the NASA TV schedule to confirm timing. Any questions the astronauts do not answer will be answered later by subject matter experts during an event on NASA's Digital Learning Network.

Virts and Hire launched to space Monday, Feb. 8, aboard space shuttle Endeavour from NASA's Kennedy Space Center in Florida. During their 13-day mission, Endeavour's crew are conducting three spacewalks and delivering the Tranquility node and a cupola to expand the space station.

The NASA Explorer Schools that submitted video questions are:

  • Phenix City Intermediate School in Phenix City, Ala.
  • Edward Harris, Jr. Middle School in Elk Grove, Calif.
  • Sequoia Middle School in Portersville, Calif.
  • Vintage Math, Science and Technology Magnet School in North Hills, Calif.
  • Goldsboro Elementary Magnet School in Sanford, Fla.
  • Stewart Magnet Middle School in Tampa, Fla.
  • Vance Elementary School in Asheville, N.C.
  • Vernon School in Portland, Ore.
  • John B. Cary Elementary School in Richmond, Va.
The NASA Explorer Schools project establishes a three-year partnership between NASA and schools in diverse communities to address local challenges in science, technology, and mathematics education. The goal is to bring educators, administrators, students, and families together in sustained involvement with NASA's education programs.

The event is part of a series with educational organizations in the U.S. and abroad to improve teaching and learning in science, technology, engineering and mathematics. The in-orbit call is part of Teaching From Space, a NASA project that uses the unique environment of human spaceflight to promote learning opportunities and build partnerships with the kindergarten through 12th grade education community.

NASA Television will air video of Virts and Hire during the downlink. For NASA TV downlink, schedule and streaming video information, visit:

http://www.nasa.gov/ntv

For information about NASA Explorer Schools, visit:

http://explorerschools.nasa.gov

For information about NASA's education programs, visit:

http://www.nasa.gov/education

For information about the space shuttle, visit:

http://www.nasa.gov/shuttle

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Congratulating the Team

Congratulating the Team
NASA Administrator Charles Bolden, left, is seen in this fish-eye view as he congratulates NASA Shuttle Launch Director Michael Leinbach and the launch team in Firing Room Four of the Launch Control Center for a successful launch of the space shuttle Endeavour and the start of the STS-130 mission at NASA Kennedy Space Center in Cape Canaveral, Fla. on Monday, Feb. 8, 2010. Endeavour and its crew will deliver to the International Space Station a third connecting module, the Italian-built Tranquility node and the seven-windowed cupola, which will be used as a control room for robotics.

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Spitzer Goes to the Olympics

This colorful cosmic view is part of a Spitzer Space Telescope art project 2010 Winter Olympics cultural festival in VancouverArtwork inspired by NASA's Spitzer Space Telescope is making an appearance at this year's Winter Olympics in Vancouver, British Columbia. No, it's not battling other telescopes for the "gold," but its observations are now on display as part of the Vancouver 2010 Cultural Olympiad Festival.

The Spitzer art project, called "We are Stardust," was created by George Legrady, a professor at the University of California, Santa Barbara. The two-screen installation maps the sequence of 36,034 observations made by the space telescope from 2003 to 2008. Spitzer sees infrared light from the cosmos, capturing images of everything from comets in our solar system to galaxies billions of light-years away.

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

Read more at http://www.ia.ucsb.edu/pa/display.aspx?pkey=2174

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

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Q and A with SDO Program Executive Dana Brewer

SDO Program Executive Dana Brewer What is SDO and what is its purpose and mission?


SDO is the Solar Dynamics Observatory. Its purpose is to study the scientific processes that produce change inside, at the surface, and in the atmosphere of the sun. Changes in the sun, or solar variability, produce changes in the levels of radiation and energy in the heliosphere (or space) within our solar system. The changes are called space weather, and they affect communications and other satellite signals, electrical power lines, radiation doses to polar aircraft/crew, and spacecraft components and occupants both near and away from Earth.

What's different or unique about SDO?

SDO will take measurements of the entire solar disc for 22 72-day time periods over SDO’s 5-year prime mission life. This equates to 4 years of data, and the prime mission lifetime is approximately half of the time period for an 11-year cyclical solar cycle. SDO’s instruments will look at the inside, surface, and corona of the sun at the same time, so the causes of solar variations can be identified together with the outcomes from the causes. For example, if there are a lot of intertwined magnetic field lines inside the sun, a specific combination of the lines and their strengths may be able to be attributed to a solar flare. If we can figure out many of these cause and effect relationships, we will have a start on developing a predictive space weather capability.

What is space weather?

Space weather is the state of the heliosphere that changes due to solar variability. The heliosphere is the region of the sun’s influence, our solar system. Space weather effects are the deleterious consequences of space weather, and they include things that can be changed by changing the ionizing radiation dose and/or the electrical and magnetic fields from the sun.

How will SDO improve our knowledge and understanding of space weather?

SDO will allow us to study causes and effects on the sun. We are viewing the entire disk of the sun all the time, and our data from viewing result in simultaneous data from the inside, surface, and atmosphere of the sun. This allows the scientists to develop cause and effect relationships between activities in the different layers of the sun. Only when this is done will we truly have a foundation to develop a predictive capability for space weather.

How will the SDO mission benefit the average person?

The SDO mission will lead to a predictive space weather capability. This capability will allow us to disconnect the connections in the electrical power grid when solar activity has the potential to damage power transmission hardware; this will allow the damage to be localized instead of resulting in an extended power outage across the eastern or western seaboard of the U.S. An extended power outage would ripple across the U.S. infrastructure, leading to problems with water distribution and loss of perishable foods, medications, heating/air conditioning, sewage disposal, phone service, etc. The space weather predictive capability will also allow accurate adjustments of satellites signals to ensure the uninterrupted retention of communications with ships, medical pagers, and telecommunications ground stations.

What is the life cycle of the SDO mission? Can it last longer?

The prime mission life of the SDO is 5 years, and, under a worst case condition, there is fuel available to extend the mission by another 5 years. There may be additional fuel if the Observatory’s fuel is not used to reach geosynchronous transfer orbit immediately after launch. The SDO lifetime also depends upon the extent of degradation of the Observatory’s microelectronics due to the harsh ionizing radiation environment in geosynchronous Earth orbit.

What science instruments will SDO carry?

SDO will carry three instruments. The Helioseismic and Magnetic Imager (HMI) will map the sun’s magnetic fields and peer beneath the sun’s surface to decipher the physics of the core of the sun which is the solar dynamo. The Atmospheric Imaging Assembly (AIA) is a set of 4 telescopes designed to photograph the sun’s surface and atmosphere in 8 wavelengths simultaneously. The Extreme Ultraviolet Variability Experiment (EVE) will measure fluctuations in the sun’s ultraviolet energy output, and this output has a direct effect of heating, changing the density, and breaking apart atoms and molecules in the Earth’s upper atmosphere.

Where will the data be stored and who will look at the data produced by SDO?

The SDO data will be transmitted from the Observatory to a ground station in Las Cruces, New Mexico. The ground station will immediately transmit the data to the two Science Operations Centers at the University of Colorado and Stanford University; it will also store the data for up to 30 days for re-transmission to the Science Operations Centers in the event that the first transmission is not successful. Each SDO instrument is part of a science investigation team that has many science co-investigators. The three science teams are responsible for initial processing of the raw science data and making the initial detailed products available to the public in as short a time as possible after SDO is commissioned. In addition, short-term quick look products may be available several times per hour. So, in the future, you may be able to routinely get a status of the sun on your cell phone or over the Internet.

What made you choose science/engineering as a career?

I enjoyed chemistry and math when I was in high school. I also thought of how great it would be to participate in the space program when I saw the Mercury and Gemini astronauts going into space. I accepted the challenge of succeeding in science when a chemistry professor told me that women should not get science degrees, because it’s a man’s field. (This was many years ago, before the onset of “women’s liberation.”) I recall that there were about 6 females in the first of three sophomore physics courses out of 600 students. By the time we got to the third course, the 6 females were still in the course, but the class size had decreased to 200. When I graduated from undergraduate school, jobs were scarce (another economic downturn), and I accepted a graduate teaching assistantship in chemistry. After obtaining my Ph.D., I did theoretical chemistry research for 10 years until an opportunity became available for me to transition from science to engineering. The rest is history. After all, where else can I live my dream? Society’s acceptance of female engineers has caught up with my activities.

What advice would you give young women interested in pursuing careers in science or engineering?

Pursue your dreams, but understand that science and engineering are more time-consuming courses of study than other majors. Accept the challenge, because you will do well and enjoy your career. Live your dream.


About Dana Brewer
  • B.S. in general Science from Penn State, Ph.D. in Quantum Chemistry from Virginia Tech.
  • Ten years as contractor at NASA Langley doing earth science atmospheric modeling.
  • 6 years as space environments requirements manager at Space Station Level II Program Office in Reston.
  • 5 years as Program Manager in spacecraft technology development (including space environments).
  • 4 years as New Millennium Program Manager (including flight validation of ion propulsion on Deep Space-1 mission.
  • 14 years as Program Executive in Heliophysics Division in Science Mission Directorate (includes formulation of Hinode, STEREO, Space Environment Testbeds and the Living With a Star and Solar Terrestrial Probes Programs; pre-formulation of Radiation Belt Storm Probes, Solar Orbiter, Solar Probe Plus; implementation of SDO, LWS program, and Space Environment Testbeds.).

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‘Go’ for Launch

At Launch Pad 39A at NASA's Kennedy Space Center in Florida, the crew of space shuttle Endeavour's STS-130 mission posed for a group portrait in front of Endeavour's external tank and one of its solid rocket boosters at the conclusion of the Terminal Countdown Demonstration Test, the dress rehearsal for their launch.

From left are Robert Behnken, Commander George Zamka, pilot Terry Virts, Kathryn Hire, Nicholas Patrick and Stephen Robinson. The primary payload on STS-130 is the International Space Station's Node 3, Tranquility, a pressurized module that will provide room for many of the station's life support systems. Endeavour is set to launch on Feb. 7.

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On Launch Pad 39A

The space shuttle Endeavour is seen after the rotating service structure is rolled back on Saturday, Feb. 6, 2010 at Launch Pad 39A of the NASA Kennedy Space Center in Cape Canaveral, Florida. Endeavour and the crew members of the STS-130 mission are set to launch on Sunday at 4:39 a.m. EST.

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STS-130 Launch Blog

Follow space shuttle Endeavour's exciting countdown to launch as Steve Siceloff blogs from inside Firing Room 3 at the Launch Control Center at NASA's Kennedy Space Center. Continuous coverage of the launch begins at 11 p.m. Sunday for a launch attempt at 4:14 a.m. Monday

George Zamka leads the six-person crew on the mission to add the Tranquility module and a new "window on the world" to the International Space Station. Tranquility is the first new pressurized module to be carried to the orbiting laboratory since STS-124 took the pressurized section of the Japanese Experiment Module "Kibo" to the station in June 2008. But station residents couldn't be blamed for looking forward most of all to the cupola Endeavour will carry into space. Once at its place on the station, the cupola will afford station crew members a place to comfortably sit among seven windows and watch the Earth spin below them. And they won't even have to wear a spacesuit. from Kennedy.

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