Wednesday, July 1, 2009

NASA Engineer Helps Comedian Tackle Fear of Flying

Langley aerospace engineer Anna McGowan and NASA 360 co-host Johnny Alonso (R) spoke with Malkoff (L) at the Newport News - Williamsburg International AirportComedian Mark Malkoff is spending the entire month living on AirTran airliners to try to overcome his fear of flying.Survey any number of airline passengers and you may not hear the most positive reaction to air travel these days. Seats are cramped. Planes are crowded. And don't even get anybody started on delays, security procedures or extra costs. So what would possess anyone to live on an airplane for a month and endure 30 days of conditions many people would prefer to avoid?

Meet Mark Malkoff.

The 33-year-old comedian/writer/filmmaker is staying on an AirTran airplane the entire month of June and sharing his experiences with the public via the web. According to his website, markonairtran.com, "Although I'll switch planes, I'll never set foot in an airport. I'll change flights by way of the tarmac."

How does somebody keep busy on a plane for an entire month? Malkoff's videos show he's already memorized the SkyMall catalogue, played Twister and called Bingo over the airplane microphone. But he's also been meeting new people, including aerospace engineer Anna McGowan from NASA's Langley Research Center in Hampton, Va.

McGowan visited with Malkoff at the nearby Newport News - Williamsburg Airport to help him learn more about flying and especially about the research NASA is doing to make more it efficient and environmentally friendly.

"We're developing technologies for the next generation of flight," said McGowan. "We're working on engines that have a much lower fuel consumption. We're also reducing the weight of airplanes using innovative materials that are lighter weight but stronger than they are today."

Malkoff started his journey "to get over my fear of flying. I've struggled with the fear for years." He says flying has definitely gotten easier. "If the fear started at a 10 ... it's now about a two," he said.

But even after flying 197 hours and 82,000 miles (approx. 132,000 km), Malkoff still had questions about why planes do some of the things they do. He asked McGowan why planes have to bank or fly at a "tilt".

"The pilot is trying very carefully to make a smooth one-G turn, so that your glasses aren't sliding off the edge of your tray and so that everybody stays level in the airplane," said McGowan. "He wants to avoid side slip."

Joining McGowan at the airport was Johnny Alonso, one of the hosts of "NASA 360," a half hour NASA TV program that explores NASA's contributions to everyday life. NASA 360 and a crew that follows Malkoff both videotaped the conversation for future shows.

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Tuesday, June 30, 2009

Ulysses Hears the Siren's Song

UlyssesUlysses, a joint NASA and European Space Agency mission, will officially cease operations Monday, June 30, when the command to switch off the transmitter is uplinked to the spacecraft. Ulysses, which operated for more than 18 years, had charted the unexplored regions of space above the poles of the sun.

The Ulysses orbital path is carrying the spacecraft away from Earth. The ever-widening gap has progressively limited the amount of data transmitted. Ulysses project managers, with the concurrence of ESA and NASA, decided it was an appropriate time to end this epic scientific adventure.

Space Shuttle Discovery launched Ulysses on Oct. 6, 1990. A combination of solid fuel motors propelled Ulysses out of low-Earth orbit and toward Jupiter. Ulysses swung by Jupiter on Feb. 8, 1992. The giant planet's gravity bent the spacecraft's flight path southward and away from the ecliptic plane, putting the probe into a final orbit that would take it over the sun's south and north poles.

The European Space Agency's European Space Research and Technology Centre and European Space Operations Centre has managed the mission in coordination with NASA's Jet Propulsion Laboratory. Ulysses is tracked by NASA’s Deep Space Network. A joint ESA/NASA team at JPL has overseen spacecraft operations and data management. Teams from universities and research institutes in Europe and the U.S. provided the 10 instruments on board.

More information about the mission is available at: http://ulysses.jpl.nasa.gov

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Monday, June 29, 2009

A Glowing Vision of the Early Universe

A composite image of a black hole (blue) lighting up a lyman alpha blob (yellow)Galaxy formation in the early universe just became a little less mysterious.

Cosmologists already knew the big picture. In the several hundred million years after the Big Bang, matter in the expanding universe began falling together into clumps; littler clumps within the clumps fell in on themselves to form the first stars; and many of the original clumps eventually coalesced into bigger pools to make modern-sized galaxies.

But why did galaxies come out the size they did, rather than staying small or growing indefinitely huge? Astronomers have new insight on this question thanks to images obtained in 2007 by NASA's Chandra X-ray Observatory and released to the public today.

Scientists have known for nearly 10 years about gassy objects in the early universe called “Lyman-alpha blobs.” They’re named for their emission of ultraviolet light at the Lyman-alpha wavelength given off by hot hydrogen atoms. The energy to make the blobs light up must come from somewhere. In a paper to be published in the July 10th Astrophysical Journal, a team describes observing a region of Lyman-alpha blobs called SSA22 about a half million light-years in diameter. They say they have found why the blobs shine and have also turned up a correlation between the blobs and active black holes at the center of galaxies within them.

Massive black holes exist in most galaxies, but only some of the holes are consuming matter fast enough to light up brightly. Co-author Jim Geach (Durham University, UK) says 1% to 10% of galaxies in general have an active-black-hole nucleus, but the percentage is five times higher among the early galaxies with Lyman-alpha blobs surrounding them. These are large galaxies in the late stages of formation, seen when the universe was only about 15% of its present age. By then the holes in question had grown very massive, to roughly a billion solar masses.

Apparently, when we see a Lyman-alpha blob we are seeing the blaze from these black holes (and perhaps from nascent stars) heating a galaxy’s remaining gas and driving it off into intergalactic space, thereby preventing it from coalescing into new stars. In other words, we’re seeing galaxies at the point when they shut off their own growth.

Theorists modeling the early universe have been eager to observe this crucial “feedback” stage in galaxy evolution. The feedback mechanism explains the strong correlation between the mass of a galaxy’s central bulge of old stars and the mass of its central black hole (the ratio is always about 700 to 1). The growing flood of radiation from the growing black hole blows remaining gas out of the galaxy — both preventing the galaxy from forming new stars and preventing the hole’s further growth. (The gassy disk of a spiral galaxy, full of younger stars, would be the result of new material falling in later.)

This transition stage should be brief in cosmic terms, which is why it has been hard to catch in progress. But the research team suspects that nearly all galaxies should go through it.

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Sunday, June 28, 2009

Magnetic field on bright star Vega

Astronomy & Astrophysics is publishing the first detection of a magnetic field on the star Vega, one of the brightest stars in the sky. Using the high-sensitivity NARVAL spectropolarimeter installed at the Bernard-Lyot telescope (Pic du Midi Observatory, France), a team of astronomers detected the effect of a magnetic field (known as the Zeeman effect) in the light emitted by Vega.

Vega is a famous star among amateur and professional astronomers. Located at only 25 light years from Earth in the Lyra constellation, it is the fifth brightest star in the sky. It has been used as a reference star for brightness comparisons. Vega is twice as massive as the Sun and has only one tenth its age. Because it is both bright and nearby, Vega has been often studied but it is still revealing new aspects when it is observed with more powerful instruments. Vega rotates in less than a day, while the Sun's rotation period is 27 days. The intense centrifugal force induced by this rapid rotation flattens its poles and generates temperature variations of more than 1000 degrees Celsius between the polar (warmer) and the equatorial regions of its surface. Vega is also surrounded by a disk of dust, in which the inhomogeneities suggest the presence of planets.

This time, astronomers analyzed the polarization of light emitted by Vega and detected a weak magnetic field at its surface. This is really not a big surprise because one knows that the charged particle motions inside stars can generate magnetic fields, and this is how solar and terrestrial magnetic fields are produced. However, for more massive stars than the Sun, such as Vega, theoretical models cannot predict the intensity and the structure of the magnetic field, so that astronomers had no clue to the strength of the signal they were looking for. After many unsuccessful attempts in past decades, both the high sensitivity of NARVAL and the full dedication of an observing campaign to Vega have made this first detection possible.

The strength of Vega magnetic field is about 50 micro-tesla, which is close to that of the mean field on Earth and on the Sun. This first observational constraint opens the way to in-depth theoretical studies about the origin of magnetic fields in massive stars. This detection also suggests that magnetic fields exist but have not been detected yet on many stars like Vega, but farther and more difficult to observe. Astronomers believe that this discovery will be a key step in understanding stellar magnetic fields and their influence on stellar evolution. As for Vega, it is now the prototype of a new class of magnetic stars and will definitely continue fascinating astronomers for years.

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Friday, June 26, 2009

Supersonic Diving Quieting the Boom

A NASA F-18 dives toward a targeted area of Edwards AFB during a SonicBOBS calibration flight.Sonic booms are a part of life at Edwards Air Force Base and in surrounding communities, so booms generated on June 11 by two F/A-18s from NASA’s Dryden Flight Research Center went relatively unnoticed. The exception included several NASA and Gulfstream engineers monitoring boom recording and measuring devices located in the Air Force Flight Test Center's museum and at a seismometer located on base.

Called Sonic Booms On Big Structures, or SonicBOBS, Phase 0, these flights were preliminary calibration flights for an upcoming NASA study scheduled for September that is designed to gather sonic boom data on larger buildings.

The project is part of a NASA effort to characterize the effect of sonic booms on ground structures. It is part of the agency's sonic boom reduction technology research to help make overland supersonic cruise a reality.

“We recorded nine loud and quiet sonic booms with a variety of sensors, both inside and outside buildings," said Ed Haering, Dryden's principal investigator for the SonicBOBS project. "These data will be used to tailor the experiment design for September’s flights,” Haering said.

For the flights, the two NASA F-18s flew both straight supersonic flight profiles as well as a unique supersonic diving profile designed to present a quieter sonic boom to specific locations along their flight path. The F-18s flew in Edwards' High Altitude Supersonic Corridor at 32,000 to 40,000 feet for the supersonic runs.

SonicBOBS complements previous efforts in 2006 and 2007 to measure the pressure and loudness of sonic booms on both older-and newer-construction base housing.

Window rattle and other contact-induced acoustic sources are important aspects of the high frequency response inside a building subjected to sonic booms. The earlier base housing research showed that indoor noise from sonic booms might be more annoying than the same booms heard outdoors.

Currently, Federal Aviation Administration regulations prohibit supersonic flight over land except in special restricted military flight corridors. A resurgent interest in the last 10 years by aerospace companies in supersonic business jets that could cruise supersonically over land led to several research projects to shape and modify supersonic shockwaves. Among them, the Shaped Sonic Boom Demonstrator Project by NASA, Northrop Grumman and DARPA and the QuietSpike Project by NASA and Gulfstream both demonstrated the successful suppression of sonic boom intensity on the ground.

NASA's Langley Research Center, Hampton, Va., and Gulfstream Aerospace Corporation, Savannah, Ga., are partners with NASA Dryden and the Air Force Flight Test Center in the project. The effort is funded by the NASA Aeronautics Research Mission Directorate’s Supersonics Project, which supports NASA's Fundamental Aeronautics program strategy of developing systems level, multidiscipline capabilities for supersonic civilian and military applications.

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Thursday, June 25, 2009

NASA Awards Space Station Support Contract to ARES Corp.

NASA has signed a $144 million follow-on contract with ARES Corp. of Burlingame, Calif., for International Space Station Program integration and control services.

ARES will provide support for configuration management, data management, information technology, safety and mission assurance, vehicle integrated performance, resource and budget analysis, program schedule development, engineering and technical services, spacecraft integration, international partner integration and strategic analysis planning.

The three-year contract is effective Oct. 1, 2009 through Sept. 30, 2012, and includes two one-year options that could extend the contract through Sept. 30, 2014. If both options are exercised, the total value of the indefinite delivery, indefinite quantity contract would be $180 million.

ARES will perform the work on-site at NASA's Johnson Space Center in Houston, or at nearby offices. Significant subcontractors include Barrios Technology and Booz-Allen Hamilton, both of Houston.

The previous contract was awarded in November 2003, and had a total value of $154 million, including all of the options that were exercised, through Sept. 30, 2009.

For more information about NASA and agency programs, visit:

http://www.nasa.gov

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Wednesday, June 24, 2009

NASA Awards Two Small Explorer Development Contracts

NASA has selected two science proposals to be developed into full missions as part of the agency's Small Explorer, or SMEX, Program. The selections will implement projects that will study our sun and some of the most exotic objects in the universe, such as neutron stars and black holes.

Both missions will launch by 2015; the first could launch by the end of 2012. Mission costs will be capped at $105 million each, excluding the launch vehicle.

"These two missions demonstrate the value of the Small Explorer Program," said Ed Weiler, associate administrator for NASA's Science Mission Directorate. "For a relatively small investment, we'll see an amazing amount of science generated."

The two winning proposals are:

1. Interface Region Imaging Spectrograph. Principal Investigator Alan M. Title, Lockheed Martin Advanced Technology Center, Palo Alto, Calif.

The Interface Region Imaging Spectrograph mission will use a solar telescope and spectrograph to explore the solar chromospheres. This is a crucial region for understanding energy transport into the solar wind and an archetype for stellar atmospheres. Recent discoveries have shown the chromosphere is significantly more dynamic and structured than previously thought. The unique instrument capabilities, coupled with state of the art 3-D modeling, will explore this dynamic region in detail. The mission will greatly extend the scientific output of existing heliophysics spacecraft that follow the effects of energy release processes from the sun to Earth.

2. Gravity and Extreme Magnetism SMEX. Principal Investigator Jean H. Swank, NASA's Goddard Space Flight Center, Greenbelt, Md.

Among the thousands of X-ray sources observed with prior and current X-ray satellites, only one astrophysical object, the Crab Nebula, has been measured in polarized X-rays. By providing an increase in sensitivity of more than 100 times, the Gravity and Extreme Magnetism SMEX mission will detect and measure the polarization of the X-rays emitted by some of the most energetic and enigmatic objects in the cosmos. These include ultra-dense neutron stars and stellar-mass black holes, which are the remains of the dying explosions of very hot, massive stars, and ultra-massive black holes at the centers of distant galaxies. By studying the changes with time and energy of their polarized X-ray emission, the mission will probe the bending of space and the curving of light in regions of extreme gravity near these objects.

The SMEX Program is designed to provide frequent, low-cost access to space for heliophysics and astrophysics missions using small- to mid-sized spacecraft. The program also seeks to raise public awareness of NASA's space science missions through educational and public outreach activities. The winning proposals are the 12th and 13th Small Explorer missions selected for flight.

Goddard manages the Explorer program for NASA's Science Mission Directorate in Washington. For more information about the program, visit:

http://explorers.gsfc.nasa.gov

For information about NASA, visit:

http://www.nasa.gov

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Tuesday, June 23, 2009

Successful Spacecraft Separation

NASA's Lunar Reconnaissance Orbiter, or LRO, successfully separated from the Centaur upper stage and Crater Observation and Sensing Satellite, or LCROSS, spacecraft at 6:16:43 p.m. EDT.

The official transfer of control from the Centaur rocket to LCROSS is expected about 9:30 p.m.

LRO will reach the moon on Tuesday at 5:43 a.m.

LCROSS and the Centaur rocket will stay attached for the next four months. They will then separate and be directed to impact the moon on Oct. 9, UTC.

Mission News

3, 2, 1, Liftoff!
Launch of the Atlas V rocket carrying the LRO and LCROSS spacecraft
NASA's Lunar Reconnaissance Orbiter and Lunar Crater Observation and Sensing Spacecraft are on their way to the moon atop the same Atlas V rocket, although they will use vastly different methods to study the lunar environment. LRO will go into orbit around the moon, turning its suite of instruments towards the moon for thorough studies. The spacecraft also will be looking for potential landing sites for astronauts.

LCROSS, on the other hand, will guide an empty upper stage on a collision course with a permanently shaded crater in an effort to kick up evidence of water at the moon's poles. LCROSS itself will also impact the lunar surface during its course of study.

Liftoff occurred at 5:32 p.m. EDT. Mission managers used the last launch opportunity due to storms surrounding the launch site.

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Sunday, June 21, 2009

LRO/LCROSS Launch Date Set

NASA's Lunar Reconnaissance Orbiter and Lunar Crater Observation and Sensing Satellite are set to lift off together aboard an Atlas V rocket on Thursday, June 18, at 5:12 p.m. EDT. Two additional launch opportunities are available at 5:22 p.m. and 5:32 p.m.

In preparation for liftoff, the Atlas V launch vehicle is scheduled to roll out to the pad Wednesday at 10 a.m.

Countdown milestones can be found on NASA's Launch Blog beginning at 2 p.m. EDT.

Atlas V Rolls to Launch Pad
In the left background is space shuttle Endeavour on pad 39A, on the right foreground is the Atlas V with LRO and LCROSS spacecrafts on top at their launch pad.
Mission Overview

NASA's Lunar Reconnaissance Orbiter and Lunar Crater Observation and Sensing Spacecraft will fly to the moon atop the same Atlas V rocket, although they will use vastly different methods to study the lunar environment. LRO will go into orbit around the moon, turning its suite of instruments towards the moon for thorough studies. The spacecraft also will be looking for potential landing sites for astronauts.

LCROSS, on the other hand, will guide an empty upper stage on a collision course with a permanently shaded crater in an effort to kick up evidence of water at the moon's poles. LCROSS itself will also impact the lunar surface during its course of study.

Liftoff currently is scheduled for June 18 at 5:12 p.m. EDT. There are two more launch opportunities that day at 5:22 p.m. and 5:32 p.m.

Additional Resources
› LRO Fact Sheet
› LRO/LCROSS Press Kit
› LRO/LCROSS Launch Coverage Events

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Friday, June 19, 2009

Endeavour Fueling Continues

Space shuttle Endeavour's external fuel tank is being filled with more than 500,000 gallons of liquid hydrogen and liquid oxygen. The three-hour operation began at 11:04 p.m. EDT. The Liquid Hydrogen Low Level Cutoff (LLCO) sensors will go "wet" at about 11:49 p.m. The tank will be completely filled, known as stable replenish, at about 2:04 a.m.

The launch countdown currently is holding at T-3 hours, which will last until 1:45 a.m. EDT.

There still is a 80 percent chance that weather will not affect the 5:40 a.m. launch of STS-127.

Space Shuttle Mission: STS-127

Space shuttle Endeavour is bathed in light on Launch Pad 39A.
STS-127 Mission Overview
The 16-day mission will feature five spacewalks and complete construction of the Japan Aerospace Exploration Agency's Kibo laboratory. Astronauts will attach a platform to the outside of the Japanese module that will allow experiments to be exposed to space.

The STS-127 crew members are Commander Mark Polansky, Pilot Doug Hurley and Mission Specialists Dave Wolf, Christopher Cassidy, Tom Marshburn, Tim Kopra and Canadian Space Agency astronaut Julie Payette. Kopra will join the space station crew and replace Japanese astronaut Koichi Wakata. Wakata will return to Earth on Endeavour to conclude a three-month stay at the station.

STS-127 Additional Resources
› Mission Press Kit (6.3 Mb PDF)
› Mission Summary (484KB PDF)
› Meet the STS-127 Crew
› Flow Valve Fact Sheet (447 Kb PDF)

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European satellites probe a new magnetar

Magnetar SGR 0501+4516On Aug. 22, 2008, NASA's Swift satellite reported multiple blasts of radiation from a rare object known as a soft gamma repeater, or SGR. Now, astronomers report an in-depth study of these eruptions using the European Space Agency's XMM-Newton and International Gamma-Ray Astrophysics Laboratory (INTEGRAL) satellites.

The object, designated SGR 0501+4516, was the first of its type discovered in a decade and is only the fifth confirmed SGR. "Some sources are extremely active, but others can be quiet for a decade or more," said Nanda Rea, University of Amsterdam, who led the study. "This suggests many members of this class remain unknown."

Astronomers think the eruptions of SGRs arise from the most highly magnetized objects in the universe -- magnetars. Magnetars are neutron stars -- the crushed cores of exploded stars -- that, for reasons not yet known, possess ultra-strong magnetic fields. With fields 100 trillion times stronger than Earth's, a magnetar placed half the moon's distance would wipe the magnetic strips of every credit card on the planet. "Magnetars allow us to study extreme matter conditions that cannot be reproduced on Earth," said Kevin Hurley, a team member at the University of California, Berkeley.

Both SGRs and a related group of high-energy neutron stars -- called anomalous X-ray pulsars -- are thought to be magnetars. But, all told, astronomers know of only 15 examples.

SGR 0501+4516, estimated to lie about 15,000 light years away, was only discovered because its outburst gave it away. Astronomers think an unstable configuration of the star's magnetic field triggers the eruptions. "Once the magnetic field resumes a more stable configuration, the activity ceases and the star returns to quiet and dim emission," Rea said.

Twelve hours after Swift pinpointed SGR 0501+4516, XMM-Newton began the most detailed study of a fading magnetar outburst ever attempted. The object underwent hundreds of small bursts over a period of more than four months. Only five days after the initial eruption, INTEGRAL detected X-rays from the object that were beyond the energy range XMM-Newton can see. It's the first time such transient high-energy X-ray emission has been detected during an SGR's outburst phase. This emission disappeared within ten days of the outburst. The findings were published online June 15 in the Monthly Notices of the Royal Astronomical Society.

The team plans further observations of SGR 0501+4516 with XMM-Newton. They hope to detect the object in a quiet state in order to probe the calm after the storm.

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Wednesday, June 17, 2009

NASA Postpones Launch of Space Shuttle Endeavour

NASA postponed space shuttle Endeavour's launch to the International Space Station on Saturday because of a leak associated with the gaseous hydrogen venting system outside the shuttle’s external fuel tank. The system is used to carry excess hydrogen safely away from the launch pad. Managers scrubbed the launch for at least 96 hours.

The earliest the shuttle could be ready to launch is June 17. However, there is a conflict on the Eastern Range that date with the scheduled launch of the Lunar Reconnaissance Orbiter/Lunar Crater Observation and Sensing Satellite.

Mission managers will hold a meeting at 2 p.m. EDT Sunday to discuss the repair options and Endeavour's launch opportunities. A news conference will follow the meeting and air on NASA Television and the agency’s Web site.

The 16-day mission will feature five spacewalks and complete construction of the Japan Aerospace Exploration Agency's Kibo laboratory. Astronauts will attach a platform to the outside of the Japanese module that will allow experiments to be exposed to space.

The STS-127 crew members are Commander Mark Polansky, Pilot Doug Hurley and Mission Specialists Dave Wolf, Christopher Cassidy, Tom Marshburn, Tim Kopra and Canadian Space Agency astronaut Julie Payette. Kopra will join the space station crew and replace Japanese astronaut Koichi Wakata. Wakata will return to Earth on Endeavour to conclude a three-month stay at the station.

Polansky, who has a Twitter account named Astro_127, can be followed online at:

http://www.twitter.com/Astro_127

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

http://www.nasa.gov/ntv

For the latest information about the STS-127 mission and its crew, visit:

http://www.nasa.gov/shuttle

For information about the International Space Station, visit:

http://www.nasa.gov/station

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Tuesday, June 16, 2009

Revealing Jamestown Settlers' Sketches of The New World

Jamestown archaeologists found a slate tablet covered with faint sketches, words and numbers thrown in what appears to be an original Jamestown well.NASA researchers who normally study futuristic materials are using their high tech scanners to reveal the past.

Technicians at NASA's Langley Research Center in Hampton, Va., just finished inspecting a 400-year-old slate tablet recently recovered from an early 17th century well at Historic Jamestowne, the 1607 site of the first permanent English settlement in North America.

NASA Langley has scanned dozens of artifacts for Preservation Virginia, since its Jamestowne Rediscovery archaeologists began the excavation of James Fort 15 years ago. But this is the first time researchers used a new, more sophisticated "micro-focus computed tomography x-ray system" that Langley installed last summer in its Nondestructive Evaluation Sciences laboratory.

"It's a three-dimensional imaging system that allows us to see inside materials without having to take them apart," said Ray Parker, nondestructive evaluation sciences engineer. "It's like a hospital CT scanner, only higher precision. We normally use it to inspect materials for aerospace use, like pieces of the shuttle or composites for hypersonic vehicles."

The eight-foot long, four-foot wide, six-foot high machine, called the X-Tek HMX-ST 225, uses X-rays and computer processing to create a 3-D "picture" of whatever it scans. In this case archaeologists are trying to determine what's written on the slate tablet they found.

"There's a deposit of rust on the tablet and it's covering up lettering and drawings," said Parker. "We're looking at the results of our scans to see if we read what's there."

This is the second time that Parker and technician John Grainger have worked with the Jamestown Rediscovery archaeologists. Last time they inspected a 16th century Scottish pistol found in one of the fort's wells.

"I think it's fantastic they're finding all this stuff and we get to inspect some of it," Parker said. "I've always had an interest in history. When I grew up we used to visit the Historic Triangle -- Jamestown, Williamsburg and Yorktown, Va. -- frequently."

NASA Langley started working with Preservation Virginia more than seven years ago helping to identify artifacts. That role expanded when NASA teamed with Jamestown 2007 to promote the spirit of exploration then, now and in the future. During the 18-month long celebration to honor the 400th anniversary of Jamestown, NASA even flew a small lead cargo tag, bearing the words "Yames Towne," and some commemorative mementoes on board the space shuttle Atlantis to commemorate the nation's pioneering spirit.

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Monday, June 15, 2009

WISE Mission Assembled and Preparing for Launch

NASA's Wide-field Infrared Survey Explorer, or WISE, has been assembled and is undergoing final preparations for a planned Nov. 1 launch from Vandenberg Air Force Base, Calif.

The mission will survey the entire sky at infrared wavelengths, creating a cosmic clearinghouse of hundreds of millions of objects -- everything from the most luminous galaxies, to the nearest stars, to dark and potentially hazardous asteroids. The survey will be the most detailed to date in infrared light, with a sensitivity hundreds of times better than that of its predecessor, the Infrared Astronomical Satellite.

"Most of the sky has never been imaged at these infrared wavelengths with this kind of sensitivity," said Edward Wright, the mission's principal investigator at UCLA. "We are sure to find many surprises."

On May 17, the mission's science instrument was delivered to Ball Aerospace & Technologies Corp. in Boulder, Colo., where it was attached to the spacecraft, built by Ball. The assembled unit was then blasted by sound to simulate the effects of launch. Tests for electronic "noise" in the detectors will be performed next.

The science instrument is a 40-centimeter (16-inch) telescope with four infrared cameras. A cryostat, or cooler, uses frozen hydrogen to chill the sensitive megapixel infrared detectors down to seven Kelvin (minus 447 degrees Fahrenheit). The instrument was built by Space Dynamics Laboratory in Logan, Utah.

Among expected finds from WISE are hundreds of thousands of asteroids in our solar system's asteroid belt, and hundreds of additional asteroids that come near Earth. Many asteroids have gone undetected because they don't reflect much visible light, but their heat makes them glow in infrared light that WISE can see. By cataloguing the objects, the mission will provide better estimates of their sizes, a critical step for assessing the risk associated with those that might impact Earth.

"We know that asteroids occasionally hit Earth, and we'd like to have a better idea of how many there are and their sizes," said Amy Mainzer of NASA's Jet Propulsion Laboratory, Pasadena, Calif., the mission's deputy project scientist. "Whether they are dark or shiny, they all emit infrared light. They can't hide from WISE."

The mission is also expected to find the coldest stars -- dim orbs called brown dwarfs that are too small to have ignited like our sun. Brown dwarfs are littered throughout our galaxy, but because they are so cool, they are often too faint to see in visible light. The infrared detectors on WISE will pick up the glow of roughly 1,000 brown dwarfs in our galaxy, including those coldest and closest to our solar system. In fact, astronomers say the mission could find a brown dwarf closer to us than the nearest known star, Proxima Centauri, located approximately 4 light-years away.

"We've been learning that brown dwarfs may have planets, so it's possible we'll find the closest planetary systems," said Peter Eisenhardt, the mission's project scientist at JPL. "We should also find many hundreds of brown dwarfs colder than 480 degrees Celsius (900 degrees Fahrenheit), a group that as of now has only nine known members."

In addition, the survey will reveal the universe's most luminous galaxies seen long ago in the dusty throes of their formation, disks of planet-forming material around stars, and other cosmic goodies. The observations will guide other infrared telescopes to the most interesting objects for follow-up studies. For example, NASA's Spitzer Space Telescope, the Herschel observatory just launched by ESA with significant NASA participation, and NASA's upcoming James Webb Space Telescope will direct their gaze at objects uncovered by WISE.

WISE will lift off from Vandenberg aboard a United Launch Alliance Delta II rocket. It will orbit Earth, mapping the entire sky in six months after a one-month checkout period. Its frozen hydrogen is expected to last several months longer, allowing WISE to map much of the sky a second time and see what has changed.

JPL manages the Wide-field Infrared Survey Explorer for NASA's Science Mission Directorate. The mission's principal investigator, Edward Wright, is at UCLA. The mission was developed under NASA's Explorer Program managed by the Goddard Space Flight Center, Greenbelt, Md. The science instrument was built by the Space Dynamics Laboratory and the spacecraft was built by Ball Aerospace & Technologies Corp. Science operations and data processing will take place at the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena. Caltech manages JPL for NASA.

More information is online at http://wise.ssl.berkeley.edu/mission.html .

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This infrared image from NASA's Spitzer Space Telescope shows three baby stars in the bustling center of our Milky Way galaxy.Astronomers have at last uncovered newborn stars at the frenzied center of our Milky Way galaxy. The discovery was made using the infrared vision of NASA's Spitzer Space Telescope.

The heart of our spiral galaxy is cluttered with stars, dust and gas, and at its very center, a supermassive black hole. Conditions there are harsh, with fierce stellar winds, powerful shock waves and other factors that make it difficult for stars to form. Astronomers have known that stars can form in this chaotic place, but they're baffled as to how this occurs. Confounding the problem is all the dust standing between us and the center of our galaxy. Until now, nobody had been able to definitively locate any baby stars.

"These stars are like needles in a haystack," said Solange Ramirez, the principal investigator of the research program at NASA's Exoplanet Science Institute at the California Institute of Technology, Pasadena. "There's no way to find them using optical light, because dust gets in the way. We needed Spitzer's infrared instruments to cut through the dust and narrow in on the objects."

The team plans to look for additional baby stars in the future, and ultimately to piece together what types of conditions allow stars to form in such an inhospitable environment as our galaxy's core.

"By studying individual stars in the galactic center, we can better understand how stars are formed in different interstellar environments," said Deokkeun An of the Infrared Processing and Analysis Center at Caltech, lead author of a paper submitted for publication in the Astrophysical Journal. "The Milky Way galaxy is just one of more than hundreds of billions of galaxies in the visible universe. However, our galaxy is so special because we can take a closer look at its individual stellar components." An started working on this program while a graduate student at Ohio State University, Columbus, under the leadership of Ohio State astronomer Kris Sellgren, the co-investigator on the project.

The core of the Milky Way is a mysterious place about 600 light-years across (light would take 600 years to travel from one end to the other). While this is just a fraction of the size of the entire Milky Way, which is about 100,000 light-years across, the core is stuffed with 10 percent of all the gas in the galaxy -- and loads and loads of stars.

Before now, there were only a few clues that stars can form in the galaxy's core. Astronomers had found clusters of massive adolescent stars, in addition to clouds of charged gas -- a sign that new stars are beginning to ignite and ionize surrounding gas. Past attempts had been unsuccessful in finding newborn stars, or as astronomers call them, young stellar objects.

Ramirez and colleagues began their search by scanning large Spitzer mosaics of our galactic center. They narrowed in on more than 100 candidates, but needed more detailed data to confirm the stars' identities. Young stellar objects, when viewed from far away, can look a lot like much older stars. Both types of stars are very dusty, and the dust lying between us and them obscures the view even further.

To sort through the confusion, the astronomers looked at their candidate stars with Spitzer's spectrograph – an instrument that breaks light apart to reveal its rainbow-like array of infrared colors. Molecules around stars leave imprints in their light, which the spectrograph can detect.

The results revealed three stars with clear signs of youth, for example, certain warm, dense gases. These youthful features are found in other places in the galaxy where stars are being formed.
These data from NASA's Spitzer Space Telescope reveal a newborn star at the center of our Milky Way."It is amazing to me that we have found these stars," said Ramirez. "The galactic center is a very interesting place. It has young stars, old stars, black holes, everything. We started mining a catalog of about 1 million sources and managed to find three young stars -- stars that will help reveal the secrets at the core of the Milky Way."

The young stellar objects are all less than about 1 million years old. They are embedded in cocoons of gas and dust, which will eventually flatten to disks that, according to theory, later lump together to form planets.

Other collaborators include Richard Arendt of NASA's Goddard Space Flight Center, Greenbelt, Md.; A. C. Adwin Boogert of NASA's Herschel Science Center, Caltech in Pasadena; Mathias Schultheis of the Besancon Observatory in France; Susan Stolovy of NASA's Spitzer Science Center, Caltech in Pasadena; Angela Cotera of SETI Institute, Mountain View, Calif.; and Thomas Robitaille and Howard Smith of Harvard Smithsonian Center for Astrophysics, Cambridge, Mass.

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 Caltech in Pasadena. Caltech manages JPL for NASA. For more information about Spitzer, visit http://www.spitzer.caltech.edu/spitzer and http://www.nasa.gov/spitzer .

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