NASA Spacecraft Burns for Home, Then Comet

Artist's concept of Epoxi spacecraft
Artist's concept of Epoxi spacecraft. › Full image and caption

NASA's Deep Impact/Epoxi spacecraft has successfully performed a trajectory correction maneuver to refine its orbit prior to an upcoming Earth flyby June 27. The maneuver, along with the Earth flyby, will place the spacecraft on a trajectory to fly past comet Hartley 2 on Nov. 4.

The maneuver began at 2 p.m. EST (11 a.m. PST) today, when the spacecraft fired its engines for 11.3 seconds. While the burn changed the spacecraft's velocity by only 0.1 meters per second (less than a quarter mile per hour), that was all the mission's navigators requested to set the stage for an Earth gravity assist on June 27.

"While it was a small burn, it was a big step in getting us to Hartley 2," said Tim Larson, project manager of NASA's Epoxi mission. "Humanity's fifth close-up view of a comet is less than five months away."

Epoxi is an extended mission of the Deep Impact spacecraft. Its name is derived from its two tasked science investigations -- the Deep Impact Extended Investigation (DIXI) and the Extrasolar Planet Observation and Characterization (EPOCh).

The University of Maryland is the Principal Investigator institution. JPL manages Epoxi for NASA's Science Mission Directorate, Washington. The spacecraft was built for NASA by Ball Aerospace & Technologies Corp., Boulder, Colo.

For information about Epoxi, visit http://www.nasa.gov/epoxi.

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X-51A Makes Longest Scramjet Flight

X-51A, artist's conceptAn engine first validated in a NASA wind tunnel successfully made the longest supersonic combustion ramjet-powered hypersonic flight to date off the southern California coast on May 26.
The air-breathing scramjet engine, built by Pratt & Whitney Rocketdyne, burned for more than 200 seconds to accelerate the U.S. Air Force's X-51A vehicle to Mach 5, or five times the speed of sound. It broke the previous record for the longest scramjet burn in a flight test, set by NASA's X-43 vehicle.

"This is great news for the hypersonics community," said Jim Pittman, principal investigator for the Hypersonics Project of NASA's Fundamental Aeronautics Program. "It's also good for NASA's research into flight at Mach 5 or faster. We will receive the X-51 flight data for analysis and comparison to the data we obtained during ground tests at NASA Langley's 8-Foot High Temperature Tunnel and to predictions from our propulsion codes."

Air Force officials called the test -- the first of four planned -- an unqualified success. The flight is considered the first use of a practical hydrocarbon-fueled scramjet in flight.

"We are ecstatic to have accomplished most of our test points on the X-51A's very first hypersonic mission," said program manager Charlie Brink of the Air Force Research Laboratory at Wright-Patterson Air Force Base in Dayton, Ohio. "We equate this leap in engine technology as equivalent to the post-World War II jump from propeller-driven aircraft to jet engines."

The X-51A launched from Edwards Air Force Base in California, carried aloft under the left wing of an Air Force Flight Test Center B-52 Stratofortress. It was released while the B-52 flew at 50,000 feet over the Pacific Ocean Point Mugu Naval Air Warfare Center Sea Range. After release, an Army Tactical Missile solid rocket booster accelerated the X-51A to about Mach 4.8 before it and a connecting interstage were jettisoned. The launch and separation were normal, according to Brink.

The SJX61-2 engine that powered the X-51A test vehicle successfully completed ground tests simulating Mach 5 flight conditions at NASA's Langley Research Center, Hampton, Va., in 2008Once the X-51A was free of its booster and interstage, its SJY61 engine ignited, initially on a mix of ethylene, similar to lighter fluid, and JP-7 jet fuel then exclusively on JP-7 jet fuel. The flight reached an altitude of about 70,000 feet and a peak speed of Mach 5.

Onboard sensors transmitted data to an airborne U.S. Navy P-3, as well was ground systems at Point Mugu, Vandenberg and Edwards Air Force bases in California. The flight was terminated after about 200 seconds of engine operation because of a technical issue. The X-51A was not designed to be recovered for examination, so engineers are busily examining the data to identify the cause of the problem.

Four X-51A cruisers have been built for the Air Force and the Defense Advanced Research Projects Agency by industry partners Pratt & Whitney Rocketdyne, West Palm Beach, Fla., and The Boeing Company, Palmdale, Calif. Brink said the Air Force intends to fly the three remaining X-51A flight test vehicles this fall on virtually identical flight profiles, building knowledge from each successive flight.

"This first flight was the culmination of a six-year effort by a small, but very talented AFRL, DARPA, NASA and industry development team," Brink said. "Now we will go back and really scrutinize our data. No test is perfect, and I'm sure we will find anomalies that we will need to address before the next flight. But anyone will tell you that we learn just as much, if not more, when we encounter a glitch."

The engine can produce between 400 and 1,000 pounds of thrust. Like a conventional jet engine, the SJY61 is capable of adjusting thrust throughout the X-51's flight envelope.

Hypersonic flight presents unique technical challenges with heat and pressure, which make conventional turbine engines impractical. Program officials said producing thrust with a scramjet has been compared to lighting a match in a hurricane and keeping it burning.

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AVIRIS

AVIRIS flew over the Gulf oil spill in a NASA ER-2 aircraft from NASA’s Dryden Flight Research Center, Edwards, Calif.

NASA Sensor Completes Initial Gulf Oil Spill Flights

AVIRIS airborne measurement
AVIRIS airborne measurement acquired May 17, 2010, over the site of the Deepwater Horizon BP oil rig disaster. The oil appears orange to brown.
› Full image and caption
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NASA's Airborne Visible/Infrared Imaging Spectrometer (AVIRIS) instrument collected an image over the site of the Deepwater Horizon BP oil rig disaster on May 17, 2010. Crude oil on the surface appears orange to brown. Scientists are using spectroscopic methods to analyze measurements for each point in images like this one to detail the characteristics of the oil on the surface.

AVIRIS extensively mapped the region affected by the spill during 11 flights conducted between May 6 and May 25, 2010, at the request of the National Oceanic and Atmospheric Administration. In total, AVIRIS measured more than 100,000 square kilometers (38,610 square miles) in support of the national oil spill response. The instrument flew at altitudes of up to 19,800 meters (65,000 feet) aboard a NASA ER-2 aircraft from NASA's Dryden Flight Research Center, Edwards, Calif.

AVIRIS is using imaging spectroscopy to map the occurrence and condition of oil on the surface of the Gulf, and to estimate the amount of oil on the surface to help scientists and responding agencies better understand the spill and how to address its effects. In addition, coastline maps created from the AVIRIS overflights will be used to provide a baseline of ecosystems and habitats that can be compared with data from future AVIRIS flights to assess the oil spill's impacts.

Figure 1 depicts AVIRIS imaging spectrometer measurements along the Gulf coast to measure the characteristics and condition of the ecosystem and habitat prior to possible oil contamination and impact. The location is near Johnson's Bayou and along the Gulf Beach Highway, between Port Arthur, La., to the west and Cameron, La., to the east. The west corner of the image includes part of the Texas Point National Wildlife Refuge. The 224 wavelengths of light measured by AVIRIS from visible to infrared are depicted in the top and left panels. The spectrum measured for each point in the image will be used to help assess the characteristics and conditions of the coastal ecosystems and habitats.

AVIRIS data provide scientists with many different types of information about the spill. Researchers at the U.S. Geological Survey's Spectroscopy Laboratory in Golden, Colo., are working to determine the characteristics of the oil based upon the AVIRIS measured spectral signature. As shown in Figure 2, acquired May 17, 2010, the signature of the oil measured in the infrared portion of the spectrum allows scientists to measure the occurrence and condition of oil and estimate the thickness of oil on the water's surface, Figure 3 depicts AVIRIS oil spill flight line measurements acquired on May 17, 2010, superimposed on a background regional image.

For more information on AVIRIS, visit http://aviris.jpl.nasa.gov/.

To read more and see related images, visit: http://photojournal.jpl.nasa.gov/catalog/?IDNumber=pia13167

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Small Near-Earth Object Probably a Rocket Part

Graphic depicting the trajectory of near-Earth object 2010 KQ
Graphic depicting the trajectory of near-Earth object 2010 KQ.
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Scientists at NASA's Near-Earth Object Program Office at NASA's Jet Propulsion Laboratory in Pasadena, Calif., have determined that a small object that safely passed Earth on May 21 is more than likely an upper-stage of a rocket that carried a spacecraft on an interplanetary trajectory.

"The orbit of this object is very similar to that of the Earth, and one would not expect an object to remain in this type of orbit for very long," said Paul Chodas, a scientist at NASA's Near-Earth Object Program Office at the Jet Propulsion Laboratory in Pasadena, Calif.

Observations by astronomer S.J. Bus, using the NASA-sponsored Infrared Telescope Facility in Mauna Kea, Hawaii, indicate that 2010 KQ's spectral characteristics do not match any of the known asteroid types, and the object's absolute magnitude (28.9) suggests it is only a few meters in size.

2010 KQ was discovered by astronomer Richard Kowalski at the NASA-sponsored Catalina Sky Survey in the mountains just north of Tucson, Ariz., on May 16. Five days later, it made its closest approach to Earth at a distance just beyond the moon's orbit. The object is departing Earth's neighborhood but will be returning in 2036.

"At present, there is a 6 percent probability that 2010 KQ will enter our atmosphere over a 30-year period starting in 2036," said Chodas. "More than likely, additional observations of the object will refine its orbit and impact possibilities. Even in the unlikely event that this object is headed for impact with Earth, whether it is an asteroid or rocket body, it is so small that it would disintegrate in the atmosphere and not cause harm on the ground."

NASA detects, tracks and characterizes asteroids and comets passing close to Earth using both ground- and space-based telescopes. The Near-Earth Object Observations Program, commonly called "Spaceguard," discovers these objects, characterizes a subset of them, and plots their orbits to determine if any could be potentially hazardous to our planet.

JPL manages the Near-Earth Object Program Office for NASA's Science Mission Directorate in Washington. JPL is a division of the California Institute of Technology in Pasadena.

More information about asteroids and near-Earth objects is at: http://www.jpl.nasa.gov/asteroidwatch.

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NASA Takes to the Air With New 'Earth Venture' Research Projects

JPL's Carbon in Arctic Reservoirs Vulnerability Experiment
JPL's Carbon in Arctic Reservoirs Vulnerability Experiment will bridge critical gaps in our knowledge and understanding of Arctic ecosystems, links between the Arctic water and terrestrial carbon cycles, and the effects of fires and thawing permafrost. › Larger view
Hurricanes, air quality and Arctic ecosystems are among the research areas to be investigated during the next five years by new NASA airborne science missions announced today.

The five competitively-selected proposals, including one from NASA's Jet Propulsion Laboratory, Pasadena, Calif., are the first investigations in the new Venture-class series of low-to-moderate-cost projects established last year.

The Earth Venture missions are part of NASA's Earth System Science Pathfinder program. The small, targeted science investigations complement NASA's larger research missions. In 2007, the National Research Council recommended that NASA undertake these types of regularly solicited, quick-turnaround projects.

This year's selections are all airborne investigations. Future Venture proposals may include small, dedicated spacecraft and instruments flown on other spacecraft.

"I'm thrilled to be able to welcome these new principal investigators into NASA's Earth Venture series," said Edward Weiler, associate administrator of the agency's Science Mission Directorate in Washington. "These missions are considered a 'tier 1' priority in the National Research Council's Earth Science decadal survey. With this selection, NASA moves ahead into this exciting type of scientific endeavor."

The missions will be funded during the next five years at a total cost of not more than $30 million each. The cost includes initial development and deployment through analysis of data. Approximately $10 million was provided through the American Recovery and Reinvestment Act toward the maximum $150 million funding ceiling for the missions.

Six NASA centers, 22 educational institutions, nine U.S. or international government agencies and three industrial partners are involved in these missions. The five missions were selected from 35 proposals.

The selected missions are:

1. Carbon in Arctic Reservoirs Vulnerability Experiment. Principal Investigator Charles Miller, NASA's Jet Propulsion Laboratory in Pasadena, Calif.

The release and absorption of carbon from Arctic ecosystems and its response to climate change are not well known because of a lack of detailed measurements. This investigation will collect an integrated set of data that will provide unprecedented experimental insights into Arctic carbon cycling, especially the release of important greenhouse gases such as carbon dioxide and methane. Instruments will be flown on a Twin Otter aircraft to produce the first simultaneous measurements of surface characteristics that control carbon emissions and key atmospheric gases.

2. Airborne Microwave Observatory of Subcanopy and Subsurface. Principal Investigator Mahta Moghaddam, University of Michigan

North American ecosystems are critical components of the global exchange of the greenhouse gas carbon dioxide and other gases within the atmosphere. To better understand the size of this exchange on a continental scale, this investigation addresses the uncertainties in existing estimates by measuring soil moisture in the root zone of representative regions of major North American ecosystems. Investigators will use NASA's Gulfstream-III aircraft to fly synthetic aperture radar that can penetrate vegetation and soil to depths of several feet.

3. Airborne Tropical Tropopause Experiment. Principal Investigator Eric Jensen, NASA's Ames Research Center in Moffett Field, Calif.

Water vapor in the stratosphere has a large impact on Earth's climate, the ozone layer and how much solar energy Earth retains. To improve our understanding of the processes that control the flow of atmospheric gases into this region, investigators will launch four airborne campaigns with NASA's Global Hawk remotely piloted aerial systems. The flights will study chemical and physical processes at different times of year from bases in California, Guam, Hawaii and Australia.

4. Deriving Information on Surface Conditions from Column and Vertically Resolved Observations Relevant to Air Quality. Principal Investigator James Crawford, NASA's Langley Research Center in Hampton, Va.

Satellites can measure air quality factors like aerosols and ozone-producing gases in an entire column of atmosphere below the spacecraft, but distinguishing the concentrations at the level where people live is a challenge. This investigation will provide integrated data of airborne, surface and satellite observations, taken at the same time, to study air quality as it evolves throughout the day. NASA's B-200 and P-3B research aircraft will fly together to sample a column of the atmosphere over instrumented ground stations.

5. Hurricane and Severe Storm Sentinel. Principal Investigator Scott Braun, NASA's Goddard Space Flight Center in Greenbelt, Md.

The prediction of the intensity of hurricanes is not as reliable as predictions of the location of hurricane landfall, in large part because of our poor understanding of the processes involved in intensity change. This investigation focuses on studying hurricanes in the Atlantic Ocean basin using two NASA Global Hawks flying high above the storms for up to 30 hours. The Hawks will deploy from NASA's Wallops Flight Facility in Virginia during the 2012 to 2014 Atlantic hurricane seasons.

"These new investigations, in concert with NASA's Earth-observing satellite capabilities, will provide unique new data sets that identify and characterize important phenomena, detect changes in the Earth system and lead to improvements in computer modeling of the Earth system," said Jack Kaye, associate director for research of NASA's Earth Science Division in the Science Mission Directorate.

Langley manages the Earth System Pathfinder program for the Science Mission Directorate. The missions in this program provide an innovative approach to address Earth science research with periodic windows of opportunity to accommodate new scientific priorities.

For information about NASA and agency programs, visit: http://www.nasa.gov .

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Spinoffs Reveal Earth Benefits of NASA Technologies

Congressional staffers in the Rayburn House Office Building on May 20 were wondering why a robot was roaming the halls. Those who followed the robot were led to further surprises: an igloo-shaped life raft, long socks full of fine powder, an inflatable antenna shaped like an enormous beach ball -- all NASA technologies that, through commercial partnerships between NASA and industry, are improving life on Earth.

The second annual Spinoff Day on the Hill, hosted by Representative Suzanne Kosmas of Florida, featured seven companies who have partnered with NASA to bring innovations to market that are saving lives, protecting the environment, and enriching how we experience our planet.

The 1958 Space Act that created NASA mandated that the Agency transfer as much of its technology as possible for the benefit of the public. To date, NASA has documented more than 1662 of these technologies, called spinoffs, in its annual Spinoff publication (http://spinoff.nasa.gov), launched in 1976.

"We invest in technologies for what they will bring to NASA in terms of future missions of science and of exploration, but we can never forget that we also invest in these things because of what they do for us right here on Earth," said NASA chief technologist Bobby Braun, who presented remarks at the event.

The products on show at Spinoff Day on the Hill all trace their origins back to space. The igloo-shaped life raft? Engineers at Johnson Space Center originally developed the self-righting raft design to prevent life rafts holding astronauts from capsizing from the downdraft of helicopters after Apollo-era splashdown landings. Now manufactured by Givens Marine Survival Co. Inc. of Tiverton, Rhode Island, the raft is credited with saving the lives of over 450 sailors.

Unirem Inc., managed by Summit International/Rasstech Industries, of Houston, exhibited its Petroleum Remediation Product, or PRP, developed through the collaboration of industry scientists and NASA researchers. The powder technology, which absorbs and captures oil as it floats on the water's surface, may soon play a role in the cleanup of the catastrophic oil spill currently endangering the nation's Gulf coast.

GATR Technologies of Huntsville, Alabama, displayed one of its inflatable antennas, developed under NASA's Small Business Innovation Research program. Quickly deployable from two suitcase-size containers, GATR's antennas enabled communications during wild fires in southern California, after Hurricane Katrina, and following the earthquake in Haiti.

Airocide, a unique air purifier that helps preserve perishable foods and destroys airborne pathogens, was presented by KES Science and Technology Inc. of Kennesaw, Georgia, and Akida Holdings of Jacksonville, Florida. Originally developed by NASA-funded researchers to help preserve plants grown in space, the technology is improving food storage and distribution in remote regions of the world, as well as helping sanitize operating rooms and doctors' offices.

Also on display was Menlo Park, California-based Allocade Inc.'s OnCue scheduling software. The technology was invented by a former Ames Research Center computer scientist who helped design scheduling software for the Hubble Space Telescope. OnCue now helps hospitals operate more efficiently by optimizing constantly changing schedules for imaging procedures.

Gigapan photographic technology, derived from the panoramic camera mast assemblies on the Mars Exploration Rovers, awed attendees with its ultra-high resolution imagery, while the Webby Award-winning NASA@Home and City interactive Web site (http://www.nasa.gov/city) shared information about spinoff technologies that can be found in homes and hometowns across the Nation.

Braun noted the economic impact NASA’s technological advancements can create, leading to "more Earth-based spinoffs, more technology-oriented jobs, and more business and industries that can compete in the global marketplace." He also highlighted the inspiration such innovation provides to students exploring education and careers in science, technology, engineering, and mathematics.

"What we have here are just a few outstanding examples, but there are so many others to learn about," said Doug Comstock, director of NASA's Innovative Partnerships Program. "The fabric of our everyday lives benefits from these space technologies."

One such example zipped along the halls of the Rayburn building even as Spinoff Day on the Hill came to an end. The Multi-function Agile Remote Control Robot, or MARCbot, was enhanced by NASA engineers and is now manufactured by Applied Geo Technologies Inc. of Choctaw, Mississippi. More than 300 of the robots are now in service overseas, keeping soldiers safer by helping identify possible explosive devices.

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NASA Satellite Spots Oil at Mississippi Delta Mouth

A new image from NASA's Terra spacecraft
Oil from the Deepwater Horizon spill laps around the mouth of the Mississippi River delta in this May 24, 2010, image from the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) instrument on NASA's Terra spacecraft. The oil appears silver, while vegetation is red. › Full image and caption
On May 24, 2010, the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) instrument on NASA's Terra spacecraft captured this false-color, high-resolution view of the very tip of the Mississippi River delta. Ribbons and patches of oil that have leaked from the Deepwater Horizon well offshore appear silver against the light blue color of the adjacent water. Vegetation is red.

In the sunglint region of a satellite image--where the mirror-like reflection of the sun gets blurred into a wide, bright strip--any differences in the texture of the water surface are enhanced. Oil smoothes the water, making it a better "mirror." Oil-covered waters are very bright in this image, but, depending on the viewing conditions (time of day, satellite viewing angle, slick location), oil-covered water may look darker rather than brighter.

The relative brightness of the oil from place to place is not necessarily an indication of the amount of oil present. Any oil located near the precise spot where the sun's reflection would appear, if the surface of the Gulf were perfectly smooth and calm, is going to look very bright in these images. The cause of the dark patch of water in the upper left quadrant of the image is unknown. It may indicate the use of chemical dispersants, skimmers or booms, or it may be the result of natural differences in turbidity, salinity or organic matter in the coastal waters.

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Astronomers Discover New Star-Forming Regions in Milky Way

An artist's conception of our Milky Way galaxy
An artist's conception of our Milky Way galaxy.
› Larger view
Astronomers studying the Milky Way have discovered a large number of previously unknown regions where massive stars are being formed. Their discovery, made with the help of NASA's Spitzer Space Telescope, provides important new information about the structure of our home galaxy and promises to yield new clues about its composition.

The star-forming regions the astronomers sought, called H II regions, are sites where hydrogen atoms are stripped of their electrons by intense radiation from massive, young stars. To find these regions, hidden from visible-light detection by the Milky Way's gas and dust, the researchers used infrared and radio telescopes.

"We found our targets by using the results of infrared surveys done with NASA's Spitzer Space Telescope and of surveys done with the National Science Foundation's Very Large Array radio telescope," said astronomer Loren Anderson of the Astrophysical Laboratory of Marseille in France, who worked on the project. "Objects that appear bright in both the Spitzer and Very Large Array images we studied are good candidates for H II regions."

Further analysis allowed the astronomers to determine the locations of the H II regions. They found concentrations of the regions at the end of the galaxy's central bar and in its spiral arms. Their analysis also showed that 25 of the regions are farther from the galaxy's center than the sun.

Read more at http://www.nrao.edu/pr/2010/gbthiiregions/ .

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NASA Orbiter Penetrates Mysteries of Martian Ice Cap

Northern Ice Cap of Mars
This image, combining data from two instruments aboard NASA's Mars Global Surveyor, depicts an orbital view of the north polar region of Mars. › Full image and caption
Data from NASA's Mars Reconnaissance Orbiter have helped scientists solve a pair of mysteries dating back four decades and provided new information about climate change on the Red Planet.

The Shallow Radar, or SHARAD, instrument aboard the Mars Reconnaissance Orbiter revealed subsurface geology allowing scientists to reconstruct the formation of a large chasm and a series of spiral troughs on the northern ice cap of Mars. The findings appear in two papers in the May 27 issue of the journal Nature.

"SHARAD is giving us a beautifully detailed view of ice deposits, whether at the poles or buried in mid-latitudes, as they changed on Mars over the last few million years," said Rich Zurek, Mars Reconnaissance Orbiter project scientist at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

On Earth, large ice sheets are shaped mainly by ice flow. According to this latest research, other forces have shaped, and continue to shape, polar ice caps on Mars. The northern ice cap is a stack of ice and dust layers up to two miles deep, covering an area slightly larger than Texas. Analyzing radar data on a computer, scientists can peel back the layers like an onion to reveal how the ice cap evolved over time.

One of the most distinctive features of the northern ice cap is Chasma Boreale, a canyon about as long as Earth's Grand Canyon but deeper and wider. Some scientists believe Chasma Boreale was created when volcanic heat melted the bottom of the ice sheet and triggered a catastrophic flood. Others suggest strong polar winds carved the canyon out of a dome of ice.

Other enigmatic features of the ice cap are troughs that spiral outward from the center like a gigantic pinwheel. Since the troughs were discovered in 1972, scientists have proposed several hypotheses about how they formed. Perhaps as Mars spins, ice closer to the poles moves slower than ice farther away, causing the semi-fluid ice to crack. Perhaps, as one mathematical model suggests, increased solar heating in certain areas and lateral heat conduction could cause the troughs to assemble.

Data from Mars now points to both the canyon and spiral troughs being created and shaped primarily by wind. Rather than being cut into existing ice very recently, the features formed over millions of years as the ice sheet grew. By influencing wind patterns, the shape of underlying, older ice controlled where and how the features grew.

"Nobody realized that there would be such complex structures in the layers," said Jack Holt, of the University of Texas at Austin's Institute for Geophysics. Holt is the lead author of the paper focusing on Chasma Boreale. "The layers record a history of ice accumulation, erosion and wind transport. From that, we can recover a history of climate that's much more detailed than anybody expected."

The Mars Reconnaissance Orbiter was launched on Aug. 12, 2005. SHARAD and the spacecraft's five other instruments began science operations in November 2006.

"These anomalous features have gone unexplained for 40 years because we have not been able to see what lies beneath the surface," said Roberto Seu, Shallow Radar team leader at the University of Rome. "It is gratifying to me that with this new instrument we can finally explain them."

The MRO mission is managed by JPL for the Mars Exploration Program at NASA's Headquarters in Washington. The Shallow Radar instrument was provided by the Italian Space Agency, and its operations are led by the InfoCom Department, University of Rome. JPL is managed for NASA by the California Institute of Technology in Pasadena, Calif.

To view images and learn more about MRO, visit: http://www.nasa.gov/mro .

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NASAs Swift Survey Finds 'Smoking Gun' Of Black Hole Activation

The optical counterparts of many active galactic nuclei (circled) detected by the Swift BAT Hard X-ray Survey clearly show galaxies in the process of mergingData from an ongoing survey by NASA's Swift satellite have helped astronomers solve a decades-long mystery about why a small percentage of black holes emit vast amounts of energy.

Only about one percent of supermassive black holes exhibit this behavior. The new findings confirm that black holes "light up" when galaxies collide, and the data may offer insight into the future behavior of the black hole in our own Milky Way galaxy. The study will appear in the June 20 issue of The Astrophysical Journal Letters.

The intense emission from galaxy centers, or nuclei, arises near a supermassive black hole containing between a million and a billion times the sun's mass. Giving off as much as 10 billion times the sun's energy, some of these active galactic nuclei (AGN) are the most luminous objects in the universe. They include quasars and blazars.

"Theorists have shown that the violence in galaxy mergers can feed a galaxy's central black hole," said Michael Koss, the study's lead author and a graduate student at the University of Maryland in College Park. "The study elegantly explains how the black holes switched on."

Until Swift's hard X-ray survey, astronomers never could be sure they had counted the majority of the AGN. Thick clouds of dust and gas surround the black hole in an active galaxy, which can block ultraviolet, optical and low-energy, or soft X-ray, light. Infrared radiation from warm dust near the black hole can pass through the material, but it can be confused with emissions from the galaxy's star-forming regions. Hard X-rays can help scientists directly detect the energetic black hole.

Since 2004, the Burst Alert Telescope (BAT) aboard Swift has been mapping the sky using hard X-rays.

"Building up its exposure year after year, the Swift BAT Hard X-ray Survey is the largest, most sensitive and complete census of the sky at these energies," said Neil Gehrels, Swift's principal investigator at NASA's Goddard Space Flight Center in Greenbelt, Md.

The survey, which is sensitive to AGN as far as 650 million light-years away, uncovered dozens of previously unrecognized systems.

"The Swift BAT survey is giving us a very different picture of AGN," Koss said. The team finds that about a quarter of the BAT galaxies are in mergers or close pairs. "Perhaps 60 percent of these galaxies will completely merge in the next billion years. We think we have the 'smoking gun' for merger-triggered AGN that theorists have predicted."

Other members of the study team include Richard Mushotzky and Sylvain Veilleux at the University of Maryland and Lisa Winter at the Center for Astrophysics and Space Astronomy at the University of Colorado in Boulder.

"We've never seen the onset of AGN activity so clearly," said Joel Bregman, an astronomer at the University Michigan, Ann Arbor, who was not involved in the study. "The Swift team must be identifying an early stage of the process with the Hard X-ray Survey."

Swift, launched in November 2004, is managed by Goddard. It was built and is being operated in collaboration with Penn State, the Los Alamos National Laboratory in New Mexico, and General Dynamics in Falls Church, Va.; the University of Leicester and Mullard Space Sciences Laboratory in the United Kingdom; Brera Observatory and the Italian Space Agency in Italy; plus additional partners in Germany and Japan.

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NASA's Webb Telescope Has 'Made It' to New York City!

The Webb telescope full scale model lit up at night in Munich, Germany in 2009The James Webb Space Telescope has finally made the "big time" at least according to the old Frank Sinatra song "New York, New York." The life-sized model of NASA's next generation space telescope is being set up in New York City's Battery Park for the 2010 World Science Festival, which runs June 1- June 6. The opening ceremony will be held in front of the model on June 1.

As the song goes, "if (the Webb telescope) can make it there, it'll make it anywhere" and scientists are hoping that it will safely arrive in its orbit one million miles from Earth.

"The World Science Festival is a great opportunity for people to get a look at, and learn more about, the future of astronomy from space," said Eric Smith, NASA's Webb Program Scientist. "The Webb telescope full scale model dramatically highlights how far the next generation of space telescopes will be from its predecessors. It’s unlike any telescope you’ve ever seen."

The James Webb Space Telescope is the next-generation premier space observatory, exploring deep space phenomena from distant galaxies to nearby planets and stars. The telescope will give scientists clues about the formation of the universe and the evolution of our own solar system, from the first light after the Big Bang to the formation of star systems capable of supporting life on planets like Earth.

For six days in June, New York City residents can get a free look at the full-scale model of the Webb telescope as it sits on display in Battery Park. The model viewing hours run from Tuesday, June 1 from 9:00 a.m. to Sunday, June 6 at 9:00 p.m. EDT. The actual size model is highly detailed. It is constructed mainly of aluminum and steel, weighs 12,000 pounds, is approximately 80 feet long, 40 feet wide and 40 feet tall. It is as large as a tennis court. The model requires 2 trucks to ship it and assembly takes a crew of 12 approximately four days. The model will be lit up from its base so that night-time viewers can take in all the details.

The full-scale model of the James Webb Space Telescope was built by the prime contractor, Northrop Grumman, to provide a better understanding of the size, scale and complexity of this satellite.

Visitors will also be able to learn about what the Webb telescope is going to show scientists. They can play with interactive exhibits, watch videos about what the Webb will be exploring in the cosmos, and even ask a scientist about the telescope.

On Friday June 4, from 8-9:30 p.m. EDT, there will be a special event at the base of the full-sized model, called "From the City to the Stars," where scientists will talk about the possible discoveries that the Webb telescope could make.

The event is also free and open to the public. Dr. John Mather, Nobel laureate and the Webb telescope’s senior project scientist; Dr. John Grunsfeld, astronaut, physicist and "chief repairman" of the Hubble Telescope and planetary astronomer Dr. Heidi Hammel will be at the event to talk about the discoveries anticipated from the Webb telescope. NASA Deputy Administrator Lori Garver will be a featured speaker at the Festival kick-off. She will share with the New York audience NASA’s strong commitment to continued scientific discovery, with missions like the Webb telescope, and talk about some of the other exciting endeavors on NASA’s new path forward.

Since 2005, the model has journeyed to Florida, Germany, Ireland and Washington, D.C. The actual Webb space telescope is going a lot further, about a million miles from Earth!

Related Links:

> "From the City to the Stars"
> World Science Festival
> James Webb Space Telescope
> Model on display in Washington, DC - May 10-12, 2007

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Why NASA Keeps a Close Eye on the Sun's Irradiance

Sunspots are darker areas of the Sun that have lower solar irradiance than other areasFor more than two centuries, scientists have wondered how much heat and light the sun expels, and whether this energy varies enough to change Earth’s climate. In the absence of a good method for measuring the sun's output, the scientific conversation was often heavy with speculation.

By 1976, that began to change when Jack Eddy, a solar astronomer from Boulder, Colo., examined historical records of sunspots and published a seminal paper that showed some century-long variations in solar activity are connected with major climatic shifts. Eddy helped show that an extended lull in solar activity during the 17th Century --called the Maunder Minimum -- was likely connected to a decades-long cold period on Earth called the "Little Ice Age."

Two years after Eddy published his paper, NASA launched the first in a series of satellite instruments called radiometers, which measure the amount of sunlight striking the top of Earth's atmosphere, or total solar irradiance. Radiometers have provided unparalleled details about how the sun's irradiance has varied in the decades since. Such measurements have helped validate and expand upon Eddy's findings. And they've led to a number of other discoveries—and questions—about the sun.

Without radiometers, scientists would probably still wonder how much energy the sun emits and whether it varies with the sunspot cycle. They wouldn't know of the competition between dark sunspots and bright spots called faculae that drives irradiance variations.

And they’d have little chance of answering a question that continues to perplex solar experts today: Has overall irradiance changed progressively throughout the past three 11-year cycles, or are variations in the sun's irradiance limited to a single cycle?

The answer has important implications for understanding climate change, as some scientists have suggested that trends in solar irradiance account for a significant portion of global warming.

The next space radiometer, slated for launch this November aboard NASA's Glory satellite, should help chip away at the uncertainty that surrounding the sun's role in climate change.

A Variable Sun It's well known today that the sun's irradiance fluctuates constantly in conjunction with sunspots, which become more and less abundant every 11 years due to turbulent magnetic fields that course through the sun's interior and erupt onto its surface.

But as recently as the 1970s, scientists assumed that the sun’s irradiance was unchanging; the amount of energy it expels was even called the "solar constant."

It was data from radiometers aboard Nimbus 7, launched in 1978, and the Solar Maximum Mission, launched two years later, that were the death knell to the solar constant. Soon after launching, instruments aboard both satellites showed that solar irradiance changed significantly as patches of sunspots rotated around the sun's surface. Irradiance would fall, for example, when groups of sunspots faced Earth. And it would recover when the sunspots rotated to the far side of the sun.
Like sunspots, solar prominences are more likely to occur during the most active part of the solar cycle
Likewise, in 2003, a radiometer aboard NASA's Solar Radiation and Climate Experiment (SORCE) satellite observed large sunspot patches that caused irradiance to drop by as much 0.34 percent, the largest short-term decrease ever recorded.

"When you look at longer scales on the sun, it's the opposite," said Lean, a solar scientist at the U.S. Naval Research Laboratory in Washington, D.C., and a member of Glory's science team. "Overall, irradiance actually increases when the sun is more active even though sunspots are more common."

How can increases in dark, cool sunspots yield increases in irradiance? "It didn't make much sense until we were able to show that sunspots are just half of the story," said Lean.

Measurements collected during the 1980s and 1990s gave scientists the evidence they needed to prove that irradiance is actually a balance between darkening from sunspots and brightening from accompanying hot regions called faculae, a word meaning "bright torch" in Latin.

When solar activity increases, as it does every 11 years or so, both sunspots and faculae become more numerous. But during the peak of a cycle, the faculae brighten the sun more than sunspots dim it.

Overall, radiometers show that the sun’s irradiance changes by about 0.1 percent as the number of sunspots varies from about 20 sunspots or less per year during periods of low activity (solar minimum) to between 100 and 150 during periods of high activity (solar maximum).

“That may seem like a tiny amount, but it’s critical we understand even these small changes if we want to understand whether the sun's output is trending up or down and affecting climate,” said Greg Kopp, a principal investigator for Glory and scientist at the Laboratory for Atmospheric and Space Physics at the University of Colorado in Boulder.

Though most scientists believe the 0.1 percent variation is too subtle to explain all of the recent warming, it's not impossible that long-term patterns -- proceeding over hundreds or thousands of years -- could cause more severe swings that could have profound impacts on climate.
Although sunspots cause a decrease in irradiance they're  accompanied by bright white blotches called faculae that cause an  overall increase in solar irradiance
Searching for a Trend Line A total of 10 radiometers have monitored the sun since Nimbus 7, and by patching all of the measurements together into one data stream, scientists have tried to identify whether the sun’s irradiance has increased or decreased over the last three cycles.

However, melding the results from different instruments has proven complicated because many of the radiometers record slightly different absolute measurements. And the areas of overlap between instruments in the long-term record aren't as robust as scientists would like.

As a result, questions remain about how the sun's irradiance has changed. Richard Willson, principal investigator for NASA's Active Cavity Radiometer Irradiance Monitor (ACRIM), reported in a 2003 paper that the overall brightness of the sun was increasing by 0.05 percent per decade.

Subsequent assessments of the same data have come to a different conclusion. Other groups of scientists have shown that the apparent upward trend is actually an artifact of the radiometers and how they degrade in orbit. Complicating the issue further, an instrument aboard NASA's Solar and Heliospheric Observatory (SOHO) measured irradiance levels during a solar minimum in 2008 that were actually lower than the previous solar minimum.

Which measurements are right? Has the sun experienced subtle brightening or dimming during the last few solar cycles? Such questions remain controversial, but the radiometer aboard Glory, called the Total Irradiance Monitor (TIM), is ready to provide answers. The Glory TIM will be more accurate and stable than previous instruments because of unique optical and electrical advances. And each of its components has undergone a rigorous regime of calibrations at a newly-built facility at the University of Colorado.

“It’s a very exciting time to be studying the sun,” said Lean. “Every day there's something new, and we’re on the verge of answering some very important questions.”

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NASA Satellites Keep Watch on Gulf Current Near Spill

Graph showing the speed and direction of surface currents in the  Gulf
NASA satellite altimetry data are being used in combination with data from other satellites to track changes in a huge warm ocean current in the Gulf of Mexico that could transport oil from the Deepwater Horizon oil rig far away from the Gulf. › Full image and caption


Scientists and agencies monitoring the oil spill in the Gulf of Mexico are keeping a wary eye on changes in the nearby Loop Current, a warm ocean current that is part of the Gulf Stream. Beginning as a large flow of warm water from the Caribbean, the Loop Current heads up into the eastern part of the Gulf of Mexico and then turns south before finally moving out through the Straits of Florida and northward into the Gulf Stream. Deep and fast moving, the Loop Current often breaks off and forms strong, clockwise rotating eddies called anticyclones that travel westward into the Gulf. The currents along the outer edges of the Loop Current, as well as these eddies, have been clocked at speeds as high as three to four knots (three to five miles per hour), comparable to the fastest ocean currents ever observed.

Because the Loop Current and its eddies are warmer, and thus higher in surface elevation, than the surrounding waters, they are easily spotted by satellite altimeters, such as those aboard the NASA/French Space Agency Jason 1 and Ocean Surface Topography Mission/Jason 2 satellites. Scientists use the latest satellite measurements of sea-surface height from these and other satellite altimeters to create maps showing the location, direction and speed of currents in the Gulf of Mexico.

This image, created on May 23, 2010, using measurements of sea surface height from multiple satellites, including Jason-1 and OSTM/Jason-2, shows the speed and direction of surface currents in the Gulf. The northern portion of the Loop Current, shown in red, appears about to detach and form a separate eddy--a large, warm, clockwise-spinning vortex of water that is the ocean's version of a cyclone. The star shows the former location of the Deepwater Horizon drilling rig that exploded and sank in April, and has been leaking oil since. Scientists believe a large eddy between the oil spill and the Loop Current could keep, at least temporarily, some of the spilling oil from reaching the Florida Straits and the Gulf Stream.

This map was produced by the Colorado Center for Astrodynamics Research in Boulder, Colo. The center processes satellite measurements of sea surface height in near real-time to create maps of the Gulf of Mexico, showing the location of medium-sized eddies and fronts. More information on these data products is available at http://argo.colorado.edu/~realtime/welcome/.

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The Glory Mission's Judith Lean Discusses Solar Variability

Judith LeanThough the sun's brightness was once thought to be constant, NASA has launched a series of satellite instruments that have helped show it actually fluctuates in conjunction with cycles of solar activity.

With a new sun-watching instrument called the Total Irradiance Monitor (TIM) scheduled to launch on NASA's Glory satellite in November, we spoke with Judith Lean, a member of the Glory science team and solar physicist at the United States Naval Research Laboratory, about solar cycles and what scientists have learned about solar variability in the last three decades.

What is a solar cycle and how long does it last?
For more than a century, people have noticed that sunspots become more and less frequent on an 11-year-cycle. That’s the main solar cycle we look at. The 11-year-cycle is really part of a 22-year-cycle of the sun’s magnetic field polarity. The changes are driven by something called the solar dynamo, a process that generates and alters the strength of the magnetic field erupting onto the sun's surface. It's the sun’s magnetic field that produces sunspots as it moves up through the sun's surface.

How much does the brightness of the sun change throughout the cycle?
It's a small amount. Total solar irradiance typically increases by about 0.1 percent during periods of high activity. However, certain wavelengths of sunlight—such as ultraviolet—vary more.

What causes irradiance to change?
It's really the balance of sunspots, which are cooler dark areas of the sun, and faculae, bright areas that appear near sunspots. The faculae overwhelm the sunspots, so the sun is actually brighter when there are more sunspots.

Can changes in the sun affect our climate?
If it wasn’t for the sun, we wouldn’t have a climate. The sun provides the energy to drive our climate, and even small changes in the sun's output can have a direct impact on Earth. There are two ways irradiance changes can alter climate: One is the direct effect from altering the amount of radiation reaching Earth. The second is that solar variability can affect ozone production, which can in turn affect the climate.

Does the 0.1 percent change in irradiance affect Earth's climate much?
Solar irradiance changes are likely connected to dynamic aspects of climate—things like the coupling of the atmosphere and ocean—El Niño being one example—or aspects of atmospheric circulation, such as the Hadley cells that dominate in the tropics.
But we've done a great deal of modeling, and the sun doesn't explain the global warming that's occurred over the last century. We think changes in irradiance account for about 10 percent global warming at most. Of course, there are also longer cycles that may have an impact on climate, but our understanding of them is limited.

There is disagreement about whether the last three cycles have gotten successively brighter. Has that been resolved?
No, it hasn't. The best understanding is that irradiance cycles have been about the same in the last three cycles, but one group reports an increasing trend whereas another group says that current levels are now the lowest of the entire 30-year record. I believe these differences are due to instrumental effects, but we really need continual, highly accurate, and stable long-term measurements to resolve this. The radiometer aboard Glory—the Total Irradiance Monitor (TIM)--will be a big step, quite an exciting advance.

What part of the 11-year cycle will Glory observe?
Glory is going is to observe during the ascending phase of the cycle. The ascending phase is relatively rapid, so we should get to the peak in about three years. Then there will be about two years or more when solar activity is high and stays high. About five years from now, activity will start to come down again so that by, say, 2019 we will be at low levels again.

What do you hope Glory will find?
The Glory TIM has been calibrated more rigorously than previous instruments, so it should help a lot in getting the absolute brightness of the sun. In addition to recording the ever-changing irradiance levels, it should measure irradiance precisely enough that will make it feasible to determine whether solar irradiance is stable or changing, if the measurements continue long enough into the future.

Are there aspects of the solar variability that TIM won't measure?
Yes. The Glory TIM looks at overall irradiance, but it doesn't measure how specific parts of the spectrum—the ultraviolet, visible, or infrared—are changing. Some of the largest changes actually happen at the shortest wavelengths, so it's extremely important that we look at the spectrum. There's an instrument related to TIM called the Solar Irradiance Monitor (SIM) aboard the SORCE satellite that lets us see how individual parts of the spectrum vary, and it's also critical.

The sun has been exceptionally quiet in recent years. Are we entering a prolonged solar minimum?
There was a period from mid-2008 to mid-2009 when the sun was without sunspots for many days. It was probably the quietest period we've seen since the first total solar irradiance measurements. But we didn't go into a prolonged minimum because the sun still had a few active regions – not sunspots, but small bright faculae regions -- and we could see the irradiance continue to fluctuate throughout this very quiet period. Now there are more dark sunspots and more bright faculae on the sun’s surface, so activity is ramping up and a new cycle--solar cycle 24--has started.

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Spacecraft Reveals Small Solar Events Have Large Scale Effects

image of the SDO satellite orbiting EarthNASA's Solar Dynamics Observatory, or SDO, has allowed scientists for the first time to comprehensively view the dynamic nature of storms on the sun. Solar storms have been recognized as a cause of technological problems on Earth since the invention of the telegraph in the 19th century.

The Atmospheric Imaging Assembly (AIA), one of three instruments aboard SDO, allowed scientists to discover that even minor solar events are never truly small scale. Shortly after AIA opened its doors on March 30, scientists observed a large eruptive prominence on the sun's edge, followed by a filament eruption a third of the way across the star's disk from the eruption.

"Even small events restructure large regions of the solar surface," said Alan Title, AIA principal investigator at Lockheed Martin Advanced Technology Center in Palo Alto, Calif. "It's been possible to recognize the size of these regions because of the combination of spatial, temporal and area coverage provided by AIA."

The AIA instrument also has observed a number of very small flares that have generated magnetic instabilities and waves with clearly-observed effects over a substantial fraction of the solar surface. The instrument is capturing full-disk images in eight different temperature bands that span 10,000 to 36-million degrees Fahrenheit. This allows scientists to observe entire events that are very difficult to discern by looking in a single temperature band, at a slower rate, or over a more limited field of view.

The data from SDO is providing a torrent of new information and spectacular images to be studied and interpreted. Using AIA's high-resolution and nearly continuous full-disk images of the sun, scientists have a better understanding of how even small events on our nearest star can significantly impact technological infrastructure on Earth.

Solar storms produce disturbances in electromagnetic fields that can induce large currents in wires, disrupting power lines and causing widespread blackouts. The storms can interfere with global positioning systems, cable television, and communications between ground controllers and satellites and airplane pilots flying near Earth's poles. Radio noise from solar storms also can disrupt cell phone service.

Launched in Feb. 2010, the spacecraft's commissioning May 14 confirmed all three of its instruments successfully passed an on-orbit checkout, were calibrated and are collecting science data.

"We're already at five million images and counting," said Dean Pesnell, the SDO project scientist at NASA's Goddard Space Flight Center in Greenbelt, Md. "With data and images pouring in from SDO, solar scientists are poised to make discoveries that will rewrite the books on how changes in solar activity have a direct effect on Earth. The observatory is working great, and it's just going to get better."

Goddard built, operates and manages the SDO spacecraft for NASA's Science Mission Directorate in Washington. SDO is the first mission of NASA's Living with a Star Program. The program's goal is to develop the scientific understanding necessary to address those aspects of the sun-Earth system that directly affect our lives and society.

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