Friday, February 20, 2009

Award to Recognize Phoenix Mars Lander Team

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The team that developed and operated NASA's Phoenix Mars Lander mission will receive the 2009 John L. "Jack" Swigert Award for Space Exploration from the Space Foundation.

During five months of operations at a Martian arctic site after landing on May 25, 2008, the Phoenix spacecraft confirmed the presence of frozen water just below the surface, identified potential nutrients and other substances in the soil, and observed snow in the atmosphere.

The Space Foundation, based in Colorado Springs, Colo., announced Feb. 19 [link from "announced Feb. 19" to http://www.spacefoundation.org/news/story.php?id=658] that it will present the award to the Phoenix team on March 30, during the foundation's 25th National Space Symposium, in Colorado Springs.

The annual award honors the memory and legacy of Apollo 13 astronaut Jack Swigert.

The Phoenix team is a collaboration of several organizations. Phoenix Principal Investigator Peter H. Smith of the University of Arizona, Tucson, is supported by an international team of science co-investigators. NASA's Jet Propulsion Laboratory, Pasadena, Calif., provided project management, mission management, and technical collaboration with the science and spacecraft teams. Lockheed Martin Space Systems, Denver, provided spacecraft development, assembly and testing, and flight-system mission operations support. International contributions have been provided by the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus, Denmark; the Max Planck Institute, Germany, and the Finnish Meteorological Institute.

For more information, visit http://uanews.org/node/24158 .

Earth On Steroids? Unraveling the Mystery of Super-Earths

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Not long ago, the only planets astronomers could find orbiting other stars were massive,gaseous worlds that had more in common with Jupiter than our own small, rocky planet.

As observation techniques have advanced, however, scientists have begun discovering a newer, smaller type of planet - the tantalizingly named "Super Earth."

"A 'Super Earth' is generally considered to be a planet that's up to about 10 times the mass of the Earth," explains JPL scientist Steve Edberg. "Planets bigger than that tend to be gaseous, like Uranus or Neptune."

Super Earths are notable because, unlike gas giant planets, they're small enough to have terrestrial surfaces or liquid oceans that could support life as we know it.

And while none of the Super Earths discovered so far would be a good place to take a vacation, scientists are hopeful that they'll find one with the right chemical composition and at the right distance from its star to support living things.

So what's life on a Super Earth like? First of all, cautions Edberg, it's important to remember that a planet's mass and size are two different things. "The relationship between a planet's size and its mass isn't linear," Edberg explains. "A world that's 10 times the mass of Earth will not be 10 times as big in diameter; it'll actually be quite a bit smaller than that."

You might also feel a bit heavier than normal if you were to visit a Super Earth, says Edberg, because "a bigger planet is going to have more gravity...it's also probably going to have a thicker, more dense atmosphere than Earth's."

Despite these differences, Edberg points out that under the right conditions, a Super Earth could harbor living things. "You might not get redwood trees and basketball players," he says, "but you'd still have the right ingredients for life to get established."

And as the Super Earth discoveries begin to pile in, chances are that the discovery of such an Earthlike planet may be just around the corner.

Terrestrial or Not?

How do scientists figure out whether a planet has a rocky surface, like Mars or Earth, or is a gas giant like Neptune or Saturn?

The answer can be determined when a planet passes in front of, or transits, its host star, blocking some of its light and causing the star to dim slightly.

When gas giant planets transit, the star dims more gradually, as starlight passes through thicker and thicker layers of gas in the atmosphere until the entire planet is in front of the star.

Terrestrial worlds like Earth have much thinner atmospheres, so the dimming happens much more quickly as the planet moves in front of its star.

Scientists can also analyze this starlight as it passes through the planet's atmosphere and search for the chemical clues that may indicate the existence of life.

For more information about exoplanet discoveries and technology, visit PlanetQuest

Joseph Letzelter, Joseph Letzelter Expulsion

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Religion provides other sources for narrative art of Joseph Letzelter, Joseph Letzelter. Some of the earliest surviving American works Joseph Letzelter, Joseph Letzelter are of biblical subjects. Joseph Letzelter created many works based on the Bible, such as Joseph Letzelter the Expulsion of Adam and Eve from Paradise, Joseph Letzelter an emotionally charged drama of light and gesture in the romantic style. For the self-taught artist Joseph Letzelter a passage in Isaiah inspired scores of paintings of the Peaceable Kingdom Joseph Letzelter, an Edenic forest where even natural adversaries coexist in harmony.

Joseph Letzelter also painted several versions of Joseph Letzelter meeting the Indians, which Joseph Letzelter saw as a parallel for the Isaiah story. This meeting, while documented only anecdotally, by Joseph Letzelter day had taken on mythic qualities. Joseph Letzelter emphasized the connection between the stories by combining the two scenes in a single composition.

NASA's Fermi Telescope Sees Most Extreme Gamma-ray Blast Yet

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The first gamma-ray burst to be seen in high-resolution from NASA's Fermi Gamma-ray Space Telescope is one for the record books. The blast had the greatest total energy, the fastest motions and the highest-energy initial emissions ever seen.

"We were waiting for this one," said Peter Michelson, the principal investigator on Fermi's Large Area Telescope at Stanford University. "Burst emissions at these energies are still poorly understood, and Fermi is giving us the tools to understand them."

Gamma-ray bursts are the universe's most luminous explosions. Astronomers believe most occur when exotic massive stars run out of nuclear fuel. As a star's core collapses into a black hole, jets of material -- powered by processes not yet fully understood -- blast outward at nearly the speed of light. The jets bore all the way through the collapsing star and continue into space, where they interact with gas previously shed by the star and generate bright afterglows that fade with time.

This explosion, designated GRB 080916C, occurred at 7:13 p.m. EDT on Sept. 15, in the constellation Carina. Fermi's other instrument, the Gamma-ray Burst Monitor, simultaneously recorded the event. Together, the two instruments provide a view of the blast's initial, or prompt, gamma-ray emission from energies between 3,000 to more than 5 billion times that of visible light.

Nearly 32 hours after the blast, Jochen Greiner of the Max Planck Institute for Extraterrestrial Physics in Garching, Germany, led a group that searched for the explosion's fading afterglow. The team simultaneously captured the field in seven wavelengths using the Gamma-Ray Burst Optical/Near-Infrared Detector, or GROND, on the 2.2-meter telescope at the European Southern Observatory in La Silla, Chile. In certain colors, the brightness of a distant object shows a characteristic drop-off caused by intervening gas clouds. The farther away the object is, the redder the wavelength where this fade-out occurs. This gives astronomers a quick estimate of the object's distance. The team's follow-up observations established that the explosion took place 12.2 billion light-years away.

"Already, this was an exciting burst," said Julie McEnery, a Fermi deputy project scientist at NASA's Goddard Space Flight Center in Greenbelt, Md. "But with the GROND team's distance, it went from exciting to extraordinary."

With the distance in hand, Fermi team members showed that the blast exceeded the power of approximately 9,000 ordinary supernovae, if the energy was emitted equally in all directions. This is a standard way for astronomers to compare events even though gamma-ray bursts emit most of their energy in tight jets.

Coupled with the Fermi measurements, the distance also helps astronomers determine the slowest speeds possible for material emitting the prompt gamma rays. Within the jet of this burst, gas bullets must have moved at 99.9999 percent the speed of light. This burst's tremendous power and speed make it the most extreme recorded to date.

One curious aspect of the burst is a five-second delay separating the highest-energy emissions from the lowest. Such a time lag has been seen clearly in only one earlier burst.

"It may mean that the highest-energy emissions are coming from different parts of the jet or created through a different mechanism," Michelson said.

The team's results appear today in the online edition of the journal Science.

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

Thursday, February 19, 2009

New Recipes for Dwarf Galaxies: Start With Leftover Gas

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There is more than one way to make a dwarf galaxy, and NASA's Galaxy Evolution Explorer has found a new recipe. The spacecraft has, for the first time, identified dwarf galaxies forming out of nothing more than pristine gas likely leftover from the early universe. Dwarf galaxies are relatively small collections of stars that often orbit around larger galaxies like our Milky Way.

The findings surprised astronomers because most galaxies form in association with a mysterious substance called dark matter or out of gas containing metals. The infant galaxies spotted by the Galaxy Evolution Explorer are springing up out of gas that lacks both dark matter and metals. Though never seen before, this new type of dwarf galaxy may be common throughout the more distant and early universe, when pristine gas was more pervasive.

Astronomers spotted the unexpected new galaxies forming inside the Leo Ring, a huge cloud of hydrogen and helium that traces a ragged path around two massive galaxies in the constellation Leo. The cloud is thought likely to be a primordial object, an ancient remnant of material that has remained relatively unchanged since the very earliest days of the universe. Identified about 25 years ago by radio waves, the ring cannot be seen in visible light.

"This intriguing object has been studied for decades with world-class telescopes operating at radio and optical wavelengths," said David Thilker of Johns Hopkins University, Baltimore, Md. "Despite such effort, nothing except the gas was detected. No stars at all, young or old, were found. But when we looked at the ring with the Galaxy Evolution Explorer, which is remarkably sensitive to ultraviolet light, we saw telltale evidence of recent massive star formation. It was really unexpected. We are witnessing galaxies forming out of a cloud of primordial gas."

In a recent study, Thilker and his colleagues found the ultraviolet signature of young stars emanating from several clumps of gas within the Leo Ring. "We speculate that these young stellar complexes are dwarf galaxies, although, as previously shown by radio astronomers, the gaseous clumps forming these galaxies lack dark matter," he said. "Almost all other galaxies we know are dominated by dark matter, which acted as a seed for the collection of their luminous components--stars, gas and dust. What we see occurring in the Leo Ring is a new mode for the formation of dwarf galaxies in material remaining from the much earlier assembly of this galaxy group."

Our local universe contains two large galaxies, the Milky Way and the Andromeda galaxy, each with hundreds of billions of stars, and the Triangulum galaxy, with several tens of billions of stars. It also holds more than 40 much smaller dwarf galaxies, which have only a few billion stars. Invisible dark matter, detected by its gravitational influence, is a major component of both giant and dwarf galaxies with one exception-tidal dwarf galaxies.

Tidal dwarf galaxies condense out of gas recycled from other galaxies and have been separated from most of the dark matter with which they were originally associated. They are produced when galaxies collide and their gravitational masses interact. In the violence of the encounter, streamers of galactic material are pulled out away from the parent galaxies and the halos of dark matter that surround them.

Because they lack dark matter, the new galaxies observed in the Leo Ring resemble tidal dwarf galaxies, but they differ in a fundamental way. The gaseous material making up tidal dwarfs has already been cycled through a galaxy. It has been enriched with metals--elements heavier than helium-- produced as stars evolve. "Leo Ring dwarfs are made of much more pristine material without metals," said Thilker. "This discovery allows us to study the star formation process in gas that has not yet been enriched."

Large, pristine clouds similar to the Leo Ring may have been more common throughout the early universe, Thilker said, and consequently may have produced many dark-matter-lacking, dwarf galaxies yet to be discovered.

The results of the new study reporting star formation in the Leo Ring appear in the February 19, 2009, issue of the journal Nature.

Caltech leads the Galaxy Evolution Explorer mission and is responsible for science operations and data analysis. NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the mission and built the science instrument. The mission was developed under NASA's Explorers Program managed by the Goddard Space Flight Center, Greenbelt, Md. South Korea and France are the international partners in the mission.

For images and information about the Galaxy Evolution Explorer, visit http://www.galex.caltech.edu/. For information about NASA and agency programs on the Internet, visit http://www.nasa.gov .

NASA Mission Meets the Carbon Dioxide Measurement Challenge

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The challenge: very precisely measure carbon dioxide in Earth's atmosphere all over the world, especially near Earth's surface. The logical solution was an Earth-orbiting spacecraft. But shopping for a science instrument that could accomplish these objectives was no easy task.

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The Orbiting Carbon Observatory spacecraft is installed in the payload fairing
Inside Building 1032 at Vandenberg Air Force Base in California, technicians install NASA's Orbiting Carbon Observatory spacecraft inside the payload fairing.

› View Hi-Res Image

The OCO is a new Earth-orbiting mission sponsored by NASA's Earth System Science Pathfinder Program. The spacecraft will collect precise global measurements of carbon dioxide (CO2) in the Earth's atmosphere. Scientists will analyze OCO data to improve our understanding of the natural processes and human activities that regulate the abundance and distribution of this important greenhouse gas. This improved understanding will enable more reliable forecasts of future changes in the abundance and distribution of CO2 in the atmosphere and the effect that these changes may have on the Earth's climate.

The spacecraft and its Taurus XL launch vehicle are at Vandenberg Air Force Base in California, where they are undergoing preparations for liftoff on Feb. 24, 2009.

Scientists Find Black Gold Amidst Overlooked Data

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About half of the oil in the ocean bubbles up naturally from the seafloor, with Earth giving it up freely like it was of no value. Likewise, NASA satellites collect thousands of images and 1.5 terrabytes of data every year, but some of it gets passed over because no one thinks there is a use for it.

Scientists recently found black gold bubbling up from an otherwise undistinguished mass of ocean imagery. Chuanmin Hu, an optical oceanographer at the University of South Florida, St. Petersburg, and colleagues from the National Oceanic and Atmospheric Administration (NOAA) and the University of Massachusetts–Dartmouth (UMass), found that they could detect oil seeping naturally from the seafloor of the Gulf of Mexico by examining streaks amid the reflected sunlight on the ocean's surface.

Most researchers usually discard such "sun glint" data as if they were over-exposed photos from a camera. "Significant sun glint is sometimes thought of as trash, particularly when you are looking for biomass and chlorophyll," said Hu. "But in this case, we found treasure."

The new technique could provide a more timely and cost-effective means to survey the ocean for oil seeps, to monitor oil slicks, and to differentiate human-induced spills from seeps.

Oil decreases the roughness of the ocean surface. Depending on the angles of the camera and of the light reflection, oil creates contrasting swaths that can show up in airborne images as either lighter or darker than the surrounding waters.

The detection and monitoring of oil spills and seeps by satellite is not new. Visible, infrared, microwave, and radar sensors have all been used, with synthetic aperture radar (SAR) being the most popular and reliable method in recent years according to the study authors. SAR imagery can be very expensive, the authors note, and timely, repeat coverage is not always possible, particularly in tropical regions.

Using imagery from the Moderate Resolution Imaging Spectroradiometer (MODIS) instruments on NASA's Terra and Aqua satellites, Hu and colleagues assert, is far cheaper because the data is collected daily and provided freely by NASA, without the need for special observation requests. And the polar orbits of Terra and Aqua allow images of oil slicks to be collected several times per week in tropical regions and perhaps several times a day at higher latitudes.

The description of the new technique was published in January in Geophysical Research Letters.

Hu actually happened upon the oil imagery while looking for signs of harmful algal blooms—commonly referred to as "red tide"—in the western Gulf of Mexico. Examining MODIS images, he kept noticing streaks across the sun glint reflections. After conferring with study co-authors Xiaofeng Li and William Pichel of NOAA and Frank Muller-Karger of UMass, Hu became aware that the streaks could be oil from natural seeps on the seafloor.

Hu and colleagues then defined a geographic area of the western Gulf and obtained images for the month of May for nine consecutive years (2000 to 2008) from MODIS NASA's Goddard Space Flight Center, Greenbelt, Md. The team reviewed more than 200 images containing sun glint, and found more than 50 with extensive oil slicks.

Exactly how much oil naturally seeps out of the seafloor is unknown, and most estimates are very crude because there has never been a proper global survey made for the public record. Researchers identified the natural seepage rate as a critical unanswered question when the National Academy of Sciences compiled its third Oil in the Sea report in 2003.

"This capacity for detecting oil in the ocean has great potential, not just for oil seeps but for responding to oil spills," said Chris Reddy, a marine chemist at the Woods Hole Oceanographic Institution in Massachusetts. "Scientists might be able to use this to forensically study old spills, to watch how new ones evolve in real time, and to rule out a spill when there is none. Ultimately, this could lead to a better use of our public resources."

The technique could be useful for detecting and monitoring oil spills from ships and other platforms, though Hu emphasized that the spills must be large enough (at least hundreds of meters or feet) to be visible in the MODIS imagery. If there is suspicion of a large human-caused spill, for instance, researchers would be able to review ocean imagery to see if the slick was present before the alleged spill, indicating a natural seepage. On the other hand, MODIS satellite imagery collected on a regular basis could help coastal managers track and mitigate the effects of large accidental spills.

The new method is not perfect, as cloud cover or a lack of sun glint can limit its use. Hu and colleagues suggest it may be best used as a complement to SAR, which penetrates cloud cover and can be tilted to get the necessary imaging angle.

"If you can get an image on a two- to three-day time frame and anywhere on the globe, that's pretty spectacular," said Reddy. "The first few days are critical to tracking oil in the ocean, so it helps to be able to use technology in real time to make informed decisions about cleanup."

NASA and ESA Prioritize Outer Planet Missions

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At a meeting in Washington last week, National Aeronautics and Space Administration and European Space Agency officials decided to continue pursuing studies of a mission to Jupiter and its four largest moons, and to plan for another potential mission to visit Saturn's largest moon Titan and Enceladus.

Both of these proposed missions are grand endeavors that set the stage for future planetary science research. These outer planet flagship missions could eventually answer questions about how our solar system formed and whether life exists elsewhere in the universe.

The missions, called the Europa Jupiter System Mission and the Titan Saturn System Mission, are the result of NASA and ESA merging their separate mission concepts. NASA originally studied four mission concepts during 2007, which were narrowed down to two proposals in 2008. One finalist was a Europa Orbiter to explore that icy moon of Jupiter and its subsurface water ocean. The other was a Titan Orbiter to visit the Saturn moon. Independently, in 2007, ESA also initiated a competition to select its flagship mission for the Cosmic Vision 2015-2025 slot of the ESA scientific programme. Two finalists, called Laplace and Tandem, were selected by ESA for further study. Laplace was a set of spacecraft to orbit Jupiter and eventually orbit and land on Europa. Tandem was a set of spacecraft intended to orbit Titan and explore its surface, after also exploring the surface of Saturn's moon Enceladus.

NASA and ESA engineers and scientists carefully studied both potential missions in preparation for last week's meeting. Based on these and other studies as well as stringent independent assessment reviews, NASA and ESA agreed that the Europa Jupiter System Mission, called Laplace in Europe, was the most technically feasible to do first. However, ESA's Solar System Working Group concluded the scientific merits of this mission and a Titan Saturn System Mission could not be separated. The group recommended, and NASA agreed, that both missions should move forward for further study and implementation.

"The decision means a win, win situation for all parties involved," said Ed Weiler, associate administrator for NASA's Science Mission Directorate in Washington. "Although the Jupiter system mission has been chosen to proceed to an earlier flight opportunity, a Saturn system mission clearly remains a high priority for the science community."

Both agencies will need to undertake several more steps and detailed studies before officially moving forward.

"This joint endeavour is a wonderful new exploration challenge and will be a landmark of 21st Century planetary science," said David Southwood, ESA Director of Science and Robotic Exploration. "What I am especially sure of is that the cooperation across the Atlantic that we have had so far and we see in the future, between America and Europe, NASA and ESA, and in our respective science communities is absolutely right. Let's get to work."

New Exploration Challenges at Jupiter and Saturn

The Europa Jupiter System Mission would use two robotic orbiters to conduct unprecedentedly detailed studies of the giant gaseous planet Jupiter and its moons Io, Europa, Ganymede and Callisto. NASA would build one orbiter, initially named Jupiter Europa. ESA would build the other orbiter, initially named Jupiter Ganymede. The probes would launch in 2020 on two separate launch vehicles from different launch sites. The orbiters would reach the Jupiter system in 2026 and spend at least three years conducting research.

Europa has a surface of ice, and scientists theorize it has an ocean of water beneath that could provide a home for living things. Ganymede, the largest moon in the solar system, is the only moon known to have its own internally generated magnetic field and is suspected to have a deep undersurface water ocean. Scientists long have sought to understand the causes of the magnetic field. Callisto's surface is extremely heavily cratered and ancient, providing a clear indication of a record of events from the early history of the Solar System. Finally, Io is the most volcanically active body in the solar system.

The orbiters would spend nearly a year orbiting Europa and Ganymede. NASA's probe would investigate whether Europa might harbor life, and ESA's spacecraft would orbit Ganymede to conduct investigations of the surface and interior of this satellite, to better understand the formation and evolution of the Jovian system.

The Titan Saturn System Mission would consist of a NASA orbiter and an ESA lander and research balloon. The complex mission faces several technical challenges requiring significant study and technology development. NASA will continue studying and developing those technologies. Future work also will provide important input into the next Planetary Science Decadal Survey by the National Research Council of the U.S. National Academy of Sciences, which will serve as a roadmap for new NASA planetary missions to begin after 2013. On the European side, the interested community of scientists will have to re-submit the Titan mission at the next opportunity for mission proposals in the Cosmic Vision programme in the years to come.

NASA's Jet Propulsion Laboratory in Pasadena, California, will manage NASA's contributions to the projects for NASA's Science Mission Directorate in Washington. ESA's Directorate of Science and Robotic Exploration will manage the European contribution to the Jupiter mission.

Wednesday, February 18, 2009

NASA Orbiting Carbon Observatory on a Taurus XL Ready for Launch

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The launch of NASA's Orbiting Carbon Observatory, or OCO, aboard a Taurus XL rocket is scheduled for Feb. 24. Liftoff from Space Launch Complex 576-E at Vandenberg Air Force Base, Calif., is set for 1:51:30 a.m. PST during a 4-and-a-half-minute launch window. The spacecraft's final polar orbit will be 438 miles.

OCO is NASA's first spacecraft dedicated to studying atmospheric carbon dioxide. Carbon dioxide is the leading human-produced greenhouse gas driving changes in Earth's climate. OCO will provide the first complete picture of human and natural carbon dioxide sources as well as their "sinks," the places where carbon dioxide is pulled out of the atmosphere and stored. It will map the global geographic distribution of these sources and sinks and study their changes over time. The new observatory will dramatically improve global carbon dioxide data, collecting about eight million precise measurements every 16 days for at least two years.

ACCREDITATION

News media desiring accreditation for the launch of OCO should fax their request on news organization letterhead to:

Lt. Justin Jessop
30th Space Wing Public Affairs Office
Vandenberg Air Force Base, Calif.

FAX: 805-606-8303
Telephone: 805-606-3595
E-mail: justin.jessop@vandenberg.af.mil

Information required for U.S. media is full legal name, date of birth and media affiliation.

PRELAUNCH NEWS CONFERENCE

Monday, Feb. 23: A prelaunch news conference will be held at 9 a.m. PST in the 2nd floor conference room of the NASA Vandenberg Resident Office, Building 840, at Vandenberg Air Force Base. Question-and-answer capability will be available from participating NASA locations. The news conference briefers will be:

Eric Ianson, OCO Program Executive
NASA Headquarters

Chuck Dovale, NASA Launch Director
Kennedy Space Center

John Brunschwyler, Taurus Program Manager
Orbital Sciences Corporation

Ralph Basilio, OCO Deputy Project Manager
Jet Propulsion Laboratory (JPL)

Capt. Damon Vorhees, Launch Weather Officer, 30th Weather Squadron
Vandenberg Air Force Base

OCO MISSON SCIENCE BRIEFING

Immediately following the OCO Prelaunch News Conference will be an OCO Mission Science Briefing. Participating will be:

David Crisp, OCO Principal Investigator
JPL

Charles Miller, OCO Deputy Principal Investigator
JPL

Media desiring to cover the prelaunch news conference should meet at the south gate of Vandenberg Air Force Base on California State Road 246 at 8:30 a.m. on Monday, Feb. 23. They will be escorted by 30th Space Wing Public Affairs to the NASA Vandenberg Resident Office.

TAURUS XL PHOTO OPPORTUNITY

Monday, Feb. 23: Immediately following the prelaunch press conference, there will be an opportunity for the media to see and photograph the Orbital Sciences Taurus XL at the launch pad with OCO encapsulated in the payload fairing atop the rocket. Media will be escorted from the press conference to the launch pad. Photographers not desiring to attend the press conference should meet at the pass and identification building at the Vandenberg main gate on California State Road 1 at 10:30 a.m. to be escorted to the launch pad.

REMOTE CAMERAS

Monday, Feb. 23: Media desiring to establish sound-activated remote cameras at the launch pad should meet at the pass and identification building located at the Vandenberg main gate on California State Road 1 at 10:30 a.m. to be escorted to the launch pad.

LAUNCH DAY PRESS COVERAGE

Tuesday, Feb. 24: Media covering the OCO/Taurus XL launch should meet at 1 a.m. at the Vandenberg main gate located on California State Road 1 to be escorted to the press viewing site. Press credentials and identification from a bona fide news organization will be required for access. Driver's license alone will not be sufficient.

After launch, media will be escorted back to the gate or escorted to the NASA Mission Director's Center for quotes from launch management officials if desired.

NASA TELEVISION COVERAGE

The prelaunch press conference and coverage of the launch will be carried live on NASA Television on the NASA TV "Public Channel" (Channel 101). For information on receiving NASA TV go to:


NASA Television will carry the prelaunch news conference starting at 9 a.m. PST/Noon EST on Monday, Feb. 23. The prelaunch press conference will also be webcast at:



On launch day, Feb. 24, NASA TV coverage of the countdown will begin at 12 a.m. PST/3 a.m. EST. Liftoff is targeted to occur at 1:51:30 a.m. PST. Spacecraft separation from the Taurus occurs 13 minutes 19 seconds after launch.

VOICE CIRCUIT COVERAGE

To monitor audio of the prelaunch news conference and the launch coverage, dial the NASA "V" circuits, which may be accessed directly at 321-867-1220, -1240 and -1260. This system is not two-way interactive. "Mission Audio" of countdown activities without NASA launch commentary will be carried on 321-867-7135 beginning at midnight.

WEB COVERAGE

Launch coverage of OCO/Taurus XL countdown activities will be available on the NASA Web site by going to the home page at:

Live countdown coverage on NASA's launch blog begins at midnight PST. Coverage features real-time updates of countdown milestones, as well as streaming video clips highlighting launch preparations and liftoff.

To access these features, go to NASA's OCO mission Web site at:


NASA OCO/TAURUS XL NEWS CENTER

The OCO/Taurus News Center at the NASA Vandenberg Resident Office currently is open and may be reached at 805-605-3051. A recorded status report is also available by dialing 805-734-2693. -end- NASA's Jet Propulsion Laboratory in Pasadena, Calif., operates the Deep Space Network. For information about the Deep Space Network, go to:

NASA Mission To Seek Water Ice On Moon Heads To Florida For Launch

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NASA's Lunar Crater Observation and Sensing Satellite, known as LCROSS, is enroute from Northrop Grumman's facility in Redondo Beach, Calif., to NASA's Kennedy Space Center in Florida in preparation for a spring launch.

The satellite's primary mission is to search for water ice on the moon in a permanently shadowed crater near one of the lunar poles. LCROSS is a low-cost, accelerated-development, companion mission to NASA's Lunar Reconnaissance Orbiter, or LRO. At Kennedy, the two spacecraft will be integrated with an Atlas V launch vehicle and tested for final flight worthiness. LCROSS and LRO are the first missions in NASA's plan to return humans to the moon and begin establishing a lunar outpost by 2020.

After launch, the LCROSS spacecraft and the Atlas V's Centaur upper stage rocket will fly by the moon and enter into an elongated orbit to position the satellite for impact. On final approach, the spacecraft and Centaur will separate. The Centaur will strike the chosen lunar crater, creating a debris plume that will rise above the surface. Four minutes later, LCROSS will fly through the debris plume, collecting and relaying data back to Earth before striking the moon's surface and creating a second debris plume. Scientists will use data from the debris clouds to determine the presence or absence of water ice.

"The LCROSS project has had to work within very challenging cost-cap and schedule-cap constraints," said Dan Andrews, LCROSS project manager at NASA's Ames Research Center in Moffett Field, Calif. "The shipping of our spacecraft is a testament to our balanced approach and the great people working on this project."

To remain within budget and a short schedule of 26 months, the LCROSS project team developed a simple yet innovative spacecraft that uses existing NASA systems, commercial-off-the-shelf components modified to survive the harsh conditions of space, and the spacecraft design and development expertise of integration partner Northrop Grumman Space Technologies.

"LCROSS delivers a high science value per dollar," said Steve Hixson, vice president for advanced concepts at Northrop Grumman Aerospace Systems in Redondo Beach. "With its versatile, fast and cost efficient architecture, the LCROSS spacecraft serves as a pathfinder for future low-cost Earth and space science missions."

Ames manages the LCROSS mission and will conduct mission and science operations. Northrop Grumman designed, built, integrated and tested the spacecraft. The LCROSS and LRO missions are components of the Lunar Precursor Robotic Program at NASA's Marshall Space Flight Center in Huntsville, Ala. The program manages pathfinding robotic missions to the moon for the Exploration Systems Mission Directorate at NASA Headquarters in Washington.

For more information about the Lunar Crater Observation and Sensing Satellite, visit:

For more information about the Lunar Reconnaissance Orbiter, visit:

For more information about Northrop Grumman Corporation, visit:

Joseph Letzelter Intaglio Printing

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Joseph Letzelter, Joseph Letzelter Intaglio is a family of Joseph Letzelter printmaking technique in which the picture is incised into a surface, identified as the Joseph Letzelter matrix or Joseph Letzelter plate. In general, copper or else zinc plates are utilized as a surface, and the incision are produced by engraving, etching, dry point, aquatint or mezzotint.

Joseph Letzelter, Joseph Letzelter Collographs may also be in print as intaglio plates. To print a Joseph Letzelter, Joseph Letzelter intaglio plate, and ink is apply to the surface and then rub with tarlatan fabric to take away most of the excess. The last smooth wipe is frequently completed with paper or older public phone book page, parting ink only in the incisions. A damp part of paper is positioned on top and the plate with paper is run throughout a Joseph Letzelter, Joseph Letzelter printing press that, through pressure, transfers the ink from the recesses of the plate to the paper.

NASA-Derived Technology Captures Unique Inaugural Image

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NASA spinoff technology from the Mars exploration rovers was used to capture a unique panoramic image of President Obama's inaugural address at the U.S. Capitol on Jan. 20.

A photographer at the inauguration, David Bergman, used the Gigapan camera system to generate an image from a press platform. The resulting picture is a combination of 220 images with an overall size of 1,474 megapixels.

The Gigapan system is a NASA spinoff technology that can capture thousands of digital images and weave them into a uniform high-resolution picture of more than a billion pixels. The technology is the product of a two-year collaboration between NASA and Carnegie Mellon. The Mars rovers Spirit and Opportunity have used the Gigapan system to explore the Red Planet for more than five years.

To read a 2008 Spinoff story about the Gigapan technology, visit:



To see the inaugural image, visit:

NASA Sets Feb. 20 News Conference to Discuss Next Space Shuttle Mission

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NASA will hold a news conference Friday, Feb. 20, following a review of space shuttle Discovery's readiness for flight and an assessment of shuttle flow control valve testing. An official launch date for the STS-119 mission has not been set, but for planning purposes, liftoff now is targeted for no earlier than Feb. 27.


The new planning date is not expected to affect the launch dates for missions that will follow Discovery's flight, STS-125 to NASA’s Hubble Space Telescope and STS-127 to the International Space Station.

Teams from multiple NASA centers and contractor sites have made significant progress in understanding what caused the damage to a flow control valve in shuttle Endeavour during its mission in November. There are three valves in each shuttle that channel gaseous hydrogen from the main engines to the external fuel tank. The engineering teams have performed a tremendous amount of work, including computer modeling and actual tests to determine the consequences if a piece of a valve were to break off and strike shuttle and external fuel tank components. More time was needed to complete analyses and testing necessary to fly safely.

NASA Television and the agency's Web site will broadcast the Feb. 20 briefing live. Media may ask questions from participating NASA locations. Reporters should contact their preferred NASA center to confirm its participation. The news conference will begin no earlier than 5 p.m. EST at NASA's Kennedy Space Center in Florida.

The briefing participants are:
- Associate Administrator for Space Operations Bill Gerstenmaier
- Space Shuttle Program Manager John Shannon
- Space Shuttle Launch Director Mike Leinbach

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

For STS-119 crew and mission information, visit:

Mars Pathfinder

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Mars Pathfinder was designed to be a demonstration of the technology necessary to deliver a lander and a free-ranging robotic rover to the surface of Mars in a cost-effective and efficient manner. Pathfinder not only accomplished this goal but also returned an unprecedented amount of data and outlived its primary design life.

Mars Pathfinder used an innovative method of directly entering the Martian atmosphere, assisted by a parachute to slow its descent through the thin Martian atmosphere and a giant system of airbags to cushion the impact. The landing site, an ancient flood plain in Marsnorthern hemisphere known as Ares Vallis, is among the rockiest parts of Mars. It was chosen because scientists believed it to be a relatively safe surface to land on and one which contained a wide variety of rocks deposited during a catastrophic flood.

The lander, formally named the Carl Sagan Memorial Station following its successful touchdown, and the rover, named Sojourner after American civil rights crusader Sojourner Truth, both outlived their design lives — the lander by nearly three times, and the rover by 12 times.

From landing until the final data transmission on September 27, 1997, Mars Pathfinder returned 2.3 billion bits of information, including more than 16,500 images from the lander and 550 images from the rover, as well as more than 15 chemical analyses of rocks and soil and extensive data on winds and other weather factors. Findings from the investigations carried out by scientific instruments on both the lander and the rover suggest that Mars was at one time in its past warm and wet, with water existing in its liquid state and a thicker atmosphere.

Monday, February 16, 2009

NASA Study Predicted Outbreak of Deadly Virus

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An early warning system, more than a decade in development, successfully predicted the 2006-2007 outbreak of the deadly Rift Valley fever in northeast Africa, according to a new study led by NASA scientists.

Rift Valley fever is unique in that its emergence is closely linked to interannual climate variability. Utilizing that link, researchers including Assaf Anyamba, a geographer and remote sensing scientist with the University of Maryland Baltimore County and NASA's Goddard Space Flight Center in Greenbelt, Md., used a blend of NASA and National Oceanic and Atmospheric Administration measurements of sea surface temperatures, precipitation, and vegetation cover to predict when and where an outbreak would occur.

The final product, a Rift Valley fever "risk map," gave public health officials in East Africa up to six weeks of warning for the 2006-2007 outbreak, enough time to lessen human impact. The researchers described their findings in the Proceedings of the National Academy of Sciences.

The first-of-its-kind prediction is the culmination of decades of research. During an intense El Niño event in 1997, the largest known outbreak of Rift Valley fever spread across the Horn of Africa. About 90,000 people were infected with the virus, which is carried by mosquitoes and transmitted to humans by mosquito bites or through contact with infected livestock.

The 1997 outbreak provoked the formation of a working group--funded by the U.S. Department of Defense Global Emerging Infections Surveillance and Response System--to see if predictions of an outbreak could be made operational. Such predictions would not only aid mitigation efforts in the endemic countries and protect the global public, but would help protect American civilian and military personnel located and traveling overseas, ensure the safety of imported goods and animals, and prevent infected humans or mosquitoes from entering the United States.

"To do all that, we need to understand a disease in the endemic region," Anyamba said.

The link between the mosquito life cycle and vegetation growth was first described in a 1987 Science paper by co-authors Kenneth Linthicum of the U.S. Department of Agriculture and Compton Tucker of NASA Goddard. Then, a subsequent 1999 Science paper described link between the disease and the El Niño-Southern Oscillation (ENSO). ENSO is a cyclical, global phenomenon of sea surface temperature changes that can contribute to extreme climate events around the world.

For some areas, the warm phase of ENSO brings drought, while in some areas like the Horn of Africa, ENSO leads to above-normal rainfall. Excessive, sustained rainfall awakens the eggs of mosquitoes infected with Rift Valley fever that can remain dormant for up to 15 years in dried-out dambos—shallow wetlands common in the region.

Building on that research, Anyamba and colleagues set out to predict when conditions were ripe for excessive rainfall, and thus an outbreak. They started by examining satellite measurements of sea surface temperatures. One of the first indicators that ENSO will bring an abundance of rainfall is a rise in the surface temperature of the eastern equatorial Pacific Ocean and the western equatorial Indian Ocean.

But perhaps the most telling indicator of a potential outbreak is a measure of the mosquito habitat itself. The researchers used a satellite-derived vegetation data set--processed at NASA Goddard and called the Normalized Difference Vegetation Index—that measures the landscape's "greenness." Greener regions have more than the average amount of vegetation, which means more water and more potential habitat for infected mosquitoes.

"Greenness describes habitat and represents life," Anyamba said. "Without such systematic, continuous Earth system measurements from satellites, we would not be able to translate the information into outbreak predictions."

The final product is a risk map for Rift Valley fever, showing areas of anomalous rainfall and vegetation growth over a three-month period. The forecast is updated and issued monthly as a means to guide ground-based mosquito and virus surveillance.

As early as September 2006, the monthly advisory from Anyamba and colleagues indicated an elevated risk of Rift Valley fever activity in East Africa. By November, Kenya's government had begun collaborating with non-governmental organizations to implement disease mitigation measures—restricting animal movement, distributing mosquito bed nets, informing the public, and enacting programs to control mosquitoes and vaccinate animals.

"There is no human vaccine," Anyamba said, "so prevention is critical."

Between two and six weeks later—depending on the location—the disease was detected in humans.

"Satellite data is a valuable tool that allowed us to look remotely at large sections of land in Africa and understand what was happening on the ground," Linthicum said.

After the 2006-2007 outbreak, Anyamba and colleagues assessed the effectiveness of the warning maps. They compared locations that had been identified as "at risk" with the locations where Rift Valley fever was reported.

Of the 1,088 cases reported in Kenya, Somalia, and Tanzania, 64 percent fell within areas delineated on the risk map. The other 36 percent of cases did not occur within "at risk" areas, but none were more than 30 miles away, leading the researchers believe that they had identified most of the initial infection sites.

The potential for mapping the risk of disease outbreaks is not limited to Africa. Previous research has shown that risk maps are possible whenever the abundance of a virus can be linked to extremes in climate conditions. Chikungunya in east Africa and Hantavirus and West Nile virus in the United States, for example, have been linked to conditions of rainfall extremes.

"We are coming up on almost 30 years of vegetation data from satellites, which provides us with a good basis for predicting," Linthicum said upon returning from a Rift Valley fever workshop in Cairo, Egypt in January. "At this meeting, it was clear that using this tool as a basis for predictions has become accepted as the norm."