Friday, March 22, 2013

Fwd: JPL Scientists Reflect on World Water Day



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From: NASA Jet Propulsion Laboratory <JPLNewsroom@jpl.nasa.gov>
Date: Fri, Mar 22, 2013 at 5:19 PM
Subject: JPL Scientists Reflect on World Water Day
To: Bob Jones <wxyznews@gmail.com>


JPL/NASA News
News feature: 2013-113                                                                       March 22, 2013

JPL Scientists Reflect on World Water Day

JPL Scientists Reflect on World Water Day

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-113&cid=release_2013-113

"We forget that the water cycle and the life cycle are one."
-- Jacques Cousteau

Water. Beautiful. Ever-changing. Life-giving. It envelops us, creates us, nurtures us, defines us, and yet can destroy us in an instant. This chemical compound -- two parts hydrogen, one part oxygen -- that we take for granted as plentiful, is actually remarkably scarce in its freshwater form. Less than three percent of Earth's water is freshwater, and more than two-thirds of that is locked up in glaciers and icecaps and therefore unavailable for drinking or agriculture. Within our solar system, water is even more scarce. And while NASA continues its quest to "follow the water" on Mars, NASA Jet Propulsion Laboratory Earth scientists and many of its Earth missions are busy studying our Water World and the complex interactions between Earth's water and its atmosphere, land and living organisms that make up our dynamic Earth system.

Each year on March 22, the member states of the United Nations observe World Water Day to focus attention on the importance of freshwater and to advocate for the sustainable management of Earth's precious freshwater resources. In December 2010, the United Nations General Assembly declared 2013 as the United Nations International Year of Water Cooperation. The objective of the year is to raise awareness of the potential for, and value of increased cooperation in relation to water.

We asked several JPL scientists to reflect on World Water Day and the importance of studying Earth's water.

"When it comes to humans and climate change, it is all about the water. It's too dry where you want it wet, too wet where you want it dry, salty where you want it fresh, liquid where you want it solid, and ultimately....you can't grow food without water."
-- Erika Podest, JPL research scientist

"We are now able to see from space all parts of the water cycle on land -- rain and snow, evapotranspiration, soil moisture and deep groundwater, and NASA has another satellite mission on its way to detect river runoff: Surface Water and Ocean Topography, or SWOT. We're combining all these 'eyes on Earth' to make better predictions of water resources, droughts and floods."
-- Josh Fisher, JPL research scientist

"Probing aquifers with NASA airborne radar can help scientists better understand Earth's fossil aquifer systems. The approximate number, occurrence and distribution of those systems remain largely unknown. Much of the evidence for climate change in Earth's deserts lies beneath the surface and is reflected in its groundwater. By mapping desert aquifers with this technology, we can detect layers deposited by ancient geological processes and trace back paleoclimatic conditions that existed thousands of years ago, when many of today's deserts were wet.

"Most recent observations, scientific interest and data analyses of global warming have concentrated on Earth's polar regions and forests, which provide direct measurable evidence of large-scale environmental changes. Arid and semi-arid environments, which represent a substantial portion of Earth's surface, have remained poorly studied. Yet water scarcity and salt content, changes in rainfall, flash floods, high rates of aquifer exploitation and growth of desert regions are all signs that suggest climate change and human activities are also affecting these arid and semi-arid zones."
-- Essam Heggy, JPL research scientist

"Water, water, every where,
And all the boards did shrink;
Water, water, every where,
Nor any drop to drink."
-- "The Rime of the Ancient Mariner"

"Since 2002, NASA's twin Gravity Recovery and Climate Experiment (GRACE) satellites have been monitoring large-scale groundwater depletion all over the globe. In northwest India, the Middle East, and also close to home in California's Central Valley aquifer, a significant fraction of the water needed to farm comes from groundwater. With GRACE, we have a tool that allows us to very accurately detect where and how much water is pumped from deep below -- unfortunately, often at unsustainable rates. For example, during the 2006 to 2010 California drought, the equivalent volume of an entire Lake Mead was extracted from the Central Valley Aquifer!"
-- Felix Landerer, JPL research scientist

"In Colombia, the country where I was born, it rained constantly for more than a year. At the same time, the United States, where I now live, was experiencing extreme droughts. The movement of water is global, giving to some what it takes from others. As Earth's climate changes, changes in precipitation and water storage will change the way we live. We need to understand how, and how we can adapt."
-- Ernesto Rodriguez, QuikScat project scientist; ISS-RapidScat principal investigator; mission design lead, Surface Water and Ocean Topography Mission

"More than 90 percent of the water vapor traveling from the tropical oceans to Earth's mid-latitudes is contained in narrow channels in the lower atmosphere called 'atmospheric rivers,' where the amount of water transported is comparable to the largest rivers on Earth. In our studies of California's Sierra Nevada Mountains, we found that snowfall produced by atmospheric rivers accounts for, on average, nearly 50 percent of the total water storage in the seasonal snowpack. However, we also found the amount of snow deposited during atmospheric river events is sensitive to air temperature changes on the order of a few degrees -- that is, similar to future projections of regional climate warming. This is one example of how vulnerable our natural water system could be, and of the importance of water cooperation."
-- Bin Guan, JPL research scientist

"Water sustains all."
-- Thales of Miletus, 600 B.C.

"Water, water everywhere, but ... almost none of it is for drinking. Why? On Earth, more than 97 percent of our precious water is in the ocean and is salty. Even though we can't drink our oceans, they have provided the unique crucible where life developed and thrived, and our oceans are the great buffer that provides our 'near-perfect' climate. But in the past century, the oceans are warming, rising and becoming more acidic. Without consideration for the consequences, humankind is upsetting the climate that has sustained our civilizations for millennia. We are behaving thoughtlessly, foolishly and dangerously. If we abuse the oceans, we put all life on Earth in peril. On this World Water Day, it's imperative that each of us pledges to handle the oceans with care."
-- Bill Patzert, JPL climatologist

"As exemplified by NASA and JPL's remarkable achievements in the search for water on Mars, we are using this world-class science and engineering expertise to measure Earth's freshwater reservoirs and fluxes. During this decade, we will see come to fruition the capabilities to monitor nearly every component of Earth's freshwater -- from the snow and ice at the poles and in our mountains to the groundwater deep beneath our feet, and all that lies between, such as water vapor, clouds and precipitation in the atmosphere and stream flow and soil moisture on the ground. As the demand for this precious resource increase with population growth and societal and ecosystem vulnerabilities change and/or grow in conjunction with climate change, these capabilities will become vital to maintaining our thriving society."
-- Duane Waliser, JPL chief Earth scientist

"When the well is dry, we know the worth of water."
-- Benjamin Franklin

"On a warming planet, the shifting water resources will cast a significant impact on our society. The steady source of freshwater from the mountaintops that has fostered human civilization for thousands of years has begun changing rapidly. We do not even have an adequate inventory of Earth's lakes. Only 15 percent of the lakes are measurable from space. Millions of small lakes have not yet been mapped and monitored. In addition, existing stream gauges cover only very large river basins, yet we do not have adequate knowledge of the river flow (or its discharge) in most of the river basins that sustain human needs.

"The Surface Water and Ocean Topography (SWOT) satellite mission planned for launch in 2020 -- jointly developed and managed by NASA, the French Space Agency (CNES) and the Canadian Space Agency -- will make measurements of the inventory of lakes and the discharge of rivers that are key to understanding the global water cycle on land; studying the dynamics of floodplains and wetlands, which have important impact on flood control and the balance of ecosystems; and providing a global assessment of water resources, including transboundary rivers, lake and reservoir storage and river dynamics."
-- Lee-Lueng Fu, JPL senior research scientist/Surface Water and Ocean Topography mission project scientist

Several of the new NASA JPL Earth satellite missions launching in 2014 and early 2015 will "follow the water" on Earth, among them:
- ISS-RapidScat, which will measure ocean surface wind speed and direction and help improve weather forecasts, including hurricane monitoring.
- Jason-3, which will extend the timeline of ocean surface topography measurements begun by the Topex/Poseidon, Jason-1 and Jason-2 satellites, making highly detailed measurements of sea level on Earth to gain insight into ocean circulation and climate change.
- Soil Moisture Active Passive (SMAP), which will measure how much water is in the top layer of Earth's soil. Among the mission's many benefits, it will help us better understand and manage water resources; better understand Earth's terrestrial water, carbon and energy cycles; and improve flood predictions and drought monitoring.

Related links:

World Water Day: http://www.worldwaterday.org
GRACE: http://www.csr.utexas.edu/grace/science/
SWOT: http://swot.jpl.nasa.gov/
SMAP: http://smap.jpl.nasa.gov/
ISS-RapidScat: http://www.nasa.gov/mission_pages/station/research/experiments/ISSRapidScat.html
Jason-3: http://sealevel.jpl.nasa.gov/missions/jason3/
JPL Western Water Resource Solutions website: http://water.jpl.nasa.gov/
JPL Earth science: http://www.jpl.nasa.gov/earth/
NASA Global Climate Change: http://climate.nasa.gov/
NASA Earth science: http://www.nasa.gov/topics/earth/index.html

JPL is managed for NASA by the California Institute of Technology in Pasadena, Calif.

Alan Buis 818-354-0474
Jet Propulsion Laboratory, Pasadena, Calif.
alan.buis@jpl.nasa.gov

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Thursday, March 21, 2013

Supercomputer Helps Planck Mission Expose Ancient Light

JPL/NASA News

News feature: 2013-110                                                                    March 21, 2013

Supercomputer Helps Planck Mission Expose Ancient Light

Supercomputer Helps Planck Mission Expose Ancient Light

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-110&cid=release_2013-110

Like archeologists carefully digging for fossils, scientists with the Planck mission are sifting through cosmic clutter to find the most ancient light in the universe.

The Planck space telescope has created the most precise sky map ever made of the oldest light known, harking back to the dawn of time. This light, called the cosmic microwave background, has traveled 13.8 billion years to reach us. It is so faint that Planck observes every point on the sky an average of 1,000 times to pick up its glow.

The task is even more complex than excavating fossils because just about everything in our universe lies between us and the ancient light. Complicating matters further is "noise" from the Planck detectors that must be taken into account.

That's where a supercomputer helps out. Supercomputers are the fastest computers in the world, performing massive amounts of calculations in a short amount of time.

"So far, Planck has made about a trillion observations of a billion points on the sky," said Julian Borrill of the Lawrence Berkeley National Laboratory, Berkeley, Calif. "Understanding this sheer volume of data requires a state-of-the-art supercomputer."

Planck is a European Space Agency mission, with significant contributions from NASA. Under a unique agreement between NASA and the Department of Energy, Planck scientists have been guaranteed access to the supercomputers at the Department of Energy's National Energy Research Scientific Computing Center at the Lawrence Berkeley National Laboratory. The bulk of the computations for this data release were performed on the Cray XE6 system, called the Hopper. This computer makes more than a quintillion calculations per second, placing it among the fastest in the world.

One of the most complex aspects of analyzing the Plank data involves the noise from its detectors. To detect the incredibly faint cosmic microwave background, these detectors are made of extremely sensitive materials. When the detectors pick up light from one part of the sky, they don't reset afterwards to a neutral state, but instead, they sort of buzz for a bit like the ringing of a bell. This buzzing affects observations made at the next part of the sky.

This noise must be understood, and corrected for, at each of the billion points observed repeatedly by Plank as it continuously sweeps across the sky. The supercomputer accomplishes this by running simulations of how Planck would observe the entire sky under different conditions, allowing the team to identify and isolate the noise.

Another challenge is carefully teasing apart the signal of the relic radiation from the material lying in the foreground. It's a big mess, as some astronomers might say, but one that a supercomputer can handle.

"It's like more than just bugs on a windshield that we want to remove to see the light, but a storm of bugs all around us in every direction," said Charles Lawrence, the U.S. project scientist for the Planck mission. "Without the exemplary interagency cooperation between NASA and the Department of Energy, Planck would not be doing the science it's doing today."

The computations needed for Planck's current data release required more than 10 million processor-hours on the Hopper computer. Fortunately, the Planck analysis codes run on tens of thousands of processors in the supercomputer at once, so this only took a few weeks.

Read about the newest results from Planck at http://www.jpl.nasa.gov/news/news.php?release=2013-109 .

More information about the National Energy Research Scientific Computing Center is online at: http:///www.nersc.gov/ .

Planck is a European Space Agency mission, with significant participation from NASA. NASA's Planck Project Office is based at JPL. JPL, a division of the California Institute of Technology, Pasadena, contributed mission-enabling technology for both of Planck's science instruments. European, Canadian and U.S. Planck scientists work together to analyze the Planck data. More information is online at http://www.nasa.gov/planck, http://planck.caltech.edu and http://www.esa.int/planck .

Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov


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Planck Mission Brings Universe Into Sharp Focus

JPL/NASA News

News release: 2013-109                                                                    March 21, 2013

Planck Mission Brings Universe Into Sharp Focus

Planck Mission Brings Universe Into Sharp Focus

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-109&cid=release_2013-109

PASADENA, Calif. -- The Planck space mission has released the most accurate and detailed map ever made of the oldest light in the universe, revealing new information about its age, contents and origins.

Planck is a European Space Agency mission. NASA contributed mission-enabling technology for both of Planck's science instruments, and U.S., European and Canadian scientists work together to analyze the Planck data.

The map results suggest the universe is expanding more slowly than scientists thought, and is 13.8 billion years old, 100 million years older than previous estimates. The data also show there is less dark energy and more matter, both normal and dark matter, in the universe than previously known. Dark matter is an invisible substance that can only be seen through the effects of its gravity, while dark energy is pushing our universe apart. The nature of both remains mysterious.

"Astronomers worldwide have been on the edge of their seats waiting for this map," said Joan Centrella, Planck program scientist at NASA Headquarters in Washington. "These measurements are profoundly important to many areas of science, as well as future space missions. We are so pleased to have worked with the European Space Agency on such a historic endeavor."

The map, based on the mission's first 15.5 months of all-sky observations, reveals tiny temperature fluctuations in the cosmic microwave background, ancient light that has traveled for billions of years from the very early universe to reach us. The patterns of light represent the seeds of galaxies and clusters of galaxies we see around us today.

"As that ancient light travels to us, matter acts like an obstacle course getting in its way and changing the patterns slightly," said Charles Lawrence, the U.S. project scientist for Planck at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "The Planck map reveals not only the very young universe, but also matter, including dark matter, everywhere in the universe."

The age, contents and other fundamental traits of our universe are described in a simple model developed by scientists, called the standard model of cosmology. These new data have allowed scientists to test and improve the accuracy of this model with the greatest precision yet. At the same time, some curious features are observed that don't quite fit with the simple picture. For example, the model assumes the sky is the same everywhere, but the light patterns are asymmetrical on two halves of the sky, and there is a spot extending over a patch of sky that is larger than expected.

"On one hand, we have a simple model that fits our observations extremely well, but on the other hand, we see some strange features which force us to rethink some of our basic assumptions," said Jan Tauber, the European Space Agency's Planck project scientist based in the Netherlands. "This is the beginning of a new journey, and we expect our continued analysis of Planck data will help shed light on this conundrum."

The findings also test theories describing inflation, a dramatic expansion of the universe that occurred immediately after its birth. In far less time than it takes to blink an eye, the universe blew up by 100 trillion trillion times in size. The new map, by showing that matter seems to be distributed randomly, suggests that random processes were at play in the very early universe on minute "quantum" scales. This allows scientists to rule out many complex inflation theories in favor of simple ones.

"Patterns over huge patches of sky tell us about what was happening on the tiniest of scales in the moments just after our universe was born," Lawrence said.

Planck launched in 2009 and has been scanning the skies ever since, mapping the cosmic microwave background, the afterglow of the theorized big bang that created our universe. This relic radiation provides scientists with a snapshot of the universe 370,000 years after the big bang. Light existed before this time, but it was locked in a hot plasma similar to a candle flame, which later cooled and set the light free.

The cosmic microwave background is remarkably uniform over the entire sky, but tiny variations reveal the imprints of sound waves triggered by quantum fluctuations in the universe just moments after it was born. These imprints, appearing as splotches in the Planck map, are the seeds from which matter grew, forming stars and galaxies. Prior balloon-based and space missions learned a great deal by studying these patterns, including NASA's Wilkinson Microwave Anisotropy Probe (WMAP) and the Cosmic Background Explorer (COBE), which earned the 2006 Nobel Prize in Physics.

Planck is the successor to these satellites, covering a wider range of light frequencies with improved sensitivity and resolution. Its measurements reveal light patterns as small as one-twelfth of a degree on the sky.

"Planck is like the Ferrari of cosmic microwave background missions," said Krzysztof Gorski, a U.S Planck scientist at JPL. "You fine tune the technology to get more precise results. For a car, that can mean an increase in speed and winning races. For Planck, it results in giving astronomers a treasure trove of spectacular data, and bringing forth a deeper understanding of the properties and history of the universe."

The newly estimated expansion rate of the universe, known as Hubble's constant, is 67.15 plus or minus 1.2 kilometers/second/megaparsec. A megaparsec is roughly 3 million light-years. This is less than prior estimates derived from space telescopes, such as NASA's Spitzer and Hubble, using a different technique. The new estimate of dark matter content in the universe is 26.8 percent, up from 24 percent, while dark energy falls to 68.3 percent, down from 71.4 percent. Normal matter now is 4.9 percent, up from 4.6 percent.

Complete results from Planck, which still is scanning the skies, will be released in 2014.

NASA's Planck Project Office is based at JPL.

More information is online at http://www.nasa.gov/planck, http://planck.caltech.edu and http://www.esa.int/planck.

Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov

J.D. Harrington 202-358-5241
NASA Headquarters, Washington
j.d.harrington@nasa.gov


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Wednesday, March 20, 2013

NASA Voyager Status Update on Voyager 1 Location

JPL/NASA News
News release: 2013-107                                                             March 20, 2013

NASA Voyager Status Update on Voyager 1 Location

NASA Voyager Status Update on Voyager 1 Location

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-107&cid=release_2013-107

"The Voyager team is aware of reports today that NASA's Voyager 1 has left the solar system," said Edward Stone, Voyager project scientist based at the California Institute of Technology, Pasadena, Calif. "It is the consensus of the Voyager science team that Voyager 1 has not yet left the solar system or reached interstellar space. In December 2012, the Voyager science team reported that Voyager 1 is within a new region called 'the magnetic highway' where energetic particles changed dramatically. A change in the direction of the magnetic field is the last critical indicator of reaching interstellar space and that change of direction has not yet been observed."

To learn more about the current status of the Voyager mission: http://www.jpl.nasa.gov/news/news.php?release=2012-381

Jia-Rui C. Cook 818-354-0850
Jet Propulsion Laboratory, Pasadena, Calif.
jccook@jpl.nasa.gov

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Tuesday, March 19, 2013

NASA to Hold News Teleconference to Discuss Planck Cosmology Findings (Update)

JPL/NASA News
News advisory: 2013-105                                                             March 19, 2013

NASA to Hold News Teleconference to Discuss Planck Cosmology Findings (Update)

NASA to Hold News Teleconference to Discuss Planck Cosmology Findings (Update)

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-105&cid=release_2013-105

PASADENA, Calif. -- NASA will host a news teleconference at 8 a.m. PDT (11 a.m. EDT), Thursday, March 21, to discuss the first cosmology results from Planck, a European Space Agency mission with significant NASA participation.

Planck launched into space in 2009 and has been scanning the skies ever since, mapping cosmic microwave background, or the afterglow, of the theoretical big bang that created the universe more than 13 billion years ago. NASA contributed mission-enabling technology for both of Planck's science instruments, and U.S., European and Canadian scientists work together to analyze the Planck data.

The teleconference participants are:

-- Paul Hertz, director of astrophysics, NASA Headquarters, Washington -- Charles Lawrence, U.S. Planck project scientist, NASA's Jet Propulsion Laboratory, Pasadena, Calif. -- Martin White, U.S. Planck scientist, University of California, Berkeley, Calif.; and Faculty Senior Scientist at Lawrence Berkeley Laboratory -- Krzysztof Gorski, U.S. Planck scientist, JPL -- Marc Kamionkowski, professor of physics and astronomy, John Hopkins University, Baltimore, Md.

This event previously was scheduled as a televised news conference.

Questions may be submitted via Twitter using the hashtag #AskNASA .

Visuals will be posted at the start of the teleconference on NASA's Planck website: http://www.nasa.gov/planck .

Audio of the teleconference will be streamed live on NASA's website at: http://www.nasa.gov/newsaudio . The event will also be streamed live on Ustream at: http://www.ustream.tv/nasajpl2 .

For additional information about Planck, visit: http://www.esa.int/planck .

Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov

J.D. Harrington 202-358-5241
NASA Headquarters, Washington
j.d.harrington@nasa.gov

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Educator Workshop: How to Think Like a NASA Scientist

JPL/NASA News



Educator Workshop                 March 19, 2013


This is a feature from the NASA/JPL Education Office.



How to Think Like a NASA Scientist: Analyzing Data, Drawing Conclusions

Date: Saturday, April 13, 2013, 8:30 a.m. - 4:30 p.m.

Target audience: Middle and high school science and mathematics educators (but all are welcome)

Location: Theodore von Kármán Auditorium, Jet Propulsion Laboratory, Pasadena, Calif.

Overview: Learn to think like a NASA scientist - and get your students thinking like one, too! This one-day workshop will show you how to teach students to read scientific graphs and draw conclusions based on real NASA data. Experts will discuss current Earth science missions and show how the scientists, themselves, draw conclusions from these data. Participants will also receive science and math application problems to take back and use in the classroom tomorrow.

A registration fee of $25 covers continental breakfast, lunch and snacks. The deadline to register is April 5, 2013.

For more information and to register, visit: http://www.jpl.nasa.gov/education/index.cfm?page=373

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Lunar Reconnaissance Orbiter Sees GRAIL's Explosive Farewell

JPL/NASA News
News feature: 2013-103                                                                       March 19, 2013

Lunar Reconnaissance Orbiter Sees GRAIL's Explosive Farewell

Lunar Reconnaissance Orbiter Sees GRAIL's Explosive Farewell

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-103&cid=release_2013-103

Many spacecraft just fade away, drifting silently through space after their mission is over, but not GRAIL. NASA's twin GRAIL (Gravity Recovery and Interior Laboratory) spacecraft went out in a blaze of glory on Dec. 17, 2012, when they were intentionally crashed into a mountain near the moon's north pole.

The successful mission to study the moon's interior took the plunge to get one last bit of science: with the spacecraft kicking up a cloud of dust and gas with each impact, researchers hoped to discover more about the moon's composition. However, with the moon about 380,000 kilometers (over 236,000 miles) away from Earth, the impact plumes would be difficult to observe from here. Fortunately, GRAIL had company. NASA's Lunar Reconnaissance Orbiter (LRO) is orbiting the moon as well, busily making high-resolution maps of the lunar surface. With just three weeks notice, the LRO team scrambled to get their orbiter in the right place at the right time to witness GRAIL's fiery finale.

"We were informed by the GRAIL team about three weeks prior to the impact exactly where the impact site would be," said LRO Project Scientist John Keller of NASA's Goddard Space Flight Center in Greenbelt, Md. "The GRAIL team's focus was on obtaining the highest-resolution gravity measurements possible from the last few orbits of the GRAIL spacecraft, which led to uncertainty in the ultimate impact site until relatively late."

LRO was only about 100 miles (160 kilometers) from the lunar surface at the time of the impact, and variations in gravity from massive features like lunar mountains tugged on the spacecraft, altering its orbit.

The site was in shadow at the time of the impact, so the LRO team had to wait until the plumes rose high enough to be in sunlight before making the observation. The Lyman Alpha Mapping Project (LAMP), an ultraviolet imaging spectrograph on board the spacecraft, saw mercury and enhancements of atomic hydrogen in the plume.

"The mercury observation is consistent with what the LRO team saw from the LCROSS impact in October 2009," said Keller. "LCROSS (Lunar CRater Observation and Sensing Satellite) saw significant amounts of mercury, but the LCROSS site was at the bottom of the moon's Cabeus crater, which hasn't seen sunlight for more than a billion years and is therefore extremely cold."

LRO's Lunar Reconnaissance Orbiter Camera was able to make an image of the craters from the GRAIL impacts despite their relatively small size.

The two spacecraft were relatively small -- cubes about the size of a washing machine with a mass of about 200 kilograms (440 pounds) each at the time of impact. The spacecraft were traveling about 3,800 mph (6,100 kilometers per hour) when they hit the surface.

"Both craters are relatively small, perhaps 4 to 6 meters (about 13 to 20 feet) in diameter and both have faint, dark, ejecta patterns, which is unusual," said Mark Robinson, LROC principal investigator at Arizona State University's School of Earth and Space Sciences, Tempe, Ariz. "Fresh impact craters on the moon are typically bright, but these may be dark due to spacecraft material being mixed with the ejecta."

"Both impact sites lie on the southern slope of an unnamed massif [mountain] that lies south of the crater Mouchez and northeast of the crater Philolaus," said Robinson. "The massif stands as much as 2,500 meters [about 8,202 feet] above the surrounding plains. The impact sites are at an elevation of about 700 meters [around 2,296 feet] and 1,000 meters [3,281 feet], respectively, about 500 to 800 meters [approximately 1,640 to 2,625 feet] below the summit. The two impact craters are about 2,200 meters [roughly 7,218 feet] apart. GRAIL B [renamed Flow] impacted about 30 seconds after GRAIL A [Ebb] at a site to the west and north of GRAIL A."

Lunar Reconnaissance Orbiter complemented the GRAIL mission in other ways as well. LRO's Diviner lunar radiometer observed the impact site and confirmed that the amount of heating of the surface there by the relatively small GRAIL spacecraft was within expectations. LRO's Lunar Orbiter Laser Altimeter (LOLA) instrument bounced laser pulses off the surface to build up a precise map of the lunar terrain, including the three-dimensional structure of features like mountains and craters.

"Combining the LRO LOLA topography map with GRAIL's gravity map yields some very interesting results," said Keller. "You expect that areas with mountains will have a little stronger gravity, while features like craters will have a little less. However, when you subtract out the topography, you get another map that reveals gravity differences that are not tied to the surface. It gives insight into structures deeper in the moon's interior."

JPL manages the GRAIL mission for NASA's Science Mission Directorate in Washington. GRAIL is part of the Discovery Program managed at NASA's Marshall Space Flight Center in Huntsville, Ala. Lockheed Martin Space Systems in Denver built the spacecraft.

For the mission's press kit and other information about GRAIL, visit: http://www.nasa.gov/grail . You can follow JPL News on Facebook at: http://www.facebook.com/nasajpl and on Twitter at: http://www.twitter.com/nasajpl .

The research was funded by the LRO mission, currently under NASA's Science Mission Directorate at NASA Headquarters in Washington. LRO is managed by NASA's Goddard Space Flight Center in Greenbelt, Md.

Images are posted at: http://www.nasa.gov/mission_pages/LRO/news/grail-results.html

DC Agle (818) 393-9011
Jet Propulsion Laboratory, Pasadena, Calif.
agle@jpl.nasa.gov

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Herschel Discovers Some of the Youngest Stars Ever Seen

JPL/NASA News

News release: 2013-102                                                                    March 19, 2013

Herschel Discovers Some of the Youngest Stars Ever Seen

Herschel Discovers Some of the Youngest Stars Ever Seen

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-102&cid=release_2013-102

PASADENA, Calif. - Astronomers have found some of the youngest stars ever seen, thanks to the Herschel space observatory, a European Space Agency mission with important NASA contributions.

Observations from NASA's Spitzer Space Telescope and the Atacama Pathfinder Experiment (APEX) telescope in Chile, a collaboration involving the Max Planck Institute for Radio Astronomy in Germany, the Onsala Space Observatory in Sweden, and the European Southern Observatory in Germany, contributed to the findings.

Dense envelopes of gas and dust surround the fledging stars known as protostars, making their detection difficult. The 15 newly observed protostars turned up by surprise in a survey of the biggest site of star formation near our solar system, located in the constellation Orion. The discovery gives scientists a peek into one of the earliest and least understood phases of star formation.

"Herschel has revealed the largest ensemble of such young stars in a single star-forming region," said Amelia Stutz, lead author of a paper to be published in The Astrophysical Journal and a postdoctoral researcher at the Max Planck Institute for Astronomy in Heidelberg, Germany. "With these results, we are getting closer to witnessing the moment when a star begins to form."

Stars spring to life from the gravitational collapse of massive clouds of gas and dust. This changeover from stray, cool gas to the ball of super-hot plasma we call a star is relatively quick by cosmic standards, lasting only a few hundred thousand years. Finding protostars in their earliest, most short-lived and dimmest stages poses a challenge.

Astronomers long had investigated the stellar nursery in the Orion Molecular Cloud Complex, a vast collection of star-forming clouds, but had not seen the newly identified protostars until Herschel observed the region.

"Previous studies have missed the densest, youngest and potentially most extreme and cold protostars in Orion," Stutz said. "These sources may be able to help us better understand how the process of star formation proceeds at the very earliest stages, when most of the stellar mass is built up and physical conditions are hardest to observe."

Herschel spied the protostars in far-infrared, or long-wavelength, light, which can shine through the dense clouds around burgeoning stars that block out higher-energy, shorter wavelengths, including the light our eyes see.

The Herschel Photodetector Array Camera and Spectrometer (PACS) instrument collected infrared light at 70 and 160 micrometers in wavelength, comparable to the width of a human hair. Researchers compared these observations to previous scans of the star-forming regions in Orion taken by Spitzer. Extremely young protostars identified in the Herschel views but too cold to be picked up in most of the Spitzer data were further verified with radio wave observations from the APEX ground telescope.

"Our observations provide a first glimpse at protostars that have just begun to 'glow' at far-infrared wavelengths," said paper coauthor Elise Furlan, a postdoctoral research associate at the National Optical Astronomy Observatory in Tucson, Ariz.

Of the 15 newly discovered protostars, 11 possess very red colors, meaning their light output trends toward the low-energy end of the electromagnetic spectrum. This output indicates the stars are still embedded deeply in a gaseous envelope, meaning they are very young. An additional seven protostars previously seen by Spitzer share this characteristic. Together, these 18 budding stars comprise only five percent of the protostars and candidate protostars observed in Orion. That figure implies the very youngest stars spend perhaps 25,000 years in this phase of their development, a mere blink of an eye considering a star like our sun lives for about 10 billion years.

Researchers hope to document chronologically each stage of a star's development rather like a family album, from before birth to early infancy, when planets also take shape.

"With these recent findings, we add an important missing photo to the family album of stellar development," said Glenn Wahlgren, Herschel Program Scientist at NASA Headquarters in Washington. "Herschel has allowed us to study stars in their infancy."

Herschel is a European Space Agency mission, with science instruments provided by a consortia of European institutes with important participation by NASA. NASA's Herschel Project Office is based at the agency's Jet Propulsion Laboratory in Pasadena, Calif. JPL is a division of the California Institute of Technology, Pasadena.

For more about Herschel, visit: http://www.nasa.gov/herschel , http://www.esa.int/SPECIALS/Herschel/index.html and http://www.herschel.caltech.edu .

Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov

J.D. Harrington 202-358-5241
NASA Headquarters, Washington
j.d.harrington@nasa.gov


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Monday, March 18, 2013

Curiosity Mars Rover Sees Trend in Water Presence

JPL/NASA News

News release: 2013-099                                                                    March. 18, 2013

Curiosity Mars Rover Sees Trend in Water Presence

Curiosity Mars Rover Sees Trend in Water Presence

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-099&cid=release_2013-099

THE WOODLANDS, Texas - NASA's Mars rover Curiosity has seen evidence of water-bearing minerals in rocks near where it had already found clay minerals inside a drilled rock.

Last week, the rover's science team announced that analysis of powder from a drilled mudstone rock on Mars indicates past environmental conditions that were favorable for microbial life. Additional findings presented today (March 18) at a news briefing at the Lunar and Planetary Science Conference in The Woodlands, Texas, suggest those conditions extended beyond the site of the drilling.

Using infrared-imaging capability of a camera on the rover and an instrument that shoots neutrons into the ground to probe for hydrogen, researchers have found more hydration of minerals near the clay-bearing rock than at locations Curiosity visited earlier.

The rover's Mast Camera (Mastcam) can also serve as a mineral-detecting and hydration-detecting tool, reported Jim Bell of Arizona State University, Tempe. "Some iron-bearing rocks and minerals can be detected and mapped using the Mastcam's near-infrared filters."

Ratios of brightness in different Mastcam near-infrared wavelengths can indicate the presence of some hydrated minerals. The technique was used to check rocks in the "Yellowknife Bay" area where Curiosity's drill last month collected the first powder from the interior of a rock on Mars. Some rocks in Yellowknife Bay are crisscrossed with bright veins.

"With Mastcam, we see elevated hydration signals in the narrow veins that cut many of the rocks in this area," said Melissa Rice of the California Institute of Technology, Pasadena. "These bright veins contain hydrated minerals that are different from the clay minerals in the surrounding rock matrix."

The Russian-made Dynamic Albedo of Neutrons (DAN) instrument on Curiosity detects hydrogen beneath the rover. At the rover's very dry study area on Mars, the detected hydrogen is mainly in water molecules bound into minerals. "We definitely see signal variation along the traverse from the landing point to Yellowknife Bay," said DAN Deputy Principal Investigator Maxim Litvak of the Space Research Institute, Moscow. "More water is detected at Yellowknife Bay than earlier on the route. Even within Yellowknife Bay, we see significant variation."

Findings presented today from the Canadian-made Alpha Particle X-ray Spectrometer (APXS) on Curiosity's arm indicate that the wet environmental processes that produced clay at Yellowknife Bay did so without much change in the overall mix of chemical elements present. The elemental composition of the outcrop Curiosity drilled into matches the composition of basalt. For example, it has basalt-like proportions of silicon, aluminum, magnesium and iron. Basalt is the most common rock type on Mars. It is igneous, but it is also thought to be the parent material for sedimentary rocks Curiosity has examined.

"The elemental composition of rocks in Yellowknife Bay wasn't changed much by mineral alteration," said Curiosity science team member Mariek Schmidt of Brock University, Saint Catharines, Ontario, Canada.

A dust coating on rocks had made the composition detected by APXS not quite a match for basalt until Curiosity used a brush to sweep the dust away. After that, APXS saw less sulfur.

"By removing the dust, we've got a better reading that pushes the classification toward basaltic composition," Schmidt said. The sedimentary rocks at Yellowknife Bay likely formed when original basaltic rocks were broken into fragments, transported, re-deposited as sedimentary particles, and mineralogically altered by exposure to water.

NASA's Mars Science Laboratory Project is using Curiosity to investigate whether an area within Mars' Gale Crater has ever offered an environment favorable for microbial life. Curiosity, carrying 10 science instruments, landed seven months ago to begin its two-year prime mission. NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the project for NASA's Science Mission Directorate in Washington.

For more about the mission, visit: http://www.jpl.nasa.gov/msl , http://marsprogram.jpl.nasa.gov/msl and http://www.nasa.gov/msl .

You can follow the mission on Facebook and Twitter at: http://www.facebook.com/marscuriosity and http://www.twitter.com/marscuriosity .

Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov


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