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Thursday, April 4, 2013

Gravity-Bending Find Leads to Kepler Meeting Einstein

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

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

News feature: 2013-124 April 4, 2013

Gravity-Bending Find Leads to Kepler Meeting Einstein

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-124&cid=release_2013-124

NASA's Kepler space telescope has witnessed the effects of a dead star bending the light of its companion star. The findings are among the first detections of this phenomenon -- a result of Einstein's theory of general relativity -- in binary, or double, star systems.

The dead star, called a white dwarf, is the burnt-out core of what used to be a star like our sun. It is locked in an orbiting dance with its partner, a small "red dwarf" star. While the tiny white dwarf is physically smaller than the red dwarf, it is more massive.

"This white dwarf is about the size of Earth but has the mass of the sun," said Phil Muirhead of the California Institute of Technology, Pasadena, lead author of the findings to be published April 20 in the Astrophysical Journal. "It's so hefty that the red dwarf, though larger in physical size, is circling around the white dwarf."

Kepler's primary job is to scan stars in search of orbiting planets. As the planets pass by, they block the starlight by miniscule amounts, which Kepler's sensitive detectors can see.

"The technique is equivalent to spotting a flea on a light bulb 3,000 miles away, roughly the distance from Los Angeles to New York City," said Avi Shporer, co-author of the study, also of Caltech.

Muirhead and his colleagues regularly use public Kepler data to search for and confirm planets around smaller stars, the red dwarfs, also known as M dwarfs. These stars are cooler and redder than our yellow sun. When the team first looked at the Kepler data for a target called KOI-256, they thought they were looking at a huge gas giant planet eclipsing the red dwarf.

"We saw what appeared to be huge dips in the light from the star, and suspected it was from a giant planet, roughly the size of Jupiter, passing in front," said Muirhead.

To learn more about the star system, Muirhead and his colleagues turned to the Hale Telescope at Palomar Observatory near San Diego. Using a technique called radial velocity, they discovered that the red dwarf was wobbling around like a spinning top. The wobble was far too big to be caused by the tug of a planet. That is when they knew they were looking at a massive white dwarf passing behind the red dwarf, rather than a gas giant passing in front.

The team also incorporated ultraviolet measurements of KOI-256 taken by the Galaxy Evolution Explorer (GALEX), a NASA space telescope now operated by the California Institute of Technology in Pasadena. The GALEX observations, led by Cornell University, Ithaca, N.Y., are part of an ongoing program to measure ultraviolet activity in all the stars in Kepler field of view, an indicator of potential habitability for planets in the systems. These data revealed the red dwarf is very active, consistent with being "spun-up" by the orbit of the more massive white dwarf.  

The astronomers then went back to the Kepler data and were surprised by what they saw. When the white dwarf passed in front of its star, its gravity caused the starlight to bend and brighten by measurable effects.

"Only Kepler could detect this tiny, tiny effect," said Doug Hudgins, the Kepler program scientist at NASA Headquarters, Washington. "But with this detection, we are witnessing Einstein's theory of general relativity at play in a far-flung star system."

One of the consequences of Einstein's theory of general relativity is that gravity bends light. Astronomers regularly observe this phenomenon, often called gravitational lensing, in our galaxy and beyond. For example, the light from a distant galaxy can be bent and magnified by matter in front of it. This reveals new information about dark matter and dark energy, two mysterious ingredients in our universe.

Gravitational lensing has also been used to discover new planets and hunt for free-floating planets.

In the new Kepler study, scientists used the gravitational lensing to determine the mass of the white dwarf. By combining this information with all the data they acquired, the scientists were also able to measure accurately the mass of the red dwarf and the physical sizes of both stars. Kepler's data and Einstein's theory of relativity have together led to a better understanding of how binary stars evolve.

Other authors include Andrew Vanderburg of the University of California, Berkeley; Avi Shporer, Juliette Becker, Jonathan J. Swift, Sasha Hinkley, J. Sebastian Pineda, Michael Bottom, Christoph Baranec, Reed Riddle, Shriharsh P. Tendulkar, Khanh Bui, Richard Dekany and John Asher Johnson of Caltech; James P. Lloyd and Jim Fuller of Cornell University; Ming Zhao of The Pennsylvania State University, University Park; Andrew W. Howard of University of Hawaii, Hilo; Kaspar von Braun of the Max Planck Institute for Astronomy, Germany; Tabetha S. Boyajian of Yale University, New Haven, Conn.; Nicholas Law of the University of Toronto, Canada; A. N. Ramaprakash, Mahesh Burse, Pravin Chordia, Hillol Das and Sujit Punnadi of the Inter-University Centre for Astronomy & Astrophysics, India.

NASA Ames manages Kepler's ground system development, mission operations and science data analysis. NASA's Jet Propulsion Laboratory in Pasadena, Calif., managed Kepler mission development. Ball Aerospace and Technologies Corp. in Boulder, Colo., developed the Kepler flight system and supports mission operations with JPL at the Laboratory for Atmospheric and Space Physics at the University of Colorado in Boulder. The Space Telescope Science Institute in Baltimore archives, hosts and distributes the Kepler science data. Kepler is NASA's 10th Discovery Mission and is funded by NASA's Science Mission Directorate at the agency's headquarters. JPL is a division of Caltech.

For more information about the Kepler mission, visit: http://www.nasa.gov/kepler .

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Wednesday, April 3, 2013

Used Parachute on Mars Flaps in the Wind

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 PHONE 818-354-5011
http://www.jpl.nasa.gov

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

Image advisory: 2013-121 April 3, 2013

Used Parachute on Mars Flaps in the Wind

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-121&cid=release_2013-121

PASADENA, Calif. – Photos from NASA's Mars Reconnaissance Orbiter show how the parachute that helped NASA's Curiosity rover land on Mars last summer has subsequently changed its shape on the ground.

The images were obtained by the High Resolution Imaging Science Experiment (HiRISE) camera on Mars Reconnaissance Orbiter.

Seven images taken by HiRISE between Aug. 12, 2012, and Jan. 13, 2013, show the used parachute shifting its shape at least twice in response to wind.

The images in the sequence of photos are available online at http://uahirise.org/releases/msl-chute.php and at http://www.jpl.nasa.gov/spaceimages/details.php?id=PIA16813 .

Researchers have used HiRISE to study many types of changes on Mars. Its first image of Curiosity's parachute, not included in this series, caught the spacecraft suspended from the chute during descent through the Martian atmosphere.

HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo. The Mars Reconnaissance Orbiter Project and Curiosity are managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena.

For more information about the Mars Reconnaissance Orbiter, which has been studying Mars from orbit since 2006, visit http://www.nasa.gov/mro .


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NASA Flies Radar South on Wide-Ranging Expedition

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 PHONE 818-354-5011
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Alan Buis 818-354-0474
Jet Propulsion Laboratory, Pasadena, Calif.
Alan.buis@jpl.nasa.gov

Steve Cole 202-358-0918
NASA Headquarters, Washington
Stephen.e.cole@nasa.gov

News release: 2013-123 April 3, 2013

NASA Flies Radar South on Wide-Ranging Expedition

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-123&cid=release_2013-123

PASADENA, Calif. – A versatile NASA airborne imaging radar system is showcasing its broad scientific prowess for studying our home planet during a month-long expedition over the Americas.

A NASA C-20A piloted aircraft carrying the Uninhabited Aerial Vehicle Synthetic Aperture Radar (UAVSAR) is wrapping up studies over the U.S. Gulf Coast, Arizona, and Central and South America. The plane left NASA's Dryden Aircraft Operations Facility in Palmdale, Calif., on March 7. NASA's Jet Propulsion Laboratory, Pasadena, Calif., built and manages UAVSAR.

The campaign is addressing a broad range of science questions, from the dynamics of Earth's crust and glaciers to the carbon cycle and the lives of ancient Peruvian civilizations. Flights are being conducted over Argentina, Bolivia, Chile, Colombia, Costa Rica, El Salvador, Ecuador, Guatemala, Honduras, Nicaragua and Peru.

UAVSAR uses a technique called interferometry that sends microwave energy pulses from the sensor on the aircraft to the ground. This technique can detect and measure subtle changes in Earth's surface, such as those caused by earthquakes, volcanoes, landslides and glacier movements. The radar's L-band microwaves can penetrate clouds and the tops of forests, making it valuable for studying cloud-covered tropical environments and mapping flooded ecosystems.

"This campaign highlights UAVSAR's versatility for Earth studies," said Naiara Pinto, UAVSAR science coordinator at JPL. "In many cases, study sites are being used by multiple investigators. For example, some volcanic sites also have glaciers. The studies also help U.S. researchers establish and broaden scientific collaborations with Latin America."

Volcano scientists will compare UAVSAR's images taken during this campaign with new imagery collected in 2014 to measure very subtle sub-centimeter changes in Earth's surface associated with the movement of magma deep beneath active volcanoes. These results are expected to improve models used to understand and potentially mitigate volcanic hazards. The volcanoes being studied are in Argentina, Bolivia, Chile, Colombia, Costa Rica, Ecuador, El Salvador, Guatemala, Nicaragua and Peru.

UAVSAR glacier data from South America's Andes Mountains will be combined with ground measurements and airborne lidar data to determine how much these glaciers move during summer and from year to year. The U.S. Geological Survey is leading the collaborative project with the Chilean government to understand glacier processes within the context of climate change impacts from human activities. The glaciers being imaged by UAVSAR provide freshwater for the residents of Santiago and water for regional agriculture.

This year's study sites include coastal mangroves in Central and South America. "Much of Earth's population lives along coasts, and its livelihood and well-being depend on services provided by marine ecosystems," said JPL's Marc Simard, one of the campaign's many principal investigators. "These regions are among the most fragile on Earth. It is critical to understand how the interactions of human activities and climate change may impact the sustainability of these ecosystems."

Another principal investigator, Kyle McDonald, jointly of JPL and the City University of New York Cooperative Remote Sensing Science and Technology Center (CREST) Institute, is leading four data collections that will support the mapping of wetlands across the greater Amazon River basin, including Pacaya-Samiria National Park in Peru. "Pacaya-Samiria contains large expanses of flooded palm swamps," McDonald said. "These ecosystems are potential major sources of atmospheric methane, an important greenhouse gas. UAVSAR will help us better understand processes involved with the exchange of methane between Earth's land and atmosphere, and with the contribution of these unique ecosystems to Earth's climate."

UAVSAR also is supporting agricultural studies of vineyards in Chile's La Serena region. The efforts will help scientists at the Universidad de La Serena's Terra Pacific Group better understand the value of soil moisture data in grape and wine production. Another study site in Argentina will be overflown by both UAVSAR and the Argentine sensor SARAT as part of a collaboration between research scientist Thomas Jackson of the U.S. Department of Agriculture and Argentina's Comision Nacional de Actividades Espaciales. These studies assist scientists preparing for the launch of NASA's Soil Moisture Active Passive (SMAP) satellite in 2014.

The radar also is imaging the northern coastal Peruvian desert, where the Moche culture lived almost 2,000 years ago. Researchers are using UAVSAR's vegetation and cloud penetrating capabilities to search for unrecorded archaeological features in an attempt to preserve sensitive sites from encroaching civilization.

JPL researcher Sassan Saatchi is using UAVSAR to study the structure, biomass and diversity of tropical cloud forests in the Peruvian Andes and Manu National Park, continuing his work there during the past decade. The data will be used to evaluate how much carbon the forests contain and assess their vulnerability to human and natural disturbances.

UAVSAR also is monitoring seasonal land subsidence and uplift in groundwater basins in Arizona's Cochise County for the Arizona Department of Water Resources. Other subsidence studies in New Orleans and the Mississippi Delta are aimed at better understanding what causes Gulf Coast subsidence and predicting future subsidence rates. The data can help agencies better manage the protection of infrastructure, including levees in the New Orleans area.

For more information on UAVSAR, visit: http://uavsar.jpl.nasa.gov . For more on NASA's Airborne Science program, visit: http://airbornescience.nasa.gov .

The California Institute of Technology in Pasadena manages JPL for NASA.

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NASA Team Investigates Complex Chemistry at Titan

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

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

James Schalkwyk 650-604-2791
Ames Research Center, Moffett Field, Calif.
james.schalkwyk@nasa.gov

News feature: 2013-120 April 3, 2013

NASA Team Investigates Complex Chemistry at Titan

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-120&cid=release_2013-120

A laboratory experiment at NASA's Jet Propulsion Laboratory, Pasadena, Calif., simulating the atmosphere of Saturn's moon Titan suggests complex organic chemistry that could eventually lead to the building blocks of life extends lower in the atmosphere than previously thought. The results now point out another region on the moon that could brew up prebiotic materials. The paper was published in Nature Communications this week.

"Scientists previously thought that as we got closer to the surface of Titan, the moon's atmospheric chemistry was basically inert and dull," said Murthy Gudipati, the paper's lead author at JPL. "Our experiment shows that's not true. The same kind of light that drives biological chemistry on Earth's surface could also drive chemistry on Titan, even though Titan receives far less light from the sun and is much colder. Titan is not a sleeping giant in the lower atmosphere, but at least half awake in its chemical activity."

Scientists have known since NASA's Voyager mission flew by the Saturn system in the early 1980s that Titan, Saturn's largest moon, has a thick, hazy atmosphere with hydrocarbons, including methane and ethane. These simple organic molecules can develop into smog-like, airborne molecules with carbon-nitrogen-hydrogen bonds, which astronomer Carl Sagan called "tholins."

"We've known that Titan's upper atmosphere is hospitable to the formation of complex organic molecules," said co-author Mark Allen, principal investigator of the JPL Titan team that is a part of the NASA Astrobiology Institute, headquartered at Ames Research Center, Moffett Field, Calif. "Now we know that sunlight in the Titan lower atmosphere can kick-start more complex organic chemistry in liquids and solids rather than just in gases."

The team examined an ice form of dicyanoacetylene -- a molecule detected on Titan that is related to a compound that turned brown after being exposed to ambient light in Allen's lab 40 years ago.

In this latest experiment, dicyanoacetylene was exposed to laser light at wavelengths as long as 355 nanometers. Light of that wavelength can filter down to Titan's lower atmosphere at a modest intensity, somewhat like the amount of light that comes through protective glasses when Earthlings view a solar eclipse, Gudipati said. The result was the formation of a brownish haze between the two panes of glass containing the experiment, confirming that organic-ice photochemistry at conditions like Titan's lower atmosphere could produce tholins.

The complex organics could coat the "rocks" of water ice at Titan's surface and they could possibly seep through the crust, to a liquid water layer under Titan's surface. In previous laboratory experiments, tholins like these were exposed to liquid water over time and developed into biologically significant molecules, such as amino acids and the nucleotide bases that form RNA.

"These results suggest that the volume of Titan's atmosphere involved in the production of more complex organic chemicals is much larger than previously believed," said Edward Goolish, acting director of NASA's Astrobiology Institute. "This new information makes Titan an even more interesting environment for astrobiological study."

The team included Isabelle Couturier of the University of Provence, Marseille, France; Ronen Jacovi, a NASA postdoctoral fellow from Israel; and Antti Lignell, a Finnish Academy of Science postdoctoral fellow from Helsinki at JPL.

Founded in 1998, the NASA Astrobiology Institute is a partnership between NASA, 15 U.S. teams and 13 international consortia. It is based at NASA Ames Research Center, Moffett Field, Calif. The Institute's goals are to promote, conduct and lead interdisciplinary astrobiology research, train a new generation of astrobiology researchers, and share the excitement of astrobiology with learners of all ages. The NAI is part of NASA's Astrobiology program, which supports research into the origin, evolution, distribution and future of life on Earth and the potential for life elsewhere. For more information, visit http://astrobiology.nasa.gov/.

JPL is a division of the California Institute of Technology, Pasadena.

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Monday, April 1, 2013

NASA Sends Unmanned Aircraft to Study Volcanic Plume

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

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

Ruth Marlaire 650-604-4709
NASA Ames Research Center, Moffett Field, Calif.
Ruth.marlaire@nasa.gov

News feature: 2013-119 April 1, 2013

NASA Sends Unmanned Aircraft to Study Volcanic Plume

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-119&cid=release_2013-119

Studying volcanos can be hazardous work, both for researchers and aircraft. To penetrate such dangerous airspace, unmanned aerial vehicles (UAVs), especially those with electric engines that ingest little contaminated air, are an emerging and effective way to gather crucial data about volcanic ash and gases.

Last month, a team of NASA researchers deployed three repurposed military UAVs with special instruments into and above the noxious sulfur dioxide plume of Costa Rica's active Turrialba volcano, near San Jose. The project was designed to improve the remote-sensing capability of satellites, including satellite data research products such as maps of the concentration and distribution of volcanic gases. It was also designed to improve computer models of how and where volcanic plumes will travel.

Led by principal investigator David Pieri of NASA's Jet Propulsion Laboratory, Pasadena, Calif., the team launched 10 flights of the remote controlled UAVs into the volcanic plume and above the rim of Turrialba's 10,500-foot (3,200-meter) summit crater between March 11 and 14.

The small, twin electric engine Dragon Eye UAVs were acquired by researchers at NASA's Ames Research Center, Moffett Field, Calif., from the United States Marine Corps. Weighing less than six pounds (2.2 kilograms) each and with a wingspan of 3.75 feet (1.1 meters), they have visible and infrared video cameras and can carry a one-pound instrument payload for up to an hour within a volcanic plume. The researchers equipped them with sulfur dioxide and particle sensors and automatic atmospheric sampling bottles keyed to measure sulfur dioxide concentration.

During the flights, the team coordinated its data gathering with NASA's Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) instrument on NASA's Terra spacecraft, allowing scientists to compare sulfur dioxide concentration measurements from the satellite with measurements taken from within the plume.

Scientists believe computer models derived from this study will contribute to safeguarding the National and International Airspace System, and will also improve global climate predictions and mitigate environmental hazards (e.g., sulfur dioxide volcanic smog, or "vog") for people who live near volcanoes.

A key constituent of such models is the intensity and character of the volcanic activity located near the eruption vent. For instance, knowing the height of ash and gas concentrations, and temperatures over the vent during an eruption are important initial factors for any model that predicts the direction of the volcanic plume.

"It is very difficult to gather data from within volcanic eruption columns and plumes because updraft wind speeds are very high and high ash concentrations can quickly destroy aircraft engines," said Pieri. "Such flight environments can be very dangerous to manned aircraft. Volcanic eruption plumes may stretch for miles from a summit vent, and detached ash clouds can drift hundreds to thousands of miles from an eruption site."

The project supports NASA's ASTER mission as well as JPL's planned Hyperspectral Infrared Imager (HyspIRI) satellite mission by improving satellite data-based retrievals of gases and solid aerosols associated with volcanic activity, as well as volcanic emission transport models. HyspIRI will study the world's ecosystems and provide critical information on natural disasters such as volcanoes, assessing their pre-eruptive behavior and the likelihood of future eruptions.

For more information, read the full Ames feature at: http://www.nasa.gov/topics/earth/earthmonth/volcanic-plume-uavs.html . For more on NASA's Airborne Science Program, visit: http://airbornescience.nasa.gov/ . For more on HyspIRI, visit: http://hyspiri.jpl.nasa.gov/ . For more on ASTER, visit: http://asterweb.jpl.nasa.gov/ .

JPL is a division of the California Institute of Technology in Pasadena.


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Thursday, March 28, 2013

REMINDER: Upcoming Educator Workshop - The Challenge of Discovery

Educator Workshop March 28, 2013

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


Educator Workshop: The Challenge of Discovery

Date: Saturday, April 6, 2013

Target audience: K-12 educators

Location/Time:
Jet Propulsion Laboratory, Pasadena, Calif.: 8:30 a.m. - 2:30 p.m. PT
University of Arizona, Tucson, Ariz.: 8:30 - 2:30 p.m. MT
Johnson Space Center, Houston: 10:30 a.m. - 4:30 p.m. CT
Applied Physics Laboratory, Laurel, Md.: 11:30 a.m - 5:30 p.m ET

Overview: What does it take to make a NASA mission happen, and who are the people who drive these tremendous projects?

In the Discovery Program's third annual multi-site professional development workshop, we delve into the stories behind some amazing NASA missions, from conception to science results. Learn how scientists, engineers and mission operators collaborate to meet the challenges of complex missions to assure the science goals are met. Investigate what it takes to move a fantastic idea from dream to reality.

The Challenge of Discovery workshop will take place in four locations (listed above). All sites will offer special speakers, hands-on activities for K-12 and out-of-school-time educators, and resource packets.

The cost of the workshop is $25. Lunch and snacks will be provided.

Learn more and register by April 1 at http://dawn.jpl.nasa.gov/discovery/challenge_of_discovery.asp

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Wednesday, March 27, 2013

Saturn is Like an Antiques Shop, Cassini Suggests

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

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

News feature: 2013-117 March 27, 2013

Saturn is Like an Antiques Shop, Cassini Suggests

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-117&cid=release_2013-117

A new analysis of data from NASA's Cassini spacecraft suggests that Saturn's moons and rings are gently worn vintage goods from around the time of our solar system's birth.

Though they are tinted on the surface from recent "pollution," these bodies date back more than 4 billion years. They are from around the time that the planetary bodies in our neighborhood began to form out of the protoplanetary nebula, the cloud of material still orbiting the sun after its ignition as a star. The paper, led by Gianrico Filacchione, a Cassini participating scientist at Italy's National Institute for Astrophysics, Rome, has just been published online by the Astrophysical Journal.

"Studying the Saturnian system helps us understand the chemical and physical evolution of our entire solar system," said Filacchione. "We know now that understanding this evolution requires not just studying a single moon or ring, but piecing together the relationships intertwining these bodies."

Data from Cassini's visual and infrared mapping spectrometer (VIMS) have revealed how water ice and also colors -- which are the signs of non-water and organic materials --are distributed throughout the Saturnian system. The spectrometer's data in the visible part of the light spectrum show that coloring on the rings and moons generally is only skin-deep.

Using its infrared range, VIMS also detected abundant water ice – too much to have been deposited by comets or other recent means. So the authors deduce that the water ices must have formed around the time of the birth of the solar system, because Saturn orbits the sun beyond the so-called "snow line." Out beyond the snow line, in the outer solar system where Saturn resides, the environment is conducive to preserving water ice, like a deep freezer. Inside the solar system's "snow line," the environment is much closer to the sun's warm glow, and ices and other volatiles dissipate more easily.

The colored patina on the ring particles and moons roughly corresponds to their location in the Saturn system. For Saturn's inner ring particles and moons, water-ice spray from the geyser moon Enceladus has a whitewashing effect.

Farther out, the scientists found that the surfaces of Saturn's moons generally were redder the farther they orbited from Saturn. Phoebe, one of Saturn's outer moons and an object thought to originate in the far-off Kuiper Belt, seems to be shedding reddish dust that eventually rouges the surface of nearby moons, such as Hyperion and Iapetus.

A rain of meteoroids from outside the system appears to have turned some parts of the main ring system – notably the part of the main rings known as the B ring -- a subtle reddish hue. Scientists think the reddish color could be oxidized iron -- rust -- or polycyclic aromatic hydrocarbons, which could be progenitors of more complex organic molecules.

One of the big surprises from this research was the similar reddish coloring of the potato-shaped moon Prometheus and nearby ring particles. Other moons in the area were more whitish.

"The similar reddish tint suggests that Prometheus is constructed from material in Saturn's rings," said co-author Bonnie Buratti, a VIMS team member based at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "Scientists had been wondering whether ring particles could have stuck together to form moons -- since the dominant theory was that the rings basically came from satellites being broken up. The coloring gives us some solid proof that it can work the other way around, too."

"Observing the rings and moons with Cassini gives us an amazing bird's-eye view of the intricate processes at work in the Saturn system, and perhaps in the evolution of planetary systems as well," said Linda Spilker, Cassini project scientist, based at JPL. "What an object looks like and how it evolves depends a lot on location, location, location."

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology, Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The visual and infrared mapping spectrometer team is based at the University of Arizona, Tucson.

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Monday, March 25, 2013

NASA Scientists Find Moon and Asteroids Share Cosmic History

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

Karen Jenvey 650-604-4789
Ames Research Center, Moffett Field, Calif.
karen.jenvey@nasa.gov

News release: 2013-114 March 25, 2013

NASA Scientists Find Moon and Asteroids Share Cosmic History

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-114&cid=release_2013-114

PASADENA, Calif. – NASA and international researchers have discovered that Earth's moon has more in common than previously thought with large asteroids roaming our solar system.

Scientists from NASA's Lunar Science Institute (NLSI) in Moffett Field, Calif., discovered that the same population of high-speed projectiles that impacted our lunar neighbor four billion years ago, also hit the giant asteroid Vesta and perhaps other large asteroids.

The research unveils an unexpected link between Vesta and the moon, and provides new means for studying the early bombardment history of terrestrial planets. The findings are published in the March issue of Nature Geoscience.

"It's always intriguing when interdisciplinary research changes the way we understand the history of our solar system," said Yvonne Pendleton, NLSI director. "Although the moon is located far from Vesta, which is in the main asteroid belt between the orbits of Mars and Jupiter, they seem to share some of the same bombardment history."

The findings support the theory that the repositioning of gas giant planets like Jupiter and Saturn from their original orbits to their current location destabilized portions of the asteroid belt and triggered a solar system-wide bombardment of asteroids billions of years ago, called the lunar cataclysm.

The research provides new constraints on the start and duration of the lunar cataclysm, and demonstrates that the cataclysm was an event that affected not only the inner solar system planets, but the asteroid belt as well.

The moon rocks brought back by NASA Apollo astronauts have long been used to study the bombardment history of the moon. Now the ages derived from meteorite samples have been used to study the collisional history of main belt asteroids. In particular, howardite and eucrite meteorites, which are common species found on Earth, have been used to study asteroid Vesta, their parent body. With the aid of computer simulations, researchers determined that meteorites from Vesta recorded high-speed impacts which are now long gone.

Researchers have linked these two datasets and found that the same population of projectiles responsible for making craters and basins on the moon were also hitting Vesta at very high velocities, enough to leave behind a number of telltale, impact-related ages.

The team's interpretation of the howardites and eucrites was augmented by recent close-in observations of Vesta's surface by NASA's Dawn spacecraft. In addition, the team used the latest dynamical models of early main belt evolution to discover the likely source of these high velocity impactors. The team determined that the population of projectiles that hit Vesta had orbits that also enabled some objects to strike the moon at high speeds.

"It appears that the asteroidal meteorites show signs of the asteroid belt losing a lot of mass four billion years ago, with the escaped mass beating up on both the surviving main belt asteroids and the moon at high speeds" says lead author Simone Marchi, who has a joint appointment between two of NASA's Lunar Science Institutes, one at the Southwest Research Institute in Boulder, Colo., and another at the Lunar and Planetary Institute in Houston. "Our research not only supports the current theory, but it takes it to the next level of understanding."

The NLSI is headquartered at NASA Ames Research Center, Moffett Field, Calif. The Dawn mission to Vesta and Ceres is managed by NASA's Jet Propulsion Laboratory, Pasadena, Calif., for NASA's Science Mission Directorate, Washington. Dawn is a project of the directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville, Ala.

To learn more about NLSI, visit: http://lunarscience.nasa.gov .

For more information about the Dawn mission, visit: www.nasa.gov/dawn .

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Friday, March 22, 2013

JPL Scientists Reflect on World Water Day

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

News feature: 2013-113 March 22, 2013

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.



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Thursday, March 21, 2013

Supercomputer Helps Planck Mission Expose Ancient Light

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
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NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
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Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.clavin@jpl.nasa.gov

News feature: 2013-110 March 21, 2013

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 .

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