Top Stories: October 2012

Wednesday, October 31, 2012

Cassini Halloween Treat: Titan Glows in the Dark

NASA Hosts Nov. 2 Teleconference About Mars Rover Progress

Tuesday, October 30, 2012

NASA Rover's First Soil Studies Help Fingerprint Martian Minerals

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 / D.C. Agle 818-354-5011
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov / agle@jpl.nasa.gov

Rachel Hoover 650-604-4789
NASA Ames Research Center, Moffett Field, Calif.
rachel.hoover@nasa.gov

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

News release: 2012-341 Oct. 30, 2012

NASA Rover's First Soil Studies Help Fingerprint Martian Minerals

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2012-341&cid=release_2012-341

PASADENA, Calif. -- NASA's Mars rover Curiosity has completed initial experiments showing the mineralogy of Martian soil is similar to weathered basaltic soils of volcanic origin in Hawaii.

The minerals were identified in the first sample of Martian soil ingested recently by the rover. Curiosity used its Chemistry and Mineralogy instrument (CheMin) to obtain the results, which are filling gaps and adding confidence to earlier estimates of the mineralogical makeup of the dust and fine soil widespread on the Red Planet.

"We had many previous inferences and discussions about the mineralogy of Martian soil," said David Blake of NASA Ames Research Center in Moffett Field, Calif., who is the principal investigator for CheMin. "Our quantitative results provide refined and in some cases new identifications of the minerals in this first X-ray diffraction analysis on Mars."

The identification of minerals in rocks and soil is crucial for the mission's goal to assess past environmental conditions. Each mineral records the conditions under which it formed. The chemical composition of a rock provides only ambiguous mineralogical information, as in the textbook example of the minerals diamond and graphite, which have the same chemical composition, but strikingly different structures and properties.

CheMin uses X-ray diffraction, the standard practice for geologists on Earth using much larger laboratory instruments. This method provides more accurate identifications of minerals than any method previously used on Mars. X-ray diffraction reads minerals' internal structure by recording how their crystals distinctively interact with X-rays. Innovations from Ames led to an X-ray diffraction instrument compact enough to fit inside the rover.

These NASA technological advances have resulted in other applications on Earth, including compact and portable X-ray diffraction equipment for oil and gas exploration, analysis of archaeological objects and screening of counterfeit pharmaceuticals, among other uses.

"Our team is elated with these first results from our instrument," said Blake. "They heighten our anticipation for future CheMin analyses in the months and miles ahead for Curiosity."

The specific sample for CheMin's first analysis was soil Curiosity scooped up at a patch of dust and sand that the team named Rocknest. The sample was processed through a sieve to exclude particles larger than 0.006 inch (150 micrometers), roughly the width of a human hair. The sample has at least two components: dust distributed globally in dust storms and fine sand originating more locally. Unlike conglomerate rocks Curiosity investigated a few weeks ago, which are several billion years old and indicative of flowing water, the soil material CheMin has analyzed is more representative of modern processes on Mars.

"Much of Mars is covered with dust, and we had an incomplete understanding of its mineralogy," said David Bish, CheMin co-investigator with Indiana University in Bloomington. "We now know it is mineralogically similar to basaltic material, with significant amounts of feldspar, pyroxene and olivine, which was not unexpected. Roughly half the soil is non-crystalline material, such as volcanic glass or products from weathering of the glass. "

Bish said, "So far, the materials Curiosity has analyzed are consistent with our initial ideas of the deposits in Gale Crater recording a transition through time from a wet to dry environment. The ancient rocks, such as the conglomerates, suggest flowing water, while the minerals in the younger soil are consistent with limited interaction with water."

During the two-year prime mission of the Mars Science Laboratory Project, researchers are using Curiosity's 10 instruments to investigate whether areas in Gale Crater ever offered environmental conditions favorable for microbial life.

NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, manages the project for NASA's Science Mission Directorate, Washington, and built Curiosity and CheMin.

For more information about Curiosity and its mission, visit: http://www.nasa.gov/msl and http://mars.jpl.nasa.gov/msl .

For more information about a commercial application of the CheMin technology, visit: http://blogs.getty.edu/iris/mars-rover-technology-helps-unlock-art-mysteries/ .

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

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Friday, October 26, 2012

NASA Oct. 30 Telecon About Mars Curiosity Progress

Thursday, October 25, 2012

NASA Radar Penetrates Thick, Thin of Gulf Oil Spill

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

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

News release: 2012-337 Oct. 25, 2012

NASA Radar Penetrates Thick, Thin of Gulf Oil Spill

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2012-337&cid=release_2012-337

PASADENA, Calif. – Researchers at NASA's Jet Propulsion Laboratory and the California Institute of Technology in Pasadena have developed a method to use a specialized NASA 3-D imaging radar to characterize the oil in oil spills, such as the 2010 BP Deepwater Horizon spill in the Gulf of Mexico. The research can be used to improve response operations during future marine oil spills.

Caltech graduate student Brent Minchew and JPL researchers Cathleen Jones and Ben Holt analyzed NASA radar imagery collected over the main slick of the BP Deepwater Horizon oil spill on June 22 and June 23, 2010. The data were acquired by the JPL-developed Uninhabited Aerial Vehicle Synthetic Aperture Radar (UAVSAR) during the first of its three deployments over the spill area between June 2010 and July 2012. The UAVSAR was carried in a pod mounted beneath a NASA C-20A piloted aircraft, a version of the Gulfstream III business jet, based at NASA's Dryden Aircraft Operations Facility in Palmdale, Calif. The researchers demonstrated, for the first time, that a radar system like UAVSAR can be used to characterize the oil within a slick, distinguishing very thin films like oil sheen from more damaging thick oil emulsions.

"Our research demonstrates the tremendous potential of UAVSAR to automate the classification of oil in a slick and mitigate the effects of future oil spill tragedies," said Jones. "Such information can help spill incidence response commanders direct cleanup operations, such as the mechanical recovery of oil, to the areas of thick oil that would have the most damaging environmental impacts."

Current visual oil classification techniques are qualitative, and depend upon the skill of the people doing the assessment and the availability of skilled observers during an emergency. Remote sensing allows larger areas to be covered in a consistent manner in a shorter amount of time. Radar can be used at night or in other low-light or poor weather conditions when visual surveys can't be conducted.

Radar had previously been used to detect the extent of oil slicks, but not to characterize the oil within them. It had generally been assumed that radar had little to no use for this purpose. The team demonstrated that UAVSAR could be used to identify areas where thick oil had mixed with the surface seawater to form emulsions, which are mixtures of oil and seawater.

Identifying the type of oil in a spill is vital for assessing its potential harm and targeting response efforts. For example, thin oil consists of sheens that measure from less than 0.0002 inches (0.005 millimeters) to about 0.002 inches (0.05 millimeters) thick. Sheens generally form when little oil is released, as in the initial stages of a spill, or from lightweight, volatile components of spill material. Because sheens contain little oil volume, they weather and evaporate quickly, and are of minor concern from an environmental standpoint. Oil emulsions, on the other hand, are 0.04 inches (1 millimeter) thick, contain more oil, and persist on the ocean surface for much longer, thereby potentially having a greater environmental impact in the open sea and along the shoreline.

"Knowing the type of oil tells us a lot about the thickness of the oil in that area," said Jones.

The researchers acquired data in June 2010 along more than 3,400 miles (5,500 kilometers) of flight lines over an area of more than 46,330 square miles (120,000 square kilometers), primarily along the Gulf Coast. They found that at the time the slick was imaged by UAVSAR, much of the surface layer of the Deepwater Horizon spill's main slick consisted of thick oil emulsions.

UAVSAR characterizes an oil spill by detecting variations in the roughness of its surface and, for thick slicks, changes in the electrical conductivity of its surface layer. Just as an airport runway looks smooth compared to surrounding fields, UAVSAR "sees" an oil spill at sea as a smoother (radar-dark) area against the rougher (radar-bright) ocean surface because most of the radar energy that hits the smoother surface is deflected away from the radar antenna. UAVSAR's high sensitivity and other capabilities enabled the team to separate thick and thin oil for the first time using a radar system.

"We knew we were going to detect the extent of the spill," said Holt. "But we had this great new instrument, so we wanted to see how it would work in this extreme situation, and it turned out to be really unique and valuable, beyond all previous radar results for spills."

"We studied an unprecedented event using data collected by a sophisticated instrument and were able to show that there was a lot more information contained in the data than was apparent when we began," said Minchew. "This is a good example of how the tools of science could be used to help mitigate disasters in real time."

UAVSAR is returning to the Gulf of Mexico area this month and will image the area around the Deepwater Horizon site to look for leaks. In the future, UAVSAR data may be combined with imaging spectroscopic data from JPL's Airborne Visible/Infrared Imaging Spectrometer (AVIRIS) instrument to further improve the ability to characterize oil spills under a broader range of environmental conditions.

In addition to characterizing the oil slick, UAVSAR imaged most of the U.S. Gulf of Mexico coastline, extending from the Florida Keys to Corpus Christi, Texas, with extensive inland coverage of the southern Louisiana wetlands around Barataria Bay, the terrestrial ecosystem that ultimately sustained the greatest oiling from the massive spill. Researchers tracked the movement of the oil into coastal waterways and marshlands, monitored impact and recovery of oil-affected wetlands, and assessed how UAVSAR can support emergency responders in future disasters.

UAVSAR is also used to detect detailed Earth movements related to earthquakes, volcanoes and glaciers, as well as for soil moisture and forestry biomass studies. For more on UAVSAR, see: http://uavsar.jpl.nasa.gov/mission_flights.html .

Results of this study are published this month in the Institute of Electrical and Electronics Engineers journal Transactions on Geoscience and Remote Sensing. Caltech manages JPL for NASA.

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NASA's Cassini Sees Burp at Saturn After Large Storm

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

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

Elizabeth Zubritsky/Nancy Neal-Jones 301-614-5438/301-286-0039
Goddard Space Flight, Center, Greenbelt, Md.
elizabeth.a.zubritsky@nasa.gov /nancy.n.jones@nasa.gov

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

News release: 2012-335 Oct. 25, 2012

NASA's Cassini Sees Burp at Saturn After Large Storm

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2012-335&cid=release_2012-335

PASADENA, Calif. -- NASA's Cassini spacecraft has tracked the aftermath of a rare massive storm on Saturn. Data reveal record-setting disturbances in the planet's upper atmosphere long after the visible signs of the storm abated, in addition to an indication the storm was more forceful than scientists previously thought.

Data from Cassini's composite infrared spectrometer (CIRS) instrument revealed the storm's powerful discharge sent the temperature in Saturn's stratosphere soaring 150 degrees Fahrenheit (83 kelvins) above normal. At the same time, researchers at NASA's Goddard Spaceflight Center in Greenbelt, Md., detected a huge increase in the amount of ethylene gas, the origin of which is a mystery. Ethylene, an odorless, colorless gas, isn't typically observed on Saturn. On Earth, it is created by natural and man-made sources.

Goddard scientists describe the unprecedented belch of energy in a paper to be published in the Nov. 20 issue of the Astrophysical Journal.

"This temperature spike is so extreme it's almost unbelievable, especially in this part of Saturn's atmosphere, which typically is very stable," said Brigette Hesman, the study's lead author and a University of Maryland scientist who works at Goddard. "To get a temperature change of the same scale on Earth, you'd be going from the depths of winter in Fairbanks, Alaska, to the height of summer in the Mojave Desert."

First detected by Cassini in Saturn's northern hemisphere on Dec. 5, 2010, the storm grew so large that an equivalent storm on Earth would blanket most of North America from north to south and wrap around our planet many times. This type of giant disturbance on Saturn typically occurs every 30 Earth years, or once every Saturn year.

Not only was this the first storm of its kind to be studied by a spacecraft in orbit around the planet, but it was the first to be observed at thermal infrared wavelengths. Infrared data from CIRS allowed scientists to take the temperature of Saturn's atmosphere and to track phenomena that are invisible to the naked eye.

Temperature measurements by the composite infrared spectrometer, first published in May 2011, revealed two unusual beacons of warmer-than-normal air shining brightly in the stratosphere. These indicated a massive release of energy into the atmosphere. After the visible signs of the storm started to fade, the instrument's data revealed the two beacons had merged. The temperature of this combined air mass shot up to more than minus 64 degrees Fahrenheit (above 220 kelvins).

According to Hesman, the huge spike of ethylene generated at the same time peaked with 100 times more of the gas than scientists thought possible for Saturn. Goddard scientists confirmed the release of ethylene using the Celeste spectrometer mounted on the McMath-Pierce Solar Telescope on Kitt Peak in Arizona.

The team still is exploring the origin of the ethylene, but has ruled out a large reservoir deep in the atmosphere.

"We've really never been able to see ethylene on Saturn before, so this was a complete surprise," said Goddard's Michael Flasar, the CIRS team lead.

A complementary paper led by Cassini team associate Leigh Fletcher of Oxford University, England, describes how the two stratospheric beacons merged to become the largest and hottest stratospheric vortex ever detected in our solar system. Initially, it was larger than Jupiter's Great Red Spot.

Their paper in the journal Icarus, which combines CIRS data with additional infrared images from other Earth-based telescopes, including NASA's Infrared Telescope Facility at Mauna Kea, Hawaii, also reports a powerful collar of clockwise winds -- encompassing a bizarre soup of gases -- around the vortex.

"These studies will give us new insight into some of the photochemical processes at work in the stratospheres of Saturn, other giants in our solar system, and beyond," said Scott Edgington, Cassini deputy project scientist at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency, and the Italian Space Agency. The mission is managed by JPL for NASA's Science Mission Directorate in Washington. Hesman's work was funded in part by NASA's Planetary Astronomy Program in Washington. The CIRS instrument and Celeste spectrometer were built at Goddard. JPL is managed by the California Institute of Technology, Pasadena.

To read more about the Fletcher paper, visit: http://www.esa.int/esaSC/SEMLPIMFL8H_index_0.html .

For information about Cassini and this observation, visit: http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov .

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Wednesday, October 24, 2012

NASA's Spitzer Sees Light of Lonesome Stars

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

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

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

News release: 2012-334 Oct. 24, 2012

NASA's Spitzer Sees Light of Lonesome Stars

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2012-334&cid=release_2012-334

PASADENA, Calif. – A new study using data from NASA's Spitzer Space Telescope suggests a cause for the mysterious glow of infrared light seen across the entire sky. It comes from isolated stars beyond the edges of galaxies. These stars are thought to have once belonged to the galaxies before violent galaxy mergers stripped them away into the relatively empty space outside of their former homes.

"The infrared background glow in our sky has been a huge mystery," said Asantha Cooray of the University of California at Irvine, lead author of the new research published in the journal Nature. "We have new evidence this light is from the stars that linger between galaxies. Individually, the stars are too faint to be seen, but we think we are seeing their collective glow."

The findings disagree with another theory explaining the same background infrared light observed by Spitzer. A group led by Alexander "Sasha" Kashlinsky of NASA's Goddard Space Flight Center in Greenbelt, Md., proposed in June this light, which appears in Spitzer images as a blotchy pattern, is coming from the very first stars and galaxies.

In the new study, Cooray and colleagues looked at data from a larger portion of the sky, called the Bootes field, covering an arc equivalent to 50 full Earth moons. These observations were not as sensitive as those from the Kashlinsky group's studies, but the larger scale allowed researchers to analyze better the pattern of the background infrared light.

"We looked at the Bootes field with Spitzer for 250 hours," said co-author Daniel Stern of NASA's Jet Propulsion Laboratory in Pasadena, Calif. "Studying the faint infrared background was one of the core goals of our survey, and we carefully designed the observations in order to directly address the important, challenging question of what causes the background glow."

The team concluded the light pattern of the infrared glow is not consistent with theories and computer simulations of the first stars and galaxies. Researchers say the glow is too bright to be from the first galaxies, which are thought not to have been as large or as numerous as the galaxies we see around us today. Instead, the scientists propose a new theory to explain the blotchy light, based on theories of "intracluster" or "intrahalo" starlight.

Theories predict a diffuse smattering of stars beyond the halos, or outer reaches, of galaxies, and in the spaces between clusters of galaxies. The presence of these stars can be attributed to two phenomena. Early in the history of our universe as galaxies grew in size, they collided with other galaxies and gained mass. As the colliding galaxies became tangled gravitationally, strips of stars were shredded and tossed into space. Galaxies also grow by swallowing smaller dwarf galaxies, a messy process that also results in stray stars.

"A light bulb went off when reading some research papers predicting the existence of diffuse stars," Cooray said. "They could explain what we are seeing with Spitzer."

More research is needed to confirm this sprinkling of stars makes up a significant fraction of the background infrared light. For instance, it would be necessary to find a similar pattern in follow-up observations in visible light. NASA's upcoming James Webb Space Telescope (JWST) might finally settle the matter for good.

"The keen infrared vision of the James Webb Telescope will be able to see some of the earliest stars and galaxies directly, as well as the stray stars lurking between the outskirts of nearby galaxies," said Eric Smith, JWST's deputy program manager at NASA Headquarters in Washington. "The mystery objects making up the background infrared light may finally be exposed."

Other authors include Joseph Smidt, Francesco De Bernardis, Yan Gong and Christopher C. Frazer of UC Irvine; Matthew L. N. Ashby of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass; Peter R. Eisenhardt of JPL; Anthony H. Gonzalez of the University of Florida in Gainesville; Christopher S. Kochanek of Ohio State University in Columbus; Szymon Koz?owski of Ohio State and the Warsaw University Observatory in Poland; and Edward L. Wright of the University of California, Los Angeles.

JPL manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate in Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology in Pasadena. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech. Caltech manages JPL for NASA.

For more information about Spitzer, visit: http://www.nasa.gov/spitzer .

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Tuesday, October 23, 2012

NASA's NuSTAR Spots Flare From Milky Way's Black Hole

Attend Lunar and Meteorite Sample Certification Workshop at NASA/JPL Educator Resource Center

Educator Workshop Oct. 23, 2012

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

NASA Lunar and Meteorite Sample Certification Program

Date: Saturday, Nov. 10, 2012, 10 a.m. - 12:30 p.m.

Target audience:Recommended for teachers in all grades in a classroom setting

Location: NASA/JPL Educator Resource Center, Pomona, Calif.

Overview: NASA makes actual lunar samples from the historic Apollo missions available to lend to teachers. You must attend this certification workshop to bring the excitement of real lunar rocks and regolith samples to your students. This workshop is being offered at the NASA/JPL Educator Resource Center located in Pomona, please call 909-397-4420 to reserve your spot.

For more information and directions, visit: http://www.jpl.nasa.gov/education/index.cfm?page=115

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Wednesday, October 17, 2012

Could a Hurricane Ever Strike Southern California?

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

News feature: 2012-329 Oct. 17, 2012

Could a Hurricane Ever Strike Southern California?

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2012-329&cid=release_2012-329

There's an old adage (with several variations) that California has four seasons: earthquake, fire, flood and drought. While Californians happily cede the title of Hurricane Capital of America to U.S. East and Gulf coasters, every once in a while, Mother Nature sends a reminder to Southern Californians that they are not completely immune to the whims of tropical cyclones. Typically, this takes the form of rainfall from the remnants of a tropical cyclone in the eastern Pacific, as happened recently when the remnants of Hurricane John brought rain and thunderstorms to parts of Southern California. But could a hurricane ever make landfall in Southern California?

The answer, as it turns out, is yes, and no. While there has never been a documented case of a hurricane making landfall in California, the Golden State has had its share of run-ins and close calls with tropical cyclones. In fact, California has been affected by at least a few tropical cyclones in every decade since 1900. Over that timeframe, three of those storms brought gale-force winds to California: an unnamed California tropical storm in 1939, Kathleen in 1976 and Nora in 1997. But the primary threat from California tropical cyclones isn't winds or storm surge. It's rainfall -- sometimes torrential -- which has led to flooding, damage and, occasionally, casualties.

We asked JPL oceanographer and climatologist Bill Patzert about the prospects for future tropical cyclones in Southern California.

Q. We've passed the September peak of hurricane season in the Atlantic and Eastern Pacific Basins -- a year that has been moderately busy for storms thus far. Of course, Southern Californians don't generally think too much about hurricanes. We worry about earthquakes…wildfires…whether the local teams will make the playoffs. But it seems as though every year or so, we get some rain from a tropical cyclone in Southern California. Which begs the question: could a hurricane ever strike here?

Patzert: The interesting thing is that it really can't happen, statistically speaking. The odds are infinitesimal -- so small that everyone should just relax. Like 1 in 1,000. Of course, there's always a chance. But there's a good reason why we don't name our West Coast sports teams the Hurricanes, but we do have the Rancho Cucamonga Quakes.

Seriously, as eastern Pacific hurricanes move northwest and weaken, what we have had are many instances where they dumped a lot of rainfall in Southern California. That's what happened with two monster storms in 1858 and 1939, both El Nino years. And there have been plenty of other examples. When Southern California does get affected by tropical systems, September is by far the most common month.

Q. So why don't we get hurricanes here?

Patzert: There are two main factors that work against hurricanes here: cool waters off the coast and the direction of the upper-level winds.

Tropical cyclones draw their fuel, so to speak, from heat stored in the upper ocean. Typically, ocean surface waters greater than 80 degrees Fahrenheit (27 degrees Celsius) are required to form and fuel these great storms. During the Northern Hemisphere summer and fall, the upper layers of the tropical oceans (down to approximately 330 feet depth) are steadily heated. By September, when hurricane season hits its peak, these waters reach their maximum temperatures, becoming, in a sense, high-octane fuel for hurricanes. But water temperatures never get that high in the coastal waters north of central Baja California. On rare occasions, they may reach about 75 degrees Fahrenheit (24 degrees Celsius) near the shore in Southern California, typically during an El Nino episode. But generally speaking, low 60s is about as warm as they get farther from shore and elsewhere in coastal California.

In the Pacific Ocean, the North Pacific Current flows from Japan eastward across the Pacific and then splits into the northern-flowing Alaska Current and the southern-flowing California Current. The cool-water California Current, which sweeps down the West Coast of the United States, really acts as hurricane repellant, protecting California and even Northern Baja California from hurricanes.

The other factor at play here is the upper-level winds, which tend to carry and steer storms to the west and northwest, away from California, and also tend to shear the tops off of hurricanes, breaking them apart. Between the upper and lower-level winds, there's a lot of wind shear off the coast here in Southern California. These prevailing northwesterly winds also push warmer surface waters offshore, drawing cooler waters up to the surface, and this further adds to the cool nature of the nearby ocean waters that would weaken any storms that did approach California.

Q. But is there a "Perfect Storm" scenario that would allow a tropical cyclone to have a major impact on Southern California?

Patzert: The best odds for a tropical cyclone to affect Southern California are during a "Godzilla" El Nino event, when the waters off the coast are warmest, like we had in 1997-98 when waters were in the low to mid 70s. Or when we're in the positive phase of the Pacific Decadal Oscillation (PDO), a long-term pattern of change in the Pacific Ocean that alternates between cool and warm periods about every five to 20 years. We're currently in the early stages of a cool phase of the PDO, which tends to dampen the effects of El Ninos. Waters in the eastern Pacific generate more hurricanes during El Nino years.

In addition, the upper-level winds would have to steer an unusually strong storm our way. That almost happened with Hurricane Linda in 1997, which briefly threatened Southern California before turning away to sea. But even if Linda had made landfall in California, it wouldn't have been a big wind event. It would have been more like an "atmospheric river" event, common in wintertime, with heavy rainfall and flooding. And storm surge, which is a big concern along the U.S. Gulf and East coasts, is really a negligible issue along most of the California coast, because much of it sits atop bluffs, above sea level.

Q. So how is this hurricane season shaping up in the Pacific and Atlantic?

Patzert: This hurricane season has been moderately active in the eastern Pacific and slightly busier than normal in the Atlantic, but there have been very few big storms. And locally, our current water temperatures off the Southern California coast are between 65 and 70 degrees Fahrenheit [18 and 21 degrees Celsius]. That's way too cold for hurricanes.

Q. Some scientists believe as Earth's climate gets warmer, the frequency and intensity of hurricanes may increase, though the jury is still out on that matter. Do you believe climate change will increase the odds of hurricanes affecting Southern California?

Patzert: Nobody knows yet, and if anybody tells you they know the answer to that question, kick 'em out of your Rolodex file. In fact it's possible that there might be fewer hurricanes in a warming world. But the bottom line for Southern Californians is that even if global temperatures were to rise six degrees, a hurricane in California would rank very low on the list of things we'd need to worry about.

Q. The winter of 1938-39 was something of a freak one for California, with multiple tropical cyclones and other storms affecting the state during the El Nino of 1938-39, resulting in major damage and a large number of fatalities. How have things changed in Southern California in terms of preparation for major storms since then?

Patzert: Anytime you get too much rain too quick, it can cause damage and death, as we saw in the winter of 1938-39. But remember that was before we had a reliable observation network, based on ground and copious satellite measurements, which provided for useful forecasts and warnings. In addition, Southern Californians are flood resistant now because of those storms in 1938-39, which led to all the major rivers here being concreted. So we're largely immunized against these kinds of catastrophic flooding events now.

Q. Do tropical cyclones have a significant impact on Southern California's annual rainfall?

Patzert: In the Southeastern United States, an awful lot of the annual water budget comes from tropical storms, which can have a positive impact as drought busters. But tropical cyclones are not a significant contributor to our rainfall here in Southern California. The average rainfall in Los Angeles in September, even with rainfall from occasional tropical cyclones, is less than half an inch. These amounts are small compared to our normal winter total of 15.1 inches (31 centimeters). But we would certainly welcome any rainfall we can get in September and October, because it can help trump the effects of the hot, dry Santa Ana winds and their associated fire threat. And those are far more real threats to Californians than hurricanes will ever be.

For a brief overview of a few of the more notable tropical cyclones to have affected Southern California in recorded history, visit: http://www.nasa.gov/topics/earth/features/earth20121017.html .

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Jupiter: Turmoil from Below, Battering from Above

Tuesday, October 16, 2012

Columbia Memorial Space Center to Host Free NASA/JPL Teacher Workshop

Educator Workshop Oct. 16, 2012

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

NASA/JPL Teacher Workshop: Go For Flight!

Date: Saturday, Oct. 27, 2012, 10 a.m. - 12 p.m.

Target audience: Teachers and pre-service teachers

Location: Columbia Memorial Space Center, 12400 Columbia Way, Downey, Calif.

Overview: Learn about the four forces of flight, math and the physics of gliders, helicopters, kites and rockets! Learn about the basic principles of flight. Conduct scientific experiments and construct aircraft models (kite, helicopter and glider). Use questioning and redesign to make these activities educationally challenging! RSVP required, call the Columbia Memorial Space Center at 562-231-1200 to save your spot!

For more information and directions, visit: http://bit.ly/Nl1DTV

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NASA to Host Mars Curiosity Rover Teleconference Oct. 18

What's Baking on Titan?

Monday, October 15, 2012

A Long and Winding Road: Cassini Celebrates 15 Years

NASA's WISE Colors in Unknowns on Jupiter Asteroids

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: 2012-322 Oct. 15, 2012

NASA's WISE Colors in Unknowns on Jupiter Asteroids

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2012-322&cid=release_2012-322

Scientists using data from NASA's Wide-field Infrared Survey Explorer, or WISE, have uncovered
new clues in the ongoing mystery of the Jovian Trojans -- asteroids that orbit the sun on the same
path as Jupiter. Like racehorses, the asteroids travel in packs, with one group leading the way in front
of the gas giant, and a second group trailing behind.

The observations are the first to get a detailed look at the Trojans' colors: both the leading and
trailing packs are made up of predominantly dark, reddish rocks with a matte, non-reflecting surface.
What's more, the data verify the previous suspicion that the leading pack of Trojans outnumbers the
trailing bunch.

The new results offer clues in the puzzle of the asteroids' origins. Where did the Trojans come from?
What are they made of? WISE has shown that the two packs of rocks are strikingly similar and do not
harbor any "out-of-towners," or interlopers, from other parts of the solar system. The Trojans do not
resemble the asteroids from the main belt between Mars and Jupiter, nor the Kuiper belt family of
objects from the icier, outer regions near Pluto.

"Jupiter and Saturn are in calm, stable orbits today, but in their past, they rumbled around and
disrupted any asteroids that were in orbit with these planets," said Tommy Grav, a WISE scientist
from the Planetary Science Institute in Tucson, Ariz. "Later, Jupiter re-captured the Trojan asteroids,
but we don't know where they came from. Our results suggest they may have been captured locally. If
so, that's exciting because it means these asteroids could be made of primordial material from this
particular part of the solar system, something we don't know much about." Grav is a member of the
NEOWISE team, the asteroid-hunting portion of the WISE mission.

The first Trojan was discovered on Feb. 22, 1906, by German astronomer Max Wolf, who found the
celestial object leading ahead of Jupiter. Christened "Achilles" by the astronomer, the roughly 220-
mile-wide (350-kilometer-wide) chunk of space rock was the first of many asteroids detected to be
traveling in front of the gas giant. Later, asteroids were also found trailing behind Jupiter. The
asteroids were collectively named Trojans after a legend, in which Greek soldiers hid inside in a giant
horse statue to launch a surprise attack on the Trojan people of the city of Troy.

"The two asteroid camps even have their own 'spy,'" said Grav. "After having discovered a handful of
Trojans, astronomers decided to name the asteroid in the leading camp after the Greek heroes and the
ones in the trailing after the heroes of Troy. But each of the camps already had an 'enemy' in their
midst, with asteroid 'Hector' in the Greek camp and 'Patroclus' in the Trojan camp."

Other planets were later found to have Trojan asteroids riding along with them too, such as Mars,
Neptune and even Earth, where WISE recently found the first known Earth Trojan:
http://www.jpl.nasa.gov/news/news.php?release=2011-230 .

Before WISE, the main uncertainty defining the population of Jupiter Trojans was just how many
individual chunks were in these clouds of space rock and ice leading Jupiter, and how many were
trailing. It is believed that there are as many objects in these two swarms leading and trailing Jupiter
as there are in the entirety of the main asteroid belt between Mars and Jupiter.

To put this and other theories to bed requires a well-coordinated, well-executed observational
campaign. But there were many things in the way of accurate observations -- chiefly, Jupiter itself.
The orientation of these Jovian asteroid clouds in the sky in the last few decades has been an
impediment to observations. One cloud is predominantly in Earth's northern sky, while the other is in
the southern, forcing ground-based optical surveys to use at least two different telescopes. The
surveys generated results, but it was unclear whether a particular result was caused by the problems
of having to observe the two clouds with different instruments, and at different times of the year.

Enter WISE, which roared into orbit on Dec. 14, 2009. The spacecraft's 16-inch (40-centimeter)
telescope and infrared cameras scoured the entire sky looking for the glow of celestial heat sources.
From January 2010 to February 2011, about 7,500 images were taken every day. The NEOWISE
project used the data to catalogue more than 158,000 asteroids and comets throughout the solar
system.

"By obtaining accurate diameter and surface reflectivity measurements on 1,750 Jupiter Trojans, we
increased by an order of magnitude what we knew about these two gatherings of asteroids," said
Grav. "With this information, we were able to more accurately than ever confirm there are indeed
almost 40 percent more objects in the leading cloud."

Trying to understand the surface or interior of a Jovian Trojan is also difficult. The WISE suite of
infrared detectors was sensitive to the thermal glow of the objects, unlike visible-light telescopes.
This means WISE can provide better estimates of their surface reflectivity, or albedo, in addition to
more details about their visible and infrared colors (in astronomy "colors" can refer to types of light
beyond the visible spectrum).

"Seeing asteroids with WISE's many wavelengths is like the scene in 'The Wizard of Oz,' where
Dorothy goes from her black-and-white world into the Technicolor land of Oz," said Amy Mainzer,
the principal investigator of the NEOWISE project at NASA's Jet Propulsion Laboratory in Pasadena,
Calif. "Because we can see farther into the infrared portion of the light spectrum, we can see more
details of the asteroids' colors, or, in essence, more shades or hues."

The NEOWISE team has analyzed the colors of 400 Trojan asteroids so far, allowing many of these
asteroids to be properly sorted according to asteroid classification schemes for the first time.

"We didn't see any ultra-red asteroids, typical of the main belt and Kuiper belt populations," said
Grav. "Instead, we find a largely uniform population of what we call D-type asteroids, which are dark
burgundy in color, with the rest being C- and P-type, which are more grey-bluish in color. More
research is needed, but it's possible we are looking at the some of the oldest material known in the
solar system."

Scientists have proposed a future space mission to the Jupiter Trojans that will gather the data needed
to determine their age and origins.

The results were presented today at the 44th annual meeting of the Division for Planetary Sciences of
the American Astronomical Society in Reno, Nev. Two studies detailing this research are accepted
for publication in the Astrophysical Journal.

JPL manages, and operated, WISE for NASA's Science Mission Directorate. The spacecraft was put
into hibernation mode in 2011, after it scanned the entire sky twice, completing its main objectives.
Edward Wright is the principal investigator and is at UCLA. The mission was selected competitively
under NASA's Explorers Program managed by the agency's Goddard Space Flight Center in
Greenbelt, Md. The science instrument was built by the Space Dynamics Laboratory in Logan, Utah.
The spacecraft was built by Ball Aerospace & Technologies Corp. in Boulder, Colo. Science
operations and data processing take place at the Infrared Processing and Analysis Center at the
California Institute of Technology in Pasadena. Caltech manages JPL for NASA. More information is
online at http://www.nasa.gov/wise , http://wise.astro.ucla.edu and http://jpl.nasa.gov/wise .

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Friday, October 12, 2012

How to Hunt a Space Rock

Thursday, October 11, 2012

Mars Rock Touched by NASA Curiosity has Surprises

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 / D.C. Agle 818-354-5011
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov / agle@jpl.nasa.gov

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

News release: 2012-318 Oct. 11, 2012

Mars Rock Touched by NASA Curiosity has Surprises

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2012-318&cid=release_2012-318

PASADENA, Calif. -- The first Martian rock NASA's Curiosity rover has reached out to touch presents a more varied composition than expected from previous missions. The rock also resembles some unusual rocks from Earth's interior.

The rover team used two instruments on Curiosity to study the chemical makeup of the football-size rock called "Jake Matijevic" (matt-EE-oh-vick) The results support some surprising recent measurements and provide an example of why identifying rocks' composition is such a major emphasis of the mission. Rock compositions tell stories about unseen environments and planetary processes.

"This rock is a close match in chemical composition to an unusual but well-known type of igneous rock found in many volcanic provinces on Earth," said Edward Stolper of the California Institute of Technology in Pasadena, who is a Curiosity co-investigator. "With only one Martian rock of this type, it is difficult to know whether the same processes were involved, but it is a reasonable place to start thinking about its origin."

On Earth, rocks with composition like the Jake rock typically come from processes in the planet's mantle beneath the crust, from crystallization of relatively water-rich magma at elevated pressure.

Jake was the first rock analyzed by the rover's arm-mounted Alpha Particle X-Ray Spectrometer (APXS) instrument and about the thirtieth rock examined by the Chemistry and Camera (ChemCam) instrument. Two penny-size spots on Jake were analyzed Sept. 22 by the rover's improved and faster version of earlier APXS devices on all previous Mars rovers, which have examined hundreds of rocks. That information has provided scientists a library of comparisons for what Curiosity sees.

"Jake is kind of an odd Martian rock," said APXS Principal Investigator Ralf Gellert of the University of Guelph in Ontario, Canada. "It's high in elements consistent with the mineral feldspar, and low in magnesium and iron."

ChemCam found unique compositions at each of 14 target points on the rock, hitting different mineral grains within it.

"ChemCam had been seeing compositions suggestive of feldspar since August, and we're getting closer to confirming that now with APXS data, although there are additional tests to be done," said ChemCam Principal Investigator Roger Wiens (WEENS) of Los Alamos National Laboratory in New Mexico.

Examination of Jake included the first comparison on Mars between APXS results and results from checking the same rock with ChemCam, which shoots laser pulses from the top of the rover's mast.

The wealth of information from the two instruments checking chemical elements in the same rock is just a preview. Curiosity also carries analytical laboratories inside the rover to provide other composition information about powder samples from rocks and soil. The mission is progressing toward getting the first soil sample into those analytical instruments during a "sol," or Martian day.

"Yestersol, we used Curiosity's first perfectly scooped sample for cleaning the interior surfaces of our 150-micron sample-processing chambers. It's our version of a Martian carwash," said Chris Roumeliotis (room-eel-ee-OH-tiss), lead turret rover planner at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

Before proceeding, the team carefully studied the material for scooping at a sandy patch called "Rocknest," where Curiosity is spending about three weeks.

"That first sample was perfect, just the right particle-size distribution," said JPL's Luther Beegle, Curiosity sampling-system scientist. "We had a lot of steps to be sure it was safe to go through with the scooping and cleaning."

Following the work at Rocknest, the rover team plans to drive Curiosity about 100 yards eastward and select a rock in that area as the first target for using the drill.

During a two-year prime mission, researchers will use Curiosity's 10 instruments to assess whether the study area ever has offered environmental conditions favorable for microbial life. JPL, a division of Caltech, manages the project and built Curiosity. For more about the Mars Science Laboratory Curiosity rover mission, visit: http://www.nasa.gov/msl and http://mars.jpl.nasa.gov/msl .

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

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