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Friday, October 30, 2015

JPL News - Day in Review

 

DAY IN REVIEW
Saturn's Geyser Moon Shines in Close Flyby Views
NASA's Cassini spacecraft has sent back new images of Saturn's active moon Enceladus, acquired during its Oct. 28 flyby.
› Read the full story
Halloween Skies to Include Dead Comet Flyby
The large space rock that will safely zip past Earth this Halloween is most likely a dead comet.
› Read the full story

 



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Thursday, October 29, 2015

JPL News - Day in Review

 

DAY IN REVIEW
Voyager 1 Helps Solve Interstellar Medium Mystery
A study provides new insights about the magnetic field of the interstellar medium, using data from Voyager 1 and other spacecraft.
› Read the full story
Rewrite of Onboard Memory Planned for NASA Mars Orbiter
NASA's Mars Reconnaissance Orbiter will suspend activities next week to perform a multi-step update of onboard memory that is crucial in case of an unplanned computer reboot.
› Read the full story
Excitement Grows as NASA Carbon Sleuth Begins Year Two
Scientists poring over data from NASA's Orbiting Carbon Observatory-2 mission are seeing patterns emerge as they seek answers to questions about atmospheric carbon dioxide.
› Read the full story

 



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Tuesday, October 27, 2015

JPL News - Day in Review

 

DAY IN REVIEW
NASA JPL latest news release
Black Hole Has Major Flare

The baffling and strange behaviors of black holes have become somewhat less mysterious recently, with new observations from NASA's Explorer missions Swift and the Nuclear Spectroscopic Telescope Array, or NuSTAR. The two space telescopes caught a supermassive black hole in the midst of a giant eruption of X-ray light, helping astronomers address an ongoing puzzle: How do supermassive black holes flare?

The results suggest that supermassive black holes send out beams of X-rays when their surrounding coronas -- sources of extremely energetic particles -- shoot, or launch, away from the black holes.

"This is the first time we have been able to link the launching of the corona to a flare," said Dan Wilkins of Saint Mary's University in Halifax, Canada, lead author of a new paper on the results appearing in the Monthly Notices of the Royal Astronomical Society. "This will help us understand how supermassive black holes power some of the brightest objects in the universe."

Supermassive black holes don't give off any light themselves, but they are often encircled by disks of hot, glowing material. The gravity of a black hole pulls swirling gas into it, heating this material and causing it to shine with different types of light. Another source of radiation near a black hole is the corona. Coronas are made up of highly energetic particles that generate X-ray light, but details about their appearance, and how they form, are unclear.

Astronomers think coronas have one of two likely configurations. The "lamppost" model says they are compact sources of light, similar to light bulbs, that sit above and below the black hole, along its rotation axis. The other model proposes that the coronas are spread out more diffusely, either as a larger cloud around the black hole, or as a "sandwich" that envelops the surrounding disk of material like slices of bread. In fact, it's possible that coronas switch between both the lamppost and sandwich configurations.

The new data support the "lamppost" model -- and demonstrate, in the finest detail yet, how the light-bulb-like coronas move. The observations began when Swift, which monitors the sky for cosmic outbursts of X-rays and gamma rays, caught a large flare coming from the supermassive black hole called Markarian 335, or Mrk 335, located 324 million light-years away in the direction of the constellation Pegasus. This supermassive black hole, which sits at the center of a galaxy, was once one of the brightest X-ray sources in the sky.

"Something very strange happened in 2007, when Mrk 335 faded by a factor of 30. What we have found is that it continues to erupt in flares but has not reached the brightness levels and stability seen before," said Luigi Gallo, the principal investigator for the project at Saint Mary's University. Another co-author, Dirk Grupe of Morehead State University in Kentucky, has been using Swift to regularly monitor the black hole since 2007.

In September 2014, Swift caught Mrk 335 in a huge flare. Once Gallo found out, he sent a request to the NuSTAR team to quickly follow up on the object as part of a "target of opportunity" program, where the observatory's previously planned observing schedule is interrupted for important events. Eight days later, NuSTAR set its X-ray eyes on the target, witnessing the final half of the flare event.

After careful scrutiny of the data, the astronomers realized they were seeing the ejection, and eventual collapse, of the black hole's corona.

"The corona gathered inward at first and then launched upwards like a jet," said Wilkins. "We still don't know how jets in black holes form, but it's an exciting possibility that this black hole's corona was beginning to form the base of a jet before it collapsed."

How could the researchers tell the corona moved? The corona gives off X-ray light that has a slightly different spectrum -- X-ray "colors" -- than the light coming from the disk around the black hole. By analyzing a spectrum of X-ray light from Mrk 335 across a range of wavelengths observed by both Swift and NuSTAR, the researchers could tell that the corona X-ray light had brightened -- and that this brightening was due to the motion of the corona.

Coronas can move very fast. The corona associated with Mrk 335, according to the scientists, was traveling at about 20 percent the speed of light. When this happens, and the corona launches in our direction, its light is brightened in an effect called relativistic Doppler boosting.

Putting this all together, the results show that the X-ray flare from this black hole was caused by the ejected corona.

"The nature of the energetic source of X-rays we call the corona is mysterious, but now with the ability to see dramatic changes like this we are getting clues about its size and structure," said Fiona Harrison, the principal investigator of NuSTAR at the California Institute of Technology in Pasadena, who was not affiliated with the study.

Many other black hole brainteasers remain. For example, astronomers want to understand what causes the ejection of the corona in the first place.

NuSTAR is a Small Explorer mission led by Caltech and managed by NASA's Jet Propulsion Laboratory in Pasadena, California, for NASA's Science Mission Directorate in Washington. NuSTAR was developed in partnership with the Danish Technical University and the Italian Space Agency (ASI). The spacecraft was built by Orbital Sciences Corp., Dulles, Virginia. NuSTAR's mission operations center is at UC Berkeley, and the official data archive is at NASA's High Energy Astrophysics Science Archive Research Center. ASI provides the mission's ground station and a mirror archive. JPL is managed by Caltech for NASA.

 



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November Educator Workshop - Climate Change

 

 

Climate Change

When: Saturday, Nov. 7, 10 a.m. to 12:30 p.m.

Where: NASA Jet Propulsion Laboratory, Von Karman Auditorium, Pasadena, California

Target Audience: Educators for grades 3-8 (all educators are welcome)

Overview: In this workshop teachers will get an overview of what we know about climate change and how we know it. Enjoy some simple chemistry, videos, games and student inventions. This is a great, standards-based way to teach and inspire students to think about our impact on our environment.

Call the Educator Resource Center at 818-393-5917 to reserve your spot.

This free workshop is offered through the NASA/JPL Educator Resource Center, which provides formal and informal educators with NASA resources and materials that support STEM learning.

Discover more upcoming educator workshops and events from NASA/JPL Education.

 

 



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Monday, October 26, 2015

JPL News - Day in Review

 

DAY IN REVIEW
NASA JPL latest news release
Seven Key Facts About Cassini's Oct. 28 'Plume Dive'

NASA's Cassini spacecraft will sample the ocean of Saturn's moon Enceladus on Wednesday, Oct. 28, when it flies through the moon's plume of icy spray.

Cassini launched in 1997 and entered orbit around Saturn in 2004. Since then, it has been studying the huge planet, its rings and its magnetic field. Here are some things to know about the mission's upcoming close flyby of Enceladus:

-- Enceladus is an icy moon of Saturn. Early in its mission, Cassini discovered Enceladus has remarkable geologic activity, including a towering plume of ice, water vapor and organic molecules spraying from its south polar region. Cassini later determined the moon has a global ocean and likely hydrothermal activity, meaning it could have the ingredients needed to support simple life.

-- The flyby will be Cassini's deepest-ever dive through the Enceladus plume, which is thought to come from the ocean below. The spacecraft has flown closer to the surface of Enceladus before, but never this low directly through the active plume.

-- The flyby is not intended to detect life, but it will provide powerful new insights about how habitable the ocean environment is within Enceladus.

-- Cassini scientists are hopeful the flyby will provide insights about how much hydrothermal activity -- that is, chemistry involving rock and hot water -- is occurring within Enceladus. This activity could have important implications for the potential habitability of the ocean for simple forms of life. The critical measurement for these questions is the detection of molecular hydrogen by the spacecraft.

-- Scientists also expect to better understand the chemistry of the plume as a result of the flyby. The low altitude of the encounter is, in part, intended to afford Cassini greater sensitivity to heavier, more massive molecules, including organics, than the spacecraft has observed during previous, higher-altitude passes through the plume.

-- The flyby will help solve the mystery of whether the plume is composed of column-like, individual jets, or sinuous, icy curtain eruptions -- or a combination of both. The answer would make clearer how material is getting to the surface from the ocean below.

-- Researchers are not sure how much icy material the plumes are actually spraying into space. The amount of activity has major implications for how long Enceladus might have been active.

An online toolkit for all three final Enceladus flybys is available at:

http://solarsystem.nasa.gov/finalflybys

The Cassini-Huygens mission is a cooperative project of NASA, ESA (European Space Agency) and the Italian Space Agency. JPL manages the mission for NASA's Science Mission Directorate in Washington.

For more information about Cassini, visit:

http://www.nasa.gov/cassini

http://saturn.jpl.nasa.gov

 



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Teachable Moment: Flying Through the Plume on Saturn's Moon Enceladus

 

 

TEACHABLE MOMENTS

Flying Through the Plume on Saturn's Moon Enceladus

Saturn's icy moon Enceladus has been making news lately, and it could make even bigger news soon! In September, scientists confirmed that there was a global ocean underneath Enceladus' thick icy shell. That was just the latest in a long history of exciting finds dating back to the beginning of NASA's Cassini-Huygens Mission to Saturn.

On October 28, Cassini will fly right through the plume jetting out of Enceladus' south pole at an altitude of only 49 kilometers (30 miles) – closer than any previous passes directly through the plume! This is an exciting moment in the mission -- one that allows science teams to use a combination of tools on board the spacecraft to strengthen previous findings and potentially make new discoveries.

Take your students on a journey with the Cassini mission as it performs one of its final flybys of the mysterious moon. Our latest Teachable Moment features a handful of lessons and resources you can use to teach key concepts related to the flyby and engage students in this exciting moment in science at Saturn.

Bonus! Download a poster featuring real science facts about Enceladus.

Read the blog

 

 



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Friday, October 23, 2015

JPL News - Day in Review

 

DAY IN REVIEW
NASA JPL latest news release
Fuel Additive Could Lead to Safer Jet Fuel

Airplane accidents are especially dangerous because jet fuel is highly flammable under crash conditions. On impact, jet fuel is dispersed in the air as a fine mist, which triggers a sequence of events that can lead to a fire engulfing an entire plane.

Researchers at the California Institute of Technology and the Jet Propulsion Laboratory, which is managed by Caltech, have been working on additives that inhibit the formation of this highly flammable mist during collisions. These additives are based on long molecules called polymers.

"This research is about making fuel safer and saving lives," said Project Manager Virendra Sarohia, based at JPL.

A new Caltech-led study in the journal Science describes polymers that could increase the safety of jet fuel and diesel fuel, particularly in the event of collision or a deliberate attempt to create a fuel explosion as part of a terrorist attack.

"The new polymers could reduce the intensity of post-crash fires, providing time for more passengers to escape," said Julia Kornfield, a professor of chemical engineering at Caltech who mentored Ming-Hsin Wei, Boyu Li and Ameri David. Their doctoral research is presented in the study.

Fuel misting also happens in jet engines under normal operations. The engine repeatedly ignites a combination of a spray of fuel and compressed air, and this process thrusts the plane forward. The problem arises when a fuel mist is created outside the engine. For example when a plane crashes, the entire volume of fuel could be involved in misting.

Read more about this study from Caltech

"Once we control the mist in a crash, this aviation fuel is hard to ignite," said Sarohia, who collaborated with JPL technologist Simon Jones. "It allows time to fight fires and time to evacuate people from the accident."

Various tests have been conducted in relation to the new study. Impact tests using jet fuel show that the polymers reduce flame propagation in the resulting mist. In other tests, the polymers showed no adverse effects on diesel engine operation, researchers say.

Video: Treated and untreated jet fuel test

Larger-scale production is needed to provide enough polymer for jet engine tests.

"Years of testing are required to achieve FAA approval for use in jet fuel, so the polymer might be used first to reduce post-crash fires on roadways," Kornfield said.

How the Polymers Work

A polymer is a large molecule that has regularly repeated units. The new technology consists of polymer chains that are able to reversibly link together through chemical groups on their ends that stick together like Velcro. If you link these polymers end-to-end, very large chains form, which the study authors call "mega-supramolecules."

"Our polymers have backbones that, like fuel, have just carbon and hydrogen, but they are much, much longer. Typically our polymers have 50,000 carbon atoms in the backbone," said Kornfield.

"Such long polymers, specially constructed for a fuel additive, are unprecedented. Many years of laboratory effort have gone into the design of their structure and the development of careful methods for their synthesis," said Jones.

Sarohia likens the mechanism of the fuel additive to the clotting of blood. While blood is in the veins, it should flow freely; clotting in the veins could be fatal. But blood is supposed to clot when it gets to the surface of skin, so that a person doesn't bleed out. Similarly, the jet fuel with the polymer added should flow normally during routine operation of the aircraft; it's only during a collision that it should act to control the mist.

JPL's Involvement

Sarohia has been working on this research since the 1970s. The Tenerife Airport disaster in the Canary Islands in 1977, in which 583 passengers aboard two planes were killed in a runway collision, demonstrated the need for safer jet fuel. An international collaboration resulted in successful sled-driven plane crash tests of a fuel additive in the early 1980s.

But the analyses of a 1984 full-scale impact test in California's Mojave Desert were mixed. There was no more activity in the research program for more than a decade.

It looked as though the program had ended for good. But Sarohia remembers that after the Sept. 11, 2001, attacks on the World Trade Center, his daughter asked him, "Where's your fuel?" That got him thinking about the polymer again.

Not long afterwards, Sarohia received the support of JPL to restart the investigation of a polymer to control fuel mist. In 2003, Sarohia and colleagues demonstrated in tests at China Lake, California, that the polymer could be effective even at 500 mph impact speeds. The results provided the impetus for the Caltech-JPL collaboration.

The fuel additive tested in the 1980s consisted of ultralong polymers that interfered with engine operation. Therefore each and every aircraft would need to be retrofitted with a device called a "degrader" to break the polymers into small segments just before injection in the engine. However, the new polymers can release their end associations during fuel-injection and disperse into smaller units that are compatible with engine operation.

"The hope is that it will not require the modification of the engine," Sarohia said.

Long-haul diesel engine tests also show that the polymer has the potential to reduce emissions of particulate matter by controlling the fuel droplet size. These megasupramolecules may also reduce resistance to flow through pipelines. Ongoing research is establishing methods to produce the larger quantities of the polymer required to explore these opportunities.

The Science study was funded by the U.S. Army Tank Automotive Research Development and Engineering Center, the Federal Aviation Administration, the Schlumberger Foundation, and the Gates Grubstake Fund.

 



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Thursday, October 22, 2015

JPL News - Day in Review

 

DAY IN REVIEW
NASA Teleconference to Preview Historic Flyby of Saturn Moon
NASA's Cassini spacecraft will sample an extraterrestrial ocean next week when it flies directly through a plume of icy spray from Enceladus. A news telecon on Monday, Oct. 26, will preview the event.
› Read the full story
NASA Calls for American Industry Ideas on ARM Spacecraft Development
NASA, through JPL, has issued a call to American industry for innovative ideas involving the Asteroid Redirect Robotic Mission.
› Read the full story

 



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Upcoming Teacher Workshop - Lunar and Meteorite Sample Certification

 

Lunar and Meteorite Sample Certification

Columbia Memorial Space Center Teacher Workshop:

Lunar and Meteorite Sample Certification

When: Saturday, Oct. 31, 10 a.m. to 12 p.m.

Where: Columbia Memorial Space Center, Downey, California

Target Audience: Fully credentialed teachers for grades K-12 (must show teacher ID)

Overview: NASA makes actual samples from the historic Apollo missions available to lend to teachers. You must attend this certification process to bring the excitement of real lunar rocks and regolith samples to your students. This certification also includes meteorite disks containing samples of extraterrestrial material collected from the frozen expanses of Antarctica.

After the workshop, participants are invited to experience a simulated space mission in the Challenger Learning Center from 1 p.m. to 3 p.m.

Register online on the City of Downey's ActiveNet portal or call (562) 231-1200.

  • This free workshop is for fully credentialed teachers only.
  • Teachers must bring a teacher ID to the workshop.
  • Preregistration is required.
  • Lunch will be provided.
The Columbia Memorial Space Center is a space science learning center in the Los Angeles area dedicated to hands-on robotics, engineering, technology and science.The Center hosts a number of educator workshops throughout the year for pre-service and fully credentialed teachers taught by NASA Jet Propulsion Laboratory education specialists and science consultants. Visit the Center's "Teacher Resources" web page to learn more about upcoming workshops.

Discover more upcoming educator workshops and events from NASA/JPL Education.

 



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Wednesday, October 21, 2015

JPL News - Day in Review

 

DAY IN REVIEW
NASA's K2 Finds Dead Star Vaporizing a Mini 'Planet'
A tiny, rocky object is likely being torn apart as it spirals around a white dwarf star.
› Read the full story
NASA Spots the 'Great Pumpkin': Halloween Asteroid a Treat for Radar Astronomers
NASA scientists are tracking the upcoming Halloween flyby of an asteroid with optical observatories and radar capabilities of the Deep Space Network at Goldstone, California.
› Read the full story

 



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Tuesday, October 20, 2015

JPL News - Day in Review

 

DAY IN REVIEW
NASA JPL latest news release
NASA Study Improves Understanding of LA Quake Risks

A new NASA-led analysis of a moderate magnitude 5.1 earthquake that shook Greater Los Angeles in 2014 finds that the earthquake deformed Earth's crust across a broad region encompassing the northern Los Angeles Basin and northern Orange County. The shallow ground movements observed from this earthquake likely reflect strain accumulated on deeper faults, which remain locked and may be capable of producing future earthquakes.

A team of NASA and university researchers led by geophysicist Andrea Donnellan of NASA's Jet Propulsion Laboratory, Pasadena, California, used GPS and NASA airborne radar data to measure surface deformation in Earth's crust caused by the March 28, 2014, earthquake, which was centered in La Habra, California. The earthquake was felt widely in Orange, Los Angeles, Ventura, Riverside, San Bernardino, Kern and San Diego counties. While the earthquake was relatively moderate in size, the earthquake's depth (3.6 miles, or 5.85 kilometers) and location within a highly populated region resulted in more than $12 million in damage. Most of the damage occurred within a 3.7-mile (6-kilometer) radius of the epicenter, with a substantial amount of damage south of the main rupture.

Donnellan's team found the earthquake deformed Earth's crust across a broad region, but mostly south of the main rupture, consistent with the observed damage. They measured 3.1 inches (80 millimeters) of northward horizontal motion and about 0.2 to 0.4 inches (5 to 10 millimeters) of upward motion.

They also discovered that the total amount of surface deformation associated with the La Habra earthquake was larger than what would be expected from the magnitude 5.1 main shock. Eighty-two percent of the surface motion was attributed to the earthquake itself, with the remaining 18 percent occurring aseismically, without producing any ground shaking. The amount of aseismic motion was greater than expected. The team's results show that even moderate earthquakes near Los Angeles can produce ground deformation and damage to water mains away from their epicenters.

The team used computer models to explain the observed patterns of ground deformation and found that the best explanation for the observed ground deformation was shallow movement along several active buried fault-like zones in the West Coyote Hills in northern Orange County; in the Chino Hills on the border of Orange, Los Angeles and San Bernardino Counties; and in the San Gabriel Valley. The modeled movements identified by the team in the San Gabriel Valley and Chino Hills are part of a series of incompletely mapped active faults in a geologically complex region. It is likely the deeper portions of these faults remain locked and thus are capable of producing future earthquakes.

"The earthquake faults in this region are part of a system of faults," said Donnellan. "They can move together in an earthquake and produce measurable surface deformation, even during moderate magnitude earthquakes. This fault system accommodates the ongoing shortening of Earth's crust in the northern Los Angeles region." Tectonic motion across the Los Angeles region is distributed on an intricate network of horizontally and vertically moving faults that eventually release accumulated strain in the form of earthquakes, such as the destructive 1994 magnitude-6.7 Northridge earthquake.

Donnellan said a future earthquake to release the accumulated strain on these faults could occur on any one or several of these fault structures, which may not have been mapped at the surface. "Identifying specific fault structures most likely to be responsible for future earthquakes for this system of many active faults is often very difficult," she said.

The earthquake ground displacements were measured by combining pre- and post-earthquake continuous GPS data from the National Science Foundation's Plate Boundary Observatory with NASA's airborne radar data from the JPL-developed Uninhabited Aerial Vehicle Synthetic Aperture Radar (UAVSAR). UAVSAR is an L-band Interferometric SAR instrument mounted beneath a C-20A Earth science research aircraft from NASA's Armstrong Flight Research Center, Edwards, California. It detects minute (less than centimeter-level) changes in Earth's surface that occur over time between flights. NASA has been using UAVSAR to monitor deformation across the Los Angeles region about every six months since 2009.

Co-author Lisa Grant Ludwig of the University of California, Irvine, said the team's analysis can be used by policymakers and government agencies to improve assessments of earthquake risk in the Los Angeles area that are critical for disaster planning.

"The study builds upon more than two decades of NASA-led research to develop new methods to better measure and monitor movements of the solid Earth using satellite and airborne data and advanced computer modeling," Donnellan said. "It also provides a means of using these technologies to identify which faults moved during earthquakes, to measure exactly how much Earth's surface deformed during earthquakes, and to use these measurements to estimate future earthquake potential."

Study results are published in the journal Earth and Space Science. Other participating institutions include Indiana University, Bloomington; University of California, Davis; and University of Nevada, Reno.

NASA is applying maturing airborne and space-based technologies, new ground-based techniques and more complex computer models to advance our understanding of earthquakes and earthquake processes. For more information on UAVSAR, visit:

http://uavsar.jpl.nasa.gov/

NASA uses the vantage point of space to increase our understanding of our home planet, improve lives and safeguard our future. NASA develops new ways to observe and study Earth's interconnected natural systems with long-term data records. The agency freely shares this unique knowledge and works with institutions around the world to gain new insights into how our planet is changing.

For more information about NASA's Earth science activities, visit:

http://www.nasa.gov/earth

 



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