Jumbo Jellyfish or Massive Star?

A sphere of stellar innards, blown out from a humongous star
A cloud of material shed by a massive star can be seen in red in this new image from WISE.
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Some might see a blood-red jellyfish in a forest of seaweed, while others might see a big, red eye or a pair of lips. In fact, the red-colored object in this new infrared image from NASA's Wide-field Infrared Survey Explorer (WISE) is a sphere of stellar innards, blown out from a humongous star.

The star (white dot in center of red ring) is one of the most massive stellar residents of our Milky Way galaxy. Objects like this are called Wolf-Rayet stars, after the astronomers who found the first few, and they make our sun look puny by comparison. Called V385 Carinae, this star is 35 times as massive as our sun, with a diameter nearly 18 times as large. It's hotter, too, and shines with more than one million times the amount of light.

Fiery candles like this burn out quickly, leading short lives of only a few million years. As they age, they blow out more and more of the heavier atoms cooking inside them -- atoms such as oxygen that are needed for life as we know it.

The material is puffed out into clouds like the one that glows brightly in this WISE image. In this case, the hollow sphere showed up prominently only at the longest of four infrared wavelengths detected by WISE. Astronomers speculate this infrared light comes from oxygen atoms, which have been stripped of some of their electrons by ultraviolet radiation from the star. When the electrons join up again with the oxygen atoms, light is produced that WISE can detect with its 22-micron infrared light detector. The process is similar to what happens in fluorescent light bulbs.

Infrared light detected by WISE at 12 microns is colored green, while 3.4- and 4.6-micron light is blue. The green, kelp-looking material is warm dust, and the blue dots are stars in our Milky Way galaxy.

This image mosaic is made up of about 300 overlapping frames, taken as WISE continues its survey of the entire sky -- an expansive search, sure to turn up more fascinating creatures swimming in our cosmic ocean.

V385 Carinae is located in the Carina constellation, about 16,000 light-years from Earth.

JPL manages the Wide-field Infrared Survey Explorer for NASA's Science Mission Directorate, Washington. The principal investigator, Edward Wright, is at UCLA. The mission was competitively selected under NASA's Explorers Program managed by the Goddard Space Flight Center, Greenbelt, Md. The science instrument was built by the Space Dynamics Laboratory, Logan, Utah, and the spacecraft was built by Ball Aerospace & Technologies Corp., 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 and http://wise.astro.ucla.edu.

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Astronomers Discover Star-Studded Galaxy Tail

A star-studded tail on a galaxy called IC 3418
NASA's Galaxy Evolution Explorer found a tail behind a galaxy called IC 3418. The star-studded tail can be seen in the image on the left, as detected by the space telescope in ultraviolet light. The tail has escaped detection in visible light, as shown by the image on the right.
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NASA's Galaxy Evolution Explorer has discovered a galaxy tail studded with bright knots of new stars. The tail, which was created as the galaxy IC 3418 plunged into the neighboring Virgo cluster of galaxies, offers new insight into how stars form.

"The gas in this galaxy is being blown back into a turbulent wake," said Janice Hester of the California Institute of Technology in Pasadena, lead author of a recent study published in the Astrophysical Journal Letters. "The gas is like sand caught up by a stiff wind. However, the particular type of gas that is needed to make stars is heavier, like pebbles, and can't be blown out of the galaxy. The new Galaxy Evolution Explorer observations are teaching us that this heavier, star-forming gas can form in the wake, possibly in swirling eddies of gas."

Collisions between galaxies are a fairly common occurrence in the universe. Our Milky Way galaxy will crash into the Andromeda galaxy in a few billion years. Galaxies tangle together, kicking gas and dust all around. Often the battered galaxies are left with tails of material stripped off during the violence.

Hester and her team studied the tail of IC 3418, which formed in a very different way. IC 3418 is mingling not with one galaxy, but with the entire Virgo cluster of galaxies 54 million light-years away from Earth. This massive cluster, which contains about 1,500 galaxies and is permeated by hot gas, is pulling in IC 3418, causing it to plunge through the cluster's gas at a rate of 1,000 kilometers per second, or more than 2 million miles per hour. At this incredible speed, the little galaxy's gas is being shoved back into a choppy tail.

The astronomers were able to find this tail with the help of the Galaxy Evolution Explorer. Clusters of massive, young stars speckle the tail, and these stars glow with ultraviolet light that the space telescope can see. The young stars tell scientists that a crucial ingredient for star formation - dense clouds of gas called molecular hydrogen - formed in the wake of this galaxy's plunge. This is the first time astronomers have found solid evidence that clouds of molecular hydrogen can form under the violent conditions present in a turbulent wake.

"IC 3418's tail of star-formation demonstrates that strong turbulence promotes cloud formation," said Mark Seibert, a co-author of the paper and a member of the Galaxy Evolution Explorer science team at the Carnegie Institute for Science in Pasadena.

Hester added that galaxy tails provide the perfect environment for isolating the factors controlling star formation.

"These tails are unique, exotic locations where we can probe the precise mechanisms behind star formation," said Hester. "Understanding star formation is pivotal to understanding the lifecycles of galaxies and the dramatic transformations that some galaxies undergo. We can also study how the process affects the development of planets like our own."

Other authors of the paper are James D. Neill, Ted K. Wyder and Christopher Martin of Caltech; Armando Gil de Paz of the Universidad de Computense de Madrid, Spain; Barry F. Madore of the Carnegie Institute of Washington; David Schiminovich of Columbia University, N.Y., N.Y; and Michael Rich of UCLA.

Caltech leads the Galaxy Evolution Explorer mission and is responsible for science operations and data analysis. NASA's Jet Propulsion Laboratory in Pasadena manages the mission and built the science instrument. The mission was developed under NASA's Explorers Program managed by the Goddard Space Flight Center, Greenbelt, Md. Researchers sponsored by Yonsei University in South Korea and the Centre National d'Etudes Spatiales (CNES) in France collaborated on this mission.

Graphics and additional information about the Galaxy Evolution Explorer is online at http://www.nasa.gov/galex/ and http://www.galex.caltech.edu .

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NASAJPL Facebook Fans Design Fantasy Space Vacation

Artist's concept of a family road trip through the universe
Some creative space vacation ideas from fans of the NASAJPL Facebook Page inspired an artist's concept of a family road trip through the universe.

We got some super-creative ideas from people on the NASAJPL Facebook page when we asked this question: "Planning a summer trip? Talk to your friends and family -- if you could design your dream space vacation, where would you go?"

As promised, we're posting a small sampling of comments here, but you can read all the comments, or post your own ideas at http://www.facebook.com/NASAJPL.

Eoghan Lappin: Moon for breakfast. Mars for lunch. Titan for dinner. Then all the way to Gliese 581d on a trip of a lifetime (Because it would take that long at least!) Epic road trip! 😀

Brian Hinson: I'd barbecue kabobs on Pele on Io.

Adam Steineck: I'd go to a watery planet with lots of beaches orbiting a binary star system so the sun would never set 🙂

Madhur Patel: My dream vacation would be the 'Asteroid belt' between Mars and Jupiter. It would be fun to go from Mars to Jupiter jumping on the asteroids on the way using a pogo-stick and taking breaks on some of the bigger asteroids like Ceres, 4 Vesta, 2 Pallas, and 10 Hygiea ! 🙂

Mike Kaberline: I would go to Mars to get Spirit unstuck and dust off the solar panels of Spirit and Opportunity.

Devon Sklair: I would go to Pluto. That way I could pass all the planets in the Solar System on my way there and hang out in the Kuiper Belt. Maybe I'd establish relations with some Plutonians. 🙂

Raees Kolah: I guess I would like to visit Andromeda galaxy and after that have a dinner with my best friends on Mars.

Grieg Pedersen: I used to have a photo of the Pleiades on my wall, framed in a window frame. I'd love to have that view from my bungalow.

Bob Breit: While my family is from Mintaka in Orion, that is a generational vacation. At this time I would enjoy a rip roarin' ski trip to Enceladus. The jets are fabulous in summer! I could spend the entire season roaming the Saturnian moons and the balloon trip around Saturn is quite a day I hear. I CAN'T WAIT!

Jeff Kuyken: How about a base jump from the Mars moon Phobos followed by a leisurely stroll up to the summit of Olympus Mons! 😉

Sarah Hill: I'd go to Alpha Centauri to see if there are any planets there with a moon with tall blue people.


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NASA Releases Kepler Data on Potential Extrasolar Planets

Artist's concept of Kepler
Artist's concept of Kepler in the distant solar system.
NASA's Kepler Mission has released 43 days of science data on more than 156,000 stars. These stars are being monitored for subtle brightness changes as part of an ongoing search for Earth-like planets outside of our solar system.

Astronomers will use the new data to determine if orbiting planets are responsible for brightness variations in several hundred stars. These stars represent a full range of temperatures, sizes and ages. Many of them are stable, while others pulsate. Some show starspots, which are similar to sunspots, and a few produce flares that would sterilize their nearest planets.

Kepler, a space observatory, looks for the data signatures of planets by measuring tiny decreases in the brightness of stars when planets cross in front of, or transit, them. The size of the planet can be derived from the change in the star's brightness.

The 28-member Kepler science team also is using ground-based telescopes and NASA's Hubble Space Telescope and Spitzer Space Telescope to perform follow-up observations on a specific set of 400 objects of interest. The star field that Kepler observes in the constellations Cygnus and Lyra can only be seen from ground-based observatories in spring through early fall. The data from these other observations will determine which of the candidates can be identified as planets. That data will be released to the scientific community in February 2011.

Without the additional information, candidates that are actual planets cannot be distinguished from false alarms, such as binary stars -- two stars that orbit each other. The size of the planetary candidates also can be only approximated until the size of the stars they orbit is determined from additional spectroscopic observations made by ground-based telescopes.

"I look forward to the scientific community analyzing the data and announcing new exoplanet results in the coming months," said Lia LaPiana, Kepler's program executive at NASA Headquarters in Washington.

"This is the most precise, nearly continuous, longest and largest data set of stellar photometry ever," said Kepler Deputy Principal Investigator David Koch of NASA's Ames Research Center in Moffett Field, Calif. "The results will only get better as the duration of the data set grows with time."

Kepler will continue conducting science operations until at least November 2012, searching for planets as small as Earth, including those that orbit stars in a warm, habitable zone where liquid water could exist on the surface of the planet. Since transits of planets in the habitable zone of solar-like stars occur about once a year and require three transits for verification, it is expected to take at least three years to locate and verify an Earth-size planet.

"The Kepler observations will tell us whether there are many stars with planets that could harbor life, or whether we might be alone in our galaxy," said the mission's science principal investigator, William Borucki of Ames.

Ames is responsible for the ground system development, mission operations and science data analysis. NASA's Jet Propulsion Laboratory in Pasadena, Calif., managed the Kepler mission development. Ball Aerospace and Technologies Corp. in Boulder, Colo., developed the Kepler flight system, and supports mission operations with the Laboratory for Atmospheric and Space Physics at the University of Colorado, Boulder. The Space Telescope Science Institute in Baltimore archives, hosts and distributes the Kepler science data.

To see the science data, visit: http://archive.stsci.edu/kepler. For more information about the Kepler mission, visit: http://www.nasa.gov/kepler.

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NASA Dryden Hosts Radar Tests for Next Mars Landing

Test at NASA Dryden of radar system for next Mars landing
This test of the radar system to be used during the August 2012 descent and landing of the NASA Mars rover Curiosity mounted an engineering test model of the radar system onto the nose of a helicopter. › Larger image

Engineers with NASA's Jet Propulsion Laboratory, Pasadena, Calif., are running diverse trials with a test version of the radar system that will enable NASA's Mars Science Laboratory mission to put the Curiosity rover onto the Martian surface in August 2012.

One set of tests conducted over a desert lakebed at NASA's Dryden Flight Research Center, Edwards, Calif., in May 2010 used flights with a helicopter simulating specific descent paths anticipated for Martian sites.

During the final stage of descent, NASA's Mars Science Laboratory mission will use a "sky crane" maneuver to lower Curiosity on a bridle from the mission's rocket-powered descent stage. The descent stage will carry Curiosity's flight radar.

The testing at Dryden included lowering a rover mockup on a tether from the helicopter to assess how the sky crane maneuver will affect the radar's descent-speed determinations by the radar. The helicopter carried the test radar on a special nose-mounted gimbal.

Helicopter-flown testing has also been conducted at other desert locations for experience in an assortment of terrains. Later in 2010, the team plans to test the higher-altitude, higher-velocity part of Curiosity's radar-aided descent by flying the test radar on dives by an F/A-18 jet from Dryden.

For more information about the Mars Science Laboratory radar testing at Dryden, see http://www.nasa.gov/mission_pages/msl/msl_rover_tests.html. More about the Mars Science Laboratory is at http://mars.jpl.nasa.gov/msl/. JPL, a division of the California Institute of Technology in Pasadena, manages the Mars Science Laboratory Project for the NASA Science Mission Directorate, Washington.

NASA Kicks Off New Summer of Innovation Initiative

NASA's Jet Propulsion Laboratory in Pasadena, Calif., hosts the  national kickoff of NASA's Summer of Innovation
NASA's Jet Propulsion Laboratory in Pasadena, Calif., hosts the national kickoff of NASA's Summer of Innovation.

NASA Administrator Charles Bolden kicked off the agency's new Summer of Innovation initiative today while at the Jet Propulsion Laboratory in Pasadena, Calf.

The Summer of Innovation program will engage thousands of middle school students in science, technology, engineering and mathematics (STEM) during the summer months when many students experience what's known as the "summer slide," a loss of skills acquired during the school year. The program is a cornerstone of the Educate to Innovate campaign announced by President Obama last November.

About 250 middle school students from the Los Angeles area participated in the kickoff festivities, which included an opportunity to interact with astronauts, NASA scientists and engineers, several hands-on educational activities; and a visit to the facility where the next Mars rover is being built. The students also were treated to musical entertainment provided by actor/rapper Daniel Curtis Lee.

"It is wonderful to feel the excitement generated by these students as they experienced first-hand what fascinating and challenging opportunities exist for students who follow STEM career paths," said Administrator Bolden. "I hope that by getting these students involved in NASA's missions and programs now, it may pave the way for a new generation of scientists and engineers, which is critically important to our nation's future."

NASA's Summer of Innovation program is a broad, nationwide effort that will leverage partnerships with academia, industry and government. This program and the agency's other education programs support NASA's commitment to excellence in science, technology, engineering and mathematics, which will play a key role in preparing, inspiring, encouraging and nurturing the nation's future work force.

To learn more about this program and the opportunities available, visit http://www.nasa.gov/soi . For information about NASA education programs, visit: http://www.nasa.gov/education .

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NASA Chief Technology Officer for IT Honored by CIO Magazine

Chris KempChris C. Kemp, NASA’s chief technology officer for Information Technology and ‘super star’ of IT innovation for the agency, has been recognized with CIO Magazine’s “CIO 100” award for his work done while he was chief information officer for NASA’s Ames Research Center in Moffett Field, Calif., in 2009. Every year, CIO Magazine identifies and honors 100 organizations that have distinguished themselves through the effective and innovative use of information technology.

“I am honored to be recognized by

CIO Magazine and to be the first honoree from Ames is truly humbling. The work that I did there in 2009 was meaningful to me and makes me extremely proud. I am inspired by NASA’s mission, and it’s been an honor to be a member of the team ” said Kemp.

The combination of Kemps’ enthusiasm for

NASA and information technology has made him extremely successful at his job.

"This year's

CIO 100 awards draws well-deserved attention to companies that are not only innovating with IT but creating genuine business value as well," said Maryfran Johnson, editor in chief of CIO Magazine. "These winning companies and their IT organizations are an inspiration to businesses everywhere."

Kemp is not afraid to venture into unchartered territory. In 2008, he began the Nebula Cloud Computing project (now a NASA-wide program) which uses open source software components to create a robust cloud environment where scientists can process and share data. Kemp also implemented an agency-wide IT Security Operations Center at Ames.

“The Nebula Platform allows scientists to focus on their research and spend less time and money on IT infrastructure. These researchers are doing amazing things, and it’s rewarding to create a platform that enables this innovation,” said Kemp.

Kemp is

NASA’s first chief technology officer for IT, a new position established to lead IT innovation across the agency. "This move will leverage Chris’ creative talents and energies," said NASA Chief Information Officer Linda Cureton.

“I’m extremely excited about my new position. I’m thrilled to be involved in supporting many of the ground-breaking IT innovations happening here” Kemp said.

Kemp joined Ames as a successful entrepreneur, having helped create several companies including the third largest online community, Classmates.com. He also helped create the leading web-based vacation rental platform Escapia, and the first online grocery shopping platform for Kroger, the world’s largest grocery store chain.

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What is Consuming Hydrogen and Acetylene on Titan?

Artist concept showing a lake on Saturn's moon Titan
This artist concept shows a mirror-smooth lake on the surface of the smoggy moon Titan.
› Full image and caption
Two new papers based on data from NASA's Cassini spacecraft scrutinize the complex chemical activity on the surface of Saturn's moon Titan. While non-biological chemistry offers one possible explanation, some scientists believe these chemical signatures bolster the argument for a primitive, exotic form of life or precursor to life on Titan's surface. According to one theory put forth by astrobiologists, the signatures fulfill two important conditions necessary for a hypothesized "methane-based life."

One key finding comes from a paper online now in the journal Icarus that shows hydrogen molecules flowing down through Titan's atmosphere and disappearing at the surface. Another paper online now in the Journal of Geophysical Research maps hydrocarbons on the Titan surface and finds a lack of acetylene.

This lack of acetylene is important because that chemical would likely be the best energy source for a methane-based life on Titan, said Chris McKay, an astrobiologist at NASA Ames Research Center, Moffett Field, Calif., who proposed a set of conditions necessary for this kind of methane-based life on Titan in 2005. One interpretation of the acetylene data is that the hydrocarbon is being consumed as food. But McKay said the flow of hydrogen is even more critical because all of their proposed mechanisms involved the consumption of hydrogen.

"We suggested hydrogen consumption because it's the obvious gas for life to consume on Titan, similar to the way we consume oxygen on Earth," McKay said. "If these signs do turn out to be a sign of life, it would be doubly exciting because it would represent a second form of life independent from water-based life on Earth."

To date, methane-based life forms are only hypothetical. Scientists have not yet detected this form of life anywhere, though there are liquid-water-based microbes on Earth that thrive on methane or produce it as a waste product. On Titan, where temperatures are around 90 Kelvin (minus 290 degrees Fahrenheit), a methane-based organism would have to use a substance that is liquid as its medium for living processes, but not water itself. Water is frozen solid on Titan's surface and much too cold to support life as we know it.

The list of liquid candidates is very short: liquid methane and related molecules like ethane. While liquid water is widely regarded as necessary for life, there has been extensive speculation published in the scientific literature that this is not a strict requirement.

The new hydrogen findings are consistent with conditions that could produce an exotic, methane-based life form, but do not definitively prove its existence, said Darrell Strobel, a Cassini interdisciplinary scientist based at Johns Hopkins University in Baltimore, Md., who authored the paper on hydrogen.

Strobel, who studies the upper atmospheres of Saturn and Titan, analyzed data from Cassini's composite infrared spectrometer and ion and neutral mass spectrometer in his new paper. The paper describes densities of hydrogen in different parts of the atmosphere and the surface. Previous models had predicted that hydrogen molecules, a byproduct of ultraviolet sunlight breaking apart acetylene and methane molecules in the upper atmosphere, should be distributed fairly evenly throughout the atmospheric layers.

Strobel found a disparity in the hydrogen densities that lead to a flow down to the surface at a rate of about 10,000 trillion trillion hydrogen molecules per second. This is about the same rate at which the molecules escape out of the upper atmosphere.

"It's as if you have a hose and you're squirting hydrogen onto the ground, but it's disappearing," Strobel said. "I didn't expect this result, because molecular hydrogen is extremely chemically inert in the atmosphere, very light and buoyant. It should 'float' to the top of the atmosphere and escape."

Strobel said it is not likely that hydrogen is being stored in a cave or underground space on Titan. The Titan surface is also so cold that a chemical process that involved a catalyst would be needed to convert hydrogen molecules and acetylene back to methane, even though overall there would be a net release of energy. The energy barrier could be overcome if there were an unknown mineral acting as the catalyst on Titan's surface.

The hydrocarbon mapping research, led by Roger Clark, a Cassini team scientist based at the U.S. Geological Survey in Denver, examines data from Cassini's visual and infrared mapping spectrometer. Scientists had expected the sun's interactions with chemicals in the atmosphere to produce acetylene that falls down to coat the Titan surface. But Cassini detected no acetylene on the surface.

In addition Cassini's spectrometer detected an absence of water ice on the Titan surface, but loads of benzene and another material, which appears to be an organic compound that scientists have not yet been able to identify. The findings lead scientists to believe that the organic compounds are shellacking over the water ice that makes up Titan's bedrock with a film of hydrocarbons at least a few millimeters to centimeters thick, but possibly much deeper in some places. The ice remains covered up even as liquid methane and ethane flow all over Titan's surface and fill up lakes and seas much as liquid water does on Earth.

"Titan's atmospheric chemistry is cranking out organic compounds that rain down on the surface so fast that even as streams of liquid methane and ethane at the surface wash the organics off, the ice gets quickly covered again," Clark said. "All that implies Titan is a dynamic place where organic chemistry is happening now."

The absence of detectable acetylene on the Titan surface can very well have a non-biological explanation, said Mark Allen, principal investigator with the NASA Astrobiology Institute Titan team. Allen is based at NASA's Jet Propulsion Laboratory in Pasadena, Calif. Allen said one possibility is that sunlight or cosmic rays are transforming the acetylene in icy aerosols in the atmosphere into more complex molecules that would fall to the ground with no acetylene signature.

"Scientific conservatism suggests that a biological explanation should be the last choice after all non-biological explanations are addressed," Allen said. "We have a lot of work to do to rule out possible non-biological explanations. It is more likely that a chemical process, without biology, can explain these results - for example, reactions involving mineral catalysts."

"These new results are surprising and exciting," said Linda Spilker, Cassini project scientist at JPL. "Cassini has many more flybys of Titan that might help us sort out just what is happening at the surface."

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. JPL, a division of the California Institute of Technology, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL.

For more information about the Cassini-Huygens mission visit http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov.

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NASA Helps in Upcoming Asteroid Mission Homecoming

Artist's concept of the Hayabusa spacecraft (left) and sample  return capsule (right)
This artist's concept depicts the Hayabusa spacecraft (left) and sample return capsule (right) entering the atmosphere over South Australia.

The space and astronomy worlds have June 13 circled on the calendar.

That's when the Japan Aerospace Exploration Agency (JAXA) expects the sample return capsule of the agency's technology demonstrator spacecraft, Hayabusa, to boomerang back to Earth. The capsule, along with its mother ship, visited a near-Earth asteroid, Itokawa, five years ago and has logged about 2 billion kilometers (1.25 billion miles) since its launch in May 2003.

With the return of the Hayabusa capsule, targeted for June 13 at Australia's remote Woomera Test Range in South Australia, JAXA will have concluded a remarkable mission of exploration -- one in which NASA scientists and engineers are playing a contributing role.

"Hayabusa will be the first space mission to have made physical contact with an asteroid and returned to Earth," said Tommy Thompson, NASA's Hayabusa project manager from the Jet Propulsion Laboratory in Pasadena, Calif. "The mission and its team have faced and overcome several challenges over the past seven years. This round-trip journey is a significant space achievement and one which NASA is proud to be part of."

Launched May 9, 2003, from the Kagoshima Space Center, Uchinoura, Japan, Hayabusa was designed as a flying testbed. Its mission: to research several new engineering technologies necessary for returning planetary samples to Earth for further study. With Hayabusa, JAXA scientists and engineers hoped to obtain detailed information on electrical propulsion and autonomous navigation, as well as an asteroid sampler and sample reentry capsule.

The 510-kilogram (950-pound) Hayabusa spacecraft rendezvoused with asteroid Itokawa in September 2005. Over the next two-and-a-half months, the spacecraft made up-close and personal scientific observations of the asteroid's shape, terrain, surface altitude distribution, mineral composition, gravity, and the way it reflected the sun's rays. On Nov. 25 of that year, Hayabusa briefly touched down on the surface of Itokawa. That was only the second time in history a spacecraft descended to the surface of an asteroid (NASA's Near Earth Asteroid Rendezvous-Shoemaker spacecraft landed on asteroid Eros on Feb. 12, 2001). Hayabusa marked the first attempt to sample asteroid surface material.

The spacecraft departed Itokawa in January 2007. The road home for the technology demonstrator has been a long one, with several anomalies encountered along the way. But now the spacecraft is three days away from its home planet, and the Australian government, working closely with JAXA, has cleared the mission for landing. A team of Japanese and American navigators is guiding Hayabusa on the final leg of its journey. Together, they calculate the final trajectory correction maneuvers Hayabusa's ion propulsion system must perform for a successful homecoming.

"We have been collaborating with the JAXA navigators since the launch of the mission," said Shyam Bhaskaran, a member of JPL's Hayabusa navigation team. "We worked closely with them during the descents to the asteroid, and now are working together to guide the spacecraft back home."

To obtain the data they need, the navigation team frequently calls upon JAXA's tracking stations in Japan, as well as those of NASA's Deep Space Network, which has antennas at Goldstone, in California's Mojave Desert; near Madrid, Spain; and near Canberra, Australia. In addition, the stations provide mission planners with near-continuous communications with the spacecraft to keep them informed on spacecraft health.

"Our task is to help advise JAXA on how to best get a spacecraft traveling at 12.2 kilometers per second (27,290 miles per hour) to intersect a very specific target point 200 kilometers (120 miles) above the Earth," said Bhaskaran. "Once that is done, and the heat shield of the sample return capsule starts glowing from atmospheric friction, our job is done."

While atmospheric entry may be the end of the line for the team that has plotted the spacecraft's every move for the past 2 billion kilometers, NASA's involvement continues for the craft's final 200 kilometers (120 miles), to the surface of the Australian Outback. A joint Japanese-U.S. team operating on the ground and in the air will monitor this most critical event to help retrieve the capsule and heat shield.

"This is the second highest velocity re-entry of a capsule in history," said Peter Jenniskens, a SETI Institute scientist at NASA's Ames Research Center in Moffett Field, Calif. "This extreme entry speed will result in high heating rates and thermal loads to the capsule's heat shield. Such manmade objects entering with interplanetary speed do not happen every day, and we hope to get a ringside seat to this one."

Jenniskens is leading an international team as it monitor the final plunge of Hayabusa to Earth using NASA's DC-8 airborne laboratory, which is managed and piloted by a crew from NASA's Dryden Flight Research Center, Edwards, Calif. The DC-8 flies above most clouds, allowing an unfettered line of sight for its instrument suite measuring the shock-heated gas and capsule surface radiation emitted by the re-entry fireball.

The data acquired by the high-flying team will help evaluate how thermal protection systems behave during these super-speedy spacecraft re-entries. This, in turn, will help engineers understand what a sample return capsule returning from Mars would undergo. The Hayabusa sample return capsule re-entry observation will be similar to earlier observations by the DC-8 team of NASA's Stardust capsule return, and the re-entry of the European Space Agency's ATV-1 ("Jules Verne") automated transfer vehicle.

Soon after the sample return capsule touches down on the ground, Hayabusa team members will retrieve it and transport it to JAXA's sample curatorial facility in Sagamihara, Japan. There, Japanese astromaterials scientists, assisted by two scientists from NASA and one from Australia, will perform a preliminary cataloging and analysis of the capsule's contents.

"This preliminary analysis follows the basic protocols used for Apollo moon rocks, Genesis and Stardust samples," said Mike Zolensky, a scientist at NASA's Astromaterials Research and Exploration Science Directorate at the Johnson Space Center, Houston. "If this capsule contains samples from the asteroid, we expect it will take a year to determine the primary characteristics of the samples, and learn how to best handle them. Then the samples will be distributed to scientists worldwide for more detailed analysis."

"The Japanese and NASA engineers and scientists involved in Hayabusa's return from asteroid Itokawa are proud of their collaboration and their joint accomplishments," said Thompson. "Certainly, any samples retrieved from Itokawa will provide exciting new insights to understanding the early history of the solar system. This will be the icing on the cake, as this mission has already taught us so much. "

For more information about the Hayabusa mission, visit:
http://www.isas.jaxa.jp/e/enterp/missions/hayabusa/index.shtml
.

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Detailed Martian Scenes in New Images from Mars Orbiter

Northern hemisphere gullies on west-facing crater slope, Mars
This image shows the west-facing side of an impact crater in the mid-latitudes of Mars' northern hemisphere. › Full image and caption

Six hundred recent observations of the Mars landscape from an orbiting telescopic camera include scenes of sinuous gullies, geometrical ridges and steep cliffs.

Each of the 600 newly released observations from the High Resolution Imaging Science Experiment (HiRISE) camera aboard NASA's Mars Reconnaissance Orbiter covers an area of several square miles on Mars and reveals details as small as desks.

The HiRISE images taken from April 5 to May 6, 2010, are now available on NASA's Planetary Data System and the camera team's website.

The camera is one of six instruments on NASA's Mars Reconnaissance Orbiter, which reached Mars in 2006. For more information about the mission, see http://mars.jpl.nasa.gov/mro/.

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NASA Rover Finds Clue to Mars’ Past and Environment for Life

Lengthy detective work with data NASA's Mars Exploration Rover  Spirit collected in late 2005 has confirmed that an outcrop called  'Comanche'
Lengthy detective work with data NASA's Mars Exploration Rover Spirit collected in late 2005 has confirmed that an outcrop called "Comanche" contains a mineral indicating that a past environment was wet and non-acidic, possibly favorable to life.
› Full image and caption
Rocks examined by NASA's Spirit Mars Rover hold evidence of a wet, non-acidic ancient environment that may have been favorable for life. Confirming this mineral clue took four years of analysis by several scientists.

An outcrop that Spirit examined in late 2005 revealed high concentrations of carbonate, which originates in wet, near-neutral conditions, but dissolves in acid. The ancient water indicated by this find was not acidic.

NASA's rovers have found other evidence of formerly wet Martian environments. However the data for those environments indicate conditions that may have been acidic. In other cases, the conditions were definitely acidic, and therefore less favorable as habitats for life.

Laboratory tests helped confirm the carbonate identification. The findings were published online Thursday, June 3 by the journal Science.

"This is one of the most significant findings by the rovers," said Steve Squyres of Cornell University in Ithaca, N.Y. Squyres is principal investigator for the Mars twin rovers, Spirit and Opportunity, and a co-author of the new report. "A substantial carbonate deposit in a Mars outcrop tells us that conditions that could have been quite favorable for life were present at one time in that place. "

Spirit inspected rock outcrops, including one scientists called Comanche, along the rover's route from the top of Husband Hill to the vicinity of the Home Plate plateau which Spirit has studied since 2006. Magnesium iron carbonate makes up about one-fourth of the measured volume in Comanche. That is a tenfold higher concentration than any previously identified for carbonate in a Martian rock.

"We used detective work combining results from three spectrometers to lock this down," said Dick Morris, lead author of the report and a member of a rover science team at NASA's Johnson Space Center in Houston."The instruments gave us multiple, interlocking ways of confirming the magnesium iron carbonate, with a good handle on how much there is."

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Massive carbonate deposits on Mars have been sought for years without much success. Numerous channels apparently carved by flows of liquid water on ancient Mars suggest the planet was formerly warmer, thanks to greenhouse warming from a thicker atmosphere than exists now. The ancient, dense Martian atmosphere was probably rich in carbon dioxide, because that gas makes up nearly all the modern, very thin atmosphere.

It is important to determine where most of the carbon dioxide went. Some theorize it departed to space. Others hypothesize that it left the atmosphere by the mixing of carbon dioxide with water under conditions that led to forming carbonate minerals. That possibility, plus finding small amounts of carbonate in meteorites that originated from Mars, led to expectations in the 1990s that carbonate would be abundant on Mars. However, mineral-mapping spectrometers on orbiters since then have found evidence of localized carbonate deposits in only one area, plus small amounts distributed globally in Martian dust.

Morris suspected iron-bearing carbonate at Comanche years ago from inspection of the rock with Spirit's Moessbauerpectrometer, which provides information about iron-containing minerals. Confirming evidence from other instruments emerged slowly. The instrument with the best capability for detecting carbonates, the Miniature Thermal Emission Spectrometer, had its mirror contaminated with dust earlier in 2005, during a wind event that also cleaned Spirit's solar panels.

"It was like looking through dirty glasses," said Steve Ruff of Arizona State University in Tempe, Ariz., another co-author of the report. "We could tell there was something very different about Comanche compared with other outcrops we had seen, but we couldn't tell what it was until we developed a correction method to account for the dust on the mirror."

Spirit's Alpha Particle X-ray Spectrometer instrument detected a high concentration of light elements, a group including carbon and oxygen, that helped quantify the carbonate content.

The rovers landed on Mars in January 2004 for missions originally planned to last three months. Spirit has been out of communication since March 22 and is in a low-power hibernation status during Martian winter. Opportunity is making steady progress toward a large crater, Endeavour, which is about seven miles away.

NASA's Jet Propulsion Laboratory, Pasadena, manages the Mars Exploration Rovers for the agency's Science Mission Directorate in Washington. For more information about the rovers, visit:

http://www.nasa.gov/rovers

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As the Sun Awakens, NASA Keeps a Wary Eye on Space Weather

Earth and space are about to come into contact in a way that's new to human history. To make preparations, authorities in Washington DC are holding a meeting: The Space Weather Enterprise Forum at the National Press Club on June 8th.

Richard Fisher, head of NASA's Heliophysics Division, explains what it's all about:

"The sun is waking up from a deep slumber, and in the next few years we expect to see much higher levels of solar activity. At the same time, our technological society has developed an unprecedented sensitivity to solar storms. The intersection of these two issues is what we're getting together to discuss."

The National Academy of Sciences framed the problem two years ago in a landmark report entitled "Severe Space Weather Events—Societal and Economic Impacts." It noted how people of the 21st-century rely on high-tech systems for the basics of daily life. Smart power grids, GPS navigation, air travel, financial services and emergency radio communications can all be knocked out by intense solar activity. A century-class solar storm, the Academy warned, could cause twenty times more economic damage than Hurricane Katrina.

Much of the damage can be mitigated if managers know a storm is coming. Putting satellites in 'safe mode' and disconnecting transformers can protect these assets from damaging electrical surges. Preventative action, however, requires accurate forecasting—a job that has been assigned to NOAA.

"Space weather forecasting is still in its infancy, but we're making rapid progress," says Thomas Bogdan, director of NOAA's Space Weather Prediction Center in Boulder, Colorado.

Bogdan sees the collaboration between NASA and NOAA as key. "NASA's fleet of heliophysics research spacecraft provides us with up-to-the-minute information about what's happening on the sun. They are an important complement to our own GOES and POES satellites, which focus more on the near-Earth environment."

Among dozens of NASA spacecraft, he notes three of special significance: STEREO, SDO and ACE.

STEREO (Solar Terrestrial Relations Observatory) is a pair of spacecraft stationed on opposite sides of the sun with a combined view of 90% of the stellar surface. In the past, active sunspots could hide out on the sun's farside, invisible from Earth, and then suddenly emerge over the limb spitting flares and CMEs. STEREO makes such surprise attacks impossible.

SDO (the Solar Dynamics Observatory) is the newest addition to NASA's fleet. Just launched in February, it is able to photograph solar active regions with unprecedented spectral, temporal and spatial resolution. Researchers can now study eruptions in exquisite detail, raising hopes that they will learn how flares work and how to predict them. SDO also monitors the sun's extreme UV output, which controls the response of Earth's atmosphere to solar variability.

Bogdan's favorite NASA satellite, however, is an old one: the Advanced Composition Explorer (ACE) launched in 1997. "Where would we be without it?" he wonders. ACE is a solar wind monitor. It sits upstream between the sun and Earth, detecting solar wind gusts, billion-ton CMEs, and radiation storms as much as 30 minutes before they hit our planet.

"ACE is our best early warning system," says Bogdan. "It allows us to notify utility and satellite operators when a storm is about to hit.”

NASA spacecraft were not originally intended for operational forecasting—"but it turns out that our data have practical economic and civil uses," notes Fisher. "This is a good example of space science supporting modern society."

2010 marks the 4th year in a row that policymakers, researchers, legislators and reporters have gathered in Washington DC to share ideas about space weather. This year, forum organizers plan to sharpen the focus on critical infrastructure protection. The ultimate goal is to improve the nation’s ability to prepare, mitigate, and respond to potentially devastating space weather events.

"I believe we're on the threshold of a new era in which space weather can be as influential in our daily lives as ordinary terrestrial weather." Fisher concludes. "We take this very seriously indeed."

For more information about the meeting, please visit the Space Weather Enterprise Forum home page at http://www.nswp.gov/swef/swef_2010.html.

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NASA Langley to Break Ground on Hydro Impact Basin

What goes up must come down, and it will be NASA Langley Research Center's job to make sure that when astronauts return from space, they land safely.

On June 8, NASA Langley will break ground on a $1.7 million Hydro Impact Basin that will serve to validate and certify that future space vehicles, such as NASA's Orion crew module, are designed for safe water landings.

The water basin will be 115 feet (35 m) long, 90 feet (27.4 m) wide and 20 feet (6.1 m) deep and will be built at the west end of Langley's historic Landing and Impact Research Facility, also known as the Gantry, where Neil Armstrong trained for walking on the moon. Construction will begin mid-June and will be completed by December 2010.

A series of water impact tests will be conducted using Orion drop test articles beginning in the spring of 2011. These tests will initially validate and improve the computer models of impact and acoustic loads used in the design and engineering process, and will ultimately qualify the final vehicle design for flight.

"We are excited about being a part of the nation's next space vehicle and it's landing system," said Lynn Bowman, who is managing the series of tests for the Orion project. "Our team has been involved with furthering the knowledge and testing of space vehicle landing systems and their components for the past few years."

The skill sets that NASA Langley engineers and technicians bring to the table as well as the capability of the gantry are two of the reasons the basin is being built at the center.

Bowman explains: "The Gantry provides the ability to control the orientation of the test article while imparting a vertical and horizontal impact velocity, which is required for human rating vehicles."

"This existing capability when combined with the water basin will provide a complete facility needed for landing certification of any manned spacecraft for water landing," added Bowman. "Even vehicles that do not perform a nominal water landing will need to certify for launch abort landings into water."

Additionally, NASA Langley has more than 40 years experience with conducting controlled impact/landing tests of instrumented vehicles, said Lisa Jones, head of the Structural Testing Branch at NASA Langley.

NASA Langley's Gantry, built in 1963, was originally used to model lunar gravity. But after the Apollo program ended, it was transformed into the Impact Dynamics Research Facility and was used to test the crash worthiness of aircraft and rotorcraft.

In 2006 the Gantry experienced a revitalization as the country shifted its focus back to space exploration. The 240-foot (73 m) high Gantry provided engineers and astronauts a means to prepare for Orion's return to Earth.

When testing began in 2006, it was thought that a dry landing on Earth would be the preferred landing for the Orion capsule as it returned from space. During this phase, engineers studied the use of airbags during landings and dropped a total of 73 test articles, including a full-scale model of the Crew exploration vehicle, with different generations of airbags attached to the bottom.

More tests followed, including a series that evaluated the crew module's energy absorbing seat system, which protects the crew during a wide range of landing conditions. Langley engineers designed and built a 20,000-pound (9,072 kg) piece of steel hardware called the Crew Impact Attenuation System (CIAS) test article, which was dropped onto crushable honeycomb material sized to represent a broad range of landing conditions Orion could face.

In all, 117 drop tests were performed.

"This team really cranked out high quality testing and excellent analysis," said Bowman, who managed the Orion Landing System Team. "117 tests is a record."

Now that ground-landing tests are complete and the decision came to design Orion for landing in the water, the team at NASA Langley is ready to shift its focus to water. The team has already gotten its feet wet with a series of elemental water impact testing that began this past fall.

During these tests engineers dropped a 20-inch (50.8 cm) hemisphere from five feet (1.5 m) into a four-foot (1.2 m) deep pool so that they could build confidence in a design tool they might use to analyze data during the full-scale water impact tests to be done at the basin.


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NASA Images Show Oil’s Invasion Along Louisiana Coast

Oil moving into Louisiana's coastal wetlands
Multiple cameras on JPL's MISR instrument on NASA's Terra spacecraft were used to create two unique views of oil moving into Louisiana's coastal wetlands.
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These images, acquired on May 24, 2010 by the Multi-angle Imaging SpectroRadiometer (MISR) instrument aboard NASA's Terra spacecraft, show the encroachment of oil from the former Deepwater Horizon rig into Louisiana's wildlife habitats. The source of the spill is located off the southeastern (bottom right) edge of the images.

Dark filaments of oil are seen approaching the shores of Blind Bay and Redfish Bay at the eastern edge of the Mississippi River delta, and also nearing Garden Island Bay and East Bay farther to the south. These areas are home to many varieties of fish. To the north, the arc-shaped pattern of land and runoff is associated with the Chandeleur Islands, which are part of the Breton National Wildlife Refuge. This refuge is the second oldest in the United States and is a habitat for dozens of seabird, shorebird and waterfowl species. Oil is reported to have reached the islands on May 6. Eighteen days later, this image shows filaments of oil crossing the island barrier -- which had been heavily eroded by Hurricane Katrina in 2005 -- and entering the Breton and Chandeleur Sounds.

The left-hand image contains data from MISR's vertical-viewing camera. It is shown in near-true color, except that data from the instrument's near-infrared band, where vegetation appears bright, have been blended with the instrument's green band to enhance the appearance of vegetation.

The Mississippi River delta is located below the image center. The slick is seen approaching the delta from the lower right, and filaments of oil are also apparent farther to the north (towards the top). The oil is made visible by sun reflecting off the sea surface at the same angle from which the instrument is viewing it, a phenomenon known as sunglint. Oil makes the surface look brighter under these viewing conditions than it would if no oil were present. However, other factors can also cause enhanced glint, such as reduced surface wind speed. To separate glint patterns due to oil from these other factors, additional information from MISR's cameras is used in the right-hand image.

Previous MISR imagery of the spill shows that the contrast of the oil against the surroundings is enhanced by using a combination of vertical views and oblique-angle views. The right-hand panel was constructed by combining data from several MISR channels. In this false-color view, oil appears in shades of inky blue to black; silt-laden water due to runoff from the Mississippi River shows up as orange, red and violet; and land and clouds appear in shades of cyan.

The images cover an area measuring 110 by 119 kilometers (68 by 74 miles).

Read more at http://photojournal.jpl.nasa.gov/catalog/?IDNumber=pia13174

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On Guard

At NASA's Kennedy Space Center in Florida, an adult osprey guards its young in a nest built on a platform in the press site parking lot, backdropped by the 209-foot by 110-foot American flag painted on the side of the Vehicle Assembly Building. The Merritt Island National Wildlife Refuge coexists with Kennedy Space Center and provides a habitat for 330 species of birds, including the osprey, and a variety of other wildlife. Kennedy's press site is located at the turn basin in Launch Complex 39, making it an ideal osprey nesting place.

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Backwards Black Holes Might Make Bigger Jets

artist’s concept showing a galaxy with a supermassive black  hole at its core
Going against the grain may turn out to be a powerful move for black holes. New research suggests supermassive black holes that spin backwards might produce more ferocious jets of gas. The results have broad implications for how galaxies change over time.

"A lot of what happens in an entire galaxy depends on what's going on in the miniscule central region where the black hole lies," said theoretical astrophysicist David Garofalo of NASA's Jet Propulsion Laboratory in Pasadena, Calif. Garofalo is lead author of a new paper that appeared online May 27 in the Monthly Notices of the Royal Astronomical Society. Other authors are Daniel A. Evans of the Massachusetts Institute of Technology, Cambridge, Mass., and Rita M. Sambruna of NASA Goddard Space Flight Center, Greenbelt, Md.

Black holes are immense distortions of space and time with gravity that is so great, even light itself cannot escape. Astronomers have known for more than a decade that all galaxies, including our own Milky Way, are anchored by tremendous, so-called supermassive black holes, containing billions of suns' worth of mass. The black holes are surrounded and nourished by disks of gas and dust, called accretion disks. Powerful jets stream out from below and above the disks like lasers, and fierce winds blow off from the disks themselves.

The black holes can spin either in the same direction as the disks, called prograde black holes, or against the flow - the retrograde black holes. For decades, astronomers thought that the faster the spin of the black hole, the more powerful the jet. But there were problems with this "spin paradigm" model. For example, some prograde black holes had been found with no jets.

Garofalo and his colleagues have been busy flipping the model on its head. In previous papers, they proposed that the backward, or retrograde, black holes spew the most powerful jets, while the prograde black holes have weaker or no jets.

The new study links the researchers' theory with observations of galaxies across time, or at varying distances from Earth. They looked at both "radio-loud" galaxies with jets, and "radio-quiet" ones with weak or no jets. The term "radio" comes from the fact that these particular jets shoot out beams of light mostly in the form of radio waves.

The results showed that more distant radio-loud galaxies are powered by retrograde black holes, while relatively closer radio-quiet objects have prograde black holes. According to the team, the supermassive black holes evolve over time from a retrograde to a prograde state.

"This new model also solves a paradox in the old spin paradigm," said David Meier, a theoretical astrophysicist at JPL not involved in the study. "Everything now fits nicely into place."

The scientists say that the backward black holes shoot more powerful jets because there's more space between the black hole and the inner edge of the orbiting disk. This gap provides more room for the build-up of magnetic fields, which fuel the jets, an idea known as the Reynold's conjecture after the theoretical astrophysicist Chris Reynolds of the University of Maryland, College Park.

"If you picture yourself trying to get closer to a fan, you can imagine that moving in the same rotational direction as the fan would make things easier," said Garofalo. "The same principle applies to these black holes. The material orbiting around them in a disk will get closer to the ones that are spinning in the same direction versus the ones spinning the opposite way."

Jets and winds play key roles in shaping the fate of galaxies. Some research shows that jets can slow and even prevent the formation of stars not just in a host galaxy itself, but also in other nearby galaxies.

"Jets transport huge amounts of energy to the outskirts of galaxies, displace large volumes of the intergalactic gas, and act as feedback agents between the galaxy's very center and the large-scale environment," said Sambruna. "Understanding their origin is of paramount interest in modern astrophysics."

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

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NASA Spacecraft Burns for Home, Then Comet

Artist's concept of Epoxi spacecraft
Artist's concept of Epoxi spacecraft. › Full image and caption
NASA's Deep Impact/Epoxi spacecraft has successfully performed a trajectory correction maneuver to refine its orbit prior to an upcoming Earth flyby June 27. The maneuver, along with the Earth flyby, will place the spacecraft on a trajectory to fly past comet Hartley 2 on Nov. 4.

The maneuver began at 2 p.m. EST (11 a.m. PST) today, when the spacecraft fired its engines for 11.3 seconds. While the burn changed the spacecraft's velocity by only 0.1 meters per second (less than a quarter mile per hour), that was all the mission's navigators requested to set the stage for an Earth gravity assist on June 27.

"While it was a small burn, it was a big step in getting us to Hartley 2," said Tim Larson, project manager of NASA's Epoxi mission. "Humanity's fifth close-up view of a comet is less than five months away."

Epoxi is an extended mission of the Deep Impact spacecraft. Its name is derived from its two tasked science investigations -- the Deep Impact Extended Investigation (DIXI) and the Extrasolar Planet Observation and Characterization (EPOCh).

The University of Maryland is the Principal Investigator institution. JPL manages Epoxi for NASA's Science Mission Directorate, Washington. The spacecraft was built for NASA by Ball Aerospace & Technologies Corp., Boulder, Colo.

For information about Epoxi, visit http://www.nasa.gov/epoxi.

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X-51A Makes Longest Scramjet Flight

X-51A, artist's conceptAn engine first validated in a NASA wind tunnel successfully made the longest supersonic combustion ramjet-powered hypersonic flight to date off the southern California coast on May 26.
The air-breathing scramjet engine, built by Pratt & Whitney Rocketdyne, burned for more than 200 seconds to accelerate the U.S. Air Force's X-51A vehicle to Mach 5, or five times the speed of sound. It broke the previous record for the longest scramjet burn in a flight test, set by NASA's X-43 vehicle.

"This is great news for the hypersonics community," said Jim Pittman, principal investigator for the Hypersonics Project of NASA's Fundamental Aeronautics Program. "It's also good for NASA's research into flight at Mach 5 or faster. We will receive the X-51 flight data for analysis and comparison to the data we obtained during ground tests at NASA Langley's 8-Foot High Temperature Tunnel and to predictions from our propulsion codes."

Air Force officials called the test -- the first of four planned -- an unqualified success. The flight is considered the first use of a practical hydrocarbon-fueled scramjet in flight.

"We are ecstatic to have accomplished most of our test points on the X-51A's very first hypersonic mission," said program manager Charlie Brink of the Air Force Research Laboratory at Wright-Patterson Air Force Base in Dayton, Ohio. "We equate this leap in engine technology as equivalent to the post-World War II jump from propeller-driven aircraft to jet engines."

The X-51A launched from Edwards Air Force Base in California, carried aloft under the left wing of an Air Force Flight Test Center B-52 Stratofortress. It was released while the B-52 flew at 50,000 feet over the Pacific Ocean Point Mugu Naval Air Warfare Center Sea Range. After release, an Army Tactical Missile solid rocket booster accelerated the X-51A to about Mach 4.8 before it and a connecting interstage were jettisoned. The launch and separation were normal, according to Brink.

The SJX61-2 engine that powered the X-51A test vehicle successfully completed ground tests simulating Mach 5 flight conditions at NASA's Langley Research Center, Hampton, Va., in 2008Once the X-51A was free of its booster and interstage, its SJY61 engine ignited, initially on a mix of ethylene, similar to lighter fluid, and JP-7 jet fuel then exclusively on JP-7 jet fuel. The flight reached an altitude of about 70,000 feet and a peak speed of Mach 5.

Onboard sensors transmitted data to an airborne U.S. Navy P-3, as well was ground systems at Point Mugu, Vandenberg and Edwards Air Force bases in California. The flight was terminated after about 200 seconds of engine operation because of a technical issue. The X-51A was not designed to be recovered for examination, so engineers are busily examining the data to identify the cause of the problem.

Four X-51A cruisers have been built for the Air Force and the Defense Advanced Research Projects Agency by industry partners Pratt & Whitney Rocketdyne, West Palm Beach, Fla., and The Boeing Company, Palmdale, Calif. Brink said the Air Force intends to fly the three remaining X-51A flight test vehicles this fall on virtually identical flight profiles, building knowledge from each successive flight.

"This first flight was the culmination of a six-year effort by a small, but very talented AFRL, DARPA, NASA and industry development team," Brink said. "Now we will go back and really scrutinize our data. No test is perfect, and I'm sure we will find anomalies that we will need to address before the next flight. But anyone will tell you that we learn just as much, if not more, when we encounter a glitch."

The engine can produce between 400 and 1,000 pounds of thrust. Like a conventional jet engine, the SJY61 is capable of adjusting thrust throughout the X-51's flight envelope.

Hypersonic flight presents unique technical challenges with heat and pressure, which make conventional turbine engines impractical. Program officials said producing thrust with a scramjet has been compared to lighting a match in a hurricane and keeping it burning.


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AVIRIS

AVIRIS flew over the Gulf oil spill in a NASA ER-2 aircraft from NASA’s Dryden Flight Research Center, Edwards, Calif.

NASA Sensor Completes Initial Gulf Oil Spill Flights

AVIRIS airborne measurement
AVIRIS airborne measurement acquired May 17, 2010, over the site of the Deepwater Horizon BP oil rig disaster. The oil appears orange to brown.
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NASA's Airborne Visible/Infrared Imaging Spectrometer (AVIRIS) instrument collected an image over the site of the Deepwater Horizon BP oil rig disaster on May 17, 2010. Crude oil on the surface appears orange to brown. Scientists are using spectroscopic methods to analyze measurements for each point in images like this one to detail the characteristics of the oil on the surface.

AVIRIS extensively mapped the region affected by the spill during 11 flights conducted between May 6 and May 25, 2010, at the request of the National Oceanic and Atmospheric Administration. In total, AVIRIS measured more than 100,000 square kilometers (38,610 square miles) in support of the national oil spill response. The instrument flew at altitudes of up to 19,800 meters (65,000 feet) aboard a NASA ER-2 aircraft from NASA's Dryden Flight Research Center, Edwards, Calif.

AVIRIS is using imaging spectroscopy to map the occurrence and condition of oil on the surface of the Gulf, and to estimate the amount of oil on the surface to help scientists and responding agencies better understand the spill and how to address its effects. In addition, coastline maps created from the AVIRIS overflights will be used to provide a baseline of ecosystems and habitats that can be compared with data from future AVIRIS flights to assess the oil spill's impacts.

Figure 1 depicts AVIRIS imaging spectrometer measurements along the Gulf coast to measure the characteristics and condition of the ecosystem and habitat prior to possible oil contamination and impact. The location is near Johnson's Bayou and along the Gulf Beach Highway, between Port Arthur, La., to the west and Cameron, La., to the east. The west corner of the image includes part of the Texas Point National Wildlife Refuge. The 224 wavelengths of light measured by AVIRIS from visible to infrared are depicted in the top and left panels. The spectrum measured for each point in the image will be used to help assess the characteristics and conditions of the coastal ecosystems and habitats.

AVIRIS data provide scientists with many different types of information about the spill. Researchers at the U.S. Geological Survey's Spectroscopy Laboratory in Golden, Colo., are working to determine the characteristics of the oil based upon the AVIRIS measured spectral signature. As shown in Figure 2, acquired May 17, 2010, the signature of the oil measured in the infrared portion of the spectrum allows scientists to measure the occurrence and condition of oil and estimate the thickness of oil on the water's surface, Figure 3 depicts AVIRIS oil spill flight line measurements acquired on May 17, 2010, superimposed on a background regional image.

For more information on AVIRIS, visit http://aviris.jpl.nasa.gov/.

To read more and see related images, visit: http://photojournal.jpl.nasa.gov/catalog/?IDNumber=pia13167

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