[meteorite-list] The Fiery Return of NASA's Space Dust Cargo
From: Gerald Flaherty <grf2_at_meteoritecentral.com>
Date: Wed Nov 30 20:22:18 2005 Message-ID: <002b01c5f615$9b85a3e0$6402a8c0_at_Dell> Wow! what an incredible range of information potential this may provide!!!!!! Jerry ----- Original Message ----- From: "Ron Baalke" <baalke_at_zagami.jpl.nasa.gov> To: "Meteorite Mailing List" <meteorite-list_at_meteoritecentral.com> Sent: Wednesday, November 30, 2005 12:15 PM Subject: [meteorite-list] The Fiery Return of NASA's Space Dust Cargo > > http://www.nasa.gov/centers/ames/research/exploringtheuniverse/stardust.html > > John Bluck > NASA Ames Research Center, Moffett Field, Calif. > Phone: 650/604-5026 > E-mail: jbluck_at_mail.arc.nasa.gov > > The Fiery Return of NASA's Space Dust Cargo > November 29, 2005 > > In search of clues about the origin of life on Earth and other secrets, > a crew flying on a NASA DC-8 aircraft will study the small, speeding > Stardust capsule returning from space early in 2006. > > Two years earlier, in January 2004, the Stardust spacecraft flew within > 147 miles (236 kilometers) of the comet Wild 2 (VILT-TWO) and survived > the high-speed impact of millions of dust particles and small rocks up > to nearly two-tenths of an inch (one half centimeter) across. With its > tennis-racket-shaped collector extended, Stardust captured thousands of > comet particles. > > The returning Stardust capsule will strike Earth's atmosphere during the > early morning darkness in mid-January 2006, at eight miles (12.8 > kilometers) per second ??" more than 10 times faster than a speeding > bullet. That is fast enough to go from San Francisco to Los Angeles in > only one minute. The DC-8 crew will face the daunting task of tracking > and observing the 101-pound (45.7 kilogram) conical object as it hurtles > through the atmosphere and slows before the spacecraft finally > parachutes down in a Utah desert. > > Scientists aboard the DC-8 also will assess how well the Stardust > capsule's heat shield protects its precious cargo of comet dust and > interstellar grains. > > Though scientists will study this captured space dust for years to come, > the separate team of researchers aboard the DC-8 will gather data only > during the brief re-entry of the space capsule into Earth's atmosphere. > > The mini, Apollo-like capsule will shoot down through the air at the > highest spacecraft re-entry speed into Earth's atmosphere ever, > generating extremely high temperatures. The capsule's special > carbon-based heat shield, developed at NASA Ames Research Center in > California's Silicon Valley, will protect the priceless cargo of comet > dust and interstellar grains. During this blistering re-entry, the DC-8 > crew will take surface-temperature and shock-radiation measurements of > the heat shield as part of it burns away. Shock radiation is light > emitted from extremely hot air. Scientists will study this light to > learn how hot the capsule gets and what chemical reactions are taking > place. These chemical reactions will result from of the violent breakup > of air molecules that collide with vapor in front of the speeding capsule. > > At the same time as the DC-8 crew is flying its mission, amateur > astronomers, willing to endure the cold of the bitter winter, may > contribute to the study by simply photographing the incoming capsule, > noting their global positions and later providing that information to > mission scientists. > > One of the goals of the researchers aboard the DC-8 is to measure the > capsule's re-entry brightness. Scientists expect it to peak at > approximately the brilliance of Venus for roughly 90 seconds. The > capsule will be brightest 37 miles (60 kilometers) high over the town of > Carlin, Nev., as the spacecraft approaches. This will occur in the early > morning cold and darkness on Sunday, Jan. 15, 2006, shortly before the > spacecraft parachutes to a landing at 3 a.m. MST. The landing zone is a > restricted area ??" the Utah Test and Training Range, located southwest of > Salt Lake City. > > "As the observer sees the approaching capsule, it will appear as a point > of light," said Peter Jenniskens, principal investigator of the Stardust > Sample Return Capsule Re-entry Observing Campaign. Jenniskens is a > meteor astronomer at the SETI Institute, Mountain View, Calif. "After it > passes the observer, the back of the capsule will be less bright, and it > will quickly fade. Each observer will have a different experience," > Jenniskens added. > > The special carbon-based heat shield material designed to protect the > Stardust capsule is a candidate for potential inclusion on NASA's next > planned spaceship, the Crew Exploration Vehicle (CEV), NASA engineers > say. This prospective future use is one reason they plan to study the > Stardust capsule as it slams into Earth's atmosphere, and the shield > rapidly heats due to friction with the air. > > "Our main interest is the performance of the heat shield and the > chemistry that takes place in it as it vaporizes and erodes during the > descent and re-entry," said Dave Jordan, a NASA Ames engineer and > project manager for the capsule observation mission. > > The spacecraft will penetrate Earth's atmosphere as if it were a normal > meteor, according to Jenniskens. > > "The capsule will be an artificial meteor that we can study for clues > about how life's molecules may have first formed on Earth," Jenniskens > said. "The carbon from the heat shield will react in the shockwave, > making new molecules that would have seeded Earth at the time of the > origin of life. The carbon in comet dust could have done the same," > Jenniskens ventured. > > After scientists examine the dust carried within the capsule, they may > soon learn what carbon compounds are found in comet dust. The spacecraft > flew through comet Wild-2's dust cloud and captured some of it in a very > light substance, called 'aerogel.' > > "It's a little > bit like collecting BBs by shooting them into Styrofoam," said Scott > Sandford, an astrophysicist at NASA Ames and a Stardust mission > co-investigator. "Some of the grains are likely to have exotic isotopic > ratios that will give us an indication that we're looking at materials > that aren't as old as the solar system, but are, in fact, older than the > solar system," Sandford asserted. > > Another mission objective was to expose the spacecraft to the > interstellar dust stream for 150 days to grab interstellar particles. > After collecting the particles, the aerogel collector retracted into the > capsule. Stardust will be the first mission to capture and return a > substantial sample from outside Earth's moon system. > > Watching the Stardust re-entry > > The capsule will approach the landing zone from a westerly direction. > The best opportunities for viewing the re-entry will be along Highway 80 > between Carlin, Nev., and Elko, Nev., and further east to the Utah > border, where the capsule's front side can be observed before it passes > over the observer on the ground. The peak brightness will decrease > further from Carlin, lessening to about the brightness of Venus (+0 > magnitude) when seen from Boise, Idaho, and Salt Lake City. Viewing will > not be as good at sites east of Carlin where the craft will be seen from > behind. > > For certain viewing locations just north of the trajectory line, the > capsule will appear to pass by the moon (above it, or below it, > depending on the viewer's location). By choosing their positions > carefully, some observers will be able to see the capsule pass in front > of the moon. As seen by the naked eye, the capsule will disappear in the > glare of moonlight, but by looking through telescopes, observers may see > a tiny dot, perhaps trailed by a dark wake of dissipating heat shield > material and hot air. The trail may form a thin line behind the capsule, > especially near the point of peak brightness where ablation (erosion of > the heat shield and dissipation of the heat that results from the > friction of the heat shield with the atmosphere) is most intense. > > "If somebody could see that line, that would be fantastic, because it > would tell us how much carbon is being lost by the heat shield at that > moment," observed Jenniskens. "It would be better yet if several > observers at different locations were to videotape the entry of the > capsule appearing in front of the moon because then we could trace the > ablation of the carbon along the capsule's trajectory, especially at > locations between Carlin and Elko," he added. Videographers should fix > the focus of their cameras at 'infinity,' because auto focus may be > unreliable for nighttime recording, according to mission technicians. > > The best way to see the capsule pass in front of the moon would be with > a large telescope at high magnification, according to Jenniskens. Due to > the long viewing distances, the tiny capsule will appear as a dark dot, > only 1-2 arcseconds across, but darker if the capsule is clearly > visible. One arcsecond is 1/3600th of a degree. > > Moving at many times the speed of sound, the capsule will take only two > to three video frames to appear to pass by the moon. > > When the Stardust capsule does not appear to be near the moon, observers > should look for 'chemi-luminance,' a faint glow in the wake of the > capsule. This glow may be created by chemical reactions between the hot > air in the capsule's wake and ozone in the air. > > According to scientists, observers using the naked eye will likely see > the capsule as a very bright pinpoint of pink-white light. This color is > the signature of excited atoms and molecules in the shock wave formed as > the capsule strikes the atmosphere, according to George Raiche of NASA > Ames. > > Light emission is caused by violent breakup of the air molecules that > collide with the speeding capsule. For the most part, these molecules > are oxygen and nitrogen atoms and ionized nitrogen molecules, Jenniskens > noted. Ablation products could cause violet light resulting from > chemical reactions between carbon and air. > > "What the re-entry of the capsule will tell us is how those carbon > compounds might be chemically changed when comet dust enters Earth's > atmosphere. Life's molecules need nitrogen and oxygen combined so that > they can become useful ingredients for living things," Jenniskens said. > > In effect, the capsule will be an artificial meteor that we can study > for clues about how life's molecules may have first formed on Earth, > according to Jenniskens. "This will be the first time we will have > scheduled observation of a manmade object entering the planet's > atmosphere at speeds comparable to natural fireballs," he noted. > > While most of this chemistry happening at high speed is very quick, > complex and elusive, it is possible to recognize the most brightly > radiating compounds in this fiery process and to look for clues about > what conditions the molecules must endure. > > Finally, the conical spacecraft will drop straight down over the > restricted zone in Utah, floating down by parachute. > > Once the capsule has landed in Utah, researchers will collect debris > from the surface of the shield and study how much of the heat shield was > lost during re-entry. "This is called an ablative heat shield," said > Michael J. Wright of NASA Ames, another scientist working on the > project. "By vaporizing some of the material from its surface, the heat > shield vapor carries some of the heat from friction away from the > capsule, keeping the payload cool," Wright explained. > > After they recover the capsule and its precious cargo, scientists will > transport the space dust to a laboratory at NASA Johnson Space Center, > Houston, for analysis. > > "The sample(s) brought back from comet Wild-2 will tell us is what > carbon compounds are in cometary dust," Jenniskens observed. > > "There'll be a small team of us at Johnson Space Center who will assess > what we actually got back from the comet so we can verify we did get a > useful sample," Sandford said. "A small portion of the samples will then > be used to make a preliminary study of the returned material. After the > preliminary examination is complete, all the samples will be made > available to the general scientific community for more detailed study. > My guess is people will be asking for and working on these samples for > decades to come." > > Besides NASA Ames and the SETI Institute, several other institutions are > partners in the NASA DC-8 airborne study: the University of Alaska at > Fairbanks; the University of Utah at Logan; Sandia National > Laboratories; Los Alamos National Laboratories; the Aerospace > Corporation; the U.S. Air Force Academy; Kobe University, Japan; and > Stuttgart University, Germany. The University of North Dakota operates > the DC-8 aircraft for NASA. > > Amateur astronomers who wish to submit photographic, video or other data > to Jenniskens will find directions and more information about the > airborne campaign at: > > http://reentry.arc.nasa.gov > > The Stardust spacecraft was launched on Feb. 7, 1999, from Cape > Canaveral Air Station, Fla., aboard a Delta II rocket. NASA's Jet > Propulsion Laboratory, Pasadena, Calif., manages Stardust, a part of > NASA's Discovery Program of low-cost, highly focused science missions. > For more information about Stardust and a background audio interview > with Sandford, visit: > > http://stardust.jpl.nasa.gov > > http://www.nasa.gov/centers/ames/multimedia/audio/sdust/sdust.html > > > ______________________________________________ > Meteorite-list mailing list > Meteorite-list_at_meteoritecentral.com > http://six.pairlist.net/mailman/listinfo/meteorite-list Received on Wed 30 Nov 2005 08:21:50 PM PST |
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