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| February 2, 1999 |
Press Contact: Steve Koppes (773) 702-8366 s-koppes@uchicago.edu |
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University of Chicago preparing instruments for first asteroid landing, two missions to MarsThe first object that humans will land on the surface of an asteroid will contain a miniature version of the University of Chicago instrument that helped make aerospace history during the Mars Pathfinder mission in 1997. Chicagos alpha proton X-ray spectrometer, or APXS, which was carried aboard the Sojourner rover, provided the first-ever chemical analysis of native Martian rock during the Pathfinder mission. Now a much smaller, Chicago-built alpha X-ray spectrometer, AXS, will provide similar data during the joint U.S.-Japanese MUSES-C mission scheduled for launch to asteroid Nereus in 2002. The AXS may even play a role in selecting a sample of the asteroid for return to Earth during the mission in 2005. We are now in the final stages of design, said Thanasis Tom Economou, Senior Scientist at Chicagos Enrico Fermi Institute. The prototype is being built, and in a few months, it will be integrated with the nanorover to make sure everything works in coordination, he said. The AXS instrument is key to accomplishing mission objectives, said Donald Yeomans, a senior research scientist at NASAs Jet Propulsion Laboratory and U.S. science team leader for the asteroid lander mission. As the rover wanders around the surface of the asteroid, were counting on Toms instrument to tell us what the various soils and rocks are made of, Yeomans said. It makes a big difference as to how the object formed. Is it a chip off a bigger object or is it an accumulation of various bits and pieces of asteroids, sort of a rubble pile? The chemical composition of the asteroid can also be compared to that of meteorites found on Earth. Once we make the link between a certain type of asteroid and a certain type of meteorite, we can remotely observe asteroids and infer what theyre made of, Yeomans said. This is possible because asteroids, planets and stars have specific spectral characteristics —they give off certain types of electromagnetic radiation that depend on the objects chemical composition. Presumably, every other asteroid having the same spectral characteristics will be made of the same stuff, Yeomans said. MUSES-C is a cooperative effort between the National Aeronautics and Space Administration and Japans Institute of Space and Astronautical Science. The mission is scheduled for launch from Japan in January 2002. The spacecraft will arrive at Nereus in early April 2003 and will land later that month. Nereus, discovered in 1982, measures less than a mile in diameter. When the spacecraft is 50 feet above the surface, it will gently drop the nanorover. The spacecraft will then land, take some samples, then take off and hover nearby for a couple months while were doing the surface analysis and investigations, Economou said. There will be an attempt to do two landings, so it is conceivable that we will tell mission controllers where to land for the second time to grab a sample of particular interest. The solar-powered nanorover, mounted on four wheels, will measure only 6 inches square. It will be equipped with a camera and a near-infrared spectrometer as well as the AXS. The nanorover is a nice little toy, Economou said. It can go over much larger rocks than itself. It can also automatically right itself up after falling on its back. The APXS that Economou built for Pathfinders rover weighed 570 grams (1.2 pounds). But for MUSES-C, Economou had to think on the Lilliputian scale of Gullivers Travels. His weight limit for the nanorovers chemical analyzer is no more than 100 grams (3.5 ounces), packed into an area measuring less than 3 cubic inches. Together the AXSs alpha and X-ray detectors can identify any chemical element except hydrogen at concentrations as low as a fraction of 1 percent. The instruments design saves weight by dispensing with the proton detector, which mostly duplicates data collected by the X-ray detector, and by sharing capabilities with the nanorover. In November, Economou was one of 11 Mars Pathfinder team members and instrument developers to receive special recognition from the National Air and Space Museum of the Smithsonian Institution. The Pathfinder team received the 1998 National Air and Space Museum Trophy for Current Achievement for its demonstration of technologies and concepts for use in future Mars missions. Economou still is analyzing data collected during the Pathfinder mission, which officially ended in 1997. He also is designing and building two more APXS instruments in collaboration with the Max Planck Institute in Germany for the rovers of the Mars Surveyor 2001 and 2003 missions. The rovers of these two missions will visit more Martian sites to collect samples, some of which will be returned to Earth during a mission set for 2005. The rover for Mars 2001, called Marie Curie, is similar to Sojourner. For 2003, there will be the Athena rover, a new type of rover, capable of traveling farther distances, carrying more instruments and carrying a drill bit to collect samples, Economou said. The Athena rovers robotic arm will pick up a sample and bring it to the APXS and other instruments. After examination, the robot arm will either drop the sample on the surface or place it in a special container for return to Earth. It will be exciting times, Economou said. http://www-news.uchicago.edu/releases/99/990202.axs.shtml Last modified at 03:51 PM CST on Wednesday, June 14, 2000. | |
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