[meteorite-list] Early Results From The Sloan Digital Sky Survey
From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Thu Apr 22 09:44:11 2004 Message-ID: <200106052309.QAA04017_at_zagami.jpl.nasa.gov> http://www.sdss.org/news/releases/20010605.edr.html Sloan Digital Sky Survey Media Contacts Michael Turner Steve Koppes SDSS Scientific Spokesman University of Chicago 773-702-7974 773-702-8366 mturner_at_oddjob.uchicago.edu s-koppes@uchicago.edu Georgia Whidden Satoru Ikeuchi Institute for Advanced Study Japan Participation Group 609-734-8239 81-52-789-2427 gwhidden_at_ias.edu ikeuchi@a.phys.nagoya-u.ac.jp Michael Purdy Hans-Walter Rix The Johns Hopkins University Max-Planck-Institut für Astronomie 410-516-7906 49-6221-528-210 mcp_at_jhu.edu rix@mpia-hd.mpg.de Rene Walterbos Barbara Kennedy Nex Mexico State University Pennsylvania State University 505-646-5990 bkk1_at_psu.edu rwalterb_at_nmsu.edu Steve Schultz Vince Stricherz Princeton University University of Washington 609-258-5729 206-543-2580 sschultz_at_princeton.edu vinces@u.washington.edu Steven Dick Bruce Gillespie U.S. Naval Observatory Apache Point Observatory 202-762-0379 505-437-6822 dick.steve_at_usno.navy.mil gillespi@apo.nmsu.edu Amber Jones Ray Villard National Science Foundation Space Telescope Science Institute 703-292-8070 410-338-4514 ajones_at_nsf.gov villard@stsci.edu For release after 9:15 a.m. PDT, June 5, 2001 SDSS 01-01 Early results from the Sloan Digital Sky Survey: From under our nose to the edge of the universe Pasadena, Calif. -- Scientists of the Sloan Digital Sky Survey today (June 5) presented results based on early data from the project. The first glimpses of what will ultimately be the most comprehensive and fully digital map of the sky included identification of the two most distant objects ever observed; new light on asteroids; and the first SDSS results on the large- scale distribution of galaxies. Sky Survey collaborators also announced the release to the worldwide astronomy community of the first large piece of the digital sky. [snip] Asteroids The SDSS collaborators presented the first clear evidence for chemical segregation in the belt of asteroids between Mars and Jupiter. By viewing the asteroids in five color bands, explained Dr. Tom Quinn of the University of Washington, the SDSS survey can reliably separate individual asteroids into two main classes, rocky silicate asteroids and more primitive carbonaceous asteroids. "The SDSS observations also showed that the two types of asteroids are spatially separated," Quinn said, "with the inner belt of rocky asteroids centered at about 2.8 AU from the sun and the outer belt of carbonaceous asteroids centered at about 3.2 AU. This distribution has important implications for unraveling how the solar system formed and suggests that planet migrations that seem to be common in other planetary systems have not occurred in ours." One astronomical unit, or AU, corresponds to the distance from the sun to the earth. The SDSS asteroid sample also turned up another surprise. "There appear to be fewer asteroids smaller than about 4 km in diameter in the asteroid belt than we previously thought," said Dr. Zeljko Ivezic of Princeton University, the leader of the SDSS asteroid team. "Since the asteroid belt is believed to be the reservoir for Earth-crossing asteroids, the new SDSS observations suggest that future asteroid collisions with Earth may be less likely than previously believed." The SDSS scanning technique allows only five minutes to follow celestial objects as they move across the field of view, said Dr. Robert Lupton of Princeton University. During this time asteroids appear to move a distance just 1/1000th the size of the moon, relative to the distant stars. "Nevertheless," Lupton said, "we can reliably detect their tiny motions and even determine their orbital motions around the sun." The asteroid observations rely on precision position-finding software developed by SDSS collaborators at the US Naval Observatory. Images available: [snip] Asteroids: * Diagram of asteroid belt http://www.sdss.org/news/releases/20010605.edr.img7.html * Graph of asteroid belt cross section http://www.sdss.org/news/releases/20010605.edr.img7.html * Asteroid size distribution http://www.sdss.org/news/releases/20010605.edr.img9.html Received on Tue 05 Jun 2001 07:09:52 PM PDT |
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