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Comet 81P/Wild 2 under a microscope
Authors:Brownlee Don  Tsou Peter  Aléon Jérôme  Alexander Conel M O'd  Araki Tohru  Bajt Sasa  Baratta Giuseppe A  Bastien Ron  Bland Phil  Bleuet Pierre  Borg Janet  Bradley John P  Brearley Adrian  Brenker F  Brennan Sean  Bridges John C  Browning Nigel D  Brucato John R  Bullock E  Burchell Mark J  Busemann Henner  Butterworth Anna  Chaussidon Marc  Cheuvront Allan  Chi Miaofang  Cintala Mark J  Clark B C  Clemett Simon J  Cody George  Colangeli Luigi  Cooper George  Cordier Patrick  Daghlian C  Dai Zurong  D'Hendecourt Louis  Djouadi Zahia  Dominguez Gerardo  Duxbury Tom  Dworkin Jason P  Ebel Denton S  Economou Thanasis E  Fakra Sirine
Affiliation:Department of Astronomy, University of Washington, Seattle, WA 98195, USA. brownlee@astro.washington.edu
Abstract:The Stardust spacecraft collected thousands of particles from comet 81P/Wild 2 and returned them to Earth for laboratory study. The preliminary examination of these samples shows that the nonvolatile portion of the comet is an unequilibrated assortment of materials that have both presolar and solar system origin. The comet contains an abundance of silicate grains that are much larger than predictions of interstellar grain models, and many of these are high-temperature minerals that appear to have formed in the inner regions of the solar nebula. Their presence in a comet proves that the formation of the solar system included mixing on the grandest scales.
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