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Deep Impact: excavating comet Tempel 1
Authors:A'Hearn M F  Belton M J S  Delamere W A  Kissel J  Klaasen K P  McFadden L A  Meech K J  Melosh H J  Schultz P H  Sunshine J M  Thomas P C  Veverka J  Yeomans D K  Baca M W  Busko I  Crockett C J  Collins S M  Desnoyer M  Eberhardy C A  Ernst C M  Farnham T L  Feaga L  Groussin O  Hampton D  Ipatov S I  Li J-Y  Lindler D  Lisse C M  Mastrodemos N  Owen W M  Richardson J E  Wellnitz D D  White R L
Institution:University of Maryland, College Park, MD 20742, USA. ma@astro.umd.edu
Abstract:Deep Impact collided with comet Tempel 1, excavating a crater controlled by gravity. The comet's outer layer is composed of 1- to 100-micrometer fine particles with negligible strength (<65 pascals). Local gravitational field and average nucleus density (600 kilograms per cubic meter) are estimated from ejecta fallback. Initial ejecta were hot (>1000 kelvins). A large increase in organic material occurred during and after the event, with smaller changes in carbon dioxide relative to water. On approach, the spacecraft observed frequent natural outbursts, a mean radius of 3.0 +/- 0.1 kilometers, smooth and rough terrain, scarps, and impact craters. A thermal map indicates a surface in equilibrium with sunlight.
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