Deep Impact: excavating comet Tempel 1.

نویسندگان

  • M F A'Hearn
  • M J S Belton
  • W A Delamere
  • J Kissel
  • K P Klaasen
  • L A McFadden
  • K J Meech
  • H J Melosh
  • P H Schultz
  • J M Sunshine
  • P C Thomas
  • J Veverka
  • D K Yeomans
  • M W Baca
  • I Busko
  • C J Crockett
  • S M Collins
  • M Desnoyer
  • C A Eberhardy
  • C M Ernst
  • T L Farnham
  • L Feaga
  • O Groussin
  • D Hampton
  • S I Ipatov
  • J-Y Li
  • D Lindler
  • C M Lisse
  • N Mastrodemos
  • W M Owen
  • J E Richardson
  • D D Wellnitz
  • R L White
چکیده

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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عنوان ژورنال:
  • Science

دوره 310 5746  شماره 

صفحات  -

تاریخ انتشار 2005