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Deep Impact: Excavating Comet Tempel 1

Authors :
H. J. Melosh
Donald Hampton
Peter H. Schultz
Olivier Groussin
Dennis D. Wellnitz
Jessica M. Sunshine
R. L. White
Michael F. A'Hearn
Don J. Lindler
M. W. Baca
Jian-Yang Li
Kenneth P. Klaasen
Peter C. Thomas
I. Busko
Carey M. Lisse
J. Veverka
Mark Desnoyer
James E. Richardson
C. A. Eberhardy
Carolyn M. Ernst
Lucy A. McFadden
Karen J. Meech
Steven M. Collins
C. J. Crockett
M. J. S. Belton
Tony L. Farnham
N. Mastrodemos
William M. Owen
Jochen Kissel
Donald K. Yeomans
W. A. Delamere
Lori M. Feaga
Sergei I. Ipatov
Source :
Science. 310:258-264
Publication Year :
2005
Publisher :
American Association for the Advancement of Science (AAAS), 2005.

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 (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.

Details

ISSN :
10959203 and 00368075
Volume :
310
Database :
OpenAIRE
Journal :
Science
Accession number :
edsair.doi.dedup.....6d7e68307a50752bd6055cc055895baf
Full Text :
https://doi.org/10.1126/science.1118923