The shape, topography, and geology of Tempel 1 from Deep Impact observations

被引:106
作者
Thomas, Peter C.
Veverka, J.
Belton, Michael J. S.
Hidy, Alan
A'Hearn, Michael F.
Farnharn, T. L.
Groussin, Olivier
Li, Jian-Yang
McFadden, Lucy A.
Sunshine, Jessica
Wellnitz, Dennis
Lisse, Carey
Schultz, Peter
Meech, Karen J.
Delamere, W. Alan
机构
[1] Cornell Univ, Ctr Radiophys & Space Res, Ithaca, NY 14850 USA
[2] Belton Space Explorat Initiat, Tucson, AZ 85716 USA
[3] Utah State Univ, Dept Geol, Logan, UT 84322 USA
[4] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
[5] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[6] Brown Univ, Dept Geol Sci, Providence, RI 02912 USA
[7] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[8] Delamere Support Serv, Boulder, CO 80306 USA
关键词
comets; nucleus; Comet Tempel-I;
D O I
10.1016/j.icarus.2006.12.013
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Deep Impact images of the nucleus of Comet Tempel 1 reveal pervasive layering, possible impact craters, flows with smooth upper surfaces, and erosional stripping of material. There are at least 3 layers 50-200 m thick that appear to extend deep into the nucleus, and several layers 1-20 m thick that parallel the Surface and are being eroded laterally. Circular depressions show geographical variation in their forms and suggest differences in erosion rates or style over scales > 1 km. The stratigraphic arrangement of these features suggests that the comet experienced substantial periods of little erosion. Smooth surfaces trending downslope suggest some form of eruption of materials from this highly porous object. The Deep Impact images show that the nucleus of Tempel 1 cannot be modeled simply as either an onion-layer or rubble pile structure. (c) 2007 Elsevier Inc. All rights reserved.
引用
收藏
页码:4 / 15
页数:12
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