Deep Impact: Excavating comet Tempel 1

被引:630
作者
A'Hearn, MF [1 ]
Belton, MJS
Delamere, WA
Kissel, J
Klaasen, KP
McFadden, LA
Meech, KJ
Melosh, HJ
Schultz, PH
Sunshine, JM
Thomas, PC
Veverka, J
Yeomans, DK
Baca, MW
Busko, I
Crockett, CJ
Collins, SM
Desnoyer, M
Eberhardy, CA
Ernst, CM
Farnham, TL
Feaga, L
Groussin, O
Hampton, D
Ipatov, SI
Li, JY
Lindler, D
Lisse, CM
Mastrodemos, N
Owen, WM
Richardson, JE
Wellnitz, DD
White, RL
机构
[1] Univ Maryland, College Pk, MD 20742 USA
[2] Belton Space Explorat Initiat, Tucson, AZ 85716 USA
[3] Delamere Support Serv, Boulder, CO 80301 USA
[4] Max Planck Inst Solar Syst Res, D-37191 Katlenburg Lindau, Germany
[5] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[6] Univ Hawaii, Honolulu, HI 96822 USA
[7] Univ Arizona, Tucson, AZ 85721 USA
[8] Brown Univ, Providence, RI USA
[9] SAIC, Chantilly, VA 20151 USA
[10] Cornell Univ, Ithaca, NY 14853 USA
[11] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[12] Ball Aerosp & Technol Corp, Boulder, CO 80301 USA
[13] Sigma Sci, Greenbelt, MD 20771 USA
[14] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
关键词
D O I
10.1126/science.1118923
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
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.
引用
收藏
页码:258 / 264
页数:7
相关论文
共 23 条
[1]   Deep impact: A large-scale active experiment on a cometary nucleus [J].
A'Hearn, MF ;
Belton, MJS ;
Delamere, A ;
Blume, WH .
SPACE SCIENCE REVIEWS, 2005, 117 (1-2) :1-21
[2]   Experimental ejection angles for oblique impacts: Implications for the subsurface flow-field [J].
Anderson, JLB ;
Schultz, PH ;
Heineck, JT .
METEORITICS & PLANETARY SCIENCE, 2004, 39 (02) :303-320
[3]  
[Anonymous], 1989, OXFORD MONOGRAPHS GE
[4]   Deep impact:: Working properties for the target nucleus -: Comet 9P/Tempel 1 [J].
Belton, MJ ;
Meech, KJ ;
A'Hearn, MF ;
Groussin, O ;
Mcfadden, L ;
Lisse, C ;
Fernández, YR ;
Pittichová, J ;
Hsieh, H ;
Kissel, J ;
Klaasen, K ;
Lamy, P ;
Prialnik, D ;
Sunshine, J ;
Thomas, P ;
Toth, I .
SPACE SCIENCE REVIEWS, 2005, 117 (1-2) :137-160
[5]   Deep impact mission design [J].
Blume, WH .
SPACE SCIENCE REVIEWS, 2005, 117 (1-2) :23-42
[6]   The morphology and surface processes of Comet 19/P Borrelly [J].
Britt, DT ;
Boice, DC ;
Buratti, BJ ;
Campins, H ;
Nelson, RM ;
Oberst, J ;
Sandel, BR ;
Stem, SA ;
Soderblom, LA ;
Thomas, N .
ICARUS, 2004, 167 (01) :45-53
[7]   Surface of young Jupiter family comet 81 P/Wild 2: View from the Stardust spacecraft [J].
Brownlee, DE ;
Horz, F ;
Newburn, RL ;
Zolensky, M ;
Duxbury, TC ;
Sandford, S ;
Sekanina, Z ;
Tsou, P ;
Hanner, MS ;
Clark, BC ;
Green, SF ;
Kissel, J .
SCIENCE, 2004, 304 (5678) :1764-1769
[8]   Thermal properties of Centaurs Asbolus and Chiron [J].
Fernández, YR ;
Jewitt, DC ;
Sheppard, SS .
ASTRONOMICAL JOURNAL, 2002, 123 (02) :1050-1055
[9]   Properties of the nuclei of Centaurs Chiron and Chariklo [J].
Groussin, O ;
Lamy, P ;
Jorda, L .
ASTRONOMY & ASTROPHYSICS, 2004, 413 (03) :1163-1175
[10]   CRATER EJECTA SCALING LAWS - FUNDAMENTAL FORMS BASED ON DIMENSIONAL ANALYSIS [J].
HOUSEN, KR ;
SCHMIDT, RM ;
HOLSAPPLE, KA .
JOURNAL OF GEOPHYSICAL RESEARCH, 1983, 88 (NB3) :2485-2499