Imaging of asteroid 433 Eros during NEAR's flyby reconnaissance

被引:57
|
作者
Veverka, J
Thomas, PC
Bell, JF
Bell, M
Carcich, B
Clark, B
Harch, A
Joseph, J
Martin, P
Robinson, M
Murchie, S
Izenberg, N
Hawkins, E
Warren, J
Farquhar, R
Cheng, A
Dunham, D
Chapman, C
Merline, WJ
McFadden, L
Wellnitz, D
Malin, M
Owen, WM
Miller, JK
Williams, BG
Yeomans, DK
机构
[1] Cornell Univ, Ithaca, NY 14853 USA
[2] Northwestern Univ, Dept Geol Sci, Evanston, IL 60208 USA
[3] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[4] SW Res Inst, Boulder, CO 80302 USA
[5] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
[6] Main Space Sci Syst Inc, San Diego, CA USA
[7] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
D O I
10.1126/science.285.5427.562
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
During the 23 December 1998 flyby of asteroid 433 Eros, the Near-Earth Asteroid Rendezvous (NEAR) spacecraft obtained 222 images of Eros, as well as supporting spectral observations. The images cover slightly more than two-thirds of Eros (best resolution is similar to 400 meters per pixel) and reveal an elongated, cratered body with a linear feature extending for at least 20 kilometers. Our observations show that Eros has dimensions of 33 X 13 X 13 kilometers. The volume, combined with the mass determined by the NEAR radio science experiment, Leads to a density of 2.5 +/- 0.8 grams per cubic centimeter. This relatively high density, and the presence of an extensive Linear feature, suggest that Eros may be a structurally coherent body.
引用
收藏
页码:562 / 564
页数:3
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