Assessment of Mars Exploration Rover landing site predictions

被引:78
作者
Golombek, MP
Arvidson, RE
Bell, JF
Christensen, PR
Crisp, JA
Crumpler, LS
Ehlmann, BL
Fergason, RL
Grant, JA
Greeley, R
Haldemann, AFC
Kass, DM
Parker, TJ
Schofield, JT
Squyres, SW
Zurek, RW
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[2] Washington Univ, St Louis, MO 63130 USA
[3] Cornell Univ, Ithaca, NY 14853 USA
[4] Arizona State Univ, Tempe, AZ 85287 USA
[5] New Mexico Museum Nat Hist & Sci, Albuquerque, NM 87104 USA
[6] Univ Oxford, Oxford OX1 3PG, England
[7] Smithsonian Inst, Washington, DC 20560 USA
关键词
D O I
10.1038/nature03600
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
Comprehensive analyses of remote sensing data during the three-year effort to select the Mars Exploration Rover landing sites at Gusev crater and at Meridiani Planum correctly predicted the atmospheric density profile during entry and descent and the safe and trafficable surfaces explored by the two rovers. The Gusev crater site was correctly predicted to be a low-relief surface that was less rocky than the Viking landing sites but comparably dusty. A dark, low-albedo, flat plain composed of basaltic sand and haematite with very few rocks was expected and found at Meridiani Planum. These results argue that future efforts to select safe landing sites based on existing and acquired remote sensing data will be successful. In contrast, geological interpretations of the sites based on remote sensing data were less certain and less successful, which emphasizes the inherent ambiguities in understanding surface geology from remotely sensed data and the uncertainty in predicting exactly what materials will be available for study at a landing site.
引用
收藏
页码:44 / 48
页数:5
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