Assessment of Mars Exploration Rover landing site predictions
Author(s) -
M. P. Golombek,
R. E. Arvidson,
J. F. Bell,
P. R. Christensen,
J. A. Crisp,
L. S. Crumpler,
B. L. Ehlmann,
R. L. Fergason,
J. A. Grant,
R. Greeley,
A. F. C. Haldemann,
D. M. Kass,
T. J. Parker,
J. T. Schofield,
S. W. Squyres,
Richard W. Zurek
Publication year - 2005
Publication title -
nature
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 15.993
H-Index - 1226
eISSN - 1476-4687
pISSN - 0028-0836
DOI - 10.1038/nature03600
Subject(s) - mars exploration program , astrobiology , exploration of mars , mars landing , mars rover , geology , aerospace engineering , environmental science , aeronautics , engineering , physics
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.
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