Soils of Eagle Crater and Meridiani Planum at the Opportunity Rover Landing Site

Author:

Soderblom L. A.12345,Anderson R. C.12345,Arvidson R. E.12345,Bell J. F.12345,Cabrol N. A.12345,Calvin W.12345,Christensen P. R.12345,Clark B. C.12345,Economou T.12345,Ehlmann B. L.12345,Farrand W. H.12345,Fike D.12345,Gellert R.12345,Glotch T. D.12345,Golombek M. P.12345,Greeley R.12345,Grotzinger J. P.12345,Herkenhoff K. E.12345,Jerolmack D. J.12345,Johnson J. R.12345,Jolliff B.12345,Klingelhöfer G.12345,Knoll A. H.12345,Learner Z. A.12345,Li R.12345,Malin M. C.12345,McLennan S. M.12345,McSween H. Y.12345,Ming D. W.12345,Morris R. V.12345,Rice J. W.12345,Richter L.12345,Rieder R.12345,Rodionov D.12345,Schröder C.12345,Seelos F. P.12345,Soderblom J. M.12345,Squyres S. W.12345,Sullivan R.12345,Watters W. A.12345,Weitz C. M.12345,Wyatt M. B.12345,Yen A.12345,Zipfel J.12345

Affiliation:

1. U.S. Geological Survey, Flagstaff, AZ 86001, USA.

2. Jet Propulsion Laboratory, Caltech, Pasadena, CA 91109, USA.

3. Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA.

4. Department of Astronomy, Cornell University, Ithaca, NY 14853, USA.

5. NASA Ames/SETI Institute, Moffett Field, CA 94035, USA.

Abstract

The soils at the Opportunity site are fine-grained basaltic sands mixed with dust and sulfate-rich outcrop debris. Hematite is concentrated in spherules eroded from the strata. Ongoing saltation exhumes the spherules and their fragments, concentrating them at the surface. Spherules emerge from soils coated, perhaps from subsurface cementation, by salts. Two types of vesicular clasts may represent basaltic sand sources. Eolian ripples, armored by well-sorted hematite-rich grains, pervade Meridiani Planum. The thickness of the soil on the plain is estimated to be about a meter. The flatness and thin cover suggest that the plain may represent the original sedimentary surface.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference31 articles.

1. The term “soil” is used here to denote any loose unconsolidated materials that can be distinguished from rocks bedrock or strongly cohesive sediments. No implication for the presence or absence of organic materials or living matter is intended.

2. M. P. Golombek et al., J. Geophys. Res.108, 8072 (2003).

3. Pancam Multispectral Imaging Results from the Opportunity Rover at Meridiani Planum

4. MOC image R0802184 was radiometrically calibrated using the ISIS (Integrated Software for Imagers and Spectrometers) available from the Astrogeology Team (http://isis.astrogeology.usgs.gov/Isis2/isis-bin/isis.cgi) of the U.S. Geological Survey in Flagstaff AZ.

5. Names have been assigned to geographic features by the Mars Exploration Rover (MER) team for planning and operations purposes. The names are not formally recognized by the International Astronomical Union.

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