Localization and Physical Property Experiments Conducted by Opportunity at Meridiani Planum

Author:

Arvidson R. E.12345,Anderson R. C.12345,Bartlett P.12345,Bell J. F.12345,Christensen P. R.12345,Chu P.12345,Davis K.12345,Ehlmann B. L.12345,Golombek M. P.12345,Gorevan S.12345,Guinness E. A.12345,Haldemann A. F. C.12345,Herkenhoff K. E.12345,Landis G.12345,Li R.12345,Lindemann R.12345,Ming D. W.12345,Myrick T.12345,Parker T.12345,Richter L.12345,Seelos F. P.12345,Soderblom L. A.12345,Squyres S. W.12345,Sullivan R. J.12345,Wilson J.12345

Affiliation:

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

2. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.

3. Honeybee Robotics, 204 Elizabeth Street, New York, NY 10012, USA.

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

5. Department of Geological Sciences, Arizona State University, Tempe, AZ 85287, USA.

Abstract

The location of the Opportunity landing site was determined to better than 10-m absolute accuracy from analyses of radio tracking data. We determined Rover locations during traverses with an error as small as several centimeters using engineering telemetry and overlapping images. Topographic profiles generated from rover data show that the plains are very smooth from meter- to centimeter-length scales, consistent with analyses of orbital observations. Solar cell output decreased because of the deposition of airborne dust on the panels. The lack of dust-covered surfaces on Meridiani Planum indicates that high velocity winds must remove this material on a continuing basis. The low mechanical strength of the evaporitic rocks as determined from grinding experiments, and the abundance of coarse-grained surface particles argue for differential erosion of Meridiani Planum.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference21 articles.

1. On the wave age dependence of wind stress over pure wind seas

2. R. E. Arvidson et al., J. Geophys. Res.108, 8070 (2003).

3. Chemical characterization of submicron aerosol particles collected over the Indian Ocean

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

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

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