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Science 3 December 2004:
Vol. 306. no. 5702, pp. 1727 - 1730
DOI: 10.1126/science.1105286

Reports

Evidence from Opportunity's Microscopic Imager for Water on Meridiani Planum

K. E. Herkenhoff,1* S. W. Squyres,2 R. Arvidson,3 D. S. Bass,4 J. F. Bell, III,2 P. Bertelsen,5 B. L. Ehlmann,3 W. Farrand,6 L. Gaddis,1 R. Greeley,7 J. Grotzinger,8 A. G. Hayes,2 S. F. Hviid,9 J. R. Johnson,1 B. Jolliff,3 K. M. Kinch,10 A. H. Knoll,11 M. B. Madsen,5 J. N. Maki,4 S. M. McLennan,12 H. Y. McSween,13 D. W. Ming,14 J. W. Rice, Jr.,7 L. Richter,15 M. Sims,16 P. H. Smith,17 L. A. Soderblom,1 N. Spanovich,17 R. Sullivan,2 S. Thompson,7 T. Wdowiak,18 C. Weitz,19 P. Whelley7

The Microscopic Imager on the Opportunity rover analyzed textures of soils and rocks at Meridiani Planum at a scale of 31 micrometers per pixel. The uppermost millimeter of some soils is weakly cemented, whereas other soils show little evidence of cohesion. Rock outcrops are laminated on a millimeter scale; image mosaics of cross-stratification suggest that some sediments were deposited by flowing water. Vugs in some outcrop faces are probably molds formed by dissolution of relatively soluble minerals during diagenesis. Microscopic images support the hypothesis that hematite-rich spherules observed in outcrops and soils also formed diagenetically as concretions.

1 U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA.
2 Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA.
3 Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA.
4 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
5 Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics and Geophysics, University of Copenhagen, Denmark.
6 Space Science Institute, Boulder, CO 80301, USA.
7 Department of Geological Sciences, Arizona State University, Tempe, AZ 85287, USA.
8 Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.
9 Max Planck Institut für Aeronomie, Katlenburg-Lindau, D-37191, Germany.
10 Institute of Physics and Astronomy, Aarhus University, Aarhus, Denmark.
11 Department of Organismic and Evolutionary Biology, Harvard University, Cambridge, MA 02138, USA.
12 State University of New York, Department of Geosciences, Stony Brook, NY 11794, USA.
13 Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996, USA.
14 Astromaterials Research and Exploration Science Office, NASA Johnson Space Center, Houston, TX 77058, USA.
15 DLR Institut fur Raumsimulation, Linder Hoehe, Koln, Germany.
16 NASA Ames Research Center, Moffett Field, CA 94035, USA.
17 Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA.
18 Department of Physics, University of Alabama, Birmingham, AL 35294, USA.
19 Planetary Science Institute, Tucson, AZ 85719, USA.

* To whom correspondence should be addressed. E-mail: kherkenhoff{at}usgs.gov

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