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In Situ Evidence for an Ancient Aqueous Environment at Meridiani Planum, Mars
S. W. Squyres,1*J. P. Grotzinger,2R. E. Arvidson,3J. F. Bell, III,1W. Calvin,4P. R. Christensen,5B. C. Clark,6J. A. Crisp,7W. H. Farrand,8K. E. Herkenhoff,9J. R. Johnson,9G. Klingelhöfer,10A. H. Knoll,11S. M. McLennan,12H. Y. McSween, Jr.,13R. V. Morris,14J. W. Rice, Jr.,5R. Rieder,15L. A. Soderblom9
Sedimentary rocks at Eagle crater in Meridiani Planum are composedof fine-grained siliciclastic materials derived from weatheringof basaltic rocks, sulfate minerals (including magnesium sulfateand jarosite) that constitute several tens of percent of therock by weight, and hematite. Cross-stratification observedin rock outcrops indicates eolian and aqueous transport. Diageneticfeatures include hematite-rich concretions and crystal-moldvugs. We interpret the rocks to be a mixture of chemical andsiliciclastic sediments with a complex diagenetic history. Theenvironmental conditions that they record include episodic inundationby shallow surface water, evaporation, and desiccation. Thegeologic record at Meridiani Planum suggests that conditionswere suitable for biological activity for a period of time inmartian history.
1 Department of Astronomy, Cornell University, Ithaca, NY 14853, USA. 2 Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA. 3 Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63031, USA. 4 Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA. 5 Department of Geological Sciences, Arizona State University, Tempe, AZ 85287, USA. 6 Lockheed Martin Corporation, Littleton, CO 80127, USA. 7 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA. 8 Space Science Institute, Boulder, CO 80301, USA. 9 U.S. Geological Survey, Flagstaff, AZ 86001, USA. 10 Johannes Gutenberg University, D-55128 Mainz, Germany. 11 Botanical Museum, Harvard University, Cambridge, MA 02138, USA. 12 Department of Geosciences, State University of New York, Stony Brook, NY 11794, USA. 13 Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996, USA. 14 NASA Johnson Space Center, Houston, TX 77058, USA. 15 Max-Planck-Institut für Chemie, Kosmochemie, D-55128 Mainz, Germany.
* To whom correspondence should be addressed. E-mail: squyres{at}astrosun.tn.cornell.edu
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