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Chemistry of Rocks and Soils in Gusev Crater from the Alpha Particle X-ray Spectrometer
R. Gellert,1,2*R. Rieder,1R. C. Anderson,3J. Brückner,1B. C. Clark,4G. Dreibus,1T. Economou,5G. Klingelhöfer,2G. W. Lugmair,1D. W. Ming,6S. W. Squyres,7C. d'Uston,8H. Wänke,1A. Yen,3J. Zipfel1
The alpha particle x-ray spectrometer on the Spirit rover determinedmajor and minor elements of soils and rocks in Gusev craterin order to unravel the crustal evolution of planet Mars. Thecomposition of soils is similar to those at previous landingsites, as a result of global mixing and distribution by duststorms. Rocks (fresh surfaces exposed by the rock abrasion tool)resemble volcanic rocks of primitive basaltic composition withlow intrinsic potassium contents. High abundance of bromine(up to 170 parts per million) in rocks may indicate the alterationof surfaces formed during a past period of aqueous activityin Gusev crater.
1 Max-Planck-Institut für Chemie, J. J. Becher-Weg 27, D-55128 Mainz, Germany. 2 Institut für Anorganische und Analytische Chemie, J. Gutenberg-Universität, D-55128 Mainz, Germany. 3 Jet Propulsion Laboratory, Pasadena, CA 911091, USA. 4 Lockheed Martin Corporation, Littleton, CO 80127, USA. 5 Laboratory for Atmospheric and Space Research, Enrico Fermi Institute, Chicago, IL 60637, USA. 6 Johnson Space Center, National Aeronautics and Space Administration (NASA), Houston, TX 77058, USA. 7 Center for Radiophysics and Space Research, Cornell University, Ithaca, NY 14853, USA. 8 Centre d'Etude Spatiale des Rayonnements, F-31028, Toulouse, France.
* To whom correspondence should be addressed. E-mail: gellert{at}mpch-mainz.mpg.de.
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