Chemistry of Rocks and Soils in Gusev Crater from the Alpha Particle X-ray Spectrometer

Author:

Gellert R.12345,Rieder R.12345,Anderson R. C.12345,Brückner J.12345,Clark B. C.12345,Dreibus G.12345,Economou T.12345,Klingelhöfer G.12345,Lugmair G. W.12345,Ming D. W.12345,Squyres S. W.12345,d'Uston C.12345,Wänke H.12345,Yen A.12345,Zipfel J.12345

Affiliation:

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.

Abstract

The alpha particle x-ray spectrometer on the Spirit rover determined major and minor elements of soils and rocks in Gusev crater in order to unravel the crustal evolution of planet Mars. The composition of soils is similar to those at previous landing sites, as a result of global mixing and distribution by dust storms. Rocks (fresh surfaces exposed by the rock abrasion tool) resemble volcanic rocks of primitive basaltic composition with low intrinsic potassium contents. High abundance of bromine (up to 170 parts per million) in rocks may indicate the alteration of surfaces formed during a past period of aqueous activity in Gusev crater.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference24 articles.

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

2. R. Rieder et al., Science278, 1770 (1997).

3. R. Rieder et al., J. Geophys. Res. 108 (no. E12), 8066 (2003).

4. The influence of the Mössbauer reference and main sources mainly scattered high-energy radiation was investigated during the development of the APXS. The introduced background was suppressed by a factor of 10 with 1-mm tantalum shields on the APXS and the Mössbauer instruments. Nevertheless the resulting background was still 2.5 times that of the original.

5. Characterizing the long-period ULF response to magnetic storms

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