Jarosite and Hematite at Meridiani Planum from Opportunity's Mössbauer Spectrometer

Author:

Klingelhöfer G.12345,Morris R. V.12345,Bernhardt B.12345,Schröder C.12345,Rodionov D. S.12345,de Souza P. A.12345,Yen A.12345,Gellert R.12345,Evlanov E. N.12345,Zubkov B.12345,Foh J.12345,Bonnes U.12345,Kankeleit E.12345,Gütlich P.12345,Ming D. W.12345,Renz F.12345,Wdowiak T.12345,Squyres S. W.12345,Arvidson R. E.12345

Affiliation:

1. Institut für Anorganische und Analytische Chemie, Johannes Gutenberg-Universität, Staudinger Weg 9, D-55128 Mainz, Germany.

2. National Aeronautics and Space Administration (NASA) Johnson Space Center, Houston, TX 77058, USA.

3. Space Research Institute IKI, 117997 Moscow, Russia.

4. Companhia Vale do Rio Doce (CVRD) Group, Vitoria, Brazil.

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

Abstract

Mössbauer spectra measured by the Opportunity rover revealed four mineralogical components in Meridiani Planum at Eagle crater: jarosite- and hematite-rich outcrop, hematite-rich soil, olivine-bearing basaltic soil, and a pyroxene-bearing basaltic rock (Bounce rock). Spherules, interpreted to be concretions, are hematite-rich and dispersed throughout the outcrop. Hematitic soils both within and outside Eagle crater are dominated by spherules and their fragments. Olivine-bearing basaltic soil is present throughout the region. Bounce rock is probably an impact erratic. Because jarosite is a hydroxide sulfate mineral, its presence at Meridiani Planum is mineralogical evidence for aqueous processes on Mars, probably under acid-sulfate conditions.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference48 articles.

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4. J. Geophys. Res. 2003 108

5. Members of the MIMOS II consortium are G. Klingelhöfer B. Bernhardt P. A. de Souza Jr. J. Foh R. Gellert P. Gütlich E. Kankeleit R. V. Morris F. Renz D. S. Rodionov C. Schröder T. Wdowiak and A. Yen.

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