Detection of Silica-Rich Deposits on Mars

Author:

Squyres S. W.12345,Arvidson R. E.12345,Ruff S.12345,Gellert R.12345,Morris R. V.12345,Ming D. W.12345,Crumpler L.12345,Farmer J. D.12345,Marais D. J. Des12345,Yen A.12345,McLennan S. M.12345,Calvin W.12345,Bell J. F.12345,Clark B. C.12345,Wang A.12345,McCoy T. J.12345,Schmidt M. E.12345,de Souza P. A.12345

Affiliation:

1. Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA.

2. Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA.

3. School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA.

4. Department of Physics, University of Guelph, Guelph, Ontario, N1G 2W1, Canada.

5. NASA Johnson Space Center, Houston, TX 77058, USA.

Abstract

Mineral deposits on the martian surface can elucidate ancient environmental conditions on the planet. Opaline silica deposits (as much as 91 weight percent SiO 2 ) have been found in association with volcanic materials by the Mars rover Spirit. The deposits are present both as light-toned soils and as bedrock. We interpret these materials to have formed under hydrothermal conditions and therefore to be strong indicators of a former aqueous environment. This discovery is important for understanding the past habitability of Mars because hydrothermal environments on Earth support thriving microbial ecosystems.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference38 articles.

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