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Final Accepted Manuscript
Author
Bristow, T. F.Grotzinger, J. P.
Rampe, E. B.
Cuadros, J.
Chipera, S. J.
Downs, G. W.
Fedo, C. M.
Frydenvang, J.
McAdam, A. C.
Morris, R. V.
Achilles, C. N.
Blake, D. F.
Castle, N.
Craig, P.
Des Marais, D. J.
Downs, R. T.
Hazen, R. M.
Ming, D. W.
Morrison, S. M.
Thorpe, M. T.
Treiman, A. H.
Tu, V.
Vaniman, D. T.
Yen, A. S.
Gellert, R.
Mahaffy, P. R.
Wiens, R. C.
Bryk, A. B.
Bennett, K. A.
Fox, V. K.
Millken, R. E.
Fraeman, A. A.
Vasavada, A. R.
Affiliation
Department of Geosciences, University of ArizonaIssue Date
2021-07-08
Metadata
Show full item recordCitation
Bristow, T. F., Grotzinger, J. P., Rampe, E. B., Cuadros, J., Chipera, S. J., Downs, G. W., Fedo, C. M., Frydenvang, J., McAdam, A. C., Morris, R. V., Achilles, C. N., Blake, D. F., Castle, N., Craig, P., Des Marais, D. J., Downs, R. T., Hazen, R. M., Ming, D. W., Morrison, S. M., … Vasavada, A. R. (2021). Brine-driven destruction of clay minerals in Gale crater, Mars. Science, 373(6551), 198–204.Journal
ScienceRights
Copyright © 2021 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Mars’ sedimentary rock record preserves information on geological (and potential astrobiological) processes that occurred on the planet billions of years ago. The Curiosity rover is exploring the lower reaches of Mount Sharp, in Gale crater on Mars. A traverse from Vera Rubin ridge to Glen Torridon has allowed Curiosity to examine a lateral transect of rock strata laid down in a martian lake ~3.5 billion years ago. We report spatial differences in the mineralogy of time-equivalent sedimentary rocks <400 meters apart. These differences indicate localized infiltration of silica-poor brines, generated during deposition of overlying magnesium sulfate–bearing strata. We propose that destabilization of silicate minerals driven by silica-poor brines (rarely observed on Earth) was widespread on ancient Mars, because sulfate deposits are globally distributed. Copyright © 2021 The Authors, some rights reserved.Note
Immediate accessISSN
0036-8075EISSN
1095-9203Version
Final accepted manuscriptSponsors
National Aeronautics and Space Administrationae974a485f413a2113503eed53cd6c53
10.1126/science.abg5449
