Carbonates identified by the Curiosity rover indicate a carbon cycle operated on ancient Mars

Ancient Mars had surface liquid water and a dense carbon dioxide (CO<sub>2</sub>)-rich atmosphere. Such an atmosphere would interact with crustal rocks, potentially leaving a mineralogical record of its presence. We analyzed the composition of an 89-meter stratigraphic section of Gale crater, Mars, using data collected by the Curiosity rover. An iron carbonate mineral, siderite, occurs in abundances of 4.8 to 10.5 weight %, colocated with highly water-soluble salts. We infer that the siderite formed in water-limited conditions, driven by water-rock reactions and evaporation. Comparison with orbital data indicates that similar strata (deposited globally) sequestered the equivalent of 2.6 to 36 millibar of atmospheric CO<sub>2</sub>. The presence of iron oxyhydroxides in these deposits indicates that a partially closed carbon cycle on ancient Mars returned some previously sequestered CO<sub>2</sub> to the atmosphere.

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Journal
Science
Published
2025-04-17
DOI
https://doi.org/10.1126/science.ado9966
Citations
35
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
40.42
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article

Carbonates identified by the Curiosity rover indicate a carbon cycle operated on ancient Mars

E. B. Rampe, David J. Des Marais, A. A. Fraeman, Valerie Tu et al.
35 citations
Science
Planetary Science and Exploration
40.42
article

Carbonates identified by the Curiosity rover indicate a carbon cycle operated on ancient Mars

E. B. Rampe, David J. Des Marais, A. A. Fraeman, Valerie Tu, T. Peretyazhko, J. P. Grotzinger, J. Frydenvang, Steve Larter, T. F. Bristow, Amelie L. Roberts, J. V. Clark, P. J. Gasda, J. C. Bridges, B. Sutter, A. H. Treiman, Sarah Simpson, D. F. Blake, M. T. Thorpe, Johannes M. Meusburger, Elisabeth M. Hausrath, H. B. Franz, Edwin S. Kite, Patricia Craig, Aditi Pandey, A. S. Yen, Benjamin M. Tutolo, David G. Burtt, A. R. Vasavada, D. T. Vaniman, W. Rapin, N. Castle, S. J. Chipera, Shaunna M. Morrison, R. V. Morris, Robert M. Hazen, Robert T. Downs, D. W. Ming, Mattéo Loche, P. D. Archer
article en
35 citations

Abstract

Ancient Mars had surface liquid water and a dense carbon dioxide (CO<sub>2</sub>)-rich atmosphere. Such an atmosphere would interact with crustal rocks, potentially leaving a mineralogical record of its presence. We analyzed the composition of an 89-meter stratigraphic section of Gale crater, Mars, using data collected by the Curiosity rover. An iron carbonate mineral, siderite, occurs in abundances of 4.8 to 10.5 weight %, colocated with highly water-soluble salts. We infer that the siderite formed in water-limited conditions, driven by water-rock reactions and evaporation. Comparison with orbital data indicates that similar strata (deposited globally) sequestered the equivalent of 2.6 to 36 millibar of atmospheric CO<sub>2</sub>. The presence of iron oxyhydroxides in these deposits indicates that a partially closed carbon cycle on ancient Mars returned some previously sequestered CO<sub>2</sub> to the atmosphere.

ScienceVol. 388(6744)
Rutgers, The State University of New Jersey (US), California Institute of Technology (US), University of Copenhagen (DK), Ames Research Center (US), Centre National de la Recherche Scientifique (FR), Planetary Science Institute (US), Goddard Space Flight Center (US), Universities Space Research Association (US), Jet Propulsion Laboratory (US), University of Nevada, Las Vegas (US), Los Alamos National Laboratory (US), University of Arizona (US), University of Leicester (GB), University of Calgary (CA), Carnegie Institution for Science (US), Centre National d'Études Spatiales (FR), University of Chicago (US), Johnson Space Center (US), Institut de Recherche en Astrophysique et Planétologie (FR), Imperial College London (GB), Lunar and Planetary Institute (US), University of Maryland, College Park (US)
Openalex Percentile: Top 0%
Planetary Science and Exploration
40.42
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