A native sulfur deposit in Gale crater, Mars

Martian rocks are known to contain sulfur-bearing species, including sulfates and sulfides. These compounds record a sulfur cycle that operated over Mars' geological evolution. We used the Curiosity rover to investigate a deposit of light-toned stones in Gediz Vallis, within Gale crater on Mars. We find that the stones are composed of native sulfur. The sulfur deposit appears to have formed in place, within a sinuous entrenched canyon cut into the floor of Gediz Vallis. The presence of native sulfur implies that a sulfur enrichment pathway involving buoyant subsurface fluids operated on ancient Mars. We propose that the primary source of this sulfur was magmatic vapor, which cooled in the near subsurface cryosphere and was released by decompression during the erosion of Gediz Vallis.

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Publication Details

Journal
Science
Published
2026-06-28
DOI
https://doi.org/10.1126/science.adu5501
Primary Topic
Planetary Science and Exploration
Type
article
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article

A native sulfur deposit in Gale crater, Mars

A. A. Fraeman, L. M. Thompson, P. L. King, B. C. Clark et al.
Science
Planetary Science and Exploration
article

A native sulfur deposit in Gale crater, Mars

A. A. Fraeman, L. M. Thompson, P. L. King, B. C. Clark, S. J. VanBommel, J. V. Clark, J. A. Berger, Aster Cowart, Abigail L. Knight, Sarah Simpson, H. B. Franz, Edwin S. Kite, A. B. Bryk, John R. Christian, R. M. E. Williams, M. A. McCraig, C. D. O’Connell‐Cooper, Christopher H. House, Deirdra M. Fey, R. Gellert, N. I. Boyd, A. R. Vasavada, William E. Dietrich
article en

Abstract

Martian rocks are known to contain sulfur-bearing species, including sulfates and sulfides. These compounds record a sulfur cycle that operated over Mars' geological evolution. We used the Curiosity rover to investigate a deposit of light-toned stones in Gediz Vallis, within Gale crater on Mars. We find that the stones are composed of native sulfur. The sulfur deposit appears to have formed in place, within a sinuous entrenched canyon cut into the floor of Gediz Vallis. The presence of native sulfur implies that a sulfur enrichment pathway involving buoyant subsurface fluids operated on ancient Mars. We propose that the primary source of this sulfur was magmatic vapor, which cooled in the near subsurface cryosphere and was released by decompression during the erosion of Gediz Vallis.

Science
University of New Brunswick (CA), Australian National University (AU), Space Science Institute (US), Planetary Science Institute (US), Goddard Space Flight Center (US), Pennsylvania State University (US), Jet Propulsion Laboratory (US), Washington University in St. Louis (US), Malin Space Science Systems (United States) (US), University of Chicago (US), Johnson Space Center (US), University of Guelph (CA)
Openalex Percentile: Top 7%
Planetary Science and Exploration
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