Soil mineralogy and chemistry on Mars: Possible clues from salts and clays in SNC meteorites
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All subgroups of shergottites, nakhlites, and chassignites contain traces of salts, including carbonates and sulfates, that have been interpreted as minerals precipitated from water.
“All subgroups of the shergottites, nakhlites, and chassignites contain traces of salts, including carbonates and sulfates, that have been interpreted as minerals precipitated from water [Gooding, 1992] to precipitate minerals in tiny fractures [ Warren, 1998].”
From A chemical model for evaporites on early Mars: Possible sedimentary tracers of the early climate and implications for exploration (1999) · cites this paper as Gooding, 1992
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- Authors
- Gooding, J. L.
- Affiliations
- National Aeronautics and Space Administration (US)
- Corresponding author
- Gooding, James L.
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 1992-09
- Volume
- 99
- Issue
- 1
- Pages
- 28-41
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W2004018625
- Cited by
- 232
- References
- 92
- Citations by year
- 2026: 2 · 2025: 2 · 2024: 2 · 2023: 1 · 2022: 3 · 2021: 25 · 2020: 8 · 2019: 3 · 2018: 6 · 2017: 7 · 2016: 2 · 2015: 4 · 2014: 7 · 2013: 4 · 2012: 8
- FWCI
- 11.20
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Icarus (publishedVersion)
- Funders
- National Aeronautics and Space Administration
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Physical Sciences › Earth and Planetary Sciences › Geochemistry and Petrology › Geochemistry and Elemental Analysis
- Keywords
- Martian meteorites, Mars, shergottites, nakhlites, chassignites, aqueous alteration, clay minerals, carbonates, sulfate, halides, ferric oxide, aluminosilicates, scapolite, smectite, illite, gypsum, clay catalysis, Martian dust
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