Geochemistry of Carbonates on Mars: Implications for Climate History and Nature of Aqueous Environments
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Carbonate is conspicuous by its low abundance on the Martian surface.
“One mineral, carbonate, is conspicuous by its low abundance on the Martian surface (Niles et al. 2013; Ehlmann & Edwards 2014).”
From The Climate of Early Mars (2016) · cites this paper as Niles et al. 2013
The absence of surface carbonates is a strong indication that early Mars was either only episodically warm, or very dry.
“Hence the absence of surface carbonates is a strong indication that early Mars was either only episodically warm, or very dry.”
From The Climate of Early Mars (2016) · cites this paper as Niles et al. 2013
Siderite implies formation from surface or subsurface fluids with higher [Fe2+]-and therefore a less oxidizing environment-than the surfaces of modern Earth or Mars.
“In either case, siderite in particular implies formation from surface or subsurface fluids with higher [Fe 2+ ]-and therefore a less oxidizing environment-than the surfaces of modern Earth or Mars [e.g., Catling, 1999;Niles et al., 2013].”
From Orbital evidence for more widespread carbonate-bearing rocks on Mars (2016) · cites this paper as Niles et al., 2013
The citation lists haven’t been fetched yet
References 183 · Cited by 184
- Authors
- Niles, P. B., Catling, D. C., Berger, G., Chassefière, E., Ehlmann, B. L., Michalski, J. R., Morris, R., Ruff, S. W., & Sutter, B.
- Affiliations
- Johnson Space Center (US)
- University of Washington (US)
- Centre National de la Recherche Scientifique (FR)
- California Institute of Technology (US)
- Planetary Science Institute (US)
- Arizona State University (US)
- Corresponding author
- Niles, Paul B.
- ORCID
- Venue
- Space Science Reviews
- Published
- 2012-10-25
- Volume
- 174
- Issue
- 1-4
- Pages
- 301-328
- ISSN
- 0038-6308 (ISSN-L)
- 1572-9672
- OpenAlex
- W1986947350
- Cited by
- 184
- References
- 183
- Citations by year
- 2026: 6 · 2025: 17 · 2024: 10 · 2023: 12 · 2022: 14 · 2021: 19 · 2020: 16 · 2019: 9 · 2018: 10 · 2017: 18 · 2016: 12 · 2015: 14 · 2014: 5 · 2013: 12 · 2012: 9
- FWCI
- 7.00
- Type
- journal article
- Language
- en
- Open access
- closed
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Space Science Reviews (publishedVersion)
- CaltechAUTHORS (California Institute of Technology) (submittedVersion)
- HAL (submittedVersion)
- The HKU Scholars Hub (University of Hong Kong) (submittedVersion)
- 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
- Mars climate history, carbon balance, Martian meteorites, ALH84001, Gusev Crater, Phoenix lander, Martian dust
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Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
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