An analysis of open-basin lake deposits on Mars: Evidence for the nature of associated lacustrine deposits and post-lacustrine modification processes
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Most minerals in open-basin crater lakes observed from orbit lack evidence of strong in situ chemical alteration.
“In addition, most of the minerals in open-basin crater lakes observed from orbit lack evidence of strong in situ chemical alteration (Goudge et al. 2012).”
From The Climate of Early Mars (2016) · cites this paper as Goudge et al. 2012
The flows responsible for eroding the late Noachian and Hesperian surface were relatively short-lived.
“This suggests that the flows responsible for eroding the late Noachian and Hesperian surface were relatively short-lived.”
From The Climate of Early Mars (2016) · cites this paper as Goudge et al. 2012
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References 115 · Cited by 146
- Authors
- Goudge, T. A., Head, J. W., Mustard, J. F., & Fassett, C. I.
- Affiliations
- Brown University (US)
- Mount Holyoke College (US)
- Corresponding author
- Goudge, Timothy A.
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 2012-05
- Volume
- 219
- Issue
- 1
- Pages
- 211-229
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W2170291577
- Cited by
- 146
- References
- 115
- Citations by year
- 2026: 11 · 2025: 9 · 2024: 12 · 2023: 17 · 2022: 19 · 2021: 15 · 2020: 9 · 2019: 8 · 2018: 12 · 2017: 5 · 2016: 9 · 2015: 9 · 2014: 6 · 2013: 2 · 2012: 3
- FWCI
- 3.50
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Icarus (publishedVersion)
- 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 › Earth-Surface Processes › Geological formations and processes
- Keywords
- Mars, lake sediments, evaporites, kaolinite, hydrated silica, carbonates, valley networks, paleolakes, volcanic activity, glacial activity, impact cratering, aeolian activity, mineralogy
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