On the original igneous source of Martian fines
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For the highland crust of early Mars, a mafic to ultramafic character is expected on the basis of the composition of Martian meteorites and fundamental geochemical considerations.
“For the highland crust of early Mars, a mafic to ultramafic character is expected on the basis of the composition of Martian meteorites [Mc-$ween, 1994] and fundamental geochemical considerations [Baird and Clark, 1981].”
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 Baird and Clark, 1981
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- Authors
- Baird, A. K., & Clark, B. C.
- Affiliations
- Pomona College (US)
- Martin Marietta (United States) (US)
- ORCID
- Clark, Benton C.
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 1981-01
- Volume
- 45
- Issue
- 1
- Pages
- 113-123
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W1977910209
- Cited by
- 66
- References
- 62
- Citations by year
- 2025: 2 · 2021: 2 · 2020: 3 · 2017: 1 · 2015: 1 · 2012: 3
- FWCI
- 5.91
- 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 › Geophysics › Geological and Geochemical Analysis
- Keywords
- mafic-ultramafic rocks, pyroxene, flood basalts, komatiite, mantle composition, planetary size
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