Ventilation of CO2 from a reduced mantle and consequences for the early Martian greenhouse
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During later events such as the formation of the Tharsis bulge, 40 mbar to 1.4 bars of CO2 could have been outgassed.
“During later events (such as the formation of the Tharsis bulge), they estimate that 40 mbar to 1.4 bars could have been outgassed.”
From The Climate of Early Mars (2016) · cites this paper as Hirschmann & Withers 2008
Between 70 mbar and 13 bar of CO2 could have been outgassed during the initial formation of the Martian crust, with the lower estimate for the most reducing conditions.
“Given this, Hirschmann & Withers (2008) estimate that between 70 mbar and 13 bar of CO 2 could have been outgassed during the initial formation of the Martian crust, with the lower estimate for the most reducing conditions.”
From The Climate of Early Mars (2016) · cites this paper as Hirschmann & Withers 2008
A high atmospheric CO2 content required for CO2-H2 warming may be inconsistent with a highly reducing mantle.
“It also requires a high atmospheric CO 2 content, which as discussed in Section 3.1 may be inconsistent with a highly reducing mantle (Hirschmann & Withers 2008).”
From The Climate of Early Mars (2016) · cites this paper as Hirschmann & Withers 2008
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References 98 · Cited by 131
- Authors
- Hirschmann, M. M., & Withers, A. C.
- Affiliations
- University of Minnesota (US)
- Corresponding author
- Hirschmann, Marc M.
- Venue
- Earth and Planetary Science Letters
- Publisher
- Elsevier BV
- Published
- 2008-06
- Volume
- 270
- Issue
- 1-2
- Pages
- 147-155
- ISSN
- 0012-821X (ISSN-L)
- OpenAlex
- W2082336068
- Cited by
- 131
- References
- 98
- Citations by year
- 2026: 3 · 2025: 3 · 2024: 10 · 2023: 3 · 2022: 8 · 2021: 10 · 2020: 4 · 2019: 8 · 2018: 8 · 2017: 9 · 2016: 8 · 2015: 7 · 2014: 7 · 2013: 13 · 2012: 14
- FWCI
- 2.96
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Earth and Planetary Science Letters (publishedVersion)
- Funders
- National Science Foundation
- 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 › Geophysics › Geological and Geochemical Analysis
- Keywords
- Martian mantle, oxygen fugacity, iron-wüstite buffer, graphite, CO2 degassing, greenhouse, Martian basalts, partial melting, magma ocean, diamond, Martian crust, liquid water on Mars, CO2 solubility
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