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Warming early Mars with CO2 and H2
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“Hence for pure clear-sky CO 2 -H 2 O atmospheres under early Martian conditions, modern radiativeconvective models obtain mean surface temperatures of 225 K or less (Wordsworth, Forget & Eymet 2010; Ramirez et al. 2014; Halevy & Head 2014).”
From The Climate of Early Mars (2016) · cites this paper as Ramirez et al. 2014
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Metadata
- Authors
- Ramirez, R. M., Kopparapu, R., Zugger, M. E., Robinson, T. D., Freedman, R., & Kasting, J. F.
- Affiliations
- Pennsylvania State University (US)
- NASA Astrobiology Institute (US)
- Ames Research Center (US)
- Corresponding author
- Ramirez, Ramses M.
- ORCID
- Venue
- Nature Geoscience
- Published
- 2013-11-24
- Volume
- 7
- Issue
- 1
- Pages
- 59-63
- ISSN
- 1752-0894 (ISSN-L)
- 1752-0908
- OpenAlex
- W2057666382
- Cited by
- 303
- References
- 86
- Citations by year
- 2026: 20 · 2025: 28 · 2024: 24 · 2023: 20 · 2022: 26 · 2021: 23 · 2020: 30 · 2019: 31 · 2018: 32 · 2017: 25 · 2016: 22 · 2015: 15 · 2014: 5 · 2013: 1
- FWCI
- 7.74
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Nature Geoscience (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Planetary Science and Exploration
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Earth and Planetary Sciences › Atmospheric Science › Geology and Paleoclimatology Research
- Keywords
- early Mars climate, global warming, carbon dioxide, volatile outgassing, volcanic outgassing, methane oxidation, liquid water on Mars, one-dimensional climate model, surface temperature, atmospheric pressure
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