Effects of obliquity and water vapor/trace gas greenhouses in the early martian climate
Abstract
We explore possible mechanisms for the generation of warm, wet climates on early Mars as a result of greenhouse warming by both water vapor and periodic volcanic trace emissions. The presence of both water vapor (a strong greenhouse gas) and other trace greenhouse gases (such as SO 2) in a predominantly CO 2 atmosphere may act, under certain conditions, to elevate surface temperatures above the freezing point of liquid water, at least episodically. Variations in obliquity are explored to investigate whether these periodic variations in insolation at Mars can broaden the regions or seasons where warm temperatures can exist. We use the Mars Weather Research and Forecasting general circulation model to perform several simulations of the conditions of the early martian atmosphere containing these gases and find global temperatures to be cooler than the elevated levels suggested by at least one recent study by Johnson et al. (2008). While achieving temperatures above 273 K globally remains challenging, the additional warming by greenhouse gases under certain obliquity states can permit for widespread seasonally warm conditions, which can help to explain the presence of fluvial surface features (e.g., valley networks) and hydrous minerals of post‐Noachian age, a period when alternate methods do not convincingly explain the sustainability of liquid water. Furthermore, we find that global warming can be achieved with the presence of a darker surface globally, which is consistent with both widespread exposure of unweathered basaltic bedrock or the presence of a large surface ocean or sea.
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Recent 3D GCM studies find that in concentrations of under 10 ppm, SO2 warming cannot cause significant melting events on early Mars.
“In contrast to their result, recent 3D GCM studies find that in concentrations of under 10 ppm, SO 2 warming cannot cause significant melting events on early Mars (Mischna et al. 2013; Kerber, Forget & Wordsworth 2015).”
From The Climate of Early Mars (2016) · cites this paper as Mischna et al. 2013
Johnson et al. (2008) used correlated-k coefficients that were later found to be in error.
“While pioneering in terms of its technical approach, this work used correlatedk coefficients that were later found to be in error (Mischna et al. 2013).”
From The Climate of Early Mars (2016) · cites this paper as Mischna et al. 2013
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Wordsworth, R. D. (2016) · Annual Review of Earth and Planetary Sciences · doi:10.1146/annurev-earth-060115-012355 · Cited by 416 · see citing works
“In contrast to their result, recent 3D GCM studies find that in concentrations of under 10 ppm, SO2 warming cannot cause significant melting events on early Mars (Mischna et al. 2013; Kerber, Forget & Wordsworth 2015).”
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- Authors
- Mischna, M. A., Baker, V., Milliken, R., Richardson, M., & Lee, C.
- Affiliations
- Jet Propulsion Laboratory (US)
- University of Arizona (US)
- Brown University (US)
- Ashima Group (United States) (US)
- Venue
- Journal of Geophysical Research: Planets
- Publisher
- American Geophysical Union (AGU)
- Published
- 2013-03
- Volume
- 118
- Issue
- 3
- Pages
- 560-576
- ISSN
- 2169-9097 (ISSN-L)
- 2169-9100
- OpenAlex
- W1561582442
- Cited by
- 84
- References
- 13
- Citations by year
- 2026: 2 · 2025: 4 · 2024: 3 · 2023: 2 · 2022: 6 · 2021: 8 · 2020: 9 · 2019: 11 · 2018: 9 · 2017: 9 · 2016: 4 · 2015: 10 · 2014: 5 · 2013: 1
- FWCI
- 3.60
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Journal of Geophysical Research Planets (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 › Atmospheric Science › Geology and Paleoclimatology Research
- Keywords
- early Mars climate, obliquity variations, global warming, water vapor, sulfur dioxide, CO2 atmosphere, surface temperature, solar irradiation, valley networks, hydrous minerals, surface albedo, Mars general circulation model, liquid water
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