Cited by 275Planetary Science and ExplorationAstro and Planetary ScienceGeology and Paleoclimatology Research

Early Mars: How Warm and How Wet?

Squyres, Steven W., Kasting, James F.·1994·Science

Abstract

Early in its history, Mars underwent fluvial erosion that has been interpreted as evidence for a warmer, wetter climate. However, no atmosphere composed of only CO2 and H2O appears capable of producing mean planetary temperatures even close to 0 degrees C. Rather than by precipitation, aquifer recharge and ground water seepage may have been enabled by hydrothermal convection driven by geothermal heat and heat associated with impacts. Some climatic warming was probably necessary to allow water to flow for long distances across the surface. Modest warming could be provided by even a low-pressure CO2 atmosphere if it was supplemented with small amounts of CH4, NH3, or SO2. Episodic excursions to high obliquities may also have raised temperatures over some portions of the planet's surface.

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Crossref · 10.1126/science.265.5173.744

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3 of 3 references verified0 citation errors · 0 not checkable

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  • The dendritic geomorphology of Martian valley networks strongly suggests an origin due to a hydrological cycle driven by precipitation as rain or snow rather than groundwater sapping or basal melting of thick ice sheets.

    “This geomorphology strongly suggests an origin due to a hydrological cycle driven by precipitation (as rain or snow) (Craddock & Howard 2002; Mangold et al. 2004; Stepinski &Stepinski 2005; Barnhart, Howard & Moore 2009; Hynek, Beach & Hoke 2010; Matsubara, Howard & Gochenour 2013) rather than e.g., groundwater sapping (Squyres & Kasting 1994) or basal melting of thick icesheets (Carr & Head 2003)”

    From The Climate of Early Mars (2016) · cites this paper as Squyres & Kasting 1994

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Authors
Squyres, S. W., & Kasting, J. F.
Affiliations
  • Cornell University (US)
  • Pennsylvania State University (US)
Venue
Science
Published
1994-08-05
Volume
265
Issue
5173
Pages
744-749
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2094017836
Cited by
275
References
3
Citations by year
2025: 6 · 2024: 5 · 2023: 5 · 2022: 4 · 2021: 5 · 2020: 4 · 2019: 6 · 2018: 8 · 2017: 1 · 2016: 11 · 2015: 4 · 2014: 5 · 2013: 11 · 2012: 16
FWCI
13.25
Type
journal article
Language
en
Open access
closed
Locations
  • Science (publishedVersion)
  • PubMed (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, fluvial erosion, groundwater recharge, groundwater seepage, hydrothermal convection, geothermal heat, impact heating, CO2 atmosphere, methane, ammonia, sulfur dioxide, obliquity, planetary temperature, paleoclimate
MeSH terms
Ammonia, Atmosphere, Carbon Dioxide, Climate, Geology, Methane, Sulfur Dioxide, Sunlight, Water, Greenhouse Effect, Mars, Exobiology, Meteoroids, Evolution, Planetary, Geological Phenomena

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