Cited by 162Planetary Science and ExplorationAstro and Planetary ScienceStellar, planetary, and galactic studies

Thermal escape of carbon from the early Martian atmosphere

Tian, Feng, Kasting, James F., Solomon, Stanley C.·2009·Geophysical Research Letters

Abstract

Observations suggest that Mars was wet and warm during the late Noachian, which probably requires a dense CO 2 atmosphere. But would a dense CO 2 early Martian atmosphere have been stable under the strong EUV flux from the young Sun? Here we show that thermal escape of carbon was so efficient during the early Noachian, 4.1 billion years ago (Ga), that a CO 2 ‐dominated Martian atmosphere could not have been maintained, and Mars should have begun its life cold. By the mid to late Noachian, however, the solar EUV flux would have become weak enough to allow a dense CO 2 atmosphere to accumulate. Hence, a sustainable warm and wet period only appeared several hundred million years (Myrs) after Mars formed.

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Crossref · 10.1029/2008gl036513

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31 of 31 references verified0 citation errors · 0 not checkable

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  • At higher levels of solar XUV radiation, the Earth's atmosphere is hotter and more expanded, leading to more rapid losses to space.

    “At higher levels of solar XUV radiation, the Earth's atmosphere is hotter and more expanded (Tian et al. 2008; Tian et al. 2009; Kuramoto et al. 2013), leading to more rapid losses to space (Lammer et al. 2008; Lichtenegger et al. 2010; Lammer et al. 2018).”

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Authors
Tian, F., Kasting, J. F., & Solomon, S. C.
Affiliations
  • Massachusetts Institute of Technology (US)
  • Pennsylvania State University (US)
  • NSF National Center for Atmospheric Research (US)
Venue
Geophysical Research Letters
Published
2009-01
Volume
36
Issue
2
ISSN
  • 0094-8276 (ISSN-L)
  • 1944-8007
OpenAlex
W1908570882
Cited by
162
References
31
Citations by year
2026: 6 · 2025: 2 · 2024: 8 · 2023: 6 · 2022: 9 · 2021: 8 · 2020: 11 · 2019: 9 · 2018: 12 · 2017: 10 · 2016: 11 · 2015: 6 · 2014: 8 · 2013: 12 · 2012: 18
FWCI
7.21
Type
journal article
Language
en
Open access
closed
Locations
Geophysical Research Letters (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 › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Keywords
thermal escape, CO2 atmosphere, Noachian period, extreme ultraviolet radiation, atmospheric escape, early Mars climate, solar luminosity, atmospheric evolution

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