Cited by 942Astro and Planetary SciencePlanetary Science and ExplorationPaleontology and Stratigraphy of Fossils

Earth and Mars: evolution of atmospheres and surface temperatures

Sagan, Carl, Mullen, George·1972·Science

Abstract

Solar evolution implies, for contemporary albedos and atmospheric composition, global mean temperatures below the freezing point of seawater less than 2.3 aeons ago, contrary to geologic and paleontological evidence. Ammonia mixing ratios of the order of a few parts per million in the middle Precambrian atmosphere resolve this and other problems. Possible temperature evolutionary tracks for Earth and Mars are described. A runaway greenhouse efect will occur on Earth about 4.5 aeons from now, when clement conditions will prevail on Mars.

Integrity signals

Registry

Crossref · 10.1126/science.177.4043.52

Cites

38 of 38 references verified0 citation errors · 0 not checkable

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  • Liquid water under a fainter Sun likely implies more abundant greenhouse gases than today.

    “Liquid water under a fainter Sun likely implies more abundant greenhouse gases than today (14, 15).”

    From The Archean atmosphere (2020) · cites this paper as [14]

  • The most plausible solution to the FYS is a big greenhouse effect.

    “The most plausible solution to the FYS is a big greenhouse effect (14, 214, 215).”

    From The Archean atmosphere (2020) · cites this paper as [14]

  • NH3 levels of 10 to 100 ppmv would provide a greenhouse effect to counteract the faint young Sun.

    “Ammonia (NH3) levels of 10 to 100 ppmv would provide a greenhouse effect to counteract the faint young Sun (FYS) (14), but these levels of NH3 cannot be sustained against UV photolysis (161).”

    From The Archean atmosphere (2020) · cites this paper as [14]

  • Another proposed early greenhouse gas is H2, if it attained percentage abundances.

    “Another proposed early greenhouse gas is H2, if it attained percentage abundances (14, 217, 218).”

    From The Archean atmosphere (2020) · cites this paper as [14]

  • The Earth with its current atmosphere would have been too cold to possess liquid oceans under the Archean Sun.

    “meaning that the Earth with its current atmosphere would have been too cold to possess liquid oceans (Sagan and Mullen 1972)”

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Authors
Sagan, C., & Mullen, G.
Affiliations
Cornell University (US)
Venue
Science
Published
1972-07-07
Volume
177
Issue
4043
Pages
52-56
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W1986601098
Cited by
942
References
38
Citations by year
2026: 17 · 2025: 25 · 2024: 20 · 2023: 43 · 2022: 24 · 2021: 25 · 2020: 44 · 2019: 54 · 2018: 55 · 2017: 37 · 2016: 32 · 2015: 30 · 2014: 25 · 2013: 40 · 2012: 31
FWCI
14.48
Type
journal article
Language
en
Open access
closed
Locations
  • Science (publishedVersion)
  • PubMed (publishedVersion)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
  • Physical Sciences › Earth and Planetary Sciences › Paleontology › Paleontology and Stratigraphy of Fossils
Keywords
atmospheric evolution, surface temperature evolution, Earth, Mars, ammonia, Precambrian atmosphere, runaway greenhouse effect, solar evolution, albedo, paleoclimate

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