Exploring the faint young Sun problem and the possible climates of the Archean Earth with a 3‐D GCM
Open accessAbstract
Different solutions have been proposed to solve the “faint young Sun problem,” defined by the fact that the Earth was not fully frozen during the Archean despite the fainter Sun. Most previous studies were performed with simple 1‐D radiative convective models and did not account well for the clouds and ice‐albedo feedback or the atmospheric and oceanic transport of energy. We apply a global climate model (GCM) to test the different solutions to the faint young Sun problem. We explore the effect of greenhouse gases (CO 2 and CH 4 ), atmospheric pressure, cloud droplet size, land distribution, and Earth's rotation rate. We show that neglecting organic haze, 100 mbar of CO 2 with 2 mbar of CH 4 at 3.8 Ga and 10 mbar of CO 2 with 2 mbar of CH 4 at 2.5 Ga allow a temperate climate (mean surface temperature between 10°C and 20°C). Such amounts of greenhouse gases remain consistent with the geological data. Removing continents produces a warming lower than +4°C. The effect of rotation rate is even more limited. Larger droplets (radii of 17 μm versus 12 μm) and a doubling of the atmospheric pressure produce a similar warming of around +7°C. In our model, ice‐free water belts can be maintained up to 25°N/S with less than 1 mbar of CO 2 and no methane. An interesting cloud feedback appears above cold oceans, stopping the glaciation. Such a resistance against full glaciation tends to strongly mitigate the faint young Sun problem.
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Three-dimensional climate models with a lower solar flux produce weaker evaporation and fewer low clouds, but a strong greenhouse effect is still required because the albedo decrease is small.
“Three-dimensional climate models with a lower solar flux produce weaker evaporation and fewer low clouds, but a strong greenhouse effect is still required because the albedo decrease is small (212, 213).”
From The Archean atmosphere (2020) · cites this paper as [212]
Section 4.4 (pp. 9–10) says the weaker Archean Sun reduced evaporation and cloud cover, lowering planetary albedo; the summary (p. 16) confirms the cloud feedback. But Section 4.4 calls the albedo decrease strong, from 0.36 to 0.30, not small. The paper models substantial greenhouse gases for a temperate climate, but does not say they are required because the albedo decrease is small. (LLM, conf=0.90)
Experimental — accuracy not yet measuredA faster Archean rotation rate reduces heat transport from equator to pole, particularly if the atmosphere had less mass.
“In general, a faster Archean rotation rate reduces heat transport from equator to pole (212, 213), particularly if the atmosphere had less mass (248).”
From The Archean atmosphere (2020) · cites this paper as [212]
Section 5.3 (p. 14) says faster rotation reduces meridional heat transport by limiting the size of baroclinic eddies. Section 5.2 (p. 13) says atmospheric pressure affects heat transport to the poles, but does not say that lower atmospheric mass particularly strengthens the rotation-related reduction. (LLM, conf=0.86)
Experimental — accuracy not yet measured
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The Pale Orange Dot: The Spectrum and Habitability of Hazy Archean Earth
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“However, as we have argued, a mean surface temperature of the freezing point of water is not a useful threshold for global habitability (Charnay et al. , 2013; Shields et al. , 2013; Wolf and Toon, 2013; Kunze et al. , 2014), so some of the Haqq-Misra et al. spherical haze results may actually be…”
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Self-citationConstraints on ocean carbonate chemistry and pCO2 in the Archaean and Palaeoproterozoic
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- Authors
- Charnay, B., Forget, F., Wordsworth, R., Leconte, J., Millour, E., Codron, F., & Spiga, A.
- Affiliations
- Laboratoire de Météorologie Dynamique (FR)
- University of Chicago (US)
- Venue
- Journal of Geophysical Research: Atmospheres
- Publisher
- American Geophysical Union (AGU)
- Published
- 2013-09-19
- Volume
- 118
- Issue
- 18
- Pages
- 10414-10431
- ISSN
- 0148-0227 (ISSN-L)
- 2169-897X
- 2169-8996
- OpenAlex
- W2594696318
- Cited by
- 144
- References
- 92
- Citations by year
- 2026: 6 · 2025: 11 · 2024: 5 · 2023: 9 · 2022: 9 · 2021: 14 · 2020: 17 · 2019: 14 · 2018: 21 · 2017: 13 · 2016: 11 · 2015: 5 · 2014: 7 · 2013: 1
- FWCI
- 6.09
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Journal of Geophysical Research Atmospheres (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Digital Access to Scholarship at Harvard (DASH) (Harvard University) (submittedVersion, cc-by)
- HAL (submittedVersion, other-oa)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Environmental Science › Global and Planetary Change › Climate variability and models
- Physical Sciences › Earth and Planetary Sciences › Atmospheric Science › Geology and Paleoclimatology Research
- Physical Sciences › Earth and Planetary Sciences › Paleontology › Paleontology and Stratigraphy of Fossils
- Keywords
- greenhouse gases, carbon dioxide, methane, organic haze, cloud feedback, ice-albedo feedback, cloud droplet size, atmospheric pressure, Earth rotation rate, continental configuration, early Earth climate
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