Low palaeopressure of the martian atmosphere estimated from the size distribution of ancient craters
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Analysis of the Dorsa Aeolis region near Gale crater using crater size distribution led to an approximate upper limit of 0.9-3.8 bars on atmospheric pressure 3.6 Ga.
“Recent analysis of the Dorsa Aeolis region near Gale crater using this technique has led to an approximate upper limit of 0.9-3.8 bars on atmospheric pressure 3.6 Ga (Kite et al. 2014).”
From The Climate of Early Mars (2016) · cites this paper as Kite et al. 2014
The Abstract passage describes crater counts in Aeolis Dorsa and gives a preferred nominal age of 3.61 Ga for the rivers; the small-crater analysis describes fitting crater-size distributions to atmospheric pressure. The passages on the palaeopressure upper limit do not give the claimed 0.9–3.8 bar range, and searches for both numbers found no passage stating it. (LLM, conf=0.81)
Experimental — accuracy not yet measuredThe late Noachian CO2 atmosphere could have been as dense as 1-2 bar, but likely no more than this.
“This atmosphere could have been as dense as 1-2 bar, but likely no more than this.”
From The Climate of Early Mars (2016) · cites this paper as Kite et al. 2014
The Error analysis and sensitivity tests section (page unavailable) describes an upper limit on ancient Martian atmospheric pressure, supporting the claim’s general point that the atmosphere was unlikely to be arbitrarily dense. But the passages do not establish a 1–2 bar limit or identify the atmosphere as CO2. The Age Control passage says the rivers were probably Early Hesperian or older and not older than Late Noachian, rather than fixing the pressure constraint specifically to the Late Noachian. (LLM, conf=0.78)
Experimental — accuracy not yet measured
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Self-citationThe Dorsa Argentea Formation and the Noachian-Hesperian climate transition
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Did Mars Possess a Dense Atmosphere During the First $\sim400$ Million Years?
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The Timing of Alluvial Fan Formation on Mars
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Crater Mound Formation by Wind Erosion on Mars
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Impact sculpting of the early martian atmosphere
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The evolutionary divergence of Mars, Venus, and Earth
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- Authors
- Kite, E. S., Williams, J.-P., Lucas, A., & Aharonson, O.
- Affiliations
- California Institute of Technology (US)
- University of California, Los Angeles (US)
- Corresponding author
- Kite, Edwin S.
- Venue
- Nature Geoscience
- Published
- 2014-04-13
- Volume
- 7
- Issue
- 5
- Pages
- 335-339
- ISSN
- 1752-0894 (ISSN-L)
- 1752-0908
- OpenAlex
- W1966047617
- Cited by
- 123
- References
- 68
- Citations by year
- 2026: 5 · 2025: 8 · 2024: 8 · 2023: 12 · 2022: 6 · 2021: 8 · 2020: 9 · 2019: 16 · 2018: 12 · 2017: 12 · 2016: 11 · 2015: 9 · 2014: 5 · 2013: 1
- FWCI
- 6.65
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Nature Geoscience (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CaltechAUTHORS (California Institute of Technology) (submittedVersion)
- arXiv (Cornell University)
- 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
- Mars atmosphere, Gale Crater, fluvial activity, greenhouse microclimate, carbon dioxide, Mars climate history
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