Outgassing History and Escape of the Martian Atmosphere and Water Inventory
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Escape processes occurring from the Hesperian onwards could not have removed more than a few 100 mbar at most since 4 Ga.
“In contrast, escape processes occurring from the Hesperian onwards appear unambiguously ineffective: ion escape, plasma instability, sputtering and non-thermal processes combined could not have removed more than a few 100 mbar at most since 4 Ga (Chassefi` ere & Leblanc 2004; Lammer et al. 2013).”
From The Climate of Early Mars (2016) · cites this paper as Lammer et al. 2013
Nonthermal escape processes appear capable of removing only up to ~10 mbar or at most ~100 mbar CO2 over the past 4.1 Gyr, so another sink for the early atmosphere is needed.
“Nonthermal escape processes appear capable of removing only up to ~10 mbar [e.g., Chassefière et al., 2013] or at most ~100 mbar CO 2 over the past 4.1 Gyr [Lammer et al., 2013], so another sink for the early atmosphere is needed.”
From Orbital evidence for more widespread carbonate-bearing rocks on Mars (2016) · cites this paper as Lammer et al., 2013
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“The chemistry of this process has not been extensively studied and may be somewhat modeldependent (Lammer et al. 2013).”
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- Authors
- Lammer, H., Chassefière, E., Karatekin, Ö., Morschhauser, A., Niles, P. B., Mousis, O., Odert, P., Möstl, U. V., Breuer, D., Dehant, V., Grott, M., Gröller, H., Hauber, E., & Pham, L. B. S.
- Affiliations
- Austrian Academy of Sciences (AT)
- Royal Observatory of Belgium (BE)
- Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR) (DE)
- Johnson Space Center (US)
- Centre National de la Recherche Scientifique (FR)
- Corresponding author
- Lammer, Helmut
- Venue
- Space Science Reviews
- Published
- 2012-11-30
- Volume
- 174
- Issue
- 1-4
- Pages
- 113-154
- ISSN
- 0038-6308 (ISSN-L)
- 1572-9672
- OpenAlex
- W2159499466
- Cited by
- 180
- References
- 200
- Citations by year
- 2026: 7 · 2025: 8 · 2024: 7 · 2023: 15 · 2022: 12 · 2021: 9 · 2020: 11 · 2019: 11 · 2018: 17 · 2017: 17 · 2016: 19 · 2015: 15 · 2014: 13 · 2013: 13 · 2012: 6
- FWCI
- 8.23
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Space Science Reviews (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- HAL (submittedVersion)
- Digital Access to Libraries (submittedVersion)
- elib (German Aerospace Center) (submittedVersion)
- Publication Database GFZ (GFZ German Research Centre for Geosciences) (submittedVersion)
- 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
- Martian atmosphere evolution, atmospheric escape, water inventory, mantle outgassing, hydrodynamic escape, thermal escape, carbonate precipitation, serpentinization, surface pressure, early Mars, Noachian, Hesperian, Amazonian
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
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