The DOI matches its Crossref record; 6 of the 6 references it cites were found in a registry or an index.
Atmospheric Evolution on Inhabited and Lifeless Worlds
Abstract
As the search for Earth-like exoplanets gathers pace, in order to understand them, we need comprehensive theories for how planetary atmospheres form and evolve. Written by two well-known planetary scientists, this text explains the physical and chemical principles of atmospheric evolution and planetary atmospheres, in the context of how atmospheric composition and climate determine a planet's habitability. The authors survey our current understanding of the atmospheric evolution and climate on Earth, on other rocky planets within our Solar System, and on planets far beyond. Incorporating a rigorous mathematical treatment, they cover the concepts and equations governing a range of topics, including atmospheric chemistry, thermodynamics, radiative transfer, and atmospheric dynamics, and provide an integrated view of planetary atmospheres and their evolution. This interdisciplinary text is an invaluable one-stop resource for graduate-level students and researchers working across the fields of atmospheric science, geochemistry, planetary science, astrobiology, and astronomy.
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In the citing paper
“Numerous redox-sensitive tracers corroborate negligible Archean O2 [reviewed, e.g., in (10, 63, 64)].”
From The Archean atmosphere (2020) · cites this paper as [64]
In the citing paper
“Within large uncertainties, volcanic and oxidative weathering inputs of N2 are comparable [(64), p. 204].”
From The Archean atmosphere (2020) · cites this paper as [64]
In the citing paper
“However, other outgassing estimates are 7 × 1010 mol N year−1 from arcs (157) or 9 ± 4 × 1010 mol N year−1 globally [(64), p. 204], such that current source and sink N fluxes balance within uncertainties.”
From The Archean atmosphere (2020) · cites this paper as [64]
In the citing paper
“As well as solar luminosity, Earth’s mean global temperature depends on the Bond albedo (the reflectivity over all wavelengths) and greenhouse effect [e.g., (64), pp. 34 to 36].”
From The Archean atmosphere (2020) · cites this paper as [64]
In the citing paper
“the atmosphere had 20 ± 10% O2 for only the last one-eighth of its history”
From Disequilibrium biosignatures over Earth history and implications for detecting exoplanet life (2018) · cites this paper as [26]
In the citing paper
“The N2-O2-H2O and O2-CH4 disequilibrium biosignatures may not have been present for much of Earth history because the atmosphere had 20 ± 10% O2 for only the last one-eighth of its history and virtually no O2 in the Archean [reviewed by Catling and Kasting (26), chap. 10].”
From Disequilibrium biosignatures over Earth history and implications for detecting exoplanet life (2018) · cites this paper as [26]
In the citing paper
“Diffusion-limited hydrogen escape would deplete an Earth-like planet of atmospheric methane in ~30 thousand years [(26), p. 215].”
From Disequilibrium biosignatures over Earth history and implications for detecting exoplanet life (2018) · cites this paper as [26]
In the citing paper
“Even in reducing atmospheres, CH4 has a geologically short lifetime.”
From Disequilibrium biosignatures over Earth history and implications for detecting exoplanet life (2018) · cites this paper as [26]
In the citing paper
“Furthermore, only 1 to 2% is due to serpentinization; the remaining 10 to 11% is from oxidation by sulfate, which does not generate H2 [(26), chap. 10; (45)].”
From Disequilibrium biosignatures over Earth history and implications for detecting exoplanet life (2018) · cites this paper as [26]
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Metadata
- Authors
- Catling, D. C., & Kasting, J. F.
- Affiliations
- University of Washington (US)
- Pennsylvania State University (US)
- Venue
- Cambridge University Press eBooks
- Publisher
- Cambridge University Press
- Published
- 2017-01-01
- OpenAlex
- W2611894198
- Cited by
- 342
- References
- 0
- Citations by year
- 2026: 16 · 2025: 31 · 2024: 35 · 2023: 39 · 2022: 33 · 2021: 31 · 2020: 41 · 2019: 41 · 2018: 62 · 2017: 9
- FWCI
- 30.40
- Type
- book
- Language
- en
- Open access
- closed
- Locations
- Cambridge University Press eBooks (publishedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
- Keywords
- atmospheric evolution, planetary atmospheres, habitability, exoplanets, atmospheric chemistry, radiative transfer, atmospheric thermodynamics, atmospheric dynamics, climate, Earth, terrestrial planets, astrobiology
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.
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