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Cited by 24Astro and Planetary SciencePlanetary Science and ExplorationGeological and Geochemical Analysis

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Venus

Fegley, B.·2003·Treatise on Geochemistry
DOI 10.1016/b0-08-043751-6/01150-6
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Research works printed but not linked: 35

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    “Venus has a 92 bar atmosphere (1 bar being approximately the pressure of Earth’s atmosphere at sea level), consisting of 96.5% CO2 and 3.5% N2 (Fegley, 2003).”
    Influential

Metadata

Authors
Fegley, B.
Affiliations
Washington University in St. Louis (US)
Corresponding author
Fegley, B.
ORCID
Fegley, B.
Venue
Treatise on Geochemistry
Publisher
Elsevier
Published
2003
Pages
487-507
DOI
10.1016/b0-08-043751-6/01150-6
OpenAlex
W3022918712
Cited by
24
References
0
Citations by year
2025: 1 · 2024: 1 · 2023: 2 · 2020: 4 · 2019: 1 · 2016: 2 · 2015: 1 · 2014: 2 · 2013: 2 · 2012: 3
FWCI
1.20
Type
book chapter
Language
en
Open access
closed
Licence
www.elsevier.com/tdm/userlicense/1.0/ (tdm)
Locations
Treatise on Geochemistry (publishedVersion)
Topics
  • Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
  • Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Planetary Science and Exploration
  • Physical Sciences › Earth and Planetary Sciences › Geochemistry and Petrology › Geological and Geochemical Analysis
Keywords
Venus, planetary geochemistry, Venus atmosphere, Venus surface, Venus interior

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