Early Habitability and Crustal Decarbonation of a Stagnant‐Lid Venus

Author:

Höning Dennis12ORCID,Baumeister Philipp34ORCID,Grenfell John Lee3ORCID,Tosi Nicola3ORCID,Way Michael J.567ORCID

Affiliation:

1. Origins Center Groningen The Netherlands

2. Department of Earth‐ and Life Sciences Vrije Universiteit Amsterdam Amsterdam The Netherlands

3. German Aerospace Center (DLR) Institute of Planetary Research Berlin Germany

4. Department of Astronomy and Astrophysics Berlin Institute of Technology Berlin Germany

5. NASA Goddard Institute for Space Studies New York NY USA

6. GSFC Sellers Exoplanet Environments Collaboration Greenbelt MD USA

7. Department of Physics and Astronomy Theoretical Astrophysics Uppsala University Uppsala Sweden

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference100 articles.

1. The formation of an impact‐generated H2O atmosphere and its implications for the early thermal history of the earth;Abe Y.;Lunar and Planetary Science Conference Proceedings,1985

2. Improved Magnus` form approximation of saturation vapor pressure

3. Simulating the thermochemical magmatic and tectonic evolution of Venus's mantle and lithosphere: Two-dimensional models

4. The need for mass balance and feedback in the geochemical carbon cycle

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