Venusian Habitable Climate Scenarios: Modeling Venus Through Time and Applications to Slowly Rotating Venus‐Like Exoplanets-Reference-Cited by-同舟云学术

Venusian Habitable Climate Scenarios: Modeling Venus Through Time and Applications to Slowly Rotating Venus‐Like Exoplanets

Published:2020-05 Issue:5 Volume:125 Page:
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Way M. J.¹²³^ORCID,Del Genio Anthony D.¹^ORCID

Affiliation:

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

2. GSFC Sellers Exoplanet Environments Collaboration Greenbelt MD USA

3. Theoretical Astrophysics, Department of Physics and Astronomy Uppsala University Uppsala Sweden

Publisher

American Geophysical Union (AGU)

Subject

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

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JE006276

Reference315 articles.

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4. Volatile accretion history of the terrestrial planets and dynamic implications

5. Alemi A. &Stevenson D.(2006).Why Venus has no moon. InAAS/Division for Planetary Sciences Meeting Abstracts #38 AAS/Division for Planetary Sciences Meeting Abstracts pp.07.03.

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