Venus as a Nearby Exoplanetary Laboratory

The key goals of the astrobiology community are to identify environments beyond Earth that may be habitable, and to search for signs of life in those environments. A fundamental aspect of understanding the limits of habitable environments and detectable signatures is the study of where such environm...

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Bibliographic Details
Published in:arXiv.org 2020-08
Main Authors: Kane, Stephen R, Arney, Giada, Byrne, Paul, Crisp, David, Domagal-Goldman, Shawn, Goldblatt, Colin, Grinspoon, David, Head, James W, Lenardic, Adrian, Meadows, Victoria, Unterborn, Cayman, Way, Michael J
Format: Article
Language:English
Subjects:
Astrobiology
Atmospheric models
Bifurcations
Extrasolar planets
Frequency analysis
Habitability
Signatures
Venus
Venus atmosphere
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Summary:The key goals of the astrobiology community are to identify environments beyond Earth that may be habitable, and to search for signs of life in those environments. A fundamental aspect of understanding the limits of habitable environments and detectable signatures is the study of where such environments can occur. Thus, the need to study the creation, evolution, and frequency of environments hostile to habitability is an integral part of the astrobiology story. The study of these environments provides the opportunity to understand the bifurcation between habitable and uninhabitable conditions on planetary bodies. The archetype of such a planet is Earth's sibling planet, Venus, which provides a unique opportunity to explore the processes that created a completely uninhabitable environment and thus define the conditions that rule out bio-related signatures. We advocate a continued comprehensive study of our neighboring planet, to include models of early atmospheres, compositional abundances, and Venus-analog frequency analysis from current and future exoplanet data. Critically, new missions to Venus that provide in-situ data are necessary to address the major gaps in our current understanding, and to enable us to take the next steps in characterizing planetary habitability.
ISSN:2331-8422