P53A:
Climatic Evolution of Venus and Venus-Like Exoplanets II Posters
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P53A:
Climatic Evolution of Venus and Venus-Like Exoplanets II Posters
Climatic Evolution of Venus and Venus-Like Exoplanets II Posters
Session ID#: 23187
Session Description:
Although Venus today is hostile and uninhabitable, recent studies have shown that its climate evolution is complex and could
permit early habitable conditions. For example, recent 3-D modeling studies have showed that Venus may have been habitable for a large fraction of our solar system’s history (e.g. Yang et al. 2014, Way et al. 2016). Also, it has been suggested that alternate modes of plate tectonics could aid volatile cycling on timescales congruentbwith stable climates on Venus-like worlds (e.g. Lenardic et al. 2016). Advances in understanding the climates of Venus-like planets are important not only to understanding the evolution of our nearest planetary neighbor, but also to understanding Venus-like exoplanets, which may represent a cosmically ubiquitous type of world (Kane et al 2014). This session hopes to explore recent advances in understanding the evolution of the Venusian climate to provide a more complete view of Venus and Venus-like exoplanets.
permit early habitable conditions. For example, recent 3-D modeling studies have showed that Venus may have been habitable for a large fraction of our solar system’s history (e.g. Yang et al. 2014, Way et al. 2016). Also, it has been suggested that alternate modes of plate tectonics could aid volatile cycling on timescales congruentbwith stable climates on Venus-like worlds (e.g. Lenardic et al. 2016). Advances in understanding the climates of Venus-like planets are important not only to understanding the evolution of our nearest planetary neighbor, but also to understanding Venus-like exoplanets, which may represent a cosmically ubiquitous type of world (Kane et al 2014). This session hopes to explore recent advances in understanding the evolution of the Venusian climate to provide a more complete view of Venus and Venus-like exoplanets.
Primary Convener: Michael Way, NASA Goddard Institute for Space Studies, New York, United States
Conveners: Giada Nicole Arney, NASA Goddard Space Flight Center, Greenbelt, United States and Adrian Lenardic, Rice University, Earth, Environmental, and Planetary Sciences, Houston, United States
Chairs: Michael Way, Uppsala University, Department of Physics and Astronomy, Uppsala, Sweden, Giada Nicole Arney, NASA Goddard Space Flight Center, Greenbelt, United States and Adrian Lenardic, Rice University, Earth, Environmental, and Planetary Sciences, Houston, United States
OSPA Liaison: Michael Way, Uppsala University, Department of Physics and Astronomy, Uppsala, Sweden
Index Terms:
5210 Planetary atmospheres, clouds, and hazes [PLANETARY SCIENCES: ASTROBIOLOGY]
6295 Venus [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
6296 Extra-solar planets [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
Abstracts Submitted to this Session:
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