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Understanding Exoplanet Atmospheres
2022The study of exoplanet atmospheres is a blossoming field. Over the past two decades, dozens of hot gas giant atmospheres have been observed using a variety of techniques with both space and ground telescopes, revealing the presence of water, the ubiquity of clouds, the presence of equatorial jets, the existence of photoevaporation, and much more. For
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2017
Atmospheres of exoplanets are our only window into the physical and chemical processes occurring in these distant worlds. These processes are important tracers of the origins and evolution of planetary systems, including our Solar System. In this broader context, we could better understand how common (or unique) are the conditions leading to the ...
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Atmospheres of exoplanets are our only window into the physical and chemical processes occurring in these distant worlds. These processes are important tracers of the origins and evolution of planetary systems, including our Solar System. In this broader context, we could better understand how common (or unique) are the conditions leading to the ...
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Science (New York, N.Y.), 2014
Exoplanets that orbit close to their host stars are much more highly irradiated than their solar system counterparts. Understanding the thermal structures and appearances of these planets requires investigating how their atmospheres respond to such extreme stellar forcing.
Kevin B, Stevenson +15 more
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Exoplanets that orbit close to their host stars are much more highly irradiated than their solar system counterparts. Understanding the thermal structures and appearances of these planets requires investigating how their atmospheres respond to such extreme stellar forcing.
Kevin B, Stevenson +15 more
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Exoplanet Interiors and Atmosphere
2022Madhu Kashyap Jagadeesh, Usha Shekhar
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Atmospheric Thermal Tides of Exoplanets
Gravitational interactions between a planet and its host star may have important effects on the orbit and rotation rates of the two bodies. Gravitational tides, through tidal friction, change the rotation period of a planet, ultimately synchronizing it with its orbital period and tidally locking it when the orbit is nearly circular. While the theory ofopenaire +1 more source

