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- W3021541185 abstract "The insolation a planet receives from its parent star is the main driver of the climate and depends on the planet's orbital configuration. Planets with non-zero obliquity and eccentricity experience seasonal insolation variations. As a result, the climate exhibits a seasonal cycle, with its strength depending on the orbital configuration and atmospheric characteristics. In this study, using an idealized general circulation model, we examine the climate response to changes in eccentricity for both zero and non-zero obliquity planets. In the zero obliquity case, a comparison between the seasonal response to changes in eccentricity and perpetual changes in the solar constant shows that the seasonal response strongly depends on the orbital period and radiative timescale. More specifically, using a simple energy balance model, we show the importance of the latitudinal structure of the radiative timescale in the climate response. We also show that the response strongly depends on the atmospheric moisture content. The combination of an eccentric orbit with non-zero obliquity is complex, as the insolation also depends on the perihelion position. Although the detailed response of the climate to variations in eccentricity, obliquity, and perihelion is involved, the circulation is constrained mainly by the thermal Rossby number and the maximum temperature latitude. Finally, we discuss the importance of different planetary parameters that affect the climate response to orbital configuration variations." @default.
- W3021541185 created "2020-05-13" @default.
- W3021541185 creator A5029226983 @default.
- W3021541185 creator A5036348596 @default.
- W3021541185 date "2020-09-21" @default.
- W3021541185 modified "2023-10-12" @default.
- W3021541185 title "Atmospheric Dynamics on Terrestrial Planets with Eccentric Orbits" @default.
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- W3021541185 doi "https://doi.org/10.3847/1538-4357/abaef8" @default.
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