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Atmospheric Circulation Of High-Obliquity Mini-Neptunes - Astrobiology
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Atmospheric Circulation Of High-Obliquity Mini-Neptunes - Astrobiology
With the operation of JWST, atmospheric characterization has now extended to low-mass exoplanets. In compact multiplanetary systems, secular spin-orbital resonance may preserve high obliquities and asynchronous rotation even for tidally-despinning, low-mass planets, potentially leading to unique atmospheric circulation patterns. To understand the impact on the atmospheric circulation and to identify the potential atmospheric observational signat…
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