Warm Jupiters Beyond the Tidal Synchronization Limit may Exhibit a Wide Range of Secondary Eclipse Depths

With the JWST we can now characterize the atmospheres of longer-orbit planets, but this moves us into a regime where we cannot assume that tidal forces from the star have eroded the planets’ obliquities and synchronized their rotation rates. These rotation vectors may be tracers of formation and evo...

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Principais autores:	Emily Rauscher, Nicolas B. Cowan, Rodrigo Luger
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2023-01-01
coleção:	The Astronomical Journal
Assuntos:	Exoplanet atmospheres Atmospheric dynamics Exoplanets Extrasolar gaseous planets James Webb Space Telescope Eclipses
Acesso em linha:	https://doi.org/10.3847/1538-3881/acd342
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