Haze Optical Depth in Exoplanet Atmospheres Varies with Rotation Rate: Implications for Observations

Haze Optical Depth in Exoplanet Atmospheres Varies with Rotation Rate: Implications for Observations

Transmission spectroscopy supports the presence of uncharacterized, light-scattering and -absorbing hazes in the atmospheres of many exoplanets. The complexity of factors influencing the formation, 3D transport, radiative impact, and removal of hazes makes it challenging to match theoretical models...

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Bibliographic Details
Main Authors: Maureen Cohen, Paul I. Palmer, Adiv Paradise, Massimo A. Bollasina, Paola Ines Tiranti
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astronomical Journal
Subjects:
Exoplanet atmospheres
Exoplanet atmospheric dynamics
Exoplanets
Extrasolar rocky planets
Online Access:https://doi.org/10.3847/1538-3881/ad1ab9

Internet

https://doi.org/10.3847/1538-3881/ad1ab9

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