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Photochemical Hazes Dramatically Alter Temperature Structure and Atmospheric Circulation in 3D Simulations of Hot Jupiters

Photochemical hazes are expected to form in hot Jupiter atmospheres and may explain the strong scattering slopes and muted spectral features observed in the transmission spectra of many hot Jupiters. Absorption and scattering by photochemical hazes have the potential to drastically alter temperature...

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Principais autores: Maria E. Steinrueck, Tommi Koskinen, Panayotis Lavvas, Vivien Parmentier, Sebastian Zieba, Xianyu Tan, Xi Zhang, Laura Kreidberg
Format: Artigo
Sprog:Inglês
Udgivet: IOP Publishing 2023-01-01
Serier:The Astrophysical Journal
Fag:
Exoplanet atmospheres
Exoplanet atmospheric dynamics
Exoplanet atmospheric structure
Online adgang:https://doi.org/10.3847/1538-4357/acd4bb
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