Effects of Ultraviolet Radiation on Sub-Neptune Exoplanet Hazes through Laboratory Experiments

Temperate sub-Neptune exoplanets could contain large inventories of water in various phases, such as water worlds with water-rich atmospheres or even oceans. Both space-based and ground-based observations have shown that many exoplanets likely also contain photochemically generated hazes. Haze parti...

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Detalles Bibliográficos

Principais autores:	Lori Huseby, Sarah E. Moran, Neil Pearson, Tiffany Kataria, Chao He, Cara Pesciotta, Sarah M. Hörst, Pierre Haenecour, Travis Barman, Vishnu Reddy, Nikole K. Lewis, Véronique Vuitton
Formato:	Artigo
Idioma:	Inglês
Publicado:	IOP Publishing 2025-01-01
Series:	The Planetary Science Journal
Assuntos:	Exoplanets Mini Neptunes Super Earths Exoplanet atmospheres Exoplanet atmospheric composition Exoplanet atmospheric evolution
Acceso en liña:	https://doi.org/10.3847/PSJ/adda4a
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