Influence of CO versus CH4 on organic haze formation in atmospheres of diverse terrestrial exoplanets

Context. Terrestrial exoplanets are expected to host secondary, high-metallicity atmospheres derived from the outgassing of volatiles such as N2, CO2, H2O, CH4, and CO. Photochemical organic hazes are likely to form in such environments, significantly impacting both atmospheric observation and plane...

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Autors principals:	Wang Sai, Yang Zhengbo, Li Haixin, He Chao, Wang Yingjian, Luo Xiao’ou, Liu Yu, Hörst Sarah M., Moran Sarah E., Vuitton Véronique, Flandinet Laurène, McGuiggan Patricia
Format:	Artigo
Idioma:	Inglês
Publicat:	EDP Sciences 2026-05-01
Col·lecció:	Astronomy & Astrophysics
Matèries:	methods: laboratory: molecular techniques: spectroscopic planets and satellites: atmospheres planets and satellites: composition planets and satellites: terrestrial planets
Accés en línia:	https://www.aanda.org/articles/aa/full_html/2026/05/aa58994-26/aa58994-26.html
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