Formation of Organic Hazes in CO2-rich Sub-Neptune Atmospheres within the Graphite Stability Regime

Super-Earths and sub-Neptunes are the most common exoplanets, with a “radius valley” suggesting that super-Earths may form by shedding sub-Neptunes’ gaseous envelopes. Exoplanets that lie closer to the super-Earth side of the valley are more likely to have lost a significant fraction of their origin...

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Autori principali:	Sai Wang, Zhengbo Yang, Chao He, Haixin Li, Yu Liu, Yingjian Wang, Xiao’ou Luo, Sarah E. Moran, Cara Pesciotta, Sarah M. Hörst, Julianne I. Moses, Véronique Vuitton, Laurène Flandinet
Natura:	Artigo
Lingua:	Inglês
Pubblicazione:	IOP Publishing 2025-01-01
Serie:	The Astrophysical Journal
Soggetti:	Exoplanet atmospheric composition Exoplanet atmospheres Laboratory astrophysics Complex organic molecules Mass spectrometry
Accesso online:	https://doi.org/10.3847/1538-4357/adfa0a
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