A cloudy fit to the atmosphere of WASP-107 b

Context. WASP-107 b has been observed comprehensively by JWST in the near- and mid-IR bands, meaning we can probe its composition and internal dynamics. Recent analyses reveal a 8 − 10 μm silicate feature, but it remains uncertain how silicate clouds form on this planet. Aims. We aim to fit the comp...

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Bibliografiske detaljer

Principais autores:	Huang Helong, Min Michiel, Ormel Chris W., Dyrek Achrène, Crouzet Nicolas
Format:	Artigo
Sprog:	Inglês
Udgivet:	EDP Sciences 2026-04-01
Serier:	Astronomy & Astrophysics
Fag:	planets and satellites: atmospheres planets and satellites: gaseous planets planets and satellites: individual: wasp-107 b
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