Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b

Hot Jupiters are among the best-studied exoplanets, but it is still poorly understood how their chemical composition and cloud properties vary with longitude. Theoretical models predict that clouds may condense on the nightside and that molecular abundances can be driven out of equilibrium by zonal...

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Main Authors:	Bell, TJ, Crouzet, N, Cubillos, PE, Kreidberg, L, Piette, AAA, Roman, MT, Barstow, JK, Blecic, J, Carone, L, Coulombe, L, Ducrot, E, Hammond, M, Mendonça, JM, Moses, JI, Parmentier, V, Stevenson, KB, Teinturier, L, Zhang, M, Batalha, NM, Bean, JL, Benneke, B, Charnay, B, Chubb, KL, Demory, B, Tan, X, Taylor, J
格式:	Journal article
語言:	English
出版:	Nature Research 2024

Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b

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