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

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...

Bibliografiset tiedot
Päätekijät:	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
Aineistotyyppi:	Journal article
Kieli:	English
Julkaistu:	Nature Research 2024

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