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14 days ago

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Nightside clouds form and winds drive disequilibrium chemistry on a hot Jupiter - Nature Astronomy

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Nightside clouds form and winds drive disequilibrium chemistry on a hot Jupiter - Nature Astronomy

Phase-curve observations of the 'hot Jupiter' exoplanet WASP-43b, made at mid-infrared wavelengths using JWST, provide evidence that fast winds limit the formation of methane on the cooler, cloudy nightside of the planet.

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Nightside clouds form and winds drive disequilibrium chemistry on a hot Jupiter - Nature Astronomy

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Nightside clouds form and winds drive disequilibrium chemistry on a hot Jupiter - Nature Astronomy

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