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- W2891047814 abstract "The nightsides of synchronously rotating planets are sensitive probes of atmospheric heat transport; detecting thermal flux from the nightside of such a planet means that energy has been transported there from its dayside. We invert orbital phase curves into longitudinally resolved brightness distributions in order to estimate the nightside effective temperatures for twelve hot Jupiters with full-orbit infrared phase curves. We find that, although dayside temperatures on hot Jupiters are proportional to their irradiation temperatures, nightside temperatures of typical hot Jupiters are approximately 1000K. The three exceptions, WASP-12b, WASP-33b, and WASP-103b, are ultra-hot Jupiters: planets with dayside temperatures hot enough to dissociate molecular hydrogen. Models predict much more varied nightside temperatures than we observe. Energy balance models provide a better fit to the observations if wave propagation is negligible for heat transport. Alternatively, the relatively uniform nightside temperatures of hot Jupiters could be due to thick clouds. Mineral or sulfide clouds, if they had sufficiently large particles, could explain the uniform nightside temperature, as well as the relatively featureless nightside spectra of these planets." @default.
- W2891047814 created "2018-09-27" @default.
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- W2891047814 date "2018-08-31" @default.
- W2891047814 modified "2023-09-26" @default.
- W2891047814 title "A Universal Nightside Temperature on Hot Jupiters due to Nocturnal Clouds" @default.
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