TRANSITIONS IN THE CLOUD COMPOSITION OF HOT JUPITERS

TRANSITIONS IN THE CLOUD COMPOSITION OF HOT JUPITERS

Over a large range of equilibrium temperatures, clouds shape the transmission spectrum of hot Jupiter atmospheres, yet their composition remains unknown. Recent observations show that the Kepler light. curves of some hot Jupiters are asymmetric: for the hottest planets, the light. curve peaks before...

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Bibliographic Details
Main Authors: Parmentier, Vivien, Fortney, Jonathan J., Showman, Adam P., Morley, Caroline, Marley, Mark S.
Other Authors: Univ Arizona, Dept Planetary Sci
Language:en
Published: IOP PUBLISHING LTD 2016
Subjects:
planets and satellites: atmospheres
planets and satellites: gaseous planets
radiative transfer
scattering
Online Access:http://hdl.handle.net/10150/622056
http://arizona.openrepository.com/arizona/handle/10150/622056

Internet

http://hdl.handle.net/10150/622056
http://arizona.openrepository.com/arizona/handle/10150/622056

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