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Discovering the atmospheres of hot Jupiters

Published online by Cambridge University Press:  24 September 2020

P. Wilson Cauley Open the ORCID record for P. Wilson Cauley [Opens in a new window]
P. Wilson Cauley*
Affiliation:
LASP, CU Boulder 1234 Innovation Dr., Boulder, CO 80305 email: paca7401@lasp.colorado.edu
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Abstract

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Hot Jupiters are an extraordinary class of exoplanets, orbiting their host stars with periods of hours to a few days. Some of these objects have day-side temperatures approaching photospheric temperatures of late K-type stars. I will give an overview of how we characterize the atmospheres of these fascinating objects and some the more recent exciting results to come from ground and space-based telescopes, as well as what the future holds for detailed characterization of short-period exoplanet atmospheres.

Keywords

planetary systemstechniques: spectroscopic
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S354: Solar and Stellar Magnetic Fields: Origins and Manifestations , June 2019 , pp. 467 - 472
Copyright
© International Astronomical Union 2020

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