Variability in the atmosphere of the hot giant planet HAT-P-7 b

David J Armstrong,E. Mooij,J. Barstow,H. Osborn,J. Blake,Nessa Fereshteh Saniee

Published 2016 in Nature Astronomy

ABSTRACT

The detection of temporal variations in the peak of the phase curve of the hot giant exoplanet HAT-P-7 b is explained by changes in wind speed and cloud coverage in its atmosphere. Such ‘weather’ has never before been observed on a giant exoplanet.

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