Publicated:
16 Feb 2024
Authors:
B. Akinsanmi, S. C. C. Barros, M. Lendl et al.
Summary:
Ultra-hot Jupiters present a unique opportunity to understand the physics and chemistry of planets at extreme conditions. WASP-12b stands out as an archetype of this class of exoplanets. We performed comprehensive analyses of the transits, occultations, and phase curves of WASP-12b by combining new CHEOPS observations with previous TESS and Spitzer data to measure the planet’s tidal deformation, atmospheric properties, and orbital decay rate.
Here you can find the link to the paper on arXiv and here from the magazine Astronomy and Astrophysics.
