# From thermal dissociation to condensation in the atmospheres of ultra hot Jupiters: WASP-121b in context

@article{Parmentier2018FromTD,
title={From thermal dissociation to condensation in the atmospheres of ultra hot Jupiters: WASP-121b in context},
author={Vivien Parmentier and Michael R. Line and Jacob L. Bean and Megan Mansfield and Laura Kreidberg and Roxana E. Lupu and Channon Visscher and J. M. D{\'e}sert and Jonathan J. Fortney and Magali Deleuil and Jacob Arcangeli and A. P. Showman and Mark S. Marley},
journal={arXiv: Earth and Planetary Astrophysics},
year={2018}
}
A new class of exoplanets has emerged: the ultra hot Jupiters, the hottest close-in gas giants. Most of them have weaker than expected spectral features in the $1.1-1.7\mu m$ bandpass probed by HST/WFC3 but stronger spectral features at longer wavelengths probed by Spitzer. This led previous authors to puzzling conclusions about the thermal structures and chemical abundances of these planets. Using the SPARC/MITgcm, we investigate how thermal dissociation, ionization, H$^-$ opacity and clouds… Expand
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