Understanding atmospheric properties and chemical composition of ultra-hot Jupiter HAT-P-7b: II. Mapping the effects of kinetic gas composition

@article{Molaverdikhani2020UnderstandingAP,
  title={Understanding atmospheric properties and chemical composition of ultra-hot Jupiter HAT-P-7b: II. Mapping the effects of kinetic gas composition},
  author={K. Molaverdikhani and C. Helling and B. Lew and R. Macdonald and D. Samra and N. Iro and P. Woitke and V. Parmentier},
  journal={Astronomy and Astrophysics},
  year={2020}
}
The atmospheres of ultra-hot Jupiters are commonly considered to be at thermochemical equilibrium. We aim to provide disequilibrium chemistry maps for a global understanding of the chemistry in HAT-P-7b's atmosphere and assess the importance of disequilibrium chemistry on UHJs. We apply a hierarchical modelling approach utilising 97 1D atmospheric profiles from 3D GCM of HAT-P-7b. For each 1D profile, we evaluate our kinetic cloud formation model consistently with the local gas-phase… Expand
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