Published September 2, 2022
| Version v2
Poster
Open
3D Climate modelling of TRAPPIST-1 c with a Venus-like atmosphere: large-scale circulation and observational prospects
Authors/Creators
- 1. Institute of Astrophysics and Space Sciences (IA), Lisbon, Portugal
- 2. Institute of Astrophysics of Andalusia (IAA – CSIC), Granada, Spain
- 3. The McGill Space Institute, Montréal, QC, Canada;
- 4. Laboratoire de Météorologie Dynamique/IPSL, CNRS, Sorbonne Université
- 5. NASA Goddard Space Flight Center, Greenbelt, MD, United States
Description
In this work we present for the first time a 3D climate simulation of a “exo-Venus” using the same atmospheric parameters as on present-day Venus. The main goals are: 1. To study the large-scale atmospheric circulation of TRAPPIST-1 c: benchmark for rocky exoplanets with Venus-like instellations orbiting late-type M-dwarfs. 2) To address observational prospects by computing thermal phase curves and transmission spectra.
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Poster_SEA2022_DQuirino_GGilli_et_al_toupload.pdf
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