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  Global Chemistry and Thermal Structure Models for the Hot Jupiter WASP-43b and Predictions for JWST

Venot, O., Crouzet, N., Carone, L., Tremblin, P., Parmentier, V., Moses, J., et al. (2018). Global Chemistry and Thermal Structure Models for the Hot Jupiter WASP-43b and Predictions for JWST. In European Planetary Science Congress.

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 Creators:
Venot, Olivia1, Author
Crouzet, Nicolas1, Author
Carone, Ludmila1, Author
Tremblin, Pascal1, Author
Parmentier, Vivien1, Author
Moses, Julianne1, Author
Cubillos, Patricio1, Author
Blecic, Jasmina1, Author
Molliere, Paul1, Author
Kreidberg, Laura1, Author
Stevenson, Kevin B.1, Author
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1Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners, ou_2421692              

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 Abstract: The James Webb Space Telescope (JWST) will be launched in 2020. The observations performed with this telescope will revolutionise the field of exoplanet characterisation. The Transiting Exoplanet Community propose to observe the exoplanet WASP-43b in order to better understand the physical structure and the chemical and dynamical processes occurring in the atmosphere of this planet. We present here the scientific objectives for this observation and the expected results.

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 Dates: 2018
 Publication Status: Issued
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Title: European Planetary Science Congress
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Start-/End Date: 2018

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Title: European Planetary Science Congress
Source Genre: Proceedings
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