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Konferenzbeitrag

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

MPG-Autoren

Venot,  Olivia
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Crouzet,  Nicolas
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Carone,  Ludmila
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Tremblin,  Pascal
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Parmentier,  Vivien
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Moses,  Julianne
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Cubillos,  Patricio
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Blecic,  Jasmina
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Molliere,  Paul
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Kreidberg,  Laura
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Stevenson,  Kevin B.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Externe Ressourcen

https://ui.adsabs.harvard.edu/abs/2018EPSC...12.1026V
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Zitation

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.


Zitierlink: https://hdl.handle.net/21.11116/0000-0005-CA72-7
Zusammenfassung
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.