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Geoscientific Model Development An interactive open-access journal of the European Geosciences Union
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GMD | Articles | Volume 13, issue 2
Geosci. Model Dev., 13, 707–716, 2020
https://doi.org/10.5194/gmd-13-707-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
Geosci. Model Dev., 13, 707–716, 2020
https://doi.org/10.5194/gmd-13-707-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Model experiment description paper 21 Feb 2020

Model experiment description paper | 21 Feb 2020

TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI): motivations and protocol version 1.0

Thomas J. Fauchez et al.

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Barstow, J. K. and Irwin, P. G. J.: Habitable worlds with JWST: transit spectroscopy of the TRAPPIST-1 system?, Mon. Not. R. Astron. Soc., 461, L92–L96, https://doi.org/10.1093/mnrasl/slw109, 2016. a, b
Bolmont, E., Selsis, F., Owen, J. E., Ribas, I., Raymond, S. N., Leconte, J., and Gillon, M.: Water loss from terrestrial planets orbiting ultracool dwarfs: implications for the planets of TRAPPIST-1, Mon. Not. R. Astron. Soc., 464, 3728–3741, https://doi.org/10.1093/mnras/stw2578, 2017. a
Bourrier, V., de Wit, J., Bolmont, E., Stamenkovic, V., Wheatley, P. J., Burgasser, A. J., Delrez, L., Demory, B.-O., Ehrenreich, D., Gillon, M., Jehin, E., Leconte, J., Lederer, S. M., Lewis, N., Triaud, A. H. M. J., and Grootel, V. V.: Temporal Evolution of the High-energy Irradiation and Water Content of TRAPPIST-1 Exoplanets, Astron. J., 154, 121, https://doi.org/10.3847/1538-3881/aa859c, 2017. a
Boutle, I. A., Mayne, N. J., Drummond, B., Manners, J., Goyal, J., Hugo Lambert, F., Acreman, D. M., and Earnshaw, P. D.: Exploring the climate of Proxima B with the Met Office Unified Model, Astron. Astrophys., 601, A120, https://doi.org/10.1051/0004-6361/201630020, 2017. a
Cantrell, J. R., Henry, T. J., and White, R. J.: The Solar Neighborhood XXIX: The Habitable Real Estate of Our Nearest Stellar Neighbors, Astron. J., 146, 99, https://doi.org/10.1088/0004-6256/146/4/99, 2013. a
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Atmospheric characterization of rocky exoplanets orbiting within the habitable zone of nearby M dwarf stars is around the corner with the James Webb Space Telescope (JWST), expected to be launch in 2021. Global climate models (GCMs) are powerful tools to model exoplanet atmospheres and to predict their habitability. However, intrinsic differences between the models can lead to various predictions. This paper presents an experiment protocol to evaluate these differences.
Atmospheric characterization of rocky exoplanets orbiting within the habitable zone of nearby M...
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