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dc.contributor.authorTURBET, M.
hal.structure.identifierNamur Center for Complex Systems [Namur] [NaXys]
dc.contributor.authorBOLMONT, E.
hal.structure.identifierLaboratoire de Météorologie Dynamique (UMR 8539) [LMD]
dc.contributor.authorFORGET, F.
hal.structure.identifierECLIPSE 2017
dc.contributor.authorLECONTE, J.
hal.structure.identifierECLIPSE 2017
dc.contributor.authorSELSIS, Franck
dc.date.conference2017-09-17
dc.description.abstractEnThe years 2016-2017 have been extremely fruitful in discoveries of interesting nearby Earth-size exoplanets. The detections of Proxima Cen b and TRAPPIST-1 planets are major discoveries mostly because these - very likely rocky - planets are the best candidates for future atmospheric characterization by transit spectroscopy, direct imaging, or thermal phase curve with the forthcoming ground (e.g. E-ELT) or space-based (e.g. JWST) astronomical observatories. We explore the possible climates of these planets and produce observational constraints that can be used to discriminate between all the possible atmospheric states of the planets.
dc.language.isoen
dc.title.enProxima Cen and TRAPPIST-1 exoplanetary systems: possible climates and observational constraints
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.conference.titleEuropean Planetary Science Congress 2017, held 17-22 September, 2017 in Riga Latvia, id. EPSC2017-320
bordeaux.countryLV
bordeaux.conference.cityRiga
bordeaux.peerReviewedoui
hal.identifierhal-01622321
hal.version1
hal.invitednon
hal.proceedingsnon
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01622321v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.au=TURBET,%20M.&BOLMONT,%20E.&FORGET,%20F.&LECONTE,%20J.&SELSIS,%20Franck&rft.genre=unknown


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