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hal.structure.identifiersSE 2011
dc.contributor.authorMAURIN, A. S.
hal.structure.identifiersSE 2011
dc.contributor.authorSELSIS, Franck
hal.structure.identifierFORMATION STELLAIRE 2011
dc.contributor.authorHERSANT, F.
hal.structure.identifiersSE 2011
dc.contributor.authorBELU, A. R.
dc.date.issued2011-10
dc.date.conference2011
dc.description.abstractEnThe photometric signal we receive from a star hosting a planet is modulated by the variation of the planet signal with its orbital phase. Future telescopes (JWST and EChO) will have the capability to measure thermal phase curves of exoplanets including hot rocky planets in transiting and nontransiting configurations. We model the thermal emission of a synchronous rocky planet with no atmosphere and its apparent variation with the orbital phase for a given orbital inclination. We assume that the planet is detected by radial velocity. We simulate observed noisy phase curves and then apply a procedure to retrieve the radius and albedo of the planet and the inclination of the orbit.
dc.language.isoen
dc.source.title2011epsc.conf..908M
dc.title.enMeasuring the albedo, inclination and radius of nontransiting terrestrial exoplanets
dc.typeCommunication dans un congrès
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
bordeaux.page908
bordeaux.countryFR
bordeaux.title.proceeding2011epsc.conf..908M
bordeaux.conference.cityNantes
bordeaux.peerReviewedoui
hal.identifierhal-00664594
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00664594v1
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