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hal.structure.identifiersSE 2011
dc.contributor.authorHEDELT, P.
dc.contributor.authorGODOLT, M.
hal.structure.identifierZentrum für Astronomie und Astrophysik [Berlin] [ZAA]
dc.contributor.authorGRENFELL, J. L.
hal.structure.identifiersSE 2011
dc.contributor.authorVON PARIS, P.
dc.contributor.authorRAUER, H.
dc.contributor.authorSCHREIER, F.
hal.structure.identifiersSE 2011
dc.contributor.authorSELSIS, Franck
hal.structure.identifierDLR Institut für Methodik der Fernerkundung / DLR Remote Sensing Technology Institute [IMF]
dc.contributor.authorTRAUTMANN, T.
dc.date.issued2011-10
dc.date.conference2011
dc.description.abstractEnWe present the spectral appearance of Earth-like exoplanets in the habitable zone of different main sequence (F, K and G-type) stars and their spectral response to small orbital distance variations. Using atmospheric profiles from a 1D atmosphere model, we compute transmission and emission spectra in the infrared using a cloud-free line-by-line radiative transfermodel. The orbital distanceswere chosen such that surface temperatures in the atmosphericmodel are in the range of 273K (outer run) to 303K (inner run). The spectra are then analyzed in light of current and future space telescopes like the JamesWebb Telescope (JWST), Spitzer and the ground based European Extremely Large Telescope (E-ELT) in order to discuss the measurability of certain spectral features.
dc.language.isoen
dc.title.enSpectral response of Earth-like planets to orbital variations
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.page729
bordeaux.countryFR
bordeaux.conference.cityNantes
bordeaux.peerReviewedoui
hal.identifierhal-00666789
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00666789v1
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