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dc.contributor.authorKALTENEGGER, L.
hal.structure.identifierCentre de Recherche Astrophysique de Lyon [CRAL]
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierUniversité Sciences et Technologies - Bordeaux 1 [UB]
dc.contributor.authorSELSIS, Franck
hal.structure.identifierResearch and Scientific Support Department, ESTEC [RSSD]
dc.contributor.authorFRIDLUND, M.
hal.structure.identifierSpace Research Institute of Austrian Academy of Sciences [IWF]
dc.contributor.authorLAMMER, H.
dc.contributor.authorBEICHMAN, Ch.
dc.contributor.authorDANCHI, W.
dc.contributor.authorEIROA, C.
hal.structure.identifierMax-Planck-Institut für Astronomie [MPIA]
dc.contributor.authorHENNING, T.
hal.structure.identifierMax-Planck-Institut für Astronomie [MPIA]
dc.contributor.authorHERBST, T.
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorLEGER, A.
dc.contributor.authorLISEAU, R.
hal.structure.identifierLunar and Planetary Laboratory [Tucson] [LPL]
dc.contributor.authorLUNINE, J.
hal.structure.identifierEuropean Southern Observatory [ESO]
dc.contributor.authorPARESCE, F.
dc.contributor.authorPENNY, A.
hal.structure.identifierLandessternwarte Königstuhl [ZAH] [LSW]
dc.contributor.authorQUIRRENBACH, A.
hal.structure.identifierLeiden Observatory [Leiden]
dc.contributor.authorROETTGERING, H.
dc.contributor.authorSCHNEIDER, Jodi
hal.structure.identifierSRON Netherlands Institute for Space Research [SRON]
dc.contributor.authorSTAM, D.
hal.structure.identifierUniversity College of London [London] [UCL]
dc.contributor.authorTINETTI, G.
hal.structure.identifierEngineering Department
dc.contributor.authorWHITE, G. J.
dc.date.created2009
dc.date.issued2010
dc.identifier.issn1531-1074
dc.description.abstractEnIn this paper we discuss how we can read a planets spectrum to assess its habitability and search for the signatures of a biosphere. After a decade rich in giant exoplanet detections, observation techniques have now reached the ability to find planets of less than 10 MEarth (so called Super-Earths) that may potentially be habitable. How can we characterize those planets and assess if they are habitable? The new field of extrasolar planet search has shown an extraordinary ability to combine research by astrophysics, chemistry, biology and geophysics into a new and exciting interdisciplinary approach to understand our place in the universe. The results of a first generation mission will most likely result in an amazing scope of diverse planets that will set planet formation, evolution as well as our planet in an overall context.
dc.language.isoen
dc.publisherMary Ann Liebert
dc.subject.enEarth and Planetary Astrophysics
dc.subject.enAstrophysics
dc.subject.enInstrumentation and Methods for Astrophysics
dc.title.enDeciphering Spectral Fingerprints of Habitable Extrasolar Planets
dc.typeArticle de revue
dc.identifier.doi10.1089/ast.2009.0381
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
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]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.identifier.arxiv0906.2263
bordeaux.journalAstrobiology
bordeaux.page89-102
bordeaux.volume10
bordeaux.issue1
bordeaux.peerReviewedoui
hal.identifierhal-00405861
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00405861v1
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