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hal.structure.identifierSpace Research Institute of Austrian Academy of Sciences [IWF]
dc.contributor.authorLAMMER, H.
dc.contributor.authorHANSLMEIER, A.
hal.structure.identifierMax-Planck-Institut für Chemie [MPIC]
dc.contributor.authorSCHNEIDER, Jodi
dc.contributor.authorSTATEVA, I. K.
hal.structure.identifierInstitut de Biologie du Développement de Marseille [IBDM]
dc.contributor.authorBARTHELEMY, M.
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierUniversité Sciences et Technologies - Bordeaux 1 [UB]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierLaboratoire Hippolyte Fizeau [FIZEAU]
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
dc.contributor.authorBELU, A. R.
dc.contributor.authorBISIKALO, D.
dc.contributor.authorBONAVITA, M.
dc.contributor.authorEYBL, V.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorCOUDÉ DU FORESTO, V.
hal.structure.identifierResearch and Scientific Support Department, ESTEC [RSSD]
dc.contributor.authorFRIDLUND, M.
hal.structure.identifierON/MCT [ON/MCT, 20921-030, Rio de Janeiro, Brazil)]
dc.contributor.authorDVORAK, R.
dc.contributor.authorEGGL, S.
dc.contributor.authorGRIESSMEIER, Jean-Mathias
dc.contributor.authorGÜDEL, M.
dc.contributor.authorGÜNTHER, E.
dc.contributor.authorHAUSLEITNER, W.
hal.structure.identifierSwedish Institute of Space Physics [Uppsala / Kiruna] [IRF]
dc.contributor.authorHOLMSTRÖM, M.
hal.structure.identifierFinnish Meteorological Institute [FMI]
dc.contributor.authorKALLIO, E.
dc.contributor.authorKHODACHENKO, M. L.
dc.contributor.authorKONOVALENKO, A. A.
dc.contributor.authorKRAUSS, S.
dc.contributor.authorKSANFOMALITY, L. V.
hal.structure.identifierPolar Geophysical Institute of Russian Academy of Sciences [PGI]
dc.contributor.authorKULIKOV, Yu. N.
dc.contributor.authorKYSLYAKOVA, K.
dc.contributor.authorLEITZINGER, M.
dc.contributor.authorLISEAU, R.
dc.contributor.authorLOHINGER, E.
dc.contributor.authorODERT, P.
dc.contributor.authorPALLE, E.
dc.contributor.authorREINERS, A.
hal.structure.identifierInstitut de Ciencies de l'Espai [Barcelona] [ICE-CSIC]
dc.contributor.authorRIBAS, I.
hal.structure.identifierSpace Research Institute of Austrian Academy of Sciences [IWF]
dc.contributor.authorRUCKER, H. O.
hal.structure.identifierNeurobiologie des états de veille et de sommeil [EA3734]
dc.contributor.authorSARDA, N.
dc.contributor.authorSECKBACH, J.
hal.structure.identifierInstitute of Astronomy of the Russian Academy of Sciences [INASAN]
dc.contributor.authorSHEMATOVICH, V. I.
dc.contributor.authorSOZZETTI, A.
dc.contributor.authorTAVROV, A.
dc.contributor.authorXIANG-GRÜSS, M.
dc.date.issued2010
dc.description.abstractEnAfter the discovery of more than 400 planets beyond our Solar System, the characterization of exoplanets as well as their host stars can be considered as one of the fastest growing fields in space science during the past decade. The characterization of exoplanets can only be carried out in a well coordinated interdisciplinary way which connects planetary science, solar/stellar physics and astrophysics. We present a status report on the characterization of exoplanets and their host stars by reviewing the relevant space- and ground-based projects. One finds that the previous strategy changed from space mission concepts which were designed to search, find and characterize Earth-like rocky exoplanets to: A statistical study of planetary objects in order to get information about their abundance, an identification of potential target and finally its analysis. Spectral analysis of exoplanets is mandatory, particularly to identify bio-signatures on Earth-like planets. Direct characterization of exoplanets should be done by spectroscopy, both in the visible and in the infrared spectral range. The way leading to the direct detection and characterization of exoplanets is then paved by several questions, either concerning the pre-required science or the associated observational strategy.
dc.language.isoen
dc.title.enExoplanet status report: Observation, characterization and evolution of exoplanets and their host stars
dc.typeArticle de revue
dc.identifier.doi10.1134/S0038094610040039
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.journalSolar System Research
bordeaux.page290-310
bordeaux.volume44
bordeaux.peerReviewedoui
hal.identifierhal-00541870
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00541870v1
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