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Origin and Formation of Planetary Systems

hal.structure.identifierLaboratoire d'astrophysique de l'observatoire de Besançon (UMR 6091) [LAOB]
dc.contributor.authorALIBERT, Y.
dc.contributor.authorBROEG, C.
hal.structure.identifierPhysikalisches Institut [Bern]
dc.contributor.authorBENZ, W.
hal.structure.identifierThüringer Landessternwarte Tautenburg [TLS]
dc.contributor.authorWUCHTERL, G.
hal.structure.identifierLaboratoire de Planétologie et Géodynamique de Nantes [UMR 6112] [LPGN]
dc.contributor.authorGRASSET, O.
hal.structure.identifierLaboratoire de Planétologie et Géodynamique de Nantes [UMR 6112] [LPGN]
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorSOTIN, C.
hal.structure.identifierUniversidad Autónoma de Madrid [UAM]
dc.contributor.authorEIROA, Carlos
hal.structure.identifierMax-Planck-Institut für Astronomie [MPIA]
dc.contributor.authorHENNING, Thomas
hal.structure.identifierMax-Planck-Institut für Astronomie [MPIA]
dc.contributor.authorHERBST, Tom
hal.structure.identifierHarvard-Smithsonian Center for Astrophysics [CfA]
dc.contributor.authorKALTENEGGER, Lisa
dc.contributor.authorLÉGER, Alain
hal.structure.identifierDepartment of Radio and Space Science [Göteborg]
dc.contributor.authorLISEAU, Réne
hal.structure.identifierSpace Research Institute of Austrian Academy of Sciences [IWF]
dc.contributor.authorLAMMER, Helmut
hal.structure.identifierNASA ExoPlanet Science Institute [NExScI]
dc.contributor.authorBEICHMAN, Charles
hal.structure.identifierNASA Goddard Space Flight Center [GSFC]
dc.contributor.authorDANCHI, William
hal.structure.identifierResearch and Scientific Support Department, ESTEC [RSSD]
dc.contributor.authorFRIDLUND, Malcolm
hal.structure.identifierLunar and Planetary Laboratory [Tucson] [LPL]
dc.contributor.authorLUNINE, Jonathan
hal.structure.identifierIstituto Nazionale di Astrofisica [INAF]
dc.contributor.authorPARESCE, Francesco
hal.structure.identifierSTFC Rutherford Appleton Laboratory [RAL]
dc.contributor.authorPENNY, Alan
hal.structure.identifierLandessternwarte Königstuhl [ZAH] [LSW]
dc.contributor.authorQUIRRENBACH, Andreas
hal.structure.identifierLeiden Observatory [Leiden]
dc.contributor.authorRÖTTGERING, Huub
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierUniversité Sciences et Technologies - Bordeaux 1 [UB]
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
dc.contributor.authorSELSIS, Franck
hal.structure.identifierObservatoire de Paris - Site de Meudon [OBSPM]
dc.contributor.authorSCHNEIDER, Jean
hal.structure.identifierSRON Netherlands Institute for Space Research [SRON]
dc.contributor.authorSTAM, Daphne
hal.structure.identifierUniversity College of London [London] [UCL]
dc.contributor.authorTINETTI, Giovanna
hal.structure.identifierSTFC Rutherford Appleton Laboratory [RAL]
hal.structure.identifierDepartment of Physics and Astronomy [Milton Keynes]
dc.contributor.authorWHITE, Glenn J.
dc.date.issued2010-01
dc.identifier.issn1531-1074
dc.description.abstractEnTo estimate the occurrence of terrestrial exoplanets and maximize the chance of finding them, it is crucial to understand the formation of planetary systems in general and that of terrestrial planets in particular. We show that a reliable formation theory should not only explain the formation of the Solar System, with small terrestrial planets within a few AU and gas giants farther out, but also the newly discovered exoplanetary systems with close-in giant planets. Regarding the presently known exoplanets, we stress that our current knowledge is strongly biased by the sensitivity limits of current detection techniques (mainly the radial velocity method). With time and improved detection methods, the diversity of planets and orbits in exoplanetary systems will definitely increase and help to constrain the formation theory further. In this work, we review the latest state of planetary formation in relation to the origin and evolution of habitable terrestrial planets.
dc.language.isoen
dc.publisherMary Ann Liebert
dc.title.enOrigin and Formation of Planetary Systems
dc.typeArticle de revue
dc.identifier.doi10.1089/AST.2009.0372
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.journalAstrobiology
bordeaux.page19-32
bordeaux.volume10
bordeaux.peerReviewedoui
hal.identifierhal-00543311
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00543311v1
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