hal.structure.identifier | Laboratoire d'astrophysique de l'observatoire de Besançon (UMR 6091) [LAOB] | |
dc.contributor.author | ALIBERT, Y. | |
dc.contributor.author | BROEG, C. | |
hal.structure.identifier | Physikalisches Institut [Bern] | |
dc.contributor.author | BENZ, W. | |
hal.structure.identifier | Thüringer Landessternwarte Tautenburg [TLS] | |
dc.contributor.author | WUCHTERL, G. | |
hal.structure.identifier | Laboratoire de Planétologie et Géodynamique de Nantes [UMR 6112] [LPGN] | |
dc.contributor.author | GRASSET, O. | |
hal.structure.identifier | Laboratoire de Planétologie et Géodynamique de Nantes [UMR 6112] [LPGN] | |
hal.structure.identifier | Jet Propulsion Laboratory [JPL] | |
dc.contributor.author | SOTIN, C. | |
hal.structure.identifier | Universidad Autónoma de Madrid [UAM] | |
dc.contributor.author | EIROA, Carlos | |
hal.structure.identifier | Max-Planck-Institut für Astronomie [MPIA] | |
dc.contributor.author | HENNING, Thomas | |
hal.structure.identifier | Max-Planck-Institut für Astronomie [MPIA] | |
dc.contributor.author | HERBST, Tom | |
hal.structure.identifier | Harvard-Smithsonian Center for Astrophysics [CfA] | |
dc.contributor.author | KALTENEGGER, Lisa | |
dc.contributor.author | LÉGER, Alain | |
hal.structure.identifier | Department of Radio and Space Science [Göteborg] | |
dc.contributor.author | LISEAU, Réne | |
hal.structure.identifier | Space Research Institute of Austrian Academy of Sciences [IWF] | |
dc.contributor.author | LAMMER, Helmut | |
hal.structure.identifier | NASA ExoPlanet Science Institute [NExScI] | |
dc.contributor.author | BEICHMAN, Charles | |
hal.structure.identifier | NASA Goddard Space Flight Center [GSFC] | |
dc.contributor.author | DANCHI, William | |
hal.structure.identifier | Research and Scientific Support Department, ESTEC [RSSD] | |
dc.contributor.author | FRIDLUND, Malcolm | |
hal.structure.identifier | Lunar and Planetary Laboratory [Tucson] [LPL] | |
dc.contributor.author | LUNINE, Jonathan | |
hal.structure.identifier | Istituto Nazionale di Astrofisica [INAF] | |
dc.contributor.author | PARESCE, Francesco | |
hal.structure.identifier | STFC Rutherford Appleton Laboratory [RAL] | |
dc.contributor.author | PENNY, Alan | |
hal.structure.identifier | Landessternwarte Königstuhl [ZAH] [LSW] | |
dc.contributor.author | QUIRRENBACH, Andreas | |
hal.structure.identifier | Leiden Observatory [Leiden] | |
dc.contributor.author | RÖTTGERING, Huub | |
hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
hal.structure.identifier | Observatoire aquitain des sciences de l'univers [OASU] | |
hal.structure.identifier | Université Sciences et Technologies - Bordeaux 1 [UB] | |
hal.structure.identifier | Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB] | |
dc.contributor.author | SELSIS, Franck | |
hal.structure.identifier | Observatoire de Paris - Site de Meudon [OBSPM] | |
dc.contributor.author | SCHNEIDER, Jean | |
hal.structure.identifier | SRON Netherlands Institute for Space Research [SRON] | |
dc.contributor.author | STAM, Daphne | |
hal.structure.identifier | University College of London [London] [UCL] | |
dc.contributor.author | TINETTI, Giovanna | |
hal.structure.identifier | STFC Rutherford Appleton Laboratory [RAL] | |
hal.structure.identifier | Department of Physics and Astronomy [Milton Keynes] | |
dc.contributor.author | WHITE, Glenn J. | |
dc.date.issued | 2010-01 | |
dc.identifier.issn | 1531-1074 | |
dc.description.abstractEn | To 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.iso | en | |
dc.publisher | Mary Ann Liebert | |
dc.title.en | Origin and Formation of Planetary Systems | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1089/AST.2009.0372 | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP] | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP] | |
bordeaux.journal | Astrobiology | |
bordeaux.page | 19-32 | |
bordeaux.volume | 10 | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-00543311 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-00543311v1 | |
bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astrobiology&rft.date=2010-01&rft.volume=10&rft.spage=19-32&rft.epage=19-32&rft.eissn=1531-1074&rft.issn=1531-1074&rft.au=ALIBERT,%20Y.&BROEG,%20C.&BENZ,%20W.&WUCHTERL,%20G.&GRASSET,%20O.&rft.genre=article | |