Afficher la notice abrégée

dc.contributor.authorCARTER-BOND, Jade C.
dc.contributor.authorO'BRIEN, David P.
hal.structure.identifierSSE 2014
dc.contributor.authorRAYMOND, Sean N.
dc.date.issued2014-04
dc.date.conference2012
dc.identifier.issn1743-9213
dc.description.abstractEnA diverse range of terrestrial planet compositions is believed to exist within known extrasolar planetary systems, ranging from those that are relatively Earth-like to those that are highly unusual, dominated by species such as refractory elements (Al and Ca) or C (as pure C, TiC and SiC)(Bond et al. 2010b). However, all prior simulations have ignored the impact that giant planet migration during planetary accretion may have on the final terrestrial planetary composition. Here, we combined chemical equilibrium models of the disk around five known planetary host stars (Solar, HD4203, HD19994, HD213240 and Gl777) with dynamical models of terrestrial planet formation incorporating various degrees of giant planet migration. Giant planet migration is found to drastically impact terrestrial planet composition by 1) increasing the amount of Mg-silicate species present in the final body; and 2) dramatically increasing the efficiency and amount of water delivered to the terrestrial bodies during their formation process.
dc.language.isoen
dc.publisherCambridge University Press (CUP)
dc.source.titleFormation, Detection, and Characterization of Extrasolar Habitable Planets, Proceedings of the International Astronomical Union, IAU Symposium, held in China, August 27, 2012, - Volume 293, pp. 229-234- 2014
dc.subject.enplanetary systems
dc.subject.enplanets and satellites: formation
dc.title.enMigration & Extra-solar Terrestrial Planets: Watering the Planets
dc.typeCommunication dans un congrès
dc.identifier.doi10.1017/S174392131301288X
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.journalProceedings of the International Astronomical Union
bordeaux.page229-234
bordeaux.volume293
bordeaux.countryCN
bordeaux.title.proceedingFormation, Detection, and Characterization of Extrasolar Habitable Planets, Proceedings of the International Astronomical Union, IAU Symposium, held in China, August 27, 2012, - Volume 293, pp. 229-234- 2014
bordeaux.conference.citybeijing
bordeaux.peerReviewedoui
hal.identifierhal-00987409
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00987409v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.btitle=Formation,%20Detection,%20and%20Characterization%20of%20Extrasolar%20Habitable%20Planets,%20Proceedings%20of%20the%20International%20Astronomical%20Union,%20IAU%20Sympos&rft.jtitle=Proceedings%20of%20the%20International%20Astronomical%20Union&rft.date=2014-04&rft.volume=293&rft.spage=229-234&rft.epage=229-234&rft.eissn=1743-9213&rft.issn=1743-9213&rft.au=CARTER-BOND,%20Jade%20C.&O'BRIEN,%20David%20P.&RAYMOND,%20Sean%20N.&rft.genre=unknown


Fichier(s) constituant ce document

FichiersTailleFormatVue

Il n'y a pas de fichiers associés à ce document.

Ce document figure dans la(les) collection(s) suivante(s)

Afficher la notice abrégée