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hal.structure.identifierUniversity College of London [London] [UCL]
dc.contributor.authorTINETTI, G.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorDROSSART, P.
dc.contributor.authorECCLESTON, P.
hal.structure.identifierMax-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
dc.contributor.authorHARTOGH, P.
hal.structure.identifierECLIPSE 2017
dc.contributor.authorLECONTE, J.
hal.structure.identifierINAF - Osservatorio Astronomico di Palermo
dc.contributor.authorMICELA, G.
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorOLLIVIER, M.
hal.structure.identifierEuropean Space Research and Technology Centre [ESTEC]
dc.contributor.authorPILBRATT, G.
hal.structure.identifierUniversity of Valencia
dc.contributor.authorPUIG, L.
dc.contributor.authorHESKE, A.
dc.contributor.authorTURRINI, D.
hal.structure.identifierInstituut voor Sterrenkunde [Leuven]
dc.contributor.authorVANDENBUSSCHE, B.
hal.structure.identifierSpace Research Centre of Polish Academy of Sciences [CBK]
dc.contributor.authorWOLKENBERG, P.
dc.date.conference2017-09-17
dc.description.abstractEnThousands of exoplanets have now been discovered with a huge range of masses, sizes and orbits: from rocky Earth-size planets to large gas giants grazing the surface of their host star. However, the essential nature of these exoplanets remains largely mysterious: there is no known, discernible pattern linking the presence, size, or orbital parameters of a planet to the nature of its parent star. We have little idea whether the chemistry of a planet is linked to its formation environment, or whether the type of host star drives the physics and chemistry of the planet's birth, and evolution. Progress with these science questions demands a large, unbiased spectroscopic survey of exoplanets. The ESA ARIEL M4 candidate mission has been conceived to conduct such a survey and to explore the nature of exoplanet atmospheres and interiors and, through this, the key factors affecting the formation and evolution of planetary systems.
dc.language.isoen
dc.title.enThe science of ARIEL
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.conference.titleEuropean Planetary Science Congress 2017, held 17-22 September, 2017 in Riga Latvia, id. EPSC2017-713
bordeaux.countryLV
bordeaux.conference.cityRiga
bordeaux.peerReviewedoui
hal.identifierhal-01622249
hal.version1
hal.invitednon
hal.proceedingsnon
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01622249v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.au=TINETTI,%20G.&DROSSART,%20P.&ECCLESTON,%20P.&HARTOGH,%20P.&LECONTE,%20J.&rft.genre=unknown


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