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hal.structure.identifierUnivers, Théorie, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) [UTINAM]
dc.contributor.authorMOUSIS, O.
hal.structure.identifierCenter for medical imaging
dc.contributor.authorATKINSON, D.
dc.contributor.authorAMATO, M.
hal.structure.identifierEnvironnement et Grandes Cultures [EGC]
dc.contributor.authorASLAM, S.
hal.structure.identifierDepartment of Atmospheric, Oceanic, and Space Sciences [Ann Arbor] [AOSS]
dc.contributor.authorATREYA, S.
dc.contributor.authorBLANC, M.
hal.structure.identifierUnivers, Théorie, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) [UTINAM]
dc.contributor.authorBRUGGER, B.
hal.structure.identifierUniversity of Oxford
dc.contributor.authorCALCUTT, S.
dc.contributor.authorCAVALIÉ, T.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorCHARNOZ, S.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorCOUSTENIS, A.
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorDELEUIL, M.
hal.structure.identifierASP 2017
dc.contributor.authorDOBRIJEVIC, M.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorENCRENAZ, T.
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorFERRI, F.
dc.contributor.authorFLETCHER, L.
hal.structure.identifierJoseph Louis LAGRANGE [LAGRANGE]
dc.contributor.authorGUILLOT, T.
hal.structure.identifierMax-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
dc.contributor.authorHARTOGH, P.
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorHOFSTADTER, M.
hal.structure.identifierEscuela Tecnica Superior de Ingenieria Bilbao
dc.contributor.authorHUESO, R.
dc.date.conference2017-09-17
dc.description.abstractEnUranus and Neptune, referred to as ice giants, are fundamentally different from the better-known gas giants (Jupiter and Saturn). Exploration of an ice giant system is a high-priority science objective, as these systems (including the magnetosphere, satellites, rings, atmosphere, and interior) challenge our understanding of planetary formation and evolution. The importance of the ice giants is reflected in NASA's 2011 Decadal Survey, comments from ESA's SSC in response to L2/L3 mission proposals and results of the 2017 NASA/ESA Ice Giants study. A crucial part of exploration of the ice giants is in situ sampling of the atmosphere via an atmospheric probe. A probe would bring insights in two broad themes: the formation history of our Solar System and the processes at play in planetary atmospheres. Here we summarize the science driver for in situ measurements at these two planets and discuss possible mission concepts that would be consistent with the constraints of ESA M-class missions.
dc.language.isoen
dc.title.enScientific rationale and concepts for in situ probe exploration of Uranus and Neptune
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. EPSC2017-299
bordeaux.countryLV
bordeaux.conference.cityRiga
bordeaux.peerReviewedoui
hal.identifierhal-01622214
hal.version1
hal.invitednon
hal.proceedingsnon
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01622214v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.au=MOUSIS,%20O.&ATKINSON,%20D.&AMATO,%20M.&ASLAM,%20S.&ATREYA,%20S.&rft.genre=unknown


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