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dc.contributor.authorVALLAT, Claire
dc.contributor.authorROATSCH, Thomas
hal.structure.identifierImperial College London
dc.contributor.authorDOUGHERTY, Michele K.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorCOUSTENIS, Athena
hal.structure.identifierGraduate School of Information Sciences [Sendai]
dc.contributor.authorKASABA, Yasumasa
hal.structure.identifierSwedish Institute of Space Physics [Uppsala / Kiruna] [IRF]
dc.contributor.authorWAHLUND, Jan-Erik
hal.structure.identifierInstitute of Atmospheric Physics [Prague] [IAP]
dc.contributor.authorSANTOLÍK, Ondřej
hal.structure.identifierSwedish Institute of Space Physics [Uppsala / Kiruna] [IRF]
dc.contributor.authorBARABASH, Stas
hal.structure.identifierINAF - Osservatorio Astronomico di Padova [OAPD]
dc.contributor.authorCREMONESE, Gabriele
hal.structure.identifierUniversità degli Studi di Napoli “Parthenope” = University of Naples [PARTHENOPE]
dc.contributor.authorPALUMBO, Pasquale
dc.contributor.authorROTHKAEHL, Hanna
hal.structure.identifierDipartimento di Ingegneria Meccanica e Aerospaziale [Roma La Sapienza] [DIMA]
dc.contributor.authorIESS, Luciano
hal.structure.identifierIstituto de Astrofisica Spaziale et Fisica cosmica [IASF]
dc.contributor.authorPICCIONI, Giuseppe
hal.structure.identifierJohns Hopkins University Applied Physics Laboratory [Laurel, MD] [APL]
dc.contributor.authorBRANDT, Pontus
hal.structure.identifierDLR Institute of Planetary Research
dc.contributor.authorHUSSMANN, Hauke
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorLANGEVIN, Yves
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorPOULET, François
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorPLAUT, Jeffrey
dc.contributor.authorLORENTE, Rosario
hal.structure.identifierDLR Institute of Planetary Research
dc.contributor.authorJAUMANN, Ralf
hal.structure.identifierEuropean Space Astronomy Centre [ESAC]
dc.contributor.authorALTOBELLI, Nicolas
hal.structure.identifierUniversity of Leicester
dc.contributor.authorFLETCHER, Leigh
dc.contributor.authorRETHERFORD, Kurt
dc.contributor.authorBUNCE, E.
dc.contributor.authorVAN HOOLST, Tim
hal.structure.identifierDLR Institute of Planetary Research
dc.contributor.authorHOFFMANN, Harald
hal.structure.identifierLaboratoire de Planétologie et Géodynamique [UMR 6112] [LPG]
dc.contributor.authorTOBIE, G.
dc.contributor.authorMUELLER-WODARG, Ingo
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorCECCONI, Baptiste
dc.contributor.authorACCOMAZZO, Andrea
hal.structure.identifierPhysikalisches Institut [Bern]
dc.contributor.authorWURZ, Peter
hal.structure.identifierLos Alamos National Laboratory [LANL]
dc.contributor.authorGURVITS, Leonid
dc.contributor.authorTOSI, Federico
dc.contributor.authorGLADSTONE, Randy
dc.contributor.authorERD, Christian
dc.contributor.authorCIMO, Giuseppe
hal.structure.identifierMax-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
dc.contributor.authorKRUPP, Norbert
hal.structure.identifierMax-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
dc.contributor.authorHARTOGH, Paul
dc.contributor.authorWITASSE, Olivier
hal.structure.identifierDepartment of Information Engineering and Computer Science [DISI]
dc.contributor.authorBRUZZONE, Lorenzo
hal.structure.identifierLaboratoire de Planétologie et Géodynamique [UMR 6112] [LPG]
dc.contributor.authorGRASSET, Olivier
dc.contributor.authorKASPI, Yohai
hal.structure.identifierMullard Space Science Laboratory [MSSL]
dc.contributor.authorMASTERS, Adam
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
hal.structure.identifierASP 2018
dc.contributor.authorCAVALIÉ, T.
dc.contributor.authorSTEVENSON, David John
dc.contributor.authorBOUTONNET, Arnaud
dc.contributor.authorMUNOZ CREGO, Claudio
dc.contributor.authorTANCO, Ignacio
dc.date.issued2018
dc.date.conference2018-07-14
dc.description.abstractEnJUICE - JUpiter ICy moons Explorer - is the first large mission in the ESA Cosmic Vision programme. Due to launch in May 2022 and arrival at Jupiter in October 2029, it will make detailed observations of the Jovian system, with a special focus on the planet itself, its giant magnetosphere, and the three icy moons: Ganymede, Callisto and Europa. The current mission baseline assumes a Jupiter tour of almost three years including two close flybys of Europa, fifteen flybys of Ganymede, and twelve flybys of Callisto, together with a high inclination phase of six months in order to characterize Jupiter high latitudes. In August 2032, JUICE will then orbit Ganymede for at least ten months, down to an altitude of 500km. The first goal of JUICE is to to characterize the conditions that might have led to the emergence of habitable environments among the Jovian satellites. Ganymede is a high-priority target as it provides a unique laboratory for analyzing the nature, evolution and habitability of icy worlds, including the characteristics of subsurface oceans, and its unique magnetosphere interaction with the Jovian magnetodisc. For Europa, the focus will be on recently active zones, while Callisto will be explored as a witness of the early Solar System. JUICE will also investigate the Jupiter system as an archetype of gas giants. The circulation, meteorology, chemistry and structure of the Jovian atmosphere will be studied from the cloud tops to the thermosphere and ionosphere. JUICE will also study the properties of the magnetodisc, and will analyse the coupling processes within the magnetosphere, ionosphere and thermosphere. The payload consists of 10 instruments plus a ground-based experiment (PRIDE) to better constrain the S/C position. A remote sensing package includes imaging (JANUS) and spectral-imaging capabilities from the UV to the sub-mm wavelengths (UVS, MAJIS, SWI). A geophysical package consists of a laser altimeter (GALA) and a radar sounder (RIME) for exploring the moons, and a radio science experiment (3GM) to sound the atmospheres and to determine the gravity fields. The in-situ package comprises a suite to study plasma and neutral gas environments (PEP) with remote sensing capabilities via energetic neutrals, a magnetometer (J-MAG) and a radio and plasma wave instrument (RPWI).
dc.language.isoen
dc.title.enJUICE: A European Mission to Jupiter and its Icy Moons
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.title42nd COSPAR Scientific Assembly. Held 14-22 July 2018, in Pasadena, California, USA, Abstract id. B5.3-31-18.
bordeaux.countryUS
bordeaux.conference.cityPasadena
bordeaux.peerReviewedoui
hal.identifierhal-01901900
hal.version1
hal.invitednon
hal.proceedingsnon
hal.conference.end2018-07-22
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01901900v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2018&rft.au=VALLAT,%20Claire&ROATSCH,%20Thomas&DOUGHERTY,%20Michele%20K.&COUSTENIS,%20Athena&KASABA,%20Yasumasa&rft.genre=unknown


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