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In situ Exploration of the Giant Planets

hal.structure.identifierLaboratoire d'astrophysique de l'observatoire de Besançon (UMR 6091) [LAOB]
dc.contributor.authorMOUSIS, Olivier
dc.contributor.authorATKINSON, David H.
hal.structure.identifierRadio and Space Plasma Physics Group [Leicester] [RSPP]
dc.contributor.authorAMBROSI, Richard
hal.structure.identifierDepartment of Atmospheric, Oceanic, and Space Sciences [Ann Arbor] [AOSS]
dc.contributor.authorATREYA, Sushil
hal.structure.identifierCornell University [New York]
dc.contributor.authorBANFIELD, Don
hal.structure.identifierSwedish Institute of Space Physics [Uppsala / Kiruna] [IRF]
dc.contributor.authorBARABASH, Stas
hal.structure.identifierPSA Peugeot - Citroën [PSA]
dc.contributor.authorBLANC, Michel
hal.structure.identifierASP 2019
dc.contributor.authorCAVALIÉ, T.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorCOUSTENIS, Athena
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorDELEUIL, Magali
hal.structure.identifierGroupe de spectrométrie moléculaire et atmosphérique [GSMA]
dc.contributor.authorDURRY, Georges
hal.structure.identifierCentro di Ateneo di Studi e Attività Spaziali “Giuseppe Colombo” [CISAS]
dc.contributor.authorFERRI, Francesca
hal.structure.identifierUniversity of Leicester
dc.contributor.authorFLETCHER, Leigh
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorFOUCHET, Thierry
hal.structure.identifierJoseph Louis LAGRANGE [LAGRANGE]
dc.contributor.authorGUILLOT, Tristan
hal.structure.identifierMax-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
dc.contributor.authorHARTOGH, Paul
hal.structure.identifierDepartamento de Fisica Aplicada [Bilbao]
dc.contributor.authorHUESO, Ricardo
dc.contributor.authorHOFSTADTER, Mark
hal.structure.identifierGroupe de Recherche sur les Institutions, le Droit de l'Aménagement, de l'Urbanisme et de l'Habitat [GRIDAUH]
dc.contributor.authorLEBRETON, Jean-Pierre
dc.contributor.authorMANDT, Kathleen E.
hal.structure.identifierDLR Institut für Planetenforschung
dc.contributor.authorRAUER, Heike
hal.structure.identifierGroupe de spectrométrie moléculaire et atmosphérique [GSMA]
dc.contributor.authorRANNOU, Pascal
hal.structure.identifierLaboratoire de Physique et Chimie de l'Environnement et de l'Espace [LPC2E]
dc.contributor.authorRENARD, Jean-Baptiste
hal.structure.identifierDepartamento de Fisica Aplicada [Bilbao]
dc.contributor.authorSANCHEZ-LAVEGA, Agustín
dc.contributor.authorSAYANAGI, Kunio
dc.contributor.authorSIMON, Amy
dc.contributor.authorSPILKER, Thomas
dc.contributor.authorVENKATAPATHY, Ethiraj
hal.structure.identifierSpace Science Division [San Antonio]
dc.contributor.authorWAITE, J. Hunter
hal.structure.identifierPhysikalisches Institut [Bern]
dc.contributor.authorWURZ, Peter
dc.date.accessioned2021-07-07T15:44:20Z
dc.date.available2021-07-07T15:44:20Z
dc.date.issued2019
dc.identifier.urihttps://oskar-bordeaux.fr/handle/20.500.12278/95254
dc.descriptionPaper submitted in response to ESA's Call for Voyage 2050 Science Themes. arXiv admin note: substantial text overlap with arXiv:1708.00235
dc.description.abstractEnRemote sensing observations suffer significant limitations when used to study the bulk atmospheric composition of the giant planets of our solar system. This impacts our knowledge of the formation of these planets and the physics of their atmospheres. A remarkable example of the superiority of in situ probe measurements was illustrated by the exploration of Jupiter, where key measurements such as the determination of the noble gases' abundances and the precise measurement of the helium mixing ratio were only made available through in situ measurements by the Galileo probe. Here we describe the main scientific goals to be addressed by the future in situ exploration of Saturn, Uranus, and Neptune, placing the Galileo probe exploration of Jupiter in a broader context. An atmospheric entry probe targeting the 10-bar level would yield insight into two broad themes: i) the formation history of the giant planets and that of the Solar System, and ii) the processes at play in planetary atmospheres. The probe would descend under parachute to measure composition, structure, and dynamics, with data returned to Earth using a Carrier Relay Spacecraft as a relay station. An atmospheric probe could represent a significant ESA contribution to a future NASA New Frontiers or flagship mission to be launched toward Saturn, Uranus, and/or Neptune.
dc.language.isoen
dc.subject.enAstrophysics - Earth and Planetary Astrophysics
dc.title.enIn situ Exploration of the Giant Planets
dc.typeAutre document
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.identifier.arxiv1908.00917
bordeaux.hal.laboratoriesLaboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804*
bordeaux.institutionUniversité de Bordeaux
bordeaux.institutionCNRS
hal.identifierhal-02282409
hal.version1
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-02282409v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2019&rft.au=MOUSIS,%20Olivier&ATKINSON,%20David%20H.&AMBROSI,%20Richard&ATREYA,%20Sushil&BANFIELD,%20Don&rft.genre=unknown


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