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hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorMOUSIS, Olivier
hal.structure.identifierUniversity College of London [London] [UCL]
dc.contributor.authorATKINSON, David
hal.structure.identifierinstituto de fisica, universidade de Brasilia
hal.structure.identifierInternational Center for Condensed Matter Physics Brasilia
dc.contributor.authorAMATO, Michael
hal.structure.identifierNASA Goddard Space Flight Center [GSFC]
dc.contributor.authorASLAM, Shahid
hal.structure.identifierDepartment of Atmospheric, Oceanic, and Space Sciences [Ann Arbor] [AOSS]
dc.contributor.authorATREYA, Sushil
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorBLANC, Michel
dc.contributor.authorBOLTON, Scott
hal.structure.identifierUnivers, Transport, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) [UTINAM]
dc.contributor.authorBRUGGER, Bastien
hal.structure.identifierUniversity of Oxford
dc.contributor.authorCALCUTT, Simon
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorCAVALIÉ, Thibault
hal.structure.identifierInstitut de Physique du Globe de Paris [IPGP]
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorCHARNOZ, Sébastien
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.identifierASP 2017
dc.contributor.authorDOBRIJEVIC, M.
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.identifierMaison régionale de l'élevage
dc.contributor.authorGAUTIER, Daniel
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.identifierThe Open University [Milton Keynes] [OU]
dc.contributor.authorHOLLAND, Andrew
dc.date.issued2017-04
dc.date.conference2017-04-23
dc.description.abstractEnThe Hera Saturn entry probe mission is proposed as an ESA M-class mission to be piggybacked on a NASA spacecraft sent to or past the Saturn system. Hera consists of an atmospheric probe built by ESA and released into the atmosphere of Saturn by its NASA companion Saturn Carrier-Relay spacecraft. Hera will perform in situ measurements of the chemical and isotopic composition as well as the structure and dynamics of Saturn's atmosphere using a single probe, with the goal of improving our understanding of the origin, formation, and evolution of Saturn, the giant planets and their satellite systems, with extrapolation to extrasolar planets. Hera will probe well into and possibly beneath the cloud-forming region of the troposphere, below the region accessible to remote sensing, to locations where certain cosmogenically abundant species are expected to be well mixed. The Hera probe will be designed from ESA elements with possible contributions from NASA, and the Saturn/Carrier-Relay Spacecraft will be supplied by NASA through its selection via the New Frontier 2016 call or in the form of a flagship mission selected by the NASA "Roadmaps to Ocean Worlds" (ROW) program. The Hera probe will be powered by batteries, and we therefore anticipate only one major subsystems to be possibly supplied by the United States, either by direct procurement by ESA or by contribution from NASA: the thermal protection system of the probe. Following the highly successful example of the Cassini-Huygens mission, Hera will carry European and American instruments, with scientists and engineers from both agencies and many affiliates participating in all aspects of mission development and implementation. A Saturn probe is one of the six identified desired themes by the Planetary Science Decadal Survey committee on the NASA New Frontier's list, providing additional indication that a Saturn probe is of extremely high interest and a very high priority for the international community.
dc.language.isoen
dc.title.enThe Hera Saturn Entry Probe Mission: a Proposal in Response to the ESA M5 Call
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.page10664
bordeaux.volume19
bordeaux.conference.title19th EGU General Assembly, EGU2017, proceedings from the conference held 23-28 April, 2017 in Vienna, Austria., p.10664
bordeaux.countryAT
bordeaux.conference.cityVienne
bordeaux.peerReviewedoui
hal.identifierhal-01523809
hal.version1
hal.invitednon
hal.proceedingsnon
hal.conference.end2017-04-28
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01523809v1
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