hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | MOUSIS, O. | |
hal.structure.identifier | University of Idaho [Moscow, USA] | |
dc.contributor.author | ATKINSON, D.H. | |
hal.structure.identifier | Jet Propulsion Laboratory [JPL] | |
dc.contributor.author | SPILKER, T. | |
hal.structure.identifier | NASA Ames Research Center [ARC] | |
dc.contributor.author | VENKATAPATHY, E. | |
hal.structure.identifier | Thales Alenia Space [Toulouse] [TAS] | |
dc.contributor.author | PONCY, J. | |
hal.structure.identifier | The Boeing Company, Huntington Beach | |
dc.contributor.author | FRAMPTON, R. | |
hal.structure.identifier | Laboratoire de Physique et Chimie de l'Environnement et de l'Espace [LPC2E] | |
dc.contributor.author | LEBRETON, Jean-Pierre | |
hal.structure.identifier | Laboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA] | |
dc.contributor.author | COUSTENIS, A. | |
hal.structure.identifier | Jet Propulsion Laboratory [JPL] | |
dc.contributor.author | REH, K. | |
hal.structure.identifier | University of Leicester | |
dc.contributor.author | FLETCHER, L.N. | |
hal.structure.identifier | Departamento de Fisica Aplicada [Bilbao] | |
dc.contributor.author | HUESO, R. | |
hal.structure.identifier | NASA Goddard Space Flight Center [GSFC] | |
dc.contributor.author | AMATO, M.J. | |
hal.structure.identifier | NASA Ames Research Center [ARC] | |
dc.contributor.author | COLAPRETE, A. | |
hal.structure.identifier | Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU] | |
dc.contributor.author | FERRI, F. | |
hal.structure.identifier | Faculty of Aerospace Engineering [Delft] | |
dc.contributor.author | STAM, D. | |
hal.structure.identifier | Physikalisches Institut [Bern] | |
dc.contributor.author | WURZ, P. | |
hal.structure.identifier | University of Michigan [Ann Arbor] | |
dc.contributor.author | ATREYA, S. | |
hal.structure.identifier | NASA Goddard Space Flight Center [GSFC] | |
dc.contributor.author | ASLAM, S. | |
hal.structure.identifier | Cornell University [New York] | |
dc.contributor.author | BANFIELD, D.J. | |
hal.structure.identifier | University of Oxford | |
dc.contributor.author | CALCUTT, S. | |
hal.structure.identifier | Space Research Institute of Austrian Academy of Sciences [IWF] | |
dc.contributor.author | FISCHER, G. | |
hal.structure.identifier | The Open University [Milton Keynes] [OU] | |
dc.contributor.author | HOLLAND, A. | |
hal.structure.identifier | Leiden Observatory [Leiden] | |
dc.contributor.author | KELLER, C. | |
hal.structure.identifier | Leibniz-Institute of Photonic Technology | |
dc.contributor.author | KESSLER, E. | |
hal.structure.identifier | School of Physical Sciences [Milton Keynes] | |
dc.contributor.author | LEESE, M. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | LEVACHER, P. | |
hal.structure.identifier | The Open University [Milton Keynes] [OU] | |
dc.contributor.author | MORSE, A. | |
hal.structure.identifier | Instituto de Astrofísica de Andalucía [IAA] | |
dc.contributor.author | MUÑOZ, O. | |
hal.structure.identifier | Laboratoire de Physique et Chimie de l'Environnement et de l'Espace [LPC2E] | |
dc.contributor.author | RENARD, Jean-Baptiste | |
hal.structure.identifier | The Open University [Milton Keynes] [OU] | |
dc.contributor.author | SHERIDAN, S. | |
hal.structure.identifier | Joseph Louis LAGRANGE [LAGRANGE] | |
dc.contributor.author | SCHMIDER, F.-X. | |
hal.structure.identifier | Leiden Observatory [Leiden] | |
dc.contributor.author | SNIK, F. | |
hal.structure.identifier | Space Science Division [San Antonio] | |
dc.contributor.author | WAITE, J.H. | |
hal.structure.identifier | Rheinische Friedrich-Wilhelms-Universität Bonn | |
dc.contributor.author | BIRD, M. | |
hal.structure.identifier | ASP 2016 | |
dc.contributor.author | CAVALIÉ, T. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | DELEUIL, M. | |
hal.structure.identifier | University of California [Santa Cruz] [UC Santa Cruz] | |
dc.contributor.author | FORTNEY, J. | |
hal.structure.identifier | Laboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA] | |
dc.contributor.author | GAUTIER, D. | |
hal.structure.identifier | Joseph Louis LAGRANGE [LAGRANGE] | |
dc.contributor.author | GUILLOT, T. | |
hal.structure.identifier | Department of Astronomy [Ithaca] | |
dc.contributor.author | LUNINE, J.I. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | MARTY, B. | |
hal.structure.identifier | NASA Goddard Space Flight Center [GSFC] | |
dc.contributor.author | NIXON, C. | |
hal.structure.identifier | Jet Propulsion Laboratory [JPL] | |
dc.contributor.author | ORTON, G.S. | |
hal.structure.identifier | University of Leicester | |
dc.contributor.author | SÁNCHEZ-LAVEGA, A. | |
dc.date.created | 2015 | |
dc.date.issued | 2016 | |
dc.identifier.issn | 0032-0633 | |
dc.description.abstractEn | The Hera Saturn entry probe mission is proposed as an M-class mission led by ESA with a contribution from NASA. It consists of one atmospheric probe to be sent into the atmosphere of Saturn, and a Carrier-Relay spacecraft. In this concept, the Hera probe is composed of ESA and NASA elements, and the Carrier-Relay Spacecraft is delivered by ESA. The probe is powered by batteries, and the Carrier-Relay Spacecraft is powered by solar panels and batteries. We anticipate two major subsystems to be supplied by the United States, either by direct procurement by ESA or by contribution from NASA: the solar electric power system (including solar arrays and the power management and distribution system), and the probe entry system (including the thermal protection shield and aeroshell). Hera is designed to perform in situ measurements of the chemical and isotopic compositions as well as the 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's aim is to probe well into the cloud-forming region of the troposphere, below the region accessible to remote sensing, to the locations where certain cosmogenically abundant species are expected to be well mixed. By leading to an improved understanding of the processes by which giant planets formed, including the composition and properties of the local solar nebula at the time and location of giant planet formation, Hera will extend the legacy of the Galileo and Cassini missions by further addressing the creation, formation, and chemical, dynamical, and thermal evolution of the giant planets, the entire solar system including Earth and the other terrestrial planets, and formation of other planetary systems. | |
dc.description.sponsorship | INITIATIVE D'EXCELLENCE AIX MARSEILLE UNIVERSITE - ANR-11-IDEX-0001 | |
dc.language.iso | en | |
dc.publisher | Elsevier | |
dc.subject.en | Probe | |
dc.subject.en | In situ measurements | |
dc.subject.en | Atmosphere | |
dc.subject.en | ESA's Cosmic Vision Medium class size call | |
dc.subject.en | Saturn | |
dc.title.en | The Hera Saturn entry probe mission | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1016/j.pss.2015.06.020 | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph] | |
dc.identifier.arxiv | 1510.07685 | |
bordeaux.journal | Planetary and Space Science | |
bordeaux.page | 80-103 | |
bordeaux.volume | 130 | |
bordeaux.peerReviewed | oui | |
hal.identifier | insu-01351010 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//insu-01351010v1 | |
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