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The Castalia mission to Main Belt Comet 133P/Elst-Pizarro

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  • معلومة اضافية
    • Contributors:
      School of Physical Sciences Milton Keynes; Faculty of Science, Technology, Engineering and Mathematics Milton Keynes; The Open University Milton Keynes (OU)-The Open University Milton Keynes (OU); Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS); Max-Planck-Gesellschaft; Department of Mechanical and Aerospace Engineering Univ Strathclyde; University of Strathclyde Glasgow; Orbitale Hochtechnologie Bremen (OHB Systems AG); Institut de Planétologie et d'Astrophysique de Grenoble (IPAG); Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ); Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes 2016-2019 (UGA 2016-2019 )-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes 2016-2019 (UGA 2016-2019 ); Space Research Institute of Austrian Academy of Sciences (IWF); Austrian Academy of Sciences (OeAW); Centro di Ateneo di Studi e Attività Spaziali “Giuseppe Colombo” (CISAS); Università degli Studi di Padova = University of Padua (Unipd); Department of Atmospheric, Oceanic and Planetary Physics Oxford (AOPP); University of Oxford; Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS); Istituto Nazionale di Astrofisica (INAF); Space and Atmospheric Physics Group London; Blackett Laboratory; Imperial College London-Imperial College London; Mullard Space Science Laboratory (MSSL); University College of London London (UCL); Astrophysics Research Centre Belfast (ARC); Queen's University Belfast (QUB); Institut d'Astrophysique et de Géophysique Liège; Université de Liège; Royal Observatory of Belgium = Observatoire Royal de Belgique (ROB); Instituto de Astrofísica de Andalucía (IAA); Consejo Superior de Investigaciones Cientificas España = Spanish National Research Council Spain (CSIC); Instituto de Astrofisica de Canarias (IAC); Centre for Astrophysics and Planetary Science Canterbury (CAPS); University of Kent Canterbury; Dipartimento di Fisica e Astronomia "Galileo Galilei"; Istituto di Astrofisica Spaziale e Fisica cosmica - Roma (IASF-Roma); Technische Universität Dresden = Dresden University of Technology (TU Dresden); Tel Aviv University (TAU); Università degli Studi di Napoli “Parthenope” = University of Naples (PARTHENOPE); Physikalisches Institut Bern; Universität Bern = University of Bern = Université de Berne (UNIBE); Universität Heidelberg Heidelberg = Heidelberg University
    • بيانات النشر:
      HAL CCSD
      Elsevier
    • الموضوع:
      2018
    • Collection:
      Institut National de la Recherche Agronomique: ProdINRA
    • نبذة مختصرة :
      International audience ; We describe Castalia, a proposed mission to rendezvous with a Main Belt Comet (MBC), 133P/Elst-Pizarro. MBCs are a recently discovered population of apparently icy bodies within the main asteroid belt between Mars and Jupiter, which may represent the remnants of the population which supplied the early Earth with water. Castalia will perform the first exploration of this population by char-acterising 133P in detail, solving the puzzle of the MBC's activity, and making the first in situ measurements of water in the asteroid belt. In many ways a successor to ESA's highly successful Rosetta mission, Castalia will allow direct comparison between very different classes of comet, including measuring critical isotope ratios, plasma and dust properties. It will also feature the first radar system to visit a minor body, mapping the ice in the interior. Castalia was proposed, in slightly different versions, to the ESA M4 and M5 calls within the Cosmic Vision programme. We describe the science motivation for the mission, the measurements required to achieve the scientific goals, and the proposed instrument payload and spacecraft to achieve these.
    • Relation:
      hal-02350051; https://hal.science/hal-02350051; https://hal.science/hal-02350051/document; https://hal.science/hal-02350051/file/1-s2.0-S0273117717306622-main.pdf
    • الرقم المعرف:
      10.1016/j.asr.2017.09.011
    • الدخول الالكتروني :
      https://hal.science/hal-02350051
      https://hal.science/hal-02350051/document
      https://hal.science/hal-02350051/file/1-s2.0-S0273117717306622-main.pdf
      https://doi.org/10.1016/j.asr.2017.09.011
    • Rights:
      http://creativecommons.org/licenses/by/ ; info:eu-repo/semantics/OpenAccess
    • الرقم المعرف:
      edsbas.CF51FD60