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The proposed Caroline ESA M3 mission to a Main Belt Comet

机译:拟议的Caroline ESA M3任务到主带彗星

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摘要

We describe Caroline, a mission proposal submitted to the European Space Agency in 2010 in response to the Cosmic Visions M3 call for medium-sized missions. Caroline would have travelled to a Main Belt Comet (MBC), characterizing the object during a flyby, and capturing dust from its tenuous coma for return to Earth. MBCs are suspected to be transition objects straddling the traditional boundary between volatile-poor rocky asteroids and volatile-rich comets. The weak cometary activity exhibited by these objects indicates the presence of water ice, and may represent the primary type of object that delivered water to the early Earth. The Caroline mission would have employed aerogel as a medium for the capture of dust grains, as successfully used by the NASA Stardust mission to Comet 81P/Wild 2. We describe the proposed mission design, primary elements of the spacecraft, and provide an overview of the science instruments and their measurement goals. Caroline was ultimately not selected by the European Space Agency during the M3 call; we briefly reflect on the pros and cons of the mission as proposed, and how current and future mission MBC mission proposals such as Castalia could best be approached. (C) 2018 COSPAR. Published by Elsevier Ltd.
机译:我们描述了卡罗琳(Caroline),这是2010年提交给欧洲航天局的一项任务建议,以回应Cosmic Visions M3对中型任务的呼吁。卡罗琳本可以前往主带彗星(MBC),在飞越过程中对物体进行表征,并从其昏迷昏迷中捕获灰尘,然后返回地球。 MBC被怀疑是跨越易挥发的岩石小行星和易挥发的彗星之间的传统边界的过渡物体。这些物体表现出的较弱的彗星活动表明存在水冰,并且可能代表了将水输送到地球早期的主要物体类型。卡罗琳号飞行任务将采用气凝胶作为捕获尘埃颗粒的媒介,这是NASA星尘任务对81P / Wild 2彗星成功使用的。我们描述了拟议的飞行任务设计,航天器的主要元素,并概述了科学仪器及其测量目标。 M3通话期间,欧洲航天局最终没有选择Caroline。我们简要回顾了所提出的任务的利弊,以及如何最好地接近当前和未来的MBC任务建议,例如Castalia。 (C)2018年COSPAR。由Elsevier Ltd.发布

著录项

  • 来源
    《Advances in space research》 |2018年第8期|1921-1946|共26页
  • 作者单位

    Univ Coll London, Mullard Space Sci Lab, Holmbury St Mary, Dorking RH5 6NT, Surrey, England;

    Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany;

    Univ Oxford, Clarendon Lab, Atmospher Phys, Parks Rd, Oxford OX1 3PU, England;

    Univ Kent, Sch Phys Sci, Ingram Bldg, Canterbury CT2 7NH, Kent, England;

    Univ Coll London, Mullard Space Sci Lab, Holmbury St Mary, Dorking RH5 6NT, Surrey, England;

    Queens Univ Belfast, Astrophys Res Ctr, Sch Math & Phys, Belfast BT7 1NN, Antrim, North Ireland;

    Planetary Sci Inst, 1700 East Ft Lowell Rd,Suite 106, Tucson, AZ 86719 USA;

    Planetary Sci Inst, 1700 East Ft Lowell Rd,Suite 106, Tucson, AZ 86719 USA;

    Johns Hopkins Univ, Appl Phys Lab, 11100 Johns Hopkins Rd, Laurel, MD 20723 USA;

    Univ Kent, Sch Phys Sci, Ingram Bldg, Canterbury CT2 7NH, Kent, England;

    Imperial Coll London, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England;

    Open Univ, Planetary & Space Sci, Sch Phys Sci, Milton Keynes MK7 6AA, Bucks, England;

    Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Asteroids; Comets; Interplanetary dust and gas;

    机译:小行星;彗星;行星际尘埃和气体;

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