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The nonmagnetic nucleus of comet 67P/Churyumov-Gerasimenko

机译:67P / Churyumov-Gerasimenko彗星的非磁性核

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摘要

Knowledge of the magnetization of planetary bodies constrains their origin and evolution, as well as the conditions in the solar nebular at that time. On the basis of magnetic field measurements during the descent and subsequent multiple touchdown of the Rosetta lander Philae on the comet 67P/Churyumov-Gerasimenko (67P), we show that no global magnetic field was detected within the limitations of analysis. The Rosetta Magnetometer and Plasma Monitor (ROMAP) suite of sensors measured an upper magnetic field magnitude of less than 2 nanotesla at the cometary surface at multiple locations, with the upper specific magnetic moment being <3.1 x 10(-5) ampere-square meters per kilogram for meter-size homogeneous magnetized boulders. The maximum dipole moment of 67P is 1.6 x 10(8) ampere-square meters. We conclude that on the meter scale, magnetic alignment in the preplanetary nebula is of minor importance.
机译:行星体磁化的知识限制了它们的起源和演化以及当时太阳星云的条件。根据在彗星67P / Churyumov-Gerasimenko(67P)上Rosetta着陆器Philae下降和随后的多次降落期间的磁场测量,我们显示在分析范围内未检测到整体磁场。罗塞塔磁力仪和等离子监视器(ROMAP)传感器套件在多个位置测量了彗星表面的小于2纳特斯拉的上部磁场强度,上部比磁矩<3.1 x 10(-5)安培平方米米大小的均质磁石每千克每公斤。 67P的最大偶极矩为1.6 x 10(8)安培平方米。我们得出的结论是,在米尺度上,行星前星云中的磁对准不太重要。

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  • 来源
    《Science》 |2015年第6247期|494-494|共1页
  • 作者单位

    Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, D-38106 Braunschweig, Germany;

    Hungarian Acad Sci, Ctr Energy Res, H-1121 Budapest, Hungary;

    Austrian Acad Sci, Space Res Inst, A-8042 Graz, Austria;

    Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, D-38106 Braunschweig, Germany;

    Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, D-38106 Braunschweig, Germany|Russian Acad Sci, Space Res Inst, Moscow 117810, Russia;

    Univ London Imperial Coll Sci Technol & Med, London SW7 2AZ, England;

    Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany;

    Max Planck Inst Extraterr Phys, D-85741 Garching, Germany;

    Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, D-38106 Braunschweig, Germany;

    Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, D-38106 Braunschweig, Germany;

    Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany;

    German Aerosp Ctr DLR, Inst Planetary Res, D-12489 Berlin, Germany;

    Austrian Acad Sci, Space Res Inst, A-8042 Graz, Austria;

    German Aerosp Ctr DLR, Inst Planetary Res, D-12489 Berlin, Germany|Tech Univ Carolo Wilhelmina Braunschweig, Inst Theoret Phys, D-38106 Braunschweig, Germany;

    Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, D-38106 Braunschweig, Germany;

    Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90095 USA;

    Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, D-38106 Braunschweig, Germany;

    Austrian Acad Sci, Space Res Inst, A-8042 Graz, Austria;

    Max Planck Inst Extraterr Phys, D-85741 Garching, Germany;

    Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, D-38106 Braunschweig, Germany|Max Planck Inst Extraterr Phys, D-85741 Garching, Germany;

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  • 入库时间 2022-08-18 02:52:04

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