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Properties of the 67P/Churyumov-Gerasimenko interior revealed by CONSERT radar

机译:CONSERT雷达显示67P / Churyumov-Gerasimenko内部的性能

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摘要

The Philae lander provides a unique opportunity to investigate the internal structure of a comet nucleus, providing information about its formation and evolution in the early solar system. We present Comet Nucleus Sounding Experiment by Radiowave Transmission (CONSERT) measurements of the interior of Comet 67P/Churyumov-Gerasimenko. From the propagation time and form of the signals, the upper part of the "head" of 67P is fairly homogeneous on a spatial scale of tens of meters. CONSERT also reduced the size of the uncertainty of Philae's final landing site down to approximately 21 by 34 square meters. The average permittivity is about 1.27, suggesting that this region has a volumetric dust/ice ratio of 0.4 to 2.6 and a porosity of 75 to 85%. The dust component may be comparable to that of carbonaceous chondrites.
机译:菲莱着陆器提供了一个独特的机会来研究彗核的内部结构,并提供有关其在早期太阳系中的形成和演化的信息。我们通过67P / Churyumov-Gerasimenko彗星内部的无线电波传输(CONSERT)测量,提出了彗星核探测实验。从信号的传播时间和形式来看,67P“头部”的上部在几十米的空间尺度上是相当均匀的。 CONSERT还将Philae最终着陆点的不确定性范围减小到约21乘34平方米。平均介电常数约为1.27,表明该区域的粉尘/冰体积比为0.4至2.6,孔隙率为75至85%。尘埃成分可以与碳质球粒陨石相当。

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  • 来源
    《Science》 |2015年第6247期|496-496|共1页
  • 作者单位

    Univ Grenoble Alpes, IPAG, F-38000 Grenoble, France;

    Univ Grenoble Alpes, IPAG, F-38000 Grenoble, France;

    CNRS, IPAG, F-38000 Grenoble, France|Aix Marseille Univ, Univ Toulon, INSU, CNRS,MIO,IRD,UM 110, F-83957 La Garde, France;

    Geodesy Observ Tahiti, Faaa 98702, Tahiti, Fr Polynesia;

    Univ Versailles St Quentin En Yvelines UVSQ, UPSay, F-78280 Guyancourt, France|CNRS INSU, F-78280 Guyancourt, France|Inst Pierre Simon Laplace, Lab Atmospheres Milieux Observat Spatiales LATMOS, F-78280 Guyancourt, France;

    Lunar & Planetary Inst, Houston, TX 77058 USA;

    Ruhr Univ Bochum, Fac Elect Engn & Informat Technol, D-44780 Bochum, Germany;

    CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA;

    Aix Marseille Univ, CNRS, Cent Marseille, Inst Fresnel UMR 7249, F-13013 Marseille, France;

    Univ Versailles St Quentin En Yvelines UVSQ, UPSay, F-78280 Guyancourt, France|CNRS INSU, F-78280 Guyancourt, France|Inst Pierre Simon Laplace, Lab Atmospheres Milieux Observat Spatiales LATMOS, F-78280 Guyancourt, France;

    CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA|Univ So Calif, Ming Hsieh Dept Elect Engn, Viterbi Sch Engn, Los Angeles, CA 90089 USA;

    Lab Astrophys Marseille Pole Etoile, F-13388 Marseille, France;

    Univ Toulouse, F-31028 Toulouse, France|UPS OMP, F-31028 Toulouse, France|IRAP, F-31028 Toulouse, France|2 CNRS, F-31028 Toulouse, France;

    Univ Paris 06, Univ Paris 04, F-75005 Paris, France|UVSQ, UPSay, F-75005 Paris, France|CNRS, INSU, F-75005 Paris, France|LATMOS IPSL, BC 102, F-75005 Paris, France;

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

    Univ Grenoble Alpes, IPAG, F-38000 Grenoble, France;

    German Aerosp Ctr DLR, D-12489 Berlin, Germany;

    Univ Grenoble Alpes, IPAG, F-38000 Grenoble, France;

    Tech Univ Dresden, D-01069 Dresden, Germany;

    Univ Grenoble Alpes, IPAG, F-38000 Grenoble, France;

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

    Tech Univ Dresden, D-01069 Dresden, Germany;

    ESA, European Space Res & Technol Ctr ESTEC Noordwijk, Noordwijk, Netherlands;

    Queen Mary Univ London, London E1 4NS, England;

    Univ Grenoble Alpes, IPAG, F-38000 Grenoble, France;

    CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA;

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  • 正文语种 eng
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