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    Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/33037

    Title: Growth and form of planetary seedlings: Results from a microgravity aggregation experiment
    Authors: Blum,J;Wurm,G;Kempf,S;Poppe,T;Klahr,H;Kozasa,T;Rott,M;Henning,T;Dorschner,J;Schrapler,R;Keller,HU;Markiewicz,WJ;Mann,I;Gustafson,BAS;Giovane,F;Neuhaus,D;Fechtig,H;Grun,E;Feuerbacher,B;Kochan,H;Ratke,L;El Goresy,A
    Contributors: 太空科學研究所
    Date: 2000
    Issue Date: 2010-07-07 10:26:30 (UTC+8)
    Publisher: 中央大學
    Abstract: The outcome of the first stage of planetary formation, which is characterized by ballistic agglomeration of preplanetary dust grains due to Brownian motion in the free molecular flow regime of the solar nebula, is still somewhat speculative. We performed
    Appears in Collections:[太空科學研究所 ] 期刊論文

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