日本地球惑星科学連合2015年大会

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セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS21] 惑星科学

2015年5月25日(月) 18:15 〜 19:30 コンベンションホール (2F)

コンビーナ:*黒澤 耕介(千葉工業大学 惑星探査研究センター)、濱野 景子(東京大学大学院理学系研究科地球惑星科学専攻)

18:15 〜 19:30

[PPS21-P01] 衝突破壊における破片形状分布が示す破壊過程

*門野 敏彦1谷川 享行1水谷 仁2 (1.産業医科大学、2.ニュートンプレス)

キーワード:衝突, 破壊, 破片, 形状, 破壊過程

The results of the previous impact experiments show that the shape of the fragments, characterized by the triaxial dimensions a, b, and c, (a ? b ? c), behaves in a very regular way (e.g., Fujiwara et al. 1989). In widely different experimental conditions, the axial ratios, b/a and c/a, have distributions peaked at about each mean value, ~ 0.7 and ~ 0.5, respectively, and flattened (i.e., small c/a) fragments are almost absence.
We find that, if the distribution of the shape parameters, (b/a, c/a), is homogeneous, and there is no fragment at c?? < k, where k is a constant (0 < k < 1; in Fujiwara et al. (1978) k was ~ 0.2), the averages of the shape parameters, (0.7, 0.5) can be realized. Then, we discuss the fracture processes to represent the homogeneous distribution in the shape parameters. The expected dominant fracture process in impact fragmentation is reported.
Fujiwara, A., et al., Nature 272, 602-603, 1978.
Fujiwara, A., et al., in Asteroids II, pp. 240-265, 1989.