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Shape and Distribution of Rubble-pile Asteroid with Impact

机译:碎石堆小行星的形状和分布

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The asteroid exploration spacecraft "HAYABUSA" took high resolution pictures of asteroid "IT0KAWA". ITOKAWA is a rubble-pile asteroid, whose shape and regolith size distribution are unique. These features are caused by composition of the Brazil-Nut effect and centrifugal force by spin. The Brazil-Nut effect is generally known as the phenomenon that causes larger particles to rise to the top of the shaken granular mixtures. In this study, the behaviors of various size particles on the ground or in the space are analyzed by numerical simulation using Multi-Particle model, which is model of a rubble-pile asteroid.At first, the behaviors of particles on the ground are simulated, and it is confirmed that Brazil-Nut effect occurs. Next, the behaviors of particles in the space are simulated. From this simulation results, the internal distribution of particles' upward trend is obtained. It is compared with the known information of ITOKAWA, and the inferred internal structure of rubble-pile asteroid is discussed.
机译:小行星勘探航天器“Hayabusa”采用了小行星“IT0Kawa”的高分辨率图片。 Itokawa是一种瓦砾桩小行星,其形状和极象尺寸分布是独一无二的。这些特征是由旋旋的巴西 - 螺母效果和离心力引起的。巴西 - 螺母效果通常称为使较大颗粒升至摇粒颗粒混合物顶部的现象。在该研究中,通过使用多粒子模型的数值模拟分析了地面或空间中各种尺寸粒子的行为,这是一种瓦砾小行星的模型。 首先,模拟地面上的颗粒的行为,并确认发生巴西 - 螺母效果。接下来,模拟空间中的粒子的行为。从该模拟结果来看,获得颗粒的内部分布。将其与ITokawa的已知信息进行比较,并讨论了瓦砾小行星的推断内部结构。

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