Joeris Kolja, Schönau Laurent, Keulen Matthias, Born Philip, Kollmer Jonathan E
Experimentelle Astrophysik, Universität Duisburg-Essen, Lotharstr. 1-21, 47057, Duisburg, Germany.
Institut für Materialphysik im Weltraum, Deutsches Zentrum für Luft- und Raumfahrt (DLR), 51170, Köln, Germany.
NPJ Microgravity. 2022 Aug 17;8(1):36. doi: 10.1038/s41526-022-00221-8.
The ballistic sorting effect has been proposed to be a driver behind the observed size sorting on the rubble pile asteroid Itokawa. This effect depends on the inelasticity of slow collisions with granular materials. The inelasticity of a collision with a granular material, in turn, depends on grain size. Here we argue that determining the inelasticity of such collisions in an asteroid-like environment is a nontrivial task. We show non-monotonic dependency of the coefficient of restitution (COR) on target particle size using experiments in microgravity. Employing numerical simulations, we explain these results with the growing influence of adhesion for smaller-sized particles. We conclude that there exists an optimum impactor to target particle size ratio for ballistic sorting.
弹道分选效应被认为是在 rubble pile 小行星糸川上观察到的尺寸分选背后的驱动因素。这种效应取决于与颗粒材料的缓慢碰撞的非弹性。反过来,与颗粒材料碰撞的非弹性又取决于颗粒大小。在这里,我们认为在类似小行星的环境中确定这种碰撞的非弹性是一项艰巨的任务。我们通过微重力实验展示了恢复系数(COR)对目标颗粒大小的非单调依赖性。利用数值模拟,我们用较小尺寸颗粒附着力增加的影响来解释这些结果。我们得出结论,对于弹道分选存在一个最佳的撞击体与目标颗粒大小比。