Back-tracing space debris using proper elements

A. Celletti, G. Pucacco, T. Vartolomei
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Abstract

Abstract Normal form methods allow one to compute quasi-invariants of a Hamiltonian system, which are referred to as proper elements. The computation of the proper elements turns out to be useful to associate dynamical properties that lead to identify families of space debris, as it was done in the past for families of asteroids. In particular, through proper elements we are able to group fragments generated by the same break-up event and we possibly associate them to a parent body. A qualitative analysis of the results is given by the computation of the Pearson correlation coefficient and the probability of the Kolmogorov-Smirnov statistical test.
使用适当的元素对空间碎片进行反向追踪
范式方法允许计算哈密顿系统的拟不变量,它被称为固有元素。计算适当的元素对于识别空间碎片家族的动力学特性是有用的,就像过去对小行星家族所做的那样。特别是,通过适当的元素,我们能够将由同一分裂事件产生的碎片分组,并可能将它们与父主体联系起来。通过计算Pearson相关系数和Kolmogorov-Smirnov统计检验的概率,对结果进行了定性分析。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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