双星系统周围的动力学(65803

R. Machado Oliveira, O. Winter, R. Sfair, G. Valvano, T. Moura, G. Borderes-Motta
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引用次数: 0

摘要

Didymos和Dimorphos分别是主要和次要的小行星,它们组成了一个双星系统,构成了近地小行星(NEAs)的集合。它们是双小行星重定向测试(DART)的目标,这是第一个致力于研究行星防御的测试任务,其主要目标是测量次级天体被kinect撞击器撞击后引起的变化。本文拟通过数值积分的方法,对分布在两个物体附近的无质量粒子的动力学进行研究。初级天体的近似形状被认为是质量浓度(mascons)的模型,次级天体被认为是一个质量点。我们的结果显示了稳定区域的位置和大小,以及它们的寿命。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Dynamics around the binary system (65803) Didymos
Abstract Didymos and Dimorphos are primary and secondary, respectively, asteroids who compose a binary system that make up the set of Near Earth Asteroids (NEAs). They are targets of the Double Asteroid Redirection Test (DART), the first test mission dedicated to study of planetary defense, for which the main goal is to measure the changes caused after the secondary body is hit by a kinect impactor. The present work intends to conduct a study, through numerical integrations, on the dynamics of massless particles distributed in the vicinity of the two bodies. An approximate shape for the primary body was considered as a model of mass concentrations (mascons) and the secondary was considered as a massive point. Our results show the location and size of stable regions, and also their lifetime.
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