Shooting stars on schedule: synchronising re-entry of particles launched from a satellite

Philip Rodriguez Blanco
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Abstract

The ALE-3 mission plans to create artificial “shooting stars” in the upper atmosphere by launching pellets sequentially from a satellite in low Earth orbit. How does one arrange for all pellets to re-enter over the intended location simultaneously? Starting with conservation of energy and angular momentum, I derive a version of Kepler’s equation that gives time as a function of radial distance in an orbit, which can be used to find the transfer time from the pellet’s ejection to its re-entry as a function of its launch velocity. I show that for a given pellet ejection speed, there is a launch angle from the satellite that results in the fastest transfer time. I use these results to determine the pellets’ launch times and velocities for simultaneous arrival at a desired re-entry point. These results can be applied to de-orbiting any set of objects launched from a satellite, and use concepts that can be covered in an advanced undergraduate course in physics or aerospace engineering. Supplementary materials are provided online.
流星如期而至:卫星发射的粒子同步重返大气层
ALE-3 任务计划通过从低地球轨道卫星上依次发射弹丸,在高层大气中制造人造 "流星"。如何安排所有弹丸同时重返预定位置?从能量守恒和角动量守恒出发,我推导出了开普勒方程的一个版本,该方程给出了时间与轨道径向距离的函数关系,可用于求出小球从弹射到重返大气层的转移时间与其发射速度的函数关系。我的研究表明,对于给定的弹丸弹射速度,有一个从卫星发射出去的发射角能带来最快的转移时间。我利用这些结果来确定弹丸的发射时间和速度,以便同时到达所需的重返点。这些结果可应用于从卫星发射的任何一组物体的脱轨,并使用物理学或航空航天工程学高级本科课程所涵盖的概念。网上提供了补充材料。
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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