The Law of Closest Approach

M. N. Tarabishy
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Abstract

In this work, we introduce the Law of Closest Approach which is derived from the properties of conic orbits and can be considered an addendum to the laws of Kepler. It states that on the closest approach, the distance between the objects is minimal and the velocity vector is perpendicular to the position vector with maximum speed. The ratio of twice the kinetic energy to the negative potential energy is equal to the eccentricity plus one. The advantage of this law is that both speed and position are at extremum making the calculation of the eccentricity more robust.
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最接近法则
在这项工作中,我们引入了 "最接近定律"(Law of Closest Approach),该定律源于圆锥轨道的特性,可视为开普勒定律的增补。该定律指出,在最接近时,天体之间的距离最小,速度矢量垂直于位置矢量,速度最大。两倍动能与负势能之比等于偏心率加一。该定律的优点是速度和位置都处于极值,从而使偏心率的计算更加稳健。
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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