{"title":"最接近法则","authors":"M. N. Tarabishy","doi":"arxiv-2409.09097","DOIUrl":null,"url":null,"abstract":"In this work, we introduce the Law of Closest Approach which is derived from\nthe properties of conic orbits and can be considered an addendum to the laws of\nKepler. It states that on the closest approach, the distance between the\nobjects is minimal and the velocity vector is perpendicular to the position\nvector with maximum speed. The ratio of twice the kinetic energy to the\nnegative potential energy is equal to the eccentricity plus one. The advantage\nof this law is that both speed and position are at extremum making the\ncalculation of the eccentricity more robust.","PeriodicalId":501565,"journal":{"name":"arXiv - PHYS - Physics Education","volume":"23 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"The Law of Closest Approach\",\"authors\":\"M. N. Tarabishy\",\"doi\":\"arxiv-2409.09097\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"In this work, we introduce the Law of Closest Approach which is derived from\\nthe properties of conic orbits and can be considered an addendum to the laws of\\nKepler. It states that on the closest approach, the distance between the\\nobjects is minimal and the velocity vector is perpendicular to the position\\nvector with maximum speed. The ratio of twice the kinetic energy to the\\nnegative potential energy is equal to the eccentricity plus one. The advantage\\nof this law is that both speed and position are at extremum making the\\ncalculation of the eccentricity more robust.\",\"PeriodicalId\":501565,\"journal\":{\"name\":\"arXiv - PHYS - Physics Education\",\"volume\":\"23 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-13\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Physics Education\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.09097\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Physics Education","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.09097","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
摘要
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。
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.