The Perihelion Shift of Mercury's Orbit

被引:1
|
作者
Amelkin, N. I. [1 ]
机构
[1] Moscow Inst Phys & Technol, Inst Skii Per 9, Dolgoprudnyi 141700, Moscow Region, Russia
关键词
solar system; limited circular three-body problem; perihelion shift of Mercury;
D O I
10.3103/S0025654419080016
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
Influence of planets of the solar system on the precession of the orbit of Mercury is studied in the framework of classical mechanics. It is shown that the average perihelion shift of the orbit of Mercury, calculated in the framework of the planar limited problem, is 556.5 arc seconds per century and coincides with the observed one with a relative accuracy of 2.5%. The incomplete coincidence between the calculated average displacement and the observational data is explained by the presence in the observed displacement of vibrational components with a total amplitude of up to 80 arc seconds and periods from several years to tens of years.
引用
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页码:1131 / 1137
页数:7
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