New High-Precision Values of the Geodetic Rotation of the Mars Satellites System, Major Planets, Pluto, the Moon and the Sun

IF 0.7 Q4 ASTRONOMY & ASTROPHYSICS Artificial Satellites-Journal of Planetary Geodesy Pub Date : 2019-06-01 DOI:10.2478/ARSA-2019-0004
V. Pashkevich, A. Vershkov
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引用次数: 7

Abstract

Abstract In this study the relativistic effects (the geodetic precession and the geodetic nutation, which consist of the effect of the geodetic rotation) in the rotation of Mars satellites system for the first time were computed and the improved geodetic rotation of the Solar system bodies were investigated. The most essential terms of the geodetic rotation were computed by the algorithm of Pashkevich (2016), which is applicable to the study of any bodies of the Solar system that have long-time ephemeris. As a result, in the perturbing terms of the physical librations and Euler angles for Mars satellites (Phobos and Deimos) as well as in the perturbing terms of the physical librations for the Moon and Euler angles for major planets, Pluto and the Sun the most significant systematic and periodic terms of the geodetic rotation were calculated. In this research the additional periodic terms of the geodetic rotation for major planets, Pluto and the Moon were calculated.
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火星卫星系统、主要行星、冥王星、月球和太阳大地自转的新高精度值
摘要本研究首次计算了火星卫星系统自转中的相对论效应(由大地自转效应组成的大地进动和大地章动),并研究了改进的太阳系天体大地自转。大地自转的最基本项是由Pashkevich(2016)的算法计算的,该算法适用于研究太阳系中任何具有长期星历的天体。因此,在火星卫星(火卫一和火卫一)的物理平动和欧拉角的扰动项中,以及在月球的物理平动的扰动项和主要行星、冥王星和太阳的欧拉角中,计算了大地自转最重要的系统和周期项。在这项研究中,计算了主要行星冥王星和月球的大地自转的附加周期项。
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