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天体自转因素导致的相对论性效应 被引量:1

RELATIVISTIC EFFECTS RESULTING FROM THE ROTATION OF CELESTIAL BODIES
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摘要 本文在PPN框架中得到了太用系内自转因素产生的瞬时轨道根数改正的一阶封闭分析解.轨道半长径和偏心率不受长期效应的影响,只受周期效应的影响;轨道倾角、升交点经度、近星点角距,平近点角既受长期效应又受周期效应的影响.我们用两种引力理论分别计算了太阳自转对地内大行星及—些小行星轨道,行星自转对自然卫星轨道,地球自转对人造卫星轨道所产生的各相对论性效应. In the PPN formalism, the first—order closed analytical solutionsof rotating celestial bodies on the improvement of instaneous orbital elements are obtained in the solar system. The semimajor axis and eccentricity are not affected by the secular relativistic effects.but are affected by the periodic relativistio effects. The inclination,longitude of ascending node, longitude of periastron and mean longitudeof epoch are affceted by both the secular and periodic relativistic effects. In two gravitational theories, the obtained results are appliedto calcualte the relativistic effects of the solar rotation on the motions of planets and minor planets , of the planetary rotation on the motions of natural satellites and of the Earth rotation on the motions of artificial satellites.
作者 韩韬
出处 《紫金山天文台台刊》 北大核心 1991年第4期276-287,共12页
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  • 1Joachim Heimberger,Michael Soffel,Hanns Ruder. Relativistic effects in the motion of artificial satellites: The oblateness of the central body II[J] 1989,Celestial Mechanics and Dynamical Astronomy(2):205~217
  • 2M. Soffel,H. Ruder,M. Schneider. The two-body problem in the (truncated) PPN — Theory[J] 1987,Celestial Mechanics(1):77~85

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