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太阳系中行星轨道分布规律的理论分析

发表时间:2012-02-15  浏览量:1339  下载量:585
全部作者: 康建新,袁威
作者单位: 哈尔滨工业大学航天学院;东北农业大学工程学院
摘 要: 简要分析太阳系的时空分布形式,并采用静质量是随时空变化相同能量的假设。在此假设情况下,理论上能够给出在空间上的质量分布,即如果一个星系稳定,那么质量在空间上的分布必须满足一定规律,这就在理论上能够给出太阳系中行星轨道的大致分布。把理论数据和观测数据相比较,发现观测数据和理论计算的数据有一些偏差,但总体趋势相同。得出结论:太阳系还处在其演化的进程之中,不能和理想状态准确一致。
关 键 词: 理论物理;广义相对论;行星轨道;引力;太阳系
Title: Theoretical analysis on distribution of planetary orbits in solar system
Author: KANG Jianxin, YUAN Wei
Organization: School of Astronautic, Harbin Institute of Technology; School of Engineering, Northeast Agricultural University
Abstract: This paper firstly analyzes time-space distribution of solar system, and uses the assumption that rest mass is the same energy changing with time and space. Under this assumption, the mass distribution in space can be theoretically given. Namely, if a star system is stable, the mass distribution in space must meet certain rules, so the approximate orbits of the planets in the solar system can be given theoretically. The results show that the theoretical data have the same trends with the observational data, though they have some difference. The conclusion is drawn that the solar system is still in the process of evolution, and can not be strictly consistent with ideal state.
Key words: theoretical physics; general relativity; planetary orbits; gravity; solar system
发表期数: 2012年2月第3期
引用格式: 康建新,袁威. 太阳系中行星轨道分布规律的理论分析[J]. 中国科技论文在线精品论文,2012,5(3):212-218.
 
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