%0 Journal Article
%T 太阳系行星、规则卫星距离规律的物理意义<br>Physical Significance of the Distance Law of Planets and Reg-ular Satellites
%A 李金宝
%J Astronomy and Astrophysics
%P 20-31
%@ 2329-1265
%D 2013
%I Hans Publishing
%R 10.12677/AAS.2013.12004
%X <div style=\"text-align:justify;\">
	<span style=\"line-height:1.5;\">太阳系形成演化过程中星云成盘状分布，在星云盘中星云绕太阳做开普勒运动。如果一个绕转体行星胎离中心天体的距离为</span><span style=\"line-height:1.5;\">R</span><span style=\"line-height:1.5;\">，它的公转周期为</span><span style=\"line-height:1.5;\">T</span><span style=\"line-height:1.5;\">，依据开普勒第三定律推导可证明位于</span><span style=\"line-height:1.5;\">1.5874</span><span style=\"line-height:1.5;\">R</span><span style=\"line-height:1.5;\">处的星云绕中心天体的公转周期恰好等于</span><span style=\"line-height:1.5;\">2</span><span style=\"line-height:1.5;\">T</span><span style=\"line-height:1.5;\">，因此：</span><span style=\"line-height:1.5;\">1</span><span style=\"line-height:1.5;\">) </span><span style=\"line-height:1.5;\">R</span><span style=\"line-height:1.5;\">处的行星胎与</span><span style=\"line-height:1.5;\">1.5874</span><span style=\"line-height:1.5;\">R</span><span style=\"line-height:1.5;\">处的星云发生</span><span style=\"line-height:1.5;\">“</span><span style=\"line-height:1.5;\">冲</span><span style=\"line-height:1.5;\">”</span><span style=\"line-height:1.5;\">、</span><span style=\"line-height:1.5;\">“</span><span style=\"line-height:1.5;\">上合</span><span style=\"line-height:1.5;\">”</span><span style=\"line-height:1.5;\">的位置将相对保持恒定；</span><span style=\"line-height:1.5;\">2</span><span style=\"line-height:1.5;\">) </span><span style=\"line-height:1.5;\">两者之间的夹角</span><span style=\"line-height:1.5;\">180</span><span style=\"line-height:1.5;\">度时，轨道为</span><span style=\"line-height:1.5;\">R</span><span style=\"line-height:1.5;\">处的行星胎对轨道为</span><span style=\"line-height:1.5;\">1.5874</span><span style=\"line-height:1.5;\">R</span><span style=\"line-height:1.5;\">处星云摄动力总是在同一向径出现；</span><span style=\"line-height:1.5;\">3</span><span style=\"line-height:1.5;\">) </span><span style=\"line-height:1.5;\">在相等的演化时间里，</span><span style=\"line-height:1.5;\">R</span><span style=\"line-height:1.5;\">处的行星胎与</span><span style=\"line-height:1.5;\">1.5874</span><span style=\"line-height:1.5;\">R</span><span style=\"line-height:1.5;\">处的星云在同一向径发生</span><span style=\"line-height:1.5;\">“</span><span style=\"line-height:1.5;\">冲</span><span style=\"line-height:1.5;\">”</span><span style=\"line-height:1.5;\">、</span><span style=\"line-height:1.5;\">“</span><span style=\"line-height:1.5;\">上合</span><span style=\"line-height:1.5;\">”</span><span style=\"line-height:1.5;\">的次数最多。在这三种因素的综合累积作用下，使星云盘在</span><span style=\"line-height:1.5;\">1.5874</span><span style=\"line-height:1.5;\">R</span><span style=\"line-height:1.5;\">处出现空隙并向轨道</span><span style=\"line-height:1.5;\">R</span><span
%K 行星；规则卫星；距离规律；开普勒第三定律；星云盘<br>Planet
%K Regular Satellite
%K Distance Law
%K Kepler’s Third Law
%K Nebula Disk
%U http://www.hanspub.org/journal/PaperInformation.aspx?PaperID=9810