ANGULAR-MOMENTUM AND TIDAL EVOLUTION OF SATURN SYSTEM

被引：2
|
作者：
BURSA, M
机构：
[1] Astronomical Institute, Czechoslovak Academy of Sciences, Prague
来源：
EARTH MOON AND PLANETS | 1991年 / 54卷 / 03期
关键词：
D O I：
10.1007/BF00056322
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
It has been demonstrated that dynamically the Saturnian system is analogous to the Jovian system; however, it is not an analogue of the Solar system as a whole. The departures in the figure parameters of the tri-axial Saturnian satellites orbiting in 1:1 resonance, from equilibrium figure parameters are not large in general, and the tidal and centrifugal distorting forces can be supposed to be responsible for the actual figures. The estimates for different dynamical parameters of the system support the hypothesis that the tri-axial satellites in 1:1 resonance were formed from the same protoplanetary nebula that gave rise to Saturn.
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页码：241 / 255
页数：15
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