SECULAR PERTURBATIONS OF FICTITIOUS SATELLITES OF URANUS

被引：41

作者：

Kinoshita, Hiroshi ^{[1
]}

Nakai, Hiroshi ^{[1
]}

机构：

[1] Natl Astron Observ, Tokyo 181, Japan

来源：

CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY | 1991年 / 52卷 / 03期

关键词：

Uranian Satellites; Solar Perturbations; Satellite Extinction;

D O I：

10.1007/BF00048489

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Secular perturbations of fictitious satellites that are initially circular and in the equatorial plane of Uranus are discussed. Satellites located in the region where the solar perturbation is dominant become highly eccentric and inclined with respect to the equator, and have a possibility to collide with Uranus. Satellites located in the region where the oblateness perturbation is dominant keep the original eccentricity and the inclination. A scenario of a possible extinction of outer satellites of Uranus is also discussed.

引用

页码：293 / 303

页数：11