THE MAIN SECULAR RESONANCES nu(6), nu(5) AND nu(16) IN THE ASTEROID BELT

被引：54

作者：

Morbidelli, Alessandro ^{[1
]}

Henrard, Jacques ^{[1
]}

机构：

[1] Fac Univ Notre Dame Paix, Dept Math, B-5000 Namur, Belgium

来源：

CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY | 1991年 / 51卷 / 02期

关键词：

asteroid belt-secular resonance-action angle variables-surface of section-numerical simulation;

D O I：

10.1007/BF00048607

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this paper an analytical model, suitable for a global description of the dynamics in a secular resonance of order 1, is derived from the general perturbation study developed in a previous paper (Morbidelli and Henrard (1991)). Such a model is then used to study the secular resonances nu(6), nu(5) and nu(16), and pictures illustrating the secular motion are obtained. The peculiarities of the nu(5) resonances are discussed in detail. The results are compared with those obtained by the theories of Yoshikawa and Nakai-Kinoshita. Some numerical simulations performed by Ch. Froeschle and H. Scholl are discussed in the light of the new theoretical results. New numerical experiments on the nu(6) resonance are also presented.

引用

页码：169 / 197

页数：29

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