Complements to the longitudinal librations of an elastic 3-layer Titan on a non-Keplerian orbit

被引：1

作者：

Richard, Andy ^{[1
,2
]}

Rambaux, Nicolas ^{[1
,2
]}

机构：

[1] UPMC, CNRS, IMCCE, Observ Paris,UMR 8028, 77 Ave Denfert Rochereau, F-75014 Paris, France

[2] UPMC Paris 06, Univ Pierre & Marie Curie, F-75005 Paris, France

来源：

COMPLEX PLANETARY SYSTEMS | 2014年 / 9卷 / 310期

关键词：

planets and satellites: individual (Titan); librations; rotation; elasticity; perturbations;

D O I：

10.1017/S174392131400773X

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Titan longitudinal librations are dependent on the satellite internal structure and the elastic behavior of the surface. The elastic deformation of the surface is related to the perturbing potential through the Love theory. In a previous paper, we described the deformation as a response to the tidal potential exerted by Saturn at orbital frequency. Here we improve the tidal deformation reponse by including the effect of the libration angle and the orbital perturbations. We then provide the libration amplitudes associated with the rotational model of a tidally deformed three-layer Titan evolving on a non-Keplerian orbit.

引用

页码：21 / 24

页数：4

共 9 条

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