On the Stability of a Class of Permanent Rotations of a Heavy Asymmetric Gyrostat

被引:10
|
作者
Iarrea, Manuel [1 ]
Lanchares, Victor [1 ]
Pascual, Ana I. [1 ]
Elipe, Antonio [2 ]
机构
[1] Univ La Rioja, Fac Ciencias & Tecnol, Madre de Dios 53, Logrono 26006, Spain
[2] Ctr Univ Def Zaragoza, Carretera Huesca S-N, Zaragoza 50090, Spain
来源
REGULAR & CHAOTIC DYNAMICS | 2017年 / 22卷 / 07期
关键词
gyrostat rotation; stability; Energy - Casimir method; DUAL-SPIN SPACECRAFT; TIME-DEPENDENT MOMENTS; RIGID-BODY DYNAMICS; ORBITAL STABILITY; FIXED-POINT; TRIAXIAL GYROSTAT; ALGEBRAIC METHODS; PERIODIC MOTIONS; CHAOTIC DYNAMICS; ROTOR;
D O I
10.1134/S156035471707005X
中图分类号
O29 [应用数学];
学科分类号
070104 ;
摘要
We consider the motion of an asymmetric gyrostat under the attraction of a uniform Newtonian field. It is supposed that the center of mass lies along one of the principal axes of inertia, while a rotor spins around a different axis of inertia. For this problem, we obtain the possible permanent rotations, that is, the equilibria of the system. The Lyapunov stability of these permanent rotations is analyzed by means of the Energy-Casimir method and necessary and sufficient conditions are derived, proving that there exist permanent stable rotations when the gyrostat is oriented in any direction of the space. The geometry of the gyrostat and the value of the gyrostatic momentum are relevant in order to get stable permanent rotations. Moreover, it seems that the necessary conditions are also sufficient, but this fact can only be proved partially.
引用
收藏
页码:824 / 839
页数:16
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