Evolution of Rotational Motion of a Planet in a Circular Orbit Under the Influence of Internal Elastic and Dissipative Forces

2020 ◽  
Vol 55 (2) ◽  
pp. 234-247
Author(s):  
N. I. Amel’kin
2019 ◽  
Vol 54 (2) ◽  
pp. 190-203 ◽  
Author(s):  
N. I. Amel’kin ◽  
V. V. Kholoshchak

2015 ◽  
Author(s):  
Levon K. Babadzanjanz ◽  
Irina Yu. Pototskaya ◽  
Yulia Yu. Pupysheva

1993 ◽  
Vol 132 ◽  
pp. 23-38
Author(s):  
Andrzej J. Maciejewski

AbstractIt was proved that the problem of perturbed planar oscillations of a rigid-body in a circular orbit is nonitegrable. Two types of perturbations were considered: solar radiations pressure and the third body torques. In the second part of the paper example of chaotic rotations of a symmetric rigid body in a circular orbit was given. It was shown numerically that the phase space is divided into two separate regions of chaotic and ordered motions.


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