Evolution of the Rotational Movement of a Dynamically Symmetric Satellite with Inner Damping in a Circular Orbit

Resumo

In this paper, we studied the effect of internal dissipation on the rotational motion of a satellite in a central gravitational field using the Lavrent'ev model. Evolution equations are derived, and the results of an evolution analysis of the rotational motion of a dynamically symmetric satellite moving in a Keplerian circular orbit depending on the parameter values and initial conditions are presented.