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


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Abstract

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.

About the authors

N. I. Amel’kin

Moscow Institute of Physics and Technology

Author for correspondence.
Email: namelkin@mail.ru
Russian Federation, Dolgoprudny, 141701

V. V. Kholoshchak

Moscow Institute of Physics and Technology

Author for correspondence.
Email: khoviktoriya@yandex.ru
Russian Federation, Dolgoprudny, 141701

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