Abstract
In the framework of the model of M.A. Lavrentiev, the effect of internal elastic and dissipative forces on the rotational motion of the planet in a central gravitational field in a circular orbit is studied. The averaged equations of the rotational motion of the planet are derived. The stability of plane rotations is investigated. The analysis of the evolution of rotational motion depending on the values of the parameters and the initial conditions is carried out.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have