Improved Numerical Model of Motion of Artificial Satellites of the Moon and its Application in Research Features of the Dynamics of Circumlunar Objects
摘要
Abstract
The paper describes the improvements made by the authors to the previously published Numerical Model of the Motion of Artificial Lunar Satellites (ALS). The results of a study of the dynamics of cislunar objects obtained by numerical modeling are presented. It is shown that the short lifespan of low-flying objects in orbits, revealed by a number of authors, is explained solely by the influence of the complex gravitational field of the Moon, primarily the radial component of the force acting on the satellites. The features of the influence of light pressure (LP) on cislunar objects are considered. It is shown that LP expands the range of action of apsidal-nodal resonances that arise in the movement of cislunar objects.