Влияние взаимных гравитационных возмущений планет Солнечной системы на эволюцию эксцентриситетов и наклонений их орбит

In the paper the classic problem of N bodies is treated as if the mass of one body (the Sun) is much larger than the mass of the rest mutually gravitating bodies. We take as the unperturbed motion the movement of a planet in an elliptical orbit, with the Sun being in one of its foci. A set of equati... View More