Numerical modelling of major planets movement on the new interaction principle basis

Abstract

Numerical integration of the equations of movement of major planets, on the basis of a new principle of interaction is spent. Elements of orbits of major planets on large time interval (1602-2200) are calculated. Results of calculations are compared with elements of the orbits defined according to coordinates and speeds by numerical theory DE405. It is shown that elements of orbits of the exterior planets, found on new algorithm, will well be coordinated with dates DE405. For internal planets Venus, the Earth and Mars have insignificant discrepancies in secular offsets of perihelions in comparison with dates DE405.

Keywords

• orbital elements
• numerical integration
• motion differential equation
• barycentric coordinates