Comments on the question of Mercury's perihelial motion

Computer Science – Numerical Analysis

Scientific paper

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Cartesian Coordinates, Kinetics, Mercury (Planet), Newton Theory, Perihelions, Polar Coordinates, Comparison, Elliptical Orbits, Mathematical Models, Numerical Analysis, Spherical Coordinates

Scientific paper

The numerical integration of the Newtonian movement equations which give values on the perihelial movement of the planet Mercury and remain unchanged at improved intervals in the integration intervals is shown. The calculations consider the relativistic velocity dependence in the mass and in the acceleration area and in the gravitation force. The calculations are compared with the independent programs in cartesian and polarity coordinates.

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