Computer Science – Numerical Analysis
Scientific paper
Mar 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982stin...8324446b&link_type=abstract
Unknown
Computer Science
Numerical Analysis
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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