The Construction of the Theory of Motion for Solar-System Bodies Based on a Universal Method for the Perturbative Function Calculation

Details The Construction of the Theory of Motion for Solar-System Bodies Based on a Universal Method for the Perturbative Function Calculation The Construction of the Theory of Motion for Solar-System Bodies Based on a Universal Method for the Perturbative Function Calculation

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000sosyr..34..509g&link_type=abstract

Solar System Research, v. 34, Issue 6, p. 509-516 (2000).

Physics

Scientific paper

A new universal method for series expansion of the perturbative function
is developed. A unified theory of motion for Solar-System bodies is
constructed on its basis. In the first part of the work, the right-hand
sides of equations are limited by the first-order terms.

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