Coefficients of the expansion of the planetary disturbing function

Published: 10 July 2019| Version 1 | DOI: 10.17632/3cb75grjz4.1
Contributor:
Denis Mikryukov

Description

Here we store the coefficients of the planetary disturbing function in computer-readable form. These were obtained by Maxima computer algebra system. The method is described by Laskar and Robutel (CMDA, 62, 193-217, 1995). We should note that our coefficients of secular Hamiltonian up to degree 4 coincide with those presented by Laskar and Robutel (see Section 7, CMDA, 62, 193-217, 1995). Therefore we hope that our expansions are error free. We plan to provide more thorough and complete comments on all of these data in the near future.

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Categories

Celestial Mechanics, Power Series

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