Coefficients of the expansion of the planetary disturbing function

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


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.



Celestial Mechanics, Power Series