Convergence of the expansions of the disturbing functions in the planar three-body planetary problem

Details Convergence of the expansions of the disturbing functions in the planar three-body planetary problem Convergence of the expansions of the disturbing functions in the planar three-body planetary problem

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sosyr..41..162s&link_type=abstract

Solar System Research, Volume 41, Issue 2, pp.162-170

Physics

95.10.Ce

Scientific paper

In the framework of the planar three-body planetary problem, conditions are found for the absolute convergence of the expansions of the disturbing functions in powers of the eccentricities, with coefficients represented by trigonometric polynomials with respect to the mean, eccentric, or true anomaly of the inner planet. It is found that using the eccentric or true anomaly as the independent variable instead of the mean anomaly (or time) extends the holomorphy domain of the principal part of the perturbation functions. The expansions of the second parts converge in open bicircles, which admit values of the eccentricity of the inner planet in excess of the Laplace limit.

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