A fourth-order solution of the ideal resonance problem

Astronomy and Astrophysics – Astronomy

Scientific paper

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Equations Of Motion, Hamiltonian Functions, Numerical Integration, Pendulums, Resonance, Degrees Of Freedom, Elliptic Functions, Jacobi Matrix Method, Libration, Newton-Raphson Method

Scientific paper

The second-order solution of the ideal resonance problem, obtained by Henrard and Wauthier (1988), is extended to the fourth order. An explicit solution is derived for the Kepler equation in terms of elliptic integrals and functions. The fourth-order formal solution is compared with numerical solutions based on direct numerical integrations of equations of motion for two specific Hamiltonian systems.

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