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An extended Ideal Resonance Problem

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Abstract

An Extended Resonance Problem is defined by the Hamiltonian,

$$F = B(y) + 2\mu ^2 A(y)[\sin x + \lambda (y)]^2 \mu<< 1,\lambda = O(\mu ).$$

It is noted here that the phase-plane trajectories exhibit adouble libration, enclosing two centers, for the initial conditions of motion satisfying the inequality

$$1 - |\lambda |< |\alpha |< 1 + |\lambda |,$$

where α is the usualresonance parameter.

A first order solution for the case of double libration is constructed here by a generalization of the procedure previously used in solving the Ideal Resonance Problem with λ=0. The solution furnishes a reference orbit for a Perturbed Ideal Problem if a double libration occurs as a result of perturbations.

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References

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Garfinkel, B. An extended Ideal Resonance Problem. Celestial Mechanics 12, 203–214 (1975). https://doi.org/10.1007/BF01230212

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  • DOI: https://doi.org/10.1007/BF01230212

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