Mathematics
Scientific paper
Oct 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978cemec..18..259g&link_type=abstract
Celestial Mechanics, vol. 18, Oct. 1978, p. 259-275.
Mathematics
15
Asteroids, Celestial Mechanics, Perturbation Theory, Three Body Problem, Trojan Orbits, Asymptotic Methods, Hamiltonian Functions, Lagrangian Equilibrium Points, Oscillations, Periodic Variations, Planetary Mass, Resonance, Trojan Asteroids, Asteroids, Period, Motion, Perturbations, Resonance, Mathematical Models, Orbits
Scientific paper
The paper considers the formal long-periodic solution for the case of 1:1 resonance in the restricted problem of three bodies, which was discussed in Part I (1977), and extends the accuracy of the solution from O(m) to O(m to the 3/2 power), where m is the mass parameter for the system. Asymptotic approximations for the period of the motion are obtained for the case of small oscillations about the Lagrangian point L4, in agreement with the classical theory, and for the vicinity of a logarithmic singularity on the mean separatrix, passing through L3. The regularizing function, which removes the singularities of the Poincare type, is extended to all orders, and the result is used to prove the periodicity of the solution.
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