Perturbing the Lagrange Solution to the General Three Body Problem

E. Piña () and L. Jiménez-Lara ()
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E. Piña: Universidad Autónoma Metropolitana-Iztapalapa, Departamento de Física
L. Jiménez-Lara: Universidad Autónoma Metropolitana-Iztapalapa, Departamento de Física

A chapter in New Advances in Celestial Mechanics and Hamiltonian Systems, 2004, pp 123-136 from Springer

Abstract: Abstract The Lagrange case of the three body problem interacting through gravitational forces was perturbed from the circular Lagrange motion around the center of mass, to the motion in a near orbit. The perturbation motion was supposed to occur in the same plane of the unperturbed Lagrange solution. The computations were performed using new sets of coordinates introduced recently for the general three body problem.

Keywords: Body Problem; Celestial Mechanics; Canonical Momentum; Periodic Coefficient; Dimensionless Masse (search for similar items in EconPapers)
Date: 2004
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Persistent link: https://EconPapers.repec.org/RePEc:spr:sprchp:978-1-4419-9058-7_8

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DOI: 10.1007/978-1-4419-9058-7_8

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