The classical restricted three-body problem is of fundamental importance because of its applications in astronomy and space navigation, and also as a simple model of a non-integrable Hamiltonian dynamical system. A central role is played by periodic orbits, of which many have been computed numerically. This is the second volume of an attempt to explain and organize the material through a systematic study of generating families, the limits of families of periodic orbits when the mass ratio of the two main bodies becomes vanishingly small. We use quantitative analysis in the vicinity of bifurcations of types 1 and 2. In most cases the junctions between branches can now be determined. A first-order approximation of families of periodic orbits in the vicinity of a bifurcation is also obtained. This book is intended for scientists and students interested in the restricted problem, in its applications to astronomy and space research, and in the theory of dynamical systems.

This is an in-depth study of an important model of a non-integrable Hamiltonian dynamical system It will certainly trigger a host of interesting future research Includes supplementary material: sn.pub/extras

Inhalt
Definitions and General Equations.- Quantitative Study of Type 1.- Partial Bifurcation of Type 1.- Total Bifurcation of Type 1.- The Newton Approach.- Proving General Results.- Quantitative Study of Type 2.- The Case 1/3 v < 1/2.- Partial Transition 2.1.- Total Transition 2.1.- Partial Transition 2.2.- Total Transition 2.2.- Bifurcations 2T1 and 2P1.