Abu Bakr Mehmood, S. Umer Abbas, Ghulam Shabbir
Published 2004-02-08Version 1
An approach is developed to find approximate solutions to the restricted circular three body problem. The solution is useful in approximately describing the position vectors of three spherically symmetric masses, one of which has a much smaller mass than the other two. These masses perform free motion under each others gravitational influence. The set of solutions is found using the lamberts wave function.
Comments: 18 pages, 4 figures
A Generalized approach for computing the trajectories associated with the Newtonian N Body Problem
Closed Form Approximations For The Three Body Problem
Saari's Conjecture for the Collinear $n$-Body Problem
