Numerical estimates for stability domains of Lagrangian solutions to the restricted three-body problem

Trajectory and stability of Lagrangian point L 2 in the Sun-Earth system

“…Although there are two new equilibrium points due to mass of the belt (larger than 0.15) as obtained by Jiang and Yeh (2006); Yeh and Jiang (2006), but they are left to be examined. All the results are computed numerically using same technique as in Grebennikov and Kozak-Skoworodkin (2007), because pure analytical methods are not suitable. For specific time intervals, and initial values, these results provide new information on the behavior of trajectories around the Lagrangian point L 2 .…”