Perturbed Restricted Three-Body Problem

Author: Tianjiang Shuo

Website: https://cislunarspace.cn

Definition

The circular restricted three-body problem augmented with gravitational perturbations from additional bodies (e.g., adding the Sun to the Earth-Moon system). The solar perturbation magnitude (~2×10⁻²) can exceed the mass ratio μ, substantially degrading the practical stability of triangular libration points.

References

• 刘林和刘慧根 - 2008 - 地月系中探测器定点在三角平动点附近的位置漂移及其控制问题