Birkhoff Equations
Author: Tianjiang Shuo
Website: https://cislunarspace.cn
Definition
A reformulation of the circular restricted three-body problem that replaces six state variables with five new ones (x, y, z, γ, νz), eliminating velocity magnitude via the Jacobi integral. In the 3D Birkhoff equations, γ is the velocity azimuth angle and νz is the velocity component perpendicular to the x-y plane. This equation set has a concise form convenient for numerical integration and manifold computation.
Application Value
Based on its definition, a reformulation of the circular restricted three-body problem that replaces six state variables with five new ones (x, y, z, γ, νz), eliminating velocity magnitude via the jacobi integral. in the 3d b.
Related Concepts
- 三体问题(Three-Body Problem)
- 最优控制(Optimal Control)
- 轨迹优化(Trajectory Optimization)
References
- Lunar capture trajectories and homoclinic connections through isomorphic mapping (Giancotti et al., 2012)
- Pontani和Teofilatto - 2016 - Polyhedral representation of invariant manifolds applied to orbit transfers in the Earth–moon system
