Restricted Four-Body Problem
Author: Tianjiang Shuo
Website: https://cislunarspace.cn
Definition
A dynamical model describing the motion of a spacecraft of negligible mass under the gravitational influence of Earth, Moon, and Sun. Compared with the restricted three-body problem, it adds solar gravitational terms for more accurate modeling of solar perturbation during Earth-Moon transfers. The equations of motion are formulated in the Earth-Moon rotating coordinate system with normalized units.
Application Value
This concept is essential for understanding motion characteristics in orbital design and control, and plays a vital role in mission success.
Related Concepts
- Minimum Norm Solution
- Rigid Body Dynamics
- Variable-Size Design Space, VSDS
- Analytical Gradient
References
- 彭祺擘和张海联 - 2016 - 载人登月地月转移轨道方案综述
