Full Ephemeris Restricted 4-Body Problem
Author: Tianjiang Shuo
Website: https://cislunarspace.cn
Definition
A high-fidelity dynamics model that considers the Sun as a fourth body and uses precise ephemerides to compute the real motion of Earth and Moon, providing more accurate orbit predictions than CR3BP.
Application Value
This provides a fundamental theoretical framework for cislunar dynamics modeling and analysis, serving as a mathematical tool for studying spacecraft motion.
Related Concepts
- Monte Carlo Trajectory Shooting, MCTS
- Powered Lunar Flyby, PLF
- Planar Circular Restricted Three-Body Problem, PCRTBP
- Insertion Delta-V
References
- Colagrossi 等 - 2021.
