Earth-Moon Three-Body Problem with Solar Perturbation

Author: Tianjiang Shuo

Website: https://cislunarspace.cn

Definition

A planar dynamical model that extends the Earth-Moon CR3BP by adding the Sun's gravitational perturbation. Used to analyze solar perturbation effects on Earth-Moon libration point orbits such as DRO. The system no longer has a conserved Jacobi constant.

Application Value

Earth-Moon Three-Body Problem with Solar Perturbation plays a critical role in trajectory optimization and multi-body dynamics analysis for solving complex trajectory design problems.

References

  • Tan Minghu et al., 2014, Transfer to long term distant retrograde orbits around the Moon
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Contributors: ouyangjiahong, Ou Yang Jiahong