2019
DOI: 10.1016/j.actaastro.2019.09.021
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A method based on Jacobi Integral variational equation for computing Earth-Moon trajectories in the four-body problem

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Cited by 5 publications
(1 citation statement)
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“…To begin, the multi-body problem refers to the problem in the CRTBP that considers the gravity of other celestial bodies. 8 When the Sun is assumed to be the celestial body of interest, the problem can be further simplified to a restricted Earth–Moon–Sun bi-circular model. 911 Boudad et al, 12 in this model, calculated and analyzed the dynamics of synodic resonance NRHOs.…”
Section: Introductionmentioning
confidence: 99%
“…To begin, the multi-body problem refers to the problem in the CRTBP that considers the gravity of other celestial bodies. 8 When the Sun is assumed to be the celestial body of interest, the problem can be further simplified to a restricted Earth–Moon–Sun bi-circular model. 911 Boudad et al, 12 in this model, calculated and analyzed the dynamics of synodic resonance NRHOs.…”
Section: Introductionmentioning
confidence: 99%