Orbital dynamics in the post-Newtonian planar circular restricted Sun–Jupiter system
Orbital dynamics in the post-Newtonian planar circular restricted Sun–Jupiter system
The theory of the post-Newtonian (PN) planar circular restricted three-body problem is used for numerically investigating the orbital dynamics of a test particle (e.g. a comet, asteroid, meteor or spacecraft) in the planar Sun–Jupiter system with a scattering region around Jupiter. For determining the orbital properties of the test particle, …