Escape dynamics and fractal basins boundaries in the three-dimensional Earth-Moon system
arXiv:1604.03403 · doi:10.1007/s10509-016-2683-6
Abstract
The orbital dynamics of a spacecraft, or a comet, or an asteroid in the Earth-Moon system in a scattering region around the Moon using the three dimensional version of the circular restricted three-body problem is numerically investigated. The test particle can move in bounded orbits around the Moon or escape through the openings around the Lagrange points and or even collide with the surface of the Moon. We explore in detail the first four of the five possible Hill's regions configurations depending on the value of the Jacobi constant which is of course related with the total orbital energy. We conduct a thorough numerical analysis on the phase space mixing by classifying initial conditions of orbits in several two-dimensional types of planes and distinguishing between four types of motion: (i) ordered bounded, (ii) trapped chaotic, (iii) escaping and (iv) collisional. In particular, we locate the different basins and we relate them with the corresponding spatial distributions of the escape and collision times. Our outcomes reveal the high complexity of this planetary system. Furthermore, the numerical analysis suggests a strong dependence of the properties of the considered basins with both the total orbital energy and the initial value of the coordinate, with a remarkable presence of fractal basin boundaries along all the regimes. Our results are compared with earlier ones regarding the planar version of the Earth-Moon system.
Published in Astrophysics and Space Science (A&SS) journal. arXiv admin note: previous papers with related context: arXiv:1512.08683, arXiv:1508.05201
References in corpus (5)
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- Beyond-Newtonian dynamics of a planar circular restricted three-body problem with Kerr-like primaries
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- On the classification of orbits in the three-dimensional Copenhagen problem with oblate primaries
- Computational Method for Phase Space Transport with Applications to Lobe Dynamics and Rate of Escape
- Orbit classification in the Hill problem: I. The classical case
- Investigating the planar circular restricted three-body problem with strong gravitational field
- Escape dynamics through a continuously growing leak