Abstract
We discuss the existence, location, and stability of the collinear equilibrium points of a generalized Hill problem with radiation of the primary (the Sun) and oblateness of the secondary (the planet), and present some remarkable fractals created as basins of attraction of Newton’s method applied for their computation in several cases of the parameters.
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Douskos, C.N. Collinear equilibrium points of Hill’s problem with radiation and oblateness and their fractal basins of attraction. Astrophys Space Sci 326, 263–271 (2010). https://doi.org/10.1007/s10509-009-0213-5
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DOI: https://doi.org/10.1007/s10509-009-0213-5