Abstract
As has been shown in Sect. 1.14, the n-body problem (which consists in determining the motion of an isolated set of n bodies, having masses m 1, m 2, …, m n , and attracting one another with Newtonian gravitational forces) cannot be solved analytically in the general case, when n is greater than two.
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de Iaco Veris, A. (2018). Numerical Integration of the Equations of Motion. In: Practical Astrodynamics. Springer Aerospace Technology. Springer, Cham. https://doi.org/10.1007/978-3-319-62220-0_6
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