The Modified Restricted Three Body Problems

Details The Modified Restricted Three Body Problems The Modified Restricted Three Body Problems

2006-10-31

arxiv.org/abs/astro-ph/0610927v1

Astronomy and Astrophysics

Astrophysics

published in RevMexAA(SC), 21, 152 (4 pages, 6 figures)

Scientific paper

The restricted three body problem is well-known and very important for dynamics of binary, multiple stars and also planetary systems. We extend the classical version of this problem to the situation that there are some external forces from the belt. We find that both the equilibrium points and solution curves become quite different from the classical case. We also determine the values of Lyapunov Exponent for some important orbits.

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