Modeling the 3 – D Secular Planetary Three-Body Problem . Discussion on the outer υ Andromedae Planetary System

@inproceedings{Michtchenko2005ModelingT3,
  title={Modeling the 3 – D Secular Planetary Three-Body Problem . Discussion on the outer υ Andromedae Planetary System},
  author={T. A. Michtchenko and Sylvio Ferraz-Mello},
  year={2005}
}
The three-dimensional secular behavior of a system composed of a central star and two massive planets is modeled semi-analytically in the frame of the general three-body problem. The main dynamical features of the system are presented in geometrical pictures allowing us to investigate a large domain of the phase space of this problem without time-expensive numerical integrations of the equations of motion and without any restriction on the magnitude of the planetary eccentricities, inclinations… CONTINUE READING
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