Abstract
This paper considers the dynamics of two planets, as the planets B and C of the pulsar PSR B1257+12, near a 3/2 mean-motion resonance. A two-degrees-of-freedom model, in the framework of the general three-body planar problem, is used and the solutions are analyzed through surfaces of section and Fourier techniques in the full phase space of the system.
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On the possibility of existence of a fourth planet in distant orbit, see Wolszczan et al., 2000
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Callegari, N., Ferraz-Mello, S. & Michtchenko, T.A. Dynamics of Two Planets in the 3/2 Mean-motion Resonance: Application to the Planetary System of the Pulsar PSR B1257+12. Celestial Mech Dyn Astr 94, 381–397 (2006). https://doi.org/10.1007/s10569-006-9002-4
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DOI: https://doi.org/10.1007/s10569-006-9002-4