Dynamics of two planets in the 3/2 mean-motion resonance: Application to the planetary system of the pulsar PSR B1257+12

Artigo

Fecha

2006-04-01

Registro en:

Celestial Mechanics & Dynamical Astronomy. Dordrecht: Springer, v. 94, n. 4, p. 381-397, 2006.

0923-2958

http://hdl.handle.net/11449/24846

10.1007/s10569-006-9002-4

WOS:000238517200002

http://repositorioslatinoamericanos.uchile.cl/handle/2250/3898023

Autor

Universidade Estadual Paulista (Unesp)

Universidade de São Paulo (USP)

Institución

Universidade Paulista Júlio de Mesquita Filho (Brasil)

Resumen

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.

Materias

chaos

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