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  1. No Access

    Article

    Dynamics of Enceladus and Dione inside the 2:1 mean-motion resonance under tidal dissipation

    In a previous work (Callegari and Yokoyama, Celest. Mech. Dyn. Astr. 98:5–30, 2007), the main features of the motion of the pair Enceladus–Dione were analyzed in the frozen regime, i.e., without considering th...

    N. Callegari Jr, T. Yokoyama in Celestial Mechanics and Dynamical Astronomy (2008)

  2. No Access

    Article

    Dynamics of two satellites in the 2/1 Mean–Motion resonance: application to the case of Enceladus and Dione

    The dynamics of a pair of satellites similar to Enceladus–Dione is investigated with a two-degrees-of-freedom model written in the domain of the planar general three-body problem. Using surfaces of section and...

    N. Callegari Jr., T. Yokoyama in Celestial Mechanics and Dynamical Astronomy (2007)

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    Article

    Dynamics of Two Planets in the 3/2 Mean-motion Resonance: Application to the Planetary System of the Pulsar PSR B1257+12

    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...

    N. Callegari Jr, S. Ferraz-Mello… in Celestial Mechanics and Dynamical Astronomy (2006)

  4. No Access

    Article

    Dynamics of Two Planets in the 2/1 Mean-Motion Resonance

    The dynamics of two planets near a first-order mean-motion resonance is modeled in the domain of the general three-body planar problem. The system studied is the pair Uranus-Neptune (2/1 resonance). The phase ...

    N. Callegari Jr., T. A. Michtchenko… in Celestial Mechanics and Dynamical Astronomy (2004)