[P-PS03] Small Solar System Bodies: Latest results and new perspectives on the Solar System evolution

[PPS03-P20] Conditions for the long term stability of Pluto's azimuthal and latitudinal perihelion librations

*Takashi Ito^1,3, Renu Malhotra² (1.National Astronomical Observatory of Japan, National Institutes of Natural Science, 2.Department of Planetary Sciences, The University of Arizona, 3.Planetary Exploration Research Center, Chiba Institute of Technology)

Keywords:Pluto, resonance, solar system dynamics, transneptunian objects

Many of the unusual properties of the dwarf planet Pluto's orbit are widely accepted as evidence for the orbital migration of the giant planets in early solar system history. However, some properties remain an enigma. Pluto's long term orbital stability is supported by two special properties of its orbit that limit the location of its perihelion in azimuth and in latitude. We revisit Pluto's orbital dynamics with a view to elucidating the individual and collective gravitational effects of the giant planets on its perihelion location. In this presentation we demonstrate with numerical experiments that, while the resonant perturbations from Neptune account for the azimuthal constraint on Pluto's perihelion location, the long term and steady persistence of the latitudinal constraint is possible only in a narrow range of additional secular forcing which arises fortuitously from the particular orbital architecture of the other giant planets. Our numerical investigations also find that Jupiter has a largely stabilizing influence whereas Uranus has a largely destabilizing influence on Pluto's orbit.