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On the secular motion of the jovian planets
Published online by Cambridge University Press: 25 May 2016
Abstract
The motion of the Jovian planets is investigated using Hamiltonian perturbation theory and numerical integrations. Experiments varying the mass of Neptune exhibit 1:1 secular resonance between the perihelion motions of Jupiter and Uranus.
- Type
- Part II - Planets and Moon: Theory and Ephemerides
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- Copyright © Kluwer 1996
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