Abstract
Using Laskar’s Frequency Map Analysis, we have performed a complete study of the dynamics of massless particles in the Solar System, from Mercury to the outer parts of the Kuiper belt, for all values of the eccentricities. This provides a complete dynamical map of the Solar System which is, in this first step, restricted to mean motion resonances. The same method is also applied to the planetary 3-body system composed of the Sun, Jupiter and Saturn.
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© 2001 Springer Science+Business Media Dordrecht
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Robutel, P., Laskar, J. (2001). Global Dynamics in the Solar System. In: Pretka-Ziomek, H., Wnuk, E., Seidelmann, P.K., Richardson, D.L. (eds) Dynamics of Natural and Artificial Celestial Bodies. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-1327-6_33
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DOI: https://doi.org/10.1007/978-94-017-1327-6_33
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-5865-2
Online ISBN: 978-94-017-1327-6
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