Abstract
The study of the structure and dynamical evolution of planetary rings is considered nowadays as an essential part of the research in the evolution of the solar system.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
M. Henon and J.M. Petit, ’Series expansions for encouter-type solutions of Hill’s problem’ Cel. Mechanics 38, 67:100 (1986).
J.M. Petit and M. Hénon, "Satellite encounters" Icarus 66, 536:555 (1986).
J.M. Petit and M. Hénon, "A numerical simulation of planetary rings - 1. Binary encounters", Astron. Astrophys. 173, 389:404 (1987).
W. H. Press, B. P. Flannery, S. A. Teukolsky and W. T. Vetterling, "Numerical Recipes - The art of scientific computing" Cambridge University Press (1986).
G. Saporta, "Probabilités, Analyse des données et Statistique", Éditions Technip, Paris (1990).
B. Grais, "Méthodes Statistiques" Dunod, Paris (1977).
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1991 Plenum Press, New York
About this chapter
Cite this chapter
Gama, F.P., Petit, JM. (1991). Statistical Analysis of the Effects of Close Encounters of Particles in Planetary Rings. In: Roy, A.E. (eds) Predictability, Stability, and Chaos in N-Body Dynamical Systems. NATO ASI Series, vol 272. Springer, Boston, MA. https://doi.org/10.1007/978-1-4684-5997-5_29
Download citation
DOI: https://doi.org/10.1007/978-1-4684-5997-5_29
Publisher Name: Springer, Boston, MA
Print ISBN: 978-1-4684-5999-9
Online ISBN: 978-1-4684-5997-5
eBook Packages: Springer Book Archive