Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-11T07:21:37.956Z Has data issue: false hasContentIssue false

Mappings for the First Order Asteroidal Resonance

Published online by Cambridge University Press:  07 August 2017

T. J. Stuchi
Affiliation:
Laboratório Nacional de ComputaçÃo - CNPq and Instituto de Matemática, Universidade Federal do Rio de Janeiro Rio de Janeiro, Brazil
W. Sessin
Affiliation:
Departamento de Mecânica do Vôo e Dinâmica Orbital-ITA/CTA, São José dos Campos, Brazil

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We construct a two step algebraic mapping from Sessin's simplified model for the first order resonance. The orbits obtained with this mapping are compared to the ones calculated with the exact solution. We also derive a reduced Hamiltonian. A plane Poincaré mapping, using delta periodic function, is constructed and compared to the reduced Hamiltonian contour curves showing the splitting of the separatrix due to delta perturbation technique.

Type
Part VII - Dynamical Systems. Maps. Integrators
Copyright
Copyright © Kluwer 1992 

References

Channel, P.J. and Scovel, J.C.:(1989), “Sympletic Integration of Hamiltonian Systems (pre-print).Google Scholar
Chirikov, B.V.:(1979), Phys. Rep. 52,263.Google Scholar
Guckenheimer, J. and Holmes, P.:(1983) “Non-linear Oscillations, Dynamical Systems and Bifurcations of Vector Fields” , Spring-Verlag, Dordrecht, Holland.Google Scholar
Sessin, W. and Ferraz-Mello, S.:(1984) Celes. Mech. 38,307.Google Scholar
Stuchi, T. J.:(1991) Doctor Thesis, Instituto Tecnológico de Aeronautica - CTA , São José dos Campos, Brazil.Google Scholar
Wisdom, J.:(1982) Astron. J. 87,577.CrossRefGoogle Scholar
Wisdom, J.:(1983) Icarus 56,51.Google Scholar