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Corotations in Some Higher-Order Resonances

Published online by Cambridge University Press:  07 August 2017

S. Ferraz-Mello ,
M. Tsuchida  and
J.C. Klafke
S. Ferraz-Mello
Affiliation:
Universidade de São Paulo, Instituto Astronômico e Geofísico BR-01051-São Paulo, SP, Brasil
M. Tsuchida
Affiliation:
Universidade de São Paulo, Instituto Astronômico e Geofísico BR-01051-São Paulo, SP, Brasil
J.C. Klafke
Affiliation:
Universidade de São Paulo, Instituto Astronômico e Geofísico BR-01051-São Paulo, SP, Brasil

Abstract

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Some results concerning the resonances 3:1, 4:1 and 5: 2 are given and compared to results published by other authors.

Type
Part III - The Asteroidal Belt
Information
Symposium - International Astronomical Union , Volume 152: Chaos, Resonance and Collective Dynamical Phenomena in the Solar System , 1992 , pp. 167 - 170
Copyright
Copyright © Kluwer 1992 

References

Ferraz-Mello, S.: 1989, “A semi-numerical expansion of the averaged disturbing function for some very-high-eccentricity orbits”, Celest. Mech. 45, 65–68.Google Scholar
Ferraz-Mello, S., Tsuchida, M. and Klafke, J.C.: 1992, “On symmetrical planetary corotations” Celest. Mech. & Dyn. Astron. (to appear).Google Scholar
Hadjidemetriou, J.D.: 1992, “The elliptic restricted problem at the 3/1 commensurability” Celest. Mech. & Dyn. Astron. (to appear).CrossRefGoogle Scholar
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Yoshikawa, M.: 1989, “A survey of the motions of asteroids in the commensurability with Jupiter” Astron. Astrophys. 213, 436–458.Google Scholar
Yoshikawa, M.: 1990, Motions of asteroids at the Kirkwood gaps. I. On the 3:1 resonance with Jupiter” Icarus 87, 78–102.CrossRefGoogle Scholar