Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-23T11:02:46.962Z Has data issue: false hasContentIssue false
  • English
  • Français

Resonance p:p+q in Satellite Orbits

Published online by Cambridge University Press:  07 August 2017

Pedro R. Grosso  and
Wagner Sessin
Pedro R. Grosso
Affiliation:
Depto. de Mecânica do Vôo e Orbital Instituto Tecnológico de Aeronáutica 12225, São José dos Campos, SP, Brasil
Wagner Sessin
Affiliation:
Depto. de Mecânica do Vôo e Orbital Instituto Tecnológico de Aeronáutica 12225, São José dos Campos, SP, Brasil

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.

In this paper we consider the motion of a satellite whose mean motion is commensurable with the frequency of the rotational motion of the planet in the ratio p:p+q.

Type
Part IV - Planetary Satellites
Information
Symposium - International Astronomical Union , Volume 152: Chaos, Resonance and Collective Dynamical Phenomena in the Solar System , 1992 , pp. 233 - 234
Copyright
Copyright © Kluwer 1992 

References

Grosso, P.R.:1989, Movimento Orbital Perturbado de um Satélite Artificial em Ressonância 2:1 , M. Sc. Thesis, ITA, São José dos Campos.Google Scholar
Kaula, W.M.:1966, Theory of Satellite Geodesy , Blaisdell Publishing Company, Massachusetts.Google Scholar
Lemaître, A.:1984, Celest. Mech. 32, 109.CrossRefGoogle Scholar