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Some Aspects of Particle's Dynamics

Published online by Cambridge University Press:  07 August 2017

R.S. Gomes
R.S. Gomes*
Affiliation:
Observatório Nacional Rio de Janeiro Brazil

Abstract

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Some features of the dynamics of particles affected by drag, in the field of the Sun and planets, are presented here. In particular mean motion and secular resonances are investigated. When dust particles are considered as a whole in the zodiacal cloud, a simple secular theory can explain much of its geometry. Dynamics of particles near an inner planet is mostly dispersive, but an average behavior can be deduced from some analytical and numerical considerations.

Keywords

dust particlesdragresonance
Type
Part VI - Meteors. Zodiacal Cloud. Nebulae
Information
Symposium - International Astronomical Union , Volume 152: Chaos, Resonance and Collective Dynamical Phenomena in the Solar System , 1992 , pp. 349 - 354
Copyright
Copyright © Kluwer 1992 

References

Dermott, S.F.;Nicholson, P.D.;Burns, J.A.;Houck, J.R. 1984 Nature 312, 505–509 CrossRefGoogle Scholar
Jackson, A.A.; Zook, H.A. 1989 Nature 337, 629 Google Scholar
Wyatt, S.P.; Whipple, F.L. 1950 Astrophys. J. 111, 134–141 Google Scholar