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Binary Asteroids: Secular Perturbations

Published online by Cambridge University Press:  07 August 2017

R. Vilhena De Moraes  and
S. M. G. Winter
R. Vilhena De Moraes
Affiliation:
Depto. de Mecânica do Vôo e Orbital Instituto Tecnológico de Aeronáutica Centro Técnico Aeroespacial 12225, São José dos Campos, SP, Brasil
S. M. G. Winter
Affiliation:
Depto. de Mecânica do Vôo e Orbital Instituto Tecnológico de Aeronáutica Centro Técnico Aeroespacial 12225, São José dos Campos, SP, Brasil

Abstract

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The motion of two small bodies orbiting each other whose barycenter is orbiting around a massive body is studied. The equations of motion are integrated considering the secular part of the disturbing function.

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. 183 - 184
Copyright
Copyright © Kluwer 1992 

References

Chauvineau, B. and Mignard, F. (1990) ‘Dynamics of Binary Asteroids’, Icarus , 83, 360–381.Google Scholar
Milani, A. and Nobili, A.M. (1988) ‘Instability of The 2+2 Body Problem’, Celest. Mech. , 41, 153–160.Google Scholar
Pojman, J.R. (1987) ‘Motion of Binary Asteroids’, M. Sc. Thesis, The University of Texas, Austin.Google Scholar
Whipple, A.L. and Szebehely, V. (1984) ‘The Restricted Problem of n + v Bodies’, Celest. Mech. , 32, 137–144.Google Scholar
Winter, S.M. (1990) ‘Perturbações Seculares no Problema Restrito de 2 + 2 Corpos’, M. Sc. Thesis, ITA, São José dos Campos.Google Scholar