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Spin-orbit coupling and chaotic rotation for eccentric coorbital bodies

Published online by Cambridge University Press:  05 January 2015

Adrien Leleu ,
Philippe Robutel  and
Alexandre C. M. Correia
Adrien Leleu
Affiliation:
IMCCE, Observatoire de Paris, CNRS, UPMC Univ. Paris 06, Univ. Lille 1, 77Av.Denfert-Rochereau, 75014 Paris, France email: [email protected], [email protected]
Philippe Robutel
Affiliation:
IMCCE, Observatoire de Paris, CNRS, UPMC Univ. Paris 06, Univ. Lille 1, 77Av.Denfert-Rochereau, 75014 Paris, France email: [email protected], [email protected]
Alexandre C. M. Correia
Affiliation:
IMCCE, Observatoire de Paris, CNRS, UPMC Univ. Paris 06, Univ. Lille 1, 77Av.Denfert-Rochereau, 75014 Paris, France email: [email protected], [email protected] Departamento de Física, I3N, Universidade de Aveiro, Campus de Santiago, 3810-193 Aveiro, Portugal email: [email protected]
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Abstract

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The presence of a co-orbital companion induces the splitting of the well known Keplerian spin-orbit resonances. It leads to chaotic rotation when those resonances overlap.

Keywords

celestial mechanicscoorbitalsrotationspin-orbit resonance
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Issue S310: Complex Planetary Systems , July 2014 , pp. 190 - 191
Copyright
Copyright © International Astronomical Union 2014 

References

Correia, A. C. M. & Robutel, P. 2013, AJ, 779, 20CrossRefGoogle Scholar
Wisdom, J., Peale, S. J., & Mignard, F. 1984, Icarus, 58, 137Google Scholar