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Rotational Dynamics of Janus and Epimetheus

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Abstract

We investigate simplified models of flat rotational motion of the coorbital satellites of Saturn, Janus and Epimetheus. We try to verify the hypothesis of chaotic rotation of the moons, caused by gravitational interaction between them. The possibility of parametric resonance in the librations of Janus is also investigated.

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References

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© 1997 Springer Science+Business Media Dordrecht

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Goździewski, K. (1997). Rotational Dynamics of Janus and Epimetheus. In: Wytrzyszczak, I.M., Lieske, J.H., Feldman, R.A. (eds) Dynamics and Astrometry of Natural and Artificial Celestial Bodies. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5534-2_36

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  • DOI: https://doi.org/10.1007/978-94-011-5534-2_36

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6330-2

  • Online ISBN: 978-94-011-5534-2

  • eBook Packages: Springer Book Archive

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