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Kozai-Lidov oscillations of Jupiter-mass planets, excited by comparable planetary or brown dwarf mass perturbers were recently shown in numerical experiments to be slowly modulated and to exhibit striking features, including extremely high eccentricities and the generation of retrograde orbits with respect to the perturber.
Milankovich, M. 1939, Bull. Serb. Acad. Math. Nat. A, 6, 1
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Lidov, M. L. 1962, Planetary and Space Science, 9, 719
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Kozai, Y. 1962, Astron. J., 67, 591
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Allan, R. R., & Ward, G. N. 1963, Proceedings of the Cambridge Philosophical Society, 59, 669
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Heisler, J., & Tremaine, S. 1986, Icarus, 65, 13
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Thompson, T. A. 2010, arXiv:1011.4322
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Naoz, S., Farr, W. M., Lithwick, Y., Rasio, F. A., & Teyssandier, J. 2011, Nature (London), 473, 187
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Katz, B., & Dong, S. 2011, arXiv:1105.3953
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Lithwick Y., & Naoz S. 2011
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