96-153 Celletti A., Chierchia L.
On the stability of realistic three-body problems (459K, Postscript) Apr 26, 96
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Abstract. We derive a three-body problem for the Sun-Jupiter-Ceres system and, after substituting the mass ratio of Jupiter/Sun (which is approximately $10^{-3}$) with a parameter $\epsilon$, we prove the existence of stable quasi--periodic motions with frequencies close to the observed (average) frequencies reported in The Astronomical Almanac" for $|\epsilon|\le 10^{-6}$. The proof is computer--assisted".

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