rations verg a span of ± 5 x 1010 yr the total epsed ti for all tegrations is ore than 5 yr， g several dedicated pcs and workstations one of the fundantal ncsions of our long-ter tegrations is that sor syste pary otion sees to be stableters of the hill stability ntioned above， at least over a ti-span of ± 4 gyr actually，our nurical tegrations the syste was far ore stable than what is defed by the hill stability criterion: not only did no close enunter happen durg the tegration period， but also all the pary orbital elents have been nfeda narrow region bothti and frequency doa， though pary otions are stochastic sce the purpose of this paper is to exhibit and overview the results of our long-ter nurical tegrations， we show typical exaple figures as evidence of the very long-ter stabil
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