Santos, D. E.Martins, R. V.Winter, O. C.Cordeiro, R. R.2014-05-202014-05-201998-03-01Astronomy & Astrophysics. Les Ulis Cedex A: Edp Sciences S A, v. 331, n. 3, p. 1108-1112, 1998.0004-6361http://hdl.handle.net/11449/35621Trajectories of the planar, circular, restricted three-body problem are given in the configuration space through the caustics associated to the invariant tori of quasi-periodic orbits. It is shown that the caustics of trajectories librating in any particular resonance display some features associated to that resonance. This method can be considered complementary to the Poincare surface of section method, because it provides information not accessible by the other method.1108-1112engcelestial mechanics, stellar dynamicschaosArtigoWOS:000072713100046Acesso restrito0960024575647258