dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorObservatoire de la Côte d’Azur
dc.contributorAristotle University of Thessaloniki
dc.date.accessioned2021-06-25T10:29:58Z
dc.date.accessioned2022-12-19T22:15:33Z
dc.date.available2021-06-25T10:29:58Z
dc.date.available2022-12-19T22:15:33Z
dc.date.created2021-06-25T10:29:58Z
dc.date.issued2021-05-01
dc.identifierCelestial Mechanics and Dynamical Astronomy, v. 133, n. 5, 2021.
dc.identifier1572-9478
dc.identifier0923-2958
dc.identifierhttp://hdl.handle.net/11449/206311
dc.identifier10.1007/s10569-021-10020-0
dc.identifier2-s2.0-85105481620
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5386908
dc.description.abstractWe describe the families of periodic orbits in the 2-dimensional 1/2 retrograde resonance at mass ratio 10 - 3, analyzing their stability and bifurcations into 3-dimensional periodic orbits. We explain the role played by periodic orbits in adiabatic resonance capture, in particular how the proximity between a stable family and an unstable family with a nearly critical segment, associated with Kozai separatrices, determines the transition between distinct resonant modes observed in numerical simulations. Combining the identification of stable, critical and unstable periodic orbits with analytical modeling, resonance capture simulations and computation of stability maps helps to unveil the complex 3-dimensional structure of resonances.
dc.languageeng
dc.relationCelestial Mechanics and Dynamical Astronomy
dc.sourceScopus
dc.subjectResonance
dc.subjectThree-body problem
dc.titleA study of the 1/2 retrograde resonance: periodic orbits and resonant capture
dc.typeArtículos de revistas


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