dc.creatorRodríguez, Adrián
dc.creatorMichtchenko, Tatiana A.
dc.creatorMiloni, Octavio
dc.date2011-08
dc.date2022-02-07T14:35:09Z
dc.date.accessioned2023-07-15T04:15:44Z
dc.date.available2023-07-15T04:15:44Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/130593
dc.identifierissn:0923-2958
dc.identifierissn:1572-9478
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7468874
dc.descriptionWe investigate the secular dynamics of two-planet coplanar systems evolving under mutual gravitational interactions and dissipative forces. We consider two mechanisms responsible for the planetary migration: star-planet (or planet-satellite) tidal interactions and interactions of a planet with a gaseous disc. We show that each migration mechanism is characterized by a specific law of orbital angular momentum exchange. Calculating stationary solutions of the conservative secular problem and taking into account the orbital angular momentum leakage, we trace the evolutionary routes followed by the planet pairs during the migration process. This procedure allows us to recover the dynamical history of two-planet systems and constrain parameters of the involved physical processes.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.format161-178
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectAstronomía
dc.subjectSecular evolution
dc.subjectMigration
dc.subjectDissipation laws
dc.subjectTidal force
dc.subjectDrag force
dc.titleAngular momentum exchange during secular migration of two-planet systems
dc.typeArticulo
dc.typeArticulo


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