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dc.date.accessioned 2022-02-07T14:35:09Z
dc.date.available 2022-02-07T14:35:09Z
dc.date.issued 2011-08
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/130593
dc.description.abstract We 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. en
dc.format.extent 161-178 es
dc.language en es
dc.subject Secular evolution es
dc.subject Migration es
dc.subject Dissipation laws es
dc.subject Tidal force es
dc.subject Drag force es
dc.title Angular momentum exchange during secular migration of two-planet systems en
dc.type Articulo es
sedici.identifier.other arXiv:1106.0014 es
sedici.identifier.other doi:10.1007/s10569-011-9359-x es
sedici.identifier.issn 0923-2958 es
sedici.identifier.issn 1572-9478 es
sedici.creator.person Rodríguez, Adrián es
sedici.creator.person Michtchenko, Tatiana A. es
sedici.creator.person Miloni, Octavio es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Celestial Mechanics and Dynamical Astronomy es
sedici.relation.journalVolumeAndIssue vol. 111, no. 1 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)