On the Satellite Capture Problem : Capture and stability regions for planetary satellites

dc.creatorBrunini, Adrián
dc.date1996
dc.date2022-04-05T19:03:32Z
dc.date.accessioned2023-07-15T04:41:02Z
dc.date.available2023-07-15T04:41:02Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/133969
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7470488
dc.descriptionThe stability and capture regions in phase space for retrograde and direct planetary satellites are investigated in the frame of the Circular Restricted Three-Body Problem. We show that a second integral of motion furnishes an accurate description for the stability limit of retrograde satellites. The distribution of heliocentric orbital elements is studied, and possible candidates to be temporary Jovian satellites are investigated. Previous results, limited to orbits satisfying the Mirror Theorem, are extended in order to give a complete set of capture conditions in phase-space.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.format79-92
dc.languagees
dc.rightshttp://creativecommons.org/licenses/by/4.0/
dc.rightsCreative Commons Attribution 4.0 International (CC BY 4.0)
dc.subjectCiencias Exactas
dc.subjectBioquímica
dc.subjectRestricted Three-Body Problem
dc.subjectPlanetary Satellites
dc.titleOn the Satellite Capture Problem : Capture and stability regions for planetary satellites
dc.typeArticulo
dc.typeArticulo


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