Disruption of co-orbital (1:1) planetary resonances during gas-driven orbital migration
نویسندگان
چکیده
منابع مشابه
Orbital Resonances in Planetary Systems
There are two main types of resonance phenomena in planetary systems involving orbital motions: (i) mean motion resonance: This is intuitively the most obvious type of resonance; it occurs when the orbital periods of two planets are close to a ratio of small integers; (ii) secular resonance: this is a commensurability of the frequencies of precession of the orientation of orbits, as described b...
متن کاملSecondary resonances of co-orbital motions
The size distribution of the stability region around the Lagrangian point L4 is investigated in the elliptic restricted three-body problem as the function of the mass parameter and the orbital eccentricity of the primaries. It is shown that there are minimum zones in the size distribution of the stability regions, and these zones are connected with secondary resonances between the frequencies o...
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We compute the length and time scales associated with resonant orbits around Kerr black holes for all orbital and spin parameters. Resonance-induced effects are potentially observable when the Event Horizon Telescope resolves the inner structure of Sgr A*, when space-based gravitational wave detectors record phase shifts in the waveform during the resonant passage of a compact object spiraling ...
متن کامل0 The Capture of Particles by Chaotic Resonances During Orbital Migration
Because a chaotic zone can reduce the long timescale capture probabilities and cause catastrophic events such as close encounters with a planet or star during temporary capture, the dynamics of migrating planets is likely to be strongly dependent on the widths of the chaotic zones in their resonances. Previous theoretical work on the resonant capture of particles into mean-motion resonances by ...
متن کاملDiversity and Origin of 2:1 Orbital Resonances in Extrasolar Planetary Systems
A diversity of 2:1 resonance configurations can be expected in extrasolar planetary systems, and their geometry can provide information about the origin of the resonances. Assembly during planet formation by the differential migration of planets due to planetdisk interaction is one scenario for the origin of mean-motion resonances in extrasolar planetary systems. The stable 2:1 resonance config...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2014
ISSN: 1365-2966,0035-8711
DOI: 10.1093/mnras/stu1008