Derivation of Capture Probabilities for the Corotation Eccentric Mean Motion Resonances
arXiv:1609.01256 · doi:10.1093/mnras/stx996
Abstract
We study in this paper the capture of a massless particle into an isolated, first order Corotation Eccentric Resonance (CER), in the framework of the Planar, Eccentric and Restricted Three-Body problem near a m+1:m mean motion commensurability (m integer). While capture into Lindblad Eccentric Resonances (where the perturber's orbit is circular) has been investigated years ago, capture into CER (where the perturber's orbit is elliptic) has not yet been investigated in detail. Here, we derive the generic equations of motion near a CER in the general case where both the perturber and the test particle migrate. We derive the probability of capture in that context, and we examine more closely two particular cases: (i) if only the perturber is migrating, capture is possible only if the migration is outward from the primary. Notably, the probability of capture is independent of the way the perturber migrates outward; (ii) if only the test particle is migrating, then capture is possible only if the algebraic value of its migration rate is a decreasing function of orbital radius. In this case, the probability of capture is proportional to the radial gradient of migration. These results differ from the capture into Lindblad Eccentric Resonance (LER), where it is necessary that the orbits of the perturber and the test particle converge for capture to be possible. Possible applications for planetary satellites are discussed.
arXiv commentSubmitted to MNRAS
References in corpus (10)
- Architecture of Kepler's Multi-transiting Systems: II. New investigations with twice as many candidates
- Overstable Librations can account for the Paucity of Mean Motion Resonances among Exoplanet Pairs
- Formation of Regular Satellites from Ancient Massive Rings in the Solar System
- Accretion of Saturn's mid-sized moons during the viscous spreading of young massive rings: solving the paradox of silicate-poor rings versus silicate-rich moons
- Migration of two massive planets into (and out of) first order mean motion resonances
- On the origin of the Trojan asteroids: Effects of Jupiter's mass accretion and radial migration
- Detection of Stars within 0.8 arcseconds of Kepler Objects of Interest
- Aegaeon (Saturn LIII), a G-ring object
- Coupling between corotation and Lindblad resonances in the elliptic planar three-body problem
- Origin of the chaotic motion of the Saturnian satellite Atlas
Cited by in corpus (6)
- Speeding past planets? Asteroids radiatively propelled by giant branch Yarkovsky effects
- Long-term Dynamical Evolution of Pallene (Saturn XXXIII) and its Diffuse, Dusty Ring
- Dynamics of multiple bodies in a corotation resonance: Conserved quantities and relevance to ring arcs
- Orbital Dynamics of Atlas (S XV): Its Current Orbit and the Recent Past
- Dust production through collisions between small bodies: an application to the G-ring arc
- Revisiting the dynamics of the Prometheus-Pandora system