Web of resonances and possible path of evolution of the small Uranian satellites
C. Charalambous, C.A. Giuppone, O.M. Guilera

TL;DR
This paper investigates the complex resonant structures of small Uranian satellites, analyzing their dynamical interactions and potential evolutionary paths through simulations of gas drag, migration, and tidal effects.
Contribution
It provides a detailed analysis of the resonant web among Uranus's small moons and explores scenarios for their current configuration using combined dynamical and evolutionary models.
Findings
Identified a web of low-order resonances among Uranus's small moons.
Demonstrated that gas drag and migration can lead to resonant capture.
Showed that tidal evolution can cause resonance crossings and orbital rearrangements.
Abstract
Satellite systems around giant planets are immersed in a region of complex resonant configurations. Understanding the role of satellite resonances contributes to comprehending the dynamical processes in planetary formation and posterior evolution. Our main goal is to analyse the resonant structure of small moons around Uranus and propose different scenarios able to describe the current configuration of these satellites. We focus our study on the external members of the regular satellites interior to Miranda, namely Rosalind, Cupid, Belinda, Perdita, Puck, and Mab, respectively. We use N-body integrations to perform dynamical maps to analyse their dynamics and proximity to two-body and three-body mean-motion resonances (MMR). We found a complicated web of low-order resonances amongst them. Employing analytical prescriptions, we analysed the evolution by gas drag and type-I migration in a…
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