Origin of Hyperion and Saturn's Rings in A Two-Stage Saturnian System Instability
Matija \'Cuk, Maryame El Moutamid, Jim Fuller, Val\'ery Lainey

TL;DR
This paper proposes a two-stage instability event involving Titan's orbital expansion, leading to the formation of Hyperion, the destabilization of inner moons, and the creation of Saturn's rings, supported by numerical simulations.
Contribution
It introduces a novel scenario linking Titan's orbital evolution to the formation of Hyperion and Saturn's rings through a two-stage instability process.
Findings
Numerical simulations support the probability of the proposed chain of events.
The model explains Hyperion's origin and the rings' formation in a unified framework.
Resonant interactions played a key role in the system's evolution.
Abstract
The age of the rings and some of the moons of Saturn is an open question, and multiple lines of evidence point to a recent (few hundred Myr ago) cataclysm involving disruption of past moons. The main driver of the evolution of the Saturnian system is the relatively rapid tidal expansion of its largest moon, Titan, which is likely driven by resonant tides within Saturn. The obliquity of Saturn and the orbit of the small moon Hyperion both serve as a record of the past orbital evolution of Titan. Saturn's obliquity was likely generated by a secular spin-orbit resonance with the planets, while Hyperion is caught in a mean-motion resonance with Titan, with both phenomena driven by Titan's orbital expansion. We propose that the breaking of Saturn's spin resonance was also the event in which Hyperion formed, when an outer mid-sized satellite (``Proto-Hyperion'') was destabilized and collided…
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Taxonomy
TopicsAstro and Planetary Science · High-pressure geophysics and materials · Paleontology and Stratigraphy of Fossils
