Tilting Ice Giants with a Spin-Orbit Resonance
Zeeve Rogoszinski, Douglas P. Hamilton

TL;DR
This paper explores how a secular spin-orbit resonance, facilitated by a massive circumplanetary disk, could explain Uranus's large obliquity and differences from Neptune, highlighting a new mechanism for planetary tilts.
Contribution
It demonstrates that a massive circumplanetary disk can induce spin-orbit resonance, providing a novel explanation for Uranus's tilt without requiring multiple giant impacts.
Findings
Resonance can tilt Uranus up to 70° with a massive disk.
A single giant impact can increase Uranus's tilt to nearly 98°.
Neptune's tilt can be explained with a less massive disk, avoiding impacts.
Abstract
Giant collisions can account for Uranus's and Neptune's large obliquities, yet generating two planets with widely different tilts and strikingly similar spin rates is a low-probability event. Trapping into a secular spin-orbit resonance, a coupling between spin and orbit precession frequencies, is a promising alternative, as it can tilt the planet without altering its spin period. We show with numerical integrations that if Uranus harbored a massive circumplanetary disk at least three times the mass of its satellite system while it was accreting its gaseous atmosphere, then its spin precession rate would increase enough to resonate with its own orbit, potentially driving the planet's obliquity to 70. We find that the presence of a massive disk moves the Laplace radius significantly outward from its classical value, resulting in more of the disk contributing to the planet's…
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