Breaking the centrifugal barrier to giant planet contraction by magnetic disc braking

TL;DR

This paper proposes that magnetic disc braking can effectively de-spin giant planets during contraction, overcoming the centrifugal barrier and explaining their observed rotation periods.

Contribution

It introduces a model where circumplanetary discs magnetic de-spin planets, providing a mechanism for contraction beyond the centrifugal barrier not previously considered.

Findings

Magnetic spin-down times are shorter than contraction timescales.

Planets can spin down to corotate with the magnetospheric radius.

Dispersal of the disc leaves planets with rotation periods 20-30 times their breakup period.

Abstract

During the runaway phase of their formation, gas giants fill their gravitational spheres of influence out to Bondi or Hill radii. When runaway ends, planets shrink several orders of magnitude in radius until they are comparable in size to present-day Jupiter; in 1D models, the contraction occurs on the Kelvin-Helmholtz time-scale $t_{\rm KH}$, which is initially a few thousand years. However, if angular momentum is conserved, contraction cannot complete, as planets are inevitably spun up to their breakup periods $P_{\rm break}$. We consider how a circumplanetary disc (CPD) can de-spin a primordially magnetized gas giant and remove the centrifugal barrier, provided the disc is hot enough to couple to the magnetic field, a condition that is easier to satisfy at later times. By inferring the planet's magnetic field from its convective cooling luminosity, we show that magnetic spin-down times are shorter than contraction times throughout post-runaway contraction: $t_{\rm mag}/t_{\rm KH}\sim(P_{\rm break}/t_{\rm KH})^{1/21}\lesssim 1$. Planets can spin down until they corotate with the CPD's magnetospheric truncation radius, at a period $P_{\rm max}/P_{\rm break} \sim (t_{\rm KH}/P_{\rm break})^{1/7}$. By the time the disc disperses, $P_{\rm max}/P_{\rm break}\sim 20-30$; further contraction at fixed angular momentum can spin planets back up to $\sim$$10 P_{\rm break}$, potentially explaining observed rotation periods of giant planets and brown dwarfs.