Extreme Pebble Accretion in Ringed Protoplanetary Discs

TL;DR

This paper explores how a planetary embryo in a dust trap can rapidly grow into a giant planet through vortex-assisted pebble accretion, influenced by thermal feedback and vortex dynamics in protoplanetary discs.

Contribution

It introduces a novel model of vortex-assisted pebble accretion driven by thermal feedback, explaining rapid giant planet formation in ringed protoplanetary discs.

Findings

Rapid planet growth to ~100 Earth masses via vortex-assisted accretion.

Vortex formation and separation influence dust accumulation and accretion efficiency.

Implications for the origin of giant planets with high heavy element content.

Abstract

Axisymmetric dust rings containing tens to hundreds of Earth masses of solids have been observed in protoplanetary discs with (sub-)millimetre imaging. Here, we investigate the growth of a planetary embryo in a massive (150M$_\oplus$) axisymmetric dust trap through dust and gas hydrodynamics simulations. When accounting for the accretion luminosity of the planetary embryo from pebble accretion, the thermal feedback on the surrounding gas leads to the formation of an anticyclonic vortex. Since the vortex forms at the location of the planet, this has significant consequences for the planet's growth: as dust drifts towards the pressure maximum at the centre of the vortex, which is initially co-located with the planet, a rapid accretion rate is achieved, in a distinct phase of ``vortex-assisted'' pebble accretion. Once the vortex separates from the planet due to interactions with the disc, it accumulates dust, shutting off accretion onto the planet. We find that this rapid accretion, mediated by the vortex, results in a planet containing $\approx$ 100M$_\oplus$ of solids. We follow the evolution of the vortex, as well as the efficiency with which dust grains accumulate at its pressure maximum as a function of their size, and investigate the consequences this has for the growth of the planet as well as the morphology of the protoplanetary disc. We speculate that this extreme formation scenario may be the origin of giant planets which are identified to be significantly enhanced in heavy elements.