Cummins, DP, Owen, JE and Booth, RA orcid.org/0000-0002-0364-937X (2022) Extreme pebble accretion in ringed protoplanetary discs. Monthly Notices of the Royal Astronomical Society, 515 (1). pp. 1276-1295. ISSN 0035-8711
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 (150 M⊕) 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 on to the planet. We find that this rapid accretion, mediated by the vortex, results in a planet containing ≈100 M⊕ 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 that are identified to be significantly enhanced in heavy elements.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | © 2022 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. |
Keywords: | accretion, accretion discs – planets and satellites: formation – planet–disc interactions – protoplanetary discs |
Dates: |
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Institution: | The University of Leeds |
Academic Units: | The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds) > Astrophysics (Leeds) |
Depositing User: | Symplectic Publications |
Date Deposited: | 20 Jul 2023 11:41 |
Last Modified: | 20 Jul 2023 11:41 |
Published Version: | http://dx.doi.org/10.1093/mnras/stac1819 |
Status: | Published |
Publisher: | Oxford University Press |
Identification Number: | 10.1093/mnras/stac1819 |
Related URLs: | |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:201002 |
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