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Kepler-223 resonance holds information about turbulence during the gas-disk phase

Hühn, L.-A. and Pichierri, G. and Bitsch, B. and Batygin, K. (2021) Kepler-223 resonance holds information about turbulence during the gas-disk phase. Astronomy and Astrophysics, 656 . Art. No. A115. ISSN 0004-6361. doi:10.1051/0004-6361/202142176. https://resolver.caltech.edu/CaltechAUTHORS:20211130-215746491

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Abstract

Context. Planet formation remains an open field of research, and many fundamental physical processes regarding planetary formation in protoplanetary disks are still imperfectly understood. It remains to be investigated how different conditions in these protoplanetary disks affect the emergence of different types of observed systems. An elusive phenomenon is the turbulence in these disks. Observations are available of planetary systems and of some protoplanetary disks, which can serve as a starting point for these investigations. The detected systems reveal different architectures of planets. One particularly interesting case to consider is the Kepler-223 system, which contains a rare configuration of four planets in a resonance chain. This implies a certain migration history. Aims. We aim to use the orbital configuration of the Kepler-223 planets to constrain the parameters of the protoplanetary disk that allow the formation of a chain of mean-motion resonances that resembles the resonances of Kepler-223. We primarily investigate the disk viscosity and surface density. Methods. We used the swift_symba N-body integrator with additional dissipative forces to mimic planet-disk interactions. Results. We constrained the surface densities and viscosities that allow the formation of a resonant chain like that of Kepler-223. We find that surface densities of up to a few minimum mass solar nebula surface densities and disk viscosity parameters α of a few × 10⁻³ up to × 10⁻² are most successful at reproducing the architecture of this particular planetary system. We describe the connection of these two quantities with each other, considering the success of reproducing the chain. We find that higher disk surface densities in turn require lower viscosities to build the chain. Conclusions. Our results show that well-characterized observed planetary systems hold information about their formation conditions in the protoplanetary disks and that it is possible to extract this information, namely the initial disk surface density and viscosity. This helps to constrain planet formation.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1051/0004-6361/202142176DOIArticle
https://arxiv.org/abs/2110.13835arXivDiscussion Paper
ORCID:
AuthorORCID
Hühn, L.-A.0000-0001-9942-7634
Pichierri, G.0000-0003-3622-8712
Bitsch, B.0000-0002-8868-7649
Batygin, K.0000-0002-7094-7908
Alternate Title:The Kepler-223 resonance holds information on turbulence during the gas disk phase
Additional Information:© L.-A. Hühn et al. 2021. Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Open Access funding provided by Max Planck Society. Received: 8 September 2021 Accepted: 24 October 2021. L.-A.H, G.P. and B.B. thank the European Research Council (ERC Starting Grant 757448-PAMDORA) for their financial support.
Funders:
Funding AgencyGrant Number
European Research Council (ERC)757448
Max Planck SocietyUNSPECIFIED
Subject Keywords:protoplanetary disks / planet-disk interactions / planets and satellites: dynamical evolution and stability / methods: numerical
DOI:10.1051/0004-6361/202142176
Record Number:CaltechAUTHORS:20211130-215746491
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20211130-215746491
Official Citation:Kepler-223 resonance holds information about turbulence during the gas-disk phase L.-A. Hühn, G. Pichierri, B. Bitsch and K. Batygin A&A, 656 (2021) A115 DOI: https://doi.org/10.1051/0004-6361/202142176
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:112112
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:30 Nov 2021 23:47
Last Modified:15 Dec 2021 20:30

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