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The role of dissipative evolution for three-planet, near-resonant extrasolar systems

Pichierri, Gabriele and Batygin, Konstantin and Morbidelli, Alessandro (2019) The role of dissipative evolution for three-planet, near-resonant extrasolar systems. Astronomy and Astrophysics, 625 . Art. No. A7. ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:20190401-160922617

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Abstract

Early dynamical evolution of close-in planetary systems is shaped by an intricate combination of planetary gravitational interactions, orbital migration, and dissipative effects. While the process of convergent orbital migration is expected to routinely yield resonant planetary systems, previous analyses have shown that the semi-major axes of initially resonant pairs of planets will gradually diverge under the influence of long-term energy damping, producing an overabundance of planetary period ratios in slight excess of exact commensurability. While this feature is clearly evident in the orbital distribution of close-in extrasolar planets, the existing theoretical picture is limited to the specific case of the planetary three-body problem. In this study, we generalise the framework of dissipative divergence of resonant orbits to multi-resonant chains, and apply our results to the current observational census of well-characterised three-planet systems. Focusing on the 2:1 and 3:2 commensurabilities, we identify three three-planet systems, whose current orbital architecture is consistent with an evolutionary history wherein convergent migration first locks the planets into a multi-resonant configuration and subsequent dissipation repels the orbits away from exact commensurability. Nevertheless, we find that the architecture of the overall sample of multi-planetary systems is incompatible with this simple scenario, suggesting that additional physical mechanisms must play a dominant role during the early stages of planetary systems’ dynamical evolution.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1051/0004-6361/201935259DOIArticle
https://arxiv.org/abs/1903.09474arXivDiscussion Paper
ORCID:
AuthorORCID
Pichierri, Gabriele0000-0003-3622-8712
Batygin, Konstantin0000-0002-7094-7908
Additional Information:© 2019 G. Pichierri et al. Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Received 12 February 2019; Accepted 13 March 2019; Published online 29 April 2019.
Group:Astronomy Department
Subject Keywords:planets and satellites: dynamical evolution and stability – planets and satellites: formation
Record Number:CaltechAUTHORS:20190401-160922617
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190401-160922617
Official Citation:The role of dissipative evolution for three-planet, near-resonant extrasolar systems. Gabriele Pichierri, Konstantin Batygin and Alessandro Morbidelli. A&A, 625 (2019) A7. DOI: https://doi.org/10.1051/0004-6361/201935259
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:94335
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:01 Apr 2019 23:40
Last Modified:20 Apr 2020 08:47

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