A Dynamical Survey of the Trans-Neptunian Region. I. Mean-motion Resonances with Neptune
In this paper, we present a large-scale dynamical survey of the trans-Neptunian region, with particular attention to mean-motion resonances (MMRs). We study a set of 4121 trans-Neptunian objects (TNOs), a sample far larger than in previous works. We perform direct long-term numerical integrations th...
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IOP Publishing
2023-01-01
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Online Access: | https://doi.org/10.3847/1538-4365/acc4c8 |
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author | E. Forgács-Dajka E. Kővári T. Kovács Cs. Kiss Zs. Sándor |
author_facet | E. Forgács-Dajka E. Kővári T. Kovács Cs. Kiss Zs. Sándor |
author_sort | E. Forgács-Dajka |
collection | DOAJ |
description | In this paper, we present a large-scale dynamical survey of the trans-Neptunian region, with particular attention to mean-motion resonances (MMRs). We study a set of 4121 trans-Neptunian objects (TNOs), a sample far larger than in previous works. We perform direct long-term numerical integrations that enable us to examine the overall dynamics of the individual TNOs as well as to identify all MMRs. For the latter purpose, we apply an own-developed FAIR method that allows the semi-automatic identification of even very high-order MMRs. Apart from searching for the more frequent eccentricity-type resonances that previous studies concentrated on, we set our method to allow the identification of inclination-type MMRs, too. Furthermore, we distinguish between TNOs that are locked in a given MMR throughout the whole integration time span (10 ^8 yr) and those that are only temporarily captured in resonances. For a more detailed dynamical analysis of the trans-Neptunian space, we also construct dynamical maps using test particles. Observing the fine structure of the 34–80 au region underlines the stabilizing role of the MMRs, with the regular regions coinciding with the positions of real TNOs. |
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spelling | doaj.art-be657ffa66e7463eb75ea1a16d531bcd2023-09-03T13:51:13ZengIOP PublishingThe Astrophysical Journal Supplement Series0067-00492023-01-012661510.3847/1538-4365/acc4c8A Dynamical Survey of the Trans-Neptunian Region. I. Mean-motion Resonances with NeptuneE. Forgács-Dajka0https://orcid.org/0000-0002-5735-6273E. Kővári1https://orcid.org/0000-0002-4491-2824T. Kovács2https://orcid.org/0000-0002-0697-6050Cs. Kiss3https://orcid.org/0000-0002-8722-6875Zs. Sándor4https://orcid.org/0000-0003-1216-913XDepartment of Astronomy, Institute of Geography and Earth Sciences, Eötvös Loránd University , H-1117 Budapest, Pázmány Péter sétány 1/A, Hungary; Centre for Astrophysics and Space Science, Eötvös Loránd University , H-1117 Budapest, Pázmány Péter sétány 1/A, Hungary; ELKH-SZTE Stellar Astrophysics Research Group , H-6500 Baja, Szegedi út, Kt. 766, Hungary; Wigner Research Centre for Physics , P.O. Box 49, Budapest H-1525, HungaryDepartment of Astronomy, Institute of Geography and Earth Sciences, Eötvös Loránd University , H-1117 Budapest, Pázmány Péter sétány 1/A, Hungary; Centre for Astrophysics and Space Science, Eötvös Loránd University , H-1117 Budapest, Pázmány Péter sétány 1/A, Hungary; Wigner Research Centre for Physics , P.O. Box 49, Budapest H-1525, HungaryELKH–ELTE Extragalctic Astrophysics Research Group, Eötvös Loránd University , H-1117 Budapest, Pázmány Péter sétány 1/A, HungaryKonkoly Observatory, Research Centre for Astronomy and Earth Sciences , Konkoly Thege 15-17, H-1121, Budapest, Hungary ; kiss.csaba@csfk.org; CSFK, MTA Centre of Excellence , Budapest, Konkoly Thege Miklós út 15-17., H-1121, Hungary; ELTE Eötvös Loránd University , Institute of Physics, Budapest, HungaryDepartment of Astronomy, Institute of Geography and Earth Sciences, Eötvös Loránd University , H-1117 Budapest, Pázmány Péter sétány 1/A, Hungary; Centre for Astrophysics and Space Science, Eötvös Loránd University , H-1117 Budapest, Pázmány Péter sétány 1/A, Hungary; Konkoly Observatory, Research Centre for Astronomy and Earth Sciences , Konkoly Thege 15-17, H-1121, Budapest, Hungary ; kiss.csaba@csfk.orgIn this paper, we present a large-scale dynamical survey of the trans-Neptunian region, with particular attention to mean-motion resonances (MMRs). We study a set of 4121 trans-Neptunian objects (TNOs), a sample far larger than in previous works. We perform direct long-term numerical integrations that enable us to examine the overall dynamics of the individual TNOs as well as to identify all MMRs. For the latter purpose, we apply an own-developed FAIR method that allows the semi-automatic identification of even very high-order MMRs. Apart from searching for the more frequent eccentricity-type resonances that previous studies concentrated on, we set our method to allow the identification of inclination-type MMRs, too. Furthermore, we distinguish between TNOs that are locked in a given MMR throughout the whole integration time span (10 ^8 yr) and those that are only temporarily captured in resonances. For a more detailed dynamical analysis of the trans-Neptunian space, we also construct dynamical maps using test particles. Observing the fine structure of the 34–80 au region underlines the stabilizing role of the MMRs, with the regular regions coinciding with the positions of real TNOs.https://doi.org/10.3847/1538-4365/acc4c8Resonant Kuiper belt objectsN-body problem |
spellingShingle | E. Forgács-Dajka E. Kővári T. Kovács Cs. Kiss Zs. Sándor A Dynamical Survey of the Trans-Neptunian Region. I. Mean-motion Resonances with Neptune The Astrophysical Journal Supplement Series Resonant Kuiper belt objects N-body problem |
title | A Dynamical Survey of the Trans-Neptunian Region. I. Mean-motion Resonances with Neptune |
title_full | A Dynamical Survey of the Trans-Neptunian Region. I. Mean-motion Resonances with Neptune |
title_fullStr | A Dynamical Survey of the Trans-Neptunian Region. I. Mean-motion Resonances with Neptune |
title_full_unstemmed | A Dynamical Survey of the Trans-Neptunian Region. I. Mean-motion Resonances with Neptune |
title_short | A Dynamical Survey of the Trans-Neptunian Region. I. Mean-motion Resonances with Neptune |
title_sort | dynamical survey of the trans neptunian region i mean motion resonances with neptune |
topic | Resonant Kuiper belt objects N-body problem |
url | https://doi.org/10.3847/1538-4365/acc4c8 |
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