The Doubly Librating Plutinos

Named for orbital kinship with Pluto, the Plutinos are a prominent group of Kuiper Belt objects whose orbital periods are in libration about a 3/2 ratio with Neptune’s. We investigate the long-term orbital dynamics of known Plutinos, with attention to the additional libration (or lack thereof) of th...

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Main Authors: Renu Malhotra, Takashi Ito
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/adacd9
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author Renu Malhotra
Takashi Ito
author_facet Renu Malhotra
Takashi Ito
author_sort Renu Malhotra
collection DOAJ
description Named for orbital kinship with Pluto, the Plutinos are a prominent group of Kuiper Belt objects whose orbital periods are in libration about a 3/2 ratio with Neptune’s. We investigate the long-term orbital dynamics of known Plutinos, with attention to the additional libration (or lack thereof) of their argument of perihelion, g , a well-known characteristic of Pluto’s orbit. We show that the g librators among the Plutinos cluster around an arc in the eccentricity–inclination parameter plane. This previously unreported dynamical structure is owed to a family of periodic orbits of the third kind in the restricted problem of three bodies, identified by Poincaré at the end of the 19th century. Approximately 16% of the currently known Plutinos exhibit g librations, a far greater fraction than the ratios of the associated libration frequencies. These results may offer new constraints for theoretical models of the dynamical history of the Plutinos and of the orbital migration history of the giant planets.
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spelling doaj-art-325efc242b2b43778a975dda2c3f58642025-02-07T07:46:45ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01980111510.3847/1538-4357/adacd9The Doubly Librating PlutinosRenu Malhotra0https://orcid.org/0000-0002-1226-3305Takashi Ito1https://orcid.org/0000-0002-0549-9002The University of Arizona , 1629 E University Boulevard, Tucson, AZ 85718, USANational Astronomical Observatory , Osawa 2–21–1 Mitaka, Tokyo 181–8588, JapanNamed for orbital kinship with Pluto, the Plutinos are a prominent group of Kuiper Belt objects whose orbital periods are in libration about a 3/2 ratio with Neptune’s. We investigate the long-term orbital dynamics of known Plutinos, with attention to the additional libration (or lack thereof) of their argument of perihelion, g , a well-known characteristic of Pluto’s orbit. We show that the g librators among the Plutinos cluster around an arc in the eccentricity–inclination parameter plane. This previously unreported dynamical structure is owed to a family of periodic orbits of the third kind in the restricted problem of three bodies, identified by Poincaré at the end of the 19th century. Approximately 16% of the currently known Plutinos exhibit g librations, a far greater fraction than the ratios of the associated libration frequencies. These results may offer new constraints for theoretical models of the dynamical history of the Plutinos and of the orbital migration history of the giant planets.https://doi.org/10.3847/1538-4357/adacd9PlutinosPlutoResonant Kuiper belt objectsTrans-Neptunian objectsSmall Solar System bodiesOrbital resonances
spellingShingle Renu Malhotra
Takashi Ito
The Doubly Librating Plutinos
The Astrophysical Journal
Plutinos
Pluto
Resonant Kuiper belt objects
Trans-Neptunian objects
Small Solar System bodies
Orbital resonances
title The Doubly Librating Plutinos
title_full The Doubly Librating Plutinos
title_fullStr The Doubly Librating Plutinos
title_full_unstemmed The Doubly Librating Plutinos
title_short The Doubly Librating Plutinos
title_sort doubly librating plutinos
topic Plutinos
Pluto
Resonant Kuiper belt objects
Trans-Neptunian objects
Small Solar System bodies
Orbital resonances
url https://doi.org/10.3847/1538-4357/adacd9
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