Please use this identifier to cite or link to this item: http://elar.urfu.ru/handle/10995/111751
Title: Dynamic Evolution of Pairs of Trans-Neptunian Objects: the Case of Binary and Single Objects in Pair
Authors: Kuznetsov, E.
Al-Shiblawi, O.
Gusev, V.
Issue Date: 2021
Publisher: Astronomical Institute, Slovak Academy of Sciences
Central Library of the Slovak Academy of Sciences
Citation: Kuznetsov E. Dynamic Evolution of Pairs of Trans-Neptunian Objects: the Case of Binary and Single Objects in Pair / E. Kuznetsov, O. Al-Shiblawi, V. Gusev // Contributions of the Astronomical Observatory Skalnate Pleso. — 2021. — Vol. 51. — Iss. 3. — P. 226-240.
Abstract: We performed a search for pairs of trans-Neptunian objects in close orbits with semi-ma jor axes of more than 30 AU. Distances in the space of Keplerian orbits were estimated using the Kholshevnikov metrics. Found 21 pairs of trans-Neptunian objects in which one of the components is binary, for Kholshevnikov metrics in five-dimensional space of Keplerian orbits less than 0.121 AU1/2. All pairs belong to cold Classical Kuiper belt objects. Based on nominal orbits, the dynamic evolution of pairs of trans-Neptunian objects in the past 10 Myr has been studied numerically. We searched for low relativevelocity close encounters between trans-Neptunian objects in pairs as well as the minima of the Kholshevnikov metrics and the convergence of the lines of nodes and apses, to estimate the age of the pairs. © 2021. All Rights Reserved.
Keywords: TRANS-NEPTUNIAN OBJECTS
CLASSICAL KUIPER BELT OBJECTS
CELESTIAL MECHANICS
URI: http://elar.urfu.ru/handle/10995/111751
Access: info:eu-repo/semantics/openAccess
SCOPUS ID: 85126371782
WOS ID: 000734714000004
PURE ID: 29226197
ISSN: 1335-1842
DOI: 10.31577/CAOSP.2021.51.3.226
metadata.dc.description.sponsorship: This work has been supported by the Russian Ministry of Science and Higher Education via the State Assignment Project FEUZ-2020-0038.
Appears in Collections:Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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