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<ri:Resource created="2023-09-15T14:44:43Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>TNOs mean-motion resonances with Neptune</title><shortName>J/ApJS/266/5</shortName><identifier>ivo://CDS.VizieR/J/ApJS/266/5</identifier><altIdentifier>doi:10.26093/cds/vizier.22660005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Forgacs-Dajka E.</name></creator><creator><name>Kovari E.</name></creator><creator><name>Kovacs T.</name></creator><creator><name>Kiss C.</name></creator><creator><name>Sandor Z.</name></creator><date role="Updated">2023-10-18T12:33:46Z</date><date role="Created">2023-09-15T14:44:43Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>solar-system</subject><subject>asteroids</subject><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 34-80au region underlines the stabilizing role of the MMRs, with the regular regions coinciding with the positions of real TNOs.</description><source format="bibcode">2023ApJS..266....5F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/266/5</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/astorb">B/astorb : Orbits of Minor Planets (Bowell+ 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/33">J/AJ/156/33 : Resonance sticking in population of scattering TNOs (Yu+, 2018)</relatedResource><relatedResource>http://ssd.jpl.nasa.gov/horizons/ : JPL Horizons on-line solar system data</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/266/5</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/266/5</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/266/5</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/266/5</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/266/5</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/266/5</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/ApJS/266/5/table1</name><description>Summary of the resonant properties of trans-Neptunian objects</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Provisional Designation (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>MMR</name><description>Ratio of the mean-motion resonance (MMR)</description><ucd>stat.fit.omc</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Type</name><description>Type of the mean-motion resonance (2)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Amp1</name><description>Amplitude of libration (3)</description><unit>deg</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>OCC</name><description>[1/9]? JPL Orbit Condition Code (0: best orbit quality; 9:poorest) (4)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>