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<ri:Resource created="2013-03-01T10:12:21Z" 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>Photometry of 16 Flora family asteroids</title><shortName>J/A+A/551/A102</shortName><identifier>ivo://CDS.VizieR/J/A+A/551/A102</identifier><altIdentifier>doi:10.26093/cds/vizier.35510102</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kryszczynska A.</name></creator><date role="Updated">2013-03-01T09:26:26Z</date><date role="Created">2013-03-01T10:12:21Z</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><subject>photometry</subject><description>It is known that the Yarkovsky effect moves small asteroids to larger/smaller semimajor axes depending on their prograde/retrograde spins. The YORP effect influences asteroid spin periods and spin axis orientations so that they evolve in time. The alignment of the spin vectors and correlations of the spin rates, now known as Slivan states and observed among members of the Koronis family, are interpreted in terms of the YORP effect and spin-orbit resonances. Splitting asteroid families into prograde and retrograde groups has recently been proposed as a result of the Yarkovsky effect. Prograde and retrograde asteroids drift in different directions, and this has never been observed directly. The influence of the Yarkovsky and YORP effects should be observable among objects in asteroid families, especially in the Flora family, which lies close to the Sun and consists of many small objects. The Flora family asteroids were modelled using the lightcurve inversion technique. As a result the orientation of spin vectors, shapes, and sidereal periods of rotation were obtained.</description><source format="bibcode">2013A&amp;A...551A.102K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/551/A102</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/J/A+A/498/313">J/A+A/498/313 : Photometry of 3 main belt asteroids (Marciniak+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/508/1503">J/A+A/508/1503 : Photometry of 3 main belt asteroids (Marciniak+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/529/A107">J/A+A/529/A107 : Photometry of 4 main belt asteroids (Marciniak+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/545/A131">J/A+A/545/A131 : Photometry of 8 main belt asteroids (Marciniak+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/546/A72">J/A+A/546/A72 : Light curves of Flora region asteroids (Kryszczynska+, 2012)</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/A+A/551/A102</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/551/A102</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/551/A102</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/551/A102</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/551/A102</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/551/A102</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"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/551/A102/objects</name><description>Asteroid fundamental parameters</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>Ast</name><description>Asteroid number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Asteroid name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>H</name><description>Absolute magnitude H parameter (1)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Diam</name><description>? IRAS diameter (1)</description><unit>km</unit><ucd>phys.size.diameter</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>i</name><description>Inclination (1)</description><unit>deg</unit><ucd>src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e</name><description>Eccentricity (1)</description><ucd>src.orbital.eccentricity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>a</name><description>Semimajor axis (1)</description><unit>AU</unit><ucd>phys.size.smajAxis</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FileName</name><description>Name of the file containing the light curve</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Orb</name><description>Details of the orbit of this asteroid, from the astorb database</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>LC</name><description>Light curve of the asteroid</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>