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<ri:Resource created="2017-02-01T08:32:32Z" 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>2015 TB145 light curve</title><shortName>J/A+A/598/A63</shortName><identifier>ivo://CDS.VizieR/J/A+A/598/A63</identifier><altIdentifier>doi:10.26093/cds/vizier.35980063</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mueller T.G.</name></creator><creator><name>Marciniak A.</name></creator><creator><name>Butkiewicz-Bak M.</name></creator><creator><name>Duffard R.</name></creator><creator><name>Oszkiewicz D.,Kaeufl H.U.</name></creator><creator><name>Szakats R.</name></creator><creator><name>Santana-Ros T.</name></creator><creator><name>Kiss C.</name></creator><creator><name>Santana-Sanz P.</name></creator><date role="Updated">2017-06-19T07:57:35Z</date><date role="Created">2017-02-01T08:32:32Z</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>asteroids</subject><subject>photometry</subject><description>The near-Earth asteroid (NEA) 2015 TB145 had a very close encounter with Earth at 1.3 lunar distances on October 31, 2015. We obtained 3-band mid-infrared observations of this asteroid with the ESO VLT-VISIR instrument covering about 4 hours in total. We also monitored the visual lightcurve during the close-encounter phase. The NEA has a (most likely) rotation period of 2.939+/-0.005-hours and the visual lightcurve shows a peak-to-peak amplitude of about 0.12+/-0.02mag. A second rotation period of 4.779+/-0.012h, with an amplitude of the Fourier fit of 0.10+/-0.02mag, also seems compatible with the available lightcurve measurements. We estimate a V-R colour of 0.56+/-0.05mag from different entries in the MPC database. A reliable determination of the object's absolute magnitude was not possible. Applying different phase relations to the available R-/V-band observations produced H_R_=18.6mag (standard H-G calculations) or H_R_=19.2mag and H_V_=19.8mag (via the H-G_12_ procedure for sparse and low-quality data), with large uncertainties of about 1mag. We performed a detailed thermophysical model analysis by using spherical and partially also ellipsoidal shape models. The thermal properties are best explained by an equator-on (+/-~30{deg}) viewing geometry during our measurements with a thermal inertia in the range 250-700J/m^2^/s^0.5^/K (retrograde rotation) or above 500J/m^2^/s^0.5^/K (prograde rotation). We find that the NEA has a minimum size of about 625m, a maximum size of just below 700m, and a slightly elongated shape with a/b~1.1.</description><source format="bibcode">2017A&amp;A...598A..63M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/598/A63</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/598/A63</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/598/A63</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/598/A63</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/598/A63</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/598/A63</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/598/A63</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/598/A63/table</name><description>Photometric data of 2015 TB145 used for this work</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>JD</name><description>Julian date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mag</name><description>Magnitude</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>