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<ri:Resource created="2017-08-09T11:58:26Z" 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>Times of transits and occultations of WASP-12b</title><shortName>J/AJ/154/4</shortName><identifier>ivo://CDS.VizieR/J/AJ/154/4</identifier><altIdentifier>doi:10.26093/cds/vizier.51540004</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Patra K.C.</name></creator><creator><name>Winn J.N.</name></creator><creator><name>Holman M.J.</name></creator><creator><name>Yu L.</name></creator><creator><name>Deming D.</name></creator><creator><name>Dai F.</name></creator><date role="Updated">2017-09-04T08:29:17Z</date><date role="Created">2017-08-09T11:58:26Z</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-planets</subject><subject>multiple-stars</subject><description>We present new transit and occultation times for the hot Jupiter WASP-12b. The data are compatible with a constant period derivative: P.=-29+/-3ms/yr and P/P.=3.2Myr. However, it is difficult to tell whether we have observed orbital decay or a portion of a 14-year apsidal precession cycle. If interpreted as decay, the star's tidal quality parameter Q_star_ is about 2*10^5^. If interpreted as precession, the planet's Love number is 0.44+/-0.10. Orbital decay appears to be the more parsimonious model: it is favored by {Delta}_{chi}^2^_=5.5 despite having two fewer free parameters than the precession model. The decay model implies that WASP-12 was discovered within the final ~0.2% of its existence, which is an unlikely coincidence but harmonizes with independent evidence that the planet is nearing disruption. Precession does not invoke any temporal coincidence, but it does require some mechanism to maintain an eccentricity of {approx}0.002 in the face of rapid tidal circularization. To distinguish unequivocally between decay and precession will probably require a few more years of monitoring. Particularly helpful will be occultation timing in 2019 and thereafter.</description><source format="bibcode">2017AJ....154....4P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/154/4</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/588/L6">J/A+A/588/L6 : WASP-12 transit light curves (Maciejewski+ 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/785/126">J/ApJ/785/126 : HIRES radial velocity measurements (Knutson+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/551/A108">J/A+A/551/A108 : Multi-site obs. of WASP-12 b transit (Maciejewski+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/161">J/ApJ/757/161 : Spectroscopy of 56 exoplanet host stars (Torres+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/18">J/ApJ/757/18 : Radial velocities for hot Jupiter host stars (Albrecht+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/727/125">J/ApJ/727/125 : Two secondary eclipses of WASP-12b with Spitzer (Campo+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/179">J/AJ/141/179 : Transits of TrES-4b, HAT-P-3b and WASP-12b (Chan+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/720/872">J/ApJ/720/872 : A spectropolarimetric analysis of WASP-12 (Fossati+, 2010)</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/AJ/154/4</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/154/4</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/154/4</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/154/4</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/154/4</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/154/4</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/AJ/154/4/table1</name><description>Transit and occultation times</description><column><name>Ref</name><description>Reference</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="45*">char</dataType></column><column><name>E</name><description>[-1640/1370] Epoch number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><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>Event</name><description>Event (occ=occultation, tra=transit)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>BJD</name><description>Barycentric Julian Date (BJD) of midtransit time (BJD_TDB_)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_BJD</name><description>[0.0001/0.0022] Uncertainty in BJD</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_Ref</name><description>[ab] Flag on Reference (a or b) (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table></schema></tableset></ri:Resource>