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<ri:Resource created="2021-07-21T14:26:35Z" 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>Transits, occultation times and RVs of WASP-12b</title><shortName>J/ApJ/888/L5</shortName><identifier>ivo://CDS.VizieR/J/ApJ/888/L5</identifier><altIdentifier>doi:10.26093/cds/vizier.18889005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yee S.W.</name></creator><creator><name>Winn J.N.</name></creator><creator><name>Knutson H.A.</name></creator><creator><name>Patra K.C.</name></creator><creator><name>Vissapragada S.</name></creator><creator><name>Zhang M.M.,Holman M.J.</name></creator><creator><name>Shporer A.</name></creator><creator><name>Wright J.T.</name></creator><date role="Updated">2021-10-25T10:19:53Z</date><date role="Created">2021-07-21T14:26:35Z</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>exoplanets</subject><subject>infrared-photometry</subject><subject>radial-velocity</subject><description>WASP-12b is a transiting hot Jupiter on a 1.09 day orbit around a late-F star. Since the planet's discovery in 2008, the time interval between transits has been decreasing by 29+/-2ms/yr. This is a possible sign of orbital decay, although the previously available data left open the possibility that the planet's orbit is slightly eccentric and is undergoing apsidal precession. Here, we present new transit and occultation observations that provide more decisive evidence for orbital decay, which is favored over apsidal precession by a {Delta}BIC of 22.3 or Bayes factor of 70000. We also present new radial-velocity data that rule out the Romer effect as the cause of the period change. This makes WASP-12 the first planetary system for which we can be confident that the orbit is decaying. The decay timescale for the orbit is P/{dot}P=3.25+/-0.23Myr. Interpreting the decay as the result of tidal dissipation, the modified stellar tidal quality factor is Q_*_^'^=1.8x10^5^.</description><source format="bibcode">2020ApJ...888L...5Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/888/L5</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/ApJ/692/L9">J/ApJ/692/L9 : Tidal evolution of transiting exoplanets (Levrard+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/709/168">J/ApJ/709/168 : Eccentric orbits in exoplanets (Anglada-Escude+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/720/872">J/ApJ/720/872 : A spectropolarimetric analysis of WASP-12 (Fossati+, 2010)</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/A+A/528/A65">J/A+A/528/A65 : WASP-12b transits (Maciejewski+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/529/A75">J/A+A/529/A75 : Limb-darkening coefficients (Claret+, 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/745/77">J/ApJ/745/77 : Photochemical model for planet WASP-12b (Kopparapu+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/18">J/ApJ/757/18 : RVs for 16 hot Jupiter host stars (Albrecht+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/161">J/ApJ/757/161 : Spectroscopy of 56 exoplanet host stars (Torres+, 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Date</name><description>UT date</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>Orbit</name><description>[1341/2026] Orbit number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BJD</name><description>[57769.5/58517.3] Midpoint in Barycentric Julian Date TDB; BJD-2400000</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_BJD</name><description>[0.00074/0.0014] Timing uncertainty</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Depth</name><description>[1089/4720] Eclipse depth</description><unit>(10-6)</unit><ucd>phot.mag;stat.min</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Depth</name><description>[71/279] Depth negative uncertainty</description><unit>(10-6)</unit><ucd>stat.error;phys.absorption.opticalDepth</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>E_Depth</name><description>[72/289] Depth positive uncertainty</description><unit>(10-6)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Source</name><description>Instrument or reference</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>r_Source</name><description>[ab] Eclipse observed in another paper (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Band</name><description>Observed photometric band</description><ucd>instr.bandpass</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Ap</name><description>[2/2.4]? 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BJD</name><description>Barycentric Julian Date; TDB</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NFlux</name><description>[0.96/1.03] Normalized flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_NFlux</name><description>[0.001/0.005] The 1{sigma} uncertainty in NFlux</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tel</name><description>Telescope code (1)</description><ucd>meta.code;instr.tel</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Orbit</name><description>[1397/2026] Orbit number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/ApJ/888/L5/table4</name><description>HIRES radial velocity measurements</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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