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<ri:Resource created="2013-12-04T10:41:59Z" status="active" updated="2025-06-13T15:25:00Z" 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>The Kepler-20 planetary system</title><shortName>J/ApJ/749/15</shortName><identifier>ivo://CDS.VizieR/J/ApJ/749/15</identifier><altIdentifier>doi:10.26093/cds/vizier.17490015</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gautier III T.N.</name></creator><creator><name>Charbonneau D.</name></creator><creator><name>Rowe J.F.</name></creator><creator><name>Marcy G.W.</name></creator><creator><name>Isaacson H.,Torres G.</name></creator><creator><name>Fressin F.</name></creator><creator><name>Rogers L.A.</name></creator><creator><name>Desert J.-M.</name></creator><creator><name>Buchhave L.A.,Latham D.W.</name></creator><creator><name>Quinn S.N.</name></creator><creator><name>Ciardi D.R.</name></creator><creator><name>Fabrycky D.C.</name></creator><creator><name>Ford E.B.,Gilliland R.L.</name></creator><creator><name>Walkowicz L.M.</name></creator><creator><name>Bryson S.T.</name></creator><creator><name>Cochran W.D.</name></creator><creator><name>Endl M.,Fischer D.A.</name></creator><creator><name>Howell S.B.</name></creator><creator><name>Horch E.P.</name></creator><creator><name>Barclay T.</name></creator><creator><name>Batalha N.,Borucki W.J.</name></creator><creator><name>Christiansen J.L.</name></creator><creator><name>Geary J.C.</name></creator><creator><name>Henze C.E.</name></creator><creator><name>Holman M.J.,Ibrahim K.</name></creator><creator><name>Jenkins J.M.</name></creator><creator><name>Kinemuchi K.</name></creator><creator><name>Koch D.G.</name></creator><creator><name>Lissauer J.J.,Sanderfer D.T.</name></creator><creator><name>Sasselov D.D.</name></creator><creator><name>Seager S.</name></creator><creator><name>Silverio K.</name></creator><creator><name>Smith J.C.,Still M.</name></creator><creator><name>Stumpe M.C.</name></creator><creator><name>Tenenbaum P.</name></creator><creator><name>Van Cleve J.</name></creator><date role="Updated">2017-12-12T14:45:17Z</date><date role="Created">2013-12-04T10:41:59Z</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 the discovery of the Kepler-20 planetary system, which we initially identified through the detection of five distinct periodic transit signals in the Kepler light curve of the host star 2MASS J19104752+4220194. From high-resolution spectroscopy of the star, we find a stellar effective temperature T_eff_= 5455+/-100 K, a metallicity of [Fe/H] = 0.01+/-0.04, and a surface gravity of log g = 4.4+/-0.1. We combine these estimates with an estimate of the stellar density derived from the transit light curves to deduce a stellar mass of M_*_ = 0.912+/-0.034 M_{sun}_and a stellar radius of R_*_ = 0.944^+0.060^_-0.095_R_{sun}_. For three of the transit signals, we demonstrate that our results strongly disfavor the possibility that these result from astrophysical false positives. We determine the orbital periods and physical radii of the three confirmed planets to be 3.70 days and 1.91^+0.12^_-0.21_R_{earth}_ for Kepler-20b, 10.85 days and 3.07^+0.20^_-0.31_R_{earth}_ for Kepler-20c, and 77.61 days and 2.75^+0.17^_-0.30_R_{earth}_ for Kepler-20d. From multi-epoch radial velocities, we determine the masses of Kepler-20b and Kepler-20c to be 8.7+/-2.2 M_{earth}_ and 16.1 +/-3.5 M_{earth}_, respectively, and we place an upper limit on the mass of Kepler-20d of 20.1 M_{earth}_(2{sigma}).</description><source format="bibcode">2012ApJ...749...15G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/749/15</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/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/204/24">J/ApJS/204/24 : Kepler planetary candidates. III. (Batalha+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/24">J/ApJS/199/24 : The first three quarters of Kepler mission (Tenenbaum+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/42">J/AJ/144/42 : Infrared photometry of 90 KOIs (Adams+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/123/412">J/PASP/123/412 : Exoplanet Orbit Database (Wright+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/197/8">J/ApJS/197/8 : Kepler's cand. multiple transiting planets (Lissauer+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/197/2">J/ApJS/197/2 : Transit timing observations from Kepler. I. (Ford+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/738/170">J/ApJ/738/170 : False positive Kepler planet candidates (Morton+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/736/L25">J/ApJ/736/L25 : Habitability of Kepler planetary cand. 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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>ID</name><description>Planet candidate designation (Kepler-NNa or KOI-NN.NN)</description><ucd>meta.id;phys.atmol.configuration;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType><flag>primary</flag></column><column><name>CentP</name><description>[0.02/0.73] PRF centroid (1)</description><unit>arcsec</unit><ucd>pos;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_CentP</name><description>CentP uncertainty</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SigP</name><description>Significance (2)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CentF</name><description>[0.07/3.07] Flux-weighted centroid (1)</description><unit>arcsec</unit><ucd>pos;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_CentF</name><description>CentF uncertainty</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SigF</name><description>Significance (2)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Per</name><description>? 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