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<ri:Resource created="2014-03-03T09:24:46Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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>Correlation metallicity / eclipse depth</title><shortName>J/ApJ/752/72</shortName><identifier>ivo://CDS.VizieR/J/ApJ/752/72</identifier><altIdentifier>doi:10.26093/cds/vizier.17520072</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dodson-Robinson S.E.</name></creator><date role="Updated">2018-01-02T13:43:14Z</date><date role="Created">2014-03-03T09:24:46Z</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>chemical-abundances</subject><subject>multiple-stars</subject><subject>solar-system-planets</subject><subject>stellar-radii</subject><description>Previous studies of the interior structure of transiting exoplanets have shown that the heavy-element content of gas giants increases with host star metallicity. Since metal-poor planets are less dense and have larger radii than metal-rich planets of the same mass, one might expect that metal-poor stars host a higher proportion of gas giants with large radii than metal-rich stars. Here I present evidence for a negative correlation at the 2.3{sigma} level between eclipse depth and stellar metallicity in the Kepler gas giant candidates. Based on Kendall's {tau} statistics, the probability that eclipse depth depends on star metallicity is 0.981. The correlation is consistent with planets orbiting low-metallicity stars being, on average, larger in comparison with their host stars than planets orbiting metal-rich stars. Furthermore, since metal-rich stars have smaller radii than metal-poor stars of the same mass and age, a uniform population of planets should show a rise in median eclipse depth with [M/H]. The fact that I find the opposite trend indicates that substantial changes in the gas giant interior structure must accompany increasing [M/H]. I investigate whether the known scarcity of giant planets orbiting low-mass stars could masquerade as an eclipse depth-metallicity correlation, given the degeneracy between metallicity and temperature for cool stars in the Kepler Input Catalog. While the eclipse depth-metallicity correlation is not yet on firm statistical footing and will require spectroscopic [Fe/H] measurements for validation, it is an intriguing window into how the interior structure of planets and even the planet formation mechanism may be changing with Galactic chemical evolution.</description><source format="bibcode">2012ApJ...752...72D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/752/72</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>IsServedBy</relationshipType><relatedResource>Conesearch 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/A+A/557/A70">J/A+A/557/A70 : Evolved planet hosts - stellar parameters (Mortier+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/551/A112">J/A+A/551/A112 : Metallicity-giant planet correlation (Mortier+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/750/114">J/ApJ/750/114 : Kepler TTVs. IV. 4 multiple-planet systems (Fabrycky+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/750/113">J/ApJ/750/113 : TTVs from Kepler. II. 2 multiplanet systems (Ford+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/421/2342">J/MNRAS/421/2342 : 4 Kepler systems transit timing obs. (Steffen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Nat/481.475">J/other/Nat/481.475 : RVs of Kepler-34b + Kepler-35b (Welsh+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/39">J/AJ/143/39 : Analysis of hot Jupiters in Kepler Q2 (Coughlin+, 2012)</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/736/19">J/ApJ/736/19 : Kepler planetary candidates. II. (Borucki+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/697/544">J/ApJ/697/544 : Planets orbiting metal-poor dwarfs. II. 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