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<ri:Resource created="2017-02-27T10:06:42Z" 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>Mass-metallicity relation for giant planets</title><shortName>J/ApJ/831/64</shortName><identifier>ivo://CDS.VizieR/J/ApJ/831/64</identifier><altIdentifier>doi:10.26093/cds/vizier.18310064</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Thorngren D.P.</name></creator><creator><name>Fortney J.J.</name></creator><creator><name>Murray-Clay R.A.</name></creator><creator><name>Lopez E.D.</name></creator><date role="Updated">2017-09-22T16:15:31Z</date><date role="Created">2017-02-27T10:06:42Z</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>stellar-masses</subject><subject>solar-system-planets</subject><description>Exoplanet discoveries of recent years have provided a great deal of new data for studying the bulk compositions of giant planets. Here we identify 47 transiting giant planets (20 M_{\Earth}_ &lt; M &lt; 20 M_J_) whose stellar insolations are low enough (F_*_ &lt; 2 x 10^8^ erg s^-1^ cm^-2^, or roughly T_eff_ &lt; 1000) that they are not affected by the hot-Jupiter radius inflation mechanism(s). We compute a set of new thermal and structural evolution models and use these models in comparison with properties of the 47 transiting planets (mass, radius, age) to determine their heavy element masses. A clear correlation emerges between the planetary heavy element mass M_z_ and the total planet mass, approximately of the form M_z_\propto\sqrtM. This finding is consistent with the core-accretion model of planet formation. We also study how stellar metallicity [Fe/H] affects planetary metal-enrichment and find a weaker correlation than has previously been reported from studies with smaller sample sizes. We confirm a strong relationship between the planetary metal-enrichment relative to the parent star Z_planet_/Z_star_ and the planetary mass, but see no relation in Z_planet_/Z_star_ with planet orbital properties or stellar mass. The large heavy element masses of many planets (&gt;50 M_{\Earth}_) suggest significant amounts of heavy elements in H/He envelopes, rather than cores, such that metal-enriched giant planet atmospheres should be the rule. We also discuss a model of core-accretion planet formation in a one-dimensional disk and show that it agrees well with our derived relation between mass and Z_planet_/Z_star_.</description><source format="bibcode">2016ApJ...831...64T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/831/64</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/B/corot">B/corot : CoRoT observation log (N2-4.4) (CoRoT 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/590/A112">J/A+A/590/A112 : Kepler-539 CAFE radial velocity measurements (Mancini+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/573/A124">J/A+A/573/A124 : Kepler-117 (KOI-209) transit-timing variations (Bruno+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/150/33">J/AJ/150/33 : Photometry &amp; spectroscopy of HATS-9 and HATS-10 (Brahm+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/166">J/AJ/149/166 : Photometry and spectroscopy of HATS-6 (Hartman+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/149">J/AJ/149/149 : Photometry and spectroscopy of HAT-P-54 (Bakos+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/210/25">J/ApJS/210/25 : Transit timing variation for planetary pairs. 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