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<ri:Resource created="2020-10-09T09:03:47Z" 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>Giant planet bulk and atmosphere metallicities</title><shortName>J/ApJ/874/L31</shortName><identifier>ivo://CDS.VizieR/J/ApJ/874/L31</identifier><altIdentifier>doi:10.26093/cds/vizier.18749031</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Thorngren D.</name></creator><creator><name>Fortney J.J.</name></creator><date role="Updated">2021-03-26T06:48:28Z</date><date role="Created">2020-10-09T09:03:47Z</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>astronomical-models</subject><subject>stellar-atmospheres</subject><subject>exoplanets</subject><description>Atmospheric characterization through spectroscopic analysis, an essential tool of modern exoplanet science, can benefit significantly from the context provided by the interior structure models. In particular, the planet's bulk metallicity, Zp, places an upper limit on the potential atmospheric metallicity. Here we construct interior structure models to derive Zp and atmospheric metallicity upper limits for 403 known transiting giant exoplanets. These limits are low enough that they can usefully inform atmosphere models. Additionally, we argue that comparing Zp to the observed atmospheric metallicity gives a useful measure of how well mixed metals are within the planet. This represents a new avenue for learning about planetary interiors. To aid in the future characterization of new planet discoveries we derive analytic prior predictions of atmosphere metallicity as a function of planet mass, and evaluate the effectiveness of our approach on Jupiter and Saturn. We include log-linear fits for approximating the metallicities of planets not in our catalog.</description><source format="bibcode">2019ApJ...874L..31T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/874/L31</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/J/ApJ/709/159">J/ApJ/709/159 : Relative Ic photometry of WASP-17 (Anderson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/531/A40">J/A+A/531/A40 : Transits of WASP-39b (Faedi+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/728/138">J/ApJ/728/138 : Follow-up photometry of HAT-P-26 (Hartman+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/542/A4">J/A+A/542/A4 : WASP-43b thirty eclipses (Gillon+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/426/1338">J/MNRAS/426/1338 : Transiting planetary system WASP-17 (Southworth+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A134">J/A+A/549/A134 : 4 new WASP transiting close-in giant planets (Hebrard+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/809/77">J/ApJ/809/77 : Transiting Exoplanet Survey Satellite (Sullivan+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/831/64">J/ApJ/831/64 : Mass-metallicity relation for giant planets (Thorngren+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/239/2">J/ApJS/239/2 : Simulated exoplanets from TESS targets (Barclay+, 2018)</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/ApJ/874/L31</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/874/L31</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/874/L31</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/874/L31</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/874/L31</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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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 identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>r_ID</name><description>Reference(s) for discovery and data (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Mass</name><description>[0.07/12.9] Mass</description><unit>(1.898187x10+27kg)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mass</name><description>[0/2.75] Uncertainty in Mass</description><unit>(1.898187x10+27kg)</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rad</name><description>[0.2/1.99] Radius</description><unit>(7.1492x10+7m)</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rad</name><description>[0/0.6] Uncertainty in Radius</description><unit>(7.1492x10+7m)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux</name><description>[0/13.21] Insolation in Giga-ergs/s/cm^2^</description><unit>MW.m**-2</unit><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Temp</name><description>[207.06/2762.7] Equilibrium temperature (2)</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MajAxis</name><description>[0.01/2.72] Orbital semi-major axis</description><unit>AU</unit><ucd>phys.size.smajAxis</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ecc</name><description>[0/0.93] Orbital eccentricity</description><ucd>src.orbital.eccentricity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Period</name><description>[0.79/1107.6] Orbital period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Zp</name><description>[0.04/0.99] Planetary bulk metallicity</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Zp</name><description>[0.01/0.15] Uncertainty in Zp</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zToH</name><description>[6.7/252660] Planetary atmosphere metallicity (3)</description><ucd>phys.abund.Z;obs.atmos</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_zToH</name><description>[2.3/13062480] Uncertainty in zToH</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_zToH</name><description>[11.3/979]? 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