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<ri:Resource created="2016-12-14T08:49:26Z" 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>Jupiter internal structure different EOS</title><shortName>J/A+A/596/A114</shortName><identifier>ivo://CDS.VizieR/J/A+A/596/A114</identifier><altIdentifier>doi:10.26093/cds/vizier.35960114</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Miguel Y.</name></creator><creator><name>Guillot T.</name></creator><creator><name>Fayon L.</name></creator><date role="Updated">2018-11-01T13:32:51Z</date><date role="Created">2016-12-14T08:49:26Z</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>solar-system-planets</subject><description>Heavy elements, even though its smaller constituent, are crucial to understand Jupiter formation history. Interior models are used to determine the amount of heavy elements in Jupiter interior, nevertheless this range is still subject to degeneracies due to uncertainties in the equations of state. Prior to Juno mission data arrival, we present Jupiter optimized calculations exploring the ect of different model parameters in the determination of Jupiter's core and heavy element's mass. We perform comparisons between equations of state published recently. The interior model of Jupiter is calculated from the equations of hydrostatic equilibrium, mass and energy conservation, and energy transport. The mass of the core and heavy elements is adjusted to match Jupiter's observational constrains radius and gravitational moments</description><source format="bibcode">2016A&amp;A...596A.114M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/596/A114</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/750/52">J/ApJ/750/52 : Jupiter model with improved EOS (Nettelmann+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/774/148">J/ApJ/774/148 : Ab initio EOS for hydrogen-helium mixtures (Militzer+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/215/21">J/ApJS/215/21 : Hydrogen and Helium EOS in brown dwarfs (Becker+, 2014)</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/A+A/596/A114</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/596/A114</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/596/A114</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/596/A114</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/596/A114</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/596/A114</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/A+A/596/A114/eos3bh</name><description>Equation of state for hydrogen REOS3b, based on Becker et al. (2014, Cat. J/ApJS/215/21)</description><column><name>logT</name><description>Temperature</description><unit>log(K)</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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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>logP</name><description>Pressure</description><unit>dyn.cm**-2</unit><ucd>phys.pressure</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logT</name><description>Temperature</description><unit>log(K)</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logrho</name><description>Density</description><unit>log(g.cm**-3)</unit><ucd>phys.density</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logs</name><description>Specific Entropy (in erg/g/K units)</description><unit>log(1e-07J.g**-1.K**-1)</unit><ucd>phys.entropy</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/A+A/596/A114/eos3sch</name><description>*Equation of state for hydrogen REOS3sc, based on Becker et al. (2014, Cat. J/ApJS/215/21) and Saumon et al. (1995ApJS...99..713S)</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logP</name><description>Pressure</description><unit>dyn.cm**-2</unit><ucd>phys.pressure</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logT</name><description>Temperature</description><unit>log(K)</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logrho</name><description>Density</description><unit>log(g.cm**-3)</unit><ucd>phys.density</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logs</name><description>Specific Entropy (in erg/g/K units)</description><unit>log(1e-07J.g**-1.K**-1)</unit><ucd>phys.entropy</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/A+A/596/A114/eos3sche</name><description>Equation of state for helium REOS3sc, based on Becker et al. (2014, Cat. J/ApJS/215/21) and Saumon et al. (1995ApJS...99..713S)</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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