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<ri:Resource created="2017-02-27T09:15:16Z" 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>C/O and Mg/Si for solar neighborhood's stars</title><shortName>J/ApJ/831/20</shortName><identifier>ivo://CDS.VizieR/J/ApJ/831/20</identifier><altIdentifier>doi:10.26093/cds/vizier.18310020</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brewer J.M.</name></creator><creator><name>Fischer D.A.</name></creator><date role="Updated">2024-12-30T20:08:34Z</date><date role="Created">2017-02-27T09:15:16Z</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>g-stars</subject><subject>chemical-abundances</subject><subject>solar-system-planets</subject><description>The carbon-to-oxygen ratio in a protoplanetary disk can have a dramatic influence on the compositions of any terrestrial planets formed. In regions of high C/O, planets form primarily from carbonates, and in regions of low C/O, the ratio of magnesium to silicon determines the types of silicates that dominate the compositions. We present C/O and Mg/Si ratios for 852 F, G, and K dwarfs in the solar neighborhood. We find that the frequency of carbon-rich dwarfs in the solar neighborhood is &lt;0.13% and that 156 known planet hosts in the sample follow a similar distribution as all of the stars as a whole. The cosmic distribution of Mg/Si for these same stars is broader than the C/O distribution and peaks near 1.0, with ~60% of systems having 1&lt;=Mg/Si&lt;2, leading to rocky planet compositions similar to the Earth. This leaves 40% of systems that can have planets that are silicate-rich and that may have very different compositions than our own.</description><source format="bibcode">2016ApJ...831...20B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/831/20</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/ApJS/225/32">J/ApJS/225/32 : Extended abundance analysis of cool stars (Brewer+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/584/A72">J/A+A/584/A72 : A rocky planet at 6.5pc from the Sun (Motalebi+ 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/568/A25">J/A+A/568/A25 : C and O abundances in stellar populations (Nissen+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/778/132">J/ApJ/778/132 : C and O abundances in 55 Cnc (Teske+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/735/41">J/ApJ/735/41 : Carbon and oxygen abundances in FGK stars (Petigura+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/725/2349">J/ApJ/725/2349 : C/O vs Mg/Si of planetary systems (Delgado Mena+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/715/1050">J/ApJ/715/1050 : Predicted abundances for extrasolar planets. 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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>SPOCS</name><description>[2/3247] SPOCS ID</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Star name (1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>Vmag</name><description>[0/13.7]? 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