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<ri:Resource created="2012-09-19T12:03:50Z" 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 vs Mg/Si of planetary systems</title><shortName>J/ApJ/725/2349</shortName><identifier>ivo://CDS.VizieR/J/ApJ/725/2349</identifier><altIdentifier>doi:10.26093/cds/vizier.17252349</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Delgado Mena E.</name></creator><creator><name>Israelian G.</name></creator><creator><name>Gonzalez Hernandez J.I.</name></creator><creator><name>Bond J.C.,Santos N.C.</name></creator><creator><name>Udry S.</name></creator><creator><name>Mayor M.</name></creator><date role="Updated">2017-07-05T06:59:27Z</date><date role="Created">2012-09-19T12:03:50Z</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>effective-temperature</subject><subject>solar-system-planets</subject><subject>multiple-stars</subject><subject>late-type-stars</subject><description>Theoretical studies suggest that C/O and Mg/Si are the most important elemental ratios in determining the mineralogy of terrestrial planets. The C/O ratio controls the distribution of Si among carbide and oxide species, while Mg/Si gives information about the silicate mineralogy. We present a detailed and uniform study of C, O, Mg, and Si abundances for 61 stars with detected planets and 270 stars without detected planets from the homogeneous high-quality unbiased HARPS GTO sample, together with 39 more planet-host stars from other surveys. We determine these important mineralogical ratios and investigate the nature of the possible terrestrial planets that could have formed in those planetary systems. We find mineralogical ratios quite different from those of the Sun, showing that there is a wide variety of planetary systems which are not similar to our solar system. Many planetary host stars present an Mg/Si value lower than 1, so their planets will have a high Si content to form species such as MgSiO_3_. This type of composition can have important implications for planetary processes such as plate tectonics, atmospheric composition, or volcanism.</description><source format="bibcode">2010ApJ...725.2349D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/725/2349</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/A+A/541/A40">J/A+A/541/A40 : Metallicity of solar-type stars (Maldonado+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/536/A71">J/A+A/536/A71 : Atmospheric parameters of nearby giant stars (Jones+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/526/A71">J/A+A/526/A71 : C abundances in G and K nearby stars (Da Silva+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A141">J/A+A/533/A141 : Stellar parameters for 582 HARPS FGK stars (Sousa+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/720/1290">J/ApJ/720/1290 : Abundances of stars hosting planets (Ghezzi+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/720/1592">J/ApJ/720/1592 : Signatures of terrestrial planets (Hernandez+, 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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