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<ri:Resource created="2011-01-03T13:18:35Z" 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>Detected planets in the Eta-Earth Survey</title><shortName>J/other/Sci/330.</shortName><identifier>ivo://CDS.VizieR/J/other/Sci/330.653</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Howard A.W.</name></creator><creator><name>Marcy G.W.</name></creator><creator><name>Johnson J.A.</name></creator><creator><name>Fischer D.A.</name></creator><creator><name>Wright J.T.,Isaacson H.</name></creator><creator><name>Valenti J.A.</name></creator><creator><name>Anderson J.</name></creator><creator><name>Lin D.N.C.</name></creator><creator><name>Ida S.</name></creator><date role="Updated">2017-10-11T05:13:33Z</date><date role="Created">2011-01-03T13:18:35Z</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>multiple-stars</subject><subject>solar-system-planets</subject><subject>stellar-masses</subject><description>The questions of how planets form and how common Earth-like planets are can be addressed by measuring the distribution of exoplanet masses and orbital periods. We report the occurrence rate of close-in planets (with orbital periods less than 50 days), based on precise Doppler measurements of 166 Sun-like stars. We measured increasing planet occurrence with decreasing planet mass (M). Extrapolation of a power-law mass distribution fitted to our measurements, df/dlogM=0.39M^-0.48^, predicts that 23% of stars harbor a close-in Earth-mass planet (ranging from 0.5 to 2.0 Earth masses). Theoretical models of planet formation predict a deficit of planets in the domain from 5 to 30 Earth masses and with orbital periods less than 50 days. 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