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<ri:Resource created="2021-02-08T14:45:38Z" 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>Kepler planet masses, radii and orbital periods</title><shortName>J/ApJ/880/L1</shortName><identifier>ivo://CDS.VizieR/J/ApJ/880/L1</identifier><altIdentifier>doi:10.26093/cds/vizier.18809001</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Armstrong D.J.</name></creator><creator><name>Meru F.</name></creator><creator><name>Bayliss D.</name></creator><creator><name>Kennedy G.M.</name></creator><creator><name>Veras D.</name></creator><date role="Updated">2021-04-27T11:12:32Z</date><date role="Created">2021-02-08T14:45:38Z</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>exoplanets</subject><subject>stellar-masses</subject><subject>astronomical-models</subject><description>Structure in the planet distribution provides an insight into the processes that shape the formation and evolution of planets. The Kepler mission has led to an abundance of statistical discoveries in regards to planetary radius, but the number of observed planets with measured masses is much smaller. By incorporating results from recent mass determination programs, we have discovered a new gap emerging in the planet population for sub-Neptune-mass planets with orbital periods less than 20 days. The gap follows a slope of decreasing mass with increasing orbital period, has a width of a few M_{Earth}_, and is potentially completely devoid of planets. Fitting Gaussian mixture models to the planet population in this region favors a bimodel distribution over a unimodel one with a reduction in Bayesian information criterion of 19.9, highlighting the gap significance. We discuss several processes that could generate such a feature in the planet distribution, including a pileup of planets above the gap region, tidal interactions with the host star, dynamical interactions with the disk, with other planets, or with accreting material during the formation process.</description><source format="bibcode">2019ApJ...880L...1A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/880/L1</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/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/787/80">J/ApJ/787/80 : 139 Kepler planets transit time variations (Hadden+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/821/89">J/ApJ/821/89 : 12yrs of RVel obs. of exoplanet systems (Bryan+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/602/A107">J/A+A/602/A107 : 231 transiting planets eccentricity and mass (Bonomo+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/109">J/AJ/154/109 : California-Kepler Survey. III. Planet radii (Fulton+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/239/2">J/ApJS/239/2 : Simulated exoplanets from TESS list of targets (Barclay+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/235/38">J/ApJS/235/38 : Kepler planetary cand. VIII. DR25 reliability (Thompson+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/239/32">J/ApJS/239/32 : APOKASC-2 catalog of Kepler evolved stars (Pinsonneault+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/48">J/AJ/155/48 : California-Kepler Survey. V. Masses and radii (Weiss+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/264">J/AJ/156/264 : CKS. VII. 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