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<ri:Resource created="2025-02-06T14:46:32Z" status="active" updated="2025-05-21T20:12:35Z" 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>Planetary eccentricity-period (PEP) distributions</title><shortName>J/AJ/168/115</shortName><identifier>ivo://CDS.VizieR/J/AJ/168/115</identifier><altIdentifier>doi:10.26093/cds/vizier.51680115</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bashi D.</name></creator><creator><name>Mazeh T.</name></creator><creator><name>Faigler S.</name></creator><date role="Updated">2025-05-21T20:12:35Z</date><date role="Created">2025-02-06T14:46:32Z</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>two-color-diagrams</subject><subject>absolute-magnitude</subject><subject>visible-astronomy</subject><description>We used the database of 1040 short-period (1&lt;=P&lt;200days) exoplanets radial-velocity orbits to study the planetary eccentricity-period (PEP) distribution. We first divided the sample into low- and high-mass exoplanet subsamples based on the distribution of the (minimum) planetary masses, which displays a clear two-Gaussian distribution, separated at 0.165M_J_. We then selected 216 orbits, low- and high-mass alike, with eccentricities significantly distinct from circular orbits. The 131 giant-planet eccentric orbits display a clear upper envelope, which we model quantitatively, rises monotonically from zero eccentricity and reaches an eccentricity of 0.8 at P~100 days. Conversely, the 85 low-mass planetary orbits display a flat eccentricity distribution between 0.1 and 0.5, with almost no dependence on the orbital period. We show that the striking difference between the two PEP distributions is not a result of the detection technique used. The upper envelope of the high-mass planets, also seen in short-period binary stars, is a clear signature of tidal circularization, which probably took place inside the planets, while the small-planet PEP distribution suggests that the circularization was not effective, probably due to dynamical interactions with neighboring planets.</description><source format="bibcode">2024AJ....168..115B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/168/115</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/375/L27">J/A+A/375/L27 : HD 80606b extremely elongated orbit (Naef+ 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/742/116">J/ApJ/742/116 : Phot. of four massive transiting exoplanets (Bakos+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/197/8">J/ApJS/197/8 : Kepler's cand. multiple transiting planets (Lissauer+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/414/1278">J/MNRAS/414/1278 : Eccentricities of transiting planets (Pont+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/824/15">J/ApJ/824/15 : Orbital circularization of Kepler EBs (Van Eylen+, 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/A+A/630/A135">J/A+A/630/A135 : Beyond the exoplanet mass-radius relation (Ulmer-Moll+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/157/82">J/AJ/157/82 : TEMP. V. Phot. of HAT-P-9, HAT-P-32 &amp; HAT-P-36 (Wang+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/888/L5">J/ApJ/888/L5 : Transits, occultation times and RVs of WASP-12b (Yee+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/649/A6">J/A+A/649/A6 : Gaia Catalog of Nearby Stars - GCNS (Gaia collaboration, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/163/227">J/AJ/163/227 : HIRES RVel follow up for Kepler-1656 (Angelo+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/262/21">J/ApJS/262/21 : 3-D selection of 167 sub-stellar companions (Feng+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/165/125">J/AJ/165/125 : Planetary Orbit Eccentricity Trends (POET). I. (An+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/670/A68">J/A+A/670/A68 : Architecture of exoplanetary systems (Mishra+, 2023)</relatedResource><relatedResource>http://exoplanetarchive.ipac.caltech.edu/ : NASA Exoplanet archive homepage</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/AJ/168/115</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/168/115</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/168/115</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/168/115</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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