| http://dbpedia.org/ontology/Planet/orbitalPeriod
|
0.022999999999999996
|
| http://dbpedia.org/ontology/abstract
|
Kepler-1647 (AB)b è un pianeta extrasolare … Kepler-1647 (AB)b è un pianeta extrasolare circumbinario che orbita attorno a Kepler-1647, una stella binaria situata nella costellazione del Cigno, distante 3700 anni luce dal sistema solare. Il pianeta è stato scoperto nel giugno 2016 con il metodo del transito, quando ha causato un piccolo oscuramento della stella primaria, e successivamente della secondaria. Il primo transito fu osservato nel 2012, tuttavia quel singolo evento non era sufficiente per poter confermare la presenza dell'esopianeta.er confermare la presenza dell'esopianeta.
, كيبلر 1647 بي (بالإنجليزية: Kepler-1647b) الذي يرمز له بالرمز KOI-2939.01، هو كوكب خارج المجموعة الشمسية، في كوكبة الدجاجة (كوكبة).
, Kepler-1647b (auch Kepler-1647(AB)b oder K … Kepler-1647b (auch Kepler-1647(AB)b oder KOI-2939b) ist ein jupitergroßer Gasriese, der den 3700 Lichtjahre von der Erde entfernten Doppelstern Kepler-1647(AB) im Sternbild Schwan umkreist. Der Planet umkreist die beiden etwa sonnengroßen Sterne zirkumbinär in relativ großem Abstand. Für einen Umlauf benötigt er 1.107 Tage und befindet sich in der habitablen Zone. Sein Alter wird auf 4,4 Milliarden Jahre geschätzt.r wird auf 4,4 Milliarden Jahre geschätzt.
, Kepler-1647b (a veces llamado Kepler-1647 … Kepler-1647b (a veces llamado Kepler-1647 (AB)-b para distinguirlo del componente secundario) es un exoplaneta circumbinario que orbita la estrella , a 3,700 años luz (1,100 pársecs) de la Tierra, en la constelación de Cygnus. Fue anunciado el 13 de junio de 2016 en San Diego, en una reunión de la American Astronomical Society. Se detectó usando el método de tránsito, cuando causó el oscurecimiento de la estrella principal, y luego cuando la estrella secundaria se "mezclaba" con el eclipse de la otra. El primer tránsito del planeta se identificó en 2012, pero en ese momento el evento aislado no fue suficiente para descartar la contaminación, o confirmarlo como un planeta. Fue descubierto por el análisis de la curva de luz de Kepler, que mostró el planeta en tránsito.Este planeta contiene una posible doble estrella.aneta contiene una posible doble estrella.
, Kepler-1647 b est une exoplanète circumbinaire appartenant au système de , ayant une période orbitale d'environ 1 107 jours et située à 3 700 années-lumière de la Terre (1 100 pc) dans la constellation du Cygne.
, Kepler-1647b (sometimes named Kepler-1647( … Kepler-1647b (sometimes named Kepler-1647(AB)-b to distinguish it from the secondary component) is a circumbinary exoplanet that orbits the binary star system Kepler-1647, 3,700 light-years (1,100 pc) from Earth in the constellation Cygnus. It was announced on June 13, 2016, in San Diego at a meeting of the American Astronomical Society. It was detected using the transit method, when it caused the dimming of the primary star, and then again of the secondary star blended with the primary star eclipse.The first transit of the planet was identified in 2012, but at the time the single event was not enough to rule out contamination, or confirm it as a planet. It was discovered by the analysis of the Kepler light-curve, which showed the planet in transit.curve, which showed the planet in transit.
, 克卜勒1647b（Kepler-1647b，有時也寫為Kepler-1647(AB) … 克卜勒1647b（Kepler-1647b，有時也寫為Kepler-1647(AB)-b代表它是系統中的次要成員星，或者可稱為KOI-2939.01）是一顆環繞聯星克卜勒1647的環聯星太陽系外行星，距離地球約3,700光年（1,100秒差距），在天球上位於天鵝座。該行星於2016年6月13日美國天文學會於加州聖地牙哥的會議上宣布發現。天文學家以凌日法發現它，並且觀測資料顯示該行星先使聯星中的主星光度下降，再使伴星光度下降。克卜勒1647b的首次凌星紀錄觀測於2012年，但當時只是單一事件，無法排除誤差或確認它是行星。之後天文學家分析克卜勒太空望遠鏡觀測資料的光變曲線，才確認了克卜勒1647b的凌星現象。天文學家分析克卜勒太空望遠鏡觀測資料的光變曲線，才確認了克卜勒1647b的凌星現象。
|
| http://dbpedia.org/ontology/detectionMethod
|
Transit
|
| http://dbpedia.org/ontology/discovered
|
"2016-06-13"^^xsd:date
|
| http://dbpedia.org/ontology/orbitalPeriod
|
1987.2
|
| http://dbpedia.org/ontology/thumbnail
|
http://commons.wikimedia.org/wiki/Special:FilePath/KEPLER_1647_%28AB%29_b.png?width=300 +
|
| http://dbpedia.org/ontology/wikiPageExternalLink
|
http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview%3Fobjname=Kepler-1647%2Bb&type=CONFIRMED_PLANET +
|
| http://dbpedia.org/ontology/wikiPageID
|
50807996
|
| http://dbpedia.org/ontology/wikiPageLength
|
7504
|
| http://dbpedia.org/ontology/wikiPageRevisionID
|
1069719576
|
| http://dbpedia.org/ontology/wikiPageWikiLink
|
http://dbpedia.org/resource/Binary_star_system +
, http://dbpedia.org/resource/Kepler_Object_of_Interest +
, http://dbpedia.org/resource/Category:Exoplanets_discovered_in_2016 +
, http://dbpedia.org/resource/Kepler-453b +
, http://dbpedia.org/resource/Category:Circumbinary_planets +
, http://dbpedia.org/resource/Kepler_%28spacecraft%29 +
, http://dbpedia.org/resource/Circumbinary_planet +
, http://dbpedia.org/resource/Accretion_%28astrophysics%29 +
, http://dbpedia.org/resource/Day +
, http://dbpedia.org/resource/Habitable_zone +
, http://dbpedia.org/resource/Light-curve +
, http://dbpedia.org/resource/2MASS +
, http://dbpedia.org/resource/Jupiter +
, http://dbpedia.org/resource/Exoplanet +
, http://dbpedia.org/resource/Protoplanet +
, http://dbpedia.org/resource/Category:Giant_planets_in_the_habitable_zone +
, http://dbpedia.org/resource/Cygnus_%28constellation%29 +
, http://dbpedia.org/resource/Category:Exoplanets_discovered_by_the_Kepler_space_telescope +
, http://dbpedia.org/resource/Category:Cygnus_%28constellation%29 +
, http://dbpedia.org/resource/Kelvin +
, http://dbpedia.org/resource/Kepler_Input_Catalog +
, http://dbpedia.org/resource/Transit_method +
, http://dbpedia.org/resource/Category:Transiting_exoplanets +
, http://dbpedia.org/resource/Kepler-16b +
|
| http://dbpedia.org/property/apsis
|
astron
|
| http://dbpedia.org/property/caption
|
Kepler-1647b
|
| http://dbpedia.org/property/discovered
|
"2016-06-13"^^xsd:date
|
| http://dbpedia.org/property/discoveryMethod
|
Transit
|
| http://dbpedia.org/property/discoverySite
|
http://dbpedia.org/resource/Kepler_%28spacecraft%29 +
|
| http://dbpedia.org/property/eccentricity
|
0.0581
|
| http://dbpedia.org/property/inclination
|
~90.1
|
| http://dbpedia.org/property/mass
|
1.52
|
| http://dbpedia.org/property/meanRadius
|
1.06
|
| http://dbpedia.org/property/name
|
Kepler-1647b
|
| http://dbpedia.org/property/period
|
1987.1999999999998
|
| http://dbpedia.org/property/star
|
Kepler-1647
|
| http://dbpedia.org/property/wikiPageUsesTemplate
|
http://dbpedia.org/resource/Template:Short_description +
, http://dbpedia.org/resource/Template:Jupiter_mass +
, http://dbpedia.org/resource/Template:Exoplanet +
, http://dbpedia.org/resource/Template:Sky +
, http://dbpedia.org/resource/Template:2016_in_space +
, http://dbpedia.org/resource/Template:Solar_mass +
, http://dbpedia.org/resource/Template:Infobox_planet +
, http://dbpedia.org/resource/Template:Solar_radius +
, http://dbpedia.org/resource/Template:Convert +
, http://dbpedia.org/resource/Template:Reflist +
, http://dbpedia.org/resource/Template:Jupiter_radius +
|
| http://purl.org/dc/terms/subject
|
http://dbpedia.org/resource/Category:Circumbinary_planets +
, http://dbpedia.org/resource/Category:Exoplanets_discovered_in_2016 +
, http://dbpedia.org/resource/Category:Giant_planets_in_the_habitable_zone +
, http://dbpedia.org/resource/Category:Transiting_exoplanets +
, http://dbpedia.org/resource/Category:Cygnus_%28constellation%29 +
, http://dbpedia.org/resource/Category:Exoplanets_discovered_by_the_Kepler_space_telescope +
|
| http://www.w3.org/ns/prov#wasDerivedFrom
|
http://en.wikipedia.org/wiki/Kepler-1647b?oldid=1069719576&ns=0 +
|
| http://xmlns.com/foaf/0.1/depiction
|
http://commons.wikimedia.org/wiki/Special:FilePath/KEPLER_1647_%28AB%29_b.png +
|
| http://xmlns.com/foaf/0.1/isPrimaryTopicOf
|
http://en.wikipedia.org/wiki/Kepler-1647b +
|
| http://xmlns.com/foaf/0.1/name
|
Kepler-1647b
|
| owl:sameAs |
http://hi.dbpedia.org/resource/%E0%A4%95%E0%A5%87%E0%A4%AA%E0%A4%B2%E0%A4%B0-1647%E0%A4%AC%E0%A5%80 +
, http://ar.dbpedia.org/resource/%D9%83%D9%8A%D8%A8%D9%84%D8%B1-1647b +
, http://es.dbpedia.org/resource/Kepler-1647b +
, http://zh.dbpedia.org/resource/%E5%85%8B%E5%8D%9C%E5%8B%921647b +
, http://fr.dbpedia.org/resource/Kepler-1647_b +
, http://de.dbpedia.org/resource/Kepler-1647b +
, https://global.dbpedia.org/id/2KGBP +
, http://www.wikidata.org/entity/Q24577721 +
, http://dbpedia.org/resource/Kepler-1647b +
, http://he.dbpedia.org/resource/%D7%A7%D7%A4%D7%9C%D7%A8-1647b +
, http://it.dbpedia.org/resource/Kepler-1647_%28AB%29b +
, http://vi.dbpedia.org/resource/Kepler-1647b +
, http://yago-knowledge.org/resource/Kepler-1647b +
|
| rdf:type |
http://dbpedia.org/ontology/Planet +
, http://dbpedia.org/ontology/CelestialBody +
, http://dbpedia.org/ontology/Location +
, http://dbpedia.org/ontology/Place +
, http://schema.org/Place +
, http://www.wikidata.org/entity/Q634 +
|
| rdfs:comment |
Kepler-1647b (auch Kepler-1647(AB)b oder K … Kepler-1647b (auch Kepler-1647(AB)b oder KOI-2939b) ist ein jupitergroßer Gasriese, der den 3700 Lichtjahre von der Erde entfernten Doppelstern Kepler-1647(AB) im Sternbild Schwan umkreist. Der Planet umkreist die beiden etwa sonnengroßen Sterne zirkumbinär in relativ großem Abstand. Für einen Umlauf benötigt er 1.107 Tage und befindet sich in der habitablen Zone. Sein Alter wird auf 4,4 Milliarden Jahre geschätzt.r wird auf 4,4 Milliarden Jahre geschätzt.
, Kepler-1647 (AB)b è un pianeta extrasolare … Kepler-1647 (AB)b è un pianeta extrasolare circumbinario che orbita attorno a Kepler-1647, una stella binaria situata nella costellazione del Cigno, distante 3700 anni luce dal sistema solare. Il pianeta è stato scoperto nel giugno 2016 con il metodo del transito, quando ha causato un piccolo oscuramento della stella primaria, e successivamente della secondaria. Il primo transito fu osservato nel 2012, tuttavia quel singolo evento non era sufficiente per poter confermare la presenza dell'esopianeta.er confermare la presenza dell'esopianeta.
, Kepler-1647b (a veces llamado Kepler-1647 … Kepler-1647b (a veces llamado Kepler-1647 (AB)-b para distinguirlo del componente secundario) es un exoplaneta circumbinario que orbita la estrella , a 3,700 años luz (1,100 pársecs) de la Tierra, en la constelación de Cygnus. Fue anunciado el 13 de junio de 2016 en San Diego, en una reunión de la American Astronomical Society. Se detectó usando el método de tránsito, cuando causó el oscurecimiento de la estrella principal, y luego cuando la estrella secundaria se "mezclaba" con el eclipse de la otra. El primer tránsito del planeta se identificó en 2012, pero en ese momento el evento aislado no fue suficiente para descartar la contaminación, o confirmarlo como un planeta. Fue descubierto por el análisis de la curva de luz de Kepler, que mostró el planeta en tránsito.Este planeta contiene ulaneta en tránsito.Este planeta contiene u
, Kepler-1647b (sometimes named Kepler-1647( … Kepler-1647b (sometimes named Kepler-1647(AB)-b to distinguish it from the secondary component) is a circumbinary exoplanet that orbits the binary star system Kepler-1647, 3,700 light-years (1,100 pc) from Earth in the constellation Cygnus. It was announced on June 13, 2016, in San Diego at a meeting of the American Astronomical Society. It was detected using the transit method, when it caused the dimming of the primary star, and then again of the secondary star blended with the primary star eclipse.The first transit of the planet was identified in 2012, but at the time the single event was not enough to rule out contamination, or confirm it as a planet. It was discovered by the analysis of the Kepler light-curve, which showed the planet in transit.curve, which showed the planet in transit.
, كيبلر 1647 بي (بالإنجليزية: Kepler-1647b) الذي يرمز له بالرمز KOI-2939.01، هو كوكب خارج المجموعة الشمسية، في كوكبة الدجاجة (كوكبة).
, Kepler-1647 b est une exoplanète circumbinaire appartenant au système de , ayant une période orbitale d'environ 1 107 jours et située à 3 700 années-lumière de la Terre (1 100 pc) dans la constellation du Cygne.
, 克卜勒1647b（Kepler-1647b，有時也寫為Kepler-1647(AB) … 克卜勒1647b（Kepler-1647b，有時也寫為Kepler-1647(AB)-b代表它是系統中的次要成員星，或者可稱為KOI-2939.01）是一顆環繞聯星克卜勒1647的環聯星太陽系外行星，距離地球約3,700光年（1,100秒差距），在天球上位於天鵝座。該行星於2016年6月13日美國天文學會於加州聖地牙哥的會議上宣布發現。天文學家以凌日法發現它，並且觀測資料顯示該行星先使聯星中的主星光度下降，再使伴星光度下降。克卜勒1647b的首次凌星紀錄觀測於2012年，但當時只是單一事件，無法排除誤差或確認它是行星。之後天文學家分析克卜勒太空望遠鏡觀測資料的光變曲線，才確認了克卜勒1647b的凌星現象。天文學家分析克卜勒太空望遠鏡觀測資料的光變曲線，才確認了克卜勒1647b的凌星現象。
|
| rdfs:label |
Kepler-1647b
, Kepler-1647 b
, 克卜勒1647b
, كيبلر-1647b
, Kepler-1647 (AB)b
|
