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Statements

Subject Item
dbr:List_of_exoplanet_extremes
dbo:wikiPageWikiLink
dbr:Kepler-36b
Subject Item
dbr:List_of_exoplanets_discovered_in_2012
dbo:wikiPageWikiLink
dbr:Kepler-36b
Subject Item
dbr:List_of_exoplanets_discovered_using_the_Kepler_space_telescope
dbo:wikiPageWikiLink
dbr:Kepler-36b
Subject Item
dbr:Eric_Agol
dbo:wikiPageWikiLink
dbr:Kepler-36b
Subject Item
dbr:Terrestrial_planet
dbo:wikiPageWikiLink
dbr:Kepler-36b
Subject Item
dbr:Kepler-36
dbo:wikiPageWikiLink
dbr:Kepler-36b
dbp:exoplanet
dbr:Kepler-36b
Subject Item
dbr:Kepler-36b
rdf:type
yago:PhysicalEntity100001930 yago:Whole100003553 dbo:Planet owl:Thing yago:NaturalObject100019128 dbo:Location yago:Planet109394007 dbo:Place dbo:CelestialBody wikidata:Q634 schema:Place yago:Object100002684 yago:CelestialBody109239740
rdfs:label
كيبلر-36b Kepler-36b Kepler-36 b Kepler-36b ケプラー36b
rdfs:comment
كيبلر 36 بي (بالإنجليزية: Kepler-36b)‏ الذي يرمز له بالرمز KOI-277.02، هو كوكب خارج المجموعة الشمسية، في كوكبة الدجاجة (كوكبة)، يتبع Kepler-36. ケプラー36b (Kepler-36b) は、地球からはくちょう座の方向に約1500光年離れた距離にある恒星ケプラー36の周りを公転する太陽系外惑星である。別名KOI-277b。 Kepler-36b is an exoplanet orbiting the star Kepler-36. This planet has the closest conjunction to Kepler-36c every 97 days. Its density is similar to that of iron. During their closest approach, Kepler-36b and Kepler-36c are located only 0.013 AU (about 1,900,000 km) from each other, which causes extreme transit-timing variations for both planets. Transit-timing variations caused by Kepler-36c are strong enough to put narrow constraints on Kepler-36b's mass. The close proximity of the planet to its host star combined with its relatively low mass caused the planet to lose all or most of its primordial hydrogen/helium envelope. Kepler-36b es un exoplaneta que orbita a la estrella Kepler-36. Fue descubierto por el Telescopio Espacial Kepler en 2012.​ Durante su máximo acercamiento, Kepler-36b y Kepler-36c se encuentran sólo 0,013 UA (menos de 2 000 000 km) entre sí, lo que provoca variaciones de tránsito temporales extremas entre ambos planetas. Las variaciones de tránsitos causados por Kepler-36c son lo suficientemente fuertes para poner limitaciones estrechas en la masa de Kepler-36b. Kepler-36 b est une exoplanète orbitant autour de l'étoile Kepler-36, elle a été découverte en 2012 par la méthode des transits. Comme la Lune avec la Terre, elle présente toujours la même face à Kepler 36.[réf. nécessaire]
foaf:name
Kepler-36b
dbp:name
Kepler-36b
dcterms:subject
dbc:Exoplanets_discovered_by_the_Kepler_space_telescope dbc:Cygnus_(constellation) dbc:Exoplanets_discovered_in_2012
dbo:wikiPageID
36216123
dbo:wikiPageRevisionID
1046845250
dbo:wikiPageWikiLink
dbr:Kepler-36c dbr:Methods_of_detecting_exoplanets dbr:Day dbc:Exoplanets_discovered_by_the_Kepler_space_telescope dbr:Kepler-36 dbr:Exoplanet dbc:Cygnus_(constellation) dbr:Iron dbc:Exoplanets_discovered_in_2012 dbr:Kepler_Mission
owl:sameAs
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dbp:wikiPageUsesTemplate
dbt:Earth_mass dbt:Earth_radius dbt:2012_in_space dbt:Extrasolar-planet-stub dbt:Convert dbt:Val dbt:Reflist dbt:Infobox_planet
dbp:apsis
astron
dbp:discovered
2012
dbp:discoveryMethod
Transit
dbp:eccentricity
<0.04
dbp:inclination
~90
dbp:mass
4.45
dbp:meanRadius
1.486
dbp:period
1195766.496
dbp:singleTemperature
K
dbp:star
dbr:Kepler-36
dbo:abstract
ケプラー36b (Kepler-36b) は、地球からはくちょう座の方向に約1500光年離れた距離にある恒星ケプラー36の周りを公転する太陽系外惑星である。別名KOI-277b。 Kepler-36b es un exoplaneta que orbita a la estrella Kepler-36. Fue descubierto por el Telescopio Espacial Kepler en 2012.​ Durante su máximo acercamiento, Kepler-36b y Kepler-36c se encuentran sólo 0,013 UA (menos de 2 000 000 km) entre sí, lo que provoca variaciones de tránsito temporales extremas entre ambos planetas. Las variaciones de tránsitos causados por Kepler-36c son lo suficientemente fuertes para poner limitaciones estrechas en la masa de Kepler-36b. Kepler-36 b est une exoplanète orbitant autour de l'étoile Kepler-36, elle a été découverte en 2012 par la méthode des transits. Comme la Lune avec la Terre, elle présente toujours la même face à Kepler 36.[réf. nécessaire] كيبلر 36 بي (بالإنجليزية: Kepler-36b)‏ الذي يرمز له بالرمز KOI-277.02، هو كوكب خارج المجموعة الشمسية، في كوكبة الدجاجة (كوكبة)، يتبع Kepler-36. Kepler-36b is an exoplanet orbiting the star Kepler-36. This planet has the closest conjunction to Kepler-36c every 97 days. Its density is similar to that of iron. During their closest approach, Kepler-36b and Kepler-36c are located only 0.013 AU (about 1,900,000 km) from each other, which causes extreme transit-timing variations for both planets. Transit-timing variations caused by Kepler-36c are strong enough to put narrow constraints on Kepler-36b's mass. The close proximity of the planet to its host star combined with its relatively low mass caused the planet to lose all or most of its primordial hydrogen/helium envelope.
gold:hypernym
dbr:Exoplanet
prov:wasDerivedFrom
wikipedia-en:Kepler-36b?oldid=1046845250&ns=0
n16:density
6800.0
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13.83989
dbo:wikiPageLength
3714
dbo:density
6800.0
dbo:detectionMethod
Transit(Kepler Mission)
dbo:orbitalPeriod
1195766.496
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wikipedia-en:Kepler-36b
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dbr:Kepler-78b
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dbr:Kepler-36b
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dbr:List_of_stars_in_Cygnus
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dbr:Kepler-36b
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dbr:Kepler-36b