Kepler-90h (original) (raw)

Property Value
dbo:Planet/orbitalPeriod 3.7000000000000005E-4
dbo:Planet/temperature 292.0
dbo:abstract كيبلر 90 إتش (بالإنجليزية: Kepler-90h)‏ هو كوكب خارج المجموعة الشمسية، في كوكبة التنين، يتبع Kepler-90. (ar) Kepler-90h (also known by its Kepler Object of Interest designation KOI-351.01) is an exoplanet orbiting within the habitable zone of the early G-type main sequence star Kepler-90, the outermost of eight such planets discovered by NASA's Kepler spacecraft. It is located about 2,840 light-years (870 parsecs), from Earth in the constellation Draco. The exoplanet was found by using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. (en) Kepler-90h es un planeta que orbita a la estrella Kepler-90 en la constelación de in Draco. (es) Kepler-90 h est une exoplanète orbitant autour de l'étoile Kepler-90, elle a été découverte en 2013. (fr) ケプラー90h(英語:Kepler-90h)とは地球からりゅう座の方向に約2500光年離れたところにある太陽よりやや大きいG型主系列星、ケプラー90を公転している8つの太陽系外惑星の内のひとつである。ケプラー宇宙望遠鏡は恒星面を惑星が通過することで恒星の光度がわずかに減光し、その減光から惑星の存在を間接的に検出するトランジット法で発見した。 (ja) Kepler-90 h è un pianeta extrasolare che orbita attorno alla stella Kepler-90, una nana gialla lievemente più massiccia del Sole distante circa 2544 anni luce dal sistema solare. Il pianeta è il più esterno e massiccio dei sette pianeti scoperti attorno alla stella con il metodo del transito dal telescopio spaziale Kepler. (it) Kepler-90h (também conhecido pela sua designação de Kepler Object of Interest KOI-351.01) é um exoplaneta orbitando dentro da zona habitável da jovem estrela da sequência principal tipo-G Kepler-90, o mais externo dos sete planetas descobertos pela sonda Kepler da NASA. Ele está localizado a cerca de 2,545 de anos-luz da Terra, na constelação de Draco. O exoplaneta foi encontrado usando-se o método de trânsito, em que o efeito de escurecimento que um planeta faz ao cruzar na frente de sua estrela é medido. (pt) Kepler-90 h (также известна, как KOI-351.01) — экзопланета в системе Kepler-90. Восьмая, самая дальняя от звезды и самая крупная планета в системе. Система расположена в созвездии Дракона на расстоянии 2840 световых лет (870 парсек) от Земли. Открыта транзитным методом в ноябре 2013 года. (ru) 克卜勒90h(Kepler-90h)是環繞天龍座恆星克卜勒90的太陽系外行星,發現於2013年11月。 (zh)
dbo:detectionMethod Transit
dbo:discovered 2013-11-12 (xsd:date)
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dbo:temperature 292.000000 (xsd:double)
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rdfs:comment كيبلر 90 إتش (بالإنجليزية: Kepler-90h)‏ هو كوكب خارج المجموعة الشمسية، في كوكبة التنين، يتبع Kepler-90. (ar) Kepler-90h (also known by its Kepler Object of Interest designation KOI-351.01) is an exoplanet orbiting within the habitable zone of the early G-type main sequence star Kepler-90, the outermost of eight such planets discovered by NASA's Kepler spacecraft. It is located about 2,840 light-years (870 parsecs), from Earth in the constellation Draco. The exoplanet was found by using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. (en) Kepler-90h es un planeta que orbita a la estrella Kepler-90 en la constelación de in Draco. (es) Kepler-90 h est une exoplanète orbitant autour de l'étoile Kepler-90, elle a été découverte en 2013. (fr) ケプラー90h(英語:Kepler-90h)とは地球からりゅう座の方向に約2500光年離れたところにある太陽よりやや大きいG型主系列星、ケプラー90を公転している8つの太陽系外惑星の内のひとつである。ケプラー宇宙望遠鏡は恒星面を惑星が通過することで恒星の光度がわずかに減光し、その減光から惑星の存在を間接的に検出するトランジット法で発見した。 (ja) Kepler-90 h è un pianeta extrasolare che orbita attorno alla stella Kepler-90, una nana gialla lievemente più massiccia del Sole distante circa 2544 anni luce dal sistema solare. Il pianeta è il più esterno e massiccio dei sette pianeti scoperti attorno alla stella con il metodo del transito dal telescopio spaziale Kepler. (it) Kepler-90h (também conhecido pela sua designação de Kepler Object of Interest KOI-351.01) é um exoplaneta orbitando dentro da zona habitável da jovem estrela da sequência principal tipo-G Kepler-90, o mais externo dos sete planetas descobertos pela sonda Kepler da NASA. Ele está localizado a cerca de 2,545 de anos-luz da Terra, na constelação de Draco. O exoplaneta foi encontrado usando-se o método de trânsito, em que o efeito de escurecimento que um planeta faz ao cruzar na frente de sua estrela é medido. (pt) Kepler-90 h (также известна, как KOI-351.01) — экзопланета в системе Kepler-90. Восьмая, самая дальняя от звезды и самая крупная планета в системе. Система расположена в созвездии Дракона на расстоянии 2840 световых лет (870 парсек) от Земли. Открыта транзитным методом в ноябре 2013 года. (ru) 克卜勒90h(Kepler-90h)是環繞天龍座恆星克卜勒90的太陽系外行星,發現於2013年11月。 (zh)
rdfs:label كيبلر-90h (ar) Kepler-90h (es) Kepler-90 h (fr) Kepler-90 h (it) Kepler-90h (en) ケプラー90h (ja) Kepler-90h (pt) Kepler-90 h (ru) 开普勒90h (zh)
rdfs:seeAlso dbr:Habitability_of_natural_satellites
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