| http://dbpedia.org/ontology/abstract
|
Алиф аль Фаркадин (ζ UMi) — пятая по светимости звезда в созвездии Малой Медведицы.
, Alifa eller Zeta Ursae Minoris (ζ Ursae Mi … Alifa eller Zeta Ursae Minoris (ζ Ursae Minoris, förkortat Zeta UMi, ζ UMi), som är stjärnans Bayer-beteckning, är en ensam stjärna i mellersta delen av stjärnbilden Lilla björnen. Den har en skenbar magnitud av 4,28 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på en årlig parallaxförskjutning av ca 8,7 mas, beräknas den befinna sig på ett avstånd va ca 380 ljusår (115 parsek).ett avstånd va ca 380 ljusår (115 parsek).
, Zeta Ursae Minoris (ζ UMi) – gwiazda w gwiazdozbiorze Małej Niedźwiedzicy, odległa od Słońca o około 369 lat świetlnych.
, 작은곰자리 제타(ζ UMi)는 작은곰자리 방향에 있는 항성이다. 전통적으로 … 작은곰자리 제타(ζ UMi)는 작은곰자리 방향에 있는 항성이다. 전통적으로 불려오던 이름으로 아랍어 أخفى الفرقدين에서 유래한 '아크파 알 파카다인' 이 있다. 이 별은 A형 주계열성으로 겉보기 등급은 +4.28이다. 지구로부터 약 380 광년 떨어져 있다. 특이한 점은 제타별은 표면 온도가 8700 켈빈으로 분광형상 A형 왜성이지만 물리적 수치는 그보다 더 크고 밝아 질량은 태양의 3.4배, 밝기는 태양의 200배에 이른다. 이 별은 사실 거성으로 바뀌기 직전 상태이다. 방패자리 델타형 변광성일 가능성도 있다.실 거성으로 바뀌기 직전 상태이다. 방패자리 델타형 변광성일 가능성도 있다.
, Alifa al Farkadain (ζ Ursae Minoris / ζ UM … Alifa al Farkadain (ζ Ursae Minoris / ζ UMi / 16 Ursae Minoris) es una estrella en la constelación de la Osa Menor de magnitud aparente +4,28 que se encuentra a 376 años luz del Sistema Solar. Su nombre, de origen árabe, significa «el más tenue de los dos becerros/terneros», en contraposición a Anwar al Farkadain (η Ursae Minoris), «el más brillante de los dos becerros». Curiosamente Alifa al Farkadain es más brillante que Anwar al Farkadain. Alifa al Farkadain es una estrella blanca de tipo espectral A3Vn con una temperatura de 8700 K. Su luminosidad, 200 veces mayor que la del Sol, es unas dos magnitudes más brillante de lo que cabría esperar para una estrella blanca de la secuencia principal, por lo que se piensa que está en el límite de terminar la combustión de hidrógeno para convertirse en una estrella gigante. Su radio es 6,2 veces más grande que el radio solar y su masa se estima unas 3,4 veces mayor que la del Sol; hace 280 millones de años comenzó su vida como una estrella blanco-azulada de tipo B7. A diferencia del Sol, cuya velocidad de rotación es de 2 km/s, Alifa al Farkaidan tiene una velocidad de rotación mucho mayor, de al menos 206 km/s, completando un giro en menos de 1,5 días. Puede ser una estrella variable del tipo Delta Scuti, lo cual aún no ha sido confirmado. Scuti, lo cual aún no ha sido confirmado.
, こぐま座ζ星（こぐまざゼータせい、ζ Ursae Minoris、ζ UMi）は、こぐま座の恒星である。見かけの等級は4.29で、太陽系からはおよそ369光年離れた位置にある。変光星である可能性が指摘されているが、確定した変光星にはなっていない。
, Alifa al Farkadain (zeta Ursae Minoris) is een ster in het sterrenbeeld Kleine Beer (Ursa Minor). Het betreft een type A-hoofdreeksster die op het punt staat te evolueren naar een rode reus.
, Alifa al Farkadain (Zeta Ursae Minoris / ζ … Alifa al Farkadain (Zeta Ursae Minoris / ζ UMi / ζ Ursae Minoris) è una stella nella costellazione dell'Orsa Minore.Il nome Alifa al Farkadain deriva dall'arabo أخفى الفرقدين aḫfa al-farqadayn e significa "il più debole dei due vitelli"; il nome era stato originariamente applicato a Pherkad, in contrapposizione a Kochab, cui invece era stato applicato il nome di Anwar al Farkadain, dall'arabo أنور الفرقدين, "il più brillante dei due vitelli", nome che ora detiene Eta Ursae Minoris.", nome che ora detiene Eta Ursae Minoris.
, Zeta Ursae Minoris (Ahfa al Farkadain, 16 … Zeta Ursae Minoris (Ahfa al Farkadain, 16 Ursae Minoris) é uma estrela na direção da constelação de Ursa Minor. Possui uma ascensão reta de 15h 44m 03.46s e uma declinação de +77° 47′ 40.2″. Sua magnitude aparente é igual a 4.29. Considerando sua distância de 376 anos-luz em relação à Terra, sua magnitude absoluta é igual a −1.02. Pertence à classe espectral A3Vn.a −1.02. Pertence à classe espectral A3Vn.
, Zeta Ursae Minoris, which is Latinized fro … Zeta Ursae Minoris, which is Latinized from ζ Ursae Minoris, is a single star in the northern circumpolar constellation of Ursa Minor, forming the northernmost part of the bowl in this "little dipper" asterism. The star has a white hue and is faintly visible to the naked eye with an apparent visual magnitude of +4.28. It is located at a distance of approximately 369 light-years from the Sun based on parallax, but is drifting further closer with a radial velocity of about –13 km/s. The stellar classification of Zeta UMi is A3Vn, a notation that indicates this is an A-type main-sequence star with broad "nebulous" absorption lines in its spectrum due to rapid rotation. Based on photometric data, some light variability was suspected by R. A. Baker in 1926, and it may be a Delta Scuti variable. It is a pulsating variable star, with a period of 15.8 hours, and it also undergoes eclipses. The star is spinning with a projected rotational velocity of 210 km/s, which is creating an equatorial bulge that is estimated to be 10% larger than the polar radius. Zeta Ursae Minoris is about 180 million years old with 6.15 times the radius of the Sun. It is radiating 227 times the luminosity of the Sun from its photosphere at an effective temperature of 8,720 K. This anomalously high temperature and an absolute magnitude of –0.98 may indicate it is on the verge of evolving into a giant star. An infrared excess has been detected from an orbiting circumstellar disk. A black body fit to the data yields a mean dust temperature of 160 K and an orbital radius of 42.5 AU. In some Arabic star charts it is listed as أخفى الفرقدين ʼakhfā al-farqadayn, meaning "the dimmer of the two calves", and paired with η Ursae Minoris as ʼanwar al-farqadayn, "the brighter of the two calves". The names may originally refer to a pair of Ibexes, and are more properly applied to γ UMi and β UMi, respectively, the brighter two stars in the rectangle of Ursa Minor. two stars in the rectangle of Ursa Minor.
, 小熊座ζ，又名BD+78 527，HD 142105、SAO 8328、HR 5903，是小熊座的一颗恒星，视星等为4.32，位于銀經112.68，銀緯35.66，其B1900.0坐标为赤經15h 47m 37.2s，赤緯+78° 35.66′ 8″,7.9太阳直径。
, Zeta Ursae Minoris (ζ UMi, ζ Ursae Minoris … Zeta Ursae Minoris (ζ UMi, ζ Ursae Minoris, Zêta Ursae Minoris), parfois nommée Akhfa Al Farkadaïn, est une étoile située à environ 380 années-lumière de la Terre dans la constellation de la Petite Ourse. Bien que classée comme une étoile blanche de la séquence principale, Zeta UMi est en fait sur le point de devenir une étoile géante. Sa masse vaut 3,4 fois celle du Soleil. Elle est environ 200 fois plus lumineuse que le Soleil et sa température de surface est d'environ 8 700 K. Zeta UMi pourrait également être une variable de type Delta Scuti.ent être une variable de type Delta Scuti.
|
| http://dbpedia.org/ontology/thumbnail
|
http://commons.wikimedia.org/wiki/Special:FilePath/Ursa_Minor_constellation_map.svg?width=300 +
|
| http://dbpedia.org/ontology/wikiPageID
|
2718156
|
| http://dbpedia.org/ontology/wikiPageLength
|
10421
|
| http://dbpedia.org/ontology/wikiPageRevisionID
|
1116663999
|
| http://dbpedia.org/ontology/wikiPageWikiLink
|
http://dbpedia.org/resource/Circumstellar_disk +
, http://dbpedia.org/resource/Absorption_line +
, http://dbpedia.org/resource/Radial_velocity +
, http://dbpedia.org/resource/Stellar_evolution +
, http://dbpedia.org/resource/Stellar_spectrum +
, http://dbpedia.org/resource/Stellar_classification +
, http://dbpedia.org/resource/Radius_of_the_Sun +
, http://dbpedia.org/resource/Category:Flamsteed_objects +
, http://dbpedia.org/resource/Absolute_magnitude +
, http://dbpedia.org/resource/Variable_star +
, http://dbpedia.org/resource/Category:Delta_Scuti_variables +
, http://dbpedia.org/resource/Asterism_%28astronomy%29 +
, http://dbpedia.org/resource/Stellar_parallax +
, http://dbpedia.org/resource/Category:Durchmusterung_objects +
, http://dbpedia.org/resource/Light-year +
, http://dbpedia.org/resource/Category:Bayer_objects +
, http://dbpedia.org/resource/%CE%97_Ursae_Minoris +
, http://dbpedia.org/resource/Photometry_%28astronomy%29 +
, http://dbpedia.org/resource/Eclipsing_binary +
, http://dbpedia.org/resource/Category:Bright_Star_Catalogue_objects +
, http://dbpedia.org/resource/Giant_star +
, http://dbpedia.org/resource/Category:Hipparcos_objects +
, http://dbpedia.org/resource/Romanization_of_Greek +
, http://dbpedia.org/resource/Sun +
, http://dbpedia.org/resource/Ursa_Minor +
, http://dbpedia.org/resource/%CE%92_UMi +
, http://dbpedia.org/resource/Photosphere +
, http://dbpedia.org/resource/Infrared_excess +
, http://dbpedia.org/resource/Black_body +
, http://dbpedia.org/resource/Star +
, http://dbpedia.org/resource/Category:Circumstellar_disks +
, http://dbpedia.org/resource/A-type_main-sequence_star +
, http://dbpedia.org/resource/Category:A-type_main-sequence_stars +
, http://dbpedia.org/resource/Category:Suspected_variables +
, http://dbpedia.org/resource/Luminosity_of_the_Sun +
, http://dbpedia.org/resource/Projected_rotational_velocity +
, http://dbpedia.org/resource/Apparent_visual_magnitude +
, http://dbpedia.org/resource/Effective_temperature +
, http://dbpedia.org/resource/Robert_Horace_Baker +
, http://dbpedia.org/resource/Delta_Scuti_variable +
, http://dbpedia.org/resource/%CE%93_UMi +
, http://dbpedia.org/resource/File:ZetaUMiLightCurve.png +
, http://dbpedia.org/resource/Category:Ursa_Minor_%28constellation%29 +
, http://dbpedia.org/resource/Circumpolar_constellation +
, http://dbpedia.org/resource/Equatorial_bulge +
, http://dbpedia.org/resource/Category:Henry_Draper_Catalogue_objects +
|
| http://dbpedia.org/property/absmagV
|
−0.98
|
| http://dbpedia.org/property/ageMyr
|
180
|
| http://dbpedia.org/property/appmagV
|
+4.29
|
| http://dbpedia.org/property/class
|
A3Vn
|
| http://dbpedia.org/property/constell
|
http://dbpedia.org/resource/Ursa_Minor +
|
| http://dbpedia.org/property/epoch
|
J2000
|
| http://dbpedia.org/property/luminosity
|
227
|
| http://dbpedia.org/property/mass
|
~3.4
|
| http://dbpedia.org/property/pError
|
0.12
|
| http://dbpedia.org/property/parallax
|
8.84
|
| http://dbpedia.org/property/propMoDec
|
−1.99
|
| http://dbpedia.org/property/propMoRa
|
19.91
|
| http://dbpedia.org/property/radius
|
6.15
|
| http://dbpedia.org/property/rotationalVelocity
|
210
|
| http://dbpedia.org/property/temperature
|
8720
|
| http://dbpedia.org/property/uB
|
+0.05
|
| http://dbpedia.org/property/variable
|
Suspected δ Sct
|
| http://dbpedia.org/property/wikiPageUsesTemplate
|
http://dbpedia.org/resource/Template:Location_mark +
, http://dbpedia.org/resource/Template:Starbox_image +
, http://dbpedia.org/resource/Template:Stars_of_Ursa_Minor +
, http://dbpedia.org/resource/Template:Odlist +
, http://dbpedia.org/resource/Template:Short_description +
, http://dbpedia.org/resource/Template:Val +
, http://dbpedia.org/resource/Template:Starbox_end +
, http://dbpedia.org/resource/Template:Starbox_character +
, http://dbpedia.org/resource/Template:Starbox_reference +
, http://dbpedia.org/resource/Template:RA +
, http://dbpedia.org/resource/Template:DEC +
, http://dbpedia.org/resource/Template:Starbox_astrometry +
, http://dbpedia.org/resource/Template:Starbox_detail +
, http://dbpedia.org/resource/Template:Starbox_observe +
, http://dbpedia.org/resource/Template:Reflist +
, http://dbpedia.org/resource/Template:Starbox_begin +
, http://dbpedia.org/resource/Template:Starbox_catalog +
|
| http://purl.org/dc/terms/subject
|
http://dbpedia.org/resource/Category:Circumstellar_disks +
, http://dbpedia.org/resource/Category:Durchmusterung_objects +
, http://dbpedia.org/resource/Category:Bayer_objects +
, http://dbpedia.org/resource/Category:Ursa_Minor_%28constellation%29 +
, http://dbpedia.org/resource/Category:Bright_Star_Catalogue_objects +
, http://dbpedia.org/resource/Category:Hipparcos_objects +
, http://dbpedia.org/resource/Category:Delta_Scuti_variables +
, http://dbpedia.org/resource/Category:Suspected_variables +
, http://dbpedia.org/resource/Category:A-type_main-sequence_stars +
, http://dbpedia.org/resource/Category:Henry_Draper_Catalogue_objects +
, http://dbpedia.org/resource/Category:Flamsteed_objects +
|
| http://purl.org/linguistics/gold/hypernym
|
http://dbpedia.org/resource/Star +
|
| http://www.w3.org/ns/prov#wasDerivedFrom
|
http://en.wikipedia.org/wiki/Zeta_Ursae_Minoris?oldid=1116663999&ns=0 +
|
| http://xmlns.com/foaf/0.1/depiction
|
http://commons.wikimedia.org/wiki/Special:FilePath/Ursa_Minor_constellation_map.svg +
, http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg +
, http://commons.wikimedia.org/wiki/Special:FilePath/ZetaUMiLightCurve.png +
|
| http://xmlns.com/foaf/0.1/isPrimaryTopicOf
|
http://en.wikipedia.org/wiki/Zeta_Ursae_Minoris +
|
| http://xmlns.com/foaf/0.1/name
|
ζ Ursae Minoris
|
| owl:sameAs |
http://sv.dbpedia.org/resource/Alifa +
, http://pt.dbpedia.org/resource/Zeta_Ursae_Minoris +
, http://yago-knowledge.org/resource/Zeta_Ursae_Minoris +
, http://nl.dbpedia.org/resource/Alifa_al_Farkadain +
, http://ru.dbpedia.org/resource/%D0%94%D0%B7%D0%B5%D1%82%D0%B0_%D0%9C%D0%B0%D0%BB%D0%BE%D0%B9_%D0%9C%D0%B5%D0%B4%D0%B2%D0%B5%D0%B4%D0%B8%D1%86%D1%8B +
, https://global.dbpedia.org/id/Qz5K +
, http://ast.dbpedia.org/resource/Alifa_al_Farkadain +
, http://ja.dbpedia.org/resource/%E3%81%93%E3%81%90%E3%81%BE%E5%BA%A7%E3%82%BC%E3%83%BC%E3%82%BF%E6%98%9F +
, http://es.dbpedia.org/resource/Alifa_al_Farkadain +
, http://rdf.freebase.com/ns/m.07zt5m +
, http://zh.dbpedia.org/resource/%E5%8B%BE%E9%99%B3%E5%9B%9B +
, http://ce.dbpedia.org/resource/%D0%A7%D1%83%D1%85%D1%87%D0%B0%D1%85%D1%8C%D0%B5%D1%80%D0%B8%D0%BD_%D0%B4%D0%B7%D0%B5%D1%82%D0%B0 +
, http://ko.dbpedia.org/resource/%EC%9E%91%EC%9D%80%EA%B3%B0%EC%9E%90%EB%A6%AC_%EC%A0%9C%ED%83%80 +
, http://fa.dbpedia.org/resource/%D8%A7%D8%AE%D9%81%DB%8C%E2%80%8C%D8%A7%D9%84%D9%81%D8%B1%D9%82%D8%AF%DB%8C%D9%86 +
, http://it.dbpedia.org/resource/Alifa_al_Farkadain +
, http://www.wikidata.org/entity/Q14065 +
, http://fr.dbpedia.org/resource/Zeta_Ursae_Minoris +
, http://dbpedia.org/resource/Zeta_Ursae_Minoris +
, http://pl.dbpedia.org/resource/Zeta_Ursae_Minoris +
|
| rdf:type |
http://dbpedia.org/class/yago/WikicatBayerObjects +
, http://dbpedia.org/class/yago/CelestialBody109239740 +
, http://dbpedia.org/ontology/CelestialBody +
, http://dbpedia.org/ontology/Location +
, http://dbpedia.org/ontology/Place +
, http://dbpedia.org/ontology/Star +
, http://dbpedia.org/class/yago/Object100002684 +
, http://dbpedia.org/class/yago/Whole100003553 +
, http://dbpedia.org/class/yago/WikicatA-typeMain-sequenceStars +
, http://dbpedia.org/class/yago/WikicatA-typeStars +
, http://dbpedia.org/class/yago/WikicatStars +
, http://dbpedia.org/class/yago/Star109444100 +
, http://dbpedia.org/class/yago/PhysicalEntity100001930 +
, http://dbpedia.org/class/yago/NaturalObject100019128 +
, http://schema.org/Place +
|
| rdfs:comment |
Zeta Ursae Minoris (Ahfa al Farkadain, 16 … Zeta Ursae Minoris (Ahfa al Farkadain, 16 Ursae Minoris) é uma estrela na direção da constelação de Ursa Minor. Possui uma ascensão reta de 15h 44m 03.46s e uma declinação de +77° 47′ 40.2″. Sua magnitude aparente é igual a 4.29. Considerando sua distância de 376 anos-luz em relação à Terra, sua magnitude absoluta é igual a −1.02. Pertence à classe espectral A3Vn.a −1.02. Pertence à classe espectral A3Vn.
, Zeta Ursae Minoris, which is Latinized fro … Zeta Ursae Minoris, which is Latinized from ζ Ursae Minoris, is a single star in the northern circumpolar constellation of Ursa Minor, forming the northernmost part of the bowl in this "little dipper" asterism. The star has a white hue and is faintly visible to the naked eye with an apparent visual magnitude of +4.28. It is located at a distance of approximately 369 light-years from the Sun based on parallax, but is drifting further closer with a radial velocity of about –13 km/s. with a radial velocity of about –13 km/s.
, 小熊座ζ，又名BD+78 527，HD 142105、SAO 8328、HR 5903，是小熊座的一颗恒星，视星等为4.32，位于銀經112.68，銀緯35.66，其B1900.0坐标为赤經15h 47m 37.2s，赤緯+78° 35.66′ 8″,7.9太阳直径。
, Алиф аль Фаркадин (ζ UMi) — пятая по светимости звезда в созвездии Малой Медведицы.
, Alifa al Farkadain (ζ Ursae Minoris / ζ UM … Alifa al Farkadain (ζ Ursae Minoris / ζ UMi / 16 Ursae Minoris) es una estrella en la constelación de la Osa Menor de magnitud aparente +4,28 que se encuentra a 376 años luz del Sistema Solar. Su nombre, de origen árabe, significa «el más tenue de los dos becerros/terneros», en contraposición a Anwar al Farkadain (η Ursae Minoris), «el más brillante de los dos becerros». Curiosamente Alifa al Farkadain es más brillante que Anwar al Farkadain.n es más brillante que Anwar al Farkadain.
, Alifa al Farkadain (zeta Ursae Minoris) is een ster in het sterrenbeeld Kleine Beer (Ursa Minor). Het betreft een type A-hoofdreeksster die op het punt staat te evolueren naar een rode reus.
, Alifa al Farkadain (Zeta Ursae Minoris / ζ … Alifa al Farkadain (Zeta Ursae Minoris / ζ UMi / ζ Ursae Minoris) è una stella nella costellazione dell'Orsa Minore.Il nome Alifa al Farkadain deriva dall'arabo أخفى الفرقدين aḫfa al-farqadayn e significa "il più debole dei due vitelli"; il nome era stato originariamente applicato a Pherkad, in contrapposizione a Kochab, cui invece era stato applicato il nome di Anwar al Farkadain, dall'arabo أنور الفرقدين, "il più brillante dei due vitelli", nome che ora detiene Eta Ursae Minoris.", nome che ora detiene Eta Ursae Minoris.
, 작은곰자리 제타(ζ UMi)는 작은곰자리 방향에 있는 항성이다. 전통적으로 … 작은곰자리 제타(ζ UMi)는 작은곰자리 방향에 있는 항성이다. 전통적으로 불려오던 이름으로 아랍어 أخفى الفرقدين에서 유래한 '아크파 알 파카다인' 이 있다. 이 별은 A형 주계열성으로 겉보기 등급은 +4.28이다. 지구로부터 약 380 광년 떨어져 있다. 특이한 점은 제타별은 표면 온도가 8700 켈빈으로 분광형상 A형 왜성이지만 물리적 수치는 그보다 더 크고 밝아 질량은 태양의 3.4배, 밝기는 태양의 200배에 이른다. 이 별은 사실 거성으로 바뀌기 직전 상태이다. 방패자리 델타형 변광성일 가능성도 있다.실 거성으로 바뀌기 직전 상태이다. 방패자리 델타형 변광성일 가능성도 있다.
, Zeta Ursae Minoris (ζ UMi, ζ Ursae Minoris … Zeta Ursae Minoris (ζ UMi, ζ Ursae Minoris, Zêta Ursae Minoris), parfois nommée Akhfa Al Farkadaïn, est une étoile située à environ 380 années-lumière de la Terre dans la constellation de la Petite Ourse. Bien que classée comme une étoile blanche de la séquence principale, Zeta UMi est en fait sur le point de devenir une étoile géante. Sa masse vaut 3,4 fois celle du Soleil. Elle est environ 200 fois plus lumineuse que le Soleil et sa température de surface est d'environ 8 700 K. Zeta UMi pourrait également être une variable de type Delta Scuti.ent être une variable de type Delta Scuti.
, Zeta Ursae Minoris (ζ UMi) – gwiazda w gwiazdozbiorze Małej Niedźwiedzicy, odległa od Słońca o około 369 lat świetlnych.
, Alifa eller Zeta Ursae Minoris (ζ Ursae Mi … Alifa eller Zeta Ursae Minoris (ζ Ursae Minoris, förkortat Zeta UMi, ζ UMi), som är stjärnans Bayer-beteckning, är en ensam stjärna i mellersta delen av stjärnbilden Lilla björnen. Den har en skenbar magnitud av 4,28 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på en årlig parallaxförskjutning av ca 8,7 mas, beräknas den befinna sig på ett avstånd va ca 380 ljusår (115 parsek).ett avstånd va ca 380 ljusår (115 parsek).
, こぐま座ζ星（こぐまざゼータせい、ζ Ursae Minoris、ζ UMi）は、こぐま座の恒星である。見かけの等級は4.29で、太陽系からはおよそ369光年離れた位置にある。変光星である可能性が指摘されているが、確定した変光星にはなっていない。
|
| rdfs:label |
Zeta Ursae Minoris
, Дзета Малой Медведицы
, Alifa al Farkadain
, 작은곰자리 제타
, Alifa
, 勾陳四
, こぐま座ゼータ星
|
