16 Puppis
http://dbpedia.org/resource/16_Puppis an entity of type: Thing
16 Puppis è una stella bianco-azzurra nella sequenza principale di magnitudine 4,39 situata nella costellazione della Poppa. Dista 473 anni luce dal sistema solare.
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16 Puppis (16 Pup), som är stjärnans Flamsteedbeteckning, är en misstänkt astrometrisk dubbelstjärna belägen i den norra delen av stjärnbilden Akterskeppet. Den har en skenbar magnitud på 4,40 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 7,0 mas, beräknas den befinna sig på ett avstånd på ca 470 ljusår (ca 143 parsek) från solen.
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船尾座16，又名BD-18 2190，HD 67797、SAO 153890、HR 3192，是船尾座的一颗恒星，视星等为4.4，位于銀經239.04，銀緯7.4，其B1900.0坐标为赤經8h 4m 33.7s，赤緯-18° 7.4′ 8″。
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16 Puppis is a suspected astrometric binary star system in the southern constellation of Puppis, and is located in the northernmost part of its constellation, almost due north of the bright star Rho Puppis, and east of Canis Major. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 4.40. The star is located is approximately 465 light years away from the Sun based on parallax. It was the brightest star in Officina Typographica, an obsolete constellation.
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16 Puppis
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16 Puppis
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16 Puppis
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弧矢增十三
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16 Puppis
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B5 V or B5 IV
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J2000
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16 Puppis is a suspected astrometric binary star system in the southern constellation of Puppis, and is located in the northernmost part of its constellation, almost due north of the bright star Rho Puppis, and east of Canis Major. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 4.40. The star is located is approximately 465 light years away from the Sun based on parallax. It was the brightest star in Officina Typographica, an obsolete constellation. The visible member is a B-type main-sequence star with a stellar classification of B5 V, according to N. Houk and M. Smith-Moore (1978). Earlier, Hoffleit et al. (1964) had listed a class of B5 IV, suggesting a more evolved subgiant star. It is spinning rapidly, which is creating an equatorial bulge that is 6% larger than the polar radius. The star is radiating 836 times the luminosity of the Sun from its photosphere at an effective temperature of 16,680 K.
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16 Puppis è una stella bianco-azzurra nella sequenza principale di magnitudine 4,39 situata nella costellazione della Poppa. Dista 473 anni luce dal sistema solare.
rdf:langString
16 Puppis (16 Pup), som är stjärnans Flamsteedbeteckning, är en misstänkt astrometrisk dubbelstjärna belägen i den norra delen av stjärnbilden Akterskeppet. Den har en skenbar magnitud på 4,40 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 7,0 mas, beräknas den befinna sig på ett avstånd på ca 470 ljusår (ca 143 parsek) från solen.
rdf:langString
船尾座16，又名BD-18 2190，HD 67797、SAO 153890、HR 3192，是船尾座的一颗恒星，视星等为4.4，位于銀經239.04，銀緯7.4，其B1900.0坐标为赤經8h 4m 33.7s，赤緯-18° 7.4′ 8″。
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7214