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30 Camelopardalis, som är stjärnans Flamst … 30 Camelopardalis, som är stjärnans Flamsteed-beteckning, är en ensam stjärna i den sydvästra delen av stjärnbilden Giraffen. Den har en skenbar magnitud på ca 6,14 och är mycket svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 6,1 mas, beräknas den befinna sig på ett avstånd på ca 539 ljusår (ca 165 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 12 km/s.liocentrisk radialhastighet på ca 12 km/s.
, 30 Camelopardalis is a star in the norther … 30 Camelopardalis is a star in the northern circumpolar constellation of Camelopardalis, located about 539 light years away from the Sun based on parallax. It can be viewed with the naked eye in good seeing conditions, appearing as a dim, white-hued point of light with an apparent visual magnitude of 6.14. This is most likely a slowly rotating A-type main-sequence star with a stellar classification of A0Vs, which indicates it is generating energy via hydrogen fusion at its core. It is moving further from the Earth with a heliocentric radial velocity of +12 km/s. heliocentric radial velocity of +12 km/s.
, 鹿豹座30，又名BD+58 863，HD 38831、SAO 25419、HR 2006，是鹿豹座的一颗恒星，视星等为6.14，位于銀經154.15，銀緯15.88，其B1900.0坐标为赤經5h 43m 28.3s，赤緯+58° 15.88′ 7″。
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| rdfs:comment |
30 Camelopardalis, som är stjärnans Flamst … 30 Camelopardalis, som är stjärnans Flamsteed-beteckning, är en ensam stjärna i den sydvästra delen av stjärnbilden Giraffen. Den har en skenbar magnitud på ca 6,14 och är mycket svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 6,1 mas, beräknas den befinna sig på ett avstånd på ca 539 ljusår (ca 165 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 12 km/s.liocentrisk radialhastighet på ca 12 km/s.
, 30 Camelopardalis is a star in the norther … 30 Camelopardalis is a star in the northern circumpolar constellation of Camelopardalis, located about 539 light years away from the Sun based on parallax. It can be viewed with the naked eye in good seeing conditions, appearing as a dim, white-hued point of light with an apparent visual magnitude of 6.14. This is most likely a slowly rotating A-type main-sequence star with a stellar classification of A0Vs, which indicates it is generating energy via hydrogen fusion at its core. It is moving further from the Earth with a heliocentric radial velocity of +12 km/s. heliocentric radial velocity of +12 km/s.
, 鹿豹座30，又名BD+58 863，HD 38831、SAO 25419、HR 2006，是鹿豹座的一颗恒星，视星等为6.14，位于銀經154.15，銀緯15.88，其B1900.0坐标为赤經5h 43m 28.3s，赤緯+58° 15.88′ 7″。
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八穀增十八
, 30 Camelopardalis
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