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16 Camelopardalis is a single star in the northern circumpolar constellation Camelopardalis, located 348 light years away from the Sun as determined from parallax measurements. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 5.28. This object is moving further from the Earth with a heliocentric radial velocity of around 12 km/s. An infrared excess indicates it has a dusty debris disk with a mean temperature of 120 K orbiting at a distance of 52 AU from the star. This disk has a combined mass equal to 2.1% the mass of the Earth.

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  • 16 de la Girafa (ca)
  • 16 Camelopardalis (en)
  • 16 Camelopardalis (es)
  • 16 Camelopardalis (sv)
  • 八穀增十一 (zh)
rdfs:comment
  • 16 de la Girafa (16 Camelopardalis) és un estel situat a la constel·lació de la Girafa. Té magnitud aparent +5'25 i s'hi troba a 336 anys llum del Sistema Solar. (ca)
  • 16 Camelopardalis (16 Cam)​ es una estrella situada en la constelación de Camelopardalis, la jirafa.Tiene magnitud aparente +5,25 y se encuentra a 336 años luz del Sistema Solar. (es)
  • 16 Camelopardalis, som är stjärnans Flamsteed-beteckning, är en ensam stjärna i den sydvästra delen av stjärnbilden Giraffen. Den har en skenbar magnitud på ca 5,28 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 9,7 mas, beräknas den befinna sig på ett avstånd på ca 336 ljusår (ca 104 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 12 km/s. (sv)
  • 鹿豹座16,又名BD+57 879,HD 34787、SAO 25161、HR 1751,是鹿豹座的一颗恒星,视星等为5.28,位于銀經153.49,銀緯11.88,其B1900.0坐标为赤經5h 14m 54.2s,赤緯+57° 11.88′ 50″。 (zh)
  • 16 Camelopardalis is a single star in the northern circumpolar constellation Camelopardalis, located 348 light years away from the Sun as determined from parallax measurements. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 5.28. This object is moving further from the Earth with a heliocentric radial velocity of around 12 km/s. An infrared excess indicates it has a dusty debris disk with a mean temperature of 120 K orbiting at a distance of 52 AU from the star. This disk has a combined mass equal to 2.1% the mass of the Earth. (en)
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absmag v
age myr
appmag v
b-v
  • −0.03 (en)
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  • A0Vn (en)
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