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3 Camelopardalis is a spectroscopic and visual binary in the constellation Camelopardalis. It is approximately 496 light years from Earth. 3 Camelopardalis is a visual binary with the two components separated by 3.7". The brighter of the pair is also a single-lined spectroscopic binary with an orbital period of 121 days. The spectroscopic companion has not been observed directly and its cannot be detected in the spectrum. It is inferred on the basis of radial velocity variations in its brighter companion. Assuming a circular orbit, it has a mass of 2.37 M☉.

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  • 3 Camelopardalis (en)
  • 3 Camelopardalis (sv)
  • 天船增七 (zh)
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  • 3 Camelopardalis, som är stjärnans Flamsteed-beteckning, är en spektroskopisk dubbelstjärna i den sydvästra delen av stjärnbilden Giraffen. Den har en genomsnittlig skenbar magnitud på ca 5,07 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 7,7 mas, beräknas den befinna sig på ett avstånd på ca 420 ljusår (ca 130 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -41 km/s. (sv)
  • 鹿豹座3,又名BD+52 865,HD 29317、SAO 24743、HR 1467,是鹿豹座的一颗恒星,视星等为5.05,位于銀經153.32,銀緯4.26,其B1900.0坐标为赤經4h 32m 1.9s,赤緯+52° 4.26′ 49″。 (zh)
  • 3 Camelopardalis is a spectroscopic and visual binary in the constellation Camelopardalis. It is approximately 496 light years from Earth. 3 Camelopardalis is a visual binary with the two components separated by 3.7". The brighter of the pair is also a single-lined spectroscopic binary with an orbital period of 121 days. The spectroscopic companion has not been observed directly and its cannot be detected in the spectrum. It is inferred on the basis of radial velocity variations in its brighter companion. Assuming a circular orbit, it has a mass of 2.37 M☉. (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/3CamLightCurve.png
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