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Nu1 Canis Majoris
Binary star system in the constellation Canis Major From Wikipedia, the free encyclopedia
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Nu1 Canis Majoris is a binary star in the constellation Canis Major. Its name is a Bayer designation that is Latinized from ν1 Canis Majoris, and abbreviated Nu1 CMa or ν1 CMa. This system is visible to the naked eye as a point of light with an apparent visual magnitude of 5.7.[2] Based on parallax shift of 12.366 mas as seen from Earth orbit,[1] this system is approximately 264 light years from the Sun. It is drifting further away with a line of sight velocity of +26 km/s.[2]
As of 2011, the pair had an angular separation of 17.29 arc seconds along a position angle of 264.2°.[7] The yellow hued magnitude 5.87[3] primary, component A, is an evolved G-type giant star with a stellar classification of G8 III.[3] It is an estimated 3[2] billion years old and has 1.4[2] times the mass of the Sun. Having exhausted the supply of hydrogen at its core, it has expanded to 7 times the Sun's radius[1] and is radiating 8 times the luminosity of the Sun from its photosphere at an effective temperature of 6,091 K.[2]
The magnitude 7.61[3] companion, component B, is a yellow-white hued F-type main sequence/subgiant hybrid with a class of F3 IV-V.[3]
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