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Canis Major is a constellation in the southern celestial hemisphere. In the second century, it was included in Ptolemy 's 48 constellations, and is counted among the 88 modern constellations . Its name is Latin for "greater dog" in contrast to Canis Minor , the "lesser dog"; both figures are commonly represented as following the constellation ...
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Beta Canis Majoris (β Canis Majoris, abbreviated Beta CMa, β CMa), also named Mirzam / ˈ m ɜːr z əm /, [13] is a star in the southern constellation of Canis Major, the "Great Dog", located at a distance of about 500 light-years (150 parsecs) from the Sun. [1] In the modern constellation it lies at the position of the dog's front leg.
Zeta Canis Majoris, or ζ Canis Majoris, also named Furud / ˈ f jʊər ə d /, [14] is a binary star system in the southern constellation of Canis Major. This system has an apparent visual magnitude of +3.0, [ 2 ] making it one of the brighter stars in the constellation and hence readily visible to the naked eye.
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Artist's illustration of Wezen, a yellow supergiant 1,600 light-years away in the Canis Major constellation. Delta Canis Majoris is a supergiant of class F8. Its surface temperature is around 5,818 K, [12] and it is 14 to 15 times more massive than the Sun. Its absolute magnitude is −6.77, [8] and it lies around 1,600 light-years away. It is ...
The star system, appearing as one star, is deemed visible to the naked eye with its combined apparent visual magnitude of 4.41. [2] Based upon an annual parallax shift of 7.74 mas as seen from Earth, [1] this system is about 420 light years from the Sun, much further than Nu 1 and Nu 2 which appear nearby when seen from one point in the Solar System.
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