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  2. Canis Major - Wikipedia

    en.wikipedia.org/wiki/Canis_Major

    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 ...

  3. File:Canis Major constellation map.svg - Wikipedia

    en.wikipedia.org/wiki/File:Canis_Major...

    The original can be viewed here: Canis major constellation map.png: . Modifications made by Kxx. I, the copyright holder of this work, hereby publish it under the ...

  4. VY Canis Majoris - Wikipedia

    en.wikipedia.org/wiki/VY_Canis_Majoris

    VY Canis Majoris (abbreviated to VY CMa) is an extreme oxygen-rich red hypergiant or red supergiant (O-rich RHG or RSG) and pulsating variable star 1.2 kiloparsecs (3,900 light-years) from the Solar System in the slightly southern constellation of Canis Major.

  5. Delta Canis Majoris - Wikipedia

    en.wikipedia.org/wiki/Delta_Canis_Majoris

    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 ...

  6. Beta Canis Majoris - Wikipedia

    en.wikipedia.org/wiki/Beta_Canis_Majoris

    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.

  7. Messier 41 - Wikipedia

    en.wikipedia.org/wiki/Messier_41

    Messier 41 (also known as M41 or NGC 2287) is an open cluster in the constellation Canis Major.It is sometimes referred to as the Little Beehive Cluster. [4] It was discovered by Giovanni Batista Hodierna before 1654 and was perhaps known to Aristotle about 325 BC. [5]

  8. Eta Canis Majoris - Wikipedia

    en.wikipedia.org/wiki/Eta_Canis_Majoris

    Eta Canis Majoris (η Canis Majoris, abbreviated Eta CMa, η CMa), also named Aludra / ə ˈ l uː d r ə, ə ˈ lj uː d r ə /, [10] is a star in the constellation of Canis Major.Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.

  9. FN Canis Majoris - Wikipedia

    en.wikipedia.org/wiki/FN_Canis_Majoris

    FN Canis Majoris is a binary star [4] system in the southern constellation Canis Major, near the northern constellation border with Monoceros. It is dimly visible to the naked eye with a combined apparent visual magnitude of 5.41. [ 3 ]