Butterfly Cluster
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The Butterfly Cluster (also known as Messier Object 6 or NGC 6405) is an open cluster in the constellation Scorpius. It was discovered by Giovanni Batista Hodierna before 1654 and catalogued by Charles Messier in 1764 as number 6 in his catalogue of comet-like objects.
Estimates of the cluster's distance have varied over the years with a mean value of around 1,600 light years, giving it a spatial dimension of some 12 light years. Most of the bright stars in this cluster are hot, blue B type stars but the brightest cluster member is a K type orange giant star. This star, known as BM Scorpii, is classed as a semiregular variable star, its brightness varying from magnitude +5.5 to magnitude +7.0. In color photographs of the Butterfly Cluster this orange star contrasts sharply with its blue neighbours in the cluster.
External links
Template:Star-cluster-stubde:Messier 6 es:Cúmulo de la Mariposa fr:Amas du Papillon it:M6 nl:Vlindercluster ja:M6 pl:Messier 6 ru:Бабочка (звёздное скопление) sk:Motýlia hviezdokopa fi:Perhosjoukko sv:M6