WebTo some, the outline of the open cluster of stars M6 resembles a butterfly. M6, also known as NGC 6405, spans about 20 light-years and lies about 2,000 light years distant. M6 can best be seen in a dark sky with binoculars towards the constellation of Scorpius, coving about as much of the sky as the full moon. Like other open clusters, M6 is composed … Web20 de mar. de 2024 · Both M7 and M6 are best viewed from the northern hemisphere around 10 p.m. in July, when the Scorpio constellation is highest in the sky. The smaller, ground-based image (lower left) taken by the European Southern Observatory, illustrates the small area of Messier 7 that Hubble observed.
Messier 6 - The Butterfly Cluster - Universe Today
Web14 de mar. de 2016 · Some, like Messier 7 cluster (aka. NGC 6475 or the Ptolemy Cluster) have been known about since classical antiquity. As the name would suggest, this open star cluster was first observed in the 2nd ... The Butterfly Cluster (cataloged as Messier 6 or M6, and as NGC 6405) is an open cluster of stars in the southern constellation of Scorpius. Its name derives from the vague resemblance of its shape to a butterfly. The Trumpler classification of II 3 r encodes it is rich in stars, ranks II out of IV for disparateness and … Ver mais • List of open clusters • List of Messier objects Ver mais • Messier 6, SEDS Messier pages • The Butterfly Cluster on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images Ver mais chip with icon flutter
Messier Monday: The Butterfly Cluster, M6 - Medium
http://sidleach.com/m6.htm WebMany of the labeled objects (for example, M6, M7, M11, M21, M23, and M25) are all open clusters! If you have a small pair of binoculars, you can slowly scan this part of the sky. You will run into open cluster after open cluster. Many stars in a variety of open clusters have also been studied spectroscopically. WebMessier 38 or M38, also known as NGC 1912 or Starfish Cluster, [4] is an open cluster of stars in the constellation of Auriga. It was discovered by Giovanni Batista Hodierna before 1654 and independently found by Le Gentil in 1749. The open clusters M36 and M37, also discovered by Hodierna, are often grouped together with M38. [5] chip w johnson