Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  M 106  ·  NGC 4217  ·  NGC 4226  ·  NGC 4231  ·  NGC 4232  ·  NGC 4248  ·  NGC 4258
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Galaxy M106 (NGC 4258) and neighbors NGC 4217, NGC 4226, NGC 4231, NGC 4232, NGC 4248, NGC 4258, AstroDinsk
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Galaxy M106 (NGC 4258) and neighbors NGC 4217, NGC 4226, NGC 4231, NGC 4232, NGC 4248, NGC 4258

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Galaxy M106 (NGC 4258) and neighbors NGC 4217, NGC 4226, NGC 4231, NGC 4232, NGC 4248, NGC 4258, AstroDinsk
Powered byPixInsight

Galaxy M106 (NGC 4258) and neighbors NGC 4217, NGC 4226, NGC 4231, NGC 4232, NGC 4248, NGC 4258

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Description

The galaxy was first described by the French astronomer Pierre Méchain, who discovered it on July 30, 1781. M 106 is a bright spiral galaxy. The tilt of M106 is very similar to that of M31 in the Andromeda Galaxy, which explains why the dust trails are so visible. The spiral arms appear to terminate in bright blue areas. These regions are likely regions of young star formation that are dominated by young, very hot, bright, and massive stars. At the core is a supermassive black hole with a mass of 36 million solar masses.

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