Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  M 106  ·  NGC 4248  ·  NGC 4258
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M 106 Spiral Galaxy in Canes Venatici, Dale A Chamberlain
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M 106 Spiral Galaxy in Canes Venatici

Acquisition type: Electronically-Assisted Astronomy (EAA, e.g. based on a live video feed)
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M 106 Spiral Galaxy in Canes Venatici, Dale A Chamberlain
Powered byPixInsight

M 106 Spiral Galaxy in Canes Venatici

Acquisition type: Electronically-Assisted Astronomy (EAA, e.g. based on a live video feed)

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Description

Messier 106 (also known as NGC 4258) is an intermediate spiral galaxy in the constellation Canes Venatici. It was discovered by Pierre Méchain in 1781. M106 is at a distance of about 22 to 25 million light-years away from Earth. M106 contains an active nucleus classified as a Type 2 Seyfert, and the presence of a central supermassive black hole has been demonstrated from radio-wavelength observations of the rotation of a disk of molecular gas orbiting within the inner light-year around the black hole. NGC 4217 is a possible companion galaxy of Messier 106. A Type II supernova was observed in M106 in May 2014.

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  • M 106 Spiral Galaxy in Canes Venatici, Dale A Chamberlain
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M 106 Spiral Galaxy in Canes Venatici, Dale A Chamberlain