File:M94 - Noao-m94.jpg

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English: M94, NGC 4736


The Sab spiral galaxy M94 in the constellation Canes Venatici is considered by some (but not others) to be in a group including M64 and various fainter galaxies. It has an extremely bright innner region surrounded by a blue ring of young star clusters, then a fainter yellowish region of older stars also surrounded by traces of young stars, and even further out a very much fainter outer ring. All of these features are visible in this picture, due to the use of a drastically compressed intensity mapping. This stretch also reveals quite a few small faint background galaxies. This picture was taken in May 1998 at the KPNO 0.9-meter telescope. Image size 17.0 arc minutes.

Credit:Hillary Mathis, N.A.Sharp/NOIRLab/NSF/AURA/
Date Dec. 16, 2002, 11:48 a.m
Source https://noirlab.edu/public/images/noao-m94/
Author Credit:Hillary Mathis, N.A.Sharp/NOIRLab/NSF/AURA/
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current21:36, 14 November 2021Thumbnail for version as of 21:36, 14 November 20213,000 × 3,000 (3.45 MB)Fabian RRRR (talk | contribs)== {{int:filedesc}} == {{Information |description={{en|1='''M94, NGC 4736 The Sab spiral galaxy M94 in the constellation Canes Venatici is considered by some (but not others) to be in a group including M64 and various fainter galaxies. It has an extremely bright innner region surrounded by a blue ring of young star clusters, then a fainter yellowish region of older stars also surrounded by traces of young stars, and even further out a very much fainter outer ring. All of these features are...

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