M90, NGC 4569
M90 is a large spiral galaxy of type Sb in the constellation Virgo. Although large, it seems to have a relatively small mass and thus be of low density. The nearby high surface brightness spiral, IC3583, is clearly visible to the north and seems a bit distorted, which led H.C.Arp to include this system in his Atlas of Peculiar Galaxies. M90 is a member of the Virgo Cluster of galaxies, which is the dominant cluster in our Local Supercluster and about 60 million light-years away. This CCD composite picture was taken in April 1998 at the Kitt Peak 0.9-meter telescope. The Virgo cluster also includes Messier galaxies M49, M58, M59, M60, M61, M84, M85, M86, M87, M88, M89, M91, M98, M99, and M100.
Credit:NOIRLab/NSF/AURA
About the Image
Id: | noao-m90 |
Type: | Observation |
Release date: | June 30, 2020, 9:33 p.m. |
Size: | 2000 x 2500 px |
About the Object
Wallpapers
1024x768
242.7 KB
1280x1024
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1600x1200
632.6 KB
1920x1200
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2048x1536
3.9 MB
Coordinates
Position (RA): | 12 36 47.79 |
Position (Dec): | 13° 10' 46.72" |
Field of view: | 11.35 x 14.18 arcminutes |
Orientation: | North is 0.8° left of vertical |