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

Name:M90, NGC 4569
Constellation:Virgo
Category:Galaxies

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1.5 MB
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Coordinates

ObjectValue
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