M77, NGC 1068
M77 is a type Sb spiral galaxy in the constellation Cetus. For various reasons, it is much more commonly referred to by its NGC number. NGC1068 is the nearest and brightest example of a type II Seyfert galaxy, showing broad and strong emission lines due to high velocity gas in the galaxy's inner regions. A strong radio source known as Cetus A sits in the nucleus.
Credit:NOIRLab/NSF/AURA
About the Image
Id: | noao-m77 |
Type: | Observation |
Release date: | June 30, 2020, 9:33 p.m. |
Size: | 820 x 680 px |
About the Object
Wallpapers
1024x768
195.4 KB
1280x1024
297.3 KB
1600x1200
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1920x1200
427.8 KB
2048x1536
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Coordinates
Position (RA): | 2 42 36.20 |
Position (Dec): | 0° 0' 8.82" |
Field of view: | 6.15 x 5.10 arcminutes |
Orientation: | North is 0.8° right of vertical |