Barred Spiral Galaxy Swirls in the Night Sky

This image shows the swirling shape of galaxy NGC 2217, in the constellation of Canis Major (The Great Dog). In the central region of the galaxy is a distinctive bar of stars within an oval ring. Further out, a set of tightly wound spiral arms almost form a circular ring around the galaxy. NGC 2217 is therefore classified as a barred spiral galaxy, and its circular appearance indicates that we see it nearly face-on.

The outer spiral arms have a bluish colour, indicating the presence of hot, luminous, young stars, born out of clouds of interstellar gas. The central bulge and bar are yellower in appearance, due to the presence of older stars. Dark streaks can also be seen in places against the galaxy’s arms and central bulge, where lanes of cosmic dust block out some of the starlight.

The majority of spiral galaxies in the local Universe — including our own Milky Way — are thought to have a bar of some kind, and these structures play an important role in the development of a galaxy. They can, for example, funnel gas towards the centre of the galaxy, helping to feed a central black hole, or to form new stars.

Credit:

ESO

About the Image

Id:potw1204a
Type:Observation
Release date:23 January 2012, 10:00
Size:1688 x 1841 px

About the Object

Name:NGC 2217
Type:• Local Universe : Galaxy : Type : Barred
• X - Galaxies
Distance:65 million light years
Constellation:Canis Major

Image Formats

Large JPEG
1.5 MB
Screensize JPEG
291.2 KB

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1024x768
285.3 KB
1280x1024
564.1 KB
1600x1200
990.2 KB
1920x1200
1.2 MB
2048x1536
1.6 MB

Coordinates

Position (RA):6 21 40.35
Position (Dec):-27° 13' 56.90"
Field of view:4.44 x 4.84 arcminutes
Orientation:North is 0.2° left of vertical
View in WorldWide Telescope:
View in WorldWide Telescope

Colours & filters

BandWavelengthTelescope
Optical
B
440 nm ESO 3.6-metre telescope
EFOSC
Optical
V
547 nm ESO 3.6-metre telescope
EFOSC
Optical
R
643 nm ESO 3.6-metre telescope
EFOSC

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