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.

Kilde:

ESO

Om bildet

ID:potw1204a
Type:Observasjon
Publiseringsdato:23. januar 2012 10:00
Størrelse:1688 x 1841 px

Om objektet

Navn:NGC 2217
Type:Local Universe : Galaxy : Type : Barred
Avstand:65 million lysår
Constellation:Canis Major
Kategori:Galaxies

Bildeformater

Stor JPEG
1,1 MB
Medium JPEG
252,8 KB

Zoombart


Skrivebordsbakgrunner

1024x768
206,2 KB
1280x1024
405,4 KB
1600x1200
724,0 KB
1920x1200
691,6 KB
2048x1536
944,2 KB

Koordinater

Position (RA):6 21 40.35
Position (Dec):-27° 13' 56.90"
Field of view:4.44 x 4.84 arcminutes
Orientering:Nord er 0.2° til venstre for vertikalen

Farger og filtre

BåndBølgelengdeTeleskop
Optisk
B
440 nmESO 3.6-metre telescope
EFOSC
Optisk
V
547 nmESO 3.6-metre telescope
EFOSC
Optisk
R
643 nmESO 3.6-metre telescope
EFOSC

 

Se også