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.

Kredit:

ESO

O snímku

Id:potw1204a
Typ:Pozorování
Datum zveřejnění:23. ledna 2012 10:00
Velikost:1688 x 1841 px

O objektu

Jméno:NGC 2217
Typ:Local Universe : Galaxy : Type : Barred
Vzdálenost:65 milion světelné roky
Constellation:Canis Major
Kategorie:Galaxies

Image Formats


Zvětšovatelný


Pozadí

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

Souřadnice

Position (RA):6 21 40.35
Position (Dec):-27° 13' 56.90"
Field of view:4.44 x 4.84 arcminutes
Orientace:Sever je 0.2° levá od svislé osy

Barvy & filtry

PásmoVlnová délkaDalekohled
Optický
B
440 nmESO 3.6-metre telescope
EFOSC
Optický
V
547 nmESO 3.6-metre telescope
EFOSC
Optický
R
643 nmESO 3.6-metre telescope
EFOSC

 

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