Located about 15 million light-years away towards the Hydra (the sea serpent) constellation, Messier 83 is a nearby face-on barred spiral with a classic grand design form. It is the main member of a small galactic group including NGC 5253 and about 9 dwarf galaxies. Messier 83 stretches over 40000 light-years, making it roughly 2, 5 times smaller than our own Milky Way. However, in some respects, Messier 83 is quite similar to our own galaxy. Both the Milky Way and Messier 83 possess a bar across their galactic nucleus, the dense spherical conglomeration of stars seen at the centre of the galaxies. Messier 83 has been a prolific producer of supernovae, with six observed in the past century. This is indicative of an exceptionally high rate of star formation coinciding with its classification as a starburst galaxy. This image was created from photographic material taken with the 1.22-metre UK Schmidt Telescope at Anglo-Australian Observatory, forming part of the Digitized Sky Survey 2. | |
Licence : | Droits gérés |
Crédit: | Science Photo Library / De Martin, Davide |
Taille de l’image : | 3292 px × 2643 px |
Model Release : | Non requis |
Property Release : | Non requis |
Restrictions : | - |