“Stephan’s Quintet is a visual grouping of five galaxies of which four form the first compact galaxy group ever discovered.[2] The group was discovered by Édouard Stephan in 1877 at Marseilles Observatory.[3] The group is the most studied of all the compact galaxy groups.[2] The brightest member of the visual grouping is NGC 7320 that is shown to have extensive H II regions, identified as red blobs, where active star formation is occurring.
These galaxies are of interest because of their violent collisions. Four of the five galaxies in Stephan’s Quintet form a physical association, and are involved in a cosmic dance that most likely will end with the galaxies merging. Radio observations in the early 1970s revealed a mysterious filament of emission which lies in inter-galactic space between the galaxies in the group. This same region is also detected in the faint glow of ionized atomic hydrogen seen in the visible part of the spectrum as the magnificent green arc in the picture to the right. Two space telescopes have recently provided new insight into the nature of the strange filament, which is now believed to be a giant intergalactic shock-wave (similar to a sonic boom but traveling in intergalactic gas rather than air) caused by one galaxy falling into the center of the group at several millions of miles per hour. As NGC 7318B collides with gas in the group, a huge shock wave bigger than the Milky Way spreads throughout the medium between the galaxies, heating some of the gas to temperatures of millions of degrees where they emit X-rays detectable with the NASA Chandra X-ray Observatory.” [wikipedia.org]
The picture is 4h of unfiltered exposure in the urban light-polluted conditions. Taken at Altummundi observatory on July 27th, 2009. It is very breath-taking experience when using amateur equipment one can reach so deeply into the universe. It is so surprising how many galaxies are visible on this image.




