April-May, 2008. The famous Pinwheel Galaxy in the northern constellation Canes Venatici. If you place your cursor over the image you will see the names of some of M51’s neighbors. M51 and its companion galaxy NGC 5195 are experiencing a close encounter of the gravitational kind. There appears to be a bridge of stars connecting the two galaxies. This would indicate that M51, with its greater mass, is disrupting NGC 5195 and stripping away its stars. Eventually the two galaxies will merge into a galaxy that will probably not resemble what we see today. The faint light surrounding with both galaxies is actually starlight from regions with a lower density of stars than the central parts of the galaxies. The number of stars in M51 and its companion, numbers in the hundreds of billions. The distance to M51 is believed to be about 30 million light years.
NGC 5198 is a giant elliptical galaxy that is about 150 million light years distant. It must be extremely luminous to appear as bright as it does at that great distance. IC 4263 and NGC 5169 are spiral galaxies.
Takahashi FSQ-106ED, SBIG STL-11000M. LRGB. |