M79 is a compact and strikingly bright globular cluster in Lepus, just below Orion's belt. The cluster contains a large population of old,
metal-poor stars and has a fairly concentrated core. M79 is special because it is presumably not an original inhabitant of the Milky Way:
many studies suggest that the cluster originated from a former dwarf galaxy that was swallowed up by our Milky Way. In astrophotographs,
M79 shows a beautiful grainy structure with countless individual stars surrounding the bright core.