
science & techESA/Hubble
Messier 62 is a 12-billion-year-old star cluster shaped like a comet
Most globular clusters are nearly perfectly round balls of ancient stars, but Messier 62 is stretched into a comet-like shape with a bright head and a long tail. It is about 12 billion years old and sits relatively close to the centre of the Milky Way, where strong tidal forces from the galaxy pull many of its stars out of place. Its mass is almost a million times that of the Sun, which makes its core one of the densest of any known cluster. Crowded cores see frequent interactions and mergers, and dying massive stars leave behind white dwarfs, neutron stars and sometimes black holes. For years astronomers thought black holes formed in clusters would be ejected quickly, but in 2013 one was found in Messier 62, the first discovered in a Milky Way globular cluster. The image combines ultraviolet and visible light from Hubble's Advanced Camera for Surveys.
The discovery of a black hole in Messier 62 overturned the assumption that such objects are flung out of dense clusters, opening a new place to search for them. The cluster's odd shape also shows how the galaxy's gravity can reshape even ancient star groups.
