Canes II Group [SEP] constellation
Canes II Group
The Canes II Group or Canes Venatici II Group (CVn II Group) is a group of galaxies about 26.1 million light-years away from Earth. The group resides in the Local Supercluster. The largest galaxy within the cluster is M106 (NGC 4258), which is a barred spiral galaxy.
Galaxies in the Cluster.
Canes II is directly behind Canes I, which makes it difficult to show which galaxy belongs in which cluster. It is generally accepted that the following galaxies belong in Canes
burst of particles as the micro black hole suddenly explodes.
Any primordial black hole of sufficiently low mass will evaporate to near the Planck mass within the lifetime of the Universe. In this process, these small black holes radiate away matter. A rough picture of this is that pairs of virtual particles emerge from the vacuum near the event horizon, with one member of a pair being captured, and the other escaping the vicinity of the black hole. The net result is the black hole loses mass (due to conservation of