Open star clusters are widely distributed in our galaxy and represent a loose collection of stars which number from a
few dozen to a few hundred stars and are weakly-held gravitationally. Perhaps the three most famous such open clusters
are the Pleiades (M45) in Taurus, the Beehive (M44) in Cancer and the double cluster in Perseus. They are all
characterized with a handful of hot and white prominent stars and nebular material surrounding these stars.
Note: Although estimates as to the age of NGC 6791 in Lyra vary dramatically, ranging from just
over 5 billion years (van den Berg, 2002) to 10.2 billion years old (Salaris, 2004), this particular open cluster is one of
the oldest and mostly studied open clusters in the Milky Way and certainly older than our solar system. In a more recent
study using Hubble data, three
populations were identified comprised of two white dwarfs groups aged 4 and 6 billion years-old as well as a third group aged
8 billion years-old. Believed to contain up to 10,000 member stars lying approximately 13,300 light-years away, the cluster
lies a few degrees immediately south of è-Lyr (mag 4.24). The cluster's discovery has been attributed to Friedrich August
Theodor Winnecke (1853) and is currently catalogued in multiple sources. The cluster is best located in late spring and early
summer when it lies overhead around midnight.
Please click on the image below to display in higher resolution (1200 x 900)