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)
Be 46, OCL 142
I 2 r
RA / Dec:
19h 20m 51s /
37° 46' 18"
15' x 15'
Jul 12-13, 2012
23:00 - 02:15 UT+3
AP 305/f3.8 Riccardi-Honders
AP 1200GTO GEM
SBIG LRGB filters
1.25" per pixel