NEBULAE & STAR CLUSTERS A  B  C  D  E  F  G  H  I  J  K  L  M  N  O  P  Q  R  S  T  U  V  W  X  Y  Z                    HOME ABOUT CATEGORIES SITE MAP COPYRIGHT ADVERTISE CONTACT entire Web this site open cluster The open cluster M39 in Cygnus. It lies about 800 light-years away and contains stars that are only about 300 million years old. Image: WIYN telescope, Kitt Peak A loose aggregation of dozens or hundreds of young stars, in a volume of space typically less than 50 light-years across. Open clusters are only weakly held together by gravity and are fated to disperse over a period of several hundred million years. An older name for these groupings is galactic clusters because they are found mostly in the disk, and especially the spiral arms, of this and other disk galaxies. The stars in open clusters have formed together within the same interstellar cloud; indeed, in many diffuse nebulae, the birth of new open clusters can be seen taking place. As open clusters drift along, some of their members escape due to velocity changes in mutual closer encounters, tidal forces in the galactic gravitational field, and encounters with field stars and interstellar clouds passing their way. Well known examples of open clusters include: Pleiades Hyades Praesepe Butterfly Cluster Ptolemy's Cluster Wild Duck Cluster NGC 752 Compare with globular clusters. Related category    • NEBULAE AND STAR CLUSTERS Also on this site: Encyclopedia of Alternative Energy & Sustainable Living Encyclopedia of History Transport Concepts & Designs (partner site) BACK TO TOP