Coma Star Cluster
|Coma Star Cluster|
|Observation data (J2000 epoch)|
|Right ascension||12h 22.5m|
|Distance||280 ly (86 pc)|
|Apparent magnitude (V)||+1.8|
|Apparent dimensions (V)||7.5° |
|Other designations||Melotte 111, Coma Ber Cluster, OCl 558.0, Collinder 256|
The Coma Star Cluster in Coma Berenices, designated Melotte 111 after its entry in the catalogue of star clusters by P. J. Melotte, is a small but nearby star cluster in our galaxy, containing about 40 brighter stars (magnitude 5 to 10) with a common proper motion. The Hipparcos satellite and infrared color-magnitude diagram fitting have been used to establish a distance to the cluster's center of approximately 86 parsecs (280 ly). The distance established via the independent analyses agree, thereby making the cluster an important rung on the cosmic distance ladder. The open cluster is roughly twice as distant as the Hyades and covers an area of more than 7.5 degrees on the sky. The cluster is approximately 450 million years old. In the FOV of a good field glass most of its stars can be seen simultaneously. The brighter stars of the cluster make out a distinctive "V" shape as seen when Coma Berenices is rising.
- "Cl Melotte 111 -- Open (galactic) Cluster". SIMBAD. Retrieved 23 October 2013.
- van Leeuwen, F. (April 2009). "Parallaxes and proper motions for 20 open clusters as based on the new Hipparcos catalogue". Astronomy and Astrophysics. 497 (1): 209–242. arXiv:0902.1039. Bibcode:2009A&A...497..209V. doi:10.1051/0004-6361/200811382.
- Majaess, D.; Turner, D.; Lane, D.; Krajci, T. (September 2011). "Deep Infrared ZAMS Fits to Benchmark Open Clusters Hosting Delta Scuti Stars". Journal of the American Association of Variable Star Observers. 39 (2): 219. arXiv:1102.1705. Bibcode:2011JAVSO..39..219M.
- Houston, Walter Scott. "Open Clusters by the Season". Sky & Telescope. p. 8. Retrieved 23 October 2013.
- Media related to Melotte 111 at Wikimedia Commons
- WEBDA page for open cluster Coma Ber by Masaryk University
|This star cluster–related article is a stub. You can help Wikipedia by expanding it.|