astro.wikisort.org - Star

Search / Calendar

The Coma Star Cluster (also known as Melotte 111 or Collinder 256) is a small but nearby open cluster located in the constellation Coma Berenices. The cluster contains about 40 brighter stars (between magnitudes 5 and 10) with a common proper motion. The brighter stars of the cluster make out a distinctive "V" shape as seen when Coma Berenices is rising. The cluster used to represent the tail of Leo. However, in around 240 BC, Ptolemy III renamed it for the Egyptian queen Berenice's legendary sacrifice of her hair.

Not to be confused with Coma Cluster.
Coma Star Cluster
The Coma Star Cluster, photographed by astronaut Donald Pettit aboard the ISS in 2003.
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12h 22.5m [1]
Declination+25° 51′[1]
Distance280 ly (86 pc[2][3])
Apparent magnitude (V)+1.8
Apparent dimensions (V)7.5° [2]
Physical characteristics
Mass- M☉
Radius-
Estimated age-
Notable featuresSecond closest open cluster[citation needed]
Other designationsComa Ber Cluster,[1] Cr 256,[4] Mel 111,[1] OCl 558.0[1]
See also: Open cluster, List of open clusters

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).[2][3] 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.[2][3] The cluster is approximately 450 million years old.

Brightest members
(mv < 6.5)[5]
Identifier Magnitude
γ Com[lower-alpha 1] 4.81
12 Com 4.81
31 Com 4.94
14 Com 4.95
16 Com 4.96
13 Com 5.18
17 Com 5.24
21 Com 5.44
18 Com[lower-alpha 2] 5.47
HD 106887 5.71
HD 105805 5.99
8 Com 6.22
22 Com 6.24
FM Com 6.43
  1. Outside a nominal 5° radius adopted as the cluster size
  2. At the same distance as Melotte 111, but its proper motion and isochrone are inconsistent.

See also



References


  1. "Cl Melotte 111 -- Open (galactic) Cluster". SIMBAD. Retrieved 23 October 2013.
  2. 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.
  3. 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.
  4. Houston, Walter Scott. "Open Clusters by the Season". Sky & Telescope. p. 8. Retrieved 23 October 2013.[permanent dead link]
  5. Tang, Shih-Yun; Chen, W. P.; Chiang, P. S.; Jose, Jessy; Herczeg, Gregory J.; Goldman, Bertrand (2018). "Characterization of Stellar and Substellar Members in the Coma Berenices Star Cluster". The Astrophysical Journal. 862 (2): 106. arXiv:1806.08322. Bibcode:2018ApJ...862..106T. doi:10.3847/1538-4357/aacb7a.



This star cluster–related article is a stub. You can help Wikipedia by expanding it.

  • v
  • t
  • e

На других языках

[de] Melotte 111

Melotte 111 oder der Coma-Berenices-Sternhaufen ist ein offener Sternhaufen im Sternbild Haar der Berenike, der mit bloßem Auge beobachtet werden kann. Der Sternhaufen bildet den Hauptteil des Sternbildes Haar der Berenike. Zudem war der Eindruck dieses Sternhaufens mit dem bloßen Auge wohl namensgebend für das Sternbild.
- [en] Coma Star Cluster

[ru] Мелотт 111

Не следует путать со скоплением галактик Волос Вероники.


Текст в блоке "Читать" взят с сайта "Википедия" и доступен по лицензии Creative Commons Attribution-ShareAlike; в отдельных случаях могут действовать дополнительные условия.

Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.

2019-2025
WikiSort.org - проект по пересортировке и дополнению контента Википедии