Messier 56

Messier 56
Messier 56
Messier 56 Hubble WikiSky.jpg
Messier 56 by Hubble Space Telescope. 3.6′ view
Credit: NASA/STScI/WikiSky
Observation data (J2000 epoch)
Class X
Constellation Lyra
Right ascension 19h 16m 35.50s[1]
Declination +30° 11′ 04.2″[1]
Distance 32.9 kly[2] (10.1 kpc)
Apparent magnitude (V) +8.3
Apparent dimensions (V) 8′.8
Physical characteristics
Radius 42 ly[3]
Other designations M56, NGC 6779, GCl 110[1]
See also: Globular cluster, List of globular clusters
Messier 56 with amateur telescope

Messier 56 (also known as M56 or NGC 6779) is a globular cluster in the constellation Lyra. It was discovered by Charles Messier in 1779. M56 is at a distance of about 32,900 light-years from Earth and measures roughly 84 light-years across.

The brightest stars in M56 are of 13th magnitude while it contains only about a dozen known variable stars, such as V6 (RV Tauri star; period: 90 days) or V1 (Cepheid: 1.510 days); other variable stars are V2 (irregular) and V3 (semiregular).

References

  1. ^ a b c "SIMBAD Astronomical Database". Results for NGC 6779. http://simbad.u-strasbg.fr/Simbad. Retrieved 2006-11-16. 
  2. ^ Valentin D. Ivanov, Jordanka Borissova, Almudena Alonso-Herrero, Tatiana Russeva (2000). "Near Infrared Photometry of Galactic Globular Clusters M56 and M15. Extending the Red Giant Branch vs. Metallicity Calibration Towards Metal Poor Systems". arXiv:astro-ph/0002118 [astro-ph]. 
  3. ^ distance × sin( diameter_angle / 2 ) = 42 ly. radius

External links

Coordinates: Sky map 19h 16m 35.50s, +30° 11′ 04.2″



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