Balbinot 1

Balbinot I is a low-luminosity globular cluster in the constellation of Pegasus. It is located 31.9 kpc away from the Sun, in the Milky Way galactic halo. Its total luminosity is similar to that of the clusters AM 4 and Koposov I, thus being one of the faintest globular clusters known. From Pan-STARRS data, the presence of tidal tails has been suggested [2]

Balbinot I
Observation data
Constellation	Pegasus
Right ascension	22^h 10^m 43.15^s.[1]
Declination	+14° 56′ 58.8″[1]
Distance	31.9 kpc (104 kly)[1]
Apparent magnitude (V)	16.31[1]
Physical characteristics
Radius	approx. 72 pc (230 ly)[1]

References

1. "A New Milky Way Halo Star Cluster In The Southern Galactic Sky - Iopscience". Iopscience.iop.org. 2015-02-26. doi:10.1088/0004-637X/767/2/101. Retrieved 2020-03-17.
2. Bernard, Edouard J.; Ferguson, Annette M. N.; Schlafly, Edward F.; Martin, Nicolas F.; Rix, Hans-Walter; Bell, Eric F.; Finkbeiner, Douglas P.; Goldman, Bertrand; Martínez-Delgado, David; Sesar, Branimir; Wyse, Rosemary F. G.; Burgett, William S.; Chambers, Kenneth C.; Draper, Peter W.; Hodapp, Klaus W.; Kaiser, Nicholas; Kudritzki, Rolf-Peter; Magnier, Eugene A.; Metcalfe, Nigel; Wainscoat, Richard J.; Waters, Christopher (December 1, 2016). "A synoptic map of halo substructures from the Pan-STARRS1 3π survey". Monthly Notices of the Royal Astronomical Society. 463 (2): 1759–1768. doi:10.1093/mnras/stw2134 – via academic.oup.com.