BL Crucis

BL Crucis

A light curve for BL Crucis, adapted from Tabur et al. (2009)
Observation data
Epoch J2000      Equinox J2000
Constellation Crux
Right ascension 12h 27m 28.88s
Declination −58° 59 30.4
Apparent magnitude (V) 5.38
Characteristics
Spectral type M4-5III
Variable type semiregular variable
Astrometry
Radial velocity (Rv)71.7 ± 0.9 km/s
Proper motion (μ) RA: -20.027 ± 0.301 mas/yr
Dec.: 3.586 ± 0.268 mas/yr
Parallax (π)6.8429±0.1942 mas
Distance480 ± 10 ly
(146 ± 4 pc)
Other designations
HD 108396, HIP 60781, HR 4739, SAO 239960, CD58° 4560
Database references
SIMBADdata

BL Crucis is a red giant and a semiregular variable in the constellation of Crux. A 5th magnitude star, it is visible to the naked eye under good observing conditions. Three periods have been detected in its light curve, 30.7, 42.3 and 43.6 days. It is 480 ± 10 light-years distant from Earth.

In 1969, Olin J. Eggen announced that the star, then called HR 4739, is a variable star. It was given its variable star designation, BL Crucis, in 1977.