Beta Librae

Beta Librae
The position of β Librae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Libra
Right ascension 15h 17m 00.41382s
Declination −09° 22′ 58.4919″
Apparent magnitude (V) 2.61
Characteristics
Evolutionary stage Main sequence
Spectral type B8 V
U−B color index −0.359
B−V color index −0.106
Variable type Suspected
Astrometry
Radial velocity (Rv)−35.2 km/s
Proper motion (μ) RA: −98.10 mas/yr
Dec.: −19.65 mas/yr
Parallax (π)17.62±0.16 mas
Distance185 ± 2 ly
(56.8 ± 0.5 pc)
Absolute magnitude (MV)−1.16
Details
Mass3.5+0.3
−0.2
 M
Radius4.77 R
Luminosity413 L
Temperature11,900 K
Metallicity [Fe/H]0.33 dex
Rotational velocity (v sin i)250 km/s
Age80+50
−40
 Myr
Other designations
Zubeneschamali, Kiffa Australis, Lanx Borealis, β Lib, 27 Librae, BD−08°3935, FK5 564, HD 135742, HIP 74785, HR 5685, NSV 7009, SAO 140430
Database references
SIMBADdata

Beta Librae is the brightest star in the zodiac constellation of Libra. It has the proper name Zubeneschamali /zˌbɛnɛʃəˈmli/, Beta Librae is its Bayer designation. From parallax measurements taken by the Hipparcos mission, its distance is measured to be 185 light-years (57 parsecs).

The apparent visual magnitude of this star is 2.6. According to Eratosthenes, Beta Librae was observed to be brighter than Antares. Ptolemy, 350 years later, said it was as bright as Antares. The discrepancy may be due to Antares becoming brighter, but this is not known for certain. It could simply be caused by Beta Librae being a variable star, showing a present-day variability of 0.03 of a magnitude.