Alpha Librae

Alpha Librae (α Librae, abbreviated Alpha Lib, α Lib) is a double star and, despite its 'alpha' designation, it is the second-brightest star system (or star) in the constellation of Libra. The two components are designated α1 Librae and α2 Librae. The system bore the traditional name of Zubenelgenubi /zˌbɛnɛlɪˈnbi/, though the International Astronomical Union now regards that name as only applying to α2 Librae.

α Librae
Location of α Librae (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Libra
α1 Lib
Right ascension 14h 50m 41.18097s
Declination −15° 59 50.0482
Apparent magnitude (V) +5.153
α2 Lib
Right ascension 14h 50m 52.71309s
Declination −16° 02 30.3955
Apparent magnitude (V) +2.741
Characteristics
α1 Lib
Spectral type F3 V
U−B color index −0.02
B−V color index +0.39
α2 Lib
Spectral type kA2hA5mA4 IV-V
U−B color index +0.10
B−V color index +0.15
Astrometry
α1 Lib
Radial velocity (Rv)−23.47 km/s
Proper motion (μ) RA: −136.27 mas/yr
Dec.: −59.04 mas/yr
Parallax (π)43.52 ± 0.43 mas
Distance74.9 ± 0.7 ly
(23.0 ± 0.2 pc)
Absolute magnitude (MV)+3.35
α2 Lib
Proper motion (μ) RA: −105.68 mas/yr
Dec.: −68.40 mas/yr
Parallax (π)43.03 ± 0.19 mas
Distance75.8 ± 0.3 ly
(23.2 ± 0.1 pc)
Orbit
Period (P)70.34 days
Semi-major axis (a)0.51 au
Eccentricity (e)0.41
Semi-amplitude (K2)
(secondary)
43.1 km/s
Details
α1 Lib
Mass1.4–1.5/0.5–0.6 M
Surface gravity (log g)4.25 cgs
Temperature6,653 K
Metallicity [Fe/H]−0.07 dex
Rotational velocity (v sin i)5.95 km/s
Age1.1+0.6
−0.8
 Gyr
α2 Lib
Mass1.95 + 1.79 M
Surface gravity (log g)3.91 cgs
Temperature8128 K
Metallicity [Fe/H]−0.24 dex
Other designations
Zubenelgenubi, Kiffa Australis, Lanx Australis, α Lib.
α1 Lib: 8 Librae, BD−15 3965, FK5 1387, HD 130819, HIP 72603, HR 5530, SAO 158836.
α2 Lib: 9 Librae, BD−15 3966, FK5 548, HD 130841, HIP 72622, HR 5531, SAO 158840.
Database references
SIMBADα Lib
α1 Lib
α2 Lib

Alpha2 Librae is 0.33 degrees north of the ecliptic so it can be occulted by the Moon and (very rarely) by planets. It was occulted by Venus on October 25, 1947; the next occultation by a planet will be by Mercury on 10 November 2052. Both components are eclipsed (occulted) by the sun from about 7–9 November. Thus the star can be viewed the whole night, crossing the sky, in early May.

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