Beta Virginis

β Virginis
(Zavijava)
Location of β Virginis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Right ascension 11h 50m 41.71824s
Declination +01° 45 52.9910
Apparent magnitude (V) 3.604
Characteristics
Evolutionary stage Main sequence turnoff
Spectral type F9 V
U−B color index +0.090
B−V color index +0.553
Astrometry
Radial velocity (Rv)+4.1 km/s
Proper motion (μ) RA: +740.23 mas/yr
Dec.: −270.43 mas/yr
Parallax (π)91.50±0.22 mas
Distance35.65 ± 0.09 ly
(10.93 ± 0.03 pc)
Absolute magnitude (MV)3.41
Details
Mass1.413±0.061 M
Radius1.681±0.008 R
Luminosity3.572±0.052 L
Surface gravity (log g)4.125±0.010 cgs
Temperature6,132±26 K
Metallicity [Fe/H]0.20 dex
Rotational velocity (v sin i)4.3 km/s
Age2.9 ± 0.3, ~3.3 Gyr
Other designations
Zavijava, Zavijah, Alaraph, β Vir, 5 Virginis, BD+02°2489, FK5 445, GJ 449, HD 102870, HIP 57757, HR 4540, SAO 119076
Database references
SIMBADdata
ARICNSdata

Beta Virginis, a name Latinised from β Virginis, is a star in the equatorial constellation of Virgo. It has the proper name Zavijava (/ˌzævɪˈævə/), and, despite its designation 'beta', is the fifth-brightest star in Virgo with an apparent visual magnitude of 3.604. The distance to this star is around 35.7 light-years based on parallax; it is drifting further away with a radial velocity of +4.1 km/s. It is 0.69 of a degree north of the ecliptic, so it can be occulted by the Moon and (rarely) by planets. The next planetary occultation of Beta Virginis will take place on 9 November 2210, by Venus; although an occultation by the same planet might be visible on 11 August 2069 from the South Pole.