Beta Aquarii

Beta Aquarii
Location of β Aquarii (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension 21h 31m 33.53171s
Declination −05° 34 16.2320
Apparent magnitude (V) 2.87
Characteristics
Evolutionary stage Yellow supergiant
Spectral type G0 Ib
U−B color index +0.58
B−V color index +0.84
Astrometry
Radial velocity (Rv)6.451±0.0627 km/s
Proper motion (μ) RA: +18.77 mas/yr
Dec.: −8.21 mas/yr
Parallax (π)5.9728±0.2147 mas
Distance541.8+18.4
−15.5
 ly
(166.12+5.64
−4.75
 pc)
Absolute magnitude (MV)−3.04
Details
Mass4.97±0.10  6.3 M
Radius47.88+1.68
−1.81
 R
Luminosity2046±180 L
Surface gravity (log g)2.05 cgs
Temperature5608±71 K
Metallicity [Fe/H]−0.03 dex
Rotational velocity (v sin i)6.3±1.3 km/s
Age56  110±10 Myr
Other designations
Sadalsuud, Saad el Sund, β Aqr, 22 Aqr, BD−06 5770, FK5 808, GC 30137, HD 204867, HIP 106278, HR 8232, SAO 145457, ADS 15050 A, CCDM J21316-0534A
Database references
SIMBADdata

Beta Aquarii is a single yellow supergiant star in the constellation of Aquarius. It has the official name Sadalsuud (/ˌsædəlˈsəd/) and the Bayer designation β Aquarii, abbreviated Beta Aqr or β Aqr. Based upon parallax measurements obtained during the Hipparcos mission, this component is located at a distance of approximately 540 light years (165 parsecs) from the Sun. It is drifting further away with a radial velocity of 6.5 km/s. The star serves as an IAU radial velocity standard.