Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Aquarius |
Right ascension | 22h 05m 47.03555s[1] |
Declination | −00° 19′ 11.4634″[1] |
Apparent magnitude (V) | 2.942[2] |
Characteristics | |
Evolutionary stage | Yellow supergiant |
Spectral type | G2 Ib[3] |
U−B color index | +0.699[2] |
B−V color index | +0.971[2] |
R−I color index | +0.49[2] |
Astrometry | |
Radial velocity (Rv) | 7.5[4] km/s |
Proper motion (μ) | RA: +18.59 mas/yr[1] Dec.: −10.45 mas/yr[1] |
Parallax (π) | 4.9451 ± 0.4296 mas[1] |
Distance | 690.8+37.8 −56.1 ly (211.9+11.6 −17.2 pc)[5] |
Absolute magnitude (MV) | −3.882[6] |
Details | |
Mass | 6.31[7] M☉ |
Radius | 70[8] R☉ |
Luminosity | 3,917[7] L☉ |
Surface gravity (log g) | 1.4[7] cgs |
Temperature | 5,190±50[9] K |
Metallicity [Fe/H] | +0.17[6] dex |
Rotational velocity (v sin i) | 6.7±1.5[10] km/s |
Age | 53[3] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Alpha Aquarii, officially named Sadalmelik (/ˌsædəlˈmɛlɪk/),[15] is a single yellow supergiant star in the constellation of Aquarius. The apparent visual magnitude of 2.94[2] makes this the second-brightest star in Aquarius. Based upon parallax measurements made by the Gaia spacecraft, it is located at a distance of roughly 690 light-years (210 parsecs) from the Sun.[5] It is drifting further away from the Sun with a radial velocity of 7.5 km/s.[4]
It forms the primary or 'A' component of a double star designated WDS J22058-0019; the secondary or 'B' component is UCAC2 31789179.[16] However, the pair is only an optical binary, with UCAC2 31789179 being a background star.[16]
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