Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquarius |
Right ascension | 22h 39m 16.03872s[1] |
Declination | −10° 01′ 40.1750″[1] |
Apparent magnitude (V) | 6.93[2] |
Characteristics | |
Spectral type | G2/3 IV/V[3] |
B−V color index | 0.619±0.009[2] |
Astrometry | |
Radial velocity (Rv) | +10.7±0.5[4] km/s |
Proper motion (μ) | RA: −60.940[1] mas/yr Dec.: +3.803[1] mas/yr |
Parallax (π) | 10.4508 ± 0.1554 mas[1] |
Distance | 312 ± 5 ly (96 ± 1 pc) |
Absolute magnitude (MV) | 2.75[2] |
Details[5] | |
Mass | 1.45±0.06 M☉ |
Radius | 2.78±0.07 R☉ |
Luminosity | 13.133±0.225[1] L☉ |
Surface gravity (log g) | 3.708±0.013 cgs |
Temperature | 5,926±97 K |
Metallicity [Fe/H] | −0.02±0.11 dex |
Rotational velocity (v sin i) | 8.75 km/s |
Age | 2.63±0.26 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
64 Aquarii is a star located 312 light years away from the Sun in the zodiac constellation of Aquarius. 64 Aquarii is its Flamsteed designation. With an apparent visual magnitude of 6.93,[2] it is too faint to be readily visible to the naked eye. The star is moving further from the Earth with a heliocentric radial velocity of +11 km/s.[4]
The stellar classification for this star is G2/3 IV/V,[3] which indicates the spectrum displays mixed traits of a G-type main-sequence star and a more evolved subgiant star. It is 2.6 billion years old and is spinning with a projected rotational velocity of 8.75 km/s. The star has 1.45 times the mass of the Sun and 2.8 times the Sun's radius.[5] It is radiating 13[1] times the luminosity of the Sun from its photosphere at an effective temperature of 5,926 K.[5]
GaiaDR2
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