94 Aquarii

94 Aquarii
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
94 Aquarii A (Aa/Ab)
Right ascension 23h 19m 06.7257s
Declination −13° 27 31.6146
Apparent magnitude (V) 5.19
94 Aquarii B
Right ascension 23h 19m 06.5609s
Declination –13° 27 18.9037
Apparent magnitude (V) 7.52
Characteristics
94 Aqr A
Spectral type G8.5 IV + K V
U−B color index +0.42
B−V color index +0.79
94 Aqr B
Spectral type K2 V
U−B color index +0.60
B−V color index +0.88
Astrometry
94 Aquarii A (Aa/Ab)
Radial velocity (Rv)+17.60±0.07 km/s
Proper motion (μ) RA: 258.738±0.944 mas/yr
Dec.: −73.014±0.928 mas/yr
Parallax (π)44.8996±0.5572 mas
Distance72.6 ± 0.9 ly
(22.3 ± 0.3 pc)
Absolute magnitude (MV)+3.52/+6.52
94 Aquarii B
Proper motion (μ) RA: 306.702±0.107 mas/yr
Dec.: −104.633±0.086 mas/yr
Parallax (π)44.5152 ± 0.0550 mas
Distance73.27 ± 0.09 ly
(22.46 ± 0.03 pc)
Absolute magnitude (MV)+5.92
Orbit
Primary94 Aquarii Aa
Companion94 Aquarii Ab
Period (P)6.321±0.010 yr
Semi-major axis (a)0.189±0.002
Eccentricity (e)0.173±0.020
Inclination (i)44.5±1.0°
Longitude of the node (Ω)341.9±1.5°
Periastron epoch (T)2012.301
Argument of periastron (ω)
(secondary)
28.3°
Details
94 Aquarii Aa
Mass1.22±0.03 M
Radius2.06±0.03 R
Luminosity3.30±0.06 L
Surface gravity (log g)3.88 cgs
Temperature5,461 K
Metallicity [Fe/H]+0.23 dex
Rotational velocity (v sin i)8 km/s
Age6.2±0.2 Gyr
94 Aquarii Ab
Mass0.81±0.04 M
Radius0.85±0.03 R
Temperature4,670 or 4,970 K
94 Aquarii B
Surface gravity (log g)4.54 cgs
Temperature5,136 K
Metallicity [Fe/H]+0.24 dex
Other designations
BD−14 6448, GJ 894.2, HD 219834, HIP 115126, HR 8866, SAO 165625
Database references
SIMBADdata

94 Aquarii (abbreviated 94 Aqr) is a triple star system in the equatorial constellation of Aquarius. 94 Aquarii is the Flamsteed designation. The brightest member has an apparent visual magnitude of 5.19, making it visible to the naked eye. The parallax measured by the Gaia spacecraft yields a distance estimate of around 73 light-years (22 parsecs) from Earth.

The inner pair of this triple star system form a spectroscopic binary with an orbital period of 6.321 years, a moderate orbital eccentricity of 0.173, and a combined visual magnitude of 5.19. The primary component of this pair has a stellar classification of G8.5 IV, with the luminosity class of IV indicating this is a subgiant star. At an angular separation of 13.0 arcseconds from this pair is a magnitude 7.52 K-type main sequence star with a classification of K2 V.