Epsilon Aquarii

Epsilon Aquarii
Location of ε Aquarii (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension 20h 47m 40.54957s
Declination −09° 29 44.7969
Apparent magnitude (V) 3.77
Characteristics
Evolutionary stage Main sequence or subgiant
Spectral type A1 V + KV
U−B color index +0.029
B−V color index −0.001
Variable type Constant
Astrometry
Radial velocity (Rv)−19.82±0.58 km/s
Proper motion (μ) RA: +33.923 mas/yr
Dec.: −34.926 mas/yr
Parallax (π)13.3619±0.3737 mas
Distance244 ± 7 ly
(75 ± 2 pc)
Absolute magnitude (MV)−0.46
Orbit
PrimaryA
CompanionB
Period (P)1.2 years
Semi-major axis (a)25.9 mas
1.7 AU
Details
A
Mass2.98±0.03 M
Radius4.2 R
Luminosity161±9 L
Surface gravity (log g)3.66±0.14 cgs
Temperature9,622±327 K
Metallicity [Fe/H]−0.08±0.35 dex
Rotational velocity (v sin i)118.0±5.9 km/s
Age388 Myr
B
Mass0.61 M
Radius0.57 R
Temperature4,070 K
Other designations
Albali, ε Aqr, 2 Aquarii, BD−10°5506, FK5 781, HD 198001, HIP 102618, HR 7950, SAO 144810
Database references
SIMBADdata

Epsilon Aquarii is a binary star system in the equatorial zodiac constellation of Aquarius, located near the western constellation border with Capricornus. Its identifier is a Bayer designation that is Latinized from ε Aquarii, and abbreviated Eps Aqr or ε Aqr, respectively. It has the proper name Albali /ælˈbli/, now formally recognized by the IAU. This system is visible to the naked eye as a point of light with an apparent visual magnitude of 3.77, and has an absolute magnitude of −0.46. Based upon parallax measurements taken by the Gaia spacecraft, it is located at a distance of approximately 244 light-years (75 pc) from Earth. The star is drifting closer with a radial velocity of −20 km/s.