Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquarius |
Right ascension | 20h 47m 40.54957s[1] |
Declination | −09° 29′ 44.79693″[1] |
Apparent magnitude (V) | 3.77[2] |
Characteristics | |
Evolutionary stage | Main sequence[3] or subgiant[4] |
Spectral type | A1 V[2] + KV[4] |
U−B color index | +0.029[5] |
B−V color index | –0.001[5] |
Variable type | Constant[6] |
Astrometry | |
Radial velocity (Rv) | −19.82±0.58[1] km/s |
Proper motion (μ) | RA: +33.923 mas/yr[1] Dec.: -34.926 mas/yr[1] |
Parallax (π) | 13.3619 ± 0.3737 mas[1] |
Distance | 244 ± 7 ly (75 ± 2 pc) |
Absolute magnitude (MV) | −0.46[7] |
Orbit[4] | |
Primary | A |
Companion | B |
Period (P) | 1.2 years |
Semi-major axis (a) | 25.9 mas 1.7 AU |
Details | |
A | |
Mass | 2.98±0.03[3] M☉ |
Radius | 4.2[4] R☉ |
Luminosity | 161±9[8] L☉ |
Surface gravity (log g) | 3.66±0.14[9] cgs |
Temperature | 9,622±327[9] K |
Metallicity [Fe/H] | −0.08±0.35[6] dex |
Rotational velocity (v sin i) | 118.0±5.9[7] km/s |
Age | 388[9] Myr |
B | |
Mass | 0.61[4] M☉ |
Radius | 0.57[4] R☉ |
Temperature | 4,070[4] K |
Other designations | |
Database references | |
SIMBAD | data |
Epsilon Aquarii, Latinized from ε Aquarii, is a binary star in the equatorial zodiac constellation of Aquarius, located near the western constellation border with Capricornus. It has the proper name Albali /ælˈbeɪli/, now formally recognized by the IAU.[11][12] It is visible to the naked eye with an apparent visual magnitude of 3.77,[2] and has an absolute magnitude of −0.46.[7] Based upon parallax measurements taken by the Gaia spacecraft, it is located at a distance of approximately 244 light-years (75 pc) from Earth.[1] The star is drifting closer with a radial velocity of −20 km/s.[1]
The primary is an A-type main-sequence star with a stellar classification of A1 V.[2] It is estimated to be estimated 388[9] million years old with a high rate of spin, showing a projected rotational velocity of around 118 km/s.[7] The elemental abundances in the stellar atmosphere are close to solar, with pronounced underabundances of aluminium and strontium.[6] The star has three[3] times the mass of the Sun and about 4.2[4] times the Sun's radius. It is radiating 161[8] times the luminosity of the Sun from its photosphere at an effective temperature of 9,622 K.[9]
The secondary component is a K-type main-sequence star with 0.6 times the mass and 0.57 times the mass of the Sun. Located at a projected separation of 26 milliarcseconds from the primary, this translates to a physical separation of 1.7 astronomical units. Albali A and B complete an orbit around their center of mass each 1.2 years.[4]
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