Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquarius |
Right ascension | 21h 39m 31.53468s[1] |
Declination | −00° 03′ 04.1095″[1] |
Apparent magnitude (V) | 6.66[2] |
Characteristics | |
Spectral type | F7 III[3] OR F7V + ? + F9V[4] |
B−V color index | +0.52[5] |
Astrometry | |
Radial velocity (Rv) | −15.86±0.06[2] km/s |
Proper motion (μ) | RA: +215.367[1] mas/yr Dec.: +17.077[1] mas/yr |
Parallax (π) | 25.0839 ± 0.6277 mas[1] |
Distance | 130 ± 3 ly (39.9 ± 1.0 pc) |
Absolute magnitude (MV) | 3.45[2] |
Orbit[6] | |
Period (P) | 48.65 yr |
Semi-major axis (a) | 0.448″ |
Eccentricity (e) | 0.868 |
Inclination (i) | 58.0° |
Longitude of the node (Ω) | 139.3° |
Periastron epoch (T) | 1971.55 |
Argument of periastron (ω) (secondary) | 293.0° |
Details[7] | |
24 Aqr Aa | |
Mass | 1.25 M☉ |
Radius | 1.42+0.05 −0.08[1] R☉ |
Luminosity | 2.864±0.080[1] L☉ |
Temperature | 6,231 K |
Metallicity [Fe/H] | –0.09 dex |
Age | 3.5 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
24 Aquarii is a triple star[6] system in the equatorial constellation of Aquarius. 24 Aquarii is the Flamsteed designation. The apparent magnitude of this system is 6.66,[2] which, according to the Bortle Dark-Sky Scale, means it is a faint star that is just visible to the naked eye from dark, rural skies. It has an annual parallax shift of 25.08 mas,[1] which is equivalent to a distance of 130 light-years (40 parsecs) from Earth. The system is moving closer to the Earth with a heliocentric radial velocity of −16 km/s.[2]
The calculated orbit of the visual binary has a period of 48.65 years and a large eccentricity of 0.868.[6] The primary, component A, is itself a single-lined spectroscopic binary with a period of 5.8839 days and an eccentricity of 0.071±0.006.[4] One study gives the system a stellar classification of F7 III,[3] suggesting it contains an evolved giant star. Other classifications give classes matching F-type main-sequence stars for components Aa and B.[4]
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