24 Aquarii

24 Aquarii
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension 21h 39m 31.53468s
Declination −00° 03′ 04.1095″
Apparent magnitude (V) 6.66
(7.08 + 15.11 + 7.90)
Characteristics
Evolutionary stage main sequence
Spectral type F5.5V + M5V + F8V
U−B color index +0.04
+0.005 (Aa)
+1.13 (Ab)
+0.15 (B)
B−V color index +0.514
+0.459 (Aa)
+1.701 (Ab)
+0.642 (B)
Astrometry
Radial velocity (Rv)−15.86±0.06 km/s
Proper motion (μ) RA: +215.367 mas/yr
Dec.: +17.077 mas/yr
Parallax (π)22.63±0.25 mas
Distance144 ± 2 ly
(44.2 ± 0.5 pc)
Absolute magnitude (MV)3.45
Orbit
Primary24 Aqr A
Name24 Aqr B
Period (P)48.98±0.07 yr
Semi-major axis (a)0.4250±0.0005
Eccentricity (e)0.8610±0.0002
Inclination (i)55.00±0.04°
Longitude of the node (Ω)140.26±0.05°
Periastron epoch (T)2020.799±0.003
Argument of periastron (ω)
(secondary)
293.95±0.07°
Orbit
Primary24 Aqr Aa
Name24 Aqr Ab
Period (P)5.883933(15) days
Semi-major axis (a)0.0706±0.0019 AU
Eccentricity (e)0.071±0.006
Inclination (i)55.8±2.9°
Periastron epoch (T)46,988.58±0.08 MJD
Argument of periastron (ω)
(secondary)
286±5°
Semi-amplitude (K1)
(primary)
14.60±0.09 km/s
Details
24 Aqr Aa
Mass1.12±0.06 M
Radius1.23±0.04 R
Luminosity2.4±0.1 L
Surface gravity (log g)4.40±0.06 cgs
Temperature6,483±80 K
Metallicity [Fe/H]–0.09 dex
Age3.612 Gyr
24 Aqr Ab
Mass0.24±0.05 M
Radius0.28±0.04 R
Surface gravity (log g)4.80±0.06 cgs
Age3.612 Gyr
24 Aqr B
Mass1.06±0.05 M
Radius1.02±0.04 R
Luminosity1.33±0.05 L
Surface gravity (log g)4.47±0.06 cgs
Temperature6,150±80 K
Age3.612 Gyr
Other designations
24 Aqr, BD−00°4245, HD 206058, HIP 106942, SAO 145566, WDS J21395-0003, LTT 8626
Database references
SIMBADdata

24 Aquarii is a triple star system in the equatorial constellation of Aquarius. 24 Aquarii is the Flamsteed designation. The apparent magnitude of this system is 6.66, 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. Based on a dynamical parallax measurement, the system is located at a distance of 144 light-years (44 parsecs). The system is moving closer to the Earth with a heliocentric radial velocity of −16 km/s.

The components A and B make up a visual binary wiith an orbital period of 48.98 years and a high eccentricity of 0.8610. Both are main sequence stars with spectral types of F5.5V and F8V, respectively. Component A is itself a single-lined spectroscopic binary with a period of 5.8839 days and an eccentricity of 0.071±0.006, being orbited by a faint red dwarf with a spectral type of M5V.