41 Aquarii

41 Aquarii
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension 22h 14m 18.03271s
Declination −21° 04 28.4330
Apparent magnitude (V) 5.354
Characteristics
Spectral type K0 III + F8 V
U−B color index +0.465
B−V color index +0.834
Astrometry
41 Aqr A
Radial velocity (Rv)−24.94±0.13 km/s
Proper motion (μ) RA: +24.827 mas/yr
Dec.: +54.923 mas/yr
Parallax (π)13.7811±0.1850 mas
Distance237 ± 3 ly
(72.6 ± 1.0 pc)
Proper motion (μ) RA: +27.266 mas/yr
Dec.: +57.272 mas/yr
Parallax (π)13.5404 ± 0.0719 mas
Distance241 ± 1 ly
(73.9 ± 0.4 pc)
Details
41 Aqr A
Radius7.88+0.09
−0.13
 R
Luminosity33.93±0.53 L
Surface gravity (log g)2.85 cgs
Temperature4,750 K
Metallicity [Fe/H]−0.13 dex
41 Aqr B
Radius1.76+0.29
−0.06
 R
Luminosity6.319±0.043 L
Temperature6,899+115
−506
 K
Other designations
41 Aqr, BD−21°6180, HD 210960, HIP 109786, HR 8480, SAO 190986, WDS J22143-2104
Database references
SIMBADdata

41 Aquarii is a double star in the equatorial constellation of Aquarius. 41 Aquarii is its Flamsteed designation. It is visible to the naked eye as a dim, orange-hued point of light with a combined apparent visual magnitude of 5.354. The pair are located at a distance of around 239 light-years (73 parsecs) from the Sun based on parallax, but are drifting closer with a radial velocity of –25 km/s.

The brighter component of the pair is a red clump giant star with a stellar classification of K0 III and a magnitude of 5.73. This is an aging star that has exhausted the supply of hydrogen at its core and is now generating energy through core helium fusion. It has eight times the girth of the Sun and is radiating 34 times the luminosity of the Sun at an effective temperature of 4,750 K.

At an angular separation of 5.148 arcseconds, the fainter companion is an F-type main sequence star with a magnitude 7.16 and a classification of F8 V. It has 1.8 times the Sun's radius and is radiating six times the Sun's luminosity from its photosphere at 6,899 K.