42 Aquarii

42 Aquarii
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Aquarius
Right ascension 22h 16m 48.04643s
Declination −12° 49 53.1673
Apparent magnitude (V) 5.34
Characteristics
Evolutionary stage giant
Spectral type K1 III
B−V color index 1.132±0.001
Astrometry
Radial velocity (Rv)+13.0±4.2 km/s
Proper motion (μ) RA: +1.89 mas/yr
Dec.: +5.03 mas/yr
Parallax (π)7.3032±0.1451 mas
Distance447 ± 9 ly
(137 ± 3 pc)
Absolute magnitude (MV)−0.93
Details
Mass3.14±0.27 M
Radius11.24+0.23
−0.32
 R
Luminosity69.950±3.907 L
Surface gravity (log g)2.90 cgs
Temperature4,980+71
−51
 K
Metallicity [Fe/H]+0.00±0.04 dex
Rotational velocity (v sin i)3.43 km/s
Age470±150 Myr
Other designations
42 Aqr, BD−13°6148, HD 211361, HIP 110000, HR 8496, SAO 164974
Database references
SIMBADdata

42 Aquarii is a single star located 447 light years away from the Sun in the zodiac constellation of Aquarius. 42 Aquarii is its Flamsteed designation. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 5.34. This object is moving further from the Sun with a heliocentric radial velocity of around +13 km/s.

This object is an evolved giant star with a stellar classification of K1 III, most likely (82% chance) on the horizontal branch. It is around 470 million years old with a projected rotational velocity of 3.4 km/s. The star has over three times the mass of the Sun and has expanded to 11 times the Sun's radius. It is radiating 70 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,980 K.