HD 23474

HD 23474
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Mensa
Right ascension 03h 36m 30.1435s
Declination −78° 19 23.0623
Apparent magnitude (V) 6.30±0.01
Characteristics
Spectral type K2 III
U−B color index +1.03
B−V color index +1.15
Astrometry
Radial velocity (Rv)2.4±0.4 km/s
Proper motion (μ) RA: −14.12 mas/yr
Dec.: +6.67 mas/yr
Parallax (π)4.34±0.36 mas
Distance750 ± 60 ly
(230 ± 20 pc)
Absolute magnitude (MV)−0.50
Details
Mass1.21 M
Radius33.51±7.44 R
Luminosity227 L
Surface gravity (log g)1.22 cgs
Temperature4,556 K
Metallicity [Fe/H]−0.03 dex
Rotational velocity (v sin i)1.2±1.3 km/s
Other designations
3 G. Mensae, CPD−78°105, FK5 2261, GC 4400, HD 23474, HIP 16827, HR 1154, SAO 256005, WDS J03365-7819AB
Database references
SIMBADdata

HD 23474 (HR 1154) is a double star in the southern circumpolar constellation Mensa. It has an apparent magnitude of 6.30, placing it near the max naked eye visibility. The system is situated at a distance of about 750 light years and is currently receding with a heliocentric radial velocity of 2.4 km/s.

As of 2018, the pair have a separation of 0.2 arcseconds along a position angle of 92°.

The primary or visible component has a stellar classification of K2 III, indicating that it is a red giant. As a result, it has expanded to a diameter of 33.51 R and has an effective temperature of 4,556 K, giving an orange hue. It has 121% the mass of the Sun and shines with a luminosity of 227 L from its enlarged photosphere. HD 23474 spins with a poorly constrained projected rotational velocity of 1.2 km/s and has a metallicity around solar level.