HD 45184

HD 45184
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Canis Major
Right ascension 06h 24m 43.87975s
Declination −28° 46 48.4163
Apparent magnitude (V) 6.37
Characteristics
Evolutionary stage main sequence
Spectral type G2Va
Apparent magnitude (B) 6.996
Apparent magnitude (J) 5.219
Apparent magnitude (H) 4.962
Apparent magnitude (K) 4.871
B−V color index 0.626±0.007
Astrometry
Radial velocity (Rv)−3.828±0.0003 km/s
Proper motion (μ) RA: −165.257 mas/yr
Dec.: −121.826 mas/yr
Parallax (π)45.5224±0.0320 mas
Distance71.65 ± 0.05 ly
(21.97 ± 0.02 pc)
Absolute magnitude (MV)4.67
Details
Mass1.08±0.04 M
Radius1.05±0.02 R
Luminosity1.178+0.002
−0.001
 L
Surface gravity (log g)4.47±0.02 cgs
Temperature5,862+72
−48
 K
Metallicity [Fe/H]0.070±0.016 dex
Rotation20.0±0.1 d
Rotational velocity (v sin i)2.1 km/s
Age3.0+0.7
−1.4
 Gyr
Other designations
CD−29°2981, GJ 3394, HD 45184, HIP 30503, HR 2318, SAO 171711, PPM 250356
Database references
SIMBADdata
Exoplanet Archivedata

HD 45184 is a star in the southern constellation of Canis Major. It is a yellow-hued star near the lower limit of visibility to the naked eye with an apparent visual magnitude of 6.37. The star is located at a distance of 71.65 light years from the Sun based on parallax. It is drifting closer with a radial velocity of −3.8 km/s.

This object is an ordinary G-type main-sequence star with a stellar classification of G2Va, and it is considered a solar twin. The mass, size, and luminosity of the star are slightly higher than for the Sun, and it has a near solar metallicity – what astronomers term the abundance of elements with higher atomic numbers than helium. The star is around three billion years old and is spinning with a 20-day period. It has a 5.14-year magnetic activity cycle that has a lower amplitude than on the Sun.