HD 37124

HD 37124 is a star in the equatorial constellation of Taurus (the Bull), positioned about a half degree to the SSW of the bright star Zeta Tauri. The apparent visual magnitude of this star is 7.68, which is too dim to be visible to the naked eye. It is located at a distance of 103 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −23 km/s. Three extrasolar planets have been found to orbit the star.

HD 37124
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Taurus
Right ascension 05h 37m 02.4867s
Declination +20° 43 50.8346
Apparent magnitude (V) 7.68
Characteristics
Spectral type G4IV-V
B−V color index 0.667±0.008
Astrometry
Radial velocity (Rv)−23.02±0.09 km/s
Proper motion (μ) RA: −79.607±0.184 mas/yr
Dec.: −420.161±0.166 mas/yr
Parallax (π)31.5536 ± 0.0751 mas
Distance103.4 ± 0.2 ly
(31.69 ± 0.08 pc)
Absolute magnitude (MV)5.05
Details
Mass0.81±0.01 M
0.92±0.01 M
Radius0.92±0.02 R
0.91+0.01
−0.04
 R
Luminosity0.839±0.003 L
0.772+0.003
−0.002
 L
Surface gravity (log g)4.41±0.01 cgs
Temperature5,763±22 K
Metallicity [Fe/H]−0.38±0.01 dex
−0.45 dex
Rotational velocity (v sin i)3.6 km/s
Age11.8±1.2 Gyr
10.62±1.74 Gyr
Other designations
BD+20°1018, GJ 209, HD 37124, HIP 26381, SAO 77323, G 100-27
Database references
SIMBADdata

The stellar classification of HD 37124 is G4IV-V, showing a spectrum with blended traits of a main sequence star and a more evolved subgiant star. It is a quiet star with a low activity index. This star is smaller than the Sun, with 81–92% of the mass of the Sun and around 92% of the Sun's radius. It is an older, thick disk star with an age of around 11 billion years, and is spinning with a projected rotational velocity of 3.6 km/s. The metallicity of the star, what astronomers term the abundance of heavier elements, is much lower than in the Sun with an iron abundance of 35–41%. It is radiating 77–84% of the Sun's luminosity from its photosphere at an effective temperature of 5,763 K.

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