37 Geminorum

37 Geminorum
Observation data
Epoch J2000      Equinox J2000
Constellation Gemini
Right ascension 06h 55m 18.66671s
Declination +25° 22 32.5038
Apparent magnitude (V) 5.74
Characteristics
Spectral type G0 V
U−B color index +0.01
B−V color index 0.573±0.010
Astrometry
Radial velocity (Rv)−14.94±0.15 km/s
Proper motion (μ) RA: −37.882 mas/yr
Dec.: +24.211 mas/yr
Parallax (π)57.2425±0.1005 mas
Distance57.0 ± 0.1 ly
(17.47 ± 0.03 pc)
Absolute magnitude (MV)4.56
Details
Mass1.146 M
Radius1.04+0.04
−0.08
 R
Luminosity1.310+0.003
−0.004
 L
Surface gravity (log g)4.29 cgs
Temperature6060+235
−118
 K
Metallicity [Fe/H]−0.25 dex
Rotation25.0 d
Rotational velocity (v sin i)1.89 km/s
Age5.49 Gyr
Other designations
BD+25°1496, GJ 252, HD 50692, HIP 33277, HR 2569, SAO 78866
Database references
SIMBADdata

37 Geminorum is a solitary Sun-like star located at the northwest part of the northern constellation of Gemini, about three degrees to the east of the bright star Epsilon Geminorum. The apparent visual magnitude of 37 Geminorum is 5.74, which is just bright enough to be visible to the naked eye on a dark night. It is located at a distance of 57 light years from the Sun based on parallax. This star is drifting closer with a radial velocity of −15 km/s, and is predicted to come as near as 13.8 light-years in approximately a million years. It is positioned close enough to the ecliptic to be subject to lunar occultations, such as happened on April 8, 1984.