HD 3765

HD 3765
View of the Andromeda Galaxy, with HD 3765 circled in red. The star is much closer than Andromeda, within the Milky Way galaxy.
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension 00h 40m 49.270s
Declination +40° 11 13.82
Apparent magnitude (V) 7.34
Characteristics
Evolutionary stage Main sequence
Spectral type K2V
Astrometry
Radial velocity (Rv)−63.33±0.12 km/s
Proper motion (μ) RA: 356.318 mas/yr
Dec.: −669.205 mas/yr
Parallax (π)55.8412±0.0235 mas
Distance58.41 ± 0.02 ly
(17.908 ± 0.008 pc)
Absolute magnitude (MV)6.16
Details
Mass0.852+0.020
−0.044
 M
Radius0.79±0.02 R
Luminosity0.383±0.011 L
Surface gravity (log g)4.58±0.03 cgs
Temperature5076+115
−160
 K
Metallicity [Fe/H]0.25 dex
Rotational velocity (v sin i)2 km/s
Other designations
BD+39 154, GJ 28, HD 3765, HIP 3206, SAO 54074, LHS 1125, Wolf 12
Database references
SIMBADdata
Exoplanet Archivedata

HD 3765 is a single K-type main-sequence star in the constellation of Andromeda, near the Andromeda Galaxy in the sky. Its surface temperature is about 5076 K. HD 3765 has an orange hue and is too faint to be seen with the naked eye, but can be seen with a small telescope. It has an apparent visual magnitude of 7.34. Based upon parallax measurements, it is located 58.4 light-years from the Sun. The object is drifting towards the Sun with a radial velocity of −63.3 km/s.