HD 102365

HD 102365
Observation data
Epoch J2000      Equinox J2000
Constellation Centaurus
A
Right ascension 11h 46m 31.07253s
Declination −40° 30 01.2859
Apparent magnitude (V) 4.88
B
Right ascension 11h 46m 32.68988s
Declination −40° 29 47.6048
Apparent magnitude (V) 15
Characteristics
Spectral type G2V + M4V
U−B color index 0.10
B−V color index 0.67
Astrometry
A
Radial velocity (Rv)16.94±0.12 km/s
Proper motion (μ) RA: −1530.971 mas/yr
Dec.: +403.287 mas/yr
Parallax (π)107.3024±0.0873 mas
Distance30.40 ± 0.02 ly
(9.319 ± 0.008 pc)
Absolute magnitude (MV)5.07
B
Radial velocity (Rv)17.23±0.27 km/s
Proper motion (μ) RA: −1534.679 mas/yr
Dec.: +381.396 mas/yr
Parallax (π)107.4237 ± 0.0351 mas
Distance30.362 ± 0.010 ly
(9.309 ± 0.003 pc)
Details
A
Mass0.84+0.04
−0.03
 M
Radius0.99±0.02 R
Luminosity0.86±0.05 L
Surface gravity (log g)4.44±0.03 cgs
Temperature5,594+49
−50
 K
Metallicity [Fe/H]−0.28 dex
Rotational velocity (v sin i)0.5 km/s
Age4.5–5.7 Gyr
Other designations
66 G. Cen, CD−39°7301, GJ 442, HD 102365, HIP 57443, HR 4523, SAO 223020, LHS 311, LTT 4373, PLX 2725.00
B: LHS 313, VB 5
Database references
SIMBADA
B
Exoplanet Archivedata
ARICNSdata

HD 102365 (66 G. Centauri) is a binary star system that is located in the northeastern part of the Centaurus constellation, at a distance of about 30.4 light-years (9.3 parsecs) from the Solar System. The larger member of the system is a G-type star that is smaller than the Sun but of similar mass. It has a common proper motion companion that was discovered by W. J. Luyten in 1960. This M-type star appears to be in a wide orbit around the primary at a current separation of about 211 astronomical units (AU), (or 211 times the separation of the Earth from the Sun). By comparison, Neptune orbits at an average distance of 30 AU.