Nu3 Canis Majoris

Nu3 Canis Majoris
Location of ν3 Canis Majoris (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Canis Major
Right ascension 06h 37m 53.421s
Declination −18° 14′ 14.93″
Apparent magnitude (V) 4.41 (4.63 + 8.56)
Characteristics
Evolutionary stage horizontal branch
Spectral type K0 II-III
U−B color index +1.04
B−V color index +1.16
Astrometry
Radial velocity (Rv)−1.50±0.70 km/s
Proper motion (μ) RA: −7.166 mas/yr
Dec.: −8.777 mas/yr
Parallax (π)6.7876±0.1054 mas
Distance481 ± 7 ly
(147 ± 2 pc)
Absolute magnitude (MV)−1.13
Details
ν3 CMa A
Mass3.38±0.37 M
Radius32.7 R
Luminosity398 L
Surface gravity (log g)2.34 cgs
Temperature4,510 K
Metallicity [Fe/H]−0.24 dex
Rotation183 d
Rotational velocity (v sin i)8 km/s
Age380±20 Myr
Other designations
HDS 915, ν3 CMa, 8 Canis Majoris, BD−18°1492, GC 8660, HD 47442, HIP 31700, HR 2443, SAO 151730, CCDM 06379-1814, WDS J06379-1814A
Database references
SIMBADdata

Nu3 Canis Majoris is a binary star system in the southern constellation of Canis Major. Its name is a Bayer designation that is Latinized from ν3 Canis Majoris, and abbreviated Nu3 CMa or ν3 CMa. The star system, appearing as one star, is deemed visible to the naked eye with its combined apparent visual magnitude of 4.41. Based upon an annual parallax shift of 6.79 mas as seen from Earth, this system is approximately 481 light-years (147 pc) distant from the Sun.