R Canis Majoris

R Canis Majoris
Location of R CMa (circled)
Observation data
Epoch J2000.0      Equinox
Constellation Canis Major
Right ascension 07h 19m 28.18202s
Declination −16° 23 42.8773
Apparent magnitude (V) 5.70 - 6.34
Characteristics
Spectral type F0V + G8IV
U−B color index +0.01
B−V color index +0.34
Variable type Algol
Astrometry
Radial velocity (Rv)−39.0 km/s
Proper motion (μ) RA: +165.37 mas/yr
Dec.: −136.18 mas/yr
Parallax (π)23.38±0.54 mas
Distance140 ± 3 ly
(42.8 ± 1.0 pc)
Absolute magnitude (MV)+2.57
Details
primary
Mass1.67 M
Radius1.78 R
Luminosity8.2 L
Surface gravity (log g)4.16 cgs
Temperature7,300 K
Rotational velocity (v sin i)78.3±3.9 km/s
secondary
Mass0.22 M
Radius1.22 R
Luminosity0.49 L
Surface gravity (log g)3.60 cgs
Temperature4,350 K
tertiary
Mass0.8 M
Radius0.83 R
Luminosity0.4 L
Surface gravity (log g)4.50 cgs
Other designations
R Canis Majoris, BD−16°1898, HR 2788, HD 57167, HIP 35487, SAO 152724, GC 9758
Database references
SIMBADdata

R Canis Majoris is an eclipsing interacting binary star system in the constellation Canis Major. It varies from magnitude 5.7 to 6.34. The system is unusual in the low mass ratio (ie. big mass difference) between the main two components and shortness of the orbital period. It is faintly visible to the naked eye of an observer with very good observing conditions.