R Canis Majoris

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 ratio between the main two components and shortness of the orbital period.

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
Distance44 pc
Absolute magnitude (MV)+2.57
Details
Mass1.67 + 0.22 + 0.8 M
Radius1.78 + 1.22 + 0.83 R
Luminosity8.2 + 0.49 + 0.4 L
Surface gravity (log g)4.16 + 3.60 + 4.50 cgs
Temperature6,964 K
Rotational velocity (v sin i)78.3±3.9 km/s
Other designations
R Canis Majoris, BD16° 1898, HR 2788, HD 57167, HIP 35487, SAO 152724, GC 9758
Database references
SIMBADdata
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.