Observation data Epoch J2000.0 Equinox | |
---|---|
Constellation | Canis Major |
Right ascension | 07h 19m 28.18202s[1] |
Declination | −16° 23′ 42.8773″[1] |
Apparent magnitude (V) | 5.70 - 6.34[2] |
Characteristics | |
Spectral type | F0V + G8IV[3] |
U−B color index | +0.01[3] |
B−V color index | +0.34[3] |
Variable type | Algol |
Astrometry | |
Radial velocity (Rv) | -39.0[4] km/s |
Proper motion (μ) | RA: 165.37[1] mas/yr Dec.: −136.18[1] mas/yr |
Parallax (π) | 23.38 ± 0.54 mas[1] |
Distance | 44[3] pc |
Absolute magnitude (MV) | +2.57[5] |
Details[3] | |
Mass | 1.67 + 0.22 + 0.8 M☉ |
Radius | 1.78 + 1.22 + 0.83 R☉ |
Luminosity | 8.2 + 0.49 + 0.4 L☉ |
Surface gravity (log g) | 4.16 + 3.60 + 4.50 cgs |
Temperature | 6,964[5] K |
Rotational velocity (v sin i) | 78.3±3.9[5] km/s |
Other designations | |
Database references | |
SIMBAD | data |
R Canis Majoris is an eclipsing interacting binary star system in the constellation Canis Major. It varies from magnitude 5.7 to 6.34.[6] The system is unusual in the low ratio between the main two components and shortness of the orbital period.[3]
budding
was invoked but never defined (see the help page).