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Star in the constellation Canes Venatici From Wikipedia, the free encyclopedia
R Canum Venaticorum is a Mira variable star in the constellation Canes Venatici. It ranges between magnitudes 6.5 and 12.9 over a period of approximately 329 days.[3]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Canes Venatici |
Right ascension | 13h 48m 57.0416s[2] |
Declination | +39° 32′ 33.174″[2] |
Apparent magnitude (V) | 6.5 - 12.9[3] |
Characteristics | |
Spectral type | M5.5e-M9e[3] |
U−B color index | +0.41[4] |
B−V color index | +1.22[4] |
Variable type | Mira[3] |
Astrometry | |
Radial velocity (Rv) | −6.80[5] km/s |
Proper motion (μ) | RA: −1.115[2] mas/yr Dec.: −5.148[2] mas/yr |
Parallax (π) | 2.1711 ± 0.1262 mas[2] |
Distance | 1,500 ± 90 ly (460 ± 30 pc) |
Details | |
Mass | 2.26[6] M☉ |
Radius | 664[6] R☉ |
Luminosity | 29,251[7] L☉ |
Temperature | 3,108[7] K |
Other designations | |
Database references | |
SIMBAD | data |
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