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| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Canes Venatici |
| Right ascension | 13h 51m 47.47504s[1] |
| Declination | +34° 26′ 39.2474″[1] |
| Apparent magnitude (V) | 4.76[2] (4.73 – 4.85)[3] |
| Characteristics | |
| Spectral type | M3- IIIa[4] |
| B−V color index | 1.611±0.006[2] |
| Variable type | Lb[3] |
| Astrometry | |
| Radial velocity (Rv) | −44.21±0.25[2] km/s |
| Proper motion (μ) | RA: −20.477[1] mas/yr Dec.: −31.626[1] mas/yr |
| Parallax (π) | 5.2734 ± 0.2529[1] mas |
| Distance | 620 ± 30 ly (190 ± 9 pc) |
| Absolute magnitude (MV) | −1.56[2] |
| Details | |
| Mass | 2.18±0.16[5] M☉ |
| Radius | 117.41+4.25 −4.57[5] R☉ |
| Luminosity | 2,387±213[5] L☉ |
| Surface gravity (log g) | 0.98±0.30[6] cgs |
| Temperature | 3,529±25[6] K |
| Metallicity [Fe/H] | −0.09±0.11[6] dex |
| Age | 1.11±0.21[5] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
AW Canum Venaticorum is a variable star[3] in the constellation Canes Venatici. It is visible to the naked eye with a nominal apparent visual magnitude of 4.76.[2] The distance to this star, as measured from its annual parallax shift of 5.3 mas,[1] is around 620 light years. It is moving closer with a heliocentric radial velocity of −44 km/s.[2]

The variability of the brightness of HR 5219 was announced by Joel Stebbins and Charles Morse Huffer in 1928, based on observations made at Washburn Observatory.[9] It was given its variable star designation, AW Canum Venaticorum, in 1977.[10]
At the age of 1.1 billion years,[5] this is an evolved red giant star with a stellar classification of M3- IIIa.[4] It is a slow irregular variable of type Lb, with a brightness that ranges between magnitudes 4.73 and 4.85.[3] The star has 2.2[5] times the mass of the Sun and has expanded to 117[5] times the Sun's radius. It is radiating 2,387[5] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,529 K.[6]