Observation data Equinox J2000.0]] (ICRS) | |
---|---|
Constellation | Canes Venatici |
Right ascension | 13h 51m 47.47504s[2] |
Declination | +34° 26′ 39.2474″[2] |
Apparent magnitude (V) | 4.76[3] (4.73 – 4.85)[4] |
Characteristics | |
Spectral type | M3- IIIa[5] |
B−V color index | 1.611±0.006[3] |
Variable type | Lb[4] |
Astrometry | |
Radial velocity (Rv) | −44.21±0.25[3] km/s |
Proper motion (μ) | RA: −20.477[2] mas/yr Dec.: −31.626[2] mas/yr |
Parallax (π) | 5.2734 ± 0.2529[2] mas |
Distance | 620 ± 30 ly (190 ± 9 pc) |
Absolute magnitude (MV) | −1.56[3] |
Details | |
Mass | 2.18±0.16[6] M☉ |
Radius | 117.41+4.25 −4.57[6] R☉ |
Luminosity | 2,387±213[6] L☉ |
Surface gravity (log g) | 0.98±0.30[7] cgs |
Temperature | 3,529±25[7] K |
Metallicity [Fe/H] | −0.09±0.11[7] dex |
Age | 1.11±0.21[6] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
AW Canum Venaticorum is a variable star[4] in the constellation Canes Venatici. It is visible to the naked eye with a nominal apparent visual magnitude of 4.76.[3] The distance to this star, as measured from its annual parallax shift of 5.3 mas,[2] is around 620 light years. It is moving closer with a heliocentric radial velocity of −44 km/s.[3]
At the age of 1.1 billion years,[6] this is an evolved red giant star with a stellar classification of M3- IIIa.[5] It is a slow irregular variable of type Lb, with a brightness that ranges between magnitudes 4.73 and 4.85.[4] The star has 2.2[6] times the mass of the Sun and has expanded to 117[6] times the Sun's radius. It is radiating 2,387[6] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,529 K.[7]
Original source: https://en.wikipedia.org/wiki/AW Canum Venaticorum.
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