Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Canes Venatici |
Right ascension | 13h 15m 31.95263s[1] |
Declination | +40° 51′ 18.7516″[1] |
Apparent magnitude (V) | 5.77[2] (5.87 + 9.48)[3] |
Characteristics | |
Evolutionary stage | main sequence[4] |
Spectral type | A7 V[5] |
B−V color index | 0.198±0.004[2] |
Astrometry | |
Radial velocity (Rv) | −21.1±2.6[6] km/s |
Proper motion (μ) | RA: −113.761[1] mas/yr Dec.: +19.858[1] mas/yr |
Parallax (π) | 13.7210 ± 0.1581 mas[1] |
Distance | 238 ± 3 ly (72.9 ± 0.8 pc) |
Absolute magnitude (MV) | 1.42[2] |
Orbit[7] | |
Period (P) | 219.2 yr |
Semi-major axis (a) | 0.745″ |
Eccentricity (e) | 0.686 |
Inclination (i) | 44.5° |
Longitude of the node (Ω) | 22.2° |
Periastron epoch (T) | 2201.7 |
Argument of periastron (ω) (secondary) | 273.3° |
Details | |
19 CVn A | |
Mass | 2.06±0.03[4] M☉ |
Radius | 2.5[8] R☉ |
Luminosity | 25.5+1.9 −1.8[4] L☉ |
Surface gravity (log g) | 4.09±0.14[9] cgs |
Temperature | 8,048±274[9] K |
Rotational velocity (v sin i) | 110[4] km/s |
Age | 366[9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
19 Canum Venaticorum is a binary star[7] system in the northern constellation of Canes Venatici, located approximately 238 light years from Sun based on its parallax. It is dimly visible to the naked eye as a white-hued star with an apparent visual magnitude of 5.77.[2] The pair orbit each other with a period of 219.2 years and an eccentricity of 0.686.[7] The system is moving closer to the Earth with a heliocentric radial velocity of −21 km/s.[6]
The magnitude +5.87 primary, component A, is an A-type main-sequence star with a stellar classification of A7 V.[3] It is 366[9] million years old with twice[4] the mass of the Sun and 2.5[8] times the Sun's radius. The star is radiating 25.5[4] times the Sun's luminosity from its photosphere at an effective temperature of 8,048 K.[9] It has a high rate of spin, showing a projected rotational velocity of 110 km/s.[4] As of 2012, its companion, designated component B, is a magnitude 9.48 star located 0.60 arcseconds from the primary along a position angle of 58°.[3]
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