19 Canum Venaticorum

19 Canum Venaticorum
Observation data
Epoch J2000      Equinox J2000
Constellation Canes Venatici
Right ascension 13h 15m 31.95263s
Declination +40° 51 18.7516
Apparent magnitude (V) 5.77 (5.87 + 9.48)
Characteristics
Evolutionary stage main sequence
Spectral type A7 V
B−V color index 0.198±0.004
Astrometry
Radial velocity (Rv)−21.1±2.6 km/s
Proper motion (μ) RA: −113.761 mas/yr
Dec.: +19.858 mas/yr
Parallax (π)13.7210±0.1581 mas
Distance238 ± 3 ly
(72.9 ± 0.8 pc)
Absolute magnitude (MV)1.42
Orbit
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
Mass2.06±0.03 M
Radius2.5 R
Luminosity25.5+1.9
−1.8
 L
Surface gravity (log g)4.09±0.14 cgs
Temperature8,048±274 K
Rotational velocity (v sin i)110 km/s
Age366 Myr
Other designations
19 CVn, BD+41°2374, FK5 461, HD 115271, HIP 64692, HR 5004, SAO 44531, WDS J13155+4051
Database references
SIMBADdata

19 Canum Venaticorum is a binary star 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. The pair orbit each other with a period of 219.2 years and an eccentricity of 0.686. The system is moving closer to the Earth with a heliocentric radial velocity of −21 km/s.

The magnitude +5.87 primary, component A, is an A-type main-sequence star with a stellar classification of A7 V. It is 366 million years old with twice the mass of the Sun and 2.5 times the Sun's radius. The star is radiating 25.5 times the Sun's luminosity from its photosphere at an effective temperature of 8,048 K. It has a high rate of spin, showing a projected rotational velocity of 110 km/s. 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°.