Beta Canum Venaticorum

Beta Canum Venaticorum (β Canum Venaticorum, abbreviated Beta CVn, β CVn), also named Chara /ˈkɛərə/, is a G-type main-sequence star in the northern constellation of Canes Venatici. At an apparent visual magnitude of 4.25, it is the second-brightest star in the constellation. Based upon an annual parallax shift of 118 mas, this star is 27.6 light-years (8.5 parsecs) distant from the Sun.

β Canum Venaticorum
Location of β Canum Venaticorum (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Canes Venatici
Right ascension 12h 33m 44.54425s
Declination +41° 21 26.9214
Apparent magnitude (V) 4.25
Characteristics
Spectral type G0 V
U−B color index 0.04
B−V color index 0.58
Astrometry
Radial velocity (Rv)+6.9 km/s
Proper motion (μ) RA: −704.702 mas/yr
Dec.: +292.155 mas/yr
Parallax (π)118.0266 ± 0.1530 mas
Distance27.63 ± 0.04 ly
(8.47 ± 0.01 pc)
Absolute magnitude (MV)4.64
Details
Mass0.97±0.04 M
Radius1.123±0.028 R
Luminosity1.151±0.018 L
Surface gravity (log g)4.60 cgs
Temperature6043±183 K
Metallicity [Fe/H]−0.18 dex
Rotational velocity (v sin i)2.9±0.4 km/s
Age3.4 to 7.1 Gyr
Other designations
Chara, Asterion, Beta CVn, 8 CVn, BD +42 2321, FK5 470, HD 109358, HIP 61317, HR 4785, SAO 44230
Database references
SIMBADdata
ARICNSdata

Along with the brighter star Cor Caroli, the pair form the "southern dog" in this constellation that represents hunting dogs.

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