Beta Corvi

Beta Corvi or β Corvi, officially named Kraz (/ˈkræz/), is the second-brightest star in the southern constellation of Corvus with an apparent visual magnitude of 2.647. Based on parallax measurements obtained during the Hipparcos mission, it is about 146 light-years (45 parsecs) distant from the Sun.

β Corvi
Location of β Corvi (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Corvus
Right ascension 12h 34m 23.23484s
Declination −23° 23 48.3374
Apparent magnitude (V) 2.647
Characteristics
Spectral type G5 II
U−B color index +0.586
B−V color index +0.898
R−I color index +0.44
Astrometry
Radial velocity (Rv)−7.6 km/s
Proper motion (μ) RA: +1.11 mas/yr
Dec.: −56.56 mas/yr
Parallax (π)22.39 ± 0.18 mas
Distance146 ± 1 ly
(44.7 ± 0.4 pc)
Absolute magnitude (MV)–0.61
Details
Mass3.7±0.1 M
Radius16 R
Luminosity164 L
Surface gravity (log g)2.52±0.03 cgs
Temperature5,100±80 K
Metallicity [Fe/H]–0.01 dex
Rotational velocity (v sin i)8 km/s
Age206 Myr
Other designations
Kraz, β Crv, Beta Corvi, Beta Crv, 9 Corvi, 9 Crv, BD−22 3401, CD−22 3401, −22 9505, CPD−22 5388, FK5 471, GC 17133, HD 109379, HIP 61359, HR 4786, SAO 180915, PPM 260512
Database references
SIMBADdata
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