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.
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 |
Distance | 146 ± 1 ly (44.7 ± 0.4 pc) |
Absolute magnitude (MV) | –0.61 |
Details | |
Mass | 3.7±0.1 M☉ |
Radius | 16 R☉ |
Luminosity | 164 L☉ |
Surface gravity (log g) | 2.52±0.03 cgs |
Temperature | 5,100±80 K |
Metallicity [Fe/H] | –0.01 dex |
Rotational velocity (v sin i) | 8 km/s |
Age | 206 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 | |
SIMBAD | data |
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