Beta Cancri

Beta Cancri (β Cancri, abbreviated Beta Cnc, β Cnc), also named Tarf /ˈtɑːrf/, is the brightest star in the zodiacal constellation of Cancer. It has an apparent visual magnitude of +3.5 and an absolute magnitude of −1.2. Based on parallax measurements obtained during the Hipparcos mission, it is approximately 290 light-years distant from the Sun. An exoplanet, designated Beta Cancri b, is believed to be orbiting the star.

β Cancri
β Cancri is the bottom right star in the "crab"
Observation data
Epoch J2000      Equinox J2000
Constellation Cancer
Right ascension 08h 16m 30.9206s
Declination +09° 11 07.961
Apparent magnitude (V) 3.50 - 3.58
Characteristics
Spectral type K4III Ba1
U−B color index +1.77
B−V color index +1.48
Variable type Suspected
Astrometry
Radial velocity (Rv)22.94 km/s
Proper motion (μ) RA: −46.80 mas/yr
Dec.: −48.65 mas/yr
Parallax (π)11.23 ± 0.97 mas
Distance290 ± 30 ly
(89 ± 8 pc)
Absolute magnitude (MV)−1.218
Details
Mass1.7±0.1 M
Radius47.2±1.3 R
Luminosity794 L
Surface gravity (log g)1.5 cgs
Temperature4092.1±17.5 K
Metallicity [Fe/H]-0.29±0.06 dex
Rotational velocity (v sin i)3.7±0.8 km/s
Age1.85±0.34 Gyr
Other designations
Tarf, β Cancri, 17 Cancri, HR 3249, HD 69267, BD+09°1917, FK5 312, HIP 40526, SAO 116569, GC 11254, ADS 6704, CCDM 08165+0911, WDS J08165+0911A.
Database references
SIMBADdata

Beta Cancri has a companion listed and together they are designated WDS J08165+0911. As the primary, Beta Cancri bears the designation WDS J08165+0911A. The companion is designated WDS J08165+0911B.

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