47 Tauri

47 Tauri (abbreviated to 47 Tau) is a binary star in the zodiac constellation of Taurus. Parallax measurements made by the Hipparcos spacecraft put it at a distance of about 330 light-years (102 parsecs) from Earth. The system has a combined apparent magnitude of about 4.89, meaning it can be faintly seen with the naked eye, according to the Bortle scale.

47 Tauri
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
Right ascension 04h 13m 56.38482s
Declination +09° 15 49.7729
Apparent magnitude (V) 4.89
(5.05 + 7.32)
Characteristics
Spectral type G5III + A7V:
U−B color index +0.46
B−V color index +0.82
Astrometry
Radial velocity (Rv)-8.2 ± 0.4 km/s
Proper motion (μ) RA: -10.31 mas/yr
Dec.: -30.01 mas/yr
Parallax (π)9.83 ± 0.64 mas
Distance330 ± 20 ly
(102 ± 7 pc)
Orbit
Period (P)479 yr
Semi-major axis (a)1.053″
Eccentricity (e)0.910
Inclination (i)128.6°
Longitude of the node (Ω)52.9°
Periastron epoch (T)B 1816.6
Argument of periastron (ω)
(secondary)
263.0°
Details
47 Tau A
Radius12.9 R
Surface gravity (log g)2.67 ± 0.11 cgs
Temperature5117 ± 58 K
Metallicity [Fe/H]-0.10 ± 0.08 dex
Other designations
BD+08° 652, HD 26722, HIP 19740, HR 1311, SAO 111674
Database references
SIMBAD47 Tau
47 Tau A
47 Tau B

47 Tauri is a visual binary, meaning that the two components can be resolved, and the orbit is derived from the positions of the two stars. The primary component is a G-type giant. Its radius is about 13 times that of the Sun. The companion is likely a white-colored A-type main-sequence star that is fainter. The two stars are separated about 1.3 arcseconds away, and because of their large separation, the two stars take some 479 years to complete an orbit.

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