66 Tauri

66 Tauri
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
Right ascension 04h 23m 51.82553s
Declination +09° 27 39.4939
Apparent magnitude (V) 5.098 (5.8 / 5.9)
Characteristics
Spectral type A3V + A4V
U−B color index +0.10
B−V color index +0.07
Astrometry
Radial velocity (Rv)−8.70±1 km/s
Proper motion (μ) RA: −20.32 mas/yr
Dec.: −5.32 mas/yr
Parallax (π)8.24±0.31 mas
Distance400 ± 10 ly
(121 ± 5 pc)
Absolute magnitude (MV)−0.32
Orbit
Period (P)54.77 yr
Semi-major axis (a)0.188″
Eccentricity (e)0.720
Inclination (i)34.2°
Longitude of the node (Ω)239.8°
Periastron epoch (T)1937.24
Argument of periastron (ω)
(secondary)
332.0°
Details
66 Tau A
Mass2.89 M
Rotational velocity (v sin i)81 km/s
66 Tau B
Mass2.76 M
Other designations
r Tau, BD+09°570, HD 27820, HIP 20522, HR 1381, SAO 111791
Database references
SIMBADdata

66 Tauri, also known as r Tauri, is a binary star in the constellation of Taurus. The combined apparent magnitude of the system is 5.098, with the magnitudes of the two components being 5.8 and 5.9, respectively. Parallax measurements by Hipparcos put 66 Tauri at some 400 light-years (121 parsecs) away.

This is a visual binary where the positions of the two stars are tracked over time, and used to calculate an orbit. The two stars orbit each other every 55 years. Their orbit is fairly eccentric, at 0.720, and the two stars are separated by 0.188 on average. Both stars are A-type main-sequence stars with similar masses.