52 Arietis

52 Arietis
Observation data
Epoch J2000      Equinox J2000
Constellation Aries
Right ascension 03h 05m 26.68819s
Declination +25° 15 18.6257
Apparent magnitude (V) 5.46
Characteristics
Spectral type B7 V + B7 V
U−B color index -0.38
B−V color index -0.03
Astrometry
Radial velocity (Rv)9 km/s
Proper motion (μ) RA: +1.44 mas/yr
Dec.: -10.26 mas/yr
Parallax (π)6.05±1.06 mas
Distanceapprox. 540 ly
(approx. 170 pc)
Orbit
Primary52 Ari A
Companion52 Ari B
Period (P)227 yr
Semi-major axis (a)0.47″
Eccentricity (e)0.73
Inclination (i)77.5°
Longitude of the node (Ω)92.8°
Periastron epoch (T)1938.5
Details
52 Ari A
Mass5.12 M
Radius3.3 R
Luminosity452 L
Temperature12,912 K
Rotational velocity (v sin i)159 km/s
52 Ari B
Mass5.12 M
Other designations
52 Arietis, ADS 2336, BD+24° 431, HIP 14376.
52 Ari A: HD 19134, HR 927.
52 Ari B: HD 19135, HR 928.
Database references
SIMBAD52 Ari
52 Ari A
52 Ari B

52 Arietis (abbreviated 52 Ari) is a triple star system in the northern constellation of Aries. 52 Arietis is the Flamsteed designation. The combined apparent magnitude is +5.46, which is bright enough to be faintly visible to the naked eye. Based upon an annual parallax shift of 6.05 mas, the system is roughly 540 light-years (170 parsecs) distant from the Earth. The inner pair of this system consist of two nearly identical B-type main sequence stars, each with about five times the mass of the Sun. The tertiary component is a smaller star with 88% of the Sun's mass, and is a common proper motion companion.