Kappa Arietis

Kappa Arietis
Location of κ Arietis (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Aries
Right ascension 02h 06m 33.92497s
Declination +22° 38 53.9476
Apparent magnitude (V) 5.02
Characteristics
Spectral type A2m
U−B color index +0.11
B−V color index +0.12
Astrometry
Radial velocity (Rv)+11.5 km/s
Proper motion (μ) RA: +20.348 mas/yr
Dec.: −35.671 mas/yr
Parallax (π)18.0292±0.3092 mas
Distance181 ± 3 ly
(55.5 ± 1.0 pc)
Absolute magnitude (MV)1.30
Orbit
Period (P)15.2938 d
Eccentricity (e)0.61
Periastron epoch (T)2,421,844.121 JD
Argument of periastron (ω)
(secondary)
358.3°
Semi-amplitude (K1)
(primary)
34.5 km/s
Semi-amplitude (K2)
(secondary)
35.4 km/s
Details
Mass2.09±0.31 M
Radius2.32±0.08 R
Luminosity24.4±1.3 L
Surface gravity (log g)4.03±0.07 cgs
Temperature8,421±125 K
Metallicity [Fe/H]+0.18 dex
Rotational velocity (v sin i)18 km/s
Other designations
κ Ari, 12 Arietis, BD+21°279, GC 2527, HD 12869, HIP 9836, HR 613, SAO 75146, PM 91364
Database references
SIMBADdata

Kappa Arietis is a binary star system in the northern constellation of Aries. Its name is a Bayer designation that is Latinized from κ Arietis, and abbreviated Kappa Ari or κ Ari. The combined apparent visual magnitude of the pair is 5.02, making the system bright enough for it to be dimly visible to the naked eye as a white-hued point of light. It is located approximately 181 light-years from the Sun based on parallax, and is drifting further away with a radial velocity of +11.5 km/s.

The binary nature of this system was announced in 1918 by Lick Observatory. It is a double-lined spectroscopic binary with an orbital period of 15.3 days and an eccentricity of 0.61. Both components displaying the spectral properties of an Am, or metallic-lined star. They have nearly the same brightness and their mass ratio is 1.03; very close to equal.