Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aries |
Right ascension | 02h 49m 59.03324s[1] |
Declination | +27° 15′ 37.8260″[1] |
Apparent magnitude (V) | 3.63[2] |
Characteristics | |
Spectral type | B8 Vn[3] |
U−B color index | –0.38[2] |
B−V color index | –0.10[2] |
Astrometry | |
Radial velocity (Rv) | +4[4] km/s |
Proper motion (μ) | RA: +66.81[1] mas/yr Dec.: –116.52[1] mas/yr |
Parallax (π) | 19.69 ± 0.19 mas[1] |
Distance | 166 ± 2 ly (50.8 ± 0.5 pc) |
Details | |
Mass | 3.1±0.1[5] M☉ |
Luminosity | 160[6] L☉ |
Temperature | 11900[6] K |
Rotational velocity (v sin i) | 175[7] km/s |
Age | 130+10 −30[5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
41 Arietis (abbreviated 41 Ari) is a triple star system in the northern constellation of Aries. With an apparent visual magnitude of 3.63,[2] this system is readily visible to the naked eye. It has an annual parallax shift of 19.69 mas,[1] which indicates it is at a distance of 166 light-years (51 parsecs) from the Sun.
The system consists of a binary pair,[9] designated 41 Arietis A, together with a third companion star, 41 Arietis D. (41 Arietis B and C form optical pairs with A, but are not physically related.[10]) The components of A are themselves designated 41 Arietis Aa (formally named Bharani /ˈbærəni/)[11] and Ab.
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