27 Arietis

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Template:Short description

27 Arietis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Aries
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 6.21[2]
Characteristics
Spectral type G8 III-IV Fe-2[3]
B−V Template:Engvar Script error: No such module "val".[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[2] km/s
Proper motion (μ) RA: +33.774[1] mas/yr
Dec.: −82.912[1] mas/yr
Parallax (π)11.6403±0.1172 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)1.48[2]
Orbit[4]
Period (P)Script error: No such module "val".
Eccentricity (e)Script error: No such module "val".
Periastron epoch (T)Script error: No such module "val".
Argument of periastron (ω)
(secondary)
Script error: No such module "val".°
Semi-amplitude (K1)
(primary)
Script error: No such module "val". km/s
Details
Mass1.29[5] Template:Solar mass
RadiusScript error: No such module "val". Template:Solar radius
Luminosity28.43[2] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[6] cgs
TemperatureScript error: No such module "val".[5] K
Metallicity [Fe/H]Script error: No such module "val".[2] dex
Rotational velocity (v sin i)1.6[4] km/s
Age5.44[5] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[7]
Database references
SIMBADdata

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27 Arietis is a binary star[4] system in the northern constellation of Aries. 27 Arietis is the Flamsteed designation. It is a dim, yellow-hued star that is close to the lower limit of what can be viewed with the naked eye, having an apparent visual magnitude is 6.21.[2] The annual parallax shift of Script error: No such module "val".[1] corresponds to a physical distance of approximately Script error: No such module "convert". from Earth. It is advancing closer to the Earth with a heliocentric radial velocity of −122.7 km/s, and may come as close as Script error: No such module "convert". in around 643,000 years.[2]

This appears to be a single-lined spectroscopic binary system with an orbital period of 130.7 days and an eccentricity of 0.366. It has an "a sin i" value of Script error: No such module "convert"., where a is the semimajor axis and i is the inclination to the line of sight from the Earth. This value provides a lower bound on the actual semimajor axis.[4] The visible component has a stellar classification of G8 III-IV Fe-2,[3] displaying mixed spectral traits of an evolved subgiant and a giant star, with a strong underabundance of iron. The CN bands of this star are very weak.[4]

References

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  7. Template:Cite simbad

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External links

Template:Stars of Aries