20 Arietis

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Template:Short description

20 Arietis
Observation data
Epoch J2000      Equinox J2000
Constellation Aries
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 5.79[2]
Characteristics
Spectral type F6 III-IV[3] or F6 IV-V[4]
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: +177.067[1] mas/yr
Dec.: −64.694[1] mas/yr
Parallax (π)24.1949±0.1121 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)2.67[2]
Details
MassScript error: No such module "val".[5] Template:Solar mass
RadiusScript error: No such module "val".[5] Template:Solar radius
LuminosityScript error: No such module "val".[6] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[5] cgs
TemperatureScript error: No such module "val".[5] K
Metallicity [Fe/H]Script error: No such module "val".[5] dex
Rotational velocity (v sin i)8.0[6] km/s
AgeScript error: No such module "val".[5] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[7]
Database references
SIMBADdata

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20 Arietis is a single[8] star in the northern constellation of Aries. 20 Arietis is the Flamsteed designation. It has an apparent visual magnitude of 5.79, which is bright enough to be just faintly visible to the naked eye as a yellow-white hued star. The star is located approximately 137 light years away from the Sun based upon parallax. It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.188 arc seconds per annum.[9] 20 Arietis is receding from the Earth with a heliocentric radial velocity of +25 km/s.[2]

Gray et al. (2001) gave the stellar classification of 20 Arietis as F6 III-IV,[3] matching an F-type star with spectral traits intermediate between a giant and a subgiant star. Harlan (1969) had found a less-evolved class of F6 IV-V.[4] The star is around two billion years old[5] with an estimated 1.5 times the mass of the Sun[5] and two times the Sun's radius.[5] It is spinning with a projected rotational velocity of 8.0 km/s[6] and has a higher than solar metallicity.[5] The star is radiating 6.6[6] times the luminosity of the Sun from its photosphere at an effective temperature of around 6,416 K.[5]

References

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External links

Template:Stars of Aries