14 Aquilae

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Template:Short description

14 Aquilae
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 5.42[2]
Characteristics
Evolutionary stage main sequence[3]
Spectral type A1 V[4]
U−B Template:Engvar –0.07[2]
B−V Template:Engvar +0.00[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] km/s
Proper motion (μ) RA: +15.558[1] mas/yr
Dec.: +2.571[1] mas/yr
Parallax (π)5.4932±0.2368 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−0.52[6]
Details
MassScript error: No such module "val".[3] Template:Solar mass
Radius2.0[7] Template:Solar radius
LuminosityScript error: No such module "val".[3] Template:Solar luminosity
TemperatureScript error: No such module "val".[3] K
Rotational velocity (v sin i)23[8] km/s
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[9]
Database references
SIMBADdata

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14 Aquilae is a probable spectroscopic binary[10] star system in the equatorial constellation of Aquila. 14 Aquilae is the Flamsteed designation though it also bears the Bayer designation g Aquilae. It is visible to the naked eye as a dim, white-hued star with an apparent visual magnitude of 5.42,[2] and it is located at a distance of approximately Script error: No such module "convert". from Sun. The star is moving closer to the Earth with a heliocentric radial velocity of Script error: No such module "val".,[5] and may come as close as Script error: No such module "convert". in around 3.5 million years.[6]

The visible component is an A-type main sequence star with a stellar classification of A1 V.[4] It has 3.25[3] times the mass of the Sun and about twice the Sun's radius. The projected rotational velocity is relatively low[10] at 23 km/s.[8] The star is radiating 214[7] times the luminosity of the Sun from its photosphere at an effective temperature of 9,908 K.

References

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External links

Template:Stars of Aquila