14 Sagittae

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Template:Short description

14 Sagittae
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 5.89[3]
Characteristics
Spectral type B9p HgMn[4]
U−B Template:Engvar −0.44[3]
B−V Template:Engvar −0.06[3]
Astrometry
Radial velocity (Rv)−21.7[5] km/s
Proper motion (μ) RA: +5.28[6] mas/yr
Dec.: −8.99[6] mas/yr
Parallax (π)4.9142±0.0849 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−0.72[1]
Orbit[7]
Period (P)61.541 d
Eccentricity (e)0.49
Periastron epoch (T)2440799.01 JD
Argument of periastron (ω)
(secondary)
345°
Semi-amplitude (K1)
(primary)
4.2 km/s
Details
14 Sge A
Luminosity291.53[1] Template:Solar luminosity
Surface gravity (log g)3.60[4] cgs
Temperature13,200[4] K
Rotational velocity (v sin i)Script error: No such module "val".[8] km/s
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[9]
Database references
SIMBADdata

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14 Sagittae is a binary star[7] system in the equatorial constellation of Aquila.[10] 14 Sagittae is the Flamsteed designation. It appears as a sixth magnitude star, near the lower limit of visibility to the naked eye, having an apparent visual magnitude of 5.89.[3] The system is located 660 light years away, as determined from its annual parallax shift of Script error: No such module "val"..[2] It is moving closer to the Earth with a heliocentric radial velocity of –22 km/s.[5]

This is a single-lined spectroscopic binary with an orbital period of 61.5 days and an eccentricity of 0.49.[7] The visible component is a chemically peculiar mercury-manganese star[11] with a stellar classification of B9p HgMn.[4] It is narrow-lined with a projected rotational velocity of 7 km/s.[8] The star is radiating 292[1] times the Sun's luminosity from its photosphere at an effective temperature of 13,200 K.[4]

References

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External links

Template:Stars of Aquila