71 Aquilae

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71 Aquilae
Template:Location mark
Location of 71 Aquilae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 4.33[2]
Characteristics
Spectral type G7.5 IIIa[3]
U−B Template:Engvar +0.68[2]
B−V Template:Engvar +0.96[2]
R−I Template:Engvar 0.46
Astrometry
Radial velocity (Rv)−5.6[4] km/s
Proper motion (μ) RA: +14.84[1] mas/yr
Dec.: −16.45[1] mas/yr
Parallax (π)9.67±0.75 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−1.03[5]
Orbit[6]
Period (P)205.2 days
Semi-major axis (a)Script error: No such module "val".
Eccentricity (e)0.000
Inclination (i)Script error: No such module "val".°
Longitude of the node (Ω)Script error: No such module "val".°
Periastron epoch (T)2423358.0 HJD
Argument of periastron (ω)
(secondary)
0.00°
Details
primary
Mass3.6[7] Template:Solar mass
Radius16.7[8] Template:Solar radius
Luminosity162[8] Template:Solar luminosity
Surface gravity (log g)2.77[8] cgs
Temperature5,046[8] K
Metallicity [Fe/H]−0.03[8] dex
Rotational velocity (v sin i)10[9] km/s
Age347[10] Myr
secondary
Mass0.88[7] Template:Solar mass
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
BD−01 4016, HD 196574, HIP 101847, HR 7884, SAO 144649.[11]
Database references
SIMBADdata

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71 Aquilae (abbreviated 71 Aql) is a binary star in the equatorial constellation of Aquila. 71 Aquilae is its Flamsteed designation though it also bears the Bayer designation l Aquilae. The apparent visual magnitude of the system is 4.33,[2] making it bright enough to be viewed by the naked eye. It has an annual parallax shift of 9.67 mas,[1] which equates to a physical distance of Script error: No such module "convert". from Earth, give or take a 30 light-year margin of error. At this distance, the brightness of the system is diminished by 0.065 in visual magnitude from extinction caused by interstellar gas and dust.[5]

This is a spectroscopic binary system where the presence of an orbiting companion is revealed by shifts in the spectral lines caused by the Doppler effect. The primary component is a giant star with a stellar classification of G7.5 IIIa and is listed as a standard star for that class.[3] The secondary is following a circular orbit with a period of 205.2 days.[6]

References

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Template:Stars of Aquila