71 Aquilae

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71 Aquilae
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension 20h 38m 20.28206s[1]
Declination −01° 06′ 18.4311″[1]
Apparent magnitude (V) 4.33[2]
Characteristics
Spectral type G8 III[3]
U−B color index +0.68[2]
B−V color index +0.96[2]
R−I color index 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[1] mas
Distance 340 ± 30 ly
(103 ± 8 pc)
Absolute magnitude (MV) –1.03[5]
Orbit[6]
Period (P) 205.2 days
Semi-major axis (a) 3.82 ± 0.81 mas
Eccentricity (e) 0.000
Inclination (i) 147.70° ± 5.90°
Longitude of the node (Ω) 314.00 ± 1.30°
Periastron epoch (T) 2423358.0 HJD
Argument of periastron (ω)
(secondary)
0.00°
Details
Surface gravity (log g) 2.87[7] cgs
Temperature 5,060[7] K
Metallicity [Fe/H] –0.13[7] dex
Rotational velocity (v sin i) 10[8] km/s
Other designations
BD-01 4016, HD 196574, HIP 101847, HR 7884, SAO 144649.[9]

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 340 light-years (100 parsecs) 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 spectrum caused by the Doppler effect. The primary component is a giant star with a stellar classification of G8 III.[3] The secondary is following a circular orbit with a period of 205.2 days.[6]

References

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External links