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68 Aquilae

Star in the constellation Aquila From Wikipedia, the free encyclopedia

68 Aquilae (abbreviated 68 Aql) is a double star in the equatorial constellation of Aquila. 68 Aquilae is its Flamsteed designation. It has an apparent visual magnitude of 6.12, which is dimly visible to the naked eye under favorable viewing conditions. The distance to the brighter component is approximately 550 light years based on parallax measurements, and it is drifting further away with a heliocentric radial velocity of –9 km/s.[4]

Quick facts Constellation, Right ascension ...
68 Aquilae
Observation data
Epoch J2000      Equinox ICRS
Constellation Aquila
Right ascension 20h 28m 24.904s[1]
Declination −03° 21′ 28.05″[1]
Apparent magnitude (V) 6.12[2]
Characteristics
Evolutionary stage main sequence[3]
Spectral type B9 V:[2]
U−B color index −0.20[2]
B−V color index −0.06[2]
Astrometry
Radial velocity (Rv)−9[4] km/s
Proper motion (μ) RA: +27.242 mas/yr[1]
Dec.: −19.118 mas/yr[1]
Parallax (π)5.9286±0.052 mas[1]
Distance550 ± 5 ly
(169 ± 1 pc)
Details
Mass3.16±0.12[3] M☉
Radius3.361±0.168[5] R☉
Luminosity159.8+29.9
−25.2
[3] L☉
Temperature10,641+50
−49
[3] K
Rotational velocity (v sin i)138[6] km/s
Other designations
68 Aql, BD−03°4906, HD 194939, HIP 100977, HR 7821, SAO 144468, WDS J20284-0321A[7]
Database references
SIMBADdata
Close

The stellar classification of the brighter component is B9 V:,[2] matching a B-type main-sequence star. However, the ':' suffix indicates some uncertainty in the classification. It has an estimated 3.2[3] times the mass of the Sun and 3.4 times the Sun's radius.[5] 68 Aquilae is radiating 160 times the Sun's luminosity from its photosphere at an effective temperature of 10,641 K.[3] The star is spinning rapidly with a projected rotational velocity of 138 km/s.[6]

There is a companion star at a projected separation of 9.00″ as of 2013. It was first reported in 1939 by R. A. Rossiter when the separation was measured at 9.8″. This star has a visual magnitude of 13.70.[8]

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