69 Aquilae

Star in the constellation Aquila From Wikipedia, the free encyclopedia

69 Aquilae, abbreviated 69 Aql, is a star in the equatorial constellation of Aquila. 69 Aquilae is its Flamsteed designation. It is visible to the naked eye with an apparent visual magnitude of 4.91.[2] Based upon an annual parallax shift of 16.2 mas,[1] it is located 201 light years away. The star is moving closer to the Earth with a heliocentric radial velocity of −22.5 km/s.[1]

Right ascension20h 29m 38.99995s[1]
Declination−02° 53 07.9176[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
69 Aquilae
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension 20h 29m 38.99995s[1]
Declination −02° 53 07.9176[1]
Apparent magnitude (V) 4.91[2]
Characteristics
Evolutionary stage red clump[3]
Spectral type K1/2 III[4]
B−V color index 1.162[5]
Astrometry
Radial velocity (Rv)−22.51±0.16[1] km/s
Proper motion (μ) RA: +70.355[1] mas/yr
Dec.: −21.523[1] mas/yr
Parallax (π)16.2388±0.2271 mas[1]
Distance201 ± 3 ly
(61.6 ± 0.9 pc)
Absolute magnitude (MV)0.97[2]
Details[5]
Mass1.54[6] M
Radius11 R
Luminosity45.7 L
Surface gravity (log g)2.5 cgs
Temperature4,529±5 K
Metallicity [Fe/H]0.03 dex
Rotational velocity (v sin i)4.0 km/s
Age3.44[6] Gyr
Other designations
69 Aql, BD−03°4918, HD 195135, HIP 101101, HR 7831, SAO 144495[7]
Database references
SIMBADdata
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The stellar classification of 69 Aquilae is K1/2 III,[4] which means this is an evolved giant star. It belongs to a sub-category called the red clump, indicating that it is on the horizontal branch and is generating energy through helium fusion at its core.[3] The star is about 3.4 billion years old with 1.54[6] times the mass of the Sun and has expanded to 11 times the Sun's radius.[5] It is radiating 45.7 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,529 K.[5]

References

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