12 Aquilae

Star in the constellation Aquila From Wikipedia, the free encyclopedia

12 Aquilae

12 Aquilae (abbreviated 12 Aql) is a star in the equatorial constellation of Aquila. 12 Aquilae has the Bayer designation of i Aquilae and is most easily recognized in the sky being next to the brighter star λ (lambda) Aquilae.

Quick Facts Observation data Epoch J2000 Equinox J2000, Constellation ...
12 Aquilae
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Location of 12 Aquilae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension 19h 01m 40.82887s [1]
Declination –05° 44 20.7222 [1]
Apparent magnitude (V) 4.02[2]
Characteristics
Spectral type K1 III[3]
U−B color index +1.04[2]
B−V color index +1.104[4]
R−I color index 0.54
Astrometry
Radial velocity (Rv)–43.92 ± 0.18[4] km/s
Proper motion (μ) RA: −22.592 mas/yr[1]
Dec.: −43.08 mas/yr[1]
Parallax (π)21.5669 ± 0.2199 mas[1]
Distance151 ± 2 ly
(46.4 ± 0.5 pc)
Absolute magnitude (MV)0.726[5]
Details
Mass1.185±0.282[6] M
Radius12.28±0.14[6] R
Luminosity58.2±3.1[7] L
Surface gravity (log g)2.31±0.11[6] cgs
Temperature4,662±59[7] K
Metallicity [Fe/H]−0.08±0.07[6] dex
Rotational velocity (v sin i)3.6[4] km/s
Age3.64±1.43[7] Gyr
Other designations
i Aquilae, BD–05 4840, HD 176678, HIP 93429, HR 7193, SAO 142931.[8]
Database references
SIMBADdata
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In Chinese, 天弁 (Tiān Biàn), meaning Market Officer, refers to an asterism consisting of 12 Aquilae, α Scuti, δ Scuti, ε Scuti, β Scuti, η Scuti, λ Aquilae, 15 Aquilae and 14 Aquilae.[9] Consequently, 12 Aquilae itself is known as 天弁六 (Tiān Biàn liù, English: the Sixth Star of Market Officer.)

This star has an apparent visual magnitude of 4.02,[2] which is bright enough to be seen with the naked eye, although, according to the Bortle Dark-Sky Scale, it is a challenge to view from the inner city. Based upon an annual parallax shift of 21.57 mas,[1] the distance to this star is 151 light-years (46 parsecs) with a margin of error of one light-year. This is an evolved giant star of stellar class K1 III.[3] It has 12 times the radius of the Sun[6] and shines with 58 times the Sun's luminosity. This energy is being radiated from its outer atmosphere at an effective temperature of 4,662 K,[6] giving it the cool orange hue of a K-type star.[10]

References

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