Kappa Aquilae

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Template:Short description

κ Aquilae
Template:Location mark
Location of κ Aquilae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) +4.957[3]
Characteristics
Spectral type B0.5 III[4]
U−B Template:Engvar Script error: No such module "val".[3]
B−V Template:Engvar Script error: No such module "val".[3]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] km/s
Proper motion (μ) RA: +0.974 mas/yr[2]
Dec.: Script error: No such module "val". mas/yr[2]
Parallax (π)1.9758±0.1533 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)Script error: No such module "val".[1]
Details
MassScript error: No such module "val".[6] Template:Solar mass
Radius12.5[7] Template:Solar radius
Luminosity52,630[6] Template:Solar luminosity
Surface gravity (log g)3.5[8] cgs
Temperature26,500[6] K
Metallicity [Fe/H]−0.16[1] dex
Rotational velocity (v sin i)265[9] km/s
AgeScript error: No such module "val".[4] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[10]
Database references
SIMBADdata

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Kappa Aquilae is a star in the equatorial constellation of Aquila. Its name is a Bayer designation that is Latinized from κ Aquilae, and abbreviated Kappa Aql or κ Aql. This is a faint star with an apparent visual magnitude of +4.957,[3] which is bright enough to be seen with the naked eye in dark suburban skies. The annual parallax is only 1.98 mas,[2] which equates to a distance of approximately Script error: No such module "convert". from Earth (with a 6% margin of error).

The spectrum of Kappa Aquilae matches a stellar classification of B0.5 III,[4] where the luminosity class of III is typically associated with evolved giant stars. It is spinning rapidly with a projected rotational velocity of 265 km/s[9] and in the past has been classified as a Be star, despite the lack of an 'e' in the class.[11] However, the weak emission is most likely coming from the outflow of a hot stellar wind rather than a decretion disk.[12] This is a star with 15.50 times the Sun's mass[6] and 12.5 times the radius of the Sun.[7] Massive stars like this are luminous; it is radiating 52,630 times the Sun's luminosity[6] from its outer atmosphere with an effective temperature of 26,500 K,[6] giving it the intense blue-white glow of a B-type star. It is only 11 million years of age.[4]

Etymology

In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Right Flag, refers to an asterism consisting of κ Aquilae, μ Aquilae, σ Aquilae, δ Aquilae, ν Aquilae, 42 Aquilae, ι Aquilae, HD 184701 and 56 Aquilae.[13] Consequently, the Chinese name for κ Aquilae itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx.)[14]

This star, together with η Aql, θ Aql, δ Aql, ι Aql and λ Aql were once part of the now-obsolete constellation Antinous.[15]

References

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  6. a b c d e f Script error: No such module "citation/CS1".
  7. a b Script error: No such module "citation/CS1".
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  9. a b Script error: No such module "citation/CS1".
  10. Template:Cite simbad
  11. Script error: No such module "citation/CS1".
  12. Script error: No such module "citation/CS1".
  13. Template:In lang 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, Template:ISBN.
  14. Template:In lang AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 3 日 Template:Webarchive
  15. Script error: No such module "citation/CS1".

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External links

Template:Stars of Aquila