Iota Aquilae

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Template:Short description

Iota Aquilae
Template:Location mark
Location of ι Aquilae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 4.364[3]
Characteristics
Spectral type B5 III[4] or B6 IV[5]
U−B Template:Engvar −0.428[3]
B−V Template:Engvar −0.083[3]
R−I Template:Engvar −0.08[6]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[2] km/s
Proper motion (μ) RA: Script error: No such module "val". mas/yr[2]
Dec.: Script error: No such module "val". mas/yr[2]
Parallax (π)5.6673±0.1947 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".[7] Template:Solar mass
RadiusScript error: No such module "val".[8] Template:Solar radius
Luminosity851[7] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[7] cgs
TemperatureScript error: No such module "val".[8] K
Metallicity [Fe/H]Script error: No such module "val".[1] dex
Rotational velocity (v sin i)55[9] km/s
Age100 ± 8[7] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[10]
Database references
SIMBADdata

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Iota Aquilae is a star in the equatorial constellation of Aquila. Its identifier is a Bayer designation that is Latinized from ι Aquilae, and abbreviated Iota Aql or ι Aql. The star has the traditional name Al Thalimain, pronounced Template:IPAc-en, which it shares with λ Aquilae. The name is derived from the Arabic term الظليمین al-ẓalīmayn meaning "The Two Ostriches".[11] With an apparent visual magnitude of 4.364,[3] this star is bright enough to be seen with the naked eye. Based upon an annual parallax shift of Script error: No such module "val".,[2] it is located at a distance of around Script error: No such module "convert". from Earth.[2] The visual magnitude of the star is diminished by 0.15 from extinction caused by intervening gas and dust.[7]

In 1968, this star was assigned a stellar classification of B5III,[4] which suggests it has exhausted its hydrogen supply at its core and evolved into a blue giant. However, stellar models from 2002 indicate it is around 100 million years old and has thus far spent 91% of its allotted lifetime on the main sequence.[7] In 2024, a study of standard stars suggested that Iota Aquilae be classified as B6 IV, matching a subgiant star.[5]

Iota Aquilae has nearly five times the mass of the Sun[7] and eight times the Sun's radius.[8] It is emitting 851 times the luminosity of the Sun from its outer atmosphere[7] at an effective temperature of 14,500 K,[12] giving it the blue-white hue of a B-type star.[13] The projected rotational velocity of this star is 55 km/s.[9]

Nomenclature

In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Right Flag, refers to an asterism consisting of ι Aquilae, μ Aquilae, σ Aquilae, δ Aquilae, ν Aquilae, 42 Aquilae, HD 184701, κ Aquilae and 56 Aquilae.[14] Consequently, the Chinese name for ι Aquilae itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx.)[15]

This star, together with η Aql, θ Aql, δ Aql, κ Aql and λ Aql were once part of the obsolete constellation Antinous.[16]

References

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  9. a b Script error: No such module "citation/CS1".
  10. Template:Cite simbad
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  13. Script error: No such module "citation/CS1".
  14. 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.
  15. Script error: No such module "citation/CS1".
  16. Script error: No such module "citation/CS1".

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External links

Template:Stars of Aquila