Iota Aquilae,
Latinized from ι Aquilae, is the
Bayer designation
A Bayer designation is a stellar designation in which a specific star is identified by a Greek or Latin letter followed by the genitive form of its parent constellation's Latin name. The original list of Bayer designations contained 1,564 stars. ...
for a
star
A star is an astronomical object comprising a luminous spheroid of plasma (physics), plasma held together by its gravity. The List of nearest stars and brown dwarfs, nearest star to Earth is the Sun. Many other stars are visible to the naked ...
in the
equatorial constellation
A constellation is an area on the celestial sphere in which a group of visible stars forms Asterism (astronomy), a perceived pattern or outline, typically representing an animal, mythological subject, or inanimate object.
The origins of the e ...
of
Aquila
Aquila may refer to:
Arts, entertainment, and media
* ''Aquila'', a series of books by S.P. Somtow
* ''Aquila'', a 1997 book by Andrew Norriss
* ''Aquila'' (children's magazine), a UK-based children's magazine
* ''Aquila'' (journal), an or ...
. It has the traditional name Al Thalimain , which it shares with
λ Aquilae. The name is derived from the
Arabic term الظليمین ''al-ẓalīmayn'' meaning "The Two Ostriches". With an
apparent visual magnitude of 4.364,
[ this star is bright enough to be seen with the naked eye. Based upon an annual ]parallax
Parallax is a displacement or difference in the apparent position of an object viewed along two different lines of sight and is measured by the angle or semi-angle of inclination between those two lines. Due to foreshortening, nearby objects ...
shift of ,[ it is located at a distance of around from Earth. At that distance, the visual magnitude of the star is diminished by 0.15][ from extinction caused by intervening gas and dust.
Although Iota Aquilae is listed in star catalogues as a giant star, calculations of its dimension show that in reality it is a main-sequence star.][ It has nearly five times the mass of the Sun and five to six times the Sun's radius.][ It is emitting 851][ times the luminosity of the Sun from its outer atmosphere at an ]effective temperature
The effective temperature of a body such as a star or planet is the temperature of a black body that would emit the same total amount of electromagnetic radiation. Effective temperature is often used as an estimate of a body's surface temperature ...
of 14,552 K,[ giving it the blue-white hue of a B-type star. The projected rotational velocity of this star is 55 km/s.][ Even though it is only around 100 million years old, it has already spent 91% of its allotted lifetime on the main sequence.][
]
Nomenclature
In Chinese, (), meaning '' Right Flag'', refers to an asterism consisting of ι Aquilae, μ Aquilae, σ Aquilae
Sigma Aquilae, Latinized from σ Aquilae, is the Bayer designation for a binary star system in the equatorial constellation of Aquila. The baseline apparent magnitude of the pair is +5.17, which, according to the Bortle Dark-Sky Scale ...
, δ Aquilae, ν Aquilae, 42 Aquilae, HD 184701, κ Aquilae and 56 Aquilae. Consequently, the Chinese name for ι Aquilae itself is (, en, the Fifth Star of Right Flag.)AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 3 日
/ref>
This star, together with η Aql, θ Aql, δ Aql, κ Aql and λ Aql were consist Antinous
Antinous, also called Antinoös, (; grc-gre, Ἀντίνοος; 27 November – before 30 October 130) was a Greek youth from Bithynia and a favourite and probable lover of the Roman emperor Hadrian. Following his premature death before his ...
, the obsolete constellation.[
]
References
External links
Image Iota Aquilae
HR 7447
{{DEFAULTSORT:Iota Aquilae
Al Thalimain
184930
Aquilae, Iota
Aquila (constellation)
B-type giants
096468
Aquilae, 41
7447
Durchmusterung objects