Eta Aquilae

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η Aquilae
Observation data
Epoch J2000.0
Constellation Aquila
Right ascension 19h 52m 28.4s
Declination +1° 00' 20"
Apparent magnitude (V) +3.87
Distance 1180 ± 390 ly
(360 ± 120 pc)
Spectral type F6Ib
Other designations
55 Aquilae, HR 7570,
HD 187929, BD+00°4337,
FK5 746, HIP 97804,
SAO 125159, GC 27517

Eta Aquilae (η Aql / η Aquilae) is a star in the constellation Aquila. It was also part of the former constellation Antinous.

It is a Cepheid variable star, varying from apparent magnitude 3.6 to 4.4 with a period of 7.176641 days. Along with Delta Cephei, Zeta Geminorum and Beta Doradus, it is one of the most prominent naked eye Cepheids; that is, both the star itself and the variation in its brightness can be distinguished by the naked eye. Some other Cepheids such as Polaris are bright but have only a very small variation in brightness.

It is about 1200 light years from Earth. It is a yellow-white supergiant, and is about 3000 times more luminous than the Sun, with a diameter about 60 times that of the Sun.

[edit] Location

The star's location in the constellation of Aquila is shown in the following map:

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