Sigma Aquilae

From Wikipedia, the free encyclopedia

σ Aquilae
Observation data
Equinox J2000.0
Constellation Aquila
Right ascension 19h 39m 11.6s
Declination +5° 23' 52"
Apparent magnitude (V) +5.18
Distance 680 ± 120 ly
(208 ± 37 pc)
Spectral type B3V+B3V
Other designations
44 Aquilae, HR 7474,
HD 185507, BD+05°4225,
HIP 96665, SAO 124903,
GC 27185, ADS 12737,
CCDM 19392+0524

Sigma Aquilae (σ Aql / σ Aquilae) is a binary star in the constellation Aquila. It is approximately 680 light years from Earth.

Sigma Aquilae is an eclipsing spectroscopic binary. Both components are detached blue-white B-type main sequence dwarfs which do not fill their Roche lobes. The mean apparent magnitude of the binary is +5.18. Because it is an eclipsing binary, σ Aquilae is also a variable star and its brightness varies by 0.2 magnitudes with a period equal to its orbital period of 1.95 days.