Omega2 Aquilae

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For other star systems with this Bayer designation, see Omega Aquilae.
Omega2 Aquilae
Diagram showing star positions and boundaries of the Aquila constellation and its surroundings
Cercle rouge 100%.svg

Location of ω2 (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Aquila
Right ascension 19h 19m 53.06650s[1]
Declination +11° 32′ 05.8750″[1]
Apparent magnitude (V) 6.023[2]
Characteristics
Spectral type A2 V[3]
U−B color index +0.07[4]
B−V color index +0.08[4]
Astrometry
Radial velocity (Rv) −26[5] km/s
Proper motion (μ) RA: 43.77[1] mas/yr
Dec.: 22.57[1] mas/yr
Parallax (π) 12.27 ± 0.52[1] mas
Distance 270 ± 10 ly
(81 ± 3 pc)
Details
Radius 2.0[6] R
Temperature 8,936[7] K
Rotational velocity (v sin i) 154[8] km/s
Other designations
29 Aquilae, 29 Aql, BD+11 3802, GC 26660, HD 181383, HIP 95002, HR 7332, PPM 136128, SAO 104728.[2]

Omega2 Aquilae (ω2 Aquilae, ω2 Aql) is the Bayer designation for a star in the equatorial constellation of Aquila, the eagle. It has an apparent visual magnitude of 6.0,[2] which is close to the lower limit of detectability with the naked eye. According to the Bortle Dark-Sky Scale, this star can be viewed from dark rural skies. As the Earth orbits about the Sun, this star undergoes a parallax shift of 12.27 mas.[1] This is equivalent to a physical distance of 270 light-years (83 parsecs) from Earth, give or take a 10 light year margin of error.

Analysis of the spectrum of this star shows it to match a stellar classification of A2 V,[3] indicating it is an A-type main sequence star. It is about double[6] the size of the Sun. The outer atmosphere is radiating energy at an effective temperature of 8,936 K,[7] giving it the white hue of an A-type star.[9] Omega2 Aquilae is spinning rapidly with a projected rotational velocity of 154 km/s.[8]

References

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External links

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