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Star in the constellation Aquila From Wikipedia, the free encyclopedia
Omega2 Aquilae, Latinized from ω2 Aquilae, is the Bayer designation for a star in the equatorial constellation of Aquila, the eagle.[10] 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 11.7 mas.[1] This is equivalent to a physical distance of 279 light-years (86 parsecs) from Earth, give or take a 2 light year margin of error. The star is drifting closer to the Sun with a radial velocity of −26 km/s.[2]
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Aquila |
Right ascension | 19h 19m 53.06713s[1] |
Declination | +11° 32′ 05.8722″[1] |
Apparent magnitude (V) | 6.03[2] |
Characteristics | |
Spectral type | A2 V[3] or F0V[2] |
U−B color index | +0.087±0.007[2] |
B−V color index | +0.08[4] |
Astrometry | |
Radial velocity (Rv) | −26.0±4.3[5][2] km/s |
Proper motion (μ) | RA: 44.042[1] mas/yr Dec.: 22.393[1] mas/yr |
Parallax (π) | 11.7035 ± 0.0703 mas[1] |
Distance | 279 ± 2 ly (85.4 ± 0.5 pc) |
Absolute magnitude (MV) | 1.48[2] |
Details | |
Mass | 2.01[6] M☉ |
Radius | 2.0[7] R☉ |
Luminosity | 22[2] L☉ |
Temperature | 8,936[8] K |
Rotational velocity (v sin i) | 154[9] km/s |
Age | 224[6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Analysis of the spectrum of this white-hued star shows it to match a stellar classification of A2 V,[3] indicating it is an A-type main sequence star. It has about double the size and mass of the Sun.[7] The star is radiating 22[2] times the luminosity of the Sun from its photosphere at an effective temperature of 8,936 K,[8] giving it the white hue of an A-type star.[11] Omega2 Aquilae is 224[6] million years old and is spinning rapidly with a projected rotational velocity of 154 km/s.[9]
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