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Star in the constellation Norma From Wikipedia, the free encyclopedia
QU Normae, also known as HR 6131, is a blue supergiant star in the constellation Norma. It is also a variable star, thought to be an α Cyg variable.
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Norma |
Right ascension | 16h 29m 42.32668s[1] |
Declination | −46° 14′ 35.6022″[1] |
Apparent magnitude (V) | 5.37[2] (5.27 - 5.41[3]) |
Characteristics | |
Spectral type | B1.5 Iap[4] |
U−B color index | −0.44[2] |
B−V color index | +0.62[2] |
Variable type | α Cyg[3] |
Astrometry | |
Radial velocity (Rv) | −14.80 ± 3.2[5] km/s |
Proper motion (μ) | RA: −4.54[1] mas/yr Dec.: −1.51[1] mas/yr |
Parallax (π) | 1.79 ± 0.70 mas[1] |
Distance | approx. 1,800 ly (approx. 600 pc) |
Absolute magnitude (MV) | −7.50[6] |
Details | |
Mass | 43[7] M☉ |
Radius | 58[8] R☉ |
Luminosity | 417,000[6] L☉ |
Surface gravity (log g) | 2.00[7] cgs |
Temperature | 17,000[7] K |
Rotational velocity (v sin i) | 44[7] km/s |
Other designations | |
Database references | |
SIMBAD | data |
The apparent magnitude of QU Normae varies somewhat irregularly between 5.27 and 5.41. The General Catalogue of Variable Stars quotes a period of 4.818 days,[3] but other research only shows likely periods longer than 10 days.[9]
QU Normae has a spectral type B1.5 Ia, a luminous supergiant that has swollen and cooled off the main sequence. Surface abundances suggest that it has not yet passed through a red supergiant phase.[6] Around 1,820 light-years distant, it shines with a luminosity approximately 417,000 times that of the Sun and has a diameter around 58 times that of the Sun.
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