Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Corona Borealis |
Right ascension | 15h 59m 30.1622s[1] |
Declination | +25° 55′ 12.613″[1] |
Apparent magnitude (V) | 2.0–10.8[2] |
Characteristics | |
Evolutionary stage | Red giant + white dwarf |
Spectral type | M3III+p[3] |
Variable type | recurrent nova[2] |
Astrometry | |
Radial velocity (Rv) | −27.79[4] km/s |
Proper motion (μ) | RA: −4.461 mas/yr[1] Dec.: 12.016 mas/yr[1] |
Parallax (π) | 1.0920 ± 0.0275 mas[1] |
Distance | 2,990 ± 80 ly (920 ± 20 pc) |
Orbit | |
Period (P) | 227.55 d[5] |
Semi-major axis (a) | 0.54 AU[6] |
Eccentricity (e) | 0.0[5] |
Inclination (i) | 67[7]° |
Details | |
Red giant | |
Mass | 1.12[6] M☉ |
Radius | 75[7] R☉ |
Luminosity | 655[8] L☉ |
Surface gravity (log g) | 2.0[9] cgs |
Temperature | 3,600[9] K |
White dwarf | |
Mass | 1.37[6] M☉ |
Luminosity | ~100[7] L☉ |
Other designations | |
Database references | |
SIMBAD | data |
T Coronae Borealis (T CrB), nicknamed the Blaze Star, is a binary star and a recurrent nova about 3,000 light-years (920 pc) away in the constellation Corona Borealis.[11] It was first discovered in outburst in 1866 by John Birmingham,[12] though it had been observed earlier as a 10th magnitude star.[13] It may have been observed in 1217 and in 1787 as well.[14][15] In February 1946 a 15-year-old schoolboy from Wales named Michael Woodman observed a flare up, subsequently writing to the Astronomer Royal and leading to the theory that the star flares each 80 years. [16]
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