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: −4.220[5] mas/yr Dec.: 12.364[5] mas/yr |
Parallax (π) | 1.2127 ± 0.0488 mas[5] |
Distance | 806 pc (2,630 ly)[6] ly |
Orbit | |
Period (P) | 227.55 d[7] |
Semi-major axis (a) | 0.54 AU[6] |
Eccentricity (e) | 0.0[7] |
Inclination (i) | 67[8]° |
Details | |
Red giant | |
Mass | 1.12[6] M☉ |
Radius | 75[8] R☉ |
Luminosity | 655[9] L☉ |
Surface gravity (log g) | 2.0[10] cgs |
Temperature | 3,600[10] K |
White dwarf | |
Mass | 1.37[6] M☉ |
Luminosity | ~100[8] L☉ |
Other designations | |
Database references | |
SIMBAD | data |
T Coronae Borealis (T CrB), nicknamed the Blaze Star, is a binary star and a recurrent nova 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] It is expected to undergo an outburst again very soon; likely during August 2024.[16]
dr1
was invoked but never defined (see the help page).gcvs
was invoked but never defined (see the help page).orbit
was invoked but never defined (see the help page).dr2
was invoked but never defined (see the help page).linford
was invoked but never defined (see the help page).fekel
was invoked but never defined (see the help page).stanishev
was invoked but never defined (see the help page).schaefer
was invoked but never defined (see the help page).wallerstein
was invoked but never defined (see the help page).