Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Centaurus |
Right ascension | 13h 41m 45.56353s [1] |
Declination | −33° 35′ 50.5600″ [1] |
Apparent magnitude (V) | 5.56 –8.44 [2] |
Characteristics | |
Evolutionary stage | AGB or post-AGB [2] |
Spectral type | K0:e-M4II:e [2] |
Variable type | semiregular [3] |
Astrometry | |
Radial velocity (Rv) | +32.6±2.5 [1] km/s |
Proper motion (μ) | RA: −27.747 mas/yr [1] Dec.: +3.365 mas/yr [1] |
Parallax (π) | 2.4007±0.0687 mas [1] |
Distance | 1,360 ± 40 ly (420 ± 10 pc) |
Other designations | |
T Cen, CD−32°9549, HD 119090, HIP 66825, HR 5147, SAO 204739 [4] | |
Database references | |
SIMBAD | data |
T Centauri is a variable star located in the far southern constellation Centaurus. It varies between magnitudes 5.56 and 8.44 over 181.4 days, making it intermittently visible to the naked eye. [2] Pulsating between spectral classes K0:e and M4II:e, it has been classed as a semiregular variable, [3] though Sebastian Otero of the American Association of Variable Star Observers has noted its curve more aligned with RV Tauri variable stars and has classified it as one. [2]
The variability of the star was discovered in 1894 by Ernest Elliott Markwick, and independently by Williamina Fleming in 1895. [6] [7]