A visual band light curve for IK Tauri, plotted from ASAS-SN data.[1] The main plot shows the brightness as a function of time, and the inset shows the same data plotted as a function of pulsation phase. | |
Observation data Epoch J2000.0 Equinox J2000.0 | |
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Constellation | Taurus |
Right ascension | 03h 53m 28.87s[2] |
Declination | +11° 24′ 21.7″[2] |
Apparent magnitude (V) | 10.8 - 16.5[3] |
Characteristics | |
Evolutionary stage | Asymptotic giant branch |
Spectral type | M6e - M10e[3] |
Apparent magnitude (K) | −1.24[4] |
U−B color index | −0.04[4] |
B−V color index | +3.64[4] |
Variable type | Mira[3] |
Astrometry | |
Radial velocity (Rv) | ~46[5] km/s |
Proper motion (μ) | RA: 32.806±0.799[6] mas/yr Dec.: −22.820±0.663[6] mas/yr |
Parallax (π) | 3.5114 ± 0.3496 mas[6] |
Distance | 930 ± 90 ly (280 ± 30 pc) |
Details | |
Mass | 1 - 1.5[7] M☉ |
Radius | 608 ± 66[7] R☉ |
Luminosity | 8,724±1,921[7] L☉ |
Surface gravity (log g) | –0.95[7] cgs |
Temperature | 2,234±86[7] K |
Other designations | |
Database references | |
SIMBAD | data |
IK Tauri or NML Tauri is a Mira variable star located about 280 parsecs (910 ly) from the Sun in the zodiac constellation of Taurus.[7]
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