HV 11423 is visible in the full-size image, just to the left (south is up) of cluster NGC 361 (below centre, between the two bright foreground stars). (Digitized Sky Survey 2) | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Tucana |
Right ascension | 01h 00m 55.20s[1] |
Declination | −71° 37′ 52.9″[1] |
Apparent magnitude (V) | 11.84 - 12.46[2] |
Characteristics | |
Evolutionary stage | Red supergiant |
Spectral type | M0 Iab[3] (K0/1 I - M4.5/5 I[4]) |
B−V color index | +1.88 - +1.95[2] |
Variable type | Lc[5] |
Astrometry | |
Radial velocity (Rv) | 108.268[6] km/s |
Parallax (π) | 0.0692 ± 0.0336 mas[7] |
Distance | 200,000 ly |
Absolute magnitude (MV) | −6.5 - −8.4[4] |
Details[4][8] | |
Radius | 1,060-1,220 (Spectral fit), 960-1,000 (V-K) R☉ |
Luminosity | 350,000-200,000 (Spectral fit), 166,000 (V-K) L☉ |
Surface gravity (log g) | −0.4-−0.2 cgs |
Temperature | 4,300-3,500 (Spectral fit), 4,4803,635 (V-K) K |
Other designations | |
PMMR 114, LI-SMC 140, 2MASS J01005519-7137529 | |
Database references | |
SIMBAD | data |
HV 11423 (PMMR 114 or 140 LI-SMC) is a red supergiant star in the Small Magellanic Cloud. It is about 200,000 light-years away towards the constellation of Tucana.
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