Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Carina |
Right ascension | 10h 09m 21.894s[2] |
Declination | −61° 32′ 56.43″[2] |
Apparent magnitude (V) | 4.5 - 10.0[3] |
Characteristics | |
Evolutionary stage | AGB[4] |
Spectral type | K5e - M6e[3] |
U−B color index | +0.93 to +1.93[5] |
B−V color index | +1.43 to +2.60[5] |
Variable type | Mira[3] |
Astrometry | |
Radial velocity (Rv) | 289.30[6] km/s |
Proper motion (μ) | RA: −94.237[2] mas/yr Dec.: 76.811[2] mas/yr |
Parallax (π) | 2.0110 ± 0.0855 mas[2] |
Distance | 1,620 ± 70 ly (500 ± 20 pc) |
Absolute magnitude (MV) | −0.71 to −3.41[7] |
Details | |
Mass | 0.6[8] M☉ |
Radius | 120[8] R☉ |
Luminosity | 2,200[5] L☉ |
Surface gravity (log g) | −0.9 - 1.0[9] cgs |
Temperature | 3,050 - 3,590[9] K |
Other designations | |
Database references | |
SIMBAD | data |
S Carinae (HD 88366) is a variable star in the constellation Carina.
S Carinae is an M-type red giant with a mean apparent magnitude of +6.94. It is approximately 1,620 light years from Earth. It is classified as a Mira type variable star and its brightness varies between magnitude +4.5 and +10.0 with a period of 149.49 days.[3] It has one of the earliest spectral types, and hence the hottest temperatures, of any Mira variable, and has a relatively short period for the class.[10] The temperature of this pulsing star is highest at visual brightness maximum and lowest at visual brightness minimum.[9]
S Carinae has exhausted its core hydrogen and expanded to become a red giant. It has also exhausted its core helium and evolved to the asymptotic giant branch, where it fuses hydrogen and helium in separate shells outside the core.[10][4]
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