Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Sculptor |
Right ascension | 23h 40m 38.14898s[1] |
Declination | −32° 04′ 23.2478″[1] |
Apparent magnitude (V) | 5.30[2] (5.30 – 5.33)[3] |
Characteristics | |
Evolutionary stage | giant |
Spectral type | K1 III[4] |
U−B color index | +0.69[5] |
B−V color index | +0.97[6] |
Variable type | suspected[3] |
Astrometry | |
Radial velocity (Rv) | +15.79±0.12[1] km/s |
Proper motion (μ) | RA: −91.30[7] mas/yr Dec.: −53.29[7] mas/yr |
Parallax (π) | 11.6622 ± 0.1228 mas[1] |
Distance | 280 ± 3 ly (85.7 ± 0.9 pc) |
Absolute magnitude (MV) | 0.54[2] |
Details | |
Mass | 1.32[8] M☉ |
Radius | 10.88+0.16 −0.13[1] R☉ |
Luminosity | 61.4±0.8[1] L☉ |
Surface gravity (log g) | 2.50[8] cgs |
Temperature | 4,899+29 −35[1] K |
Metallicity [Fe/H] | −0.21[2] dex |
Rotational velocity (v sin i) | 2.6[9] km/s |
Other designations | |
Database references | |
SIMBAD | data |
μ Sculptoris, Latinized as Mu Sculptoris, is a solitary,[11] orange-hued star in the southern constellation of Sculptor. It is visible to the naked eye as a dim point of light with an apparent visual magnitude of +5.30.[2] This star is located approximately 291 light years from the Sun based on parallax,[7] and it is drifting further away with a radial velocity of +16 km/s.[1]
This object is an aging K-type giant star with a stellar classification of K1 III.[4] Having exhausted the supply of hydrogen at its core, this star expanded and cooled off the main sequence. At present it has 11[1] times the girth of the Sun. It is a suspected variable star of unknown type, with its brightness measured as varying from magnitude 5.30 down to 5.33.[3] The star has 1.32[8] times the mass of the Sun and is radiating 61[1] times the Sun's luminosity from its swollen photosphere at an effective temperature of 4899 K.[1]
GaiaDR2
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