Beta Sculptoris

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β Sculptoris
Location of β Sculptoris (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Sculptor
Right ascension 23h 32m 58.25898s[1]
Declination −37° 49′ 05.7570″[1]
Apparent magnitude (V) 4.37[2]
Characteristics
Evolutionary stage Main sequence[3]
Spectral type B9.5IIIp(HgMnSi)[4]
U−B color index −0.36[2]
B−V color index −0.09[2]
Variable type suspected α2 CVn[5]
Astrometry
Radial velocity (Rv)+0.4±0.6[6] km/s
Proper motion (μ) RA: +95.97[1] mas/yr
Dec.: +38.29[1] mas/yr
Parallax (π)18.74±0.15 mas[1]
Distance174 ± 1 ly
(53.4 ± 0.4 pc)
Absolute magnitude (MV)0.74[7]
Details
Mass3.2±0.2[3] M
Radius2.0[8] R
Luminosity81[9] L
Surface gravity (log g)4.13[3] cgs
Temperature12,500[3] K
Metallicity [Fe/H]+0.23[3] dex
Rotation1.9311[10] d
Rotational velocity (v sin i)26[9][3] km/s
Other designations
β Scl, CD−38°15527, FK5 886, GC 32744, HD 221507, HIP 116231, HR 8937, SAO 214615, GSC 08013-01357[11]
Database references
SIMBADdata

Beta Sculptoris, Latinized from β Sculptoris, is a single,[12] blue-white hued star in the southern constellation of Sculptor. It has an apparent visual magnitude of 4.37,[2] which is bright enough to be seen with the naked eye. Based upon an annual parallax shift of 18.74 mas as seen from Earth, it is located 174 light years from the Sun.

A light curve for Beta Sculptoris, adapted from Pedersen et al. (2019)[13]

This is a B-type main-sequence star,[3] despite its stellar classification of B9.5IIIp(HgMnSi) containing the luminosity class of a giant.[4] It belongs to the class of chemically peculiar stars known as a Mercury-Manganese star,[14] showing overabundances of mercury, manganese, and silicon in its spectrum. It is a suspected α2 CVn variable with magnitude variation from 4.35 to 4.39.[5] The star has nearly three[9] times the mass of the Sun and double[8] the Sun's radius. It is radiating 81[9] times the Sun's luminosity from its photosphere at an effective temperature of 12,110 K.[9]

References

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