Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Centaurus |
Right ascension | 11h 17m 14.32361s[1] |
Declination | −41° 56′ 03.5646″[1] |
Apparent magnitude (V) | 6.44±0.01[2] |
Characteristics | |
Spectral type | A0 V[3] |
U−B color index | −0.04[4] |
B−V color index | +0.03[4] |
Astrometry | |
Proper motion (μ) | RA: −55.255 mas/yr[1] Dec.: −7.836 mas/yr[1] |
Parallax (π) | 9.3823 ± 0.0298 mas[1] |
Distance | 348 ± 1 ly (106.6 ± 0.3 pc) |
Absolute magnitude (MV) | +1.35[5] |
Details | |
Mass | 2.5±0.3[6] M☉ |
Radius | 2.04[7] R☉ |
Luminosity | 28.3[8] L☉ |
Surface gravity (log g) | 4.1[9] cgs |
Temperature | 9,774+157 −220[6] K |
Metallicity [Fe/H] | −0.09[10] dex |
Other designations | |
Database references | |
SIMBAD | data |
HD 98176, also designated as HIP 55133 and rarely 22 G. Centauri, is a solitary, white hued star located in the southern constellation Centaurus. It has an apparent magnitude of 6.44,[2] placing it near the limit for naked eye visibility. Based on parallax measurements from Gaia DR3, the object is estimated to be 348 light years distant.[1] At its current distance, its brightness is diminished by 0.32 magnitudes due to interstellar dust.[13] Pauzen et al. (2001) lists it as a potential λ Boötis star.[14]
This is an ordinary A-type main-sequence star with a stellar classification of A0 V.[3] Pauzen et al. (2001) gives it a slightly cooler class of A1 Vn,[14] which includes broad absorption lines due to rapid rotation. It has 2.5 times the mass of the Sun[6] and double its radius.[7] It radiates 28.3 times the luminosity of the Sun[8] from its photosphere at an effective temperature of 9,774 K.[6] Based on parameters derived from extinction in the Gaia passband, HD 98176 has an iron abundance 19% below solar levels.
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