Przybylski's Star

Przybylski's Star

Star field containing Przybylski's Star (bright star at center, north is down)
Observation data
Epoch J2000      Equinox J2000
Constellation Centaurus
Right ascension 11h 37m 37.04096s
Declination −46° 42 34.8779
Apparent magnitude (V) 7.996–8.020
Characteristics
Evolutionary stage main sequence
Spectral type F0, F5, or G0 (F3 Ho)
U−B color index +0.20
B−V color index +0.76
Variable type roAp
Astrometry
Radial velocity (Rv)+12.4±3 km/s
Proper motion (μ) RA: −46.783 mas/yr
Dec.: +34.193 mas/yr
Parallax (π)9.1496±0.0213 mas
Distance356.5 ± 0.8 ly
(109.3 ± 0.3 pc)
Absolute magnitude (MV)+2.8
Details
Mass1.4 M
Radius1.90 R
Luminosity5.55 L
Surface gravity (log g)3.97 cgs
Temperature6,131 K
Metallicity [Fe/H]−2.40 dex
Rotation188 years
Rotational velocity (v sin i)3.50 km/s
Age1.5±0.1 Gyr
Other designations
V816 Cen, CD−46°7232, HD 101065, HIP 56709, SAO 222918
Database references
SIMBADdata

Przybylski's Star (pronounced /pʃɪˈbɪlskz/ or /ʃɪˈbɪlskz/), or HD 101065, is a rapidly oscillating Ap star at roughly 356 light-years (109 parsecs) from the Sun in the southern constellation of Centaurus. It is an unusual chemically peculiar star with a unique spectrum showing over-abundances of most rare-earth elements, for example, but under-abundances of more common elements such as iron.