HD 119921

HD 119921 is a single, white-hued star in the southern constellation of Centaurus. it has the Bayer designation z Centauri. This is faintly visible to the naked eye, having an apparent visual magnitude of 5.15. It forms a wide double star with a faint, magnitude 12.50 visual companion, which is located at an angular separation of 27.20 as of 2010. HD 119921 is moving closer to us with a heliocentric radial velocity of around −10 km/s, and is currently located some 420±10 light year from the Sun. At that distance, the visual magnitude of this star is diminished by 0.15 from extinction due to interstellar dust.

HD 119921
Observation data
Epoch J2000      Equinox J2000
Constellation Centaurus
Right ascension 13h 46m 56.35149s
Declination –36° 15 06.9563
Apparent magnitude (V) 5.15
Characteristics
Spectral type A0 V or B9.5 III-n
Astrometry
Radial velocity (Rv)−9.8±2.8 km/s
Proper motion (μ) RA: −13.293 mas/yr
Dec.: −11.115 mas/yr
Parallax (π)7.7881 ± 0.2382 mas
Distance420 ± 10 ly
(128 ± 4 pc)
Absolute magnitude (MV)0.93
Details
Luminosity125.24 L
Temperature8,801 K
Rotational velocity (v sin i)220 km/s
Age337 Myr
Other designations
z Cen, CD−35°8995, FK5 3091, HD 119921, HIP 67244, HR 5174, SAO 204835, WDS J13469-3615A
Database references
SIMBADdata

This is an A-type main-sequence star with a stellar classification of A0 V, per Houk (1979). However, Gray & Garrison (1987) have it classed as B9.5 III-n, suggesting it is a more evolved giant star. HD 119921 is spinning rapidly with a projected rotational velocity of 220 km/s. The star is radiating around 125 times the Sun's luminosity from its photosphere at an effective temperature of 8,801 K.

In 1983, Molaro et al. reported the presence of super-ionized elements (triple-ionized carbon and silicon) in the far ultraviolet spectrum of HD 119921. These anomalous features are not normally detected from a star in this temperature range. Instead, these blue-shifted absorption features may originate in the local interstellar medium.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.