Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Centaurus |
Right ascension | 14h 01m 43.49909 s[1] |
Declination | −45° 36′ 12.2767″[1] |
Apparent magnitude (V) | +4.33[2] |
Characteristics | |
Spectral type | F7 II/III[3] |
U−B color index | +0.26[2] |
B−V color index | +0.61[2] |
Variable type | None[4] |
Astrometry | |
Radial velocity (Rv) | −7.8±7.4[5] km/s |
Proper motion (μ) | RA: +8.64±1.09[1] mas/yr Dec.: −16.25±0.88[1] mas/yr |
Parallax (π) | 2.57 ± 1.05 mas[1] |
Distance | approx. 1,300 ly (approx. 400 pc) |
Absolute magnitude (MV) | −3.51[4] |
Orbit[6] | |
Period (P) | 207.357 d |
Eccentricity (e) | 0.55 |
Periastron epoch (T) | 2423880.5 JD |
Argument of periastron (ω) (secondary) | 88° |
Semi-amplitude (K1) (primary) | 12.7 km/s |
Details | |
Mass | 6.86±0.39[7] M☉ |
Luminosity (bolometric) | 3,919[7] L☉ |
Surface gravity (log g) | 2.00[8] cgs |
Temperature | 6,495[7] K |
Rotational velocity (v sin i) | 0.0[8] km/s |
Age | 45.9±4.0[9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Upsilon2 Centauri (υ2 Centauri) is a binary star[6] system in the southern constellation Centaurus. It is visible to the naked eye with an apparent visual magnitude of +4.33.[2] Based upon an annual parallax shift of just 2.57 mas as seen from Earth,[1] this star is located roughly 1,300 light years from the Sun. Relative to its neighbors, the system has a peculiar velocity of 39.2+8.8
−15.2 km/s and it may form a runaway star system.[9]
This is a single-lined spectroscopic binary star system with an orbital period of 207.357 days and an eccentricity of 0.55.[6] The primary component has the spectrum of an evolved F-type giant/bright giant hybrid with a stellar classification of F7 II/III.[3] It is around 46[9] million years old with 6.9 times the mass of the Sun. The star is radiating 3,919 times the Sun's luminosity from its photosphere at an effective temperature of 6,495 K.[7]
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