Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Centaurus |
Right ascension | 14h 19m 04.83414s[1] |
Declination | −59° 22′ 44.5272″[1] |
Apparent magnitude (V) | 6.637[2] |
Characteristics | |
Spectral type | K3 IV[3] |
U−B color index | +0.905[4] |
B−V color index | +1.025[4] |
Astrometry | |
Radial velocity (Rv) | −14.9[5] km/s |
Proper motion (μ) | RA: −454.895[1] mas/yr Dec.: −810.729[1] mas/yr |
Parallax (π) | 84.4535 ± 0.0349 mas[1] |
Distance | 38.62 ± 0.02 ly (11.841 ± 0.005 pc) |
Absolute magnitude (MV) | 6.28[2] |
Details | |
Mass | 0.806±0.017[6] M☉ |
Radius | 0.83+0.02 −0.01[1] R☉ |
Luminosity | 0.347±0.001[1] L☉ |
Surface gravity (log g) | 4.48[3] cgs |
Temperature | 4,858+47 −59[1] K |
Metallicity [Fe/H] | −0.70[7] dex |
Rotational velocity (v sin i) | 3.97[8] km/s |
Age | 9.98[7] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 125072 is a star in the southern constellation of Centaurus. It is a challenge to view with the naked eye, having an apparent visual magnitude of 6.637.[2] The star is located at a distance of 38.6 light years from the Sun based on parallax.[1] It is drifting closer with a radial velocity of −14.9 km/s.[5] The components of the space velocity for this star are U=−18.5, V=−6.9 and W=−26.9 km/s.[7]
The stellar classification of this star is K3 IV,[3] matching a K-type subgiant that is evolving into a giant. It has 81%[6] of the Sun's mass and 83%[1] of the radius of the Sun. The star is radiating 34.7% of the Sun's luminosity from its photosphere at an effective temperature of 4,858 K.[1] Based on the composition and kinematics of this star, it has an estimated age of about 10 billion years.[7] It is spinning with a projected rotational velocity of 4 km/s.[8]
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