HD 125072

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. The star is located at a distance of 38.6 light years from the Sun based on parallax. It is drifting closer with a radial velocity of −14.9 km/s. The components of the space velocity for this star are U=18.5, V=6.9 and W=26.9 km/s.

HD 125072
Observation data
Epoch J2000      Equinox J2000
Constellation Centaurus
Right ascension 14h 19m 04.83414s
Declination −59° 22 44.5272
Apparent magnitude (V) 6.637
Characteristics
Spectral type K3 IV
U−B color index +0.905
B−V color index +1.025
Astrometry
Radial velocity (Rv)−14.9 km/s
Proper motion (μ) RA: −454.895 mas/yr
Dec.: −810.729 mas/yr
Parallax (π)84.4535 ± 0.0349 mas
Distance38.62 ± 0.02 ly
(11.841 ± 0.005 pc)
Absolute magnitude (MV)6.28
Details
Mass0.806±0.017 M
Radius0.83+0.02
−0.01
 R
Luminosity0.347±0.001 L
Surface gravity (log g)4.48 cgs
Temperature4,858+47
−59
 K
Metallicity [Fe/H]−0.70 dex
Rotational velocity (v sin i)3.97 km/s
Age9.98 Gyr
Other designations
CD−58°5564, GJ 542, HD 125072, HIP 69972, SAO 241627, LHS 2892, LTT 5625
Database references
SIMBADdata

The stellar classification of this star is K3 IV, matching a K-type subgiant that is evolving into a giant. It has 81% of the Sun's mass and 83% 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. Based on the composition and kinematics of this star, it has an estimated age of about 10 billion years. It is spinning with a projected rotational velocity of 4 km/s.

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