HD 53143

HD 53143
A millimetre image of the disk with the REASONS survey
Observation data
Epoch J2000      Equinox J2000
Constellation Carina
Right ascension 06h 59m 59.65545s
Declination −61° 20 10.2546
Apparent magnitude (V) 6.80
Characteristics
Spectral type G9 V
U−B color index +0.43
B−V color index +0.80
Astrometry
Radial velocity (Rv)+21.3 km/s
Proper motion (μ) RA: -161.59 mas/yr
Dec.: +264.67 mas/yr
Parallax (π)54.57±0.34 mas
Distance59.8 ± 0.4 ly
(18.3 ± 0.1 pc)
Absolute magnitude (MV)6.30
Details
Radius0.85 ± 0.02 R
Luminosity0.7 L
Temperature5,224 K
Metallicity [Fe/H]0.22 dex
Rotation9.6 ± 0.1 days
Rotational velocity (v sin i)4.0 ± 1.0 km/s
Age1.01 ± 0.13 Gyr
Other designations
Gl 260, CD-61° 1535, HD 53143, LTT 2715, SAO 249700, HIP 33690.
Database references
SIMBADdata

HD 53143 is a star in the Carina constellation, located about 59.8 light-years (18.3 parsecs) from the Earth. With an apparent visual magnitude of 6.80, this star is a challenge to view with the naked eye even under ideal viewing conditions.

Using the technique of gyrochronology, which measures the age of a low-mass star based on its rotation, HD 53143 is about 1,010 ± 130 million years old. Depending on the source, the stellar classification for this star is G9 V or K1V, placing it near the borderline between G-type and K-type main sequence stars. In either case, it is generating energy through the thermonuclear fusion of hydrogen at its core. This star is smaller than the Sun, with about 85% of the Sun's radius. It is emitting only 70% of the Sun's luminosity. The effective temperature of the star's outer envelope is cooler than the Sun at 5,224 K, giving it a golden-orange hue.