HD 125383 is a binary star in the constellation Lupus. At a combined apparent magnitude of +5.55, it is faintly visible to the naked eye in locations far from light pollution. Parallax measurements give distances of 410 light-years (125.8 parsecs) and 406 light-years (124.6 parsecs) for the primary and secondary, respectively.
Characteristics The two components are separated by 3.5" along a position angle of 301°, as of 2016. They have apparent magnitudes of 5.77 and 7.94. The primary (A) has a spectral class of G8 III, with the luminosity class 'III' suggesting it is a giant that has exhausted the hydrogen at its core. The star has expanded to 11.8 times the Sun's radius and now radiates 84 times the Sun's luminosity from its photosphere at an effective temperature of 5,784 K. This temperature gives it a yellow hue typical of a G-type star. The secondary (B) has a spectral class of G0 IV, with the luminosity class 'IV' suggesting it is a subgiant that has exhausted the hydrogen at its core. The star has expanded to 2.0 times the Sun's radius and has an effective temperature of 5,947 K. This temperature gives it a yellow hue typical of a G-type star.
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