41 Capricorni

41 Capricorni is a binary star system in the southern constellation of Capricornus. It is faintly visible to the naked eye with an apparent visual magnitude of +5.24. The distance to this star, based upon an annual parallax shift of $0.991$, is around 171 light years. It is moving closer with a heliocentric radial velocity of −45 km/s.

This is a yellow K-type giant star with a stellar classification of K0 III. At the age of around 550 million years it has become a red clump star, which indicates it is generating energy via helium fusion at its core. It has an estimated 2.55 times the mass of the Sun and is radiating 48 times the Sun's luminosity from its photosphere at an effective temperature of 4,910 K. The magnitude 11.5 companion lies at an angular separation of $−45.1$, as of 2008.