Rho Orionis

Rho Orionis, Latinised from ρ Orionis, is the Bayer designation for an orange-hued binary star system in the equatorial constellation of Orion. It is visible to the naked eye with an apparent visual magnitude of +4.44. The star shows an annual parallax shift of 9.32 mas due to the orbital motion of the Earth, which provides a distance estimate of roughly 350 light-years from the Sun. It is moving away from the Sun with a radial velocity of +40.5 km/s. About 2.6 million years ago, Rho Orionis made its perihelion passage at a distance of around 3.1 pc.

This is a single-lined spectroscopic binary system with an orbital period of 2.8 years and an eccentricity of 0.1. The visible component is an evolved giant star of type K with a stellar classification of K0 III. Its measured angular diameter is $2.19 mas$, which, at its estimated distance yields a physical size of about 25 times the radius of the Sun. It has 2.67 times the mass of the Sun and is about 650 million years old. The star is radiating 251 times the Sun's luminosity from its enlarged photosphere at an effective temperature of $4,533 K$.