64 Arietis is a possible binary star[2] system in the northern constellation of Aries.
It is faintly visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of +5.67.
[2] Based upon an annual parallax shift of 15.2 mas,[1] this star is approximately 214 light-years (66 parsecs) distant from the Sun.
[3] With the supply of hydrogen at its core exhausted, the star has expanded to 11 times the radius of the Sun and it shines with 42 times the Sun's luminosity.
[5] This energy is being radiated from the outer envelope at an effective temperature of 4,426 K,[5] giving it the orange-hued glow of a K-type star.