Theta1 Crucis is a spectroscopic binary star system in the southern constellation of Crux. Its name is a Bayer designation that is Latinized from θ1 Crucis and abbreviated Theta1 Cru or θ1 Cru. This system is visible to the naked eye as a point of light with an apparent visual magnitude of 4.30m. The distance to this star, as determined using parallax measurements, is around 224 light-years (69 pc). The pair orbit each other closely with a period of 24.5 days and an eccentricity of 0.61. The primary component is an Am star, which is a chemically peculiar A-type star that shows anomalous variations in absorption lines of certain elements. It has a stellar classification of A3(m)A8-A8. With a mass 157% times that of the Sun, it radiates 81 times the Sun's luminosity from its outer atmosphere at an effective temperature of 7341 K. Unusually for a fully radiative A-type star, X-ray emissions have been detected, which may instead be coming from the orbiting companion.
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