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Binary star system in the constellation Aries
For other stars with this Bayer designation, see τ Arietis.
The Tau Arietis system contains three stars. The inner pair form an eclipsing binary system, with the brightness of the pair decreasing by 0.06 in magnitude during an eclipse of the primary. Its period is 2.20356 days. The third component is located at an angular separation of 0.810 arcseconds and has a magnitude of 8.17. The primary component is a subgiant star with a stellar classification of B5 IV. It has five times the mass of the Sun with about four times the Sun's radius.
This system is a member of the Cas-Tau OB association of stars that share a common motion through space.
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