V1094 Tauri is a system of at least three stars in the constellation of Taurus. Two stars are resolved apart; the brighter is an eclipsing binary. In 2015, the parameters for the eclipsing pair were precisely measured. Radial velocity data also revealed apsidal motion with a period of , which may indicate a third star.
The star system was included in a 2003 study that featured GK Draconis and V1094 Tauri. The study suggested a mass of for the primary star and a mass of for the secondary. The two stars orbit each other at a distance of around 0.091 to 0.092 astronomical units and have an orbital period of around 9 days.
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