XZ Tauri is a binary system approximately 460 light-years away in the constellation Taurus. The system consists of two T Tauri stars orbiting each other about 6 billion kilometers apart (roughly the same distance as Pluto is from the Sun). The system made news in 2000 when a superflare was observed in the system. A third star, component C, has been observed at a separation of 0.09″, but subsequent observations failed to find it. The T Tauri star HL Tauri, 23″ away, is also sometimes listed as a companion. The discovery by Pelageya Fedorovna Shajn, that XZ Tauri is a variable star, was announced in 1928.
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External links "Movies from Hubble Show the Changing Faces of Infant Stars". HubbleSite. NASA. 21 September 2000. Retrieved 23 August 2009. XZ Tauri at Constellation Guide




