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IRAS 16293-2422 is a very well studied young stellar system seen inprojection towards the L1689N cloud in the Ophiuchus complex. However, itsdistance is still uncertain with a range of values from 120 pc to 180 pc. Ourgoal is to measure the trigonometric parallax of this young star by means ofH$_2$O maser emission. We use archival data from 15 epochs of VLBA observationsof the 22.2 GHz water maser line. By modeling the displacement on the sky ofthe H$_2$O maser spots, we derived a trigonometric parallax of $7.1\pm1.3$ mas,corresponding to a distance of $141_{-21}^{+30}$ pc. This new distance is ingood agreement with recent values obtained for other magnetically active youngstars in the L1689 cloud. We relate the kinematics of these masers with theoutflows and the recent ejections powered by source A in the system.

A revised distance to IRAS 16293$-$2422 from VLBA astrometry of associated water masers