  We report on annual parallax and proper motion observations of H2O masers in
S235AB-MIR, which is a massive young stellar object in the Perseus Arm. Using
multi-epoch VLBI astrometry we measured a parallax of pi = 0.63 +- 0.03 mas,
corresponding to a trigonometric distance of D = 1.56+-0.09 kpc, and source
proper motion of ( u alpha cos d , u d) = (0.79 +- 0.12, -2.41 +- 0.14) mas/yr.
Water masers trace a jet of diameter 15 au which exhibits a definite radial
velocity gradient perpendicular to its axis. 3D maser kinematics were well
modelled by a rotating cylinder with physical parameters: v_out = 45+-2 km/s,
v_rot = 22+-3 km/s, i = 12+-2 degrees, which are the outflow velocity,
tangential rotation velocity and line-of-sight inclination, respectively. One
maser feature exhibited steady acceleration which may be related to the jet
rotation. During our 15 month VLBI programme there were three `maser burst'
events caught `in the act' which were caused by the overlapping of masers along
the line of sight.
