  Multi-epoch GHz Very Long Baseline Interferometry (VLBI) data of the
radio-loud quasar J1101+7225 were analyzed to estimate the proper motion of
extended optically thin jet components. Two components separated from the core
could be mapped at 1.66 GHz, which is consistent with earlier observations. In
one case we found evidence of high apparent superluminal motion (beta_app=
22.5+/-4) at large (deprojected) distances to the core (22 mas ~ 4 kpc at z=
1.46). Typically in other quasars such high separation velocities are only
found much closer to the core component. Furthermore the Doppler factor, the
magnetic field strength, and the angular size of the optically thick core were
derived using published X-ray data. Analysis of 5 GHz VLBI data reveals the
existence of further jet components within the central 5 mas. Additionally the
data published so far on the GHz-spectrum were discussed at all angular
resolutions. J1101+7225 turns out to be a standard quasar for studying
different aspects of radio jet kinematics out to kpc-scales.
