  We have extended the time baseline for observations of the proper motions of
radio sources in the Orion BN/KL region from 14.7 to 22.5 years. We present
improved determinations for the sources BN and I. In addition, we address the
proper motions of the double radio source n, that have been questioned in the
literature. We confirm that all three sources are moving away at transverse
velocities of tens of km s$^{-1}$ from a region in-between them, where they
were located about 500 years ago. Source n exhibits a new component that we
interpret as due to a one-sided ejection of free-free emitting plasma that took
place after 2006.36. We used the highly accurate relative proper motions
between sources BN and I to determine that their closest separation took place
in the year 1475$\pm$6, when they were within $\sim$100 AU or less from each
other in the plane of the sky.
