  This paper shows that the inclinations of bodies captured into mean motion
resonances in the Kuiper belt have remained very nearly unchanged, being only
slightly increased from initial lower values by migration and/or by long-term
planetary perturbations. Thus the observed maximum as high as ~ 30 deg of the
i's of bodies in resonance must reflect either a broad initial range at least
to that level for capturable bodies or an elevating process possibly
exemplified by the sweeping of secular resonances. We have obtained capture
probabilities for 2 well-populated resonances, showing reduced but finite
values for i's up to 35 deg. Whatever led to the present distribution must have
produced increases in i for some, but not for all, resonant bodies in the belt.
