  This work explores the orbital distribution of minor bodies in the outer
Solar System emplaced as a result of a Nice model migration from the
simulations of Brasser & Morbidelli (2013). This planetary migration scatters a
planetesimal disk from between 29-34 AU and emplaces a population of objects
into the Kuiper belt region. From the 2:1 Neptune resonance and outward, the
test particles analyzed populate the outer resonances with orbital
distributions consistent with trans-Neptunian object (TNO) detections in
semi-major axis, inclination, and eccentricity, while capture into the closest
resonances is too efficient. The relative populations of the simulated
scattering objects and resonant objects in the 3:1 and 4:1 resonances are also
consistent with observed populations based on debiased TNO surveys, but the 5:1
resonance is severely underpopulated compared to population estimates from
survey results. Scattering emplacement results in the expected orbital
distribution for the majority of the TNO populations, however the origin of the
large observed population in the 5:1 resonance remains unexplained.
