So, what happened to the mass?
  1. Dynamical excitation: Something excited the KB feeding most of mass inward.
  2. Collisional Grinding: In an excited KB collisions grind it down. Img
But, none of these appear to work very well.
We can circumvent the mass depletion problem if:
  1. we imagine the planetesimal disk was truncated near 30AU (Levison & Morbidelli 2003: ) , and
  2. the Kuiper belt was pushed out.
The Nice Model supplies us a mechanism to doing this (and getting the orbits as well Img Img):
image image image