The region of the solar system immediately beyond Neptune's orbit is densel
y populated with small bodies. This region, known as the Kuiper Belt, consi
sts of objects that may predate Neptune, the orbits of which provide a foss
il record of processes operative in the young solar system. The Kuiper Belt
contains some of the Solar System's most primitive, least thermally proces
sed matter. It is probably the source of the short-period comets and Centau
rs, and may also supply collisionally generated interplanetary dust. I disc
uss the properties of the Kuiper Belt and provide an overview of the outsta
nding scientific issues.