  More than 100 extrasolar planets have been discovered since 1990s. Different
from the solar system, these planets' orbital eccentricities cover a huge range
from 0 to 0.7. Incidently, the first Kuiper Belt Object was discovered in 1992.
Thus, an interesting and important question will be whether extrasolar
planetary systems could have structures like Kuiper Belt or asteroid belt. We
investigate the stability of these planetary systems with different orbital
eccentricities by the similar procedures in Rabl & Dvorak (1988) and Holman &
Wiegert (1999). We claim that most extrasolar planetary systems can have their
own belts at the outer regions. However, we find that the orbits with
high--eccentricity is very powerful in depletion of these populations.
