Since the periodicity of comets was first established by Halley, the q
uestion of their origin has fascinated astronomers. It is clear that t
hey have to be stored somewhere, since their life time in the inner So
lar System is short, Around 1950 the idea emerged that cometary nuclei
could be stored in a belt beyond Neptune, and this belt became known
as the Kuiper Belt or perhaps more fairly the Kuiper-Edgeworth Belt. I
n the late 80's optical searches for the belt became numerous and in 1
992, the first detection (of 1992 QB1) was made. At the time of writin
g 39 objects have been discovered and the current state of knowledge r
egarding these ''Kuiper-Edgeworth Belt'', or Trans-Neptunian, Objects
is reviewed here.