We consider a cosmological model in which our Universe is a spherically sym
metric bubble wall in 5-dimensional anti-de Sitter-time. We argue that the
bubble on which we live will undergo collisions with other similar bubbles
and estimate the spectrum of such collisions. The collision rate is found t
o be independent of the age of our Universe. Collisions with small bubbles
provide an experimental signature of this scenario, while collisions with l
arger bubbles would be catastrophic. (C) 2001 Published by Elsevier Science
B.V.