A class of static solution around a global monopole resulting from the
breaking of a global SO(3) symmetry is obtained in a five-dimensional
spacetime, whose three-dimensional usual space section is spherically
symmetric. Depending on the choice of the arbitrary constants, the so
lutions may be shown to interpolate between a five-dimensional Schwarz
schild-like solution with a singularity at the origin and a nonsingula
r solution representing a soliton. However, this nonsingular behaviour
breaks down when viewed from an effective four-dimensional formalism.
Analysis of null and time-like orbits in our spacetime reveals the ex
istence of the trapping surfaces as well as repulsive barriers. This p
aper extends earlier work of Barriola and Vilenkin to its five-dimensi
onal analogue and also a five-dimensional vacuum metric of Gross and F
erry through the inclusion of an external scalar field.