The n-time generalization of the Tangherlini solution is considered. T
he equations of geodesics for the metric are integrated. For n = 2 it
is shown that the naked singularity is absent only for two sets of par
ameters, corresponding to the trivial extensions of the Tangherlini so
lution. The motion of a relativistic particle in a multi-temporal back
ground is considered. This motion is governed by the gravitational mas
s tensor. Some generalizations of the solution, including the multi-te
mporal analogue of the Myers-PetTy charged black bole solution, are ob
tained.