Exploiting the five-dimensional Schwarzschild black hole, we study the geometrical natures of higher-dimensional black holes to yield the (6+1)-dimensional global embedding Minkowski space structure. We next obtain the Hawking temperature and entropy on this five-dimensional manifold, and the results are different from the four-dimensional ones. On the contrary, the radial component of the Einstein equation for the massive particles or photons on the five-dimensional spacetime is shown to have the same form as that for the four-dimensional black hole one. Moreover, we construct an effective potential on the equatorial plane of the restricted three-brane to investigate the behavior of the particles or photons on this restricted brane.