  We study the shadow cast by the H$D$ Schwarzschild-Tangherlini black hole,
and analytically calculate the influence of extra dimensions on the shadow of a
black hole. A black hole casts a shadow as an optical appearance because of its
strong gravitational field which is known to be a dark zone covered by a circle
for a Schwarzschild black hole. We demonstrate that the null geodesic equation
can be integrated by Hamilton-Jacobi approach, which enables us to investigate
the shadow cast by the H$D$ Schwarzschild-Tangherlini black holes.
Interestingly, it turns out that, for fixed values of the mass parameter, the
shadow in H$D$ spacetimes are smaller when compared with 4$D$ Schwarzschild
black hole. Further, the shadows of H$D$ Schwarzschild-Tangherlini black holes
are concentric circles with a radius of the circle decreases with increase in
$D$. We visualize the photon regions and the shadows in various dimensions for
different values of the parameters, and the energy emission rates are is also
investigated. Our results, in the limit $D=4$, reduced exactly to
\emph{vis-$\grave{a}$-vis} Schwarzschild black hole case.
