  We argue that the Smarr Formula for black holes can be expressed in terms of
a Noether charge surface integral plus a suitable volume integral, for any
gravitational theory. The integrals can be constructed as an application of
Wald's formalism. We apply this formalism to compute the mass and the Smarr
Formula for static Lovelock black holes. Finally, we propose a new prescription
for Wald's entropy in the case of Lovelock black holes, which takes into
account topological contributions to the entropy functional.
