Kirchhoff's thermodynamically based classical theorem (the energy dens
ity of the radiation in equilibrium is a function of T only) is used t
o obtain a relation relevant to study of the Casimir effect. We use it
to obtain the zero-temperature Casimir energy without recourse to reg
ularization. The intimate connection between the zero-point energy and
the thermal Bose occupancy expression noted by Einstein and Stern at
the turn of the century is invoked to account for the results.