The vacuum energy is calculated for a free, conformally-coupled scalar
field on the orbifold space-time R x S2/GAMMA where GAMMS is a finite
subgroup of O(3) acting with fixed points. The energy vanishes when G
AMMA is composed of pure rotations but not otherwise. It is shown on g
eneral grounds that the same conclusion holds for all even-dimensional
factored spheres and the vacuum energies are given as generalised Ber
noulli functions. The relevant zeta-functions are analysed in some det
ail and several identities are incidentally derived. The general discu
ssion is presented in terms of finite reflection groups.