  We find the static spherically symmetric solutions (with vanishing shift
function) of the complete nonprojectable Horava theory explicitly, writing the
space-time metrics as explicit tensors in local coordinate systems. This
completes previous works of other authors that have studied the same
configurations. The solutions depend on the coupling constant alpha of the
(partial_i ln N)^2 term. The lambda = 1/3 case of the theory does not possess
any extra mode, hence the range of alpha is in principle not limited by the
linear stability of any extra mode. We study the full range of alpha, both in
the positive and negative sectors. We find the same wormhole solutions and
naked singularities that were found for the Einstein-aether theory in a sector
of the space of alpha. There also arise wormholes in other sector of alpha. Our
coordinate systems are valid at the throats of the wormholes. We also find the
perturbative solutions for small alpha. We give this version of the solutions
directly on the original radial coordinate r, which is particularly suitable
for representing the exterior region of solutions with localized sources.
