  We study spherically symmetric, stationary vacuum configurations in general
covariant theory (U(1) extension) of Ho\v{r}ava-Lifshitz gravity with the
projectability condition and an arbitrary coupling constant $\lambda$, and
obtain all the solutions in closed forms. If the gauge field $A$ and the
Newtonian prepotential $\varphi$ do not directly couple to matter fields, the
theory is inconsistent with solar system tests for $\lambda\not=1$, no matter
how small $|\lambda-1|$ is. This is shown to be true also with the most general
ansatz of spherical (but not necessarily stationary) configurations. Therefore,
to be consistent with observations, one needs either to find a mechanism to
restrict $\lambda$ precisely to $\lambda_{GR}=1$, or to consider $A$ and/or
$\varphi$ as parts of the 4-dimensional metric on which matter fields
propagate. In the latter, requiring that the line element be invariant not only
under the foliation-preserving diffeomorphism but also under the local U(1)
transformations, we propose the replacements, $N \rightarrow N - \upsilon(A -
{\cal{A}})/c^2$ and $N^i \rightarrow N^i+N\nabla^{i}\varphi$, where $\upsilon$
is a dimensionless coupling constant to be constrained by observations, $N$ and
$N^i$ are, respectively, the lapse function and shift vector, and ${\cal{A}}
\equiv - \dot{\varphi} + N^i\nabla_{i}\varphi + N(\nabla_{i}\varphi)^2/2$. With
this prescription, we show explicitly that the aforementioned solutions are
consistent with solar system tests for both $\lambda=1$ and $\lambda\not=1$,
provided that $|\upsilon-1|<10^{-5}$. From this result, the physical and
geometrical interpretations of the fields $A$ and $\varphi$ become clear.
However, it still remains to be understood how to obtain such a prescription
from the action principle.
