  Several recent works have claimed that the Weak Gravity Conjecture (WGC)
excludes super-Planckian displacements of axion fields, and hence large-field
axion inflation, in the absence of monodromy. We argue that in theories with
$N\gg1$ axions, super-Planckian axion diameters $\cal{D}$ are readily allowed
by the WGC. We clarify the nontrivial relationship between the kinetic matrix
$K$ --- unambiguously defined by its form in a Minkowski-reduced basis --- and
the diameter of the axion fundamental domain, emphasizing that in general the
diameter is not solely determined by the eigenvalues $f_1^2 \le ... \le f_N^2$
of $K$: the orientations of the eigenvectors with respect to the
identifications imposed by instantons must be incorporated. In particular, even
if one were to impose the condition $f_N<M_{pl}$, this would imply neither
${\cal D}<M_{pl}$ nor ${\cal D}<\sqrt{N}M_{pl}$. We then estimate the actions
of instantons that fulfill the WGC. The leading instanton action is bounded
from below by $S \ge {\cal S} M_{pl}/f_N$, with ${\cal S}$ a fixed constant,
but in the universal limit $S\gtrsim {\cal S} \sqrt{N}M_{pl}/f_N$. Thus, having
$f_N>M_{pl}$ does not immediately imply the existence of unsuppressed higher
harmonic contributions to the potential. Finally, we argue that in effective
axion-gravity theories, the zero-form version of the WGC can be satisfied by
gravitational instantons that make negligible contributions to the potential.
