  We investigate several predictions about the properties of IIB flux vacua on
Calabi-Yau orientifolds, by constructing and characterizing a very large set of
vacua in a specific example, an orientifold of the Calabi-Yau hypersurface in
$WP^{4}_{1,1,1,1,4}$. We find support for the prediction of Ashok and Douglas
that the density of vacua on moduli space is governed by ${\rm det}(-R -
\omega)$ where $R$ and $\omega$ are curvature and K\"ahler forms on the moduli
space. The conifold point $\psi=1$ on moduli space therefore serves as an
attractor, with a significant fraction of the flux vacua contained in a small
neighborhood surrounding $\psi=1$. We also study the functional dependence of
the number of flux vacua on the D3 charge in the fluxes, finding simple power
law growth.
