  We consider the prospects for the direct detection of dark matter in pure
gravity meditation (PGM) models of supersymmetry breaking. Minimal PGM models
require only two parameters, the gravitino mass, $m_{3/2}$, which sets the UV
mass for all scalar masses, and $\tan\beta$. Gaugino masses are generated
through anomaly mediation. Typically the lightest supersymmetric state (the
dark matter candidate) is a wino. Here, we consider a one-parameter extension
of the minimal model by allowing the Higgs soft masses to deviate from
universality. For simplicity, we take these to be equal and use the $\mu$-term
as a surrogate. We also consider non-universal stop masses. When $|\mu| \sim 1$
TeV, the Higgsino is a viable dark matter candidate when the gravitino mass is
of order $\sim 1$ PeV and $\tan\beta \simeq 2$. We calculate the spin-dependent
and spin-independent cross sections for dark matter scattering on protons. For
spin-independent scattering, existing experimental limits place constraints on
the PGM parameter space. Much of the currently allowed parameter space lies
above the irreducible neutrino background. Thus, future direct detection
experiments will be able to probe much of the remaining PGM parameter space.
