  We explore dark matter in the Finely Tuned Minimal Supersymmetric Standard
model recently proposed by Arkani-Hamed and Dimopoulos. Relative to the MSSM,
there are fewer particles at freeze-out, so the calculation of the relic
abundance simplifies. Similarly, the predictions for direct detection of the
dark matter sharpen. There is a large region of mixed bino--higgsino dark
matter where the lightest supersymmetric particle will be accessible at both
the LHC and future direct detection experiments, allowing for a conclusive
identification of the dark matter particle. Typical dark matter-nucleon cross
sections are 10^{-45}-10^{-44} cm^{2}. This model also possesses a novel region
where the dark matter annihilates via an s-channel Higgs boson resonance.
