  We derive Newton's Law from the formalism of Holographic Space-Time (HST).
More precisely, we show that for a large class of Hamiltonians of the type
proposed previously for the HST description of a geodesic in Minkowski space,
the eikonal for scattering of two massless particles at large impact parameter
scales as expected with the impact parameter and the energies of the particles
in the center of mass (CM) frame. We also discuss the criteria for black hole
production in this collision, and find an estimate, purely within the HST
framework, for the impact parameter at which it sets in, which coincides with
the estimate based on general relativity.
