The detection of astrophysical Gamma-Ray Bursts (GRBs) has always been intertwined with the challenge of identifying the direction of the source. Accurate angular localization of better than a degree has been achieved to date only with heavy instruments on large satellites, and a limited field of view. The recent discovery of the association of GRBs with neutron star mergers gives new motivation for observing the entire $gamma$-ray sky at once with high sensitivity and accurate directional capability. We present a novel $gamma$-ray detector concept, which utilizes the mutual occultation between many small scintillators to reconstruct the GRB direction. We built an instrument with 90 (9,mm)$^3$ csi~scintillator cubes attached to silicon photomultipliers. Our laboratory prototype tested with a 60,keV source demonstrates an angular accuracy of a few degrees for $sim$25 ph,cm$^{-2}$ bursts. Simulations of realistic GRBs and background show that the achievable angular localization accuracy with a similar instrument occupying $1$l volume is $<2^circ$. The proposed concept can be easily scaled to fit into small satellites, as well as large missions.
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