The phenomenological possibilities of the Randall-Sundrum noncompact extra
dimension scenario with the AdS horizon increased to approximately a millim
eter length, corresponding to an effective brane tension of (Tev)(4), are i
nvestigated. The corrections to the Newtonian potential are found to be the
only observationally accessible probe of this scenario, as previously sugg
ested in the literature. In particular, the presence of the continuum of Ka
luza-Klein modes does not lead to any observable collider signatures. The e
xtent to which experimental tests of Newtonian gravity can distinguish this
scenario from the scenario of Arkani-Hamed, Dimopoulos, and Dvali, with 1-
and 2-mm size extra dimensions, is explicitly demonstrated.