  Relatively simple models can be constructed in which supersymmetry is
dynamically broken at energies of $10^5-10^7$ GeV. Models of this kind do not
suffer from the naturalness and cosmological difficulties of conventional
supergravity models, and make definite predictions for the spectrum of
supersymmetric particle masses. Thus ``Renormalizable Visible Sector Models''
are a viable alternative to more conventional approaches. This talk mostly
summarizes the results of a recent paper written with Michael Dine and Yuri
Shirman.
