Perturbative calculations suggest that the electroweak phase transitio
n in the minimal supersymmetric standard model (MSM) can be strong eno
ugh for baryogenesis for Higgs masses up to m(H) similar to 105 GeV, p
rovided that the lightest stop mass is in the range 100-160 GeV. We ha
ve performed large-scale lattice Monte Carlo simulations of the MSSM e
lectroweak phase transition. We find that the transition is in fact st
ronger than in perturbation theory. This guarantees that the perturbat
ive mass bounds are conservative ones, and provides a strong motivatio
n for further studies of MSSM baryogenesis.