Comparison of the probability distributions for the Upper Scorpius and Taurus median disks. The striking differences in the disk scale height and flaring index show that the median Upper Scorpius SED represents a disk that has experienced more dust settling than in Taurus. The low dust mass hints at the potential importance of grain growth in reducing opacity and hence detectable dust mass. The sharp edges to the Upper Scorpius distributions are due to the sampling of the parameter space.