Physical parameters and radial pulsation modes are determined for three Delta Scuti stars in the Praesepe cluster: HD 73345, HD 73712, and HD 73746. Their agest and evolutionary massesM eare interpolated in the track systems of Iben (1967) and Paczyński (1970). By combining these age estimates with our previous results for nine other Delta Scuti-stars in the Praesepe cluster (Tsvetkov, 1989), the following weighted mean age estimates of this cluster are obtained: (14.2 ± 1.3) × 108 yr (Iben) and (5.4 ± 0.4) × 108 yr (Paczyński). Age and evolutionary mass estimates of the twelve cluster variables are also obtained in the modern track system of Maeder and Meynet (1988), in which the weighted mean cluster age is (15.3 ± 1.0) × 108 yr. Pulsation massesM Qcalculated from the fitting formulae of Faulkner (1977) and Fitch (1981) as well as massesM g=gR 2 / G were evaluated for the twelve cluster variables by Tsvetkov (1990) or in the present paper. In most cases there is a satisfactory agreement between our estimates of massesM e,M g, andM Q. Due to a large disagreement between the long period and low luminosity of the star HD 73746, its radial pulsation mode and pulsation massM Qcannot be evaluated.