Updated proper motions for 328 probable members of the Praesepe are used to
determine the distance to this open cluster by Hertzsprung's geometric met
hod. The cluster distance was found to be r = 171 +/- 15 pc, which correspo
nds to the distance modulus V-0-M-V = 6(m).16 +/- 0.19. The distance scale
for open clusters is discussed. (C) 2000 MAIK "Nauka/Interperiodica".