We summarize the evidence that most Population I Cepheids with periods
less than similar to 8 days pulsate in the first overtone mode. Funda
mental mode and first overtone pulsators must follow different period-
luminosity (P-L) relations. We demonstrate these different relations f
or different stellar systems, especially for the calibrating Cepheids
in clusters and for Cepheids in the LMC, the SMC, M31, and IC 4182.