  We perform mode identification for five $\delta$ Scuti stars in the Pleiades
star cluster, using custom light curves from K2 photometry. By creating
\'echelle diagrams, we identify radial and dipole mode ridges, comprising a
total of 28 radial and 16 dipole modes across the five stars. We also suggest
possible identities for those modes that lie offset from the radial and dipole
ridges. We calculate non-rotating stellar pulsation models to verify our mode
identifications, finding good agreement within the age and metallicity
constraints of the cluster. We also find that for all stars, the least dense
models are preferred, reflecting the lower density of these oblate, rotating
stars. Three of the five stars show rotationally-split multiplets. We conclude
that the sample shows promise for asteroseismic rotation rates, masses, and
ages with rotating models in the future. Our preliminary modelling also
indicates some sensitivity to the helium abundance.
