  We present 10.27$ \rm{hrs}$ of photometry of the roAp star HD 134214 obtained
by the MOST satellite. The star is shown to be monoperiodic and oscillating at
a frequency of 2948.97$ \pm 0.55 \mu\rm{Hz}$. This is consistent with earlier
ground based photometric campaigns (e.g. Kreidl et al. 1994). We do not detect
any of the additional frequencies identified in the recent spectroscopic study
by Kurtz et al. (2006) down to an amplitude limit of 0.36$ \rm{mmag}$
($2\sigma$ significance limit).
