  We propose that the 3.2 sigma excess at ~150 GeV in the dijet mass spectrum
of W + jets reported by CDF is the technipion $\pi_T$ of low-scale technicolor.
Its relatively large cross section is due to production of a narrow $Wjj$
resonance, the technirho, which decays to W + $\pi_T$. We discuss ways to
enhance and strengthen the technicolor hypothesis and suggest companion
searches at the Tevatron and LHC.
