  One of the most important questions in the study of compact objects is the
nature of pulsars, including whether they consist of neutron matter or strange
quark matter (SQM). However, few mechanisms for distinguishing between these
two possibilities have been proposed. The purpose of this paper is to show that
a strange star (one made of SQM) will have a vibratory mode with an oscillation
frequency of approximately 250 GHz (millimeter wave). This mode corresponds to
motion of the center of the expected crust of normal matter relative to the
center of the strange quark core, without distortion of either. Radiation from
currents generated in the crust at the mode frequency would be a SQM signature.
We also consider effects of stellar rotation, estimate power emission and
signal-to-noise ratio, and discuss briefly possible mechanisms for exciting the
mode.
