  KIC 3230227 is a short period ($P\approx 7.0$ days) eclipsing binary with a
very eccentric orbit ($e=0.6$). From combined analysis of radial velocities and
{\it Kepler} light curves, this system is found to be composed of two A-type
stars, with masses of $M_1=1.84\pm 0.18M_{\odot}$, $M_2=1.73\pm 0.17M_{\odot}$
and radii of $R_1=2.01\pm 0.09R_{\odot}$, $R_2=1.68\pm 0.08 R_{\odot}$ for the
primary and secondary, respectively. In addition to an eclipse, the binary
light curve shows a brightening and dimming near periastron, making this a
somewhat rare eclipsing heartbeat star system. After removing the binary light
curve model, more than ten pulsational frequencies are present in the Fourier
spectrum of the residuals, and most of them are integer multiples of the
orbital frequency. These pulsations are tidally driven, and both the amplitudes
and phases are in agreement with predictions from linear tidal theory for $l=2,
m=-2$ prograde modes.
