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2M1938+4603 (KIC 9472174) displays a spectacular light curve dominated by a strong reflection effect and rather shallow, grazing eclipses. The orbital period is 0.126 d, the second longest period yet found for an eclipsing sdB+dM, but still close to the minimum 0.1‐d period among such systems. The phase‐folded  Kepler  light curve was used to detrend the orbital effects from the data set. The amplitude spectrum of the residual light curve reveals a rich collection of pulsation peaks spanning frequencies from ∼50 to 4500 μHz. The presence of a complex pulsation spectrum in both the p‐ and g‐mode regions has never before been reported in a compact pulsator.  Eclipsing sdB+dM stars are very rare, with only seven systems known and only one with a pulsating primary. Pulsating stars in eclipsing binaries are especially important since they permit masses derived from seismological model fits to be cross‐checked with orbital mass constraints. We present a first analysis of this star based on the  Kepler  9.7‐d commissioning light curve and extensive ground‐based photometry and spectroscopy that allow us to set useful bounds on the system parameters. We derive a radial‐velocity amplitude   K  1 = 65.7 ± 0.6  km s  −1  , inclination angle , and find that the masses of the components are   M  1 = 0.48 ± 0.03  M ⊙   and   M  2 = 0.12 ± 0.01  M ⊙  .

2M1938+4603: a rich, multimode pulsating sdB star with an eclipsing dM companion observed with Kepler