We make predictions for the rate of discovery of eclipsing white dwarf-main-sequence (WD-MS) binaries in terrestrial-planet transit searches, taking the planned Kepler and Eddington missions as examples. We use a population synthesis model to characterize the Galactic WD-MS population, and we find that, despite increased noise due to stellar variability compared with the typical planetary case, discovery of ≳10 2 nonaccreting, eclipsing WD-MS systems is likely using Kepler and Eddington , with periods of 2-20 days and transit amplitudes of |Δ m | ~ 10 -4±0.5 mag. Follow-up observations of these systems could accurately test the theoretical white dwarf mass-radius relation or theories of binary star evolution.
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