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Kepler will monitor enough stars that it is likely to detect single transitsof planets with periods longer than the mission lifetime. We show that bycombining the Kepler photometry of such transits with precise radial velocity(RV) observations taken over ~3 months, and assuming circular orbits, it ispossible to estimate the periods of these transiting planets to better than 20%(for planets with radii greater than that of Neptune) and the masses to withina factor of 2 (for planet masses m_p > M_Jup). We also explore the effects ofeccentricity on our estimates of these uncertainties.

Getting More For Your Money: Identifying and Confirming Long-Period Planets with Kepler