  We present an early result from an automated search of Kepler eclipsing
binary systems for circumbinary companions. An intriguing tertiary signal has
been discovered in the short period eclipsing binary KIC002856960. This third
body leads to transit-like features in the light curve occurring every 204.2
days, while the two other components of the system display eclipses on a 6.2
hour period. The variations due to the tertiary body last for a duration of
\sim1.26 days, or 4.9 binary orbital periods. During each crossing of the
binary orbit with the tertiary body, multiple individual transits are observed
as the close binary stars repeatedly move in and out of alignment with the
tertiary object. We are at this stage unable to distinguish between a planetary
companion to a close eclipsing binary, or a hierarchical triply eclipsing
system of three stars. Both possibilities are explored, and the light curves
presented.
