  The CoRoT and Kepler satellites were the first space platforms designed to
perform high-precision photometry for a large number of stars. Multiple systems
display a wide variety of photometric variability, making them natural
benefactors of these missions. I review the work arising from CoRoT and Kepler
observations of multiple systems, with particular emphasis on eclipsing
binaries containing giant stars, pulsators, triple eclipses and/or low-mass
stars. Many more results remain untapped in the data archives of these
missions, and the future holds the promise of K2, TESS and PLATO.
