  Planetary materials orbiting white dwarf stars reveal the ultimate fate of
the planets of the Solar System and all known transiting exoplanets. Observed
metal pollution and infrared excesses from debris disks support that planetary
systems or their remnants are common around white dwarf stars; however, these
planets are difficult to detect since a very high orbital inclination angle is
required for a small white dwarf to be transited, and these transits have very
short (minute) durations. The low odds of catching individual transits could be
overcome by a sufficiently wide and fast photometric survey. I demonstrate
that, by obtaining over 100 million images of white dwarf stars with 30-second
exposures in its first three years, the Zwicky Transient Facility (ZTF) is
likely to record the first exoplanetary transits of white dwarfs, as well as
new systems of transiting, disintegrating planetesimals. In these proceedings,
I describe my project strategy to discover these systems using the ZTF data.
