  There are many competing theories and models describing the formation,
migration and evolution of exoplanet systems. As both the precision with which
we can characterize exoplanets and their host stars, and the number of systems
for which we can make such a characterization increase, we begin to see
pathways forward for validating these theories. In this white paper we identify
predicted, observable correlations that are accessible in the near future,
particularly trends in exoplanet populations, radii, orbits and atmospheres
with host star age. By compiling a statistically significant sample of
well-characterized exoplanets with precisely measured ages, we should be able
to begin identifying the dominant processes governing the time-evolution of
exoplanet systems.
