  Young stellar populations provide a record of past star formation, and by
establishing their members' dynamics and ages, it is possible to reconstruct
the full history of star formation events. Gaia has greatly expanded the number
of accessible stellar populations, with one of the most notable
recently-discovered associations being Cepheus Far North (CFN), a population
containing hundreds of members spanning over 100 pc. With its proximity (d
$\lesssim$ 200 pc), apparent substructure, and relatively small population, CFN
represents a manageable population to study in depth, with enough evidence of
internal complexity to produce a compelling star formation story. Using Gaia
astrometry and photometry combined with additional spectroscopic observations,
we identify over 500 candidate CFN members spread across 7 subgroups. Combining
ages from isochrones, asteroseismology, dynamics, and lithium depletion, we
produce well-constrained ages for all seven subgroups, revealing a largely
continuous 10 Myr star formation history in the association. By tracing back
the present-day populations to the time of their formation, we identify two
spatially and dynamically distinct nodes in which stars form, one associated
with $\beta$ Cephei which shows mostly co-spatial formation, and one associated
with EE Draconis with a more dispersed star formation history. This detailed
view of star formation demonstrates the complexity of the star formation
process, even in the smallest of regions.
