  The iconic planetary nebula (PN) NGC 7027 is bright, nearby (D ~ 1 kpc),
highly ionized, intricately structured, and well observed. This nebula is hence
an ideal case study for understanding PN shaping and evolution processes.
Accordingly, we have conducted a comprehensive imaging survey of NGC 7027
comprised of twelve HST Wide Field Camera 3 images in narrow-band and continuum
filters spanning the wavelength range 0.243--1.67 microns. The resulting
panchromatic image suite reveals the spatial distributions of emission lines
covering low-ionization species such as singly ionized Fe, N, and Si, through H
recombination lines, to more highly ionized O and Ne. These images, combined
with available X-ray and radio data, provide the most extensive view of the
structure of NGC 7027 obtained to date. Among other findings, we have traced
the ionization structure and dust extinction within the nebula in sub-arcsecond
detail; uncovered multipolar structures actively driven by collimated winds
that protrude through and beyond the PN's bright inner core; compared the
ionization patterns in the WFC3 images to X-ray and radio images of its
interior hot gas and to its molecular outflows; pinpointed the loci of thin,
shocked interfaces deep inside the nebula; and more precisely characterized the
central star. We use these results to describe the recent history of this young
and rapidly evolving PN in terms of a series of shaping events. This
evolutionary sequence involves both thermal and ram pressures, and is far more
complex than predicted by extant models of UV photoionization or winds from a
single central progenitor star, thereby highlighting the likely influence of an
unseen binary companion.
