  We present a multi-wavelength analysis to reveal the nature of the enigmatic
T Tauri triple star system. New optical and infrared measurements are coupled
with archival X-ray, UV and mm datasets to show morphologies of disk material
and outflow kinematics. A dark lane of obscuring material is seen in silhouette
in several emission lines and in model-subtracted ALMA mm continuum dust
residuals near the position of T Tau Sa+Sb, revealing the attenuating
circumbinary ring around T Tau S. The flux variability of T Tau S is linked in
part to the binary orbit; T Tau Sb brightens near orbital apastron as it
emerges from behind circumbinary material. Outflow diagnostics confirm that T
Tau N powers the blue-shifted western outflow, and the T Tau S binary drives
the northwest-southeastern flow. Analysis of the southern outflow shows
periodic arcs ejected from the T Tau system. Correlation of these arc locations
and tangential kinematics with the orbit timing suggests that launch of the
last four southern outflow ejections is contemporaneous with, and perhaps
triggered by, the T Tau Sa+Sb binary periastron passage. We present a geometry
of the T Tau triple that has the southern components foreground to T Tau N,
obscured by a circumbinary ring, with mis-aligned disks and interacting
outflows. Particularly, a wind from T Tauri Sa that is perpendicular to its
circumstellar disk might interact with the circumbinary material, which may
explain conflicting high contrast measurements of the system outflows in the
literature. T Tauri is an important laboratory to understand early dynamical
processes in young multiple systems. We discuss the historical and future
characteristics of the system in this context.
