  The diversity of planetary systems that have been discovered are revealing
the plethora of possible architectures, providing insights into planet
formation and evolution. They also increase our understanding of system
parameters that may affect planetary habitability, and how such conditions are
influenced by initial conditions. The AU~Mic system is unique among known
planetary systems in that it is a nearby, young, multi-planet transiting
system. Such a young and well characterized system provides an opportunity to
study orbital dynamical and habitability studies for planets in the very early
stages of their evolution. Here, we calculate the evolution of the Habitable
Zone of the system through time, including the pre-main sequence phase that the
system currently resides in. We discuss the planetary atmospheric processes
occurring for an Earth-mass planet during this transitionary period, and
provide calculations of the climate state convergence age for both volatile
rich and poor initial conditions. We present results of an orbital dynamical
analysis of the AU~Mic system that demonstrate the rapid eccentricity evolution
of the known planets, and show that terrestrial planets within the Habitable
Zone of the system can retain long-term stability. Finally, we discuss
follow-up observation prospects, detectability of possible Habitable Zone
planets, and how the AU Mic system may be used as a template for studies of
planetary habitability evolution.
