  We present detailed characterization of the extremely dusty main sequence
star TYC 8830 410 1. This system hosts inner planetary system dust (Tdust~300
K) with a fractional infrared luminosity of ~1%. Mid-infrared spectroscopy
reveals a strong, mildy-crystalline solid-state emission feature. TYC 8830 410
1 (spectral type G9V) has a 49.5" separation M4-type companion co-moving and
co-distant with it, and we estimate a system age of ~600 Myr. TYC 8830 410 1
also experiences "dipper"-like dimming events as detected by ASAS-SN, TESS, and
characterized in more detail with the LCOGT. These recurring eclipses suggest
at least one roughly star-sized cloud of dust orbits the star in addition to
assorted smaller dust structures. The extreme properties of the material
orbiting TYC 8830 410 1 point to dramatic dust-production mechanisms that
likely included something similar to the giant-impact event thought to have
formed the Earth-Moon system, although hundreds of millions of years after such
processes are thought to have concluded in the solar system. TYC 8830 410 1
holds promise to deliver significant advances in our understanding of the
origin, structure, and evolution of extremely dusty inner planetary systems.
