  The study of active asteroids has attracted a great deal of interest in
recent years since the recognition of main-belt comets (which orbit in the main
asteroid belt, but exhibit comet-like activity due to the sublimation of
volatile ices) as a new class of comets in 2006, and the discovery of the first
disrupted asteroids (which, unlike MBCs, exhibit comet-like activity due to a
physical disruption such as an impact or rotational destabilization, not
sublimation) in 2010. In this paper, I will briefly discuss key areas of
interest in the study of active asteroids.
