  Lithium is a sensitive probe to mixing processes operating in stellar
interiors. For many years, a connection has been suspected to exist between
lithium abundances and stellar rotation, presumably the result of
rotationally-induced internal mixing. In recent years, several studies have
confirmed and refined this relationship for low-mass young stars. In various
star forming regions and young open clusters, rapidly rotating K dwarfs are
found to be lithium-rich compared to their more slowly rotating siblings. While
this lithium-rotation correlation is contrary to naive expectations, several
models have been put forward to account for it. We review here recent
observational results, and briefly discuss proposed interpretations.
