  The dynamics of fluids is a long standing challenge that remained as an
unsolved problem for centuries. Understanding its main features, chaos and
turbulence, is likely to provide an understanding of the principles and
non-linear dynamics of a large class of systems far from equilibrium. We
consider a conceptually new viewpoint to study these features using black hole
dynamics. Since the gravitational field is characterized by a curved geometry,
the gravity variables provide a geometrical framework for studying the dynamics
of fluids: A geometrization of turbulence.
