  Jupiter is one of the major targets for planetary exploration, and dust in
the Jovian system is of great interest to researchers in the field of planetary
science. In this paper, we review the five dust populations outside the ring
system: grains in the region of the Galilean moons, potential dust from plumes
on Europa, Jovian stream particles, particles in the outer region of the Jovian
system ejected from the irregular satellites, and dust in the region of the
Trojan asteroids. The physical environment for the dust dynamics is described,
including the gravity, the magnetic field and the plasma environment. For each
population, the dust sources are described, and the relevant perturbation
forces are discussed. Observations and results from modeling are reviewed, and
the distributions of the individual dust populations are shown. The
understanding of the Jovian dust environment allows to assess the dust hazard
to spacecraft, and to characterize the material exchange between the Jovian
moons, their surface properties and distribution of non-icy constituents.
