For the simulation of the first stage of preplanetary dust aggregation, we
developed the cosmic dust aggregation experiment (CODAG). With CODAG, we in
tend to study the aggregational behaviour of a cloud of micron-sized dust p
articles due to Brownian motion of the grains. For a realistic simulation o
f the processes in the young solar system, the dust grains have to be dispe
rsed in a rarefied gas so that mutual collisions are ballistic. Fast sedime
ntation of the grains in the Earth's gravitational field leads to unrealist
ic collision velocities and to a rapid loss of particles to the container w
alls. Therefore, CODAG was designed to work in a microgravity environment.
In this paper, we present an overview of the experimental design of CODAG w
hich was recently flown in a Get Away Special container during the STS-95 m
ission.