This session provides a framework for discussing the properties of micrometeoroids, meteorites, and interplanetary and interstellar dust, with sizes ranging from the nano-dust to cm-sized, or even larger objects. Papers are invited discussing compositional aspects as well as dynamical investigations of the smallest bodies in our Solar System.
Remote-sensing investigations of the zodiacal cloud, or studies related to interstellar dust are welcome. Spacecraft data of New Horizon, Cassini and STEREO are unique and provide insights into the dynamics and evolution of dusty phenomena in our Solar System.