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Hiroaki Katsuragi, a granular physics expert from Nagoya University, and Jürgen Blum of the Technische Universität Braunschweig have done just that. Blum has constructed a drop tower where microgravity and vacuum conditions are achieved to mimic the environment in space.
They fired various kinds of projectiles – plastic, lead, glass – of varying sizes at clumps of dust – which are soft and fragile – as well as at loose, dense clumps of relatively rigid glass beads. The team then carefully analyzed the impact-induced expansion and found evidence for universal energy transfer and dissipation scaling laws. In addition, the team found that the scaling laws are applicable not only to the porous agglomerate clusters but also to the dense glass-bead clusters.
Katsuragi, explains: “The result is useful to deeply understand the planet-formation process. At the same time, we are surprised at the agreement of the expansion dynamics between porous (fragile) clusters and dense (rigid) clusters. Actually, the porous clusters consist of tiny grains of powder clumped together, and these clusters of many sizes are themselves clustered together. We found that this type of hierarchical structure does not affect the impact-induced dynamics.”
This study links the physics of planetary formation and clump formation through the microgravity experiment. The drop tower used in the study is unique in that short-duration impact experiments can readily be repeated at low cost. The interdisciplinary collaboration team is also unique. Hiroaki Katsuragi is a granular physicist and Jürgen Blum is a planetary physicist and both share the common goal of understanding the impact of porous and dense granular matter.
Katsuragi notes finally, “We’re all familiar with clumps of powder: they’re formed whenever we make a cake with flour. Nevertheless, the physics of clumps – of hierarchical granular matter – has not been studied well so far. This study could open up a novel research direction in the physics of granular matter.”