ARISE: A granular matter experiment on the International Space Station
arXiv:1911.05429 · doi:10.1063/1.5095213
Abstract
We developed an experiment to study different aspects of granular matter under microgravity. The 1.5U small experiment was carried out on the International Space Station. About 3500 almost identical spherical glass particles with 856 um diameter were placed in a container of 50*50 mm cross section. Adjusting the height between 5 and 50 mm, the filling factor can be varied. The sample was vibrated under different frequencies and amplitudes. The majority of the data are video images of the particles motion. Here, we first give an overview of the general setup and a first qualitative account of different phenomena observed in about 700 experimental runs. These phenomena include collisional cooling, collective motion via gas-cluster coupling, and the influence of electrostatic forces on particle-particle interactions.
arXiv commentThis article may be downloaded for personal use only. Any other use requires prior permission of the author and AIP Publishing. This article appeared in (Review of Scientific Instruments 90:10 2019) and may be found at (https://aip.scitation.org/doi/10.1063/1.5095213)
References in corpus (11)
- The outcome of protoplanetary dust growth: pebbles, boulders, or planetesimals? II. Introducing the bouncing barrier
- Energy Dissipation in Driven Granular Matter in the Absence of Gravity
- Collisions of CO Ice Grains in Planet Formation
- Ice Grain Collisions in Comparison: CO, HO and their Mixtures
- Experimental Study on Bouncing Barriers in Protoplanetary Disks
- Failed Growth at the Bouncing Barrier in Planetesimal Formation
- Early-stage aggregation in three-dimensional charged granular gas
- Are Pebble Pile Planetesimals Doomed?
- Impact-induced energy transfer and dissipation in granular clusters under microgravity conditions
- Dense Particle Clouds in Laboratory Experiments in Context of Drafting and Streaming Instability
- NanoRocks: Design and Performance of an Experiment Studying Planet Formation on the International Space Station
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- Zero-gravity thermal convection in granular gases