| タイトル | Strata-1: An International Space Station Experiment into Fundamental Regolith Processes in Microgravity |
| 本文（外部サイト） | http://hdl.handle.net/2060/20160003139 |
| 著者（英） | Colwell, J.; Durda, D.; John, K.; Dove, A.; Fries, M.; Graham, L.; Love, S.; Abell, P.; Britt, D.; Brisset, J.; Hartzell, C. |
| 発行日 | 2016-03-21 |
| 言語 | eng |
| 内容記述 | The Strata-1 experiment will study the evolution of asteroidal regolith through long-duration exposure of simulant materials to the microgravity environment on the International Space Station (ISS). Many asteroids feature low bulk densities, which implies high values of porosity and a mechanical structure composed of loosely bound particles, (i.e. the "rubble pile" model), a prime example of a granular medium. Even the higher-density, mechanically coherent asteroids feature a significant surface layer of loose regolith. These bodies are subjected to a variety of forces and will evolve in response to very small perturbations such as micrometeoroid impacts, planetary flybys, and the YORP effect. Our understanding of this dynamical evolution and the inter-particle forces involved would benefit from long-term observations of granular materials exposed to small vibrations in microgravity. A detailed understanding of asteroid mechanical evolution is needed in order to predict the surface characteristics of as-of-yet unvisited bodies, to understand the larger context of samples collected by missions such as OSIRIS-REx and Hayabusa 1 and 2, and to mitigate risks for both manned and unmanned missions to asteroidal bodies. Understanding regolith dynamics will inform designs of how to land and set anchors, safely sample/move material on asteroidal surfaces, process large volumes of material for in situ resource utilization (ISRU) purposes, and, in general, predict behavior of large and small particles on disturbed asteroid surfaces. |
| NASA分類 | Lunar and Planetary Science and Exploration |
| レポートNO | JSC-CN-35560 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
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