Study of the rheological properties of water and Martian soil simulant mixtures for engineering applications on the red planet

被引:6
作者
Taylor, Lewis [1 ]
Alberini, Federico [1 ]
Sullo, Antonio [2 ]
Meyer, Marit E. [3 ]
Alexiadis, Alessio [1 ]
机构
[1] Univ Birmingham, Sch Chem Engn, Birmingham B15 2TT, W Midlands, England
[2] Diageo, Dunmow Rd, Birchanger CM23 5RG, Bishops Stortfo, England
[3] NASA, Glenn Res Ctr, Cleveland, OH 44135 USA
关键词
Rheology; Thixotropy; Solid dispersion; Martian regolith simulant; In situ resource utilization (ISRU); YIELD-STRESS; LUNAR; CONSTRUCTION; BEHAVIOR;
D O I
10.1016/j.asr.2017.12.037
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The rheological properties of mixtures of water and the Martian soil simulant JSC-Mars-1A are investigated by preparing and testing samples at various solids concentrations. The results indicate that the dispersion is viscoelastic and, at small timescales (similar to 0.1 s), reacts to sudden strain as an elastic solid. At longer timescales the dispersion behaves like a Bingham fluid and exhibits a yield stress. Hysteresis loops show that rapid step-changes (2 s duration) of shear-rate result in thixotropic behaviour, but slower changes (>10 s duration) can result in rheopexy. These observations are explained with the breakdown and recovery of the packing structure under stress. The rheological information is used to generate practical tools, such as the system curve and the Moody chart that can be used for designing piping systems, and calculating pump sizes and pressure requirements. (C) 2018 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:1490 / 1500
页数:11
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