Permeability of JS']JSC-1A: A lunar soil simulant

被引:28
|
作者
LaMarche, Casey Q. [1 ]
Curtis, Jennifer Sinclair [1 ]
Metzger, Philip T. [2 ]
机构
[1] Univ Florida, Dept Chem Engn, Gainesville, FL 32611 USA
[2] NASA, Granular Mech & Surface Syst Lab, Kennedy Space Ctr, FL 32899 USA
关键词
Moon; surface; Regoliths; Cratering; Ices; GAS-TRANSPORT; POROUS-MEDIA; ICE; SURFACE; MOON; SUBLIMATION; ANTARCTICA; POROSITY; MERCURY; WATER;
D O I
10.1016/j.icarus.2010.12.015
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The permeability of lunar soil simulant, JSC-1A, is measured over a range of bulk densities from 1550 to 2000 kg m(-3). The corresponding viscous flow permeability is 1 x 10(-12) m(2) to 6.1 x 10(-12) m(2) for this bulk density range. Implications of these values on the contamination of regolith by rockets, on barrier/enhancement to bulk flow of ice, and on cratering are discussed. Although the particle size and shape distribution of the JSC-1A are extremely wide, the permeability measurements agree surprisingly well with the Carman-Kozeny equation. The results provide evidence that the Carman-Kozeny model could be applicable to other naturally occurring soils if effective soil properties are considered. (C) 2010 Elsevier Inc. All rights reserved.
引用
收藏
页码:383 / 389
页数:7
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