间接和直接聚光加热月球土壤的烧结行为

Diprajit Biswas, Thomas C. Cox, J. Lapp
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引用次数: 1

摘要

建筑材料是在月球上长期居住的一项重要需求。当太阳辐射以高热流集中时,可以加热月球土壤或风化层,直到它在900°C以上的温度下烧结。固体烧结的风化层可用作建筑材料。本文从直接辐照烧结和间接烧结两方面探讨了导致月壤有效烧结的条件。利用不同热流强度的氙弧灯聚光烧结月球土壤模拟物。记录了烧结深度、烧结量和烧结材料的抗压强度。烧结范围为860℃~ 1140℃。有限抗压强度数据表明间接烧结强度更高。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Sintering Behavior of Lunar Soil Heated by Indirect and Direct Concentrated Sunlight
Construction material is one important need for long-term habitation on the moon. Solar radiation, when concentrated for high heat flux, can heat lunar soil, or regolith, until it sinters at temperatures above 900°C. The solid, sintered regolith can be used for construction material. This work explores the conditions which lead to effective sintering of lunar soil for both directly irradiated sintering and indirect sintering. Lunar soil simulants were sintered using concentrated light from a xenon-arc lamp with varying heat flux intensity. The resulting depth of sintering, amount of material sintered, and the compressive strength of the sintered material were recorded. A sintering range of 860°C–1140°C was identified. Limited compressive strength data showed higher strength for indirect sintering.
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