Preparation and evaluation of geopolymer based on BH-2 lunar regolith simulant under lunar surface temperature and vacuum condition

被引:72
作者
Zhou, Siqi [1 ]
Yang, Zhanning [1 ]
Zhang, Rongrong [1 ]
Zhu, Xingyi [2 ]
Li, Feng [1 ]
机构
[1] Beihang Univ, Sch Transportat Sci & Engn, Beijing 100191, Peoples R China
[2] Tongji Univ, Key Lab Rd & Traff Engn, Minist Educ, Shanghai 200092, Peoples R China
基金
中国国家自然科学基金;
关键词
Moon; Lunar base; Geopolymer; Lunar regolith simulant; Lunar temperature; SOIL;
D O I
10.1016/j.actaastro.2021.08.039
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The construction of a lunar base and habitation on the moon has always been of great significance to utilizing lunar resources and deep space exploration. In this paper, a new type of lunar regolith simulant denoted as BH-2 of similar compositions and particle size distribution with real one was developed and used for geopolymer synthesis under simulated lunar surface temperature and vacuum conditions. The geopolymer products were characterized by compressive strength test, Mercury Intrusion Porosimetry (MIP), Scanning Electron Microscope coupled, and Si-29 magic angle spinning-nuclear magnetic resonance (Si-29 MAS-NMR). The results showed that BH-2 lunar regolith simulant could be used to synthesize geopolymer. And the 72-h compressive strength of the geopolymer cured at the temperature of group C, corresponding to the 324-384 h of one lunar day, could reach 38.2 MPa, which was advantageous in the early stages of lunar construction because no additional curing equipment is required. The pores originated from lunar regolith simulant and caused by incomplete geo-polymerization resulted in decreased compressive strength of the resulting geopolymer. Vacuum conditions on the moon favored the preparation of lunar geopolymers due to the lack of carbon dioxide weakening the efflorescence effect. This study benefits to lunar base construction with in-situ resource.
引用
收藏
页码:90 / 98
页数:9
相关论文
共 37 条
[1]   Geopolymers from lunar and Martian soil simulants [J].
Alexiadis, Alessio ;
Alberini, Federico ;
Meyer, Marit E. .
ADVANCES IN SPACE RESEARCH, 2017, 59 (01) :490-495
[2]   Partial replacement of low reactive volcanic ash by cassava peel ash in the synthesis of volcanic ash based geopolymer [J].
Baenla, J. ;
Mbah, J. B. Bike ;
Li Ndjock, I. B. Djon ;
Elimbi, A. .
CONSTRUCTION AND BUILDING MATERIALS, 2019, 227
[3]   Phase-dependent space weathering effects and spectroscopic identification of retained helium in a lunar soil grain [J].
Burgess, K. D. ;
Stroud, R. M. .
GEOCHIMICA ET COSMOCHIMICA ACTA, 2018, 224 :64-79
[4]   Building components for an outpost on the Lunar soil by means of a novel 3D printing technology [J].
Cesaretti, Giovanni ;
Dini, Enrico ;
De Kestelier, Xavier ;
Colla, Valentina ;
Pambaguian, Laurent .
ACTA ASTRONAUTICA, 2014, 93 :430-450
[5]  
David Carrier W., 1968, J GEOTECH GEOENVIRON, V16, P956
[6]   GEOPOLYMERS - INORGANIC POLYMERIC NEW MATERIALS [J].
DAVIDOVITS, J .
JOURNAL OF THERMAL ANALYSIS, 1991, 37 (08) :1633-1656
[7]   Preparation of lunar regolith based geopolymer cement under heat and vacuum [J].
Davis, Gabrielle ;
Montes, Carlos ;
Eklund, Sven .
ADVANCES IN SPACE RESEARCH, 2017, 59 (07) :1872-1885
[8]   Evidence for water ice near the lunar poles [J].
Feldman, WC ;
Maurice, S ;
Lawrence, DJ ;
Little, RC ;
Lawson, SL ;
Gasnault, O ;
Wiens, RC ;
Barraclough, BL ;
Elphic, RC ;
Prettyman, TH ;
Steinberg, JT ;
Binder, AB .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 2001, 106 (E10) :23231-23251
[9]  
Gonzalez CP, 2012, IRAN STUD SER-LEIDEN, P1
[10]  
Hamideh M., 2018, RHEOLOGY ACTIVATED P, V113