W. Han, L. Ding, C. Zhou, Y. Zhou, F. Dang | 2024 | Science China Technological Sciences
DOI 10.1007/s11431-023-2675-0Review state
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This paper investigates the feasibility of laser welding vacuum-sintered HUST-1 lunar regolith simulant (HLRS) for lunar base construction. The study examines microstructure, mineral composition, element distribution, and shear strength of welded joints. Key findings include reduced weld shear strength due to micro-cracks and thermal decomposition gas, with optimal shear strength (15.69 N/cm) achieved at 1000 W laser power. This study investigates the laser welding of sintered lunar regolith samples to simulate potential welding applications on future lunar bases. The sintered samples were produced using a vacuum sintering process at 1050°C for 2 hours, resulting in square column samples with a compressive strength of 145.39 MPa. Laser welding experiments were conducted using a YLR2000 fiber laser with power levels of 400, 600, 800, 1000, and 1200 W under atmospheric conditions. The microstructure, phase transitions, surface cavity depth, and weld shear strength were analyzed. The results show that increasing laser power leads to the formation of surface cracks due to rapid heating and cooling, which induces thermal stress. The study highlights the importance of optimizing laser pa
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Laser welding of vacuum-sintered HUST-1 lunar regolith simulant
Feasibility study
Shear strength testing of welded joint
Mechanical testing
Particle size distribution analysis of HLRS
Material characterization
Chemical composition analysis of HLRS
Material characterization
Weld shear strength testing
Mechanical testing
EDS analysis of granular precipitates
elemental analysis
XRD analysis of SLR
mineral composition
EDS analysis of flocculent and foliaceous materials
elemental analysis
Melting point
1200-1250 C
Particle size distribution
5-35 m
Shear strength
15.69 N/cm
Laser power
400, 600, 800, 1000, 1200 W
Thermal expansion
leads to crack formation
Volatilization of minerals
magnesia-containing minerals vaporize during melting
Precipitation of minerals
Na and Mg-containing minerals
Formation of flocculent particles
high-temperature melting