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Lunar dust can affect the lunar rover's operation and endanger astronauts' health. Therefore, it is necessary to efficiently detect lunar dust particles' motion characteristics and cumulative distribution. We use the multi-physical field simulation software to simulate the multi-ring bias lunar dust detector. The motion and cumulative distribution of lunar dust less than 2 μm were calculated and analyzed by the simulation model established by COMSOL. The cumulative distribution of 2 μm lunar dust particles on the annular electrode is studied experimentally. The simulation results show that when the inner ring bias is + 30 V and the other ring bias is − 50 V, the dust collection efficiency of the 6-ring detector for 400 simulated dust with an initial velocity of 0.4 m/s below 2 μm is 98.75%, and the particle distribution is the most in the 4th ring. The 12-ring electrode structure with the same bias setting can achieve about 100% collection of the same charged dust, and the most particle distribution is the 10th ring. The experimental results show that the dust collected by the 6-ring electrode accounts for about 88.27% of the total, and the dust collected by the 12-ring electrode accounts for approximately 96.63% of the total. The distribution characteristics are similar to the simulation results. The results show that the 12-ring bias lunar dust detector can achieve higher collection rate detection corresponding to the lunar dust particles below 2 μm, accounting for 95%. However, as the charge–mass ratio of lunar dust decreases, the collection efficiency of the detector will gradually decrease.
International Journal of Aeronautical and Space Sciences – Springer Journals
Published: May 5, 2023
Keywords: Lunar dust; Bias detector; Multi-ring electrode; Collecting efficiency; Multiphysics simulation; Lunar exploration
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