Ultrasonic Actuation Technology for Particulate Mitigation on Martian Solar Panels

The rapid developments in interplanetary exploration underscore the need for more efficient, self-sustaining energy production while exposing major limitations in current autonomous decontamination technologies. With the recent focus on Martian exploration, there have been six rovers sent to the Red Planet; four of which used solar as a primary energy source, and none of which included reliable decontamination technology. Studies have shown that Martian regolith accumulation on solar panels results in an average power loss of 0.2% per sol, with some missions experiencing even higher rates depending on local conditions [1]. In order to combat these losses and improve the effectiveness of future Mars exploration missions and habitation, this study explores Near-Field Acoustic Levitation (NFAL) as a non-contact dust removal method for solar energy. Experimental tests assessed the effectiveness of placing tempered glass above a solar panel and optimized ultrasonic transducer positioning for efficient dust removal. Using a solar simulator, the glass demonstrated an improved solar power output of up to 9.3 ± 0.1%. Optimization with dust simulants identified an emitter-receiver configuration—emitter at the glass’s bottom—as the most effective, achieving a 95 ± 4% dust mass reduction after 20 seconds of actuation and with an angle of 20° with respect to the ground. Video analysis of the actuation supported these values with a steady state dust coverage reduced to 6 ± 3% of initial coverage. Testing with various dust types to confirm experimental validity showed comparable results. Specifically, MGS-1 particles achieved 94 ± 3% mass removal in terrestrial atmospheric conditions following 120 seconds of actuation. Furthermore, initial tests in low-pressure environments (<0.4 torr ambient pressure) demonstrated effective dust removal. Additional tests will characterize the response at angles below 20º using charged MGS-1 particles. Ultrasonic solar cleaning provides an effective solution to dust accumulation in extraterrestrial applications, an absolute necessity as humans attempt to extend their reach into the cosmos. [1] Lorenz, R. D., Martínez, G. M., Spiga, A., Vicente-Retortillo, A., Newman, C. E., Murdoch, N., Forget, F., Millour, E., and Pierron, T., “Lander and rover histories of dust accumulation on and removal from solar arrays on Mars,” Planetary and Space Science, vol. 207, Nov. 2021, p. 105337. https://doi.org/10.1016/j.pss.2021.105337

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Publication Details

Published
2025-01-01
DOI
https://doi.org/10.2514/6.2025-99554
Primary Topic
Spacecraft Design and Technology
Type
article
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article

Ultrasonic Actuation Technology for Particulate Mitigation on Martian Solar Panels

Matthew Gilpin, W. D. MacDonald, Emily Hesby, Kelly Slosar et al.
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Spacecraft Design and Technology
article

Ultrasonic Actuation Technology for Particulate Mitigation on Martian Solar Panels

Matthew Gilpin, W. D. MacDonald, Emily Hesby, Kelly Slosar, Nicolas Tapies
article en

Abstract

The rapid developments in interplanetary exploration underscore the need for more efficient, self-sustaining energy production while exposing major limitations in current autonomous decontamination technologies. With the recent focus on Martian exploration, there have been six rovers sent to the Red Planet; four of which used solar as a primary energy source, and none of which included reliable decontamination technology. Studies have shown that Martian regolith accumulation on solar panels results in an average power loss of 0.2% per sol, with some missions experiencing even higher rates depending on local conditions [1]. In order to combat these losses and improve the effectiveness of future Mars exploration missions and habitation, this study explores Near-Field Acoustic Levitation (NFAL) as a non-contact dust removal method for solar energy. Experimental tests assessed the effectiveness of placing tempered glass above a solar panel and optimized ultrasonic transducer positioning for efficient dust removal. Using a solar simulator, the glass demonstrated an improved solar power output of up to 9.3 ± 0.1%. Optimization with dust simulants identified an emitter-receiver configuration—emitter at the glass’s bottom—as the most effective, achieving a 95 ± 4% dust mass reduction after 20 seconds of actuation and with an angle of 20° with respect to the ground. Video analysis of the actuation supported these values with a steady state dust coverage reduced to 6 ± 3% of initial coverage. Testing with various dust types to confirm experimental validity showed comparable results. Specifically, MGS-1 particles achieved 94 ± 3% mass removal in terrestrial atmospheric conditions following 120 seconds of actuation. Furthermore, initial tests in low-pressure environments (<0.4 torr ambient pressure) demonstrated effective dust removal. Additional tests will characterize the response at angles below 20º using charged MGS-1 particles. Ultrasonic solar cleaning provides an effective solution to dust accumulation in extraterrestrial applications, an absolute necessity as humans attempt to extend their reach into the cosmos. [1] Lorenz, R. D., Martínez, G. M., Spiga, A., Vicente-Retortillo, A., Newman, C. E., Murdoch, N., Forget, F., Millour, E., and Pierron, T., “Lander and rover histories of dust accumulation on and removal from solar arrays on Mars,” Planetary and Space Science, vol. 207, Nov. 2021, p. 105337. https://doi.org/10.1016/j.pss.2021.105337

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