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Investigating Particle-Particle Electrostatic Effects on Charged Lunar Dust Transport via Discrete Element ModelingNASA surface exploration missions have always seen negative effects of dust including the Apollo missions. The astronaut-witnessed unusual behavior of the dust particles that surround the vehicle after engine cutoff has the potential to have more of an influence on surface systems dust loading than the high velocity lunar rocket plume ejecta in the landing process. The levitation and transport of the fine components of regolith on lunar surface has been linked to electrostatic effects and electric field, but so far there is no accurate model considering the inter-particle electrostatic interactions, especially when the particles are charged by rocket plume or other mechanical interactions due to exploration activities. This study is proposed to investigate the dynamics of charged lunar regolith with a discrete element method (DEM) approach focusing on the inter-particle interactions and contact charge transfer. The grain dynamics is coupled with mechanical and electrical particle interactions, and both short- and long-range interactions between spherical particles are incorporated. A tribo-charging model based on instantaneous collisions between particles is adopted and validated by comparing the simulation results to existing experimental data. Sensitivity analysis is conducted to quantify the effects of initial charge, tribo-charging, and E-field on transport of lunar dust based on JSC-1 simulants with a radius of 50 lm. DEM simulations are also conducted in a near realistic lunar environment with the estimations of initial conditions that shows the difference in position and velocity distributions between charged particles and uncharged particles. The results indicate that the charged dust particles have higher dispersion of position and velocity by several orders of magnitude due to electrostatic effects. This provides a potential explanation for the phenomena of the approximately 30 s dust lofting following Apollo Lunar Module landing.
Document ID
20230005914
Acquisition Source
Kennedy Space Center
Document Type
Reprint (Version printed in journal)
Authors
Hao Wang
(University of Central Florida Orlando, Florida, United States)
James R. Phillips III
(Kennedy Space Center Merritt Island, Florida, United States)
Adrienne R. Dove
(University of Central Florida Orlando, Florida, United States)
Tarek A. Elgohary
(University of Central Florida Orlando, Florida, United States)
Date Acquired
April 17, 2023
Publication Date
September 6, 2022
Publication Information
Publication: Advances in Space Research
Publisher: Elsevier
Volume: 70
Issue: 10
Issue Publication Date: November 15, 2022
ISSN: 0273-1177
URL: https://www.sciencedirect.com/science/article/pii/S027311772200816X
Subject Category
Physics (General)
Space Sciences (General)
Funding Number(s)
WBS: 295670.01.20.76.06
WBS: 950152.04.10.19.76
CONTRACT_GRANT: 80NSSC20P0391
CONTRACT_GRANT: NNX13AJ45A
CONTRACT_GRANT: 80NSSC19M0214
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
Keywords
Lunar dust
Discrete element method
Planetary science
Aerospace
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