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| Main Authors: | , , , , , |
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| Format: | Preprint |
| Published: |
2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2504.06944 |
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| _version_ | 1866916681383673856 |
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| author | Dotson, B. John, A. St. Hall, R. Sapkota, D. Britt, D. Metzger, P. |
| author_facet | Dotson, B. John, A. St. Hall, R. Sapkota, D. Britt, D. Metzger, P. |
| contents | With humans returning to the Moon under the Artemis program, understanding and mitigating effects from Plume Surface Interactions (PSI) will be essential for the protection of personnel and equipment on the Moon. To help characterize the underlying mechanics associated with viscous erosion and crater formation, experimental measurements using regolith simulants and subsonic, non-reacting flows were completed using compressed air in a splitter plate, plume cratering setup. More specifically, these investigations examined the underlying effects of bulk density, cohesion, and exhaust flow characteristics on viscous erosion rates and crater formation using Lunar highlands simulant (LHS-1), Lunar mare simulant (LMS-1), LHS-1D (Dust) simulants, and 40-80 um glass beads in atmosphere. Results show that particle size distribution can ultimately influence crater shapes and erosion rates, likely owing to internal angle of friction. Measurements show that increasing bulk density, especially from an uncompacted to a slightly compacted state, decreases erosion rate by as much as 50%. While cohesion of granular material can mitigate erosion rates to some extent, higher levels of cohesion above 1,000 Pa may actually increase viscous erosion rates due to particle clumping. A modified version of Metzger's (2024a) equation for volumetric erosion rate is presented, with limitations discussed. These modified equations for viscous erosion, with limitations noted, show that geotechnical properties play an important role in viscous erosion and should be considered in PSI computer models for future mission planning. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2504_06944 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Understanding The Effects of Geotechnical Properties on Viscous Erosion Rate from Plume Surface Interactions Dotson, B. John, A. St. Hall, R. Sapkota, D. Britt, D. Metzger, P. Space Physics With humans returning to the Moon under the Artemis program, understanding and mitigating effects from Plume Surface Interactions (PSI) will be essential for the protection of personnel and equipment on the Moon. To help characterize the underlying mechanics associated with viscous erosion and crater formation, experimental measurements using regolith simulants and subsonic, non-reacting flows were completed using compressed air in a splitter plate, plume cratering setup. More specifically, these investigations examined the underlying effects of bulk density, cohesion, and exhaust flow characteristics on viscous erosion rates and crater formation using Lunar highlands simulant (LHS-1), Lunar mare simulant (LMS-1), LHS-1D (Dust) simulants, and 40-80 um glass beads in atmosphere. Results show that particle size distribution can ultimately influence crater shapes and erosion rates, likely owing to internal angle of friction. Measurements show that increasing bulk density, especially from an uncompacted to a slightly compacted state, decreases erosion rate by as much as 50%. While cohesion of granular material can mitigate erosion rates to some extent, higher levels of cohesion above 1,000 Pa may actually increase viscous erosion rates due to particle clumping. A modified version of Metzger's (2024a) equation for volumetric erosion rate is presented, with limitations discussed. These modified equations for viscous erosion, with limitations noted, show that geotechnical properties play an important role in viscous erosion and should be considered in PSI computer models for future mission planning. |
| title | Understanding The Effects of Geotechnical Properties on Viscous Erosion Rate from Plume Surface Interactions |
| topic | Space Physics |
| url | https://arxiv.org/abs/2504.06944 |