AI Article Synopsis
- Protecting mechanical parts from dust is essential for Moon and Mars missions; this study analyzes how lunar and Martian regolith affects abrasion using specific tests.
- Results showed friction coefficients stabilized between 0.2 and 0.4 across all simulants, with Martian regolith causing less abrasion than lunar regolith.
- The abrasion mechanism involved micro-ploughing and micro-cutting, resulting in different wear patterns on the materials tested.
Article Abstract
For space missions to either the Moon or Mars, protecting mechanical moving parts from the abrasive effects of prevailing surface dust is crucial. This paper compares the abrasive effects of two lunar and two Martian simulant regoliths using special pin-on-disc tests on a stainless steel/polytetrafluoroethylene (PTFE) sealing material pair. Due to the regolith particles entering the contact zone, a three-body abrasion mechanism took place. We found that friction coefficients stabilised between 0.2 and 0.4 for all simulants. Wear curves, surface roughness measurements, and microscopic images all suggest a significantly lower abrasion effect of the Martian regoliths than that of the lunar ones. It applies not only to steel surfaces but also to the PTFE pins. The dominant abrasive micro-mechanism of the disc surface is micro-ploughing in the case of all tests, while the transformation of the counterface is mixed. The surface of pin material is plastically transformed through micro-ploughing, while the material is removed through micro-cutting due to the slide over hard soil particles.
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|---|---|
| http://www.ncbi.nlm.nih.gov/pmc/articles/PMC11396534 | PMC |
| http://dx.doi.org/10.3390/ma17174240 | DOI Listing |
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