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Investigating the Resilience of Ceramic Coatings for Lunar EnvironmentsAs the number of missions to land on the Moon with and without crew continues to increase, there are a plethora of factors to consider that could affect aerospace structures. Lunar dust, or lunar regolith, composed of small rock fragments, glass beads, and minerals, is transformed by years of meteorite impacts. Lunar dust is quite corrosive, abrasive, reactive and adherent, necessitating effective mitigation strategies. Ceramics have emerged as a promising material selection in the aerospace industry for structural protection due to their high strength, excellent thermal properties, and resistance to degradation. Among these ceramics, zirconia (ZrO2) is a promising material, exhibiting exceptional mechanical and thermal properties. This study evaluates the resilience of an 8-wt.% yttria-stabilized zirconia (8YSZ) ceramic coating, tested against wear and erosion to characterize its degradation over time.
Document ID
20240016393
Acquisition Source
Langley Research Center
Document Type
Presentation
Authors
Ashley Tirado Pujols
(Embry–Riddle Aeronautical University Daytona Beach, Florida, United States)
Zachary Stein
(Embry–Riddle Aeronautical University Daytona Beach, Florida, United States)
Seetha Raghavan
(Embry–Riddle Aeronautical University Daytona Beach, Florida, United States)
Christopher Wohl
(Langley Research Center Hampton, United States)
Valerie Wiesner
(Langley Research Center Hampton, United States)
Date Acquired
December 20, 2024
Subject Category
Chemistry and Materials (General)
Meeting Information
Meeting: AIAA SciTech Forum
Location: Orlando, FL
Country: US
Start Date: January 6, 2025
End Date: January 10, 2025
Sponsors: American Institute of Aeronautics and Astronautics
Funding Number(s)
CONTRACT_GRANT: 80NSSC21M0309
WBS: 295670.01.24.23.05
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
NASA Technical Management
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