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Dust Mitigation RoadmapAs humans return to the Moon and set their sites on Mars with spacesuits, rovers, habitats, and other assets during the Artemis missions, the lunar and Martian regolith (i.e. dust) covering the surface will be an environmental and performance challenge to nominal and contingency operations. Accounts from Apollo astronauts and analysis of hardware returned from the surface illustrate just how deleterious the dust can be. During Apollo missions, the lunar dust adhered to the spacesuits mechanically and electrostatically, and the rovers experienced mechanical malfunctions. It is anticipated that during Artemis, with longer and more complicated lunar surface missions, off-nominal effects due to lunar dust contamination will increase exponentially, underscoring the need for dust mitigation technology development and characterization efforts.
Document ID
20250009401
Acquisition Source
Johnson Space Center
Document Type
Extended Abstract
Authors
J H Litofsky
(Johnson Space Center Houston, United States)
Date Acquired
September 19, 2025
Publication Date
April 28, 2026
Publication Information
Publisher: Lunar Surface Innovation Consortium
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: Lunar Surface Innovation Consortium (LSIC) Spring Meeting
Location: Baltimore, MD
Country: US
Start Date: April 28, 2026
End Date: April 30, 2026
Sponsors: Johns Hopkins University Applied Physics Laboratory
Funding Number(s)
WBS: 830724.06.06.04
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
Technical Review
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