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Dust Mitigation Technology Roadmap: LSIC Spring 2026As 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. The Exploration Systems Development Mission Directorate (ESDMD) defines and manages systems development for programs critical to NASA’s Artemis program and planning for NASA’s Moon to Mars (M2M) exploration approach. ESDMD manages the human exploration system development for lunar orbital, lunar surface, and Mars exploration.
Document ID
20260001844
Acquisition Source
Johnson Space Center
Document Type
Presentation
Authors
Josh Litofsky
(Johnson Space Center Houston, United States)
Date Acquired
March 2, 2026
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
NASA Peer Committee
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