Thermo-Optical Properties of Lunar Dust SimulantsLunar dust coverage can significantly impact the thermo-optical properties of external surfaces for spacecraft and systems operating in the Lunar orbit or on the Lunar surface. This impacts the thermal control of these vehicles. Testing must be done to determine how much surface optics are affected by varying levels of lunar dust coverage. Optics and Particle Size Distributions (PSDs) of the dust simulant used in these tests are critical to the results. Many lunar dust simulants are available for testing, but their thermooptical properties are not well characterized. To resolve this unknown, 13 different lunar dust simulants’ IR emissivity and solar absorptivity were measured and are presented with their PSDs here.
Document ID
20230003042
Acquisition Source
Johnson Space Center
Document Type
Poster
Authors
Abigail A. Zinecker (Johnson Space Center Houston, Texas, United States)
Brittany H. Spivey (Jacobs (United States) Dallas, Texas, United States)
Date Acquired
March 7, 2023
Subject Category
Lunar and Planetary Science and ExplorationAeronautics (General)Optics
Meeting Information
Meeting: 54th Lunar and Planetary Science Conference (LPSC)
Location: The Woodlands, TX
Country: US
Start Date: March 13, 2023
End Date: March 17, 2023
Sponsors: Universities Space Research Association, Lunar and Planetary Institute
Funding Number(s)
WBS: 651937.06.03.72.12
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
Single Expert
Keywords
lunar dustsimulantthermal controllunar surfaceemissivityabsorptivityparticle size distributionradiatordust coveragelunar dust simulantmaterial analog