Through the Artemis Program, NASA will send the first astronauts to the Moon since the Apollo Era before 2030. They will be joined by multiple space agencies, like the ESA and China, who plan to send astronauts (and “taikonauts”) there for the first time. Beyond this, all plan to build permanent habitats in the South Pole-Aitken Basin and the necessary infrastructure that will lead to a permanent human presence. This presents many challenges, the most notable being those arising from the nature of the lunar environment.
Aside from the extremes in temperature, a 14-day diurnal cycle, and the airless environment, there’s the issue of lunar regolith (aka moondust). In addition to being coarse and jagged, lunar regolith sticks to everything because it is electrostatically charged. Because of how this dust plays havoc with astronaut health, equipment, and machinery, NASA is developing technologies to mitigate dust buildup. Seven of these experiments will be tested during a flight test using a Blue Origin New Shepard rocket to evaluate their ability to mitigate lunar dust.
Another major problem with lunar regolith is how it gets kicked up and distributed by spacecraft plumes. With essentially no atmosphere and lower gravity (16.5% of Earth’s), this dust can remain aloft for extended periods of time. Its jagged nature, resulting from billions of years of meteor and micrometeoroid impacts and a total lack of weathering, is abrasive to any surface it comes into contact with, ranging from spacesuits and equipment to human skin, eyes, and lungs. It will also build up on solar panels, preventing missions from drawing enough power to survive a lunar night.
In addition, it can also cause equipment to overheat as it coats thermal radiators and accumulates on windows, camera lenses, and visors, making it harder to see, navigate, and acquire accurate images. Kristen John, the Lunar Surface Innovation Initiative technical integration lead at NASA’s Johnson Space Center, said in a NASA press release: “The fine grain nature of dust contains particles that are smaller than the human eye can see, which can make a contaminated surface appear to look clean.”
Addressing the Problem
These technologies were developed by NASA’s Game Changing Development program within the agency’s Space Technology Mission Directorate (STMD). The “Lunar Gravity Simulation via Suborbital Rocket” flight test will study regolith mechanics and lunar dust transport in a simulated lunar gravity environment. The payload includes projects for mitigating and cleaning dust using multiple strategies. They include:
ClothBot:
This compact robot is designed to simulate and measure how dust behaves in a pressurized environment, which astronauts could bring back after conducting Extravehicular Activities (EVAs). The robot relies on pre-programmed motions that simulate astronauts’ movements when removing their spacesuits (aka “doffing”), releasing a small dose of lunar regolith simulant. A laser-illuminated imaging system will then capture the dust flow in real-time while sensors record the size and number of particles.
Electrostatic Dust Lofting (EDL):
The EDL will examine how lunar dust is “lofted” (kicked up) when it becomes electrostatically charged to improve models on dust lofting. During the lunar gravity phase of the flight, a dust sample will be released that the EDL will illuminate using a UV light source, causing the particles to become charged. The dust will then pass through a sheet laser as it rises from the surface while the EDL observes and records the results. The EDL’s camera will continue to record the dust until the mission ends, even after the lunar gravity phase ends and the UV light is shut off.
Hermes Lunar-G:
The Hermes Lunar-G project, developed by NASA, Texas A&M, and Texas Space Technology Applications and Research (T-STAR), is based on a facility (Hermes) that previously operated on the International Space Station (ISS). Like its predecessor, the Lunar-G project will rely on repurposed Hermes hardware to study lunar regolith simulants. This will be done using four canisters containing compressed lunar dust simulants. When the flight enters its lunar gravity phase, these simulants will decompress and float around in the canisters while high-speed cameras and sensors capture data. The results will be compared to microgravity data from the ISS and similar flight experiments.
The data obtained by these projects will provide information on regolith generation rates, transport, and mechanics that will help scientists refine computational models. This will allow mission planners and designers to develop better strategies for dust mitigation for future missions to the Moon and Mars. Already, this challenge informs several aspects of NASA’s technological developments, ranging from In-Situ Resource Utilization (ISRU) and construction to transportation and surface power. Said John:
“Learning some of the fundamental properties of how lunar dust behaves and how lunar dust impacts systems has implications far beyond dust mitigation and environments. Advancing our understanding of the behavior of lunar dust and advancing our dust mitigation technologies benefits most capabilities planned for use on the lunar surface.”
The test flight and vehicle enhancements that will enable the simulation of lunar gravity are being funded through NASA’s Flight Opportunities program.
Further Reading: NASA