A team at NASA’s Kennedy Space Center in Florida assesses the Dust Concentration Monitor and the Millimeter Wave Doppler Radar inside a regolith bin at the Granular Mechanics and Regolith Operations (GMRO) lab at the spaceport’s Swamp Works on July 28, 2022, as part of Plume Surface Interaction (PSI) Instrumentation testing. The PSI Project is advancing both modeling and testing capabilities to understand exactly how rocket exhaust plumes affect a planetary landing site. This advanced modeling will help engineers evaluate the risks of various plumes on planetary surfaces, which will help them more accurately design landers for particular locations.

The Dust Concentration Monitor and the Millimeter Wave Doppler Radar undergo testing inside a regolith bin at the Granular Mechanics and Regolith Operations (GMRO) lab at the Kennedy Space Center’s Swamp Works on July 28, 2022, as part of Plume Surface Interaction (PSI) Instrumentation testing. The PSI Project is advancing both modeling and testing capabilities to understand exactly how rocket exhaust plumes affect a planetary landing site. This advanced modeling will help engineers evaluate the risks of various plumes on planetary surfaces, which will help them more accurately design landers for particular locations.

A team at NASA’s Kennedy Space Center in Florida assesses the Dust Concentration Monitor and the Millimeter Wave Doppler Radar inside a regolith bin at the Granular Mechanics and Regolith Operations (GMRO) lab at the spaceport’s Swamp Works on July 28, 2022, as part of Plume Surface Interaction (PSI) Instrumentation testing. The PSI Project is advancing both modeling and testing capabilities to understand exactly how rocket exhaust plumes affect a planetary landing site. This advanced modeling will help engineers evaluate the risks of various plumes on planetary surfaces, which will help them more accurately design landers for particular locations.

The Dust Concentration Monitor and the Millimeter Wave Doppler Radar undergo testing inside a regolith bin at the Granular Mechanics and Regolith Operations (GMRO) lab at the Kennedy Space Center’s Swamp Works on July 28, 2022, as part of Plume Surface Interaction (PSI) Instrumentation testing. The PSI Project is advancing both modeling and testing capabilities to understand exactly how rocket exhaust plumes affect a planetary landing site. This advanced modeling will help engineers evaluate the risks of various plumes on planetary surfaces, which will help them more accurately design landers for particular locations.

A team at NASA’s Kennedy Space Center in Florida assesses the Dust Concentration Monitor and the Millimeter Wave Doppler Radar inside a regolith bin at the Granular Mechanics and Regolith Operations (GMRO) lab at the spaceport’s Swamp Works on July 28, 2022, as part of Plume Surface Interaction (PSI) Instrumentation testing. The PSI Project is advancing both modeling and testing capabilities to understand exactly how rocket exhaust plumes affect a planetary landing site. This advanced modeling will help engineers evaluate the risks of various plumes on planetary surfaces, which will help them more accurately design landers for particular locations.

A team at NASA’s Kennedy Space Center in Florida assesses the Dust Concentration Monitor and the Millimeter Wave Doppler Radar inside a regolith bin at the Granular Mechanics and Regolith Operations (GMRO) lab at the spaceport’s Swamp Works on July 28, 2022, as part of Plume Surface Interaction (PSI) Instrumentation testing. The PSI Project is advancing both modeling and testing capabilities to understand exactly how rocket exhaust plumes affect a planetary landing site. This advanced modeling will help engineers evaluate the risks of various plumes on planetary surfaces, which will help them more accurately design landers for particular locations.

Beverly Kemmerer and Austin Adkins, right, and Austin Langton, perform testing with a Millimeter Wave Doppler Radar at NASA’s Kennedy Space Center’s Granular Mechanics and Regolith Operations Lab on July 16, 2021. The testing at the Florida spaceport is part of a project to identify a suite of instrumentation capable of acquiring a comprehensive set of flight data from a lunar lander. Researchers at NASA will use that data to validate computational models being developed to predict plume surface interaction effects on the Moon.

Austin Langton, a researcher at NASA's Kennedy Space Center in Florida, creates a fine spray of the regolith simulant BP-1, to perform testing with a Millimeter Wave Doppler Radar at the Granular Mechanics and Regolith Operations Lab on July 16, 2021. The testing occurred inside the "Big Bin," an enclosure at Swamp Works that holds 120 tons of regolith simulant. The testing at the Florida spaceport is part of a project to predict plume surface interaction effects on the Moon, with testing happening at Kennedy, and NASA's Marshal Space Flight Center and Glenn Research Center.

Beverly Kemmerer and Austin Adkins perform testing with a Millimeter Wave Doppler Radar at NASA’s Kennedy Space Center’s Granular Mechanics and Regolith Operations Lab on July 16, 2021. The testing at the Florida spaceport is part of a project to identify a suite of instrumentation capable of acquiring a comprehensive set of flight data from a lunar lander. Researchers at NASA will use that data to validate computational models being developed to predict plume surface interaction effects on the Moon.