Electrostatic Discharging of Dust near the Surface of Mars
C. E. Krauss, M. Horányi, Scott Robertson
Abstract
C. E. Krauss, M. Horányi, Scott Robertson
Abstract
Due to the prevalence of Martian dust devils and dust storms, an understanding of the physics of electrical discharges in Martian dust is critical to future Mars exploratory missions. Measurements done in our lab on the charging of single dust grains show that particles of JSC‐Mars‐1, a Martian regolith simulant, can have large electrical potentials due to triboelectric charging. We have conducted experiments to determine the range of pressures and wind speeds over which discharges can be observed in a low‐pressure CO2 atmosphere. We have also examined the affects of particle‐size distribution on the observed discharge rates.
A significance statement is not available in the OpenAlex record.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
Due to the prevalence of Martian dust devils and dust storms, an understanding of the physics of electrical discharges in Martian dust is critical to future Mars exploratory missions. Measurements done in our lab on the charging of single dust grains show that particles of JSC‐Mars‐1, a Martian regolith simulant, can have large electrical potentials due to triboelectric charging. We have conducted experiments to determine the range of pressures and wind speeds over which discharges can be observed in a low‐pressure CO2 atmosphere. We have also examined the affects of particle‐size distribution on the observed discharge rates.
Key concepts: Mars Exploration Program, Atmosphere of Mars, Martian, Dust storm, Astrobiology, Triboelectric effect, Regolith, Environmental science