Due to the prevalence of Martian dust devils and dust storms, an understand
ing of the underlying physics of electrical discharges in Martian dust is c
ritical to future Mars exploratory missions. Measurements on the charging o
f single dust grains show that particles of Martian regolith simulant can h
ave large electric potentials due to triboelectric charging. As a result of
this charging, agitated Martian regolith simulant in a low-pressure CO2 at
mosphere produces electrical discharges. Under extremely dark viewing condi
tions, electrical discharges are visually observed at pressures between 0.1
and 50 torr, Measurements of the frequency and intensity of these discharg
es as a function of pressure (from 0.1 to 5 torr) and stirring speed (corre
sponding to wind speeds from 0.1 to 2.6 m/s) show that discharges occur at
pressures and wind speeds similar to those expected on the Martian surface.