DPS 34th Meeting, October 2002
Session 15. Mars
Poster, Chair(s): , Tuesday, October 8, 2002, 3:30-6:00pm, Exhibit Hall

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[15.17] Electrical Discharging of Dust near the Surface of Mars

C.E. Krauss, M. Horanyi (LASP, Univ. of Colorado), S. Robertson (Dept. of Physics, Univ. of Colorado)

Due to the prevalence of Martian dust devils and dust storms, an understanding of the underlying physics of electrical discharges in Martian dust is critical to future Mars exploratory missions. When dust particles come into contact, charge can be transferred between the grains. Wind driven dust studies (Weather, 1969) show that in the case of particles with identical compositions, the particle with the larger radius in a collision preferentially becomes positively charged. The stratification of particle sizes generated by upwinds within a dust cloud causes an electric dipole to form. When the electric potential within the cloud exceeds the breakdown voltage of the surrounding atmosphere, a discharge occurs.

Mars' low atmospheric pressure and arid, windy environment suggest that the dust near the surface of Mars is even more susceptible to triboelectric charging than terrestrial dust. Electrical discharges on Mars should occur more frequently but at lower intensities than those seen on Earth.

We have conducted laboratory experiments to examine the creation of discharges due to vertical charge separation in a simulated Martian environment. The range of pressures and the amount of mass loading required to produce these discharges have been examined. 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. When JSC-Mars-1 is vertically dropped in a low-pressure CO2 atmosphere, electrical discharges are both visually and electronically detected. Measurements of the frequency and intensity of these discharges show that they can occur under conditions expected on the Martian surface.

This work is supported by NASA Space Science GSRP, NGT5-50345.

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Bulletin of the American Astronomical Society, 34, #3< br> © 2002. The American Astronomical Soceity.