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Measurements of Charging of Apollo 17 Lunar Dust Grains by Electron Impact
Author(s) -
M. M. Abbas,
D. Tankosić,
James F. Spann,
Michael J. Dube,
Jessica A. Gaskin,
Mohamed S. ElGenk
Publication year - 2008
Publication title -
aip conference proceedings
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.177
H-Index - 75
eISSN - 1551-7616
pISSN - 0094-243X
DOI - 10.1063/1.2845061
Subject(s) - levitation , astrobiology , cosmic dust , secondary emission , interplanetary dust cloud , photoelectric effect , electron , dusty plasma , materials science , environmental science , physics , solar system , optoelectronics , quantum mechanics , magnet
It is well known since the Apollo missions that the lunar surface is covered with a thick layer of micron size dust grains with unusually high adhesive characteristics. The dust grains levitated and transported on the lunar surface are believed to have a hazardous impact on the robotic and human missions to the Moon. The observed dust phenomena are attributed to the lunar dust being charged positively during the day by UV photoelectric emissions, and negatively during the night by the solar wind electrons. The current dust charging and the levitation models, however, do not fully explain the observed phenomena, with the uncertainty of dust charging processes and the equilibrium potentials of the individual dust grains. It is well recognized that the charging properties of individual dust grains are substantially different from those determined from measurements made on bulk materials that are currently available. An experimental facility has been developed in the Dusty Plasma Laboratory at MSFC for invest...

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