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These dust devils are frequently observed using visible cameras onboard landers or rovers.
These dust detectors are time-of-flight mass spectrometers which analyse the plasma generated upon hypervelocity impacts.
These dust grains could affect the optical quality of the lunar environment for astronomical observations and interfere with exploration activities.
A significant fraction of these dust particles may capture free electrons from the ambient medium and get charged negatively.
The optical depth of these dust trails are 10−9 to 10−8, which is consistent with IRAS measurements.
These dust streams, which were first discovered in 1992, flow out about 175 million miles, or nearly twice the distance of the Earth to the sun.
These dust materials are characterised by a bi-modal particle size distribution, one mode in the clay and another in the coarse-medium silt.
Although the extraction of information from each type of archive is slightly different, the basic controls on these dust indicators are the same.
The characteristics of these dust populations are of scientific interest and engineering importance for the design of future equipment to operate on the lunar surface.
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When Earth's path around the Sun intersects one of these dust-populated orbits, a meteor shower occurs.
They were scattered all over the city, these dust-baked cars, remnants of a civilisation so fantastic that it was hard to believe it really existed, that it wasn't just a dream.
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