Flux and composition of micrometeoroids in the diameter range 1-10 microns

Mathematics – Logic

Scientific paper

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Meteorite Craters, Meteoritic Composition, Meteoritic Damage, Meteoroid Concentration, Micrometeoroids, Apollo 15 Flight, Flux Density, Glass, Hypervelocity Impact, Iron Meteorites, Lunar Craters, Lunar Rocks, Morphology, Radiation Pressure, Solar Radiation, Stony Meteorites

Scientific paper

A morphological study of microcraters observed on glassy lunar spherules from the Apollo 15 fines obtained from Spur crater near Hadley Rille and of those created on glassy materials in the laboratory is evaluated. Craters were produced in soda lime and tektite glasses by the bombardment of iron and aluminum microparticles which were electrostatically accelerated using a 2 MV Van de Graaff generator. It was suggested that three material crater groupings result from the impacts of micrometeoroids of distinctly different physical properties. The result indicated that 20% of the total mass of micrometeoroid material is associated with iron micrometeoroids while the remaining 80% is divided between low density stony groups.

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