Apollo 14 soils: Size distribution and particle types
D. S. McKay, Grant Heiken, Ruth M. Taylor, U. S. Clanton, D. A. Morrison, G. H. Ladle
Abstract
D. S. McKay, Grant Heiken, Ruth M. Taylor, U. S. Clanton, D. A. Morrison, G. H. Ladle
Abstract
Particle size characteristics are discussed together with particle types, abundances, variation in the soils, questions of soil maturity, coarse fines, and ropy glasses. It is found that agglutinates are formed primarily by micrometeorite impact into lunar soil. Agglutinates appear to be the major particle type now being formed on the lunar surface. Agglutinate content of a soil increases with particle track densities and with surface exposure time.
OpenAlex reports 60 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
Particle size characteristics are discussed together with particle types, abundances, variation in the soils, questions of soil maturity, coarse fines, and ropy glasses. It is found that agglutinates are formed primarily by micrometeorite impact into lunar soil. Agglutinates appear to be the major particle type now being formed on the lunar surface. Agglutinate content of a soil increases with particle track densities and with surface exposure time.
Key concepts: Soil water, Lunar soil, Particle-size distribution, Particle size, Particle (ecology), Maturity (psychological), Soil science, Environmental science