Apollo 14 soils - Size distribution and particle types.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.
Document ID
19730034938
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Mckay, D. S.
Heiken, G. H.
Taylor, R. M.
Clanton, U. S.
Morrison, D. A. (NASA Manned Spacecraft Center Planetary and Earth Sciences Div., Houston, Tex., United States)
Ladle, G. H. (Lockheed Electronics Co., Inc. Houston, Tex., United States)