The production curve for agglutinates in planetary regoliths.

Details The production curve for agglutinates in planetary regoliths. The production curve for agglutinates in planetary regoliths.

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983jgr....88..193m&link_type=abstract

Journal of Geophysical Research, Vol. 88, Suppl., p. B193 - B199

Physics

15

Moon Soil:Evolution, Planetary Surfaces:Evolution

Scientific paper

Models for the production of agglutinates are developed that can be applied to the lunar surface or to any planetary or asteroidal body lacking an atmosphere. Models are developed using rate equations for progressively more complex situations and range from Model 1, which is a simple linear increase of agglutinate content with time, to Model 4, which includes provision for recycling of existing agglutinates and replenishment and burial of exposed soil. The models predict that agglutinates should be low in abundance in areas of thin regolith, such as the Lunokhod-2 site on the moon, and on asteroids. The models may also help explain the apparent low agglutinate abundances of lunar regolith breccias and meteorite regolith breccias.

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