Microcrater populations on Apollo 17 rocks

Details Microcrater populations on Apollo 17 rocks Microcrater populations on Apollo 17 rocks

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974icar...22..459s&link_type=abstract

Icarus, vol. 22, Aug. 1974, p. 459-473.

Physics

6

Lunar Craters, Lunar Rocks, Meteorite Craters, Micrometeoroids, Abundance, Apollo 17 Flight, Frequency Distribution, Lunar Surface, Surface Properties, Tables (Data)

Scientific paper

Approximately 6000 microcraters were investigated using binocular microscope techniques on Apollo 17 rocks 70215, 72215, 72235, 72395, 72435, 73216, 73218, 73275, 74275, 76135, 76136, and 79155. The crater populations observed have identical characteristics to those obtained from previous missions. Special emphasis was placed on assessing the influence of target properties on the observable crater populations. Although these properties cannot be quantitatively evaluated at present, the empirical results indicate that crater populations on glass, breccia, and crystalline rock surfaces may differ fundamentally. As a consequence, lunar surface exposure ages of individual rocks based on micrometeoroid craters may be subject to criticism.

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