Depositional history of Luna 24 drill core soil samples

Details Depositional history of Luna 24 drill core soil samples Depositional history of Luna 24 drill core soil samples

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979e%26psl..44..325g&link_type=abstract

Earth and Planetary Science Letters, vol. 44, no. 2, Aug. 1979, p. 325-334.

Computer Science

2

Core Sampling, Deposition, Lunar Soil, Lunik Lunar Probes, Particle Tracks, Rare Gases, Abundance, Argon Isotopes, Chemical Composition, Lunar Evolution, Lunar Geology, Lunar Surface, Neon Isotopes, Particle Density (Concentration), X Ray Analysis, Luna 24, Core-Tube Samples, Soils, Particle Tracks, Rare Gases, Composition, Regolith, Concentrations, Data, Depositional History, Craters, Lunar, Irradiation, Cratering, Samples, Experiments, Crisium, Mare, Analysis, Spallation, Neon, Petrology, Grain Size, Isot

Scientific paper

Six soil samples from various depths of the Luna 24 drill core column have been analyzed for their particle track records and light noble gas compositions. The observed particle track records indicate a higher degree of maturity for the upper zone (about 1 m) of this regolith column as compared with the soils in the lower zone (about 0.4 m). The cosmogenic Ne-21 concentrations decrease rapidly with depth to 1 m, after which the concentrations level off or increase slightly. These data suggest a multistage depositional history for this drill core soil column consisting of: (1) rapid deposition of regolith material, (2) a cratering event about 400 m.y.B.P., leading to excavation to a depth of about 1 m from the present regolith surface, (3) a relatively rapid fill up of the crater with near-surface irradiated material, and (4) in situ irradiation during the last 250-300 m.y. Such a depositional sequence can also explain the observed lack of correlation between different surface exposure-correlated maturity indices in these drill core soil samples.

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