An Impact Event on the Lunar Surface at ~3.3 Ga Inferred From 40Ar/39Ar Thermochronometry of Multiple Samples in Apollo 16 Soil 63503

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1040 Radiogenic Isotope Geochemistry, 1140 Thermochronology, 1160 Planetary And Lunar Geochronology, 6055 Surfaces

Scientific paper

High-Resolution 40Ar/39Ar thermochronometry conducted on 8 separate whole-rock samples including shocked anorthosites, anorthositic impact melts, and fragmented breccias from Apollo 16 soil 63503 reveals an apparently short-duration thermal disturbance at ~3.3 Ga. Using feedback-controlled laser heating, we quantified the Ar diffusion kinetics and spatial distribution of radiogenic 40Ar (primarily contained in plagioclase) for each rock. Five of the samples show clear evidence for a partial resetting event in the K-Ar system at ~3.3 ± 0.1 Ga, despite two of them having 40Ar/39Ar "plateau" ages of ~3.9 Ga, and 3 having ages of ~4.2 Ga. Assuming that the observed Ar diffusion kinetics applies over all time, we constrained a time-temperature (t-T) pair required to diffusively perturb each of the 40Ar distributions at 3.3 Ga and result in the observed 40Ar/39Ar age spectra today. For each sample, this calculation quantified the non-dimensional parameter Dt/a2, with an estimated uncertainty. With each sample's Ar diffusion kinetics, the value of Dt/a2 corresponds to a non- unique family of t-T pairs (shown as continuous curves in t versus T); each pair would result in equivalent diffusive disturbance of the 40Ar spatial distribution at 3.3 Ga. Assuming there exists a best- fit solution for all 8 samples (i.e., that all samples experienced a common thermal event at 3.3 Ga), we constrain the unique t-T solution by minimizing the differences between each. We find that an instantaneous increase in temperature from ambient lunar near-surface conditions to ~530 °C for ~2.5 hours at 3.3 Ga would best explain the entire dataset, although longer durations (~days) spent cooling down to lower temperatures are permissible within the data uncertainty. The dataset also excludes the possibility of significant thermal disturbances after 3.3 Ga. We interpret the best-fit solution to represent the mean thermal state of the rocks during an impact event at ~3.3 Ga. This event may have helped mix separate ejecta units in the Cayley Plains and resulted in an admixture of both ~3.9 Ga and ~4.2 Ga aged rocks in lunar soil 63503.

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