AI Article Synopsis

  • * An ion microprobe analysis revealed that the majority of analyzed phosphates indicate a U-Pb isochron age of 3.15±0.12 billion years, which aligns with previous dating results from isotopic studies.
  • * The study found no notable age differences between the phosphates in the shock melt vein and the host rock, while presenting evidence of intense shock metamorphism and a rapid cooling rate exceeding 140 K/s.

Article Abstract

Northwest Africa (NWA) 2977 is a lunar basaltic meteorite that was found in 2005 and has been classified as an olivine cumulate gabbro. This meteorite contains a shock melt vein (SMV) induced by an intense shock event. We report herein on an analysis of phosphates in the host gabbro and the shock vein for the U-Pb dating of NWA 2977 using an ion microprobe, NanoSIMS. The majority of the analyzed phosphates, in both the SMV and host-rock, lie on a linear regression in U/Pb-Pb/Pb-Pb/Pb three-dimensional space, indicating a total Pb/U isochron age of 3.15±0.12 Ga (95% confidence level), which is consistent ages determined in previous isotopic studies of NWA 2977 (Sm-Nd age of 3.10±0.05 Ga, Rb-Sr age of 3.29±0.11 Ga, and Pb-Pb baddeleyite age of 3.12±0.01 Ga), and identical to the age of the U-Pb phosphate in a paired meteorite NWA 773, 3.09±0.20 Ga, derived from our dataset. There was no clear difference in the formation age between the phosphates found in the SMV and host-rock, although the shape and size of the grains and the Raman spectra show the evidence of intense shock metamorphism. Based on these findings, the cooling rate of the phosphate was very rapid, constrained to be larger than 140 K/s.

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Source
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC10209660PMC
http://dx.doi.org/10.5702/massspectrometry.A0115DOI Listing

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