NanoSIMS and EPMA dating of lunar zirconolite

Abstract Zirconolite is a common Zr-rich accessary mineral in mafic rocks. It is also an ideal U–Pb/Pb–Pb chronometer because it commonly contains high U content (mostly 0.1–10 wt%) and negligible initial Pb. However, zirconolite is usually very small (e.g., ~ 1 μm in width) in lunar rocks, requirin...

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Main Authors: Nian Wang, Qian Mao, Ting Zhang, Jialong Hao, Yangting Lin
Format: Article
Language:English
Published: SpringerOpen 2021-09-01
Series:Progress in Earth and Planetary Science
Subjects:
Online Access:https://doi.org/10.1186/s40645-021-00446-3
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author Nian Wang
Qian Mao
Ting Zhang
Jialong Hao
Yangting Lin
author_facet Nian Wang
Qian Mao
Ting Zhang
Jialong Hao
Yangting Lin
author_sort Nian Wang
collection DOAJ
description Abstract Zirconolite is a common Zr-rich accessary mineral in mafic rocks. It is also an ideal U–Pb/Pb–Pb chronometer because it commonly contains high U content (mostly 0.1–10 wt%) and negligible initial Pb. However, zirconolite is usually very small (e.g., ~ 1 μm in width) in lunar rocks, requiring a high spatial resolution analysis. We analyzed a single, large (25 μm × 20 μm) grain of zirconolite in lunar meteorite NWA 4485 using Pb–Pb dating by NanoSIMS and U–Th–Pb dating by EPMA. The resultant U–Th–Pb age is 4540 ± 340 Ma (2σ) with a spatial resolution of 1.3 μm. The Pb–Pb age by NanoSIMS is 4348.5 ± 4.8 Ma (2σ) with a spatial resolution of ~ 2 μm, consistent with the age of 4352 ± 10 Ma and 4344 ± 14 Ma reported in the same meteorite and its paired meteorite NWA 4472. Although U–Th–Pb age is somewhat older, it still includes the NanoSIMS results within the analytical uncertainty. This work demonstrates the potential application of the combined EPMA dating and REE analysis of lunar zirconolite, with the benefits of high spatial resolution, non-destructive, and readily accessibility of the instrument. The precision of the EPMA dating (7.6%, 2σ) can be improved by increasing the counting time for Pb, U and Th. We expect to apply this EPMA technique for a quick and non-destructive age survey and geochemical study of zirconolite grains from the lunar mare basalts newly returned by Chang’E-5 mission which landed on a very young (1.2–2.0 Ga by crater-counting chronology) basalt unit in Procellarum KREEP Terrain.
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spelling doaj.art-44e79a4c80644316a252e3e44a9787c02022-12-21T20:03:48ZengSpringerOpenProgress in Earth and Planetary Science2197-42842021-09-01811810.1186/s40645-021-00446-3NanoSIMS and EPMA dating of lunar zirconoliteNian Wang0Qian Mao1Ting Zhang2Jialong Hao3Yangting Lin4Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of SciencesState Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics, Chinese Academy of SciencesKey Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of SciencesKey Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of SciencesKey Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of SciencesAbstract Zirconolite is a common Zr-rich accessary mineral in mafic rocks. It is also an ideal U–Pb/Pb–Pb chronometer because it commonly contains high U content (mostly 0.1–10 wt%) and negligible initial Pb. However, zirconolite is usually very small (e.g., ~ 1 μm in width) in lunar rocks, requiring a high spatial resolution analysis. We analyzed a single, large (25 μm × 20 μm) grain of zirconolite in lunar meteorite NWA 4485 using Pb–Pb dating by NanoSIMS and U–Th–Pb dating by EPMA. The resultant U–Th–Pb age is 4540 ± 340 Ma (2σ) with a spatial resolution of 1.3 μm. The Pb–Pb age by NanoSIMS is 4348.5 ± 4.8 Ma (2σ) with a spatial resolution of ~ 2 μm, consistent with the age of 4352 ± 10 Ma and 4344 ± 14 Ma reported in the same meteorite and its paired meteorite NWA 4472. Although U–Th–Pb age is somewhat older, it still includes the NanoSIMS results within the analytical uncertainty. This work demonstrates the potential application of the combined EPMA dating and REE analysis of lunar zirconolite, with the benefits of high spatial resolution, non-destructive, and readily accessibility of the instrument. The precision of the EPMA dating (7.6%, 2σ) can be improved by increasing the counting time for Pb, U and Th. We expect to apply this EPMA technique for a quick and non-destructive age survey and geochemical study of zirconolite grains from the lunar mare basalts newly returned by Chang’E-5 mission which landed on a very young (1.2–2.0 Ga by crater-counting chronology) basalt unit in Procellarum KREEP Terrain.https://doi.org/10.1186/s40645-021-00446-3ZirconoliteChemical ageLunar sampleNWA 4485Chang’E-5Lunar basalt
spellingShingle Nian Wang
Qian Mao
Ting Zhang
Jialong Hao
Yangting Lin
NanoSIMS and EPMA dating of lunar zirconolite
Progress in Earth and Planetary Science
Zirconolite
Chemical age
Lunar sample
NWA 4485
Chang’E-5
Lunar basalt
title NanoSIMS and EPMA dating of lunar zirconolite
title_full NanoSIMS and EPMA dating of lunar zirconolite
title_fullStr NanoSIMS and EPMA dating of lunar zirconolite
title_full_unstemmed NanoSIMS and EPMA dating of lunar zirconolite
title_short NanoSIMS and EPMA dating of lunar zirconolite
title_sort nanosims and epma dating of lunar zirconolite
topic Zirconolite
Chemical age
Lunar sample
NWA 4485
Chang’E-5
Lunar basalt
url https://doi.org/10.1186/s40645-021-00446-3
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AT qianmao nanosimsandepmadatingoflunarzirconolite
AT tingzhang nanosimsandepmadatingoflunarzirconolite
AT jialonghao nanosimsandepmadatingoflunarzirconolite
AT yangtinglin nanosimsandepmadatingoflunarzirconolite