Uranium‐lead ages for lunar zircons: Evidence for a prolonged period of granophyre formation from 4.32 to 3.88 Ga
- 1 May 1996
- journal article
- Published by Wiley in Meteoritics & Planetary Science
- Vol. 31 (3) , 370-387
- https://doi.org/10.1111/j.1945-5100.1996.tb02075.x
Abstract
The ages of a number of small fragments of lunar granophyre have been determined by the in situ U‐Th‐Pb isotopic analysis of zircon using a sensitive high mass‐resolution ion microprobe (SHRIMP I). The zircon from lunar granophyre is characterized by consistently high U and Th contents (most 200–500 ppm and 100–300 ppm, respectively) compared to zircon from mafic lunar rocks. Some fragments of lunar granophyre are found to be as old as 4.32 Ga, supporting other evidence that the original lunar magma ocean crystallized completely within ∼200 Ma of the formation of the Moon itself. Other fragments are as young as 3.88 Ga, which is much later than the time of formation of most of the lunar crust. The older lunar granophyres have rare‐earth‐element (REE) patterns that are similar to lunar KREEP, whilst the younger granophyres have bow‐shaped REE patterns that feature a greater relative enrichment in the heavy REE. The wide range of ages of numerous lunar zircons, lunar granophyres and other rocks indicates that zircon‐forming magmatism in the lunar highlands was most active prior to 4.3 Ga but continuous until at least 3.88 Ga.The U‐Pb isotopic composition of much lunar zircon is near concordant, but the effects of isotopic disturbance as late as ∼1.0 Ga are observed in some zircon, both within granophyre fragments recrystallized by reheating and within fragments in which the original delicate silica‐K‐feldspar granophyric intergrowth is well preserved. It is therefore essential to make multiple analyses of individual zircon grains, and preferably analyses of suites of zircons from lunar igneous rocks if they are to be dated reliably by the U‐Pb method.It is possible that some of the younger lunar granophyres are the product of large‐scale silicate‐liquid immiscibility within late‐stage differentiates, but this remains unproven until remnants of demonstrably cogenetic, Fe‐rich, immiscible liquid are positively identified.Keywords
This publication has 39 references indexed in Scilit:
- SmNd constraints on early lunar differentiation and the evolution of KREEPPublished by Elsevier ,2002
- The age and Pb loss behaviour of zircons from the Isua supracrustal belt as determined by ion microprobeEarth and Planetary Science Letters, 1986
- Petrology and chemistry of two “large” granite clasts from the moonEarth and Planetary Science Letters, 1983
- High-resolution ion-microprobe measurement of lead isotopes: Variations within single zircons from Lac Seul, northwestern OntarioEarth and Planetary Science Letters, 1979
- Plagiogranites as late-stage immiscible liquids in ophiolite and mid-ocean ridge suites: An experimental studyEarth and Planetary Science Letters, 1979
- The origin of KREEPReviews of Geophysics, 1979
- Lunar sample 15405: Remnant of a KREEP basalt-granite differentiated plutonEarth and Planetary Science Letters, 1976
- U, Th, Pb and REE abundances and207Pb/206Pb ages of individual minerals in returned lunar material by ion microprobe mass analysisEarth and Planetary Science Letters, 1972
- Li, K, Rb, Sr, Ba and rare-earth concentrations, and RbSr age of lunar rock 12013Earth and Planetary Science Letters, 1970
- Mineralogy and petrology of Apollo 12 sample No. 12013: A progress reportEarth and Planetary Science Letters, 1970