Article (Scientific journals)
The very late-stage crystallization of the lunar magma ocean and the composition of immiscible urKREEP
Zhang, Yishen; Charlier, Bernard; Krein, Stephanie B. et al.
2024In Earth and Planetary Science Letters, 646, p. 118989
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Keywords :
Differentiation; Ilmenite; KREEP basalt; Liquid immiscibility; Lunar magma ocean; Late stage; Magma ocean; Magmatisms; Residual melts; Silicate liquids; SiO 2; Geophysics; Geochemistry and Petrology; Space and Planetary Science; Earth and Planetary Sciences (miscellaneous)
Abstract :
[en] The latest stages of the lunar magma ocean (LMO) crystallization led to the formation of ilmenite-bearing cumulates and urKREEP, residual melts enriched in K, rare earth elements (REEs), P, and other incompatible elements. Those highly evolved lithologies had major impacts on the petrogenesis of lunar volcanic rocks and the compositional diversity of post-LMO magmatism resulting from mantle remelting. Here, we present new experimental results constraining the composition of the very last liquids produced during LMO crystallization. To test the potential role of silicate liquid immiscibility in the formation of urKREEP, synthetic samples representative of residual melts of bulk Moon compositions were placed in double platinum-graphite capsules at 1020–980 °C and 0.08–0.10 GPa in an internally-heated pressure vessel. The produced silicate liquids are multiply saturated with plagioclase, augite, silica phases, and ilmenite (± fayalitic olivine ± pigeonite). Our experiments show that the liquid line of descent reaches a two-liquid field at 1000 °C and >97% crystallization for a range of whole-Moon compositions. Under these conditions, a small proportion of silica-rich melt (70.0–71.4 wt.% SiO2, 6.4–7.3 wt.% FeO, 5.4–6.1 wt.% K2O, 0.2–0.3 wt.% P2O5) coexists within an abundant Fe-rich melt (42.6–44.1 wt.% SiO2, 27.6–28.8 wt.% FeO, 0.9–1.0 wt.% K2O, 2.8–3.2 wt.% P2O5) with sharp two-liquid interfaces. Our experimental results also constrain the relative onset of ilmenite crystallization compared to the development of immiscibility and indicate that an ilmenite-bearing layer formed in the lunar interior before immiscibility was attained. Using a self-consistent physicochemical LMO model, we constrain the thickness and depth of the ilmenite-bearing layer during LMO differentiation. The immiscible K-Si-rich and P-Fe-rich melts together also produced an immiscible urKREEP layer ∼2–6 km thick and ∼30–50 km deep depending on the trapped liquid fraction in the cumulate column (≤10%) and the thickness of the buoyant anorthosite crust (30–50 km). We provide constraints on the relationship between the compositions of immiscible urKREEP melts and those of KREEPy rocks. By modeling the mixing of KREEP-poor basalt and the immiscible melt pairs, we reproduce the K and P enrichments and apparent decoupling of K from P in KREEPy rocks. Our results highlight that processes such as the assimilation of evolved heterogeneous mantle lithologies may be involved in hybridization during post-LMO magmatism. The immiscible K-Si-rich lithology may also have contributed to lunar silicic magmatism.
Disciplines :
Earth sciences & physical geography
Author, co-author :
Zhang, Yishen ;  Department of Earth and Environmental Sciences, KU Leuven, Leuven, Belgium ; Department of Earth, Environmental and Planetary Sciences, Rice University, Houston, United States
Charlier, Bernard  ;  Université de Liège - ULiège > Département de géologie > Pétrologie, géochimie endogènes et pétrophysique ; Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, Cambridge, United States ; Institut für Erdsystemwissenschaften, IESW, Abteilung Mineralogie, Leibniz Universität Hannover, Hannover, Germany
Krein, Stephanie B.;  Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, Cambridge, United States
Grove, Timothy L.;  Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, Cambridge, United States
Namur, Olivier ;  Department of Earth and Environmental Sciences, KU Leuven, Leuven, Belgium ; Institut für Erdsystemwissenschaften, IESW, Abteilung Mineralogie, Leibniz Universität Hannover, Hannover, Germany
Holtz, Francois ;  Institut für Erdsystemwissenschaften, IESW, Abteilung Mineralogie, Leibniz Universität Hannover, Hannover, Germany
Language :
English
Title :
The very late-stage crystallization of the lunar magma ocean and the composition of immiscible urKREEP
Publication date :
15 November 2024
Journal title :
Earth and Planetary Science Letters
ISSN :
0012-821X
eISSN :
1385-013X
Publisher :
Elsevier B.V.
Volume :
646
Pages :
118989
Peer reviewed :
Peer Reviewed verified by ORBi
Funding text :
BC acknowledges support by a Marie Curie International Outgoing Fellowship within the 7th European Community Framework Programme. This work was supported by the Fonds de la Recherche Scientifique \u2013 FNRS under Grant 33653710. BC is a Research Associate of the Belgian Fund for Scientific Research-FNRS. Discussions with Oliver Shorttle, Attilio Rivoldini, and Dian Ji are highly appreciated. R. Dennen is thanked for his help in editing the manuscript. We thank Frederic Moynier for editorial handling. Constructive comments from Nick Dygert and an anonymous reviewer significantly improved the quality of the paper.
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