Revisiting magnesium isotope constraints on the petrogenesis of the Fe-Ti oxide-bearing mafic–ultramafic intrusions

IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Geochimica et Cosmochimica Acta Pub Date : 2025-01-15 Epub Date: 2024-09-21 DOI:10.1016/j.gca.2024.09.025
Ping-Ping Liu , Ben Ma , Fang-Zhen Teng , Zhen-Chao Wang
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Abstract

Stable isotopes of metals, such as magnesium (Mg) and iron (Fe), typically undergo minimal fractionation at magmatic temperatures. However, in Fe-Ti oxide-bearing intrusions, significant Mg isotope fractionation (Δ26Mg values of up to 23 ‰) has been observed between silicates and Fe-Ti oxides. The mechanism responsible for this substantial fractionation remains unclear. This study presents Mg isotopic compositions for bulk rocks and mineral separates—including olivine, clinopyroxene, titanomagnetite, ilmenite—from sixteen Fe-Ti oxide ores in both the lower and the upper zones of the Baima layered mafic–ultramafic intrusion, as well as bulk rocks from three high-Ti basalts of the Emeishan large igneous province, SW China. Oxide ores from the lower zone and the lower section of the upper zone of the Baima intrusion are characterized by a low abundance of volatile-bearing minerals, such as apatite and hornblende. These ores exhibit δ26Mg values ranging from −0.30 to −0.14 ‰ for olivine, −0.26 to −0.06 ‰ for clinopyroxene, 0.16 to 0.60 ‰ for titanomagnetite and −0.33 to −0.21 ‰ for ilmenite, indicative of near-equilibrium fractionation. In contrast, oxide ores from the upper section of the upper zone exhibit a high abundance of volatile-bearing minerals and significantly different δ26Mg values, ranging from −0.19 to −0.05 ‰ for olivine, −0.25 to −0.10 ‰ for clinopyroxene, 0.57 to 0.60 ‰ for titanomagnetite and 0.86 to 2.34 ‰ for ilmenite, indicative of disequilibrium fractionation. A negative correlation between Fo content and δ26Mg value in olivine suggests that Mg isotopes fractionate as olivine undergoes fractional crystallization. Trapped liquid fractions, calculated based on Ce contents in apatite, suggest that rocks with high volatile-bearing mineral content have undergone re-equilibration with trapped liquids during cooling. The large disequilibrium Mg isotopic fractionation between silicates and Fe-Ti oxides is likely due to sub-solidus re-equilibration between minerals and trapped liquids. We propose that the extent of sub-solidus, diffusion-driven kinetic Mg isotopic fractionation in Fe-Ti oxide-bearing intrusions likely correlates with the volume of trapped liquids, which may serve as a significant medium accelerating ion exchange between silicates and Fe-Ti oxides. Moreover, mass balance calculations indicate that data of Mg isotopes on their own are insufficient to determine the petrogenesis of Fe-Ti oxides in layered intrusions. This insufficiency is primarily due to the low MgO content in titanomagnetite and ilmenite, where their separation causes minimal Mg isotopic fractionation of the melts.
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镁同位素对含铁钛氧化物镁铁质-超镁铁质侵入岩成因的制约
金属的稳定同位素,如镁(Mg)和铁(Fe),通常在岩浆温度下发生最小的分馏。然而,在含Fe-Ti氧化物侵入体中,在硅酸盐和Fe-Ti氧化物之间观察到显著的Mg同位素分馏(Δ26Mg值高达23‰)。造成这种严重分馏的机制尚不清楚。本文研究了白马层状基性-超基性岩体下、上带16个铁钛氧化物矿石以及峨眉山大火成岩省3个高钛玄武岩的大块岩石和矿物分离物(包括橄榄石、斜辉石、钛磁铁矿、钛铁矿)的Mg同位素组成。白马岩体下带和上带下段的氧化矿石以含磷灰石、角闪石等挥发物丰度低为特征。其中橄榄石δ26Mg值为- 0.30 ~ - 0.14‰,斜辉石δ26Mg值为- 0.26 ~ - 0.06‰,钛磁铁矿δ26Mg值为- 0.16 ~ 0.60‰,钛铁矿δ26Mg值为- 0.33 ~ - 0.21‰,属于近平衡分选。上带上段氧化矿石含挥发物丰度高,δ26Mg值差异显著,橄榄石为- 0.19 ~ - 0.05‰,斜辉石为- 0.25 ~ - 0.10‰,钛磁铁矿为0.57 ~ 0.60‰,钛铁矿为0.86 ~ 2.34‰,表现为分选不平衡。橄榄石中Fo含量与δ26Mg值呈负相关,表明Mg同位素分馏为橄榄石分馏结晶。根据磷灰石中Ce含量计算的捕获液体分数表明,具有高挥发性矿物含量的岩石在冷却过程中与捕获液体发生了再平衡。镁同位素在硅酸盐和铁钛氧化物之间的大量不平衡分馏可能是由于矿物和被困液体之间的亚固体再平衡。我们提出,在含Fe-Ti氧化物侵入体中,亚固体扩散驱动的Mg同位素分馏的程度可能与捕获液体的体积有关,这些液体可能是加速硅酸盐和Fe-Ti氧化物之间离子交换的重要介质。此外,质量平衡计算表明,Mg同位素本身的数据不足以确定层状侵入体中Fe-Ti氧化物的岩石成因。这种不足主要是由于钛磁铁矿和钛铁矿中MgO含量低,它们的分离导致熔体中Mg同位素分馏最小。
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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
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