Rubidium isotopes reveal dehydration and melting of the subducting slab beneath the Mariana arc - INSU - Institut national des sciences de l'Univers
Article Dans Une Revue Earth and Planetary Science Letters Année : 2024

Rubidium isotopes reveal dehydration and melting of the subducting slab beneath the Mariana arc

Ding-Sheng Jiang
  • Fonction : Auteur
Xiao-Tong Peng
  • Fonction : Auteur
Wen-Jing Xu
  • Fonction : Auteur
Xia Hu
  • Fonction : Auteur
Xi-Sheng Xu
  • Fonction : Auteur
Guo-Liang Zhang
  • Fonction : Auteur
Chong-Jin Pang
  • Fonction : Auteur
Hao-Chen Duan
  • Fonction : Auteur
Fang Huang
  • Fonction : Auteur

Résumé

Rubidium (Rb) is a strongly incompatible and highly fluid-mobile element and Rb isotopes have the potential to track subducted material recycling to the mantle source of arc magmas. However, the behavior of Rb isotopes during slab subduction and associated processes remains unconstrained. This study for the first time presents Rb isotope data for the altered oceanic crust (AOC) from IODP Site U1365, subducted sediments, and lavas from the Southern Mariana arc. The δ87Rb of the AOC varies between –0.16 ± 0.03 ‰ to 0.07 ± 0.02 ‰ with a weighted average of –0.02 ± 0.06 ‰, which is higher than that of fresh mid-ocean ridge basalts (MORB; –0.12 ± 0.08 ‰). Such Rb isotope fractionation may be attributed to the preferential loss of 85Rb into seawater during the dissolution of primary phases and the preferential structural incorporation of 87Rb into secondary phases and preferential 87Rb adsorption by clays. The δ87Rb of the sediments varies from –0.20 ± 0.07 ‰ to –0.03 ± 0.02 ‰ with an average of –0.11 ± 0.12 ‰, identical to that of the upper continental crust (UCC; –0.14 ± 0.08 ‰). The correlations observed between δ87Rb and sediment depth (and loss on ignition; LOI) suggest that hydrodynamic sorting of sediments which enriches the upper stratigraphic intervals in clays, exerts a first-order control on the Rb isotope fractionation in subducted sediments. The formation of authigenic clays, which act as a sink of 85Rb from seawater, could partially account for the elevated δ87Rb of seawater (0.14 ± 0.12 ‰) relative to the Bulk Silicate Earth (BSE; –0.12 ± 0.06 ‰). For the Mariana lavas, the δ87Rb decreases from fore-arc lavas (–0.03 ± 0.04 ‰ to 0.09 ± 0.02 ‰) to frontal arc lavas (–0.12 ± 0.04 ‰ to –0.01 ± 0.03 ‰), which are all higher than the average δ87Rb of fresh MORB (–0.12 ± 0.08 ‰). The elevated δ87Rb of the lavas reflects the addition of AOC-derived aqueous fluids with a high δ87Rb (∼0.08 ‰) to the magma source, which is higher than the average δ87Rb (–0.02 ± 0.18 ‰) of the Site-1365 AOC. The variation of δ87Rb with 143Nd/144Ndi values of the lavas indicates that AOC-derived aqueous fluids are increasingly mixed with a component with a low δ87Rb that most likely represents sediment melts. The estimated δ87Rb of sediment melts is about –0.27 ‰, lower than the average δ87Rb (–0.11 ± 0.12 ‰) of the Mariana sediments. Thus, our study suggests that Rb isotopes can be fractionated during AOC dehydration and sediment partial melting. Overall, the across-arc Rb isotope variation reflects slab dehydration and melting at different subduction depths. Our findings demonstrate that Rb isotopes are a powerful novel tool for probing deep recycling of subducted slabs. Furthermore, they can distinguish contributions from AOC-derived fluids versus sediment-derived melts to the source of arc magmas.
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Dates et versions

insu-04719394 , version 1 (03-10-2024)

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Citer

Ding-Sheng Jiang, Xiao-Tong Peng, Wen-Jing Xu, Xia Hu, Saskia Erdmann, et al.. Rubidium isotopes reveal dehydration and melting of the subducting slab beneath the Mariana arc. Earth and Planetary Science Letters, 2024, 646, ⟨10.1016/j.epsl.2024.118978⟩. ⟨insu-04719394⟩
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