Yunzhe Chen , Peng Wu , Tiago Angelo , Christopher Spencer , Long Li
{"title":"Magmatic N2 degassing dominates nitrogen loss during sediment subduction and granitoid genesis","authors":"Yunzhe Chen , Peng Wu , Tiago Angelo , Christopher Spencer , Long Li","doi":"10.1016/j.epsl.2024.119094","DOIUrl":null,"url":null,"abstract":"<div><div>Subducting sediments contain much more abundant nitrogen (N) than the other slab components. The fate of sedimentary N along subduction directly determines the quantity of surficial N that can be released back to the atmosphere/crust or further delivered to the deep mantle, which has a strong impact on the long-term evolution of the N budgets and isotopic signatures of Earth's major reservoirs. Previous studies on the fate of subducted sedimentary N have been intensively focused on assessing the extent of metamorphic N devolatilization from metasedimentary rocks varying from ultrahigh-pressure eclogites facies (subducted to as deep as 90 km) in cold subduction zones to medium-pressure amphibolite facies in extremely hot subduction zones. However, the fate of sedimentary N after these metamorphic stages, particularly during sediment melting and subsequent magmatic crystallization, has not been examined so far. Here, we present the N data of the Cretaceous peraluminous granitoids in the Oman-United Arab Emirates area, which were formed by melting of subducted pelagic sediments followed by intrusion and crystallization in the lithospheric mantle before the entire lithospheric section was obducted to form the Oman-United Arab Emirates ophiolites. The 27 studied samples show surprisingly low N contents (4.0 - 13.7 ppm; mean: 6.9 ± 2.3 ppm; 1σ) and a narrow δ<sup>15</sup>N range (mostly in the range of –1.4‰ to +2.2‰; mean: +0.4 ± 1.5‰; 1σ). Data modeling indicates that the N in these granitoids contains little mantle contribution and was predominantly inherited from their source rocks. Compared with potential source rocks, these granitoids display orders of magnitude lower N contents but comparable δ<sup>15</sup>N values, indicating that the significant N loss during the genesis of these granitoids was associated with little N isotope fractionation. This suggests that magmatic N<sub>2</sub> degassing (with minor N isotope fractionation) rather than metamorphic N devolatilization (with much larger N isotope fractionation) is the dominant mechanism driving the N loss from subducted sediments.</div></div>","PeriodicalId":11481,"journal":{"name":"Earth and Planetary Science Letters","volume":"648 ","pages":"Article 119094"},"PeriodicalIF":4.8000,"publicationDate":"2024-11-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Earth and Planetary Science Letters","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0012821X24005260","RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Subducting sediments contain much more abundant nitrogen (N) than the other slab components. The fate of sedimentary N along subduction directly determines the quantity of surficial N that can be released back to the atmosphere/crust or further delivered to the deep mantle, which has a strong impact on the long-term evolution of the N budgets and isotopic signatures of Earth's major reservoirs. Previous studies on the fate of subducted sedimentary N have been intensively focused on assessing the extent of metamorphic N devolatilization from metasedimentary rocks varying from ultrahigh-pressure eclogites facies (subducted to as deep as 90 km) in cold subduction zones to medium-pressure amphibolite facies in extremely hot subduction zones. However, the fate of sedimentary N after these metamorphic stages, particularly during sediment melting and subsequent magmatic crystallization, has not been examined so far. Here, we present the N data of the Cretaceous peraluminous granitoids in the Oman-United Arab Emirates area, which were formed by melting of subducted pelagic sediments followed by intrusion and crystallization in the lithospheric mantle before the entire lithospheric section was obducted to form the Oman-United Arab Emirates ophiolites. The 27 studied samples show surprisingly low N contents (4.0 - 13.7 ppm; mean: 6.9 ± 2.3 ppm; 1σ) and a narrow δ15N range (mostly in the range of –1.4‰ to +2.2‰; mean: +0.4 ± 1.5‰; 1σ). Data modeling indicates that the N in these granitoids contains little mantle contribution and was predominantly inherited from their source rocks. Compared with potential source rocks, these granitoids display orders of magnitude lower N contents but comparable δ15N values, indicating that the significant N loss during the genesis of these granitoids was associated with little N isotope fractionation. This suggests that magmatic N2 degassing (with minor N isotope fractionation) rather than metamorphic N devolatilization (with much larger N isotope fractionation) is the dominant mechanism driving the N loss from subducted sediments.
期刊介绍:
Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.