{"title":"Evolution in Fluid Composition During Subduction","authors":"A. A. Helm, M. J. Caddick, R. J. Bodnar","doi":"10.1029/2026GC013086","DOIUrl":null,"url":null,"abstract":"<p>Fluid-rock reactions play important roles in seismicity, arc-magma chemistries, and volatile cycling at convergent plate boundaries. In subduction environments, metamorphic reactions involving hydrous fluids facilitate metasomatic alteration and mass transport. Fingerprinting the source of fluids that move across subducting lithologies is, however, challenging. We predict evolving mineralogy and fluid compositions during subduction along representative <i>PT</i>-paths, assessing closed and open system assumptions using phase assemblage modeling. Our calculations consider simplified hydrated harzburgite, hydrated mid-ocean ridge basalt, average subducted sediments, and subducted carbonates. Predict equilibrium mineralogy, fluid composition, and this allows us to identify fluid solute ratios that might be unique to a given source lithology or mineral breakdown reaction. In general, fluids derived from average subducting sediments are predicted to have a higher proportion of Na to Mg and Si than those derived from basalts at the same subduction PT condition. Fluids produced during deserpentinization of hydrated harzburgite contain a higher proportion of Mg and Ca. Together, these results help to constrain the potential sources of fluids that metasomatize subducting rocks and the overlying mantle wedge. Comparing results to examples of metasomatism and fluid inclusions from the rock record indicates that although imperfect, modeled major element fluid signatures can be an effective tool to assess the source lithology of altering fluids.</p>","PeriodicalId":50422,"journal":{"name":"Geochemistry Geophysics Geosystems","volume":"27 8","pages":""},"PeriodicalIF":3.3000,"publicationDate":"2026-08-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2026GC013086","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Geochemistry Geophysics Geosystems","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2026GC013086","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Fluid-rock reactions play important roles in seismicity, arc-magma chemistries, and volatile cycling at convergent plate boundaries. In subduction environments, metamorphic reactions involving hydrous fluids facilitate metasomatic alteration and mass transport. Fingerprinting the source of fluids that move across subducting lithologies is, however, challenging. We predict evolving mineralogy and fluid compositions during subduction along representative PT-paths, assessing closed and open system assumptions using phase assemblage modeling. Our calculations consider simplified hydrated harzburgite, hydrated mid-ocean ridge basalt, average subducted sediments, and subducted carbonates. Predict equilibrium mineralogy, fluid composition, and this allows us to identify fluid solute ratios that might be unique to a given source lithology or mineral breakdown reaction. In general, fluids derived from average subducting sediments are predicted to have a higher proportion of Na to Mg and Si than those derived from basalts at the same subduction PT condition. Fluids produced during deserpentinization of hydrated harzburgite contain a higher proportion of Mg and Ca. Together, these results help to constrain the potential sources of fluids that metasomatize subducting rocks and the overlying mantle wedge. Comparing results to examples of metasomatism and fluid inclusions from the rock record indicates that although imperfect, modeled major element fluid signatures can be an effective tool to assess the source lithology of altering fluids.
期刊介绍:
Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged.
Areas of interest for this peer-reviewed journal include, but are not limited to:
The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution
Principles and applications of geochemical proxies to studies of Earth history
The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them
The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales
Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets
The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets
Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.