2D reactive transport simulations of mid-ocean ridge hydrothermal systems

Water-rock interactions in mid-ocean ridge hydrothermal systems are a critical part of Earth system evolution. Extensive insights have been developed from vent fluid chemistry and laboratory experiments, but these leave unanswered many questions about the temporal evolution and spatial structure of...

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Main Authors: DePaolo Donald, Sonnenthal Eric, Pester Nicholas
Format: Article
Language:English
Published: EDP Sciences 2019-01-01
Series:E3S Web of Conferences
Online Access:https://www.e3s-conferences.org/articles/e3sconf/pdf/2019/24/e3sconf_wri-162018_05006.pdf
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spelling doaj-cab00f6737334dd38924358f8ecc43cf2021-03-02T10:45:42ZengEDP SciencesE3S Web of Conferences2267-12422019-01-01980500610.1051/e3sconf/20199805006e3sconf_wri-162018_050062D reactive transport simulations of mid-ocean ridge hydrothermal systemsDePaolo DonaldSonnenthal Eric0Pester NicholasLawrence Berkeley National LaboratoryWater-rock interactions in mid-ocean ridge hydrothermal systems are a critical part of Earth system evolution. Extensive insights have been developed from vent fluid chemistry and laboratory experiments, but these leave unanswered many questions about the temporal evolution and spatial structure of the hydrothermal systems that can only be addressed with reactive transport simulations. Other issues are the effects of changing spreading rates and seawater chemistry through Earth history. We are addressing this problem using the Toughreact code, starting with 2D static (no seafloor spreading) simulations of the near-axis region where most of the interaction occurs. The simulations use a dual-permeability grid to represent fractured rocks, and also have a formulation for Sr isotope exchange. Vent fluid Ca, Mg, SO4, and Na concentrations and Sr isotopes can be used as a guide to fluid chemical evolution. Initial simulations reproduce modern vent fluid chemistry even with maximum temperature only at 380°C, and suggest that fluids need not be in equilibrium with the rocks at any point in the system. Model fluids continue to evolve chemically even in the upflow zone prior to venting. The effects of different seawater chemical composition, as proposed for the Cretaceous, for example, can be captured with charge-balance models.https://www.e3s-conferences.org/articles/e3sconf/pdf/2019/24/e3sconf_wri-162018_05006.pdf
collection DOAJ
language English
format Article
sources DOAJ
author DePaolo Donald
Sonnenthal Eric
Pester Nicholas
spellingShingle DePaolo Donald
Sonnenthal Eric
Pester Nicholas
2D reactive transport simulations of mid-ocean ridge hydrothermal systems
E3S Web of Conferences
author_facet DePaolo Donald
Sonnenthal Eric
Pester Nicholas
author_sort DePaolo Donald
title 2D reactive transport simulations of mid-ocean ridge hydrothermal systems
title_short 2D reactive transport simulations of mid-ocean ridge hydrothermal systems
title_full 2D reactive transport simulations of mid-ocean ridge hydrothermal systems
title_fullStr 2D reactive transport simulations of mid-ocean ridge hydrothermal systems
title_full_unstemmed 2D reactive transport simulations of mid-ocean ridge hydrothermal systems
title_sort 2d reactive transport simulations of mid-ocean ridge hydrothermal systems
publisher EDP Sciences
series E3S Web of Conferences
issn 2267-1242
publishDate 2019-01-01
description Water-rock interactions in mid-ocean ridge hydrothermal systems are a critical part of Earth system evolution. Extensive insights have been developed from vent fluid chemistry and laboratory experiments, but these leave unanswered many questions about the temporal evolution and spatial structure of the hydrothermal systems that can only be addressed with reactive transport simulations. Other issues are the effects of changing spreading rates and seawater chemistry through Earth history. We are addressing this problem using the Toughreact code, starting with 2D static (no seafloor spreading) simulations of the near-axis region where most of the interaction occurs. The simulations use a dual-permeability grid to represent fractured rocks, and also have a formulation for Sr isotope exchange. Vent fluid Ca, Mg, SO4, and Na concentrations and Sr isotopes can be used as a guide to fluid chemical evolution. Initial simulations reproduce modern vent fluid chemistry even with maximum temperature only at 380°C, and suggest that fluids need not be in equilibrium with the rocks at any point in the system. Model fluids continue to evolve chemically even in the upflow zone prior to venting. The effects of different seawater chemical composition, as proposed for the Cretaceous, for example, can be captured with charge-balance models.
url https://www.e3s-conferences.org/articles/e3sconf/pdf/2019/24/e3sconf_wri-162018_05006.pdf
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