Mineralogical Changes and H2 Generation Yield During Hydrothermal Alteration of a Magnetite-Siderite Assemblage
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F25%3A10510395" target="_blank" >RIV/00216208:11320/25:10510395 - isvavai.cz</a>
Výsledek na webu
<a href="https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=el.nSA8kfG" target="_blank" >https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=el.nSA8kfG</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1029/2024JB030724" target="_blank" >10.1029/2024JB030724</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Mineralogical Changes and H2 Generation Yield During Hydrothermal Alteration of a Magnetite-Siderite Assemblage
Popis výsledku v původním jazyce
To date, the generation of natural hydrogen (H<inf>2</inf>) from the alteration of Fe<sup>II</sup>-bearing minerals has mainly been studied through serpentinization in (ultra)mafic rocks. This study explores Banded Iron Formations (BIF), which are rich in Fe<sup>II</sup> minerals, as a potential source for H<inf>2</inf>. We conducted a hydrothermal experiment at 200°C with a combined magnetite-siderite assemblage, two major components of BIF. The experiment, designed with a high water-to-rock ratio and a gas phase (W-R = 300) enabled to assess mineral transformations during the alteration. Thermodynamic simulations were finally conducted, to explore H<inf>2</inf>-generating yields in more realistic geological scenarios (no gas phase, lower W-R). Our experimental findings show that H<inf>2</inf> is produced through complete siderite dissolution and magnetite precipitation. Concomitantly, non-stoichiometric primary magnetite (Fe<sup>II</sup>/Fe<sup>III</sup> < 0.5) did not enhance H<inf>2</inf> yield; instead, it acted as a sink for dissolved Fe<sup>2+</sup>, sequestrating about 10% of the iron from siderite without oxidation to recover a more ideal stoichiometry. This suggests that abundant, non-stoichiometric magnetite in natural settings may reduce H<inf>2</inf> generation yields. Mass balance calculations indicate that 83% of the expected H<inf>2</inf> generated was unaccounted for, consistent with suspected CO<inf>2</inf> reduction and formation of dissolved organic compounds in the fluids. Thermodynamic simulations at varying W-R ratios (from 300 to 1) reveal that H<inf>2</inf> yield ranges widely (39 mmol-73 μmol H<inf>2</inf> per kg of siderite), since lower W-R prevent from siderite dissolution and enhance H<inf>2</inf> consumption via carbon reduction. These findings imply that low W-R ratios in BIF -and other siderite-bearing lithologies, may limit H<inf>2</inf> resources.
Název v anglickém jazyce
Mineralogical Changes and H2 Generation Yield During Hydrothermal Alteration of a Magnetite-Siderite Assemblage
Popis výsledku anglicky
To date, the generation of natural hydrogen (H<inf>2</inf>) from the alteration of Fe<sup>II</sup>-bearing minerals has mainly been studied through serpentinization in (ultra)mafic rocks. This study explores Banded Iron Formations (BIF), which are rich in Fe<sup>II</sup> minerals, as a potential source for H<inf>2</inf>. We conducted a hydrothermal experiment at 200°C with a combined magnetite-siderite assemblage, two major components of BIF. The experiment, designed with a high water-to-rock ratio and a gas phase (W-R = 300) enabled to assess mineral transformations during the alteration. Thermodynamic simulations were finally conducted, to explore H<inf>2</inf>-generating yields in more realistic geological scenarios (no gas phase, lower W-R). Our experimental findings show that H<inf>2</inf> is produced through complete siderite dissolution and magnetite precipitation. Concomitantly, non-stoichiometric primary magnetite (Fe<sup>II</sup>/Fe<sup>III</sup> < 0.5) did not enhance H<inf>2</inf> yield; instead, it acted as a sink for dissolved Fe<sup>2+</sup>, sequestrating about 10% of the iron from siderite without oxidation to recover a more ideal stoichiometry. This suggests that abundant, non-stoichiometric magnetite in natural settings may reduce H<inf>2</inf> generation yields. Mass balance calculations indicate that 83% of the expected H<inf>2</inf> generated was unaccounted for, consistent with suspected CO<inf>2</inf> reduction and formation of dissolved organic compounds in the fluids. Thermodynamic simulations at varying W-R ratios (from 300 to 1) reveal that H<inf>2</inf> yield ranges widely (39 mmol-73 μmol H<inf>2</inf> per kg of siderite), since lower W-R prevent from siderite dissolution and enhance H<inf>2</inf> consumption via carbon reduction. These findings imply that low W-R ratios in BIF -and other siderite-bearing lithologies, may limit H<inf>2</inf> resources.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10302 - Condensed matter physics (including formerly solid state physics, supercond.)
Návaznosti výsledku
Projekt
—
Návaznosti
S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2025
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Journal of Geophysical Research: Solid Earth
ISSN
2169-9313
e-ISSN
2169-9356
Svazek periodika
130
Číslo periodika v rámci svazku
8
Stát vydavatele periodika
US - Spojené státy americké
Počet stran výsledku
17
Strana od-do
1-17
Kód UT WoS článku
001547177000001
EID výsledku v databázi Scopus
2-s2.0-105012627113