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Hydrogen Produced by Reduction of H2O in Rock Reaction: Peridotite vs Basalt

机译:通过减少岩石反应中的H2O产生的氢气:橄榄石VS玄武岩

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The extraction of abiogenic H2 from the earth as an energy resource[1] is a possibility raised by the recognition that ultramafic rocks yield hydrogen in the course of serpentinization [2–5], through which water is reduced to H2 as ferrous iron from peridotite minerals oxidizes. Given the straightforward oxidation of iron silicate to magnetite to make H2, it would appear that other mafic rocks such as basalt should also yield H2, however, H2 production from basalt-hosted springs and geothermal fluids is small, e.g. Icelandic waters, as compiled by Arnorsson, et al. [6]. To examine whether the apparent difference in H2 production between peridotite and basalt is rooted in thermodynamically constrained mineral-water equilibria, we compare computed reactions of water with basalt and peridotite. We find that the serpentinization of peridotite yields abundant H2 as ferrous iron silicates oxidize to form magnetite, but that little H2 forms in basalt reaction because ferrous silicates alter to ferrous iron chlorite instead of magnetite or other ferric minerals. A principal cause of the difference is that chlorite requires alumina to form, but alumina concentration is minimal in peridotite although substantial in basalt.
机译:从地球作为能量资源的辐射H2的提取是通过识别出在蛇形化[2-5]过程中的识别中的识别提出的可能性,通过该岩石在恒星中将水还原成H 2作为铁铁矿物质氧化。鉴于铁硅酸盐的直接氧化磁铁矿制作H2,似乎玄武岩如玄武岩的其他乳头岩也应该产生H2,然而,来自玄武岩宿主的弹簧和地热流体的H 2产生是小的,例如,来自玄武岩宿主的H2。冰岛水域,由Arnorsson等人编制。 [6]。为了检查恒星和玄武岩之间的H2产生的表观差异是否根植于热力学限制的矿泉水平衡,我们将水与玄武岩和恒星的计算反应比较。我们发现恒星的蛇形化产生了丰富的H2,因为铁铁硅酸盐氧化形成磁铁矿,但是在玄武岩反应中形成少量的H2形式,因为铁硅酸铁硅酸铁或其他铁矿石或其他铁矿石。差异的主要原因是氯酸盐需要氧化铝形成,但氧化铝浓度在恒星中最小,但在玄武岩中很大。

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