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大洋中脊(MOR)附近的非生物氢(H)源和汇及其对海底生物圈的影响。

Abiotic hydrogen (H) sources and sinks near the Mid-Ocean Ridge (MOR) with implications for the subseafloor biosphere.

机构信息

Division of Earth and Ocean Sciences, Nicholas School of the Environment, Duke University, Durham, NC 27708;

Division of Earth and Ocean Sciences, Nicholas School of the Environment, Duke University, Durham, NC 27708.

出版信息

Proc Natl Acad Sci U S A. 2020 Jun 16;117(24):13283-13293. doi: 10.1073/pnas.2002619117. Epub 2020 Jun 1.

DOI:10.1073/pnas.2002619117
PMID:32482880
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC7306814/
Abstract

Free hydrogen (H) is a basal energy source underlying chemosynthetic activity within igneous ocean crust. In an attempt to systematically account for all H within young oceanic lithosphere (<10 Ma) near the Mid-Ocean Ridge (MOR), we construct a box model of this environment. Within this control volume, we assess abiotic H sources (∼6 × 10 mol H/y) and sinks (∼4 × 10 mol H/y) and then attribute the net difference (∼2 × 10 mol H/y) to microbial consumption in order to balance the H budget. Despite poorly constrained details and large uncertainties, our analytical framework allows us to synthesize a vast body of pertinent but currently disparate information in order to propose an initial global estimate for microbial H consumption within young ocean crust that is tractable and can be iteratively improved upon as new data and studies become available. Our preliminary investigation suggests that microbes beneath the MOR may be consuming a sizeable portion (at least ∼30%) of all produced H, supporting the widely held notion that subseafloor microbes voraciously consume H and play a fundamental role in the geochemistry of Earth's ocean-atmosphere system.

摘要

游离氢(H)是火成海洋地壳中化学合成活动的基础能源。为了尝试系统地计算中洋脊(MOR)附近年轻海洋岩石圈(<10 百万年)中所有的 H,我们构建了该环境的箱式模型。在这个控制体积内,我们评估了非生物 H 源(∼6 × 10 mol H/y)和汇(∼4 × 10 mol H/y),然后将净差值(∼2 × 10 mol H/y)归因于微生物消耗,以平衡 H 预算。尽管细节受到限制且存在很大的不确定性,但我们的分析框架允许我们综合大量相关但目前不同的信息,以便在有新的数据和研究结果时,可以提出一个适用于年轻海洋地壳中微生物 H 消耗的初始全球估算,这个估算具有可操作性,并可以不断改进。我们的初步研究表明,MOR 下方的微生物可能正在消耗大量产生的 H(至少∼30%),这支持了这样一种广泛的观点,即海底微生物贪婪地消耗 H,并在地球海洋-大气系统的地球化学中发挥着重要作用。