Modeling the global oceanic barium cycle and implications for paleoceanographic proxies

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Hengdi Liang , Tristan J. Horner , Seth G. John
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引用次数: 0

Abstract

Barium (Ba) abundance is widely utilized as a proxy for deep ocean nutrients and organic carbon export. However, significant uncertainties remain regarding key aspects of the marine Ba cycle, including the primary Ba source to barite, the depths and rates of barite formation and dissolution, mechanisms linking the dissolved Ba and silicon cycles, and regional variability in the barium-to-organic matter ratio of exported particulates. Here, we integrate dissolved Ba observations from GEOTRACES with a model of barite saturation state and employ a mechanistic framework to constrain the major biogeochemical processes governing dissolved Ba distributions. Our results indicate that seawater, rather than organic matter, is the primary Ba source for pelagic barite, with 90 % of precipitation occurring above 900 m. Approximately two-thirds of pelagic barite dissolution occurs in the water column, while the remainder takes place at the seafloor. Dissolution rates appear independent of ambient saturation state, with the best model–data fit achieved when dissolution is treated as a constant-rate process. The similarities between marine Ba and silicon distributions are primarily driven by ocean circulation rather than biological uptake or similarities in the remineralization length scales of barite and opal. Furthermore, our model predicts significant spatial variability in barium-to-organic matter ratios of sinking particulates, challenging the use of Ba as a quantitative proxy for export productivity. Overall, this study provides new insights into the modern marine Ba cycle, highlighting the key role of pelagic barite in regulating dissolved Ba distributions and elucidating the processes that control barite formation and dissolution.
全球海洋钡循环的模拟及其对古海洋学代用物的影响
钡(Ba)丰度被广泛用作深海营养和有机碳输出的代表。然而,海洋钡循环的关键方面仍然存在重大的不确定性,包括钡的主要来源重晶石,重晶石形成和溶解的深度和速率,将溶解的钡和硅循环联系起来的机制,以及出口颗粒中钡与有机质比率的区域变异性。在此,我们将GEOTRACES的溶解钡观测数据与重晶石饱和状态模型相结合,并采用机制框架来约束控制溶解钡分布的主要生物地球化学过程。结果表明,海水而非有机质是中上层重晶石Ba的主要来源,90%的降水发生在900 m以上。大约三分之二的远洋重晶石溶解发生在水柱中,而其余的发生在海底。溶解速率似乎与环境饱和状态无关,当溶解被视为恒定速率过程时,模型数据拟合最佳。海洋钡和硅分布的相似性主要是由海洋环流驱动的,而不是由生物吸收或重晶石和蛋白石再矿化长度尺度的相似性驱动的。此外,我们的模型预测下沉颗粒物的钡与有机质比率存在显著的空间变异性,这对使用钡作为出口生产率的定量代表提出了挑战。总体而言,该研究为现代海洋钡旋回提供了新的认识,突出了远洋重晶石在调节溶解钡分布中的关键作用,阐明了控制重晶石形成和溶解的过程。
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来源期刊
Earth and Planetary Science Letters
Earth and Planetary Science Letters 地学-地球化学与地球物理
CiteScore
10.30
自引率
5.70%
发文量
475
审稿时长
2.8 months
期刊介绍: Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.
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