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深层岩芯沉积物有机质中生物早期成岩作用和太阳辐射驱动的古生产力标志。

Biological early diagenesis and insolation-paced paleoproductivity signified in deep core sediment organic matter.

机构信息

Department of Environment & Energy, Sejong University, Seoul, 05006, South Korea.

Petroleum and Marine Research Division, Korea Institute of Geoscience and Mineral Resources, 124 Gwahang-no, Yuseong-gu, Daejeon, 34132, South Korea.

出版信息

Sci Rep. 2017 May 8;7(1):1581. doi: 10.1038/s41598-017-01759-4.

Abstract

The dynamics of a large stock of organic matter contained in deep sediments of marginal seas plays pivotal role in global carbon cycle, yet it is poorly constrained. Here, dissolved organic matter (DOM) in sediments was investigated for core sediment up to ~240 meters deep in the East/Japan Sea. The upper downcore profile (≤118 mbsf, or meters below seafloor) at a non-chimney site (U1) featured the exponential production of dissolved organic carbon (DOC) and optically active DOM with time in the pore water above sulfate-methane-transition-zone (SMTZ), concurrent with the increases of nutrients and alkalinity, and the reduction of sulfate. Such depth profiles signify a biological pathway of the DOM production during the early diagenesis of particulate organic matter presumably dominated by sulfate reduction. Below the SMTZ, an insolation-paced oscillation of DOM in a ~405-Kyr cycle of orbital eccentricity was observed at site U1, implying astronomically paced paleoproductivity stimulated by light availability. Furthermore, DOM dynamics of the deep sediments were likely governed by intensive humification as revealed by the less pronounced protein-like fluorescence and the lower H/C and O/C ratios below SMTZ among 15,281 formulas identified. Our findings here provide novel insights into organic matter dynamics in deep sediments.

摘要

深海边缘海沉积物中大量有机质的动态在全球碳循环中起着关键作用,但目前对此了解甚少。本研究调查了东海/日本海约 240 米深的沉积物中的溶解有机质 (DOM)。在非烟囱站点 (U1) 的沉积物中,从地表以下约 118 米深的上剖面 (mbsf,或米深海底以下) 的孔隙水中,溶解有机碳 (DOC) 和具有光活性的 DOM 随时间呈指数增长,伴随着营养物质和碱度的增加以及硫酸盐的减少。这种深度剖面表明,在颗粒有机物质的早期成岩作用中,DOM 的产生可能主要由硫酸盐还原作用主导的生物途径。在 SMTZ 以下,在 U1 站点观察到 DOM 以约 405 千周期的轨道偏心率为节奏的光周期波动,暗示由光照可用性驱动的天文节奏古生产力。此外,在 SMTZ 以下,通过较少的蛋白质样荧光以及在 15281 个公式中确定的较低的 H/C 和 O/C 比,表明强烈的腐殖化作用可能控制了深部沉积物中的 DOM 动态。本研究结果为深入了解深部沉积物中的有机质动态提供了新的见解。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/9cec/5431472/73886e099dd0/41598_2017_1759_Fig1_HTML.jpg

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