晚白垩世赤道大西洋构造对氮循环和海洋通气动力学的控制

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Yong Du , Huyue Song , Thomas J. Algeo , Lei Zhong , Jing Li , Haijun Song
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引用次数: 0

摘要

晚白垩世赤道大西洋门户(EAG)的打开从根本上重塑了海洋环流和生物地球化学循环。广泛的研究集中在Cenomanian-Turonian Oceanic Anoxic Event (OAE-2)期间的氮动力学,表明氨主导条件下全球氮同位素(δ15N)值(<0‰)降低。然而,在EAG逐渐加深和扩大的过程中,oae -2后氮循环的演变仍然是一个谜。本文基于ODP站点1258(西赤道大西洋)新生成的体沉积物δ15N,结合其他Demerara隆起站点的现有数据,研究了晚白垩世至早大年(~ 102-65 Ma)赤道大西洋的营养循环和古海洋条件的变化。我们的数据揭示了与东洋构造发育直接相关的两阶段氮循环转变。第一阶段记录于塞诺曼—三东期富有机质沉积物(第四单元),δ15N值较低(约为- 2‰),反映了有限海洋环境下氨主导的氮循环。异常高的总有机碳(TOC)含量(5 - 15%)和Corg/N比值(>30)表明营养陷阱内的铵循环强烈,这导致了在缺氧条件下的高生产力和有效的有机质保存。第二阶段为坎帕尼亚—马斯特里赫特期δ15N由+4‰逐渐增加到+9‰,标志着深水通风增强和氧最小带扩大的部分反硝化作用驱动的硝酸盐主导的氮循环。这种变化与TOC(0.08 - 0.25%)和cog /N比率(<5)的下降相关,表明EAG打开后,养分保留减弱,区域垂直混合增强。观测到的氮循环重组与一个关键的构造阈值有关(Δlat >;6.1±0.1°和Δlong >;13.9±1.5°(即赤道大西洋纵向和纬度的累积裂谷扩展)源于板块重建,超过此范围,持续的深水环流启动了深海通风。我们的研究结果表明,东洋期的构造节奏是新生大西洋向硝酸盐主导的氮循环基本转变的关键驱动力,解决了oae -2后氮循环演化的长期谜题,并将晚白垩世深海氧合作用与现代omz驱动的氮循环的出现建立了机制联系。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Tectonic controls on nitrogen cycling and ocean ventilation dynamics in the Late Cretaceous equatorial Atlantic
The Late Cretaceous opening of the Equatorial Atlantic Gateway (EAG) fundamentally reshaped oceanic circulation and biogeochemical cycles. Extensive studies have focused on nitrogen dynamics during the Cenomanian-Turonian Oceanic Anoxic Event (OAE-2), showing globally reduced nitrogen isotope (δ15N) values (<0 ‰) under ammonium-dominated conditions. However, the post-OAE-2 evolution of nitrogen cycling during the progressive deepening and widening of the EAG remains enigmatic. Here, we investigate changes in nutrient cycling and paleoceanographic conditions in the equatorial Atlantic Ocean during the Late Cretaceous to early Danian (∼102–65 Ma) based on newly generated bulk-sediment δ15N from ODP Site 1258 (western equatorial Atlantic), integrated with existing data from other Demerara Rise sites. Our dataset reveals a two-phase nitrogen-cycle transition directly tied to EAG's tectonic development. The first phase, recorded in organic-rich sediments of Cenomanian-Santonian age (Unit IV), exhibit low δ15N values (ca. −2 ‰), reflecting an ammonium-dominated nitrogen cycle in a restricted oceanic environment. The exceptionally high total organic carbon (TOC) content (5–15 %) and Corg/N ratios (>30) indicate intense ammonium recycling within a nutrient trap, which led to high productivity and efficient organic matter preservation under euxinic conditions. The second phase is recorded by a stepwise increase of δ15N from +4 ‰ to +9 ‰ during the Campanian–Maastrichtian stages, marking the shift to a nitrate-dominated nitrogen cycle driven by enhanced deep-water ventilation and partial denitrification in expanding oxygen-minimum zones. This shift correlates with declining TOC (0.08–0.25 %) and Corg/N ratios (<5), indicating weakened nutrient retention and strengthened regional vertical mixing following opening of the EAG. The observed nitrogen-cycle reorganization correlates with a critical tectonic threshold (Δlat > 6.1 ± 0.1° and Δlong > 13.9 ± 1.5°, i.e., the cumulative latitudinal and longitudinal rift extension in the equatorial Atlantic) derived from plate reconstructions, beyond which sustained deep-water circulation initiated deep-ocean ventilation. Our findings establish the EAG’s tectonic pacing as the key driver of a fundamental transition to a nitrate-dominated nitrogen cycle in the nascent Atlantic Ocean, resolving the long-standing enigma of post-OAE-2 nitrogen-cycle evolution and mechanistically linking Late Cretaceous deep-ocean oxygenation to the emergence of modern OMZ-driven nitrogen cycling.
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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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