Yong Du , Huyue Song , Thomas J. Algeo , Lei Zhong , Jing Li , Haijun Song
{"title":"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","authors":"Yong Du , Huyue Song , Thomas J. Algeo , Lei Zhong , Jing Li , Haijun Song","doi":"10.1016/j.epsl.2025.119517","DOIUrl":null,"url":null,"abstract":"<div><div>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 (δ<sup>15</sup>N) 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 δ<sup>15</sup>N 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 δ<sup>15</sup>N 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 C<sub>org</sub>/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 δ<sup>15</sup>N 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 C<sub>org</sub>/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 (Δ<sub>lat</sub> > 6.1 ± 0.1° and Δ<sub>long</sub> > 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.</div></div>","PeriodicalId":11481,"journal":{"name":"Earth and Planetary Science Letters","volume":"667 ","pages":"Article 119517"},"PeriodicalIF":4.8000,"publicationDate":"2025-06-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Tectonic controls on nitrogen cycling and ocean ventilation dynamics in the Late Cretaceous equatorial Atlantic\",\"authors\":\"Yong Du , Huyue Song , Thomas J. Algeo , Lei Zhong , Jing Li , Haijun Song\",\"doi\":\"10.1016/j.epsl.2025.119517\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>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 (δ<sup>15</sup>N) 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 δ<sup>15</sup>N 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 δ<sup>15</sup>N 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 C<sub>org</sub>/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 δ<sup>15</sup>N 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 C<sub>org</sub>/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 (Δ<sub>lat</sub> > 6.1 ± 0.1° and Δ<sub>long</sub> > 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.</div></div>\",\"PeriodicalId\":11481,\"journal\":{\"name\":\"Earth and Planetary Science Letters\",\"volume\":\"667 \",\"pages\":\"Article 119517\"},\"PeriodicalIF\":4.8000,\"publicationDate\":\"2025-06-25\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Earth and Planetary Science Letters\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0012821X25003152\",\"RegionNum\":1,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"GEOCHEMISTRY & GEOPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Earth and Planetary Science Letters","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0012821X25003152","RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
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.
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.