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首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >Nd isotope systematics on ODP Sites 756 and 762 sediments reveal major volcanic, oceanic and climatic changes in South Indian Ocean over the last 35Ma
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Nd isotope systematics on ODP Sites 756 and 762 sediments reveal major volcanic, oceanic and climatic changes in South Indian Ocean over the last 35Ma

机译:ODP 756和762沉积物上的Nd同位素系统揭示了过去35Ma期间南印度洋的主要火山,海洋和气候变化

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摘要

We have analyzed the Nd isotopic composition of both ancient seawater and detrital material from long sequences of carbonated oozes of the South Indian Ocean which are ODP Site 756 (Ninety East Ridge (-30°S), 1518m water depth) and ODP Site 762 (Northwest Australian margin, 1360m water depth). The measurements indicate that the ε _(Nd) changes in Indian seawater over the last 35Ma result from changes in the oceanic circulation, large volcanic and continental weathering Nd inputs. This highlights the diverse nature of those controls and their interconnections in a small area of the ocean.These new records combined with those previously obtained at the equatorial ODP Sites 757 and 707 in the Indian Ocean (Gourlan et al., 2008) established that the distribution of intermediate seawater ε Nd was uniform over most of the Indian Ocean from 35Ma to 10Ma within a geographical area extending from 40°S to the equator and from -60°E to 120°E. However, the ε Nd value of Indian Ocean seawater which kept an almost constant value (at about -7 to -8) from 35 to 15Ma rose by 3 ε _(Nd) units from 15 to 10Ma. This sharp increase has been caused by a radiogenic Nd enrichment of the water mass originating from the Pacific flowing through the Indonesian Passage. Using a two end-members model we calculated that the Nd transported to the Indian Ocean through the Indonesian Pathway was 1.7 times larger at 10Ma than at 15Ma.The Nd isotopic composition of ancient seawater and that of the sediment detrital component appear to be strongly correlated for some specific events. A first evidence occurs between 20 and 15Ma with two positive spikes recorded in both ε Nd signals that are clearly induced by a volcanic crisis of, most likely, the St. Paul hot-spot. A second evidence is the very large ε _(Nd) decrease recorded at ODP Sites 756 and 762 during the past 10Ma which has never been previously observed. The synchronism between the ε Nd decrease in seawater from 10 to 5Ma and evidences of desertification in the western part of the nearly Australian continent suggests enhanced weathering inputs in this ocean from this continent as a result of climatic changes.
机译:我们分析了南印度洋长序列的碳酸盐软泥中的古海水和碎屑物质的Nd同位素组成,这些序列是ODP站点756(九十东岭(-30°S),水深1518m)和ODP站点762(澳大利亚西北边缘,水深1360m)。测量结果表明,印度洋在最后35Ma的ε_(Nd)变化是由于海洋环流,大火山和大陆风化Nd输入的变化造成的。这些新记录与先前在印度洋赤道ODP站点757和707获得的记录相结合(Gourlan et al。,2008),证实了这些控制的多样性和它们在海洋的一小部分之间的相互联系。在从40°S到赤道和从-60°E到120°E的地理区域内,印度洋大部分地区从35Ma到10Ma的中间海水εNd分布是均匀的。然而,从35Ma到15Ma几乎保持恒定值(约-7到-8)的印度洋海水的εNd值从15Ma到10Ma上升了3ε_(Nd)单位。这种急剧增加是由于放射状的Nd富集来自太平洋流经印度尼西亚通道的水团。使用两个末端成员模型,我们计算出了通过印度尼西亚途径运往印度洋的Nd在10Ma时是在15Ma时的1.7倍。古代海水的Nd同位素组成与沉积物碎屑成分似乎密切相关。对于某些特定事件。第一个证据出现在20Ma和15Ma之间,两个εNd信号中都记录了两个正尖峰,这显然是由最有可能是圣保罗热点的火山危机引起的。第二个证据是在过去10Ma内在ODP站点756和762处记录到的非常大的ε_(Nd)下降,这是以前从未观察到的。海水中的εNd从10Ma下降到5Ma的同步性和近澳大利亚大陆西部的沙漠化迹象表明,由于气候变化,该大陆对该海洋的风化投入增加。

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