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doi:10.1016/0016-7037(88)90068-3    
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Copyright © 1988 Published by Elsevier Ltd.

Article

Geochemistry of sediments on the Rio Grande Rise and the redox evolution of the South Atlantic Ocean

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X. Hu1, *, Y.L. Wang2 and R.A. Schmitt1

1Departments of Chemistry and Geology, the Radiation Center and the College of Oceanography, Oregon State University, Corvallis, OR 97331, U.S.A.

2Chengdu College of Geology, Shilidian, Chengdu, Sichuan 610059, People's Republic of China


Received 18 December 1986; 
accepted 26 October 1987. 
Available online 14 April 2003.

Abstract

Sediment samples (32) from DSDP Holes 516 and 516F, Leg 72 were subjected to INAA (instrumental neutron activation analysis). Thirty-two major, minor and trace elements were determined. Ce anomalies, CeA ≡ Ce (obs.)/Ce* (interpolated between La and Nd and relative to the N.A.S.C. (North American Shale Composite)) = Ce (obs.)/[1.44 La (obs.) + 0.66 Nd (obs.)], in the carbonate phase were obtained. Calculations indicate that the Ce anomaly changed from 0.80 (80 My), 0.68 (67 My) to 0.30 (56 My), 0.27 (39 My) and 0.12–0.43 (avg. 0.26) (15−0.3 My). The CeA change observed at not, vert, similar55 My coincides with the CeA change at not, vert, similar58 My in marine carbonates from the Walvis Ridge, Hole 525A. These changes are attributed to improved water circulation caused by either the widening of the north-south Atlantic passage, subsidence of the Rio Grande Rise or subsidence of the Romanche Fracture Zone. The ultimate driving force behind the CeA changes is related to the pH and PO2 of the seawater and also related to global circulation of bottom ocean water and transport of the external terrestrial input from riverine or/and aeolian sources.


* Present address: Institute for Radiation Protection, Taiyuan, Shanxi, People's Republic of China.

 
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