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Neogene turbidite sequence on the Madeira Abyssal Plain: Basin filling and diagenesis in the deep ocean

Neogene turbidite sequence on the Madeira Abyssal Plain: Basin filling and diagenesis in the deep ocean
Neogene turbidite sequence on the Madeira Abyssal Plain: Basin filling and diagenesis in the deep ocean
The Madeira Abyssal Plain (MAP) has been formed by the accumulation of turbidite sediments from three principal sources: the northwest African continental margin, the Canary Islands and the Hyères/Cruiser/Great Meteor seamount chain. Turbidites derived from each of these sources have distinct chemical signatures enabling the development of a high-resolution chemostratigraphy, in addition to the conventional bio- and lithostratigraphies. Individual beds can be up to a few meters thick, and many are traceable across the whole plain. The first turbidites rapidly infilled the fracture zone valleys through the middle Miocene. By 16 Ma, the fracture zones were nearly filled, and flows began to spread across wider areas to form the plain. Between 16 and 13 Ma, individual flows became much larger, so that after this time, correlation of individual beds is possible between Sites 950, 951, and 952, which are spaced 50–60 km apart. Accumulation rates of the three principal groups of turbidites increased between 7 and 6.5 Ma, and remain high to the present day. One subgroup, termed "gray nonvolcanic turbidites," show a pulsed input to the plain, which may be related to the early growth phases of individual Canary Islands. The pelagic interbeds are composed of clay through the Eocene to middle Miocene, but at 8 Ma, they show a small increase in carbonate content. This increases again at ~5 Ma, and at 3.5 Ma, the carbonate began to oscillate between clays and oozes, reflecting the Pliocene–Quaternary climatic fluctuations.

Diagenesis of MAP Miocene–Holocene sediments is dominated by oxic processes that occurred when organic-rich turbidites were first emplaced on the plain. Diffusion of seawater oxygen into the upper few decimeters of turbidite tops and over time periods of a few thousand years caused the near-complete destruction of labile organic matter in the sediment, and promoted the early diagenetic migration of trace metals around a sharply defined redox interface. Pore-water data demonstrate that subsequent burial to depths of >350 meters below seafloor, and for time periods in excess of 10 m.y., has led to the progressive development of post-oxic, sulfate-reducing, and methanogenic environments, but these have had remarkably little effect on bulk sediment composition, trace-metal distributions, or organic-matter geochemistry. Oxygen availability appears to be an overriding control on diagenetic processes and rates during early burial in these pelagic environments.
619-634
Texas A&M University Ocean Drilling Program
Weaver, P.P.E.
1ab10035-6132-46aa-8a5c-6fb23a1b8ab4
Jarvis, I.
695bdaeb-0e98-4e86-b203-b27caaf845ab
Lebreiro, S.M.
78293150-2273-4880-8e05-915756304f99
Alibés, B.
80494289-9640-4951-a824-a5f1184e417e
Baraza, J.
c3b21132-79e5-4887-a0fa-67b4a591e121
Howe, R.
b74151a4-42d8-49de-b2f0-3bf32b22f3c9
Rothwell, R.G.
fe473057-bf44-46d1-8add-88060037beb5
Weaver, P.P.E.
Schminke, H.-U.
Firth, J.V.
Duffield, W.
Weaver, P.P.E.
1ab10035-6132-46aa-8a5c-6fb23a1b8ab4
Jarvis, I.
695bdaeb-0e98-4e86-b203-b27caaf845ab
Lebreiro, S.M.
78293150-2273-4880-8e05-915756304f99
Alibés, B.
80494289-9640-4951-a824-a5f1184e417e
Baraza, J.
c3b21132-79e5-4887-a0fa-67b4a591e121
Howe, R.
b74151a4-42d8-49de-b2f0-3bf32b22f3c9
Rothwell, R.G.
fe473057-bf44-46d1-8add-88060037beb5
Weaver, P.P.E.
Schminke, H.-U.
Firth, J.V.
Duffield, W.

Weaver, P.P.E., Jarvis, I., Lebreiro, S.M., Alibés, B., Baraza, J., Howe, R. and Rothwell, R.G. (1998) Neogene turbidite sequence on the Madeira Abyssal Plain: Basin filling and diagenesis in the deep ocean. Weaver, P.P.E., Schminke, H.-U., Firth, J.V. and Duffield, W. (eds.) In Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 157. Texas A&M University Ocean Drilling Program. pp. 619-634 . (doi:10.2973/odp.proc.sr.157.136.1998).

Record type: Conference or Workshop Item (Paper)

Abstract

The Madeira Abyssal Plain (MAP) has been formed by the accumulation of turbidite sediments from three principal sources: the northwest African continental margin, the Canary Islands and the Hyères/Cruiser/Great Meteor seamount chain. Turbidites derived from each of these sources have distinct chemical signatures enabling the development of a high-resolution chemostratigraphy, in addition to the conventional bio- and lithostratigraphies. Individual beds can be up to a few meters thick, and many are traceable across the whole plain. The first turbidites rapidly infilled the fracture zone valleys through the middle Miocene. By 16 Ma, the fracture zones were nearly filled, and flows began to spread across wider areas to form the plain. Between 16 and 13 Ma, individual flows became much larger, so that after this time, correlation of individual beds is possible between Sites 950, 951, and 952, which are spaced 50–60 km apart. Accumulation rates of the three principal groups of turbidites increased between 7 and 6.5 Ma, and remain high to the present day. One subgroup, termed "gray nonvolcanic turbidites," show a pulsed input to the plain, which may be related to the early growth phases of individual Canary Islands. The pelagic interbeds are composed of clay through the Eocene to middle Miocene, but at 8 Ma, they show a small increase in carbonate content. This increases again at ~5 Ma, and at 3.5 Ma, the carbonate began to oscillate between clays and oozes, reflecting the Pliocene–Quaternary climatic fluctuations.

Diagenesis of MAP Miocene–Holocene sediments is dominated by oxic processes that occurred when organic-rich turbidites were first emplaced on the plain. Diffusion of seawater oxygen into the upper few decimeters of turbidite tops and over time periods of a few thousand years caused the near-complete destruction of labile organic matter in the sediment, and promoted the early diagenetic migration of trace metals around a sharply defined redox interface. Pore-water data demonstrate that subsequent burial to depths of >350 meters below seafloor, and for time periods in excess of 10 m.y., has led to the progressive development of post-oxic, sulfate-reducing, and methanogenic environments, but these have had remarkably little effect on bulk sediment composition, trace-metal distributions, or organic-matter geochemistry. Oxygen availability appears to be an overriding control on diagenetic processes and rates during early burial in these pelagic environments.

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Published date: 1998
Organisations: Marine Geoscience

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Local EPrints ID: 355615
URI: http://eprints.soton.ac.uk/id/eprint/355615
PURE UUID: 3c6a3fe2-7d1d-43c9-bbde-8a8e69cc15fe

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Date deposited: 08 Aug 2013 15:35
Last modified: 14 Mar 2024 14:35

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Contributors

Author: P.P.E. Weaver
Author: I. Jarvis
Author: S.M. Lebreiro
Author: B. Alibés
Author: J. Baraza
Author: R. Howe
Author: R.G. Rothwell
Editor: P.P.E. Weaver
Editor: H.-U. Schminke
Editor: J.V. Firth
Editor: W. Duffield

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