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Tracing fluid–rock reaction and hydrothermal circulation at the Saldanha hydrothermal field

Tracing fluid–rock reaction and hydrothermal circulation at the Saldanha hydrothermal field
Tracing fluid–rock reaction and hydrothermal circulation at the Saldanha hydrothermal field
The Saldanha hydrothermal field is positioned on the top of a seamount located in a non-transformoffset (NTO5)
on the Mid-Atlantic Ridge (MAR). This hydrothermal system was first described as a low-temperature diffuse field, driven by peridotite–seawater reactions following the detection of high concentrations of CH4 and H2 in the
water column, and the occurrence of serpentinite outcrops in the vent area. We have studied the geochemistry and isotopic composition of sediment and rock samples collected across the area and show that hydrothermal
circulation at Saldanha is complex and spatially variable, comprising areas of low-temperature diffuse flow but also more focused higher-temperature venting zones. While most sediment samples have an isotopic composition that is similar to normal pelagic sediments, one core (SCD7) show significant hydrothermal influence, sulphide mineralization, non-radiogenic Pb and radiogenicNdisotope ratios and positive Eu anomalies. This is best explained by mineral precipitation from high-temperature hydrothermal fluids that have circulated through mafic rocks. The host rock lithology and alteration is also highly variable and comprises both fresh basalts, serpentinites and hydrothermally altered rocks (metabasalts, metagabbros and steatites). Serpentinites
have REE patterns and ?Nd(0) values that fall between seawater and mantle peridotite reference values, resulting
from extensive interaction of seawater with the original peridotite. This process was probably favoured by the deeply penetrating and long-lived faults occurring at this NTO. Steatites have a positive Eu anomaly and nonradiogenic
Pb isotopic values. These signatures, together with the sulphide mineralisation and the extensive Si input necessary for steatization of serpentinites, imply that higher-temperature hydrothermal fluids reacted with
gabbroic intrusions at depth. The more hydrothermally altered sediment and rock samples appear to be associated with the Saldanha fault network that promotes a more focused fluid flow and thus enhances hydrothermal alteration within a region of low-temperature diffuse flow.
0009-2541
168-179
Dias, A.S.
49ec581c-be39-447d-96d8-e589a157000a
Mills, R.A.
a664f299-1a34-4b63-9988-1e599b756706
Ribeiro da Costa, I.
48534ab8-8b09-4a19-927c-9252e71e3bb5
Costa, R.
008b752b-177f-4437-8bbc-f8b4d429a35f
Taylor, R.N.
094be7fd-ef61-4acd-a795-7daba2bc6183
Cooper, M.J.
54f7bff0-1f8c-4835-8358-71eef8529e7a
Barriga, F.J.A.S.
63134db0-7768-4f9f-8eb3-f851887d72ba
Dias, A.S.
49ec581c-be39-447d-96d8-e589a157000a
Mills, R.A.
a664f299-1a34-4b63-9988-1e599b756706
Ribeiro da Costa, I.
48534ab8-8b09-4a19-927c-9252e71e3bb5
Costa, R.
008b752b-177f-4437-8bbc-f8b4d429a35f
Taylor, R.N.
094be7fd-ef61-4acd-a795-7daba2bc6183
Cooper, M.J.
54f7bff0-1f8c-4835-8358-71eef8529e7a
Barriga, F.J.A.S.
63134db0-7768-4f9f-8eb3-f851887d72ba

Dias, A.S., Mills, R.A., Ribeiro da Costa, I., Costa, R., Taylor, R.N., Cooper, M.J. and Barriga, F.J.A.S. (2010) Tracing fluid–rock reaction and hydrothermal circulation at the Saldanha hydrothermal field. Chemical Geology, 273 (3-4), 168-179. (doi:10.1016/j.chemgeo.2010.02.020).

Record type: Article

Abstract

The Saldanha hydrothermal field is positioned on the top of a seamount located in a non-transformoffset (NTO5)
on the Mid-Atlantic Ridge (MAR). This hydrothermal system was first described as a low-temperature diffuse field, driven by peridotite–seawater reactions following the detection of high concentrations of CH4 and H2 in the
water column, and the occurrence of serpentinite outcrops in the vent area. We have studied the geochemistry and isotopic composition of sediment and rock samples collected across the area and show that hydrothermal
circulation at Saldanha is complex and spatially variable, comprising areas of low-temperature diffuse flow but also more focused higher-temperature venting zones. While most sediment samples have an isotopic composition that is similar to normal pelagic sediments, one core (SCD7) show significant hydrothermal influence, sulphide mineralization, non-radiogenic Pb and radiogenicNdisotope ratios and positive Eu anomalies. This is best explained by mineral precipitation from high-temperature hydrothermal fluids that have circulated through mafic rocks. The host rock lithology and alteration is also highly variable and comprises both fresh basalts, serpentinites and hydrothermally altered rocks (metabasalts, metagabbros and steatites). Serpentinites
have REE patterns and ?Nd(0) values that fall between seawater and mantle peridotite reference values, resulting
from extensive interaction of seawater with the original peridotite. This process was probably favoured by the deeply penetrating and long-lived faults occurring at this NTO. Steatites have a positive Eu anomaly and nonradiogenic
Pb isotopic values. These signatures, together with the sulphide mineralisation and the extensive Si input necessary for steatization of serpentinites, imply that higher-temperature hydrothermal fluids reacted with
gabbroic intrusions at depth. The more hydrothermally altered sediment and rock samples appear to be associated with the Saldanha fault network that promotes a more focused fluid flow and thus enhances hydrothermal alteration within a region of low-temperature diffuse flow.

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Published date: 15 May 2010

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Local EPrints ID: 148835
URI: http://eprints.soton.ac.uk/id/eprint/148835
ISSN: 0009-2541
PURE UUID: c4dbf634-7e84-4047-9a03-296398b1654d
ORCID for R.A. Mills: ORCID iD orcid.org/0000-0002-9811-246X
ORCID for R.N. Taylor: ORCID iD orcid.org/0000-0002-9367-0294
ORCID for M.J. Cooper: ORCID iD orcid.org/0000-0002-2130-2759

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Date deposited: 29 Apr 2010 08:02
Last modified: 14 Mar 2024 02:45

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Contributors

Author: A.S. Dias
Author: R.A. Mills ORCID iD
Author: I. Ribeiro da Costa
Author: R. Costa
Author: R.N. Taylor ORCID iD
Author: M.J. Cooper ORCID iD
Author: F.J.A.S. Barriga

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