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Fluid flow through carbonate platforms: constraints from U-234/U-238 and Cl- in Bahamas pore-waters

Abstract:
The geometry, timing, and rate of fluid-flow through carbonate margins and platforms is not well constrained. In this study, we use U concentrations and isotope ratios measured on small volumes of pore-water from Bahamas slope sediment, coupled with existing chlorinity data, to place constraints on the fluid-flow in this region and, by implication, other carbonate platforms. These data also allow an assessment of the behaviour of U isotopes in an unusually well constrained water-rock system. We report pore-water U concentrations which are controlled by dissolution of high-U organic material at shallow depths in the sediment and by reduction of U to its insoluble 4+ state at greater depths. The dominant process influencing pore-water (234U/238U) is alpha recoil. In Holocene sediments, the increase of pore-water (234U/238U) due to recoil provides an estimate of the horizontal flow rate of 11 cm/year, but with considerable uncertainty. At depths in the sediment where conditions are reducing, features in the U concentration and (234U/238U) profiles are offset from one another which constrains the effective diffusivity for U in these sediments to be ~1-2 x 10-8 cm2 s-1. At depths between the Holocene and these reducing sediments, pore-water (234U/238U) values are unusually low due to a recent increase in the dissolution rate of grain surfaces. This suggests a strengthening of fluid flow, probably due to the flooding of the banks at the last deglaciation and the re-initiation of thermally-driven venting of fluid on the bank top and accompanying recharge on the slopes. Interpretation of existing chlorinity data, in the light of this change in flow rate, constrain the recent horizontal flow rate to be 10.6 (±3.4) cm/year. Estimates of flow rate from (234U/238U) and C1- are therefore in agreement and suggest flow rates close to those predicted by thermally-driven models of fluid flow. This agreement supports the idea that flow within the Bahamas Banks is mostly thermally driven and suggests that flow rates on the order of 10 cm/year are typical for carbonate platforms where such flow occurs.
Publication status:
Published

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Publisher copy:
10.1016/S0012-821X(99)00065-5

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Institution:
University of Oxford
Division:
MPLS
Department:
Earth Sciences
Role:
Author


Journal:
EARTH AND PLANETARY SCIENCE LETTERS More from this journal
Volume:
169
Issue:
1-2
Pages:
99-111
Publication date:
1999-05-30
DOI:
ISSN:
0012-821X


Language:
English
Keywords:
Pubs id:
pubs:102800
UUID:
uuid:0a5b8d49-85e7-4a63-8868-27e1f6923cd5
Local pid:
pubs:102800
Source identifiers:
102800
Deposit date:
2012-12-19
ARK identifier:

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