Sandstone-hosted concretionary cements of the Hebrides, Scotland

The geometries of the sandstone-hosted calcite concretions of the Jurassic Valtos Sandstone Formation and Bearreraig Sandstone Formation are described and related to the processes operating during concretion growth. As concretionary bodies analogous to those studied form potential permeability barri...

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Main Author: Wilkinson, Mark
Published: University of Leicester 1989
Subjects:
551
Online Access:http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.256289
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spelling ndltd-bl.uk-oai-ethos.bl.uk-2562892018-04-04T03:29:54ZSandstone-hosted concretionary cements of the Hebrides, ScotlandWilkinson, Mark1989The geometries of the sandstone-hosted calcite concretions of the Jurassic Valtos Sandstone Formation and Bearreraig Sandstone Formation are described and related to the processes operating during concretion growth. As concretionary bodies analogous to those studied form potential permeability barriers within some North Sea petroleum reservoirs; the relationship between the growth processes and permeability barrier formation is examined. The growth times for model spherical concretions are calculated for the complex carbonate-water system. Two growth processes are modelled, solute transport and surface reaction. Growth times for a 1m diameter concretion forming under geologically reasonable conditions are predicted to be 22.3Ma, which reduces to 8.8Ma in porewaters flowing at 1m/year. The depth of formation of the concretions is assessed, through an examination of depth dependent properties of both the host-sediment and the calcite cement, and is found to be less than 500m. Concretion formation preceeded the Paleocene igneous activity which affected the Hebrides. The majority of the concretions examined formed at burial depths which were too great to allow effective contact between the concretions and seawater. The major source of carbonate was the dissolution of aragonitic shell material from within the host sandbody. The nature of the porewaters from which the concretions formed is assessed. The majority were meteoric in origin, though some marine influence is noted. The minor element contents of the cements cannot be used to calculate porewater compositions, as disequilibrium between the porewaters and the cements can be demonstrated. A model is proposed to account for the minor element patterns. Crystal breeding can be demonstrated to have occurred during concretion growth. A hypothesis is presented to explain the petrographic features of a typical Valtos Sandstone Formation concretion.551Permeability barrier/North SeaUniversity of Leicesterhttp://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.256289http://hdl.handle.net/2381/34983Electronic Thesis or Dissertation
collection NDLTD
sources NDLTD
topic 551
Permeability barrier/North Sea
spellingShingle 551
Permeability barrier/North Sea
Wilkinson, Mark
Sandstone-hosted concretionary cements of the Hebrides, Scotland
description The geometries of the sandstone-hosted calcite concretions of the Jurassic Valtos Sandstone Formation and Bearreraig Sandstone Formation are described and related to the processes operating during concretion growth. As concretionary bodies analogous to those studied form potential permeability barriers within some North Sea petroleum reservoirs; the relationship between the growth processes and permeability barrier formation is examined. The growth times for model spherical concretions are calculated for the complex carbonate-water system. Two growth processes are modelled, solute transport and surface reaction. Growth times for a 1m diameter concretion forming under geologically reasonable conditions are predicted to be 22.3Ma, which reduces to 8.8Ma in porewaters flowing at 1m/year. The depth of formation of the concretions is assessed, through an examination of depth dependent properties of both the host-sediment and the calcite cement, and is found to be less than 500m. Concretion formation preceeded the Paleocene igneous activity which affected the Hebrides. The majority of the concretions examined formed at burial depths which were too great to allow effective contact between the concretions and seawater. The major source of carbonate was the dissolution of aragonitic shell material from within the host sandbody. The nature of the porewaters from which the concretions formed is assessed. The majority were meteoric in origin, though some marine influence is noted. The minor element contents of the cements cannot be used to calculate porewater compositions, as disequilibrium between the porewaters and the cements can be demonstrated. A model is proposed to account for the minor element patterns. Crystal breeding can be demonstrated to have occurred during concretion growth. A hypothesis is presented to explain the petrographic features of a typical Valtos Sandstone Formation concretion.
author Wilkinson, Mark
author_facet Wilkinson, Mark
author_sort Wilkinson, Mark
title Sandstone-hosted concretionary cements of the Hebrides, Scotland
title_short Sandstone-hosted concretionary cements of the Hebrides, Scotland
title_full Sandstone-hosted concretionary cements of the Hebrides, Scotland
title_fullStr Sandstone-hosted concretionary cements of the Hebrides, Scotland
title_full_unstemmed Sandstone-hosted concretionary cements of the Hebrides, Scotland
title_sort sandstone-hosted concretionary cements of the hebrides, scotland
publisher University of Leicester
publishDate 1989
url http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.256289
work_keys_str_mv AT wilkinsonmark sandstonehostedconcretionarycementsofthehebridesscotland
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