The Late Cryogenian Warm Interval, NE Svalbard:Chemostratigraphy and genesis
The Late Cryogenian Warm Interval (LCWI) refers to a non-glacial interval that separates presumed representatives of the Sturtian and Marinoan panglaciations. Its duration is poorly constrained radiometrically and its deposits are relatively poorly known in most geographic regions. This paper aims t...
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Online Access: | https://hdl.handle.net/1983/9580a092-5ce9-452d-82a9-13af3d9c3e4d https://research-information.bris.ac.uk/en/publications/9580a092-5ce9-452d-82a9-13af3d9c3e4d https://doi.org/10.1016/j.precamres.2016.05.013 https://research-information.bris.ac.uk/ws/files/80894131/Fairchild_et_al_2016.pdf |
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ftubristolcris:oai:research-information.bris.ac.uk:publications/9580a092-5ce9-452d-82a9-13af3d9c3e4d 2023-11-12T04:27:04+01:00 The Late Cryogenian Warm Interval, NE Svalbard:Chemostratigraphy and genesis Fairchild, Ian J. Bonnand, Pierre Davies, Tesni Fleming, Edward J. Grassineau, Nathalie Halverson, Galen P. Hambrey, Michael J. McMillan, Emily M. McKay, Elizabeth Parkinson, Ian J Stevenson, Carl T.E. 2016-08 application/pdf https://hdl.handle.net/1983/9580a092-5ce9-452d-82a9-13af3d9c3e4d https://research-information.bris.ac.uk/en/publications/9580a092-5ce9-452d-82a9-13af3d9c3e4d https://doi.org/10.1016/j.precamres.2016.05.013 https://research-information.bris.ac.uk/ws/files/80894131/Fairchild_et_al_2016.pdf eng eng info:eu-repo/semantics/openAccess Fairchild , I J , Bonnand , P , Davies , T , Fleming , E J , Grassineau , N , Halverson , G P , Hambrey , M J , McMillan , E M , McKay , E , Parkinson , I J & Stevenson , C T E 2016 , ' The Late Cryogenian Warm Interval, NE Svalbard : Chemostratigraphy and genesis ' , Precambrian Research , vol. 281 , pp. 128-154 . https://doi.org/10.1016/j.precamres.2016.05.013 Cryogenian Shale Rhythmic sedimentation Chemostratigraphy Orbital forcing Dolomite article 2016 ftubristolcris https://doi.org/10.1016/j.precamres.2016.05.013 2023-11-02T23:30:17Z The Late Cryogenian Warm Interval (LCWI) refers to a non-glacial interval that separates presumed representatives of the Sturtian and Marinoan panglaciations. Its duration is poorly constrained radiometrically and its deposits are relatively poorly known in most geographic regions. This paper aims to constrain the duration, palaeoenvironments and petrogenesis of such deposits in the classic region of NE Spitsbergen, Svalbard. The succession comprises a 200–205 m dolomitic shale (Macdonaldryggen Member, known as E3, of the Elbobreen Formation) overlain by oolitic dolomite Slangen Member (E4), 15–25 m thick, with limestone developed at top and base of E3 in the south of the area. The assumed age context of the succession has been confirmed by the presence of a typical Sturtian cap carbonate profile of negative to positive δ 13 C, and primary Sr isotope compositions of basal E3 limestones <0.7072 and of upper E3 limestones of 0.7076. At the base of E3, interstratification of cap carbonate with ice-rafted and redeposited glacial sediments occurs. Early diagenetic stabilization of carbonate mineralogy from a precursor, possibly ikaite, to calcite or dolomite is inferred. E3 is predominantly dolomitic silt-shale, with sub-millimetre lamination, lacking sand or current-related sedimentary structures. Thin fine laminae are partly pyritized and interpreted as microbial mats. Dolomite content is 25–50%, with δ 13 C values consistently around +4‰, a value attributed to buffering by dissolution of a precursor metastable carbonate phase. Local calcite cement associates with low δ 13 C values. The carbonates form silt-sized, chemically zoned rhombic crystals from an environment with dynamically changing Fe and Mn. Three-dimensional reconstructions of cm-scale disturbance structures indicate that they represent horizontally directed sock-like folds, developed by release of overpressure into thin surficial sediment overlying an early-cemented layer. A shoaling upwards unit near the top of E3 displays calcium sulphate ... Article in Journal/Newspaper Svalbard Spitsbergen University of Bristol: Bristol Research Svalbard Precambrian Research 281 128 154 |
institution |
Open Polar |
collection |
University of Bristol: Bristol Research |
op_collection_id |
ftubristolcris |
language |
English |
topic |
Cryogenian Shale Rhythmic sedimentation Chemostratigraphy Orbital forcing Dolomite |
spellingShingle |
Cryogenian Shale Rhythmic sedimentation Chemostratigraphy Orbital forcing Dolomite Fairchild, Ian J. Bonnand, Pierre Davies, Tesni Fleming, Edward J. Grassineau, Nathalie Halverson, Galen P. Hambrey, Michael J. McMillan, Emily M. McKay, Elizabeth Parkinson, Ian J Stevenson, Carl T.E. The Late Cryogenian Warm Interval, NE Svalbard:Chemostratigraphy and genesis |
topic_facet |
Cryogenian Shale Rhythmic sedimentation Chemostratigraphy Orbital forcing Dolomite |
description |
The Late Cryogenian Warm Interval (LCWI) refers to a non-glacial interval that separates presumed representatives of the Sturtian and Marinoan panglaciations. Its duration is poorly constrained radiometrically and its deposits are relatively poorly known in most geographic regions. This paper aims to constrain the duration, palaeoenvironments and petrogenesis of such deposits in the classic region of NE Spitsbergen, Svalbard. The succession comprises a 200–205 m dolomitic shale (Macdonaldryggen Member, known as E3, of the Elbobreen Formation) overlain by oolitic dolomite Slangen Member (E4), 15–25 m thick, with limestone developed at top and base of E3 in the south of the area. The assumed age context of the succession has been confirmed by the presence of a typical Sturtian cap carbonate profile of negative to positive δ 13 C, and primary Sr isotope compositions of basal E3 limestones <0.7072 and of upper E3 limestones of 0.7076. At the base of E3, interstratification of cap carbonate with ice-rafted and redeposited glacial sediments occurs. Early diagenetic stabilization of carbonate mineralogy from a precursor, possibly ikaite, to calcite or dolomite is inferred. E3 is predominantly dolomitic silt-shale, with sub-millimetre lamination, lacking sand or current-related sedimentary structures. Thin fine laminae are partly pyritized and interpreted as microbial mats. Dolomite content is 25–50%, with δ 13 C values consistently around +4‰, a value attributed to buffering by dissolution of a precursor metastable carbonate phase. Local calcite cement associates with low δ 13 C values. The carbonates form silt-sized, chemically zoned rhombic crystals from an environment with dynamically changing Fe and Mn. Three-dimensional reconstructions of cm-scale disturbance structures indicate that they represent horizontally directed sock-like folds, developed by release of overpressure into thin surficial sediment overlying an early-cemented layer. A shoaling upwards unit near the top of E3 displays calcium sulphate ... |
format |
Article in Journal/Newspaper |
author |
Fairchild, Ian J. Bonnand, Pierre Davies, Tesni Fleming, Edward J. Grassineau, Nathalie Halverson, Galen P. Hambrey, Michael J. McMillan, Emily M. McKay, Elizabeth Parkinson, Ian J Stevenson, Carl T.E. |
author_facet |
Fairchild, Ian J. Bonnand, Pierre Davies, Tesni Fleming, Edward J. Grassineau, Nathalie Halverson, Galen P. Hambrey, Michael J. McMillan, Emily M. McKay, Elizabeth Parkinson, Ian J Stevenson, Carl T.E. |
author_sort |
Fairchild, Ian J. |
title |
The Late Cryogenian Warm Interval, NE Svalbard:Chemostratigraphy and genesis |
title_short |
The Late Cryogenian Warm Interval, NE Svalbard:Chemostratigraphy and genesis |
title_full |
The Late Cryogenian Warm Interval, NE Svalbard:Chemostratigraphy and genesis |
title_fullStr |
The Late Cryogenian Warm Interval, NE Svalbard:Chemostratigraphy and genesis |
title_full_unstemmed |
The Late Cryogenian Warm Interval, NE Svalbard:Chemostratigraphy and genesis |
title_sort |
late cryogenian warm interval, ne svalbard:chemostratigraphy and genesis |
publishDate |
2016 |
url |
https://hdl.handle.net/1983/9580a092-5ce9-452d-82a9-13af3d9c3e4d https://research-information.bris.ac.uk/en/publications/9580a092-5ce9-452d-82a9-13af3d9c3e4d https://doi.org/10.1016/j.precamres.2016.05.013 https://research-information.bris.ac.uk/ws/files/80894131/Fairchild_et_al_2016.pdf |
geographic |
Svalbard |
geographic_facet |
Svalbard |
genre |
Svalbard Spitsbergen |
genre_facet |
Svalbard Spitsbergen |
op_source |
Fairchild , I J , Bonnand , P , Davies , T , Fleming , E J , Grassineau , N , Halverson , G P , Hambrey , M J , McMillan , E M , McKay , E , Parkinson , I J & Stevenson , C T E 2016 , ' The Late Cryogenian Warm Interval, NE Svalbard : Chemostratigraphy and genesis ' , Precambrian Research , vol. 281 , pp. 128-154 . https://doi.org/10.1016/j.precamres.2016.05.013 |
op_rights |
info:eu-repo/semantics/openAccess |
op_doi |
https://doi.org/10.1016/j.precamres.2016.05.013 |
container_title |
Precambrian Research |
container_volume |
281 |
container_start_page |
128 |
op_container_end_page |
154 |
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1782340812901711872 |