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Petrogenesis of the Swartruggens and Star Group II kimberlite dyke swarms, South Africa

Bibliography: leaves 139-146.

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Bibliographic Details
Main Author: Coe, Nancy
Other Authors: Le Roex, Anton
Format: Thesis
Language:English
Published: Department of Geological Sciences 2014
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access_status_str Open Access
author Coe, Nancy
author2 Le Roex, Anton
author_browse Coe, Nancy
Le Roex, Anton
author_facet Le Roex, Anton
Coe, Nancy
author_sort Coe, Nancy
collection Thesis
description Bibliography: leaves 139-146.
format Thesis
id oai:open.uct.ac.za:11427/4191
institution University of Cape Town (South Africa)
language eng
last_indexed 2026-06-10T12:40:25.483Z
license_str Not specified — see source repository
provenance_str_mv Harvested via OAI-PMH from UCTD — University of Cape Town Open Access Repository
publishDate 2014
publishDateRange 2014
publishDateSort 2014
publisher Department of Geological Sciences
publisherStr Department of Geological Sciences
record_format dspace
source_str UCTD — University of Cape Town Open Access Repository
spelling oai:open.uct.ac.za:11427/4191 Petrogenesis of the Swartruggens and Star Group II kimberlite dyke swarms, South Africa Coe, Nancy Le Roex, Anton Gurney, John J Geological Sciences Bibliography: leaves 139-146. The Swartruggens (156 Ma) and Star (128 Ma) kimberlites are two Group II, diamondiferous, hypabyssal kimerlite dyke swarms, situated in the Northern Province and the Free State respectively, South Africa. Representative samples from all dykes exposed in the mining operations, the Main and Changhouse Dykes, South Fissure and the barren Muil Dyke at Swartruggens, and the Wynandsfontein, East Star, Clewer, Byrnes and Barren dykes at Star, have been analysed for their major and trace element contents and Sr, Nd and Hf isotope compositions. Primary kimberlite magma chemistry is subjected to considerable modification due to the incorporation of both mantle and crustal material during ascent to the surface, crystal fractionation, and post-emplacement alteration by deuteric fluids. This study aims to constrain the effects of these processes, and thus to identify least-modified, close-to-primary, parental magma compositions, with the view to understanding the source region characteristics of, and the petrogenetic processes giving rise to, these kimberlites. 2014-07-30T17:25:27Z 2014-07-30T17:25:27Z 2004 Master Thesis Masters MSc http://hdl.handle.net/11427/4191 eng application/pdf Department of Geological Sciences Faculty of Science University of Cape Town
spellingShingle Geological Sciences
Coe, Nancy
Petrogenesis of the Swartruggens and Star Group II kimberlite dyke swarms, South Africa
thesis_degree_str Master's
title Petrogenesis of the Swartruggens and Star Group II kimberlite dyke swarms, South Africa
title_full Petrogenesis of the Swartruggens and Star Group II kimberlite dyke swarms, South Africa
title_fullStr Petrogenesis of the Swartruggens and Star Group II kimberlite dyke swarms, South Africa
title_full_unstemmed Petrogenesis of the Swartruggens and Star Group II kimberlite dyke swarms, South Africa
title_short Petrogenesis of the Swartruggens and Star Group II kimberlite dyke swarms, South Africa
title_sort petrogenesis of the swartruggens and star group ii kimberlite dyke swarms south africa
topic Geological Sciences
url http://hdl.handle.net/11427/4191
work_keys_str_mv AT coenancy petrogenesisoftheswartruggensandstargroupiikimberlitedykeswarmssouthafrica