U–Pb baddeleyite geochronology and geochemistry of the White Mfolozi Dyke Swarm : unravelling the complexities of 2.70–2.66 Ga dyke swarms across the eastern Kaapvaal Craton, South Africa
(2016) In GFF 138(1). p.115-132- Abstract
On the south-easternmost Kaapvaal Craton, a NE-trending plagioclase-megacrystic dolerite dyke swarm, herein named the White Mfolozi Dyke Swarm (WMDS), has been identified. New U–Pb baddeleyite ages presented here indicate that the WMDS was emplaced within less than 10 million years, with our three most robust results yielding a weighted mean age of 2662 ± 2 Ma. The WMDS is coeval with the youngest dykes of a 2.70–2.66 Ga radiating dyke swarm already identified further north on the eastern side of the Kaapvaal Craton. This dyke swarm radiates out from the eastern lobe of the ca. 2.05 Ga Bushveld Complex. A clustering of ages from the WMDS and the 2.70–2.66 Ga radiating dyke swarm identify potential magmatic peaks at 2701–2692 Ma,... (More)
On the south-easternmost Kaapvaal Craton, a NE-trending plagioclase-megacrystic dolerite dyke swarm, herein named the White Mfolozi Dyke Swarm (WMDS), has been identified. New U–Pb baddeleyite ages presented here indicate that the WMDS was emplaced within less than 10 million years, with our three most robust results yielding a weighted mean age of 2662 ± 2 Ma. The WMDS is coeval with the youngest dykes of a 2.70–2.66 Ga radiating dyke swarm already identified further north on the eastern side of the Kaapvaal Craton. This dyke swarm radiates out from the eastern lobe of the ca. 2.05 Ga Bushveld Complex. A clustering of ages from the WMDS and the 2.70–2.66 Ga radiating dyke swarm identify potential magmatic peaks at 2701–2692 Ma, 2686–2683 Ma and 2665–2659 Ma. Geochemical signatures of the dykes do not correlate with these age groups, but are rather unique to specific areas. The northern part of the eastern Kaapvaal Craton hosts relatively differentiated 2.70–2.66 Ga dolerite dykes that could have been derived from a moderately enriched mantle source, whereas the ca. 2.66 Ga WMDS from the southernmost area exhibit much more depleted signatures. In between these two margins, the central area hosts more andesitic 2.70–2.66 Ga dykes that may have assimilated substantial amounts of partly digested tonalite–trondhjemite–granodiorite crust from the basement. We investigate the evolution for the Kaapvaal Craton during a highly magmatic period that extends for over 60 million years from extensive Ventersdorp volcanism to the eruption of proto-basinal volcanic rocks at the base of the Transvaal Supergroup.
(Less)
- author
- Gumsley, Ashley LU ; Rådman, Johan ; Söderlund, Ulf LU and Klausen, Martin
- organization
- publishing date
- 2016-01-02
- type
- Contribution to journal
- publication status
- published
- subject
- keywords
- geochemistry, Kaapvaal Craton, U–Pb baddeleyite geochronology, White Mfolozi Dyke Swarm
- in
- GFF
- volume
- 138
- issue
- 1
- pages
- 18 pages
- publisher
- Taylor & Francis
- external identifiers
-
- scopus:84959078836
- wos:000371812700009
- ISSN
- 1103-5897
- DOI
- 10.1080/11035897.2015.1122665
- project
- Validating the existence of the supercraton Vaalbara in the Mesoarchaean to Palaeoproterozoic
- language
- English
- LU publication?
- yes
- id
- dd0c926e-a8e7-499a-8ac4-29fb41e4e15c
- date added to LUP
- 2016-09-20 13:39:47
- date last changed
- 2024-02-02 23:48:29
@article{dd0c926e-a8e7-499a-8ac4-29fb41e4e15c,
abstract = {{<p>On the south-easternmost Kaapvaal Craton, a NE-trending plagioclase-megacrystic dolerite dyke swarm, herein named the White Mfolozi Dyke Swarm (WMDS), has been identified. New U–Pb baddeleyite ages presented here indicate that the WMDS was emplaced within less than 10 million years, with our three most robust results yielding a weighted mean age of 2662 ± 2 Ma. The WMDS is coeval with the youngest dykes of a 2.70–2.66 Ga radiating dyke swarm already identified further north on the eastern side of the Kaapvaal Craton. This dyke swarm radiates out from the eastern lobe of the ca. 2.05 Ga Bushveld Complex. A clustering of ages from the WMDS and the 2.70–2.66 Ga radiating dyke swarm identify potential magmatic peaks at 2701–2692 Ma, 2686–2683 Ma and 2665–2659 Ma. Geochemical signatures of the dykes do not correlate with these age groups, but are rather unique to specific areas. The northern part of the eastern Kaapvaal Craton hosts relatively differentiated 2.70–2.66 Ga dolerite dykes that could have been derived from a moderately enriched mantle source, whereas the ca. 2.66 Ga WMDS from the southernmost area exhibit much more depleted signatures. In between these two margins, the central area hosts more andesitic 2.70–2.66 Ga dykes that may have assimilated substantial amounts of partly digested tonalite–trondhjemite–granodiorite crust from the basement. We investigate the evolution for the Kaapvaal Craton during a highly magmatic period that extends for over 60 million years from extensive Ventersdorp volcanism to the eruption of proto-basinal volcanic rocks at the base of the Transvaal Supergroup.</p>}},
author = {{Gumsley, Ashley and Rådman, Johan and Söderlund, Ulf and Klausen, Martin}},
issn = {{1103-5897}},
keywords = {{geochemistry; Kaapvaal Craton; U–Pb baddeleyite geochronology; White Mfolozi Dyke Swarm}},
language = {{eng}},
month = {{01}},
number = {{1}},
pages = {{115--132}},
publisher = {{Taylor & Francis}},
series = {{GFF}},
title = {{U–Pb baddeleyite geochronology and geochemistry of the White Mfolozi Dyke Swarm : unravelling the complexities of 2.70–2.66 Ga dyke swarms across the eastern Kaapvaal Craton, South Africa}},
url = {{http://dx.doi.org/10.1080/11035897.2015.1122665}},
doi = {{10.1080/11035897.2015.1122665}},
volume = {{138}},
year = {{2016}},
}