Next Article in Journal
Fingerprinting Paranesti Rubies through Oxygen Isotopes
Next Article in Special Issue
Modeling the Crystallization and Emplacement Conditions of a Basaltic Trachyandesitic Sill at Mt. Etna Volcano
Previous Article in Journal
Gem-Quality Zircon Megacrysts from Placer Deposits in the Central Highlands, Vietnam—Potential Source and Links to Cenozoic Alkali Basalts
Previous Article in Special Issue
Impulsive Supply of Volatile-Rich Magmas in the Shallow Plumbing System of Mt. Etna Volcano
Article Menu
Issue 2 (February) cover image

Export Article

Open AccessArticle
Minerals 2019, 9(2), 90; https://doi.org/10.3390/min9020090

Unravelling the Crustal Architecture of Cape Verde from the Seamount Xenolith Record

1
Mineralogy Petrology Tectonics, Department of Earth Sciences, Uppsala University, Villavägen 16, SE-752 36 Uppsala, Sweden
2
Centre of Natural Hazards and Disaster Sciences (CNDS), Villavägen 16, SE-752 36 Uppsala, Sweden
3
GEOMAR Helmholtz Centre for Ocean Research Kiel, Wischhofstraße, 1-3, D-24148 Kiel, Germany
*
Author to whom correspondence should be addressed.
Received: 30 December 2018 / Revised: 28 January 2019 / Accepted: 29 January 2019 / Published: 1 February 2019
Full-Text   |   PDF [11560 KB, uploaded 1 February 2019]   |  

Abstract

The Cape Verde oceanic plateau hosts 10 islands and 11 seamounts and provides an extensive suite of alkaline lavas and pyroclastic rocks. The volcanic rocks host a range of crustal and mantle xenoliths. These xenoliths provide a spectrum of lithologies available to interact with magma during transport through the lithospheric mantle and crust. We explore the origin and depth of formation of crustal xenoliths to develop a framework of magma-crust interaction and a model for the crustal architecture beneath the Cape Verde oceanic plateau. The host lavas are phononephelinites to phonolites and the crustal xenoliths are mostly mafic plutonic assemblages with one sedimentary xenolith. REE profiles of clinopyroxene in the host lavas are light rare-earth element (LREE) enriched whereas clinopyoxene from the plutonic xenoliths are LREE depleted. Modelling of REE melt compositions indicates the plutonic xenoliths are derived from mid-ocean ridge basalt (MORB)-type ocean crust. Thermobarometry indicates that clinopyroxene in the host lavas formed at depths of 17 to 46 km, whereas those in the xenoliths formed at 5 to 20 km. This places the depth of origin of the plutonic xenoliths in the oceanic crust. Therefore, the xenoliths trace magma-crust interaction to the MORB oceanic crust and overlying sediments located beneath the Cape Verde oceanic plateau. View Full-Text
Keywords: alkaline volcanics; crustal xenoliths; thermobarometry; magma-crust interaction alkaline volcanics; crustal xenoliths; thermobarometry; magma-crust interaction
Figures

Graphical abstract

This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited (CC BY 4.0).

Supplementary material

SciFeed

Share & Cite This Article

MDPI and ACS Style

Barker, A.K.; Hansteen, T.H.; Nilsson, D. Unravelling the Crustal Architecture of Cape Verde from the Seamount Xenolith Record. Minerals 2019, 9, 90.

Show more citation formats Show less citations formats

Note that from the first issue of 2016, MDPI journals use article numbers instead of page numbers. See further details here.

Related Articles

Article Metrics

Article Access Statistics

1

Comments

[Return to top]
Minerals EISSN 2075-163X Published by MDPI AG, Basel, Switzerland RSS E-Mail Table of Contents Alert
Back to Top