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Continental margin subsidence from shallow mantle convection: Example from West Africa

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posted on 2018-01-08, 14:46 authored by Bhavik Harish Lodhia, Gareth G. Roberts, Alastair J. Fraser, Stewart Fishwick, Saskia Goes, Jerry Jarvis
Spatial and temporal evolution of the uppermost convecting mantle plays an important role in determining histories of magmatism, uplift, subsidence, erosion and deposition of sedimentary rock. Tomographic studies and mantle flow models suggest that changes in lithospheric thickness can focus convection and destabilize plates. Geologic observations that constrain the processes responsible for onset and evolution of shallow mantle convection are sparse. We integrate seismic, well, gravity, magmatic and tomographic information to determine the history of Neogene-Recent ( < 23 Ma) upper mantle convection from the Cape Verde swell to West Africa. Residual ocean-age depths of +2 km and oceanic heat flow anomalies of +16 ± 4 mW m −2 are centered on Cape Verde. Residual depths decrease eastward to zero at the fringe of the Mauritania basin. Backstripped wells and mapped seismic data show that 0.4–0.8 km of water-loaded subsidence occurred in a ∼500 × 500 km region centered on the Mauritania basin during the last 23 Ma. Conversion of shear wave velocities into temperature and simple isostatic calculations indicate that asthenospheric temperatures determine bathymetry from Cape Verde to West Africa. Calculated average excess temperatures beneath Cape Verde are > +100 °C providing ∼10 3 m of support. Beneath the Mauritania basin average excess temperatures are < −100 °C drawing down the lithosphere by ∼10 2 to 10 3 m. Up- and downwelling mantle has generated a bathymetric gradient of ∼1/300 at a wavelength of ∼10 3 km during the last ∼23 Ma. Our results suggest that asthenospheric flow away from upwelling mantle can generate downwelling beneath continental margins.

Funding

HL is supported by a National Environment Research Council Oil & Gas CDT studentship. We are grateful to R. Cowan, R. Newton and colleagues at Tullow Oil Plc. and TGS for providing access to seismic and well data. IRIS Data Management Centre, and Geofon Program GFZ Potsdam were used to access seismic waveforms. Thanks are given to C. Ebinger, G. Ruempker, D. Shillington and co-investigators for early access to data not publicly available.

History

Citation

Earth and Planetary Science Letters, 2018, 481, pp. 350-361

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/School of Geography, Geology and the Environment

Version

  • AM (Accepted Manuscript)

Published in

Earth and Planetary Science Letters

Publisher

Elsevier

issn

0012-821X

Acceptance date

2017-10-08

Copyright date

2017

Available date

2018-11-25

Publisher version

http://www.sciencedirect.com/science/article/pii/S0012821X17305836

Notes

The file associated with this record is under embargo until 12 months after publication, in accordance with the publisher's self-archiving policy. The full text may be available through the publisher links provided above.

Language

en

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