Influence of Hotspot Magmatism on Breakup Modes and Oceanic Crust
Architecture along a Passive Margin: Insights from
Mauritania/Senegal/Guinea Basin
Abstract
The breakup of the Central Atlantic is known to terminate around 190Myrs
while the CAMP (Central Atlantic Magmatic Province) activity was ending.
A dense seismic dataset, acquired along the MSG Basin, provide detailed
images of the continent-ocean transition and oceanic crust architecture.
Five oceanic/magmatic crust facies were described and mapped. They
reveal, in the north, a progressive increase of magmatism. In the south,
a 9-11 km thick magmatic crust is observed. Locally, a peculiar facies,
with intra-oceanic SDR, is observed and correlated with the formation of
the African Black Spur Magnetic Anomaly (ABSMA). In the North, seismic
data suggest a typical magma-poor margin profile with an extremely
thinned continental crust and mantle exhumation at the COT. In the
South, the continental crust thinning is associated with SDR
emplacement, and a thick magmatic crust emplaced in the distal domain,
which is typical of magma-rich margins.
Therefore, in the South, the breakup was forced through the continental
crust due to the remnant activity of a CAMP derive hotspot. In the
North, the magmatic input seems directly linked to the plate motion in
the exception of the ABSMA during which, despite a brief and sudden
acceleration of the plate motion, an increase of mantle temperature is
needed to explain the change in oceanic crust thickness and facies.
This evolution emphasizes that the architecture, and thus processes
leading to breakup, can vary considering the influence of thermal
vertical forces and mechanical horizontal forces, both being necessary
for a rift to succeed.