No abstract

• Deep seismic data reveal oceanic-like axial ridge beneath central Red Sea. • Axial high is similar to those of hotspot-affected spreading centres. • Bouguer anomalies predict low average density beneath axis. • This low density implies thickened crust and/or low mantle density. • Normal thickness predicted from Na8.0 implies recent transition from thinner crust.

Transverse structures in the central part of the Red Sea are mapped according to bathymetric, seismic, gravity and magnetic data. Five classes of structures are detected. Three of these are fractures, intertrough zones and transform faults. The remaining two are classified as transform zones and pseudo-transform faults. Most structures can be related to ancient lineaments on land. Intertrough and transform zones are manifestations of unorganized seafloor spreading, and their crustal structure is of an oceanic nature that might be similar to quiet magnetic zones.

Summary The axial region of the Central Red Sea has been shown to be floored by oceanic crust, but this leaves the low amplitudes of off-axis magnetic anomalies to be explained.  Furthermore, if seafloor spreading occurred in the late Miocene, it is unclear how that occurred as widespread evaporites were being deposited then and may have covered the spreading centre. In this study, we derive crustal magnetization for a constant-thickness source layer within the uppermost basement by inverting aeromagnetic anomalies using basement depths derived from seismic reflection and gravity data.  Peak-to-trough variations in magnetization away from the axis are found to be slightly less than half of those of normal oceanic crust, but not greatly diminished, and hence the magnetic anomalies are mostly reduced by the greater depth of basement, which is depressed by isostatic loading by the evaporites (kilometres in thickness in places). There is no relationship between seafloor spreading anomalies and the modern distribution of evaporites mapped out using multi-beam sonar data; magnetizations are still significant even where the basement lies several kilometres under the evaporites. This suggests that magnetizations have not been more greatly affected by alteration under the evaporites than typically exposed oceanic crust. A prominent magnetization peak commonly occurs at 60–80 km from the axis on both tectonic plates, coinciding with a basement low suggested previously to mark the transition to continental crust closer to the coasts.  We suggest an initial burst of volcanism occurred at Chron 5 (at ∼10 Ma) to produce this feature. Furthermore, an abrupt change is found at ∼5 Ma from low-frequency anomalies off-axis to high-frequency anomalies towards the present axis. This potentially represents the stage at which buried spreading centres became exposed. In this interpretation, intrusions such as sills at the buried spreading centre led to broad magnetic anomalies, whereas the later exposure of the spreading centre led to a more typical development of crustal magnetization by rapid cooling of extrusives.

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