In situ motions of the American continents; Caribbean consequences
DSDP Leg 10 data demonstrated the relatively rapid late Cretaceous foundering of the Gulf of Mexico deep sea plain
27; while recovered Albian and older deposits were consistently of shallow-water nature, younger strata became abyssal between late Albian and the Santonian. This break-down of continental crust was not an isolated Gulf of Mexico affair – it was global, notably in the oceans. Embryonic deep sea basins, which had been under way since the Middle Jurassic, reached in the Upper Cretaceous abyssal depths for the first time in Earth history. Hence, it appears that the upper mantle hydrostatic pressures and volatile content, necessary to accelerate eclogitization and associated sub-crustal delaminating processes, took most of geological time to accumulate
13. The build-up and release of upper mantle hydrostatic pressures, causing repeated uplift and subsidence of the developing oceanic basins, were apparently in phase with the transgression-regression cyclicity affecting low-lying lands
13. Until the late Mesozoic, the South Atlantic trans-oceanic ‘land bridges’ were still relatively unimpaired, but due to the pre-existing sets of ubiquitous parallel fractures, the evolving continental margins became closely parallel
28. The popular view that parallel margins is prima facie evidence of hypothesized sea floor spreading has come to rest.
The deep sea basins that formed during the Jurassic were only of limited extent, frequently giving rise to anoxic conditions and black shale formation. These basins were surrounded by a mosaic of sub-aerially exposed semi-continental regions (less affected by sub-crustal break-down processes), a physiographic situation similar to that of the Caribbean. Many oceanic fragments of former land can still be recognized by the multitude of aseismic ridges and plateaus having intermediately thick crust – in the Caribbean and elsewhere. Towards the end of the Cretaceous the modern continent-ocean physiography was approaching its present state. The Moho interface as well as upper mantle volatile- and melt-holding low-velocity layers – the asthenosphere – had reached more mature stages, and substantial crustal loss to the mantle led to jerky changes in Earth’s moments of inertia. The dynamic consequences were phases of true polar wander (distinct spatial reorientations of the globe) and an overall acceleration in the Earth’s rate of rotation. For the first time in Earth history, remaining continental masses were
- surrounded by thin and mechanically fragile oceanic crust, and
- a more developed asthenosphere was in place – factors that provided a tectonically unstable situation.
The development had paved the way for a global geological revolution – the Alpine climax, during which also the principal Caribbean tectonic structures became entrenched.