Classical plate tectonic theory was developed in the 1960s.
It proposed that the outer layer of our planet is made up of a small number of rigid plates separated by narrow boundaries. The surface of Earth could be viewed as a simple jigsaw puzzle with just nine large plates and a bunch of much smaller ones.
Read more: Breaking new ground – the rise of plate tectonics
But what was glossed over when global plate tectonic models were first developed was the enormous deformation experienced by these seemingly rigid plates.
Fifty years after the plate tectonic revolution, we are pretty sure the continental parts of plates are not uniform, nor are they rigid. The giant forces that slowly move continents across the viscous mantle layer underneath, like biscuits gliding over a warm toffee ocean, stress the continents, and twist and contort the crust. This is a process that has taken place over millions of years.
As part of recent research, we worked with a team of international collaborators to build a computer model to show just how much the continents have been deformed since the Triassic Period, about 250 million years ago. The supercontinent Pangea began breaking apart soon after, ripping along the seams between Africa and North America.
We detail this new understanding of continent mangling in a paper published this month in the journal Tectonics.
Read more: Plate tectonics: new findings fill out the 50-year-old theory that explains Earth's landmasses
Immense forces
We already knew that that colossal tectonic forces act along plate boundaries. We can see this when continents collide, such as when Africa collided with Eurasia, forming mountains like the Alps, or forming basins when continents are torn apart, as is happening in East Africa.
Our new research used geological and geophysical data to pinpoint all major zones of continental deformation, built into a global model of plate motions using our GPlates software.
We show that at least one third of all continental crust has been massively deformed since Pangea first started breaking up. That’s a whopping 75 million km2, roughly the size of North and South America and Africa combined.
Read more: Curious Kids: how do mountains form?
Deformed continental regions include large stretched and submerged continents like Zealandia, as well as crustal contraction where collisions have occurred, producing mountain belts such as the Himalayas, the European Alps, Iran’s Zagros Mountains and the southern Alps of New Zealand.
The cradle of humankind
When crust is being thinned and stretched, the crustal contortions are usually hidden away from view because they are quickly covered up by sediments. But there are exceptions.
The East African Rift valley is one of the most spectacular examples of crustal extension visible at the surface. It has not subsided below sea level because the region is being pushed up by a mantle plume, a large upwelling of hot molten material causing uplift and volcanism.
The rift valley is underlain by a giant fault system that is splitting Africa in two. The rift turned a flat landscape into one with 4km high mountains and lake basins with vegetation ranging from desert to cloud forest. This variety of surface environments paved the way for the early evolution and diversification of humans.
Read more: Africa is splitting in two – here is why
The importance of stress
We may not like stress in our daily lives, but the continuous stress and strain acting on continents provides us with an important record of Earth’s history.
Modelling the patterns of continental deformation through time allows us to explore regional patterns of earthquakes and volcanism and explain dramatic changes in Earth’s climate over time.
It also provides a framework based on tectonic data to seek mineral resources such as the metals cobalt and tungsten, which are needed for a sustainable energy future.
Dietmar Müller receives funding from The University of Sydney, the Australian Research Council Industrial Transformation Research Hub for Basin Geodynamics and Evolution of Sedimentary Systems (Basin GENESIS Hub), and the Deep Carbon Observatory (DCO).
Maria Seton receives funding from the Australian Research Council and has received ship time funding on Australia's Marine National Facility.
Sabin Zahirovic receives funding from The University of Sydney, the Australian Research Council Industrial Transformation Research Hub for Basin Geodynamics and Evolution of Sedimentary Systems (Basin GENESIS Hub), and the Deep Carbon Observatory (DCO).
This article was originally published on The Conversation. Read the original article.
