Plate Tectonics

An important feature that sets the Earth apart from its planetary siblings is the process of plate tectonics, whereby rafts of rigid rock 'floating' on a sea of more mobile rock move slowly over the surface, powered by the dynamo of convection currents in the liquid metal of the Earth's outer core.

Why is this process important for life? Plate tectonics is a vital part of the global cycle that maintains the carbon balance between atmosphere, hydrosphere and lithosphere.

The phenomenon of plate tectonics, also known as "continental drift", derives directly from the internal structure of the Earth: a molten outer metallic core surrounding a solid inner metallic core, overlain by the mantle, a layer of partially molten silicate rocks, above which is the buoyant but rigid lithosphere.

Sliding plates

The upper part of the lithosphere, the crust, is thinner below the oceans (~ 7 km thick) than it is below the continents (generally ~ 35 km thick, but can be up to 80 km in places).

The lithosphere is not a continuous layer of material, but is made up of individual pieces, or plates, that fit together like the pieces of a giant jigsaw puzzle. The plates are bodies of slowly moving rock floating on top of the mantle. The plates are in constant motion, colliding with each other in some parts of the globe, or sliding past each other, or moving apart.

Tectonic activity at plate boundaries

The plate boundaries (see the diagram) are characterised by different types of tectonic activity, depending on whether new crust is being formed or old crust destroyed. Where two oceanic plates collide, or an oceanic plate collides with a continental plate, there is a subduction zone, where the lithosphere is dragged down into the mantle and melted. A typical example is along the line of the Andes in South America, where the eastwards moving oceanic Nazca plate is being pulled below the westwards moving South American continental plate, at a rate of ~ 9cm per year.

Subduction zones are marked by arcs of volcanic activity. At collision zones between continents, rocks are uplifted into mountain chains. For example, the Himalayas have formed where the Indian plate moves northwards against the Eurasian plate at a rate of ~ 5cm per year. Where plates move past each other, transform faults develop, associated with which are some of the world's major earthquake zones, e.g., the San Andreas fault in California, where the Pacific plate is moving eastwards against the north-north westwards moving North American plate at a rate of ~ 1 cm per year.

Spreading centres are regions where plates are moving apart, where new ocean crust is forming (e.g., the mid-Atlantic ridge, where the North American plate moves away from the Eurasian plate at a rate of ~ 4 cm per year). Spreading centres are usually characterised by chains of volcanoes, hydrothermal vents and hot springs.

The important role of plate tectonics

The Earth is delicately poised between snowball and greenhouse, and the key to this balance is the fate of carbon dioxide (CO2). The balance is maintained by the process of plate tectonics, removing CO2 at subduction margins and producing CO2 at volcanoes and hot springs.

As far as we know, the Earth is the only planet in the Solar System to exhibit plate tectonics, although there has been a suggestion that a limited type of tectonic activity occurred early in Mars' history.

Allied to the significance of plate tectonics in terms of the carbon cycle are the importance of mountain building and the competing process of erosion. At collision boundaries, rocks are uplifted into mountain chains. Gradual erosion of the mountains is countered by continued uplift.

Without plate tectonics no Life

If plate tectonics were to cease, then so would this mountain building activity. Erosion would then, eventually, abrade down the mountains. Sediments removed by erosion, carried into the oceans by rivers and streams would eventually lead to a rise in sea level. If the process continued, it is calculated that eventually a global ocean would cover the Earth completely, resulting in catastrophic extinction of all land-based species.

Last updated June 28, 2001