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Slab pull

earth science Maturity 9-11 Next article →

Slab pull is a major geophysical mechanism. It is a force that drives the movement of tectonic plates. This process occurs when a tectonic plate cools down over time. As the plate cools, it becomes more dense. This density causes the plate to sink into the mantle. This sinking creates a downward force along the rest of the plate. This force is a primary driver of plate tectonics on Earth.

The mechanism of slab pull works through a specific sequence of events. First, an oceanic plate moves away from a ridge and cools. This cooling makes the plate denser than the material beneath it. The dense part of the plate then begins to sink at oceanic trenches. This sinking part is known as a subducting plate. As the slab sinks, its weight pulls the rest of the plate behind it. This action is often paired with slab suction. Together, these forces account for almost all the force driving plate motion.

Scientists have identified different ways this force manifests. It can appear in two extreme forms. One form is aseismic back-arc extension. We see this in the Izu–Bonin–Mariana Arc. In this case, the movement does not cause many earthquakes. The other form involves strong earthquakes and back-arc thrusting. Examples of this include the Aleutian and Chile tectonics. These variations show how different plates respond to these massive forces.

Researchers have used math to define the slab pull force. Scientists look at several specific variables to calculate it. They use gravitational acceleration, which is 9.81 m/s2. They also measure the mean density difference between the slab and the asthenosphere. This difference is approximately 80 kg/m3. The calculation also requires the slab length. This length is only measured above the 670 km boundary. Finally, they include the age of the slab in Ma, or millions of years.

Our understanding of these forces changed due to important studies. In 1975, researchers Forsyth and Uyeda conducted a study. They used the inverse theory method to analyze plate motion. Their work showed that slab pull is the strongest driving force. Before this, some models suggested plates rode on convection cells. These models acted like conveyor belts. However, most modern scientists believe this is not the case. They found that the asthenosphere does not cause motion through basal friction.

The significance of slab pull is clear when comparing it to other forces. Ridge push is another force caused by rifts. However, ridge push contributes only 5 to 10% of the total force. Slab pull and slab suction are much more powerful. We can see the impact of these forces in the Pacific Ring of Fire. The subducting slabs there help cool the Earth and its core-mantle boundary. This process helps regulate the temperature of our planet's deep interior.

Different plates interact with these systems in unique ways. Some plates do not have subducting slabs at all. The North American Plate is not currently being subducted. The African, Eurasian, and Antarctic Plates are also not subducting. These plates move due to ridge push instead. In contrast, the African Plate experiences upwelling mantle plumes. These plumes come from the core-mantle boundary. This process produces rifting in the African and Ethiopian rift valleys.

The history of the Farallon Plate provides a complex example of these changes. It showed an evolution in slab width and movement. It once had a huge slab width. This caused the Nevada, Sevier, and Laramide orogenies. Later, it experienced the Mid-Tertiary ignimbrite flare-up. Eventually, it was left as the Juan de Fuca and Cocos plates. This area also shows the Basin and Range Province. This province is under extension due to slab break off and mantle return flow.

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