Plate Tectonics
Plate tectonics describes the large-scale motion of Earth's lithosphere, which is broken into tectonic plates. This section begins with a review of previous knowledge on Earth's structure and the changes continents and oceans undergo over time. It emphasizes the work of early theorists like Abraham Ortelius and Alfredo Wegener, who suggested that continents were once joined and later drifted apart, culminating in the comprehensive Plate Tectonics theory presented by McKenzie and Parker in 1967.
Key Historical Concepts
- Continental Drift: Wegener's theory that continents at one time formed a single supercontinent named Pangaea, surrounded by Panthalassa. This idea was bolstered by how coastlines of South America and Africa fit together and similarities in rock formations and fossils across oceans.
Evidence Supporting Continental Drift
- Matching Coastlines: Notably, the symmetrical fit of the South American and African coastlines.
- Rock Age Correlation: Ancient rocks of similar ages found on opposite sides of oceans.
- Glacial Tillite: Evidence of glacial formations in rocks across different continents supports the drifting theory.
- Fossil Record: Identical fossils found on separated continents suggest they were once connected.
Plate Tectonics Theory
- Movement of Plates: Unlike Wegener's focus on continents moving independently, Plate Tectonics explains that the entire plate, consisting of both oceanic and continental crust, moves.
- Types of Plate Boundaries: Divergent (plates move apart), convergent (plates collide), and transform (plates slide past each other).
- Driving Forces: Includes convection currents in the mantle and the Earth's rotational forces.
This section sets the foundation for understanding how plate tectonics shapes our planet's surface and drives geological phenomena like earthquakes and volcanic eruptions.