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Continental Drift

Also known as:Continental DisplacementWegener's Hypothesis

Continental drift is the hypothesis that Earth's continents were once joined together in a single supercontinent called Pangaea and have since moved apart over geological time to their current positions. Proposed by Alfred Wegener in 1912, the hypothesis was supported by the jigsaw-fit of continents, matching fossil records across oceans, and similar rock formations on different continents. Continental drift later became a cornerstone of plate tectonic theory, which provided the mechanism of seafloor spreading to explain how continents move.

Evidence Supporting Continental Drift

Evidence TypeDescriptionContinents Involved
Geometric FitCoastlines of Africa and South America align like puzzle piecesAfrica, South America
Fossil MatchMesosaurus fossils found only in South America and AfricaAfrica, South America
Rock CorrelationIdentical rock sequences in Scotland and NewfoundlandEurope, North America
Glacial StriationsIce age scratch marks indicate past polar positions in tropicsIndia, Africa, Australia
Climate FossilsTropical plant fossils found in AntarcticaAntarctica

Interactive Tools

PALEOMAP Project

Animated reconstructions of continental positions through geological time

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Khan Academy — Continental Drift

Video lesson on Wegener's continental drift hypothesis and evidence

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USGS Historical Perspective on Plate Tectonics

USGS historical overview of continental drift and plate tectonic theory

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Animation showing the breakup of Pangaea and movement of continents over 250 million years

Wikimedia Commons, CC BY-SA

Related Terms

Earth Science

Plate Tectonics

Plate tectonics is the scientific theory describing how Earth's lithosphere is divided into large, rigid segments called tectonic plates that move over the underlying asthenosphere. These plates interact at their boundaries through convergence, divergence, or lateral sliding, driving processes such as mountain building, ocean floor spreading, and volcanic activity. The theory unifies many geological phenomena and explains the distribution of earthquakes, volcanoes, and major landforms across Earth's surface.

Earth Science

Rock Cycle

The rock cycle is a continuous geological process by which rocks are transformed from one type to another through processes such as melting, cooling, erosion, deposition, compaction, cementation, heat, and pressure over geological timescales. The three main rock types — igneous, sedimentary, and metamorphic — are interconnected in this cycle, each capable of being converted into another type under the right conditions. Understanding the rock cycle helps geologists interpret Earth's history, locate mineral resources, and predict geological hazards.

Earth Science

Sedimentary Rock

Sedimentary rock is formed from the accumulation and compaction of sediments — particles of minerals, organic matter, or chemical precipitates — deposited by water, wind, ice, or gravity over time. This process, called lithification, involves compaction (pressure from overlying sediment) and cementation (mineral-rich groundwater binding particles together). Sedimentary rocks cover about 75% of Earth's land surface, host nearly all fossil records, and contain major reserves of coal, oil, natural gas, and economically important minerals.

From Latin "continens" (continuous landmass) and Middle English "driften" (to float or be carried). Alfred Wegener used the German term "Kontinentalverschiebung" (continental displacement) in 1912; the English phrase "continental drift" became standard in geological literature by the 1920s.

continental driftpangaeawegenergeologyearth historysupercontinent