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Continental drift hypothesis

The comparison of geographic and geologic continental features across oceans that encouraged the continental drift hypothesis.

The comparison of continental coastline geometries, rock types and patterns, fossils, and glacial formations across oceans that encouraged the continental drift hypothesis.

This map displays a simplified view of the early supercontinent Gondwana. During the time of Gondwana, present-day continents were geographically assembled like a jigsaw puzzle. Continental deformation such as mountain chains, glacial erosion patterns, and the distribution of plants and animals left their marks across the entire supercontinent. When it eventually split up, at around 180 Million years ago, some of these marks were preserved in the geologic record of the dispersed present-day continents.

Geologists, amongst which Antonio Snider-Pellegrini and Alfred Wegener, realised that some of the fossils of similar organisms matched across the present-day continents and encouraged the revolutionary theory of continental drift. Continental drift describes one of the earliest ways geologists thought continents moved over time. More than fifty years later, this theory evolved into the concept of Ocean-plate tectonics, that describes the plate motion at the Earth’s surface as the uppermost dynamic part of mantle convection, the overturn of Earth’s solid but viscous silicate mantle.

The typeface ‚Fufu‘ by Lucia Perez-Diaz is used.

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Plate boundaries & Euler pole

Illustration of how plates move across the Earth featuring the Euler pole and plate boundary end-members.

Illustration of how plates move across the Earth. The motion of (almost) rigid surface portions on a sphere can be described by a rotation around a rotation axis, which cuts the surface at the so-called Euler pole. This relative motion of the plates is mainly accommodated by localised deformation at plate boundaries. Three general types of plate boundaries exist: transform plate boundaries allow the plates to move alongside each other, and convergent and divergent plate boundaries allow for plate destruction and creation, respectively. Transform and divergent plate boundaries are almost straight features, but spreading ridges are generally offset laterally by transform intersections. Subduction zones are usually arcuate (i.e., concave toward the upper plate) due to interaction with mantle flow. Variations of these plate boundaries exist depending on the given combination of upper and lower plate nature (i.e., continental or oceanic).

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