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Laurasia

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Laurasia was a massive continental landmass located in the northern hemisphere. It formed as a primary component of the supercontinent Pangaea. To understand Laurasia, one must look at its two main counterparts. One part was the southern supercontinent known as Gondwana. The other was the massive, singular landmass of Pangaea itself. Laurasia is a portmanteau, which is a word made by joining two other names. It combines the names Laurentia and Eurasia.

Laurasia 330Ma
Laurasia 330Ma

The formation of Laurasia was a complex process involving many collisions. It began with the creation of Laurussia, also called Euramerica. This happened when Laurentia, the core of North America, collided with Baltica and Avalonia. This event is known as the Caledonian orogeny, which occurred around 430 to 420 million years ago.

Laurussia Euramerica
Laurussia Euramerica

Later, the landmass grew larger through more additions. Siberia and Kazakhstania collided with the existing mass during the Late Permian period. These additions transformed the smaller Laurussia into the much larger Laurasia. Eventually, Laurussia collided with Gondwana to form the supercontinent Pangaea.

Laurasia 430Ma
Laurasia 430Ma

Geological history shows that these landmasses were part of even older systems. Long before Laurasia, there was a supercontinent called Columbia, assembled between 2,100 and 1,800 million years ago. During this time, Laurentia and Baltica formed a mass called Proto-Laurasia.

Paleoglobe NO 1590 mya-vector-colors
Paleoglobe NO 1590 mya-vector-colors

Later, Laurentia formed the core of another supercontinent named Rodinia around 1,260 to 900 million years ago. The exact arrangement of continents within Rodinia is still a subject of scientific debate. Some reconstructions suggest Australia and East Antarctica were on Laurentia's western margin. Other models place Siberia near Laurentia's northern margin.

Rodinia 900Ma
Rodinia 900Ma

Scientists have used many different methods to reconstruct these ancient worlds. In 1904, Austrian geologist Eduard Suess proposed that southern continents were once merged into Gondwana. In 1915, German meteorologist Alfred Wegener proposed the existence of the supercontinent Pangaea. Later, in 1937, South African geologist Alexander du Toit provided a crucial detail. He proposed that Pangaea was divided into two large masses. He identified Laurasia in the north and Gondwana in the south. They were separated by a body of water called the Tethys Ocean.

Rodinia 900Ma
Rodinia 900Ma

The movement of these plates created significant geological changes. During the Devonian period, the Iapetus Ocean closed due to subduction. Subduction is a process where one part of the ocean floor sinks beneath another. This closure helped form Laurussia. In the Late Devonian, tetrapods, which are four-limbed animals, began to evolve from fish. The oldest known fossils of these creatures are found in Greenland.

Mollweide Paleographic Map of Earth, 405 Ma (Emsian Age)
Mollweide Paleographic Map of Earth, 405 Ma (Emsian Age)

High productivity of plankton also caused anoxic events. Anoxic means a lack of oxygen, which left black shales in the basins of Laurentia.

Laurasia's eventual breakup shaped the modern world map. The separation from Gondwana began during the late Triassic period. As Pangaea broke apart, Laurasia drifted further north. A major turning point occurred 56 million years ago. This was when the North Atlantic Ocean opened up. This opening caused Laurasia to become an independent continental mass.

Laurasia 330Ma
Laurasia 330Ma

The pieces of Laurasia eventually became the continents we recognize today, including parts of North America, Europe, and Asia.

The study of Laurasia connects many different scientific fields. It links plate tectonics with the history of life through fossil records. For example, the movement of continents changed how marine animals could spread. During the Cambrian period, only plankton could cross wide oceans. As continents moved closer, bottom-dwelling animals like brachiopods and trilobites could spread between landmasses. This shows how the physical movement of the Earth directly influences the biological history of our planet.

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🖼️ Images & Media (6)
File:Paleoglobe NO 1590 mya-vector-colors.svg
Paleoglobe NO 1590 mya-vector-colors.svg
File:Rodinia 900Ma.jpg
Rodinia 900Ma.jpg
File:Laurasia 430Ma.jpg
Laurasia 430Ma.jpg
File:Laurussia Euramerica.svg
Laurussia Euramerica.svg
File:Mollweide Paleographic Map of Earth, 405 Ma (Emsian Age).png
Mollweide Paleographic Map of Earth, 405...
File:Laurasia 330Ma.jpg
Laurasia 330Ma.jpg
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