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The Tethys Ocean (Greek: Τηθύς) was an ocean that existed between the continents of Gondwana and Laurasia during the Mesozoic era before the opening of the Indian Oceanmarker.

Modern theory

About 250 million years ago, during the Triassic, a new ocean began forming in the southern end of the Paleo-Tethys Ocean. A rift formed along the northern continental shelf of Southern Pangaea (Gondwana). Over the next 60 million years, that piece of shelf, known as Cimmeria, traveled north, pushing the floor of the Paleo-Tethys Ocean under the eastern end of Northern Pangaea (Laurasia). The Tethys Ocean formed between Cimmeria and Gondwana, directly over where the Paleo-Tethys used to be.

The Tethys Ocean closes again, about 90 million years ago
During the Jurassic Period (150 Ma), Cimmeria finally collided with Laurasia. There it stalled, the ocean floor behind it buckling under, forming the Tethyan Trench. Water levels rose and the western Tethys came to shallowly cover significant portions of Europe, forming the (first) Tethys Sea. Around the same time, Laurasia and Gondwana began drifting apart, opening an extension of the Tethys Sea between them that today is the part of the Atlantic Oceanmarker between the Mediterraneanmarker and Caribbeanmarker. As North and South America were still attached to the rest of Gondwana and Laurasia, respectively, the Tethys Ocean in its widest extension was part of a continuous oceanic belt running around the Earth between about latitude 30° N and the Equator. Thus, ocean currents at that time – around the Early Cretaceous – ran radically differently from the way they do today.

Between the Jurassic and the Late Cretaceous (which started about 100 Ma), even Gondwana began breaking up, pushing Africa and Indiamarker north, across the Tethys and opening up the Indian Oceanmarker. As these land masses pushed in on it from all sides, up until as recently as the Late Miocene (15 Ma), the Tethys ocean continued to shrink, becoming the Tethys Seaway or (second) 'Tethys Sea'.

Today, India, Indonesiamarker and the Indian Oceanmarker cover the area once occupied by the Tethys Ocean, and Turkeymarker, Iraqmarker, and Tibet sit on Cimmeria. What was once the Tethys Sea has become the Mediterranean Seamarker. Other remnants are the Blackmarker, Caspianmarker and Aralmarker Seas (via a former inland branch known as the Paratethys). Most of the floor of the Tethys Ocean disappeared under Cimmeria and Laurasia. Geologists like Suess have found fossils of ocean creatures in rocks in the Himalayasmarker, indicating that those rocks were once underwater, before the Indian continental shelf began pushing upward as it smashed into Cimmeria. We can see similar geologic evidence in the Alpine orogeny of Europe, where the movement of the African plate raised the Alps.

Paleontologists also find the Tethys Ocean particularly important because much of the world's sea shelves were found around its margins for such an extensive period of time. Marine, marsh-dwelling, and estuarian fossils from these shelves are of considerable paleontological interest.

Historical theory

In 1893, using fossil records from the Alps and Africa, Eduard Suess proposed the theory that an inland sea had once existed between Laurasia and the continents which formed Gondwana II. In this moment of Earth's life, however, these two continental masses were united in a unique supercontinent, known as Gondwana III or Pangaea. He named it the 'Tethys Sea' after the Greek sea goddess Tethys. When the theory of plate tectonics became established in the 1960s it became clear Suess's "sea" had in fact been an ocean. Plate tectonics also provided the mechanism by which the former ocean disappeared. In plate tectonic theory oceanic crust can subduct under continental crust.

Terminology and subdivisions

Like every science, geology is a continuously evolving system of theories, and the terms used to describe various pre-historic formations have fluctuated as more accurate theories have emerged. For example, many internet sources use "Tethys Ocean" to refer to the "Tethys Sea" and vice versa. Some even appear to erroneously refer to the growing Atlantic Oceanmarker during the Jurassic as the Tethys Sea.

The western part of the Tethys Ocean is called Tethys Sea, Western Tethys Ocean or Alpine Tethys Ocean. The Blackmarker, Caspianmarker and Aralmarker Seas are thought to be its crustal remains (though the Black Sea may in fact be a remnant of the older Paleo-Tethys Ocean ). However, this "Western Tethys" was not simply a single open ocean. It covered many small plates, Cretaceous island arcs and microcontinents. Many small oceanic basin (Valais Ocean, Piemont-Liguria Ocean, Meliata ocean) were separated from each other by continental terranes on the Alboran, Iberian, and Apulian plates. The high sealevel in the Mesozoic age flooded most of these continental domains forming shallow seas.

During the Oligocene, large parts of central and eastern Europe were covered by a northern branch of the Tethys Ocean, called the Paratethys. The Paratethys was separated from the Tethys by the formation of the Alps, Carpathiansmarker, Dinarides, Taurusmarker and Elburzmarker mountains during the Alpine orogeny. It gradually disappeared during the late Miocene, becoming an isolated inland sea.

The eastern part of the Tethys Ocean is likewise sometimes referred to as Eastern Tethys.

As theories have improved, scientists have extended the "Tethys" name to refer to similar oceans that preceded it. The Paleo-Tethys Ocean, mentioned above, existed from the Silurian (440 Ma) through the Jurassic eras, between the Hunic terranes and Gondwana (later the Cimmerian terranes). Before that, the Proto-Tethys Ocean existed from the Ediacaran (600 Ma) into the Devonian (360 Ma), and was situated between Baltica and Laurentia to the north and Gondwana to the south. Neither Tethys oceans should be confused with the Rheic Ocean, which existed to the west of them in the Silurian era.

See also


  1. Palaeos Mesozoic: Triassic: Middle Triassic

External links

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