Alpine orogeny

From Wikipedia, the free encyclopedia

Geology of the Alps
Mont Blanc
Tectonic subdivision

Helvetic nappes

Penninic nappes
Austroalpine nappes
Southern Alps
Formations & rocks

Bündner slate | flysch | molasse

Geological structures

Aarmassif | Dent Blanche klippe | Engadine window | Flysch zone | Giudicárie line | Greywacke zone | Hohe Tauern window | Molasse basin | Penninic thrustfront | Periadriatic Seam | Ivrea zone | Lepontin dome | Rechnitz window | Rhône-Simplon line | Sesia unit

Paleogeografic terminology

Valais Ocean

Briançonnais microcontinent
Piemont-Liguria Ocean
Apulian or Adriatic plate

The Alpine orogeny (sometimes also called Alpide orogeny) is an orogenic phase in the Tertiary that formed the mountain ranges of the Alpide belt. These mountains include (from west to east) the Atlas, the Pyrenees, the Alps, the Dinaric Alps, the Hellenides, the Balkan, the Taurus, the Caucasus, the Alborz, the Zagros, the Hindu Kush, the Pamir, the Karakoram, and the Himalayas. Sometimes other names occur to describe the formation of separate mountain ranges: for example Carpathean orogeny for the Carpathians, Hellenic orogeny for the Hellenides or the Himalayan orogeny for the Himalayas.

The Alpine orogeny occurred when the continents Africa and India and the small Cimmerian plate collided (from the south) with Eurasia in the north. Convergent movements between the tectonic plates (the Indian plate and the African plate from the south, the Eurasian plate from the north, and many smaller plates and microplates) began already in the early Cretaceous, but the major phases of mountain building began in the Paleocene to Eocene. Currently the process still continues in some of the Alpide mountain ranges.

The Alpine orogeny is considered one of the three major phases of orogeny in Europe that define the geology of that continent. The three are:

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