Chilean Coast Range

Last updated
Chilean Coastal Range
Oncolvista.jpg
View from Cerro Oncol
Highest point
Peak Cerro Vicuña Mackenna
Elevation 3,114 m (10,217 ft) [1]
Coordinates 24°27′01″S70°02′55″W / 24.4502778°S 70.0486111°W / -24.4502778; -70.0486111 [1]
Dimensions
Length3,100 km (1,900 mi)North-South
Geography
Cordillera de la costa.JPG
The eastern border of the Chilean Coast Range is marked with yellow. Uncertain borders are marked with dots.
CountryChile
Range coordinates 32°58′32″S71°00′49″W / 32.9756°S 71.0135°W / -32.9756; -71.0135
Parent range Andes

The Chilean Coastal Range (Spanish : Cordillera de la Costa) is a mountain range that runs from north to south along the Pacific coast of South America parallel to the Andean Mountains, extending from Morro de Arica in the north to Taitao Peninsula, where it ends at the Chile Triple Junction, in the south. The range has a strong influence on the climate of Chile since it produces a rain shadow to the east. Because of this the vegetation growing on the seaward slopes is much more exuberant than in the interior. Compared to the coastal lowlands and the Intermediate Depression, it is sparsely populated with land use varying from protected areas to grazing and silviculture. The range is present in all Chilean regions, except for Coquimbo Region and Magallanes Region.

Contents

Geography

Like the Andes, the coastal range becomes progressively lower with increasing latitude. The range begins at Morro de Arica in the north and reaches its highest point, of 3114 m, in Sierra Vicuña Mackenna in the Antofagasta Region. Between Copiapó and Aconcagua rivers, in the so-called Norte Chico region, the range fuses with the Andes. Just north of Santiago the range separates from the Andes but comes close to it again near Paine, a southern suburb of Santiago, and San Fernando. From Santiago south the range loses height until reaching the Bío-Bío River, beyond which the Nahuelbuta range emerges which reaches about 1500 m in its central parts. South of Nahuelbuta Range, in the Araucanía Region, the coastal range is replaced by a flatland area. South of Toltén River the range rises again as the Cordillera de Mahuidanchi. Beyond the heights of Corral this range changes into Cordillera Pelada. From Chacao Channel south the range is penetrated by the sea creating islands and peninsulas. Chiloé Island, the largest of these, has two ranges: Cordillera del Piuchén from Chacao Channel to Cucao Lake and Pirulil Range in the southern half. South of Chiloé the portions of the range above sea level form the Guaitecas and the Chonos Archipelagos. The southern extreme of the range forms the Taitao Peninsula and its sub-peninsula Tres Montes.

The range can be divided in several minor ranges. Some of these ranges and their boundaries are:

Cerro Armazones, home of the E-ELT, is located in the Sierra Vicuna Mackenna. The Road to the Future.jpg
Cerro Armazones, home of the E-ELT, is located in the Sierra Vicuña Mackenna.

Geology

The range has no single structural or lithological origin but is the result of the alignment of horst, forearc highs and upthrusted blocks along Chile's coast. The range was separated from the Andes during the Tertiary rise of the Andes due to the subsidence of the Intermediate Depression.

The range is made of different lithological units. From Valparaíso Region to Lanalhue Fault the bedrock is largely made up of the Coastal Batholith of central Chile. These igneous rocks were once part of a proto-Andean magmatic belt. South of Lanalhue Fault most of the range is made up by the Bahía Mansa Metamorphic Complex which is made up of medium grade metamorphic rocks including schists. The analogous granites of the northern part of the coast range are placed inside the Andes in this latitudes.

During the Miocene regions of the Chilean Coast Range hosted several volcanoes. At present it does not show any sign of volcanic activity.

The northern part of the Chilean Coast Range contains a series of iron ore deposits known as the Chilean Iron Belt which are aligned along the Atacama Fault. [2]

See also

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The Vicuña Mackenna Batholith is a group of plutons in the Chilean Coast Range of northern Chile. The plutons of the batholith formed between the Early Jurassic and the Late Cretaceous. The magmas that formed the batholith originated in Earth's mantle and have not suffered any significant crustal contamination. A group of Early Cretaceous plutons were intruded syn-tectonically on the Atacama Fault.

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References

  1. 1 2 "Cerro Vicuña Mackenna". Wikimapia.
  2. Tornos, Fernando; Hanchar, John M.; Munizaga, Rodrigo; Velasco, Francisco; Galindo, Carmen (2020). "The role of the subducting slab and melt crystallization in the formation of magnetite-(apatite) systems, Coastal Cordillera of Chile". Mineralium Deposita . 56 (2): 253–278. doi:10.1007/s00126-020-00959-9. S2CID   212629723.