Meteorización de mármoles dolomíticos y su relación con la arena dolomítica de la Cueva de Nerja (Málaga, España)
- Arantza Aranburu 1
- Martín Arriolabengoa 1
- Arantxa Bodego 1
- Irantzu Álvarez 1
- Peru Bilbao-Lasa 1
- Iñaki Yusta 1
- Cristina Liñán Baena 2
- 1 Universidad del País Vasco, España
- 2 Fundación Cueva de Nerja, España
ISSN: 0213-683X
Argitalpen urtea: 2018
Zenbakien izenburua: Comunicaciones presentadas en la LXIV Sesión Científica / Ávila, 1 de Junio de 2018
Zenbakia: 64
Orrialdeak: 123-126
Mota: Artikulua
Beste argitalpen batzuk: Geogaceta
Laburpena
The karstic system of the Nerja Cave is developed in the dolomitic marbles of the Almijara Nappe. These marbles show little edaphic development but abundant weathering features. Weathering processes of dolomitic marbles caused brecciation, disintegration and formation of dolomitic sands, as well as deposits of diverse secondary carbonates: calcretas and speleothems. The Nerja Cave contains detrital deposits, mostly dolomitic sands. The objective of this work is to characterize and relate the edaphic processes of the exokarstic environment with the detrital sediments of the interior of the karst. Thus, the dolomitic sand or regolith can i) become part of the edaphic horizons, as at present; ii) be embedded in the calcrete; or iii) be transported to the interior of the karst by hydrological and gravitational processes.