Article (Scientific journals)
Karst and Underground Landscapes in the Cretaceous Chalk and Calcarenite of the Belgian-Dutch Border—The Montagne Saint-Pierre
Willems, Luc; Rodet, Joël
2018In Landscapes and Landforms of Belgium and Luxembourg, p. 177-192
Peer reviewed
 

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Keywords :
Chalk karst; Blind cave; Underground quarrying; Solution pipe
Abstract :
[en] The eastern part of the Hesbaye plateau, which extends into the Dutch Limburg, was excavated by many underground quarries that mainly exploited the Cretaceous chalk of the Maastrichtian. In this area, the Meuse and its tributaries cut into the shallow dipping formations. Thus, entries of quarries usually are on hillsides. Most galleries sink horizontally along calcarenite layers, a coarse chalk also called «Tuffeau of Maastricht». The dimensions and extensions of these networks create real underground landscapes. These galleries intersect thousands of karst features and allow a privileged observation in three dimensions. These karst phenomena have dual characteristics: they mainly grow in a very porous lithology and outside fractures, so a context unfavourable to, a priori, a necessary concentrated weathering. Once dewatered, they cease to function, thus fossilizing a karst system in one of the rarely seen early genetic phases.
Disciplines :
Earth sciences & physical geography
Author, co-author :
Willems, Luc ;  Université de Liège - ULiège > Département de géologie > Pétrologie sédimentaire
Rodet, Joël;  CNRS > UMR 6143 - Laboratory of GeologyUniversity of Rouen
Language :
English
Title :
Karst and Underground Landscapes in the Cretaceous Chalk and Calcarenite of the Belgian-Dutch Border—The Montagne Saint-Pierre
Alternative titles :
[en] Karst and Underground Landscapes in the Cretaceous Chalk and Calcarenite of the Belgian-Dutch Border—The Montagne Saint-Pierre
Publication date :
2018
Journal title :
Landscapes and Landforms of Belgium and Luxembourg
ISSN :
2213-2090
eISSN :
2213-2090
Publisher :
Springer Nature
Pages :
177-192
Peer reviewed :
Peer reviewed
Available on ORBi :
since 24 February 2018

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