Experimental and numerical investigations on density-driven dissolution of CO2 and related carbonate dissolution in karst water

Department of Hydromechanics and Modelling of Hydrosystems

Research Project funded by the German Research Fondation (DFG) - Project number 508470891


Karst systems in carbonate rocks are formed in the presence of water that is charged with carbonic acid. It is common knowledge in karst hydrology that the main sources of this CO2 are the activity of microorganisms in the soil and root respiration. The biological activity in soil is subject to seasonal fluctuations (e.g. Dreybrodt, 1998; Ford & Williams, 2007; White, 2018; Klimchouk et al., 2000, and many others). These textbooks and papers also explain that meteoric water is percolating through the unsaturated zone, where it dissolves the CO2. Consequently, corrosion of carbonate rocks starts preferably close to the ground surface, where it causes karst denudation. Karst hydrologists are challenged in explaining why caves with often large cavities form also deep inside the rock. There are currently most notably two accepted explanations. The first one is denoted as ‘mixing corrosion’ and was introduced by Bögli (1980). Mixing corrosion is explained by the always calcite-aggressive behavior of water that is mixed from two water streams, which are each in calco-carbonic equilibrium. This can happen, for example, in joints. The calcite-aggressive mixing water then has new potential to dissolve more carbonates and form cavities. A second explanation assumes non- linear dissolution kinetics, which says that water would keep some of its remaining potential for dissolving carbonates while it is penetrating deep into the rock. This was discussed, e.g., by Gabrovsek & Dreybrodt, 2000; Ford & Ewers, 1978; Dreybrodt, 2004; Kaufmann et al., 2014. A third explanation for CO2 replenishment, in the absence of percolating meteoric water, was recently proposed by us (Class et al., 2021a) and is concerned with density-driven dissolution of CO2 at the epiphreatic karst-water table (Figure 1). We are confident that our preliminary work has demonstrated the plausibility of our hypothesis (see below), but more evidence is still needed in order to substantiate its relevance relative to ‘classical’ theories.

Project leader

apl. Prof. Dr.-Ing. Holger Class


Kai  Wendel (M.Sc.)


  • Dr. Bettina Strauch, Deutsches GeoForschungsZentrum Helmholtz-Zentrum Potsdam
  • Dr. Martin Zimmer, Deutsches GeoForschungsZentrum Helmholtz-Zentrum Potsdam


1.2023 - 12.2025



This image shows Holger Class

Holger Class

apl. Prof. Dr.-Ing.

Akademischer Oberrat

This image shows Kai Wendel

Kai Wendel


Academic Staff

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