1
Introduction to Karst
Karst is the term used to describe a special style of landscape containing caves and extensive underground water systems that is developed on especially soluble rocks such as limestone, marble, and gypsum. Large areas of the ice-free continental area of the Earth are underlain by karst developed on carbonate rocks (Figure 1.1) and roughly 20–25% of the global population depends largely or entirely on groundwaters obtained from them. These resources are coming under increasing pressure and have great need of rehabilitation and sustainable management. In the chapters that follow, we show the close relationship between karst groundwater systems (hydrogeology) and karst landforms (geomorphology), both above and below the surface. And we explain the place of karst within the general realms of hydrogeology and geomorphology.
Experience shows that many hydrogeologists mistakenly assume that if karst landforms are absent or not obvious on the surface, then the groundwater system will not be karstic. This assumption can lead to serious errors in groundwater management and environmental impact assessment, because karst groundwater circulation can develop even though surface karst is not apparent. Diagnostic tests are available to clarify the situation. The prudent default situation in carbonate terrains is to assume karst exists unless proved otherwise.
We found in our first book (Ford and Williams 1989) that hydrological and chemical processes associated with karst are best understood from a systems perspective. Therefore we will continue to follow this approach here. Karst can be viewed as an open system composed of two closely integrated hydrological and geochemical subsystems operating upon the karstic rocks. Karst features above and below ground are the products of the interplay of processes in these linked subsystems.
1.1 DEFINITIONS
The word karst can be traced back to pre-Indoeuropean origins (Gams 1973a, 1991a, 2003; Kranjc 2001a). It stems from karra/gara meaning stone, and its derivatives are found in many languages of Europe and the Middle East. The district referred to as the ‘Classic Karst’, which is the type site where its natural characteristics first received intensive scientific investigation, is in the north-western corner of the Dinaric Karst, about two-thirds being in Slovenia and one-third in Italy. In Slovenia the word kar(r)a underwent linguistic evolution via kars to kras, which in addition to meaning stony, barrén ground also became the regional name for the district inland of Trieste. In the Roman period the regional name appeared as Carsus and Carso but, when it became part of the Austro-Hungarian Empire, it was germanicized as the Karst. The geographical and geological schools of Vienna during that time exercised a decisive influence on the word as an international scientific term. Its technical use started in the late 18th century and by the mid-19th century it was well-established. The unusual natural features of the Kras (or Karst) region became known as ‘karst phenomena’ and so too, by extension, did similar features found elsewhere in the world.
We may define karst as comprising terrain with distinctive hydrology and landforms that arise from a combination of high rock solubility and well developed secondary (fracture) porosity. Such areas are characterized by sinking streams, caves, enclosed depressions, fluted rock outcrops, and large springs. Considerable rock solubility alone is insufficient to produce karst. Rock structure and lithology are also important: dense, massive, pure and coarsely fractured rocks develop the best karst. Soluble rocks with extremely high primary porosity (~30–50%) usually have poorly developed karst. Yet soluble rocks with negligible primary porosity (<1%) that have later evolved a large secondary porosity support excellent karst. The key to the expression of karst is the development of its unusual subsurface hydrology, the evolution of which is driven by the hydrological cycle – the ‘engine’ that powers karst processes. The distinctive surface and subterranean features that are a hallmark of karst result from rock dissolution by natural waters along pathways provided by the geological structure.
Figure 1.1 Global distribution of major outcrops of carbonate rocks. Accuracy varies according to detail of mapping. Generalization occurs in areas with interbedded lithologies and where superficial deposits mask outcrops. (Map assembled using GIS on Eckert IV equal-area projection from regional maps, many of which were subsequently published in Gunn (2000a)).
The main features of the karst system are illustrated in Figure 1.2. The primary division is into erosional and depositional zones. In the erosional zone there is net removal of the karst rocks, by dissolution alone and by dissolution serving as the trigger mechanism for other processes. Some redeposition of the eroded rock occurs in the zone, mostly in the form of precipitates, but this is transient. In the net deposition zone, which is chiefly offshore or on marginal (inter- and supratidal) flats, new karst rocks are created. Many of these rocks display evidence of transient episodes of dissolution within them. This book is concerned primarily with the net erosion zone, the deposition zone being the field of sedimentologists (e.g. see Alsharhan and Kendall 2003).
Within the net erosion zone, dissolution along groundwater flow paths is the diagnostic characteristic of karst. Most groundwater in the majority of karst systems is of meteoric origin, circulating at comparatively shallow depths and with short residence times underground. Deep circulating, heated waters or waters originating in igneous rocks or subsiding sedimentary basins mix with the meteoric waters in many regions, and dominate the karstic dissolution system in a small proportion of them. At the coast, mixing between seawater and fresh water can be an important agent of accelerated dissolution.
In the erosion zone most dissolution occurs at or near the bedrock surface where it is manifested as surface karst landforms. We refer to forms as being small scale where their characteristic dimensions (such as diameter) are commonly less than ~10m, intermediate scale in the range of 10 to 1000 m, and large scale where dimensions are greater than 1000 m. In a general systems framework most surface karst forms can be assigned to input, throughput or output roles. Input landforms predominate. They discharge water into the underground and their morphology differs distinctly from landforms created by fluvial or glacial processes because of this function. Some distinctive valleys and flat-floored depressions termed poljes convey water across a belt of karst (and sometimes other rocks) at the surface and so serve in a throughput role. Varieties of erosional gorges and of precipitated or constructional landforms, such as travertine dams, may be created where karst groundwater is discharged as springs, i. e. they are output landforms. Residual karstic hills, sometimes of considerable height and abruptness may survive on the alluvial plains below receding spring lines and beside rivers.
Figure 1.2 The comprehensive karst system: a composite diagram illustrating the major phenomena encountered in active karst terrains. Reproduced from Ford, D.C. and Williams, P.W. (1989) Karst Geomorphology and Hydrology.
Some karsts are buried by later consolidated rocks and are inert, i.e. they are hydrologically decoupled from the contemporary system. We refer to these as palaeokarsts. They have often experienced tectonic subsidence and frequently lie unconformably beneath clastic cover rocks. Occasionally they are exhumed and reintegrated into the active system, thus resuming a development that was interrupted for perhaps tens of millions of years. Contrasting with these are relict karsts, which survive within the contemporary system but are removed from the situation in which they were developed, just as river terraces – representing floodplains of the past – are now remote from the river that formed them. Relict karsts have often been subject to a major change in baselevel. A high-level corrosion surface with residual hills now located far above the modern water table is one example; drowned karst on the coast another. Drained upper level passages in multilevel cave systems are found in perhaps the majority of karsts.
Karst rocks such as gypsum, anhydrite and salt are so soluble that they have comparatively little exposure at the Earth’s surface in net erosion zones, in spite of their widespread occurrence (Figure 1.3). Instead, they are protected by less soluble or insoluble cover strata such as shales. Despite this protection, circulating waters are able to attack them and selectively remove them over large areas, even where they are buried as deeply as 1000 m. The phenomenon is termed interstratal karstification and may be manifested by collapse or subsidence structures in the overlying rocks or at the surface. Interstratal karstification occurs in carbonate rocks also, but is of less significance. Intrastratal karstification refers to the preferential dissolution of a particular bed or other unit within a sequence of soluble rocks, e.g. a gypsum bed in a dolomite formation.
Reference is often made in European literature to exokarst, endokarst and cryptokarst. Exokarst refers to the suit of karst features developed at the surface. Endokarst concerns those developed underground. It is often divided into hyperkarst, in which the underground dissolution is by circulating meteoric waters, and hypokarst – dissolution by juvenile or connate waters (Figure 1.2). Some Russian authors further differentiate hypokarst into that dissolved in the soluble rocks by waters that are ascending into them from deeper formations, and that created entirely within a soluble formation by the process of pressure solution that utilizes its contained water. Cryptokarst refers to karst forms developed beneath a blanket of permeable sediments such as soil, till, periglacial deposits and residual clays. Karst barré denotes an isolated karst that is impounded by impermeable rocks. Stripe karst is a barré subtype where a narrow band of limestone, etc., crops out in a dominantly clastic sequence, usually with a stratal dip that is very steep or vertical. Recently there has been an emphasis on contact karst, where water flowing from adjoining insoluble terrains creates exceptionally high densities or large sizes of landforms along the geological contact with the soluble strata (Kranjc 2001b).
Figure 1.3 The global distribution of evaporite rocks (after Kozary, M.T. et al, Incidence of saline deposits in geologic time, Special Paper 88 © 1968 Geological Society of America). See Klimchouk and Andrejchuk (1996) for a global map of areas of gypsum and anhydrite deposition during the Precambrian and through the Palaeozoic.
Karst-like landforms produced by processes other than dissolution or corrosion-induced subsidence and collapse are known as pseudokarst. Caves in glaciers are pseudokarst, because their development in ice involves a change in phase, not dissolution. Thermokarst is a related term applied to topographic depressions resulting from thawing of ground ice. Vulcanokarst comprises tubular caves within lava flows plus mechanical collapses of the roof into them. Piping is the mechanical washout of conduits in gravels, soils, loess, etc., plus associated collapse. On the other hand, dissolution forms such as karren (see section 9.2) on outcrops of quartzite, granite and basalt are karst features, despite their occurrence on lithologies of that are of low solubility when compared with typical karst rocks.
The extent to which karst develops on lithologies other than carbonate and evaporite rocks depends largely on the efficiency of the processes that are competing with dissolution in the particular environment. If the competitors are very weak, the small-scale (karren) solutional landforms such as flutes, pits and pans can develop on monominerallic rocks of lower solubility and even on polyminerallic rocks such as granite and basalt, although rates of development appear to be lower. Quartzites and dense siliceous sandstones can be viewed as transitional, occupying part of the continuum between karst and normal fluvial landscapes. In thermal waters their solubility approaches that of carbonate rocks and regular solutional caves may form. Given sufficient time, under normal environmental temperatures and pressures intergranular dissolution of quartz along fractures and bedding planes can permit penetration of meteoric waters underground. When there is also a sufficient hydraulic gradient, this can give rise to turbulent flow capable of flushing the detached grains and enlarging conduits by a combination of mechanical erosion and further dissolution. Thus in some quartzite terrains vadose caves develop along the flanks of escarpments or gorges where hydraulic gradients are high. The same process leads to the unclogging of embryonic passages along scarps in sandy or argillaceous limestones. Development of a phreatic zone with significant water storage and permanent water-filled caves is generally precluded. The landforms and drainage characteristics of these siliceous rocks thus can be regarded as a style of fluvio-karst, i.e., a landscape and subterranean hydrology that develops as a consequence of the operation of both dissolution and mechanical erosion by running water.
1.2 THE RELATIONSHIPS OF KARST WITH GENERAL GEOMORPHOLOGY AND HYDROGEOLOGY
Geomorphology is concerned with understanding the form of the ground surface, the processes that mould it, and the history of its development. Carbonate and evaporate lithologies displaying at least some karst occur over ~20% of the Earth’s ice-free continental area and occupy a complete range of altitude and latitude. Thus karsts around the world are exposed to the full suite of geomorphological processes – aeolian, coastal, fluvial, glacial, physical and chemical weathering, etc. Hence to understand karst we must consider the same set of natural processes that affect all other rocks and landscape styles, including plate tectonics and climatic change. However, we must also recognize that dissolution is of paramount importance in developing karst compared with its relatively minor role in other lithologies. Chemical solution of karst rocks develops a distinctive suite of features (above and below ground) that reflect the dominance of dissolution and dissolution induced processes, such as collapse, compared with other processes. Even so, under extreme climatic conditions other processes, such as frost-shattering, can totally mask the effects of dissolution. Thus in high mountains, glacial, periglacial, and mass-movement processes are the principal landscape-forming agents. No karst has been reported on Mount Everest (Jolmo Lungma), for example, even though it consists mainly of carbonate rocks, although karst circulation may occur in the more stable regime underground.
Karst groundwater circulation can occur only if subterranean connections are established between uplands and valley bottoms; otherwise runoff will simply flow across the surface. Where bedrock is porous, as in many sandstones, water will infiltrate and circulate underground via interconnected pores, later to discharge at the surface as springs. In such rocks, the movement of water is by laminar flow and chemical solution has no significant effect on storage capacity and transmission of groundwater. Further, long-term circulation of water has no effect on the ultimate transmissivity or storage capacity of the groundwater system. This is not the case in karst, despite the fact that karst rocks are affected by exactly the same set of forces that drive subterranean groundwater circulation in other lithologies. This is because dissolution plays a fundamental role in karst. The very act of groundwater circulation causes progressive solutional enlargement of void space and a commensurate increase in permeability. Thus although initial groundwater flow in karst is laminar, it becomes progressively more turbulent. The karst groundwater system evolves over time, distinguishing it from other groundwater systems. Consequently, the equations that can be used to describe laminar water flow in typically porous aquifers become inapplicable to karst as the flow through large subterranean conduits becomes turbulent and dominates the groundwater throughput.
The progressive evolution of karst groundwater networks and the development of turbulent flow conditions are intimately related to the evolution of karst landforms. Although karst rocks may have primary intergranular porosity and secondary fracture porosity, most water flow through them is transmitted by conduits (tertiary porosity) developed by solution. These systems receive most of their inputs from point recharge sites at the surface, such as enclosed depressions (dolines, etc.) and stream-sinks, which also evolve over time as a consequence of dissolution. Thus both surface landscape and subterranean conduit system evolve together, an unusual circumstance applicable only to karst. For this reason, if one is to understand karst hydrogeology it is also necessary to understand karst geomorphology, and vice versa. This reality determines the structure and content of this book.
1.3 THE GLOBAL DISTRIBUTION OF KARST
The distribution of the principal karst rocks is shown in Figures 1.1 and 1.3. In the aggregate their surface and near-surface outcrops occupy ~20% of the planet’s dry ice-free land. Regional detail depicted on these maps is of variable quality depending on the information available. The mapping is also generalized and approximate; many very small outcrops are omitted, and possibly some large ones. Thus many sites shown on Figure 1.1 in Russia, for example, are areas in which carbonates are common, but not necessarily continuous in outcrop. Carbonates are particularly abundant in the Northern Hemisphere. The old Gondwana continents expose comparatively small outcrops except around their margins, where there are some large spreads of Cretaceous or later age carbonates (post break-up of the supercontinent), such as the Nullarbor Plain in Australia. Not all carbonates display distinctive karst landforms and/or significant karst groundwater circulations because some are impure and their insoluble residues clog developing conduits; thus we estimate carbonate karst to occur over 10–15% of the continental area.
Figure 1.3 shows the maximum aggregate of gypsum, anhydrite and salt known to have accumulated over geological time. Most of it is now buried beneath later carbonate or clastic (detrital) rocks. Also, many occurrences have been partly removed by dissolution or much reduced in geographical extent by folding and thrusting, e.g. in the Andes. More than 90% of the anhydrite/gypsum and more than 99% of the salt displayed here does not crop out; nevertheless, there is gypsum and/or salt beneath ~25% of the continental surfaces. Gypsum and salt karst that is exposed at the surface is much smaller in extent than the carbonate karst, but interstratal karst is of the same order of magnitude. Hydrologically active karst within these evaporite rocks probably covers an area comparable to active carbonate karsts.
1.4 THE GROWTH OF IDEAS
The Mediterranean basin is the cradle of karstic studies. Although ancient Assyrian kings between 1100 BC and 852 BC undertook the first recorded (in carvings and bronzes) explorations of caves in the valley of the Tigris River, Greek and Roman philosophers made the first known contributions to our scientific ideas on karst, as well as contributing to a mythology that, like the River Styx, lives on in the place names given by cavers and others. P...