Abstract
Indirect indicators are critically important for recognizing hypogene karst that is too deep-seated to have explorable hypogene caves. We have suggested in previous publications that an extensive network of non-tectonic synclines in otherwise flat-lying Eocene limestone in Egypt might be such an indirect indicator. We proposed that synclines formed by sag of limestone layers overlying a zone of hypogene karst that today remains deep below the surface and suggested that hypogene speleogenesis resulted from ascending aggressive fluids associated with crustal extension and magmatism in Egypt during Red Sea Rift initiation. Without hypogene caves to explore, however, we were unable to provide compelling evidence for hypogene karst processes. By doubling our mapping area from 4,000 to 8,000 km2, a clear picture has emerged of patterns in the syncline network that provide compelling evidence for hypogene speleogenesis. Over this larger area, the network displays two distinct patterns: 1) synclines and ridges that outline polygons 700–2,000 m across, and 2) narrow N–S zones of synclines spaced 5–10 km apart, with WNW–ESE to NW–SE trending shallow synclines and ridges traversing the panels between N–S zones. The geometries suggest that the syncline network is controlled by two structural patterns in rocks underlying the limestones: 1) polygonal faults in underlying shales and 2) reactivated N–S, left-lateral basement faults that are largely blind at the current level of erosion. These structures served as conduits that conveyed fluids upward into the overlying Eocene limestones, triggering dissolution at depth and a pattern of sag above that was inherited from the nature and pattern of faults and fractures in rocks underlying the limestones. The unique patterns and characteristics of this network of synclines are applicable elsewhere as an indirect indicator of deep-seated hypogene karst. Our new data also strongly suggest that syncline formation spanned the time of crustal extension in Egypt associated with onset of Red Sea rifting ∼23–22 Ma. Endogenic CO2 associated with mantle-derived basaltic magmas was likely a significant component of fluids, perhaps involving highly aggressive supercritical CO2. Mantle-derived C and He in modern Egyptian oasis water suggest that hypogene speleogenesis may still be locally active.
Highlights
Over the past 25 years, hypogene karst has been recognized and studied on every continent across the globe (Klimchouk et al, 2017, which contains 61 papers from occurrences all over the world)
The features of the syncline network provide no direct evidence for hypogene speleogenesis, we suggested that sag in overlying limestone layers might provide indirect evidence of hypogene speleogenesis at depth
We show that the syncline pattern varies systematically across the region and is strongly controlled by the pattern of fault and fracture networks in units underlying the limestones, especially the Esna Formation, suggesting upward fluid flow and supporting a model of hypogene speleogenesis at depth in the limestones, with sag in overlying layers
Summary
Over the past 25 years, hypogene karst has been recognized and studied on every continent across the globe (Klimchouk et al, 2017, which contains 61 papers from occurrences all over the world). The features that we think of as diagnostic of hypogene speleogenesis will remain inaccessible and essentially invisible unless uplift and erosion exposes the hypogene karst zone for exploration. For hypogene karst systems that remain inaccessible in the subsurface, the challenge becomes how we might detect the presence of hypogene karst systems that are too deep to be explored. Is it possible, for example, to find areas where the features at the surface might be the “smoking gun” that indicates the presence of hypogene karst at depth?. The plateau stands 200–350 m above the Nile Valley to the east and the Kharga Valley to the west and is flanked by escarpments on both sides. The vast majority of the plateau is remote and inaccessible
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