EVIDENCE FOR CLIMATIC VARIATION WITHIN THE ~2.0 GA UPPER MAKGABENG FORMATION, SOUTH AFRICA
The upper Makgabeng Formation is broken into a lower and upper paleo-dune field/erg by a playa or saline pan deposit. The lower dune field consists of meter-scale dune sets with interbedded lenses of wet interdune strata, up to 60 cm in thickness and traceable to a maximum of 55 m. The overlying inferred playa reflects considerable variation in precipitation. The basal playa deposit consists of alternating mud and sandstone beds with both deep and shallow penetrating mud cracks. Above this lower mud-phase, the playa is fully sand dominated, featuring wave- and current-ripples, low-angle eolian wind-ripple stratification, scour marks, potential evaporitic crust features and evaporite dissolution structures. Overlying the playa is the upper dune field that consists of laterally continuous thick eolian sets with sparse, thin lenses of dry interdune deposits. Characterizing the upper dune field is a vertical transition from medium- to coarse-grained sandstone. In addition to the grain size change, fluvial, sheet-flood deposits, eolian cross-beds sculpted by mass flows, and a geographically restricted playa sequence is recognizable.
These facies demonstrate shifts in precipitation that are reflected in changing water table levels. Fluvial and playa facies record high water tables. Low water tables are reflected in the erg deposits. The transition from low to higher water tables is recorded in the appearance of wet interdunes and massive flow interspersed within the dune strata. These climatic alterations, in precipitation levels, radically changed the Makgabeng landscape through time.