Permian reefs re-examined: extrinsic control mechanisms of gradual and abrupt changes during 40 my of reef evolution

Abstract

The evolution of Permian reefs is characterized by the following sequence of events: (1) Late Carboniferous–Cisuralian radiation, (2) early Late Cisuralian (Artinskian–Kungurian) turnover, (3) Guadalupian radiation, (4) end-Guadalupian crisis, (5) Lopingian radiation, (6) end-Lopingian crisis at the PTB (Permian–Triassic boundary), and (7) the at least 7 my (million years) metazoan reef gap during the Early Triassic. The early Late Cisuralian turnover and the end-Guadalupian reef crisis are gradual changes, while the end-Lopingian reef crisis represents an abrupt event. Lopingian reefs occur in a zone from 40 °N to 15 °S, Guadalupian reefs in an extended equatorial zone from 35 °N to 35 °S, and Lopingian reefs in a narrow equatorial zone of 20 °N and 20 °S. This pattern resulted from a network of global and regional control mechanisms including the assemblage of Pangea, the northward drift of continents, the opening of Neo-Tethys, and second-order sea level changes. The mechanism of the extinction has been intensely debated and a combination of the above mentioned long-term changes and abrupt ocean anoxia or hypercapnia (CO 2-poisoning) for the end-Guadalupian reef crisis is considered.