Permian extinction, also called Permian-Triassic extinction or end-Permian extinction, a series of extinction pulses that contributed to the greatest mass extinction in Earth’s history. Many geologists and paleontologists contend that the Permian extinction occurred over the course of 15 million years during the latter part of the Permian Period (299 million to 252 million years ago). However, others claim that the extinction interval was much more rapid, lasting only about 200,000 years, with the bulk of the species loss occurring over a 20,000-year span near the end of the period. The Permian extinction was characterized by the elimination of about 90 percent of the species on Earth, which included more than 95 percent of the marine species and 70 percent of the terrestrial species. In addition, more than half of all taxonomic families present at the time disappeared. This event ranks first in severity of the five major extinction episodes that span geologic time.

Shallow warm-water marine invertebrates, which included the trilobites, rugose and tabulate corals, and two large groups of echinoderms (blastoids and crinoids), show the most-protracted and greatest losses during the Permian extinction. Using the maximum number of different genera in the middle part of the Guadalupian Epoch (about 272.3 million to 259.8 million years ago) as a benchmark, extinction within marine invertebrate faunas significantly reduced the number of different genera by 12 to 70 percent by the beginning of the Capitanian Age some 266 million years ago. The diversity levels of many of these faunas plummeted to levels lower than at any prior time in the Permian Period. Extinctions at the boundary between the Guadalupian and Lopingian epochs (259.8 million to 252.2 million years ago) were even more severe—bordering on catastrophic—with a reduction of 70 to 80 percent from the Guadalupian generic maxima. A great many invertebrate families, which were highly successful prior to these extinctions, were affected.

The series of extinction episodes that occurred during both the last stage of the Guadalupian Epoch and throughout the Lopingian Epoch, each apparently more severe than the previous one, extended over about 15 million years. Disruptive ecological changes eventually reduced marine invertebrates to crisis levels (about 5 percent of their Guadalupian maxima)—their lowest diversity since the end of the Ordovician Period. The final extinction episode, sometimes referred to as the terminal Permian crisis, while very real, took 15 million years to materialize and likely eliminated many ecologically struggling faunas that had already been greatly reduced by previous extinction episodes leading up to the terminal Permian crisis.

The Permian extinction was not restricted to marine invertebrates. Several groups of aquatic vertebrates, such as the acanthodians, thought to be the earliest jawed fishes, and the placoderms, a group of jawed fishes with significant armour, were also eliminated. Notable terrestrial groups, such as the pelycosaurs (fin-backed reptiles), Moschops (a massive mammal-like reptile), and numerous families of insects also met their demise. In addition, a number of groups (such as sharks, bony fishes, brachiopods, bryozoans, ammonoids, therapsids, reptiles, and amphibians) experienced significant declines by the end of the Permian Period.

Causes

Temperature crises

Although other single-event causes have been suggested, current explanations of Permian extinction events have focused on how biological and physical causes disrupted nutrient cycles. Hypotheses of temperature crises, especially of those occurring in shallow marine (surface) waters, are based in part on studies of oxygen isotopes and the ratios of calcium to magnesium in Permian fossil shell materials. The highest estimated temperatures of ocean surface waters (estimated to be 25–28 °C [about 77–82 °F]) until that time occurred during the end of the Guadalupian Epoch and the beginning of the Lopingian Epoch. Subsequently, by the end of the Lopingian Epoch, calcium-to-magnesium ratios suggest that water temperatures may have dropped to about 22–24 °C (about 72–75 °F), decreasing further during the very beginning of the Triassic Period. One hypothesis proposes that water temperatures greater than 24–28 °C (about 75–82 °F) may have been too warm for many invertebrates; only those specialized for high temperatures, such as those living in shallow lagoons, survived.

Alteration of the carbon cycle

The ratio between the stable isotopes of carbon (12C/13C) seems to indicate that significant changes in the carbon cycle took place starting about 500,000 to 1,000,000 years before the end of the Permian Period and crossing the boundary into the Induan Age (the first age of the Triassic Period). These changes appear to coincide closely with two Permian extinction events, suggesting some cause-and-effect relationship with changes in the carbon cycle.

Several studies have suggested that changes in the carbon isotope record may indicate a disrupted biological cycle. Some scientists consider the unusually high amounts of 12C trapped in Permian sediments to be a result of widespread oceanic anoxia (very low levels of dissolved oxygen). They associate this anoxia with the prolonged eruption of the Siberian flood basalts (the so-called Siberian Traps), which probably led to higher levels of carbon dioxide in the atmosphere. Clouds of volcanic ash may have worsened the situation by restricting the amount of sunlight available for photosynthesis, thereby inhibiting the process of carbon fixation by plants and lowering the extraction rate of carbon dioxide from the atmosphere. In addition, high amounts of carbon dioxide may have been injected into the atmosphere by the venting of volcanic gases from the eruption of flood basalts, combined with the ignition of large coal seams, or by the burning of forests by hot lava.

The Great Dying: The Permian Mass Extinction :nuke:

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