Mass Extinctions

Mass Extinctions
When we study evolutionary change on an even larger timescale, we observe periodic events in which large numbers of taxa go extinct simultaneously. These events are called mass extinctions (see Figure 6-32). The most cataclysmic of these extinction episodes happened about 225 million years ago, when at least half of the families of shallow-water marine invertebrates, and fully 90% of marine invertebrate species disappeared within a few million years. This event was the Permian extinction. The Cretaceous extinction, which occurred about 65 million years ago, marked the end of the dinosaurs, as well as numerous marine invertebrates and many small reptilian taxa.

Twin craters of Clearwater Lakes in Canada show that multiple impacts on the earth are not as unlikely as they might seem. Evidence suggests that at least two impacts within a short time were responsible for the Cretaceous mass extinction.
Figure 6-34 Twin craters of Clearwater
Lakes in Canada show that multiple
impacts on the earth are not as unlikely as
they might seem. Evidence suggests that
at least two impacts within a short time
were responsible for the Cretaceous mass
extinction.
The causes of mass extinctions and their occurrence at intervals of approximately 26 million years are difficult to explain. Some people have proposed biological explanations for these periodic mass extinctions and others consider them artifacts of our statistical and taxonomic analyses. Walter Alvarez proposed that the earth was periodically bombarded by asteroids, causing these mass extinctions (Figure 6-34). The drastic effects of such bombardment of a planet were observed in July 1994 when fragments of Comet Shoemaker-Levy 9 bombarded Jupiter. The first fragment to hit Jupiter was estimated to have the force of 10 million hydrogen bombs. Twenty additional fragments hit Jupiter within the following week, one of which was 25 times more powerful than the first fragment. This bombardment was the most violent event in the recorded history of the solar system. A similar bombardment on earth would send debris into the atmosphere, blocking sunlight and causing drastic changes of climate. Temperature changes would challenge ecological tolerances of many species. Alvarez’s hypothesis is being tested in several ways, including a search for impact craters left by asteroids and for altered mineral content of rock strata where mass extinctions occurred. Atypical concentrations of the rareearth element iridium in some strata imply that this element entered the earth’s atmosphere through asteroid bombardment.

Sometimes, lineages favored by species selection or effect macroevolution are unusually susceptible to mass extinction. Climatic changes produced by the hypothesized asteroid bombardments could produce selective challenges very different from those encountered at other times in the earth’s history. Selective discrimination of particular biological traits by events of mass extinction is termed catastrophic species selection. For example, mammals survived the end-Cretaceous mass extinction that destroyed the dinosaurs and other prominent vertebrate and invertebrate groups. Following this event, mammals were able to use environmental resources that previously had been denied them, leading to their adaptive radiation.

Natural selection, species selection, effect macroevolution, and catastrophic species selection interact to produce the macroevolutionary trends that we see in the fossil record. Studies of these interacting causal processes have made modern evolutionary paleontology an active and exciting field.