02.05.2013 Views

Evolution__3rd_Edition

Evolution__3rd_Edition

Evolution__3rd_Edition

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

..<br />

Figure 23.2<br />

The observed extinction rate<br />

for marine animals during<br />

the history of life, from the<br />

Cambrian to the present,<br />

expressed as percentages of<br />

genera going extinct per time<br />

unit (based on almost 29,000<br />

genera). Note the general<br />

decline, and the series of<br />

peaks (for mass extinctions).<br />

Terrestrial life shows a similar<br />

pattern, though there is less<br />

evidence. Redrawn, by<br />

permission of the publisher,<br />

from Sepkoski (1996).<br />

Two of the five are particularly<br />

striking ...<br />

. . . and define the three main<br />

phases of geological history<br />

% Extinction<br />

70<br />

60<br />

50<br />

40<br />

30<br />

20<br />

10<br />

0<br />

Late Cambrian<br />

End-Ordovician<br />

Late Devonian<br />

CHAPTER 23 / Extinction and Radiation 649<br />

End-Permian<br />

Late Triassic<br />

Ca O S D C P Tr J K T<br />

500 400 300 200 100 0<br />

Geological time (×10 6 years)<br />

Permian, the late Triassic, and the end of the Cretaceous. These are sometimes called<br />

the “big five.”<br />

Three of the “big five” are open to doubt. The three less certain mass extinctions are<br />

the ones in the late Ordovician, the late Devonian, and the late Triassic. The big five<br />

may therefore be reduced to a big four, big three, or even a big two, with the two most<br />

important mass extinctions being at the end of the Permian and the end of the<br />

Cretaceous. The end-Permian mass extinction is the biggest in history, with 80–96%<br />

(depending how the estimate is made) of species going extinct. In the Cretaceous–<br />

Tertiary mass extinction, at least half, and perhaps 60–75% of species went extinct.<br />

The observations now explained by mass extinctions have been known about for a<br />

long time. The geologists of the nineteenth century who worked out the main eras of<br />

the Earth’s history did so by looking for characteristic fossil faunas that lasted for a<br />

noticeable time (or rather, depth) in the sediments. Different characteristic faunas were<br />

recognized as different time periods. They recognized three large-scale faunal types and<br />

named them the Paleozoic, Mesozoic, and Cenozoic, with shorter term characteristic<br />

faunas within each of the three. Two major faunal transitions divide the three eras: the<br />

Permo-Triassic boundary, between the Paleozoic and Mesozoic, and the Cretaceous–<br />

Tertiary boundary, between the Mesozoic and Cenozoic. These two major faunal transitions<br />

correspond to the two main mass extinctions. Smaller transitions occurred<br />

between the stages within the main eras, and many of these correspond to smaller, but<br />

still elevated, peaks in Sepkoski’s (1996) graph (Figure 23.2).<br />

The extinction rate, in terms of number of species going extinct per million years,<br />

varies continuously through the history of life. Sometimes it is high, other times it is<br />

low, other times it is in between. No evidence exists for a distinct type of event that<br />

causes mass extinctions. The observed mass extinctions are just the times at the<br />

extreme of a continuum of extinction rates (Section 23.4 below). However, paleobiologists<br />

often study mass extinctions separately from the periods between, and for research<br />

K–T

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!