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Evolution__3rd_Edition

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..<br />

Position (m)<br />

300<br />

340<br />

330<br />

KT<br />

0 100 200<br />

Ir (ppt)<br />

An iridium anomaly is associated<br />

with the KT boundary<br />

Peak at<br />

3,000 ppt<br />

CHAPTER 23 / Extinction and Radiation 651<br />

Figure 23.4<br />

The iridium (Ir) concentration increases suddenly by 2–3 orders<br />

of magnitude at the Cretaceous–Tertiary (KT) boundary rocks<br />

at Gubbio, Italy. (100 ft ≈ 39.5 m.) Redrawn, by permission of<br />

the publisher, from Alvarez et al. (1990). © 1990 American<br />

Association for the Advancement of Science.<br />

purposes it is convenient to distinguish between “mass extinctions” and “background<br />

extinctions.” Background extinctions are the extinctions that are going on all the time,<br />

even when the extinction rate is not exceptionally high.<br />

23.3.2 The best studied mass extinction occurred at the<br />

Cretaceous–Tertiary boundary<br />

The mass extinction at the end of the Cretaceous has been found in all regions of the<br />

globe, and affected more or less every group of plants and animals (Figure 23.3). The<br />

fossil record of small, abundant, microfossil groups such as Foraminifera provides<br />

the best evidence for the fine-scale pattern of the extinction, but the demise of larger<br />

groups provides its drama. Some groups, such as the dinosaurs and ammonites, were<br />

driven finally extinct; most large groups were drastically reduced in diversity, though<br />

some odd groups, such as crocodiles, were not noticeably affected at all. The obvious<br />

question is: why did it happen?<br />

In 1980, Alvarez et al. published an influential observation. They sampled the rocks<br />

of the Cretaceous–Tertiary boundary from Gubbio in Italy, and found exceptionally<br />

large concentrations of rare earth elements, particularly iridium (Figure 23.4). These<br />

elements also have high concentrations in extraterrestrial objects. Alvarez and his colleagues<br />

explained the biological mass extinction, and the geochemical iridium anomaly,<br />

by the collision of a large asteroid with the Earth. Since then, similar iridium anomalies<br />

have been found in Cretaceous–Tertiary boundary rocks at several other sites. Some<br />

geologists have argued that the iridium anomaly could have had a terrestrial cause, by<br />

volcanic eruptions; but asteroids are the most widely accepted explanation.

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