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Authors: Jerry A. Coyne

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Evolutionary theory, then, makes predictions that are bold and clear. Darwin spent some twenty years amassing evidence for his theory before publishing
The Origin.
That was more than a hundred and fifty years ago. So much knowledge has accumulated since then! So many more fossils found; so many more species collected and their distributions mapped around the world; so much more work in uncovering the evolutionary relationships of different species. And whole new branches of science, undreamt of by Darwin, have arisen, including molecular biology and systematics, the study of how organisms are related.
As we’ll see, all the evidence—both old and new—leads ineluctably to the conclusion that evolution is true.
Chapter 2
Written in the Rocks
The crust of the earth is a vast museum; but the natural collections have been made only at intervals of time immensely remote.
 

Charles Darwin,
On the Origin of Species
 
 
 
T
he story of life on earth is written in the rocks. True, this is a history book torn and twisted, with remnants of pages scattered about, but it is there, and significant portions are still legible. Paleontologists have worked tirelessly to piece together the tangible historical evidence for evolution: the fossil record.
When we admire breathtalting fossils such as the great dinosaur skeletons that grace our natural history museums, it is easy to forget just how much effort has gone into discovering, extracting, preparing, and describing them. Time-consuming, expensive, and risky expeditions to remote and inhospitable corners of the world are often involved. My University of Chicago colleague Paul Sereno, for instance, studies African dinosaurs, and many of the most interesting fossils lie smack in the middle of the Sahara Desert. He and his colleagues have braved political troubles, bandits, disease, and of course the rigors of the desert itself to discover remarkable new species such as
Afrovenator abakensis
and
jobaria tiguidensis,
specimens that have helped rewrite the story of dinosaur evolution.
Such discoveries involve true dedication to science, many years of painstaking work, persistence, and courage—as well as a healthy dose of luck. But many paleontologists would risk their lives for finds like these. To biologists, fossils are as valuable as gold dust. Without them, we’d have only a sketchy outline of evolution. All we could do would be to study living species and try to infer evolutionary relationships through similarities in form, development, and DNA sequence. We would know, for example, that mammals are more closely related to reptiles than to amphibians. But we wouldn’t know what their common ancestors looked like. We’d have no inkling of giant dinosaurs, some as large as trucks, or of our early australopithecine ancestors, small-brained but walking erect. Much of what we’d like to know about evolution would remain a mystery. Fortunately, advances in physics, geology, and biochemistry, along with the daring and persistence of scientists throughout the world, have provided these precious insights into the past.
Making the Record
FOSSILS HAVE BEEN KNOWN since ancient times: Aristotle discussed them, and fossils of the beaked dinosaur
Protoceratops
may have given rise to the mythological griffin of the ancient Greeks. But the real meaning of fossils wasn’t appreciated until much later. Even in the nineteenth century, they were simply explained away as products of supernatural forces, organisms buried in Noah’s flood, or remains of still-living species inhabiting remote and uncharted parts of the globe.
But within these petrified remains lies the history of life. How can we decipher that history? First, of course, you need the fossils—lots of them. Then you have to put them in the proper order, from oldest to youngest. And then you must find out exactly when they were formed. Each of these requirements comes with its own set of challenges.
The formation of fossils is straightforward, but requires a very specific set of circumstances. First, the remains of an animal or plant must find their way into water, sink to the bottom, and get quickly covered by sediment so that they don’t decay or get scattered by scavengers. Only rarely do dead plants and land-dwelling creatures find themselves on the bottom of a lake or ocean. This is why most of the fossils we have are of marine organisms, which live on or in the ocean floor, or naturally sink to the floor when they die.
Once buried safely in the sediments, the hard parts of fossils become infiltrated or replaced by dissolved minerals. What remains is a cast of a living creature that becomes compressed into rock by the pressure of sediments piling up on top. Because soft parts of plants and animals aren’t easily fossilized, this immediately creates a severe bias in what we can know about ancient species. Bones and teeth are abundant, as are shells and the hard outer skeletons of insects and crustaceans. But worms, jellyfish, bacteria, and fragile creatures like birds are much rarer, as are all terrestrial species compared to aquatic ones. Over the first 80 percent of the history of life, all species were soft-bodied, so we have only a foggy window into the earliest and most interesting developments in evolution, and none at all into the origin of life.
Once a fossil is formed, it has to survive the endless shifting, folding, heating, and crushing of the earth’s crust, processes that completely obliterate most fossils. Then it must be discovered. Buried deeply beneath the earth’s surface, most are inaccessible to us. Only when the sediments are raised and exposed by the erosion of wind or rain can they be attacked with the paleontologist’s hammer. And there is only a short window of time before these semiexposed fossils are themselves effaced by wind, water, and weather.
Taking into account all of these requirements, it’s clear that the fossil record must be incomplete. How incomplete? The total number of species that ever lived on earth has been estimated to range between 17 million (probably a drastic underestimate given that at least 10 million species are alive today) and 4 billion. Since we have discovered around 250,000 different fossil species, we can estimate that we have fossil evidence of only 0.1 percent to 1 percent of all species—hardly a good sample of the history of life! Many amazing creatures must have existed that are forever lost to us. Nevertheless, we have enough fossils to give us a good idea of how evolution proceeded, and to discern how major groups split off from one another.
Ironically, the fossil record was originally put in order not by evolutionists but by geologists who were also creationists, and who accepted the account of life given in the book of Genesis. These early geologists simply ordered the different layers of rocks that they found (often from canal excavations that accompanied the industrialization of England) using principles based on common sense. Because fossils occur in sedimentary rocks that begin as silt in oceans, rivers, or lakes (or more rarely as sand dunes or glacial deposits), the deeper layers, or “strata,” must have been laid down before the shallower ones. Younger rocks lie atop older ones. But not all layers are laid down at any one place—sometimes there’s no water to form sediments.
To establish a complete ordering of rock layers, then, you must cross-correlate the strata from different localities around the world. If a layer of the same type of rock, containing the same type of fossils, appears in two different places, it’s reasonable to assume that the layer is of the same age in both places. So, for example, if you find four layers of rock in one location (let’s label them, from shallowest to deepest, as ABDE), and then you find just two of those same layers in another place, interspersed with yet another layer—BCD—you can infer that this record includes at least five layers of rock, in the order, from youngest to oldest, of ABCDE. This
principle of superposition
was first devised in the seventeenth century by the Danish polymath Nicolaus Steno, who later became an archbishop and was canonized by Pope Pius XI in 1988—surely the only case of a saint making an important scientific contribution. Using Steno’s principle, the geological record was painstakingly ordered in the eighteenth and nineteenth centuries: all the way from the very old Cambrian to the Recent. So far, so good. But this tells you only the relative ages of rocks, not their
actual
ages.
Since about 1945 we have been able to measure the actual ages of some rocks—using radioactivity. Certain radioactive elements (“radioisotopes”) are incorporated into igneous rocks when they crystallize out of molten rock from beneath the earth’s surface. Radioisotopes gradually decay into other elements at a constant rate, usually expressed as the “half-life”—the time required for half of the isotope to disappear. If we know the half-life, how much of the radioisotope was there when the rock formed (something that geologists can accurately determine), and how much remains now, it’s relatively simple to estimate the age of the rock. Different isotopes decay at different rates. Old rocks are often dated using uranium-238 (U-238), found in the common mineral zircon. U-238 has a half-life of around 700 million years. Carbon-14, with a half-life of 5,730 years, is used for much younger rocks, or even human artifacts such as the Dead Sea Scrolls. Several radioisotopes usually occur together, so the dates can be cross-checked, and the ages invariably agree. The rocks that bear fossils, however, are not igneous but sedimentary, and can’t be dated directly. But we can obtain the ages of fossils by bracketing the sedimentary layers with the dates of adjacent igneous layers that contain radioisotopes.
Opponents of evolution often attack the reliability of these dates by saying that rates of radioactive decay might have changed over time or with the physical stresses experienced by rocks. This objection is often raised by “young-earth” creationists, who hold the earth to be six to ten thousand years old. But it is specious. Since the different radioisotopes in a rock decay in different ways, they wouldn’t give consistent dates if decay rates changed. Moreover, the half-lives of isotopes don’t change when scientists subject them to extreme temperatures and pressures in the laboratory. And when radiometric dates can be checked against dates from the historical record, as with the carbon-14 method, they invariably agree. It is radiometric dating of meteorites that tells us that the earth and solar system are 4.6 billion years old. (The oldest earth rocks are a bit younger—4.3 billion years in samples from northern Canada—because older rocks have been destroyed by movements of the earth’s crust.)
There are yet other ways to check the accuracy of radiometric dating. One of them uses biology, and involved an ingenious study of fossil corals by John Wells of Cornell University. Radioisotope dating showed that these corals lived during the Devonian period, about 380 million years ago. But Wells could also find out when these corals lived simply by looking closely at them. He made use of the fact that the friction produced by tides gradually slows the earth’s rotation over time. Each day—one revolution of the earth-is a tiny bit longer than the last one. Not that you would notice: to be precise, the length of a day increases by about two seconds every 100,000 years. Since the duration of a year—the time it takes the earth to circle the sun—doesn’t change over time, this means that the number of days per year must be decreasing over time. From the known rate of slowing, Wells calculated that when his corals were alive—380 million years ago if the radiometric dating was correct—each year would have contained about 396 days, each 22 hours long. If there was some way that the fossils themselves could tell how long each day was when they were alive, we could check whether that length matched up with the 22 hours predicted from radiometric dating.
But corals can do this, for as they grow they record in their bodies how many days they experience each year. Living corals produce both daily and annual growth rings. In fossil specimens, we can see how many daily rings separate each annual one: that is, how many days were included in each year when that coral was alive. Knowing the rate of tidal slowing, we can cross check the “tidal” age against the “radiometric” age. Counting rings in his Devonian corals, Wells found that they experienced about 400 days per year, which means that each day was 21.9 hours long. That’s only a tiny deviation from the predicted 22 hours. This clever biological calibration gives us additional confidence in the accuracy of radiometric dating.
The Facts
WHAT WOULD CONSTITUTE EVIDENCE for evolution in the fossil record? There are several types. First, the big evolutionary picture: a scan through the entire sequence of rock strata should show early life to be quite simple, with more complex species appearing only after some time. Moreover, the youngest fossils we find should be those that are most similar to living species.
We should also be able to see cases of evolutionary change within lineages : that is, one species of animal or plant changing into something different over time. Later species should have traits that make them look like the descendants of earlier ones. And since the history of life involves the splitting of species from common ancestors, we should be able to see this splitting—and find evidence of those ancestors—in the fossil record. For example, nineteenth-century anatomists predicted that, from their bodily similarities, mammals evolved from ancient reptiles. So we should be able to find fossils of reptiles that were becoming more mammal-like. Of course because the fossil record is incomplete, we can’t expect to document
every
transition between major forms of life. But we should at least find some.
When writing
The
Origin, Darwin bemoaned the sketchy fossil record. At that time we lacked transitional series of fossils or “missing links” between major forms that could document evolutionary change. Some groups, like whales, appeared suddenly in the record, without known ancestors. But Darwin still had some fossil evidence for evolution. This included the observation that ancient animals and plants were very different from living species, resembling modern species more and more as one moved up to more recently formed rocks. He also noted that fossils in adjacent layers were more similar to each other than to those found in layers more widely separated, implying a gradual and continuous process of divergence. What’s more, at any given place, the fossils in the most recently deposited rocks tended to resemble the modern species living in that area, rather than the species living in other parts of the world. Fossil marsupials, for instance, were found in profusion only in Australia, and that’s where most modern marsupials live. This suggested that modern species descended from the fossil ones. (Those fossil marsupials include some of the most bizarre mammals that ever lived, including a giant ten-foot kangaroo with a flat face, huge claws, and a single toe on each foot.)
BOOK: Why Evolution Is True
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