49 pages • 1 hour read
Elizabeth KolbertA modern alternative to SparkNotes and CliffsNotes, SuperSummary offers high-quality Study Guides with detailed chapter summaries and analysis of major themes, characters, and more.
In Gubbio, Italy, just north of Rome, Kolbert looks at the bands of limestone along the Gola del Bottaccione, a narrow gorge. Millions of years ago, this entire area was under water and was brought up by the same uplift that created the Apennine Mountains. Kolbert notes that walking through this area today is like walking through time.
In this same gorge, during the 1970s, Walter Alvarez, a geologist, discovered the first remnants of a giant asteroid that brought the Cretaceous period to an end. After the asteroid struck the earth, “some three-quarters of all species had been wiped out” (71). The impact of the asteroid can be seen today in a thin clay layer in the gorge that hundreds of tourists have stuck their fingers into.
Inspired by his mother, Alvarez became interested in geology, eventually earning a research post at the Lamont-Doherty Earth Observatory, where he began to study how the Italian peninsula was created through plate tectonics. Alvarez ended up working in Gubbio with geologist Isabella Premoli Silva, an expert on tiny sea creatures called Foraminifera (or forams). The two geologists noticed that the limestone from the Cretaceous period had many large, diverse forams but that right above it was a layer of clay that had no forams in it at all. Above this earth was limestone with more forams, but these were tiny and different from the larger ones below.
Alvarez realized that the limestone had captured points in time when extinctions had occurred, but he couldn’t immediately say how much time had passed between those points. He turned to his father, Luis, a Nobel Prize winner, for assistance. It was Alvarez’s father who thought to use iridium to determine the time frame between the layers of limestone and clay in the gorge.
Kolbert points out that iridium is rarely found on earth’s surface, but is found in meteorites. Luis Alvarez theorized that “the longer it had taken the clay layer to accumulate, the more cosmic dust would have fallen” and the more iridium it would contain (74). The men had samples of the clay sent to Berkley for testing, and nine months later, they received the news that the clay’s iridium levels were extremely high. After months of study, the Alvarezes developed what they termed an impact hypothesis:
“On an otherwise ordinary day sixty-five million years ago, an asteroid six miles wide collided with the earth. Exploding on contact, it released energy on the order of a hundred million megatons of TNT, or more than a million of the most powerful H-bombs ever tested. Debris, including iridium from the pulverized asteroid, spread around the globe. Day turned to night, and temperatures plunged. A mass extinction ensued.” (75)
The Alvarezes published a paper on their findings in 1980 to great acclaim, and their Cretaceous extinction theory became popular even among the general public. But within scientific circles, the Alvarezes and their argument were downplayed and dismissed, with many paleontologists disparaging the Alvarezes’ work as ignorant and simple.
According to Kolbert, the issue under debate stems back to Lyell and the initial division of life into three chapters: Paleozoic, Mesozoic, and Cenozoic. Because the fossils from each of these three periods were so different, John Phillips, Lyell’s contemporary and a geologist, had thought that each segment represented “distinct acts of creation” (76).
Differences of opinion led to increased tensions within the scientific community, with most paleontologists agreeing that some cosmic cataclysm may have taken place at the end of the Cretaceous period, but few believing it had resulted in any mass extinctions. However, it turned out that the Alvarezes were right, and in time, many set minds in the sciences slowly changed to adopt their theory. A key to that change was ammonites.
Kolbert explains that ammonites were small shelled creatures whose fossils can be found worldwide. They floated in shallow oceans for over 300 million years. Ammonites created spiral shells with multiple chambers and inhabited only the largest and last chamber themselves. Kolbert notes that “evolutionary development allowed ammonites to build shells that were at once light and robust—capable of withstanding many atmospheres’ worth of water pressure” (84). A distant relative of the octopus, ammonites probably liked living in water but were not the best swimmers.
Neil Landman, a paleontologist, shares with Kolbert his studies of ammonites and the previously accepted explanation for their extinction: that they just “d[ied] out” (85). But further studies, prompted by the Alvarezes’ paper, caused Landman to realize that ammonites were, in fact, thriving before the meteorite hit the earth at the end of the Cretaceous period. That impact resulted in the decimation of forests, the collapse of marine ecosystems, and the extinction on land of “every animal larger than a cat” (86)—including, of course, the dinosaurs.
Kolbert explains that Lyell’s reading of the fossil record, the interpretation that so many years of scientific work had been based on, only considered slow extinctions that appeared abruptly; in fact, relatively sudden extinctions actually looked drawn out in these scientific records. Lyell had been reading the record backward. The tiny forams found in the upper levels of clay in Gubbio, from the post-Cretaceous period, are proof of the shrunken, smaller creatures who survived or came into existence after this cataclysmic event. This phenomenon is called the Lilliput effect.
No one knows what part of the meteorite’s impact caused the ammonite to become extinct, although Kolbert theorizes that the animals’ inability to survive may be attributable to the small size of its eggs. In effect, Kolbert notes that all living organisms today have descended from an organism that survived this extinction period. But she argues that this survival has nothing to do with Darwin’s theory, for “how could a creature be adapted, either well or ill, for conditions it has never before encountered in its entire evolutionary history” (90)? Landman states that ammonites had been functioning and breeding perfectly well, with high distribution rates, but could not withstand an event that they were not evolutionarily prepared to survive.
Kolbert references an undergraduate study conducted at Harvard in 1948 that focused on perception, how it changes, and why it changes. Thomas Kuhn, a famous twentieth-century scientist, was fascinated by this playing card experiment because “it revealed how people process disruptive information” (92). Man’s first instinct is to push that information into familiar and known settings, and any signs of anything amiss or out of the ordinary are ignored until they can’t be avoided any longer. That moment of crisis is called the “My God! reaction” by scientists (92).
To Kuhn, this experiment’s results made perfect sense. Any information that didn’t fit the accepted theories, standards, or beliefs of the day would be dismissed or explained away for as long as possible. From this concept came Kuhn’s term “paradigm shift,” or, in his words, “novelty emerging only with difficulty” (93), which was, in essence, his explanation for why scientists were so reluctant to abandon old traditional modes of thinking for newer, more accurate ones.
Broad paradigm shifts in scientific thinking were prompted by the paradigm shift that acknowledged the cataclysmic events that had caused mass extinctions. While Lyell and Darwin had stubbornly argued that extinction was a slow, lonely event, the Alvarezes’ discovery provided proof that catastrophes had happened and that whole species could be wiped out in a short time. The reluctance to embrace the Alvarezes’ stance, and its slow acceptance, is an example of Kuhn’s paradigm shift.
To further explore this paradigm shift, Kolbert visits Scotland, where she examines the rocks in Dob’s Linn, which date back roughly 445 million years to the end of the Ordovician period. That was a time when the land on earth was one conjoined mass, and a time directly following the prolific Cambrian period, when a multitude of new life forms appeared. During this time, the first reefs appeared, and the first plants began to grow and spread on land.
Then, 444 million years ago, nearly 85 percent of marine species died off. Initially, scientists thought a small catastrophe had happened at this time, but today this moment is considered the first of the Big Five extinctions, an extinction caused by a natural force.
In Scotland, Kolbert discusses the graptolite, a small marine organism that thrived before the end of the Ordovician period, then nearly died out in the extinction event that followed. The sensitive and delicate frame of these creatures meant they made excellent fossils for identifying the ages of successive layers of rock. Kolbert describes the physical changes that occurred in this small animal over time, some of its attributes being lost forever. She draws a comparison between the tiny graptolite and the mighty dinosaurs, both being “highly successful form[s] relegated to oblivion” (99).
By 1984, scientists had determined that aside from the five major mass extinctions, there had been lesser extinction events as well. They argued that extinctions occurred periodically, which spawned theories such as the “Nemesis” star or “death-star theory,” which was alternately celebrated and panned in the media. Luis Alvarez went so far as to travel to southern China to obtain rock samples, expecting to find iridium levels on par with those in Gubbio, only to be disappointed when the levels were minuscule at best. Eventually, the iridium levels were “attributed to the vagaries of sedimentation” (102).
Gradually, the theory developed that the mass extinction at the end of the Ordovician was caused by climate change, specifically glaciation. A greenhouse climate had rapidly changed at this time, with carbon dioxide levels dropping. Temperatures fell, sea levels dropped, the ocean’s chemistry changed, and animals died off, including the graptolites.
This situation contrasts with the extinction event at the end of the Permian period, when a massive release of carbon into the air raised temperatures to the point where species were eliminated. Kolbert thus theorizes that each mass extinction event was unique unto itself. All they have in common is “the very freakishness of the events …[;] all of a sudden, organisms find themselves facing conditions for which they are, evolutionarily, unprepared” (103).
Kolbert considers the role of human beings in current times, and what our role will look like to scientists of the future. According to her Scottish guide, Zalasiewicz, “We have already left a record that is now indelible” (105). For example, Kolbert discusses the nomadic movements of human beings, and how those travels have wrought unexpected and unplanned havoc on the environment. She uses rats as a prime example of creatures that have been found in all corners of the world and could only be there because they traveled with humans to those places. Rat populations then exploded due to a lack of predators, and in some areas of the world, the number of rats caused irreversible impacts on other species. Kolbert cites the Norway rat (actually from China) as destroying reptile and bird populations and creating its own “ecospace” (105).
Scientists have argued about what to call the current age of the Earth, and it was Danish chemist Paul Crutzen who used the word “Anthropocene” to describe this most recent epoch, beginning 11,700 years ago. Crutzen felt the term was wholly appropriate due to the dominance of humanity during this period and to the geological changes that have occurred due to human activity. Crutzen’s suggestion convinced Zalasiewicz, and, as the head of the Anthropocene Working Group, he hopes to have the term officially accepted and adopted as the name of the newest and current epoch.
Kolbert next visits the tiny island of Castello Aragonese, just west of Naples, due to its formation by the pressure of the African and Eurasian plates pushing into each other. This phenomenon causes gas to vent out of the sea floor, a gas that is almost wholly carbon dioxide. Kolbert is given a chance to see the vents with two marine biologists, Maria Christina Buia and Jason Hall-Spencer. In the water, Kolbert examines sea urchins and other marine life, but she notes that the closer they get to the bubbling vents, the less marine life they find.
Kolbert relates this expedition to the ecological damage done by human beings since the start of the Industrial Revolution. The burning of fossil fuels and deforestation have added significant amounts of carbon to the atmosphere. The result is that higher levels of carbon now exist in the air than at any other time in the last 800,000 years. By 2050, carbon levels are expected to help raise the earth’s temperature between 3.5 and 7 degrees Fahrenheit, causing a series of worldwide, permanent events such as the melting of ice caps and flooding of coastal cities.
Because the Castello Aragonese vents are a preview of what oceans will look like in the next thirty years, Kolbert wants to examine them to understand better what will happen to marine environments and why. She enters the local marine biological station to observe the specimens they have in tanks. All the aquatic animals have suffered in some physiological way due to the high levels of carbon to which they’ve been exposed. Hall-Spencer explains that “some of these lower organisms … just got to tolerate what’s happening outside, and so they get pushed beyond their limits” (116).
The Castello Aragonese vents are a perfect example of what the world’s oceans will be like in a relatively short period. The closer one moves toward the vents, the higher the acidity of the water (i.e., the lower the pH level). Kolbert reasons that this area is “like having access to an underwater time machine” (116). Despite this notion, Hall-Spencer notes that it took some convincing to get his studies funded to test his theory; when it finally was, scientists found that even the most well-known and widespread marine life, like mussels and barnacles, were nowhere to be found near the vents.
Most alarming, according to Hall-Spencer, is that the marine ecosystem will begin to crash when pH levels hit 7.8, a level expected to be reached by the year 2100. Although some marine life will learn to thrive and survive, the acidification of the ocean will exterminate many other species, from the recognizable clownfish to other less recognizable animals essential to proper marine ecosystem functions. The main result, according to Ulf Riebesell, a biological oceanographer in Germany, is that “there is going to be a reduction in biodiversity” (120). In short, ocean acidification will have a significant enough impact to be considered a catastrophic event.
Kolbert explains why ocean acidification is so deadly, namely that it will affect basic ecological and physiological functions such as metabolism, change the amount of light passing through water, alter the availability of nitrogen and iron, and impact the level of noise in the water. It may also promote more rapid growth of algae, impact photosynthesis, and affect the way compounds are formed by dissolved metals, potentially causing toxicity.
Of all these possible effects, Kolbert is most concerned about the impact on marine calcifiers, small creatures who build shells or external skeletons. Starfish, clams, oysters, mollusks, and sea urchins are examples of calcifiers. To produce calcification, these animals “alter the chemistry of the water to, in effect, impose a chemistry of their own” (121). Ocean acidification destroys the efforts of these calcifiers by requiring the animals to expend more energy in an attempt to calcify, and once the water reaches corrosive acidic levels, the calcium carbonate of these marine creatures dissolves.
The carbon spewing from the Castello Aragonese vents has been doing so for centuries, and no calcifier has been able to adapt to the change in pH, or we would have proof of it. Ocean acidification will most likely result, therefore, in the extinction of many of these marine animals. Kolbert posits that this news is made worse by how quickly it is occurring, thanks to human damage being done daily to the environment.
In these chapters, Kolbert travels to multiple locations in order to provide modern examples of environmental impact while also discussing the means and methods by which scientific theories have been posed, argued, dismissed, and established with regard to whether the earth is facing another extinction event.
Kolbert investigates the ammonite bands of fossils found in clay deposits within the gorge walls in Gubbio, Italy, and discusses how these segments prompted the Alvarezes’ theory regarding large extinction events, especially the meteorite that preceded the end of the Cretaceous period, as well as how that theory was argued and proven in some ways but disproven in others. The ammonites themselves provide proof of a thriving species that was not evolutionarily equipped to handle a sudden cataclysmic change in environment.
In Scotland, Kolbert examines the ancient rocks at Dob’s Linn and studies the role of the small marine graptolite as an example of how environmental damage caused by human beings has irreversibly impacted the Earth. The term “Anthropocene” is posed as an apt name for the current epoch because of the biological, ecological, and physiological changes that are happening now due to human activity.
Visiting the Castello Aragonese allows Kolbert the opportunity to see ocean acidification in action and to reflect on what devastating impact it may have within only a matter of decades. The high amount of carbon in the air due to human activity not only changes animals’ abilities to complete essential physical functions but may also lead to extinctions via a sizeable cataclysmic event.
By Elizabeth Kolbert