Welcome to this lecture of the Origins course, where we will be looking at mass extinction
events. Mass extinctions are catastrophic events in
the history of our planet, where a large percentage of species disappeared within a relatively
short time span. This meant that dominating groups of organisms
disappeared, but also allowed new ones to radiate, drastically restructuring the fauna
and floras of the Earth, while redirecting the course of the history of life on the planet.
My name is Bent Lindow, and I am a vertebrate palaeontologist and educator at the Natural
History Museum of Denmark. This first video will review what defines
a mass extinction, and we will briefly look at the history of how scientists came to recognize
their importance in the history of life on Earth.
Finally, we will look at how geologists and palaeontologists study mass extinctions.
The second video will take us on a journey back to the greatest mass extinction of all
time some 251 million years ago, at the end of the Permian Age.
Here around 90% of Earth's species disappeared in just a few tens of thousands of years.
Finally, the third video will take us back some 65 million years and look at the Cretaceous-Tertiary
mass extinction, which claimed two thirds of Earth's species.
We will travel to a locality in eastern Denmark, which preserves physical evidence of this
disaster. Extinction is pretty much the norm for all
species on Earth, and eventually a species will either evolve into a new one, or go extinct.
98% of all known species are extinct. They are only known from fossils.
Through the lens of evolution, extinction is a breakdown of evolution, so to speak.
Evolution by natural selection is a process, whereby a species is continually adapted to
its environment and changes in it. However, if the environment changes too rapidly
for the species to adapt successfully, it disappears.
Evolution breaks down, so to speak. And as Earth's environments continually change
due to changes in climate and suchlike, extinction is perfectly normal.
It has been estimated that within a period of 1 million years, between 5 and 10% of the
all living species disappear. This is called the background extinction level.
At the same time, new species evolve, and the average duration of a species is set at
5 million years. However, this can vary between groups of organisms,
ranging from durations of 15 million years to as little as 100,000 years.
Mass extinctions are events or "biotic crises", where extinction rates suddenly peak above
the normal background extinctions. They are sudden short periods, where the amount
and diversity among living organisms plummet. The rate of extinction vastly outmatches the
origin rate of new species. In other words, many more species disappear
than newly evolved within a short time span. To qualify as a mass extinction event, geologists
and palaeontologists generally agree that it must display these common features:
More than 30% of Earth's species must disappear. The event must encompass a broad span of ecologies
and groups of organisms, both in the sea and on land.
It must be worldwide. And it must happen within a short time span.
Extinction level is significantly higher than background extinction rate
Before we delve into how modern scientists study mass extinction, it is worthwhile to
look at how the concept of mass extinction developed in the geological and palaeontological
sciences. Beginning in the early 1800s, geologists had
started to subdivide the past into a succession of different time periods.
At the time, the absolute age or duration of these periods was not known, as radiometric
dating would not be developed until the 1950s. Instead, the subdivisions were based on the
kind of fossils found in various rock layers. It was quickly noted that different species,
kinds of organisms and also faunal combinations characterized different time periods.
As one moved from one set of deposits or period to another, new taxa and organisms appeared,
and the previous ones disappeared. Indeed, a given taxon or species was only
found in one specific time span and would never reappear again later in the geological
column. This became known as the principle of faunal
succession - specific sets of various plants and animals living in one time period being
replaced by new sets. The question of why species disappeared rose
quickly. This gave rise to two revolutionary insights:
one was the notion of extinction - that a species or organism could disappear completely
from the surface of the Earth - and also the notion of catastrophism.
One of the main proponents of the idea catastrophes or properly termed "revolutions" in the prehistory
of the Earth was the French zoologist and palaeontologist Georges Cuvier.
Amongst others, in his time Cuvier founded the science of comparative anatomy, and showed
conclusively that species could even become extinct.
Now, Cuvier also worked on deposits in the area around Paris.
He pioneered the use of fossils as tools to correlate between geographically disparate
geological deposits. Here, he noted that layers containing the
fossil remains of land-living animals were topped by layers containing the fossil shells
and skeletons of sea-living animals. He also noted that there were large differences
between the land-living animals from one layer to another, while the marine animals changed
little from layer to layer. Cuvier used this to explain the extinction
and faunal successions of groups of organisms with catastrophes.
From time to time a worldwide revolution - probably a flooding event, where the sea rose, as indicated
by the fact that these events impacted much harder on terrestrial than marine animals,
would sweep over the planet, clean out and eliminate many species.
Following the catastrophic revolution, a new set of organisms would appear or be introduced.
These would then exist for a period of time, until they too were eradicated by a new catastrophe.
And so forth. Cuvier died in 1832.
And in his final years, another opposing viewpoint about the succession of life on Earth appeared
which quickly came to dominate at least the English-speaking part of geology: gradualism.
Between 1830 and 1833, English geologist and lawyer Charles Lyell published the three volumes
of his hugely influential book Principles of Geology.
In these books Lyell argued that only modern, observable phenomena were needed to explain
processes in the Earth's past - anything else was dangerous, un-scientific speculation.
Lyell's argument can be simply summed up as "the present is the key to the past".
In order to explain observations from the geological past, we should invoke natural
processes in the present by finding similar observations.
For example, on the wall behind me is a slab of rock with a number of parallel ridges on
it. The ridges are asymmetric: one slope is longer
than the other. All of the long slopes on all the ridges all
face in the same direction, while the short slopes all face in the other direction.
To explain these, I should go out and find a similar form in recent nature: current ridges
at the bottom of present-day streams. They are made of loose, unconsolidated sand,
but have the same shape as the fossilized ones on the surface of this rock.
By observing the present, I can explain the past: in this case what I have behind me is
a piece of the fossilized bed of an ancient stream.
Lyell elaborated much more on his concept, which he named the principle of uniformity
or uniformitarianism. However, he actually used uniformitarianism
in four different ways in his books: The first was Uniformity of law: The laws
of nature - such as chemical processes, the force of gravity and so forth - have been
constant through time. They have not changed.
Second was Uniformity of process: i.e. only observable modern phenomena and processes
should be used to interpret the past. This is also known as actualism - we use processes
observable in the present to explain events and processes in the past.
Thirdly: Uniformity of rate: Processes in the past must have occurred at the same rate
and scale as today. It is not allowable to imagine a process being
speedier or larger than anything observable in the present.
This notion is also known as gradualism. And fourth and finally: Uniformity of state:
Lyell considered that change on Earth was both in a dynamic balance and yet cyclical
- there is no progress in our planet's evolution. At any given time the climate, volcanism,
type of deposition and types of organisms are in some kind of balance.
Although the overall balance would change through time, at some point it would gradually
revert back to a previous equilibrium. For example, fossils indicated that the present
Tertiary era was a relatively cool period with large mammals dominating the land and
sea, with birds in the air. This had superseded the Mesozoic era, which
was a warm period, with large reptiles, dinosaurs, dominating the earth, the sea and the skies.
Lyell contented that further back in time - in the Silurian before the Mesozoic - the
climate would have been cooler and mammals would have been the dominant life-form once
more. Needless to say, Lyell's fourth principle
of "uniformity of state" was quickly refuted in the nineteenth century: fossils showed
that life on Earth had irreversibly progressed from simple to more complex forms and there
were no mammals in the Silurian. But Lyell's first, second and third principles
were to remain well-accepted amongst English-speaking geologists for over a hundred years.
Henning HaackAssociate Professor
James ConnellyProfessor
Vivi VajdaProfessor
Jon FjeldsåProfessor, Curator
Thomas GilbertProfessor
Michael Houmark-NielsenAssociate Professor
Bent Erik Kramer LindowCurator
Gilles Guy Roger CunyAssociate Professor
Ole SebergAssociate Professor
Gitte PetersenAssociate Professor
Tais Wittchen DahlAssistant Professor of Geobiology
Arne Thorshøj NielsenAssociate Professor
Martin Vinther SørensenAssociate Professor, Curator
Svend StougeAssociate Professor
Danny Eibye JacobsenAssociate Professor, Curator
Jan Audun RasmussenAssociate Professor
Emily Catherine PopeAssistant professor
