There have been five mass extinctions in Earth’s history

There have been five big mass extinctions in Earth’s history – these are called the “Big Five”. Understanding the reasons and timelines of these events is important to understand the speed and scale of species extinctions today.

When and why did these mass extinction events happen?

First, we must be clear on what we mean by “mass extinction”. Extinctions are a normal part of evolution: they occur naturally and periodically over time.¹

There’s a natural background rate to the timing and frequency of extinctions: 10% of species are lost every million years, 30% every 10 million years, and 65% every 100 million years.² It would be wrong to assume that species going extinct is out of line with what we would expect. Evolution occurs through the balance of extinction – the end of species – and speciation – the creation of new ones.

Extinctions occur periodically at what we would call the “background rate”. We can therefore identify periods of history when extinctions were happening much faster than this background rate – this would tell us that there was an additional environmental or ecological pressure creating more extinctions than we would expect. 

However, mass extinctions are periods with much higher extinction rates than normal. They are defined by both magnitude and rate. Magnitude is the percentage of species that are lost. Rate is how quickly this happens. These metrics are inevitably linked, but we need both to qualify as a mass extinction.

In a mass extinction, at least 75% of species go extinct within a relatively (by geological standard) short period of time.³ Typically less than two million years.

There have been five mass extinction events in Earth’s history, at least since 500 million years ago. We know very little about extinction events in the Precambrian and early Cambrian earlier, which predate this.⁴ These are called the “Big Five” for obvious reasons.

In the chart, we see the timing of events in Earth’s history.⁵ It shows the changing extinction rate (measured as the number of families that went extinct per million years). Again, note that this number was never zero: background extinction rates were low – typically less than 5 families per million years – but ever-present.

We see the spikes in extinction rates marked as the five events:

1. End Ordovician (444 million years ago; mya)
2. Late Devonian (360 mya)
3. End Permian (250 mya)
4. End Triassic (200 mya) – many people mistake this as the event that killed off the dinosaurs. But in fact, they were killed off at the end of the Cretaceous period – the fifth of the “Big Five”.
5. End Cretaceous (65 mya) – the event that killed off the dinosaurs.

Finally, at the end of the timeline, we have the question of what will come. Perhaps we are headed for a sixth mass extinction. But we are currently far from that point.

There are a range of trajectories that the extinction rate could take in the decades and centuries to follow; which one we follow is determined by us.

All of the “Big Five” were caused by some combination of rapid and dramatic changes in climate, combined with significant changes in the composition of environments on land or the ocean (such as ocean acidification or acid rain from intense volcanic activity).

In the table here, I detail the proposed causes for each of the five extinction events.⁶