How Volcanoes Froze the Earth (Twice)

Summary

Highlights

• The Earth turned into a giant snowball not once but twice between 716 and 635 million years ago! 🧊
• Dropstones and carbonates reveal extensive historical glaciation even at the equator. 🪨
• Initial hypotheses included Earth flipping on its side due to unlikely equatorial ice findings. 🤯
• The breakup of Rodinia disrupted CO2 levels, leading to massive glaciations. 🌍
• Volcanic sulfur eruptions added to the cooling, kickstarting the ice ages. 🌋
• Runaway icehouse effect kept Earth in a frozen state until volcanoes released enough CO2 to warm it up. 🥶
• The Cryogenian period ended as ice melted, ushering in a new era of diverse animal life. 🌐

Key Takeaways

• Volcanic activity had a major role in both triggering and ending the Snowball Earth glaciations. 🌋
• Supercontinent breakup and a dimmer sun significantly contributed to global freezing. ❄️
• Despite harsh conditions, early life, including sponges, managed to survive through these ice ages. 🧽
• The runaway icehouse effect explains how the planet stayed frozen for so long without thawing. ❄️
• The end of these glaciations led to a burst of animal life in the warmer oceans of the Ediacaran period. 🌊

Overview

Chapters

• 00:00 - 00:30: Introduction to Snowball Earth The chapter titled 'Introduction to Snowball Earth' describes a time when our planet was completely covered in ice, with temperatures plummeting to extreme lows. At the poles, temperatures may have reached negative 130 degrees Celsius, and even at the equator, temperatures dropped below freezing. Both land and sea were blanketed with ice, creating a still and quiet world. Notably, this icy episode occurred not just once but twice during significant glaciation periods.
• 00:30 - 01:30: Global Freezes and Evidence The chapter titled 'Global Freezes and Evidence' discusses the period known as the Cryogenian, which occurred 716 million and 635 million years ago. This time is often referred to as Snowball Earth, characterized by the planet being covered in ice. The chapter seeks to answer how this global freeze happened and why the Earth eventually thawed. The intriguing answer to both questions involves volcanic activity.
• 01:30 - 02:30: Glaciation and Continental Shifts The chapter discusses the concept of 'snowball earth,' a period in Earth's history when glaciers covered vast parts of the planet. Evidence for this phenomenon is found on every continent, primarily through the discovery of dropstones. These rocks, picked up and transported by glaciers, ended up in the oceans as icebergs broke off and melted, leaving the stones in marine sediments. Scientists have been uncovering these clues since the early 1900s, highlighting the historical shifts in Earth's climate and continental arrangements.
• 02:30 - 04:00: Theories Behind Equatorial Ice In the chapter titled 'Theories Behind Equatorial Ice,' scientists discuss how the ancient positions of ocean sediments are reconstructed using magnetic particles preserved within the formations. These particles reveal the direction of the North Pole at the time, helping to identify the original locations where dropstones, transported by ice, settled. The findings indicate that ice sheets extended from the poles to the tropics during the Cryogenian period. Notably, extensive glaciations occurred twice between 716 and 635 million years ago, affecting regions as far as the equator.
• 05:00 - 06:00: Carbon Cycle and Rodinia The chapter titled "Carbon Cycle and Rodinia" begins by mentioning two significant glacial episodes that occurred millions of years ago: the first began 716 million years ago and lasted for about 36 million years, while the second occurred from about 650 to 635 million years ago. Unlike the current glaciers, the interesting aspect of these ancient glaciations was their extensive reach, contrasting with today’s warm tropical temperatures, approximately 31°C in the afternoon.
• 07:00 - 08:30: Eruptions and Sulfur's Role This chapter explores the concept of how Earth, a generally temperate planet, might have experienced freezing conditions significant enough to lead to the presence of ice at the equator. It begins with an examination of the initial scientific hypothesis that perhaps Earth's axis had tilted over time, turning equatorial regions into polar zones. This surprising geological evidence of ancient ice in tropical regions prompted imaginative theories to explain such anomalies.
• 09:00 - 10:00: Runaway Icehouse Effect The chapter explores the concept of a 'Runaway Icehouse Effect,' where evidence suggests that almost all of Earth, including the equator and the poles, froze over. Initially, it was considered that a change in Earth's tilt might have caused such an effect, but extensive evidence, including the presence of dropstones and carbonate rock, indicates otherwise. Carbonate rock, which forms when other rocks on continents weather and release ions into water, provided crucial evidence for this global freezing event.
• 10:30 - 11:30: Volcanoes and CO2 Build-up During the Cryogenian period, carbonate rocks disappeared from ocean sediments due to the planet being covered in ice, which halted land weathering. As the ice melted, weathering resumed, leading to significant carbonate deposits. This disappearance and reappearance of carbonate rocks indicate significant changes in the Earth's geological and atmospheric processes, particularly related to CO2 levels.
• 12:00 - 13:30: Post-Cryogenian Life The chapter titled 'Post-Cryogenian Life' discusses Earth's condition during the Cryogenian period when it was largely covered in ice, creating a paradox for biologists. Despite this icy environment, life forms such as photosynthetic cyanobacteria and even some early animal life like sponges had already evolved before the ice sheets formed. This raises questions about how these early life forms could have survived under such conditions, leading scientists to hypothesize the existence of open, unfrozen areas that allowed life to persist.
• 14:30 - 15:00: Call to Action and Conclusion The chapter discusses the Slushball Earth hypothesis, which proposes there was water at the equator necessary for life to persist. This model is contrasted with the geological evidence, suggesting an alternative where ice was everywhere but thin enough for light to penetrate, supporting photosynthetic life. Studies of cyanobacteria in Antarctica indicate life could thrive on ice sheets, indicating the abundance of ice, regardless of its thickness.

How Volcanoes Froze the Earth (Twice) Transcription

• 00:00 - 00:30 Imagine a world covered in ice. Estimates vary, but some scientists think at the poles, it could reach negative 130 degrees celsius. And there was no escaping the cold even at the equator, where temperatures would have dipped below 0 degrees. Sheets of ice coat both land and sea, and beneath them, the world is quiet and relatively still. It may sound like some far-off planet, but that’s what our own planet once looked like. And actually, it happened twice during a pair of episodes of intense glaciation between
• 00:30 - 01:00 716 million and 635 million years ago. These global freezes occurred within that period of geologic time known as the Cryogenian, or “Time of Ice.” But most people refer to this chapter in our history simply as Snowball Earth. So how did this happen? How did the world become covered in ice? And most importantly for us, why did the planet eventually thaw again? Strangely enough, for both questions, the answer lies in volcanoes.
• 01:00 - 01:30 The evidence for snowball earth is written on every continent today. Since the early 1900’s, scientists have been finding clues all over the world, in the form of dropstones. These are rocks and pebbles that were picked up by glaciers as they moved across the land. And once the glaciers met the seas, icebergs broke off and floated away, carrying the rocks with them. When the ice melted, the stones dropped into the ocean. These dropstones show up in ancient marine formations all over our planet.
• 01:30 - 02:00 And while the continents have shifted since the Cryogenian, scientists have been able to reconstruct the original positions of those ocean sediments using magnetic particles preserved in the formations themselves. These particles record the direction of the North Pole, which tells us where on the planet the dropstones originally fell into the sediment. And when you reconstruct where these dropstones were deposited, you can see that they stretched from the poles to the tropics. Which means ice did too. Now we know that this extensive glaciation actually happened twice between 716 and 635
• 02:00 - 02:30 million years ago. The first episode started 716 million years ago, and lasted for about 36 million years. And the second lasted from about 650 to about 635 million years ago. Now, there have been glaciers on our planet before – in fact, we have some now – but what makes these two periods so interesting is the extent of that ice. After all, today the tropics are pretty warm – a balmy 31* C in the afternoon, which
• 02:30 - 03:00 is awfully warm if you’re trying to freeze over an ocean. So how did our lovely temperate world get cold enough to freeze? Well, at first, scientists thought: If there’s evidence of ice having been at the equator, then maybe the equator wasn’t actually at the equator. Maybe earth had been tipped over on its side at some point – which would’ve made the equator part of the poles. That’s how weird it was to find evidence of ice in the tropics: Scientists thought
• 03:00 - 03:30 it was more likely that Earth fell over than that the equatorial oceans had frozen. But we now know that the evidence is too widespread for a change in Earth’s tilt to explain it. In fact, the evidence is so complete that it’s likely that almost all of earth froze over, including both the equator AND the poles. Because, in addition to dropstones, more evidence has been found, in the form of carbonate rock. This rock is created when other rocks on the continents weather and break down to form ions, which eventually make their way into the water.
• 03:30 - 04:00 When those ions attach to dissolved CO2, they join together to form carbonate. And studies of ocean sediments all over the world have found that, during parts of the Cryogenian, these carbonate rocks disappear. Because, when the world was covered in ice, almost no weathering took place on land, so carbonates became really rare. But when the ice started to melt, weathering resumed -- and huge deposits of carbonates began to form again. Most geologists think that the absence and reappearance of these rocks is a sign that
• 04:00 - 04:30 earth was mostly to completely covered in ice. But while that makes sense to the geologists, it doesn’t make sense to some biologists. Life had existed on Earth for over a billion years by the time the Cryogenian started. And organisms like photosynthetic cyanobacteria, and even animal life like sponges, had evolved before the ice sheets grew. Which raises the question of how early life could have survived under the ice. Some scientists have suggested that there must have been a fair amount of open, unfrozen
• 04:30 - 05:00 water at the equator for life to persist. This model is called Slushball Earth, but it doesn’t line up with all of the geological evidence. So yet another hypothesis is that there was ice everywhere, but that it was thin enough in places for light to shine through and to allow photosynthetic life to survive. Studies of modern cyanobacteria in Antarctica suggest that life may even have thrived on top of the ice sheets themselves. But whether it was thick ice, or thin ice, the ice was abundant.
• 05:00 - 05:30 So, then, why did these massive glaciations actually happen in the first place? Well, the most popular theory is that our planet’s thermostat just … failed. That thermostat is the Carbon Cycle – the swapping back and forth of carbon between the atmosphere and the earth’s crust. And it starts with volcanoes, which, over the course of thousands to millions of years, gradually emit CO2 into the atmosphere, where it helps keep the world warm. But CO2 levels are kept in check, because that gas gets stored in carbonate rocks during
• 05:30 - 06:00 the process of weathering. So volcanic emissions and rock-weathering are the two counterbalances that keep earth not too hot, and not too cold. But in the Cryogenian, an early supercontinent known as Rodinia messed with the thermostat by breaking up. Breaking up is hard to do and rocks usually do it pretty violently. But the breakup of Rodinia was especially intense, because it pumped out a lot of a volcanic rock known as basalt. And basalt is really, really good at soaking up CO2 in the process of weathering.
• 06:00 - 06:30 Plus, Rodinia was sitting at the equator at the time, where it was warmer and wetter, which weathered the rock even faster. So scientists think that this could have thrown off the carbon cycle, soaking up CO2 faster than volcanoes could release it. And there was another contributing factor: the sun. During the Cryogenian, the sun was actually about 7% dimmer than it is today. That doesn’t sound like a lot, but it was enough that, once the levels of CO2 dropped, it was so cold that the glaciers started to grow.
• 06:30 - 07:00 And in the last few years, scientists have discovered yet another driving force behind this phenomenon: a truly massive and spectacular eruption that took place 18 million years before the glaciation even started. Today, the remains of that eruption are known the Franklin Large Igneous Province: more than a thousand square kilometers of basalt lava that cover the Canadian Arctic. But what sets these rocks apart from others is that they were full of another planet-cooling
• 07:00 - 07:30 gas: sulfur. When you pump sulfur into the air, it cools the earth – but normally, it doesn’t do it for long. Sulfur dioxide interacts with water in the atmosphere and forms acid rain, typically leaving the atmosphere within a couple of years. But these eruptions weren’t made by your standard volcanoes. Instead they sprayed out huge jets of lava called fire fountains, which could have erupted for years, spraying plumes of sulfur gases up to 12 kilometers into the atmosphere.
• 07:30 - 08:00 And that high above Earth’s surface, near the stratosphere, sulfur dioxide would take a lot longer to break down and rain out. So, low CO2 levels let things cool down, and a dimmer sun didn’t help. Then suddenly, 716 million years ago, vast amounts of sulfur dioxide may have been a final blow to earth’s thermostat - and ice began to form. The second glaciation may have had similar causes, but it isn’t as well dated or understood as the first. But for both episodes, the real problem came when the ice started to grow.
• 08:00 - 08:30 Ice reflects more light than water does, which makes the world cooler, which makes more ice grow, which makes the world even cooler – and so on. This feedback loop is called a runaway icehouse effect. And scientists who have modeled this process found that, once our planet had ice below about 30 degrees latitude – the latitude of Modern-Day New Orleans -  the growing ice was basically unstoppable. So why are we not still stuck on a world that’s basically ... Hoth?
• 08:30 - 09:00 Because of our old friend carbon dioxide. Rodinia didn’t stop splitting apart just because it was covered with ice. As it kept breaking up, volcanoes kept forming and releasing CO2 into the atmosphere. But this time, because the planet’s rocks were mostly locked beneath ice sheets, they weren’t able to absorb all of that greenhouse gas. So instead, it began to build up in the air. It took almost 50 million years for enough CO2 to melt the first round of glaciers, and about 10 to 15 million years to melt the second.
• 09:00 - 09:30 Between the two glaciations, Rodinia continued to break up near the equator - which is why the thermostat broke twice during the Cryogenian. But by the end of the Cryogenian, Rodinia was largely in the southern hemisphere, and had stopped splitting so dramatically, so the thermostat could re-set itself. Once most of the ice had melted by about 635 million years ago, the warmer oceans suddenly began to fill with animal life. The period that immediately followed the Cryogenian -- known as the Ediacaran period -- is full
• 09:30 - 10:00 of some strange and varied forms, descendants of the survivors of snowball earth. But animal life itself didn’t actually first evolve in the Ediacaran. Molecular clock analyses suggest the most recent common ancestor of all animal life lived long before that -- some 800 million years ago. Which means that somehow, animal life actually lived through Snowball earth. How? Well, the earliest animals were practically unkillable – and it turns out, they not
• 10:00 - 10:30 only survived snowball earth, they helped change oceans for the better. But that’s a story for another time. So come back soon to learn all about the enterprising, trail blazing, and nearly indestructible animals that clung to life throughout the snowballs: the sponges. Thanks to this month’s Eontologists: Patrick Seifert, Jake Hart, Jon Davison Ng, and Steve. If you’d like to join them and our other patrons in supporting what we do here, then
• 10:30 - 11:00 go to patreon.com/eons and make your pledge! And if you want to join us for more adventures in deep time, just go to youtube.com/eons and subscribe. Thanks for joining me today in the Konstantin Haase studio, and if you’d like to learn more about the very deep past, then watch “The Search For the Earliest Life.”