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When scientists reconstruct ancient climates from ice cores, how do they create an accurate timeline?

Researchers use chemical analyses, computer models, and other tools to date these valuable climate archives.

 

October 9, 2025

Beneath the snowy surfaces of our planet’s ice sheets and glaciers lies a trove of information about past climates. As snow falls year after year, it gets buried and compressed into a frigid chronicle of Earth history: Ice, and the impurities and air bubbles trapped inside it, preserve evidence of ancient temperatures, greenhouse gases, and even volcanic eruptions. To get at this record, scientists drill down and remove cylindrical “cores” of ice that can span hundreds of thousands of years.1

That means ice core researchers have (so to speak) a lot of time on their hands. And building a reliable timeline for a core, linking what happened in Earth’s past to when it happened, is important—not just to make sense of the ice core itself, but to compare it with other ancient “archives,” like seafloor sediments or stalagmites.

“If you see something interesting 100,000 years ago in one archive, you have to be able to compare it confidently to another archive and know that you’re comparing the same time period,” says David McGee, professor of Earth and planetary sciences at MIT. And by placing key events in order, scientists can investigate causes and effects in the saga of Earth’s climate history—piecing together “not just how climate changed, but why it changed.”

So how do researchers date an ice core?

The most straightforward method is to count backward, one year at a time. For example, seasonal differences in snow and in impurities like dust can show up as alternating lighter and darker bands in a core2—helping divide the icy logbook into yearly chapters. Some aspects of snow that aren’t visible to the naked eye, like the molecular properties of water, also vary with the season.3 By counting off seasonal cycles, visible or invisible, scientists can in some cases pick out annual layers going back tens of thousands of years.4

That reveals the age of the ice itself. But the ice also contains another source of information: air bubbles, which bottle up ancient gases and show how the contents of Earth’s atmosphere have changed over time.

This direct access to ancient air is “really unusual” and deeply valuable, McGee says. But in a tricky twist, the air bubbles are younger than the ice around them, sometimes by thousands of years. As fallen snow is gradually compressed into ice by the weight of fresh layers, the air buried with it can still mix with the atmosphere until there’s been enough compaction to trap it in closed-off bubbles.

Dating these air bubbles, then, calls for additional tools, such as computer models of how snow becomes ice. Researchers also look at the nitrogen gas in the bubbles. Nitrogen comes in different “isotopes,” some of which are heavier and settle downward more readily. This means the mix of isotopes helps reveal the depth at which air was finally cut off from the atmosphere.5

More challenges arise deeper inside an ice core. Ice doesn’t simply pile up neatly “like layers of a cake,” McGee says. “It’s also flowing actively.” Think of pancake batter spreading on a griddle, he says. “As you go further and further down in an ice core, you’re sampling layers that have experienced more flow outward, and that’s caused them to thin.” In other words, “each centimeter is more and more time that’s been compressed.”

Eventually, that makes annual layers imperceptible. “As layers thin and thin, you lose the ability to continue to layer-count,” says McGee. “So then you have to use other methods to estimate the relationship between depth and age.”

Here again, computer models come in handy, simulating how ice flows and layers thin with depth. Researchers also hunt through an ice core for volcanic ashes, which McGee says can “anchor” the core in time. By examining their chemical makeup, scientists can link those ashes to an eruption whose age is known—for instance, based on the gradual decay of radioactive material, which provides a kind of ticking clock for the remnants near the volcano.6 (Radioactive decay can also help date the core directly; McGee says this is an important tool today as scientists hunt for super-old ice that’s been pushed up toward the surface.7

Still other methods rely on the “calendar” of Earth’s orbit, which shifts slightly over time. These shifts change how much sunlight reaches the poles, in predictable cycles that have been modeled deep into the past. Helpfully, these cycles go hand-in-hand with changes in the precise ratio of gases that get trapped in air bubbles. That means scientists can measure the changes in a core’s trapped air and match them up with the cycles of sunlight—effectively, situating data from the core within Earth’s orbital timeline.8

So researchers have assembled a toolkit of creative ways to date ice and trapped air. And McGee emphasizes that scientists aim never to rely on just one. By using several different tools—simulations of ice flow, annual layer counts, markers of volcanic eruptions—and gauging how well they agree, scientists can spot errors and build the most robust timeline possible.9

Ultimately, “age uncertainties do increase as we go back in time,” McGee says, and the record does lose some of its detail in deeper sections. Say, for example, that you want to know how high carbon dioxide (CO2) levels were in the past (crucial data as we try to understand today’s climate change, which is driven by the vast amounts of CO2 humanity is adding to the atmosphere). Near the top of the core, clear layers might let you track CO2 backward year-by-year. But lower down, McGee says, you may have to settle for average levels over a decade, or a century, or even a millennium.

Despite the challenges, ice cores are incredibly rich sources of information about our planet’s past. And they’ve proven their reliability, McGee says, as researchers compare them to one another and to other records of Earth’s ancient climates. “We feel really confident in the information that comes from them.”

 

Thank you to Robert Miller of Masterton, New Zealand, for the question.

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Footnotes

1 Bouchet, Marie, et al. "The Antarctic Ice Core Chronology 2023 (AICC2023) chronological framework and associated timescale for the European Project for Ice Coring in Antarctica (EPICA) Dome C ice core." Climate of the Past 19 (2023). https://doi.org/10.5194/cp-19-2257-2023.

2 Thompson, Lonnie G., and Ellen Mosley-Thompson. "Icy secrets preserved in Earth's glaciers." In St. John, Kristen, and Krissek, Lawrence (Eds.), Climate Change: A Geoscience Perspective (pp. 139-182). 2025. Springer. https://doi.org/10.1007/978-3-031-82869-0_4.

3 Kuramoto, Takayuki, et al. "Seasonal variations of snow chemistry at NEEM, Greenland." Annals of Glaciology 52 (2011). https://doi.org/10.3189/172756411797252365.

4 Sigl, Michael, et al. "The WAIS Divide deep ice core WD2014 chronology—Part 2: Annual-layer counting (0-31 ka BP)." Climate of the Past 12 (2016). https://doi.org/10.5194/cp-12-769-2016; Svensson, Anders, et al. "A 60000 year Greenland stratigraphic ice core chronology." Climate of the Past 4 (2008). https://doi.org/10.5194/cp-4-47-2008.

5 Bréant, Camille, et al. "Modelling firn thickness evolution during the last deglaciation: constraints on sensitivity to temperature and impurities." Climate of the Past 13 (2017). https://doi.org/10.5194/cp-13-833-2017.

6 Narcisi, Biancamaria, et al. "A volcanic marker (92ka) for dating deep east Antarctic ice cores." Quaternary Science Reviews 25 (2006). https://doi.org/10.1016/j.quascirev.2006.07.009; Dunbar, Nelia W., and Kurbatov, Andrei V. "Tephrochronology of the Siple Dome ice core, West Antarctica: correlations and sources." Quaternary Science Reviews 30 (2011). https://doi.org/10.1016/j.quascirev.2011.03.015.

7 Yan, Yuzhen, et al. "Two-million-year-old snapshots of atmospheric gases from Antarctic ice." Nature 574 (2019). https://doi.org/10.1038/s41586-019-1692-3.

8 Oyabu, Ikumi, et al. "The Dome Fuji ice core DF2021 chronology (0-207 kyr BP)." Quaternary Science Reviews 294 (2022). https://doi.org/10.1016/j.quascirev.2022.107754.

9 Bouchet et al (2023) (see ref. 1); Parrenin, Frédéric, et al. "IceChrono1: a probabilistic model to compute a common and optimal chronology for several ice cores." Geoscientific Model Development 8 (2015). https://doi.org/10.5194/gmd-8-1473-2015.

Want to learn more?

Listen to this episode of MIT's "Today I Learned: Climate" podcast on Earth's climate history.

Transcriptions

LHF: Hello, I’m Laur Hesse Fisher, and you’re listening to Today I Learned: Climate from the Massachusetts Institute of Technology.

Imagine, for a moment, that you’re standing on a massive sheet of ice that spans from the high Arctic, all the way into the northern United States. At its thickest point you could drill down through almost two miles of solid ice before reaching land. 

Today on our episode, we are going back in time to visit past versions of our Earth that are wildly different from today’s. 

And why? Well, because the Earth’s climate has changed before—many times before!—and folks like you have written in and asked us about it. What caused the Earth’s climate to change in the past? And what can it tell us about the climate change that we’re experiencing today?

Fortunately, we know someone at MIT who knows a lot about the history of the Earth’s climate.

DM: My name's David McGee, and I'm a professor in the Department of Earth, Atmospheric and Planetary Sciences at MIT. And I study paleoclimate, which is the study of the natural history of Earth's climate.

LHF: It turns out that our planet has changed a lot before we humans came onto the scene. There was a time, for instance, when the whole center of North America was engulfed by an inland sea, a time when alligators crawled in the Arctic, and forests flourished near the south pole. 

And that’s because the Earth has gone through some wild changes in temperature.

DM: Even in the last 1% of Earth history, so last like 45 million years, we've seen changes in the Earth's mean temperature of roughly 30 to 40 degrees Fahrenheit. So huge changes in the mean global temperature.

LHF: But how do we know about these big changes in temperature? Well that, really, is the story of paleoclimate, and it begins in earnest in the 1700s, with some peculiar rocks.

DM: People had noticed boulders that didn't match the local bedrock, in places where it didn't really make sense that there should be boulders, in Scotland, Ireland, around eastern North America. They noticed striations or grooves in the bedrock. And they realized that these striations were things that were observed near modern glaciers. And so people started to piece together this story that there had been very large ice sheets in places where there weren't currently ice sheets.

LHF: In 1824, a geologist named Jens Esmark first proposed that these ice sheets were not just local, but a single vast mass of ice that once covered much of the Northern Hemisphere: in other words, that the world had undergone an ice age.

Over the next century, scientists would find more and more evidence proving his theory, eventually learning that, 20,000 years ago, a quarter of the Earth’s land surface was covered in ice, year round. And that raised a new question: just how cold was the Earth during this ice age? To answer that, scientists needed some extraordinary new tools.

DM: Paleoclimate is the art of the possible. You know, there's only so many things that you have that are left over from thousands of years ago, there's even fewer that are left over from millions of years ago, and even fewer from hundreds of millions of years ago.

So we have to rely upon natural archives, things that grow or are deposited and somehow record information about the climate around them as they form.

LHF: And these archives need to be preserved for a very long time. Scientists have only found a few of these relics of the deep past: often buried in unchanging environments, like Antarctic ice or sediments in the deep sea.

DM: And in both of these archives, you have deposits building up year after year after year. And if you're able to drill or core down into them, you essentially have a time machine.

I'll just give you an example. There is a certain type of plankton that lives in the surface ocean. These are called foraminifera, and they're about the size of a grain of sand. Really small. They happen to form small calcium carbonate shells. So just like a clam might, but they're so small that they're able to float around in the surface ocean.

LHF: And when the foraminifera die, their shells fall to the ocean floor and are preserved in layers of sediment. So what does that have to do with the temperature? Well, it turns out that foraminifera that grow in warmer waters build their shells a little differently.

DM: As the temperature gets hotter, the forams become more sloppy chemists and they allow more magnesium into their calcium carbonate shell. And so you can measure the magnesium to calcium ratio, and that's a very strong function of temperature.

LHF: And there are other time-traveling thermometers found in tree rings, ice cores, and stalagmites deep in caves. When you combine these separate lines of evidence, we can build a window into climates from long ago.

What’s more, when scientists tracked these temperature records further and further back in time, a surprising new picture appeared.

DM: They were able to see, oh wow, there hasn't just been one ice age. There's been this cycle going back and forth between ice ages and warmer periods.

So the earth has been going in and out of ice ages over the last million years at a rate of roughly one cycle per 100,000 years. So you'll have a period like the peak of the last ice age about 20,000 years ago. And then temperatures will rise into warm climates like we've enjoyed for the last 10 thousand years.

LHF: How? And why? Well, the answer, amazingly, lies not here on Earth, but out in the solar system.

So you might know that the Earth orbits the sun in an ellipsis—not a perfect circle. And the Earth is also tilted. At any time, one pole faces the sun—that’s the half of the Earth that experiences summer—and the other half faces away—that’s the Earth that experiences winter. But over thousands of years, that orbit and tilt… well, it shifts.

DM: The Earth's orbit gradually changes as we get pulled by the other planets in the solar system. And so the Earth's orbit becomes more elliptical or more circular through time. The Earth's tilt changes a little bit through time in a cyclical manner. 

LHF: And gradually, our north and south poles might find that, during the summer, they’re no longer tilted so strongly toward the sun.

DM: That decreases how much sunlight comes into the Arctic during local summer and makes it harder to melt away the previous winter’s snow and ice, and it builds up and builds up and builds up, and eventually forms an ice sheet.

So, then the question is, okay, you're building up some ice sheets in Northern Canada and Scandinavia. Why does that make the whole world cold? The real reason that ice ages are a global phenomenon is because, as you grow an ice sheet, the ice sheet changes ocean circulation in such a way that more carbon dioxide gets stored in the deep ocean rather than sticking around in the atmosphere.

LHF: You probably remember that CO2 is the most important of the heat-trapping gases in our atmosphere that are causing today’s climate change. And throughout Earth’s history there’s been a close relationship between the average temperature of our planet and the amount of CO2 in our atmosphere. Now, scientists use the tools of paleoclimate to look at how much CO2 was in the air during the ice ages. In fact, we can actually measure directly the air of the ancient past—because some of it is still around.

DM: In Antarctica in particular, as the snow builds up and then gets compressed beneath other layers of snow above it and gradually turns into ice, it traps little bubbles of air. And that air is pristine samples of the ancient atmosphere. And so scientists will collect these ice cores, bring them back to the lab, and then measure directly how much carbon dioxide is in the air from times in the past.

LHF: That’s really cool. All right, so let’s recap. So the Earth shifts slightly in space over thousands of years, making the Arctic summer darker and colder. And ice sheets form and spread, and the ocean circulation changes. This traps CO2 deep in the ocean, and because there is less heat-trapping CO2 in the atmosphere, the entire planet begins to cool.

DM: And so it's quite a chain of events that leads from the changes in Earth's orbit to the ice ages themselves.

LHF: So how much do these changes add up? Well, in the last ice age, which was 20,000 years ago, CO2 in the atmosphere fell by about a third. So do you want to guess how much the Earth cooled as a result?

DM: We now know that in the peak of the last Ice Age, it was about 10 degrees Fahrenheit colder than it was during pre-industrial times.

LHF: Did you guess correctly? Or were you way off? Maybe you’re asking yourself now—wait, what? Just ten degrees? Isn’t that the difference between a chilly fall day and a crisp spring afternoon?

DM: Yeah, it's really striking to me how different the world was, given only 10 degrees Fahrenheit difference in mean temperatures. So, where I'm sitting around Boston, Massachusetts, would have had about a mile of ice on top of me right now. 

LHF: From just 10 degrees of cooling! (Which is about five and a half degrees Celsius, by the way.) But this is the crucial difference between weather and climate. If the weather changes by 10 degrees, well, you put on a jacket. But if the average climate changes by 10 degrees… well, you’ve got the planet where woolly mammoths roamed as far south as Illinois and Spain. 

DM: And then slow changes in Earth's orbit gradually increase how much summer sunlight there is in the Arctic and start to melt back those ice sheets and the changes go in reverse. So the ocean circulation responds and allows carbon dioxide that has been stored in the deep ocean to come back into the atmosphere.

LHF: And those rising CO2 levels warm the entire world. Like they are today.

Except, not quite like today. We really are living through something that’s different now. So for one thing, today’s climate change is timed all wrong. The Earth’s position in space is not setting us up for more warming.

DM: The variations in Earth's orbit are fairly subtle right now, and then they'll get larger over the next few tens of thousands of years. So if there weren't human-caused climate change, we would eventually go back into another ice age.

LHF: And a huge difference between the end of the last ice age, and today’s warming—is how fast it’s happening.

DM: So if you look at the warming coming out of the last ice age, temperatures were low until about 17,000 years ago, and then CO2 started to rise and global temperatures started to rise. And they rose that 10 degrees Fahrenheit in about 7,000 years. Modern temperature change is about 10 times faster.

LHF: Which means that today, we’re facing climate change at a speed that even our distant, nomadic ancestors in the ice age never confronted. Let alone the more recent humans who laid the foundations of civilization as we know it.

DM: The last 10,000 years have been a period of stability in global temperatures. And that period of stability has coincided with the growth of complex human societies and the shift to agriculture as the basis for human society and you know, dramatic expansions in human population. And this I think is more than a coincidence.

LHF: It’s true that the Earth has gone through immense climate change before, many times over, in fact. But human civilization… has not. And especially not this fast.

Today, we are the ones changing the balance of our atmosphere. And we’re the ones who get to decide. Do we want to rapidly shake our planet loose from the stability that we’ve always known? Or will we be happier, and safer, if we act to preserve the climate in which humanity has flourished for the last ten thousand years?

That is our show today. Thank you to everyone who sent us in questions about the ice ages. You can send us your own question by leaving us a voicemail message at 617 253 3566 or visiting https://climate.mit.edu/ask.

Today I Learned: Climate is the climate change podcast of the Massachusetts Institute of Technology. Aaron Krol is our Writer and Executive Producer. David Lishansky is our Sound Editor and Producer. Michelle Harris is our fact-checker. The music is by Blue Dot Sessions. And I’m your Host and Senior Editor, Laur Hesse Fisher. 

Thank you Prof. David McGee for speaking with us, and to all of you, for listening. Keep up your climate curiosity.