Nearly 1,800 miles beneath the surface, two continent-sized structures of superheated rock have long shaped Earth's volcanic history, diamond deposits, and perhaps the fate of species — yet only now are scientists beginning to understand that these formations are not fixed monuments but restless, shifting presences. New computational models reveal that these mantle blobs migrate, merge, and reorganize over geological time in patterns that mirror the movement of continents above them, with the African blob having assumed its current form as recently as 60 million years ago. This discovery invit
Earth's Giant Mantle Blobs Shift Shape Like Continents, New Models Show
The blobs shift and reshape like continents assembling into supercontinents
So these blobs are real structures we can detect, not just theoretical constructs?
Exactly. Seismic waves from earthquakes pass through them differently than through surrounding mantle rock. They slow down, which tells us the blobs are hotter and denser. It's like seeing a shadow on an X-ray.
But we're inferring their composition and behavior from seismic data alone, right? We can't actually sample them directly.
That's right. The models are based on what we know about plate tectonics and how rock flows under extreme pressure and heat. They're constrained by surface observations—where volcanoes erupt, where diamonds come up.
And the new finding is that these blobs move around, not stay locked in place?
Yes. The computer simulations show them assembling and breaking apart over a billion years, much like continents do at the surface. The African blob came together only 60 million years ago.
How confident are we in that 60-million-year figure? Is that a precise date or a range?
It's a model result, so there's uncertainty built in. But it's dramatically different from earlier estimates that suggested the blob could be hundreds of millions of years old in its current form.
Why does it matter if the blob is 60 million years old versus 600 million years old?
It tells us how dynamic Earth's interior is. If the blob is younger than we thought, it means major structures reorganize faster than we assumed.
And the practical angle—finding nickel and diamonds—that depends on these models being accurate about where the blobs are now and where they've been?
Exactly. If we understand the blob's history and current location, we can predict where mantle plumes are likely to bring valuable minerals to the surface.
So this is geology that could actually change where mining companies look?
Potentially, yes. It gives them a better framework for targeting exploration.
The Pulse
- Two massive rock structures deep in Earth's mantle — long assumed to be stationary — have been shown to drift, reshape, and even merge across billions of years, upending a foundational assumption in geoscience.
- These blobs are not passive: they drive volcanic supereruptions, may have contributed to the extinction of the dinosaurs, and act as the delivery mechanism for diamonds rising from extraordinary depths.
- Advanced simulations run on Australia's national supercomputing infrastructure reconstructed a billion years of mantle flow, revealing that sinking ocean floor physically shoves the blobs aside as tectonic plates collide above.
- The African blob's surprisingly recent assembly — just 60 million years ago, not hundreds of millions as previously believed — signals that Earth's deep interior reorganizes on timescales far shorter than scientists had assumed.
- Despite overturning old models, the new simulations still account for the volcanic and kimberlite eruption record observed at the surface, lending the findings credibility without discarding prior evidence.
- The practical stakes are rising: mapping blob movement could direct geologists toward untapped deposits of diamonds and nickel — a mineral critical to batteries and the renewable energy transition.
Nearly 1,800 miles beneath the surface, two continent-sized structures of superheated rock have long shaped Earth's volcanic history, diamond deposits, and perhaps the fate of species — yet only now are scientists beginning to understand that these formations are not fixed monuments but restless, shifting presences. New computational models reveal that these mantle blobs migrate, merge, and reorganize over geological time in patterns that mirror the movement of continents above them, with the African blob having assumed its current form as recently as 60 million years ago. This discovery invites us to reconsider the deep interior of Earth not as a stable foundation beneath the drama of surface life, but as an active participant in it — one whose movements may yet guide us toward the mineral resources a changing civilization will require.
Two continent-sized accumulations of superheated rock sit nearly 1,800 miles beneath Earth's surface — one under Africa, one under the Pacific. Geologists call them blobs, and they have known about them for decades because they slow seismic waves from earthquakes in ways that betray their unusual heat. What remained unclear was whether these formations were fixed in place or something more restless.
They are far from inert. The blobs are thought to be the source of deep mantle plumes — towering columns of rock that rise toward the surface and fuel some of Earth's most violent volcanic events. The eruptions linked to these plumes contributed to the mass extinction that ended the age of dinosaurs. The blobs also appear to govern the movement of kimberlite, the rock type that carries diamonds from depths of 120 kilometers or more up to where humans can find them.
For years, the dominant view held that the blobs were essentially anchored in place while tectonic plates rearranged themselves above. New simulations, run on Australia's National Computational Infrastructure and modeling a billion years of mantle flow, challenge that picture entirely. When ocean floor is pushed downward during plate collisions, the cold dense rock eventually reaches depths where it physically displaces the hot blobs. Over time, this causes the blobs to migrate, merge into a single 'superblob,' and drift apart again — a cycle that mirrors the assembly and breakup of supercontinents at the surface.
The most striking finding: the African blob took on its current shape only about 60 million years ago, far more recently than earlier models implied. This compresses the timescale on which Earth's deep interior reorganizes itself, suggesting a more dynamic planet than previously understood. Crucially, the new models still reproduce the pattern of volcanic and kimberlite activity recorded in surface rocks — meaning the revised picture reframes the evidence rather than contradicting it.
The origin of the blobs remains an open question. They may be primordial material preserved from Earth's earliest history, or they may have built up gradually from dense oceanic rock carried down by subducting slabs. Either way, the research carries practical weight: by tracing blob movement, geologists can better target searches for diamonds and magmatic sulfide deposits rich in nickel — a metal essential to lithium-ion batteries and the infrastructure of renewable energy. The deep Earth, it turns out, is not merely a record of the planet's past but a map to resources its future will depend on.
Two continent-sized structures lurk nearly 1,800 miles beneath your feet, one anchored under Africa, the other under the Pacific Ocean. Geologists call them blobs—massive accumulations of rock in Earth's mantle, the thick layer of slowly flowing stone between the crust and the core. We know they exist because they slow down seismic waves from earthquakes, a telltale sign that they are hotter than the rock surrounding them. For decades, scientists have watched these formations with a mixture of fascination and uncertainty, knowing they were there but puzzled about how they had moved and changed across billions of years.
These blobs are not inert. They are thought to be the source regions for deep mantle plumes—towering columns of superheated rock that rise toward Earth's surface and trigger some of the planet's most violent volcanic eruptions. When these plumes breach the crust, the results can be catastrophic. The extinction event that killed the dinosaurs 65.5 million years ago was partly driven by volcanic activity linked to mantle plumes. The blobs also appear to control the movement of kimberlite, a type of rock that carries diamonds from depths of 120 to 150 kilometers, and sometimes from as far down as 800 kilometers, up to where humans can find them.
For a long time, the prevailing theory held that these blobs were essentially fixed in place—anchors locked into the mantle for hundreds of millions of years while tectonic plates shuffled around above them. But new research challenges that picture entirely. Using Australia's National Computational Infrastructure, a team of geologists ran advanced simulations modeling a billion years of mantle flow. What they found was striking: the blobs do not stay put. Instead, they shift position and reshape themselves in patterns strikingly similar to how continents assemble into supercontinents and then break apart.
The models work by reconstructing how tectonic plates have moved across Earth's surface over deep time. When plates collide, ocean floor gets pushed downward in a process called subduction. That cold, dense rock sinks deeper into the mantle, and once it reaches about 2,000 kilometers down, it physically shoves the hot blobs aside. Over geological time, this process causes the blobs to migrate, merge, and separate. The African blob and the Pacific blob can come together to form what the researchers call a "superblob," then drift apart again as plate movements shift.
One finding proved particularly surprising: the African blob assembled into its current configuration only about 60 million years ago—far more recently than earlier models suggested. Previous work had implied the blob might have held roughly its present shape for nearly ten times as long. This revision matters because it means the deep interior of Earth is more dynamic than scientists had assumed, with major structures reorganizing on timescales that, while still vast, are measurably shorter than once believed.
Yet the models do something else important: they still account for the pattern of volcanic eruptions and kimberlite activity observed at Earth's surface across the geological record. This consistency is crucial. It means the new picture of mobile, shape-shifting blobs does not contradict the evidence geologists have gathered from rocks and eruption sites. Instead, it reframes what that evidence tells us about how Earth's interior works.
The origin of the blobs themselves remains unsolved. They may be denser than surrounding mantle rock because they consist of primordial material separated out early in Earth's history—a possibility that could help explain why Earth's overall mineral composition differs from what meteorite studies would predict. Alternatively, they may have accumulated over time as dense oceanic material from subducting slabs piled up in the mantle. The models suggest that continental fragments are more likely to be transported to the African blob than the Pacific blob, a finding that aligns with recent work showing that mantle plumes rising from beneath Africa carry continental material, while those from beneath the Pacific do not.
Beyond the fundamental science, the research has practical implications. By mapping how the blobs have moved and where they are likely to be, geologists can better target the search for minerals associated with mantle upwelling. Diamonds brought to the surface by kimberlite are one example. Magmatic sulfide deposits, which contain most of the world's nickel reserves, are another. Nickel is essential for lithium-ion batteries and other renewable energy technologies. As the world transitions away from fossil fuels, understanding where these critical minerals are likely to be found becomes increasingly valuable. The blobs, it turns out, are not just monuments to Earth's deep history—they are signposts to resources the future economy will need.
Notable Quotes
The blobs can assemble—forming 'superblobs' as in the current configuration—and break up over time, much like continents and supercontinents at Earth's surface— Research team (Bodur, Flament, Merdith, Williams)