A billion years ago, in what is now the heart of Australia, there was a supervolcano so immense that it dwarfs anything alive today. Known as the Talbot Sub-basin, this prehistoric volcano unleashed eruptions with volumes exceeding 1,800 cubic kilometres of molten rock in a single blast — enough to bury an entire modern city beneath kilometres of ash and volcanic glass. It erupted repeatedly for over thirty million years, each time creating new overlapping calderas in a cycle of destruction and renewal. When it was alive, it spanned nearly fifty kilometres across, blasting material deep into the sky with an intensity that would have rivalled or surpassed Yellowstone, Taupo, or Toba. Unlike Yellowstone, its VEI 7 to 8 eruptions were fed not by a mantle plume but by the slow cooking of a continent’s crust — a “supervolcano without a hotspot,” operating in the thinning heart of a continent that was still coming together.
This was no ordinary eruption centre. The Talbot volcano was part of a vast bimodal volcanic system — basalt from the mantle below and silica-rich rhyolite from the melting of the crust above. Its rhyolites are chemically unique, depleted in heavy oxygen isotopes, marking them as products of intense interaction between magma and surface water at astonishingly shallow depths. Over time, these eruptions built a volcanic pile up to nine kilometres thick and left behind what is now the largest known accumulation of low- delta eighteen O rhyolite on Earth. What remains is the eroded skeleton of a super-eruption province, an ancient furnace that forged new crust and helped shape the very foundations of Australia.
Today, if you stand on the dusty plains near the borders of Western Australia, South Australia, and the Northern Territory, there’s little to give away the violence that once raged here. The desert is quiet, its mesas low and sun-baked, and the wind drags across quartz pebbles and dry salt pans. But hidden beneath your feet lies the scar of that colossal engine — the long-frozen remains of magma chambers and caldera walls that, a billion years ago, would have plunged the world into volcanic winter.

*Image depicts the location of the Talbot Sub-Basin
Back in the Mesoproterozoic Era, around 1.08 billion years ago, Australia as we know it did not exist. The land was a patchwork of drifting continental blocks slowly colliding and welding together into the supercontinent Rodinia. Between these growing masses lay zones of weakness, regions of thinned crust where heat from the mantle could seep upward. One such region was the Musgrave Province, trapped between the North Australian and South Australian cratons — two of the most ancient fragments of Earth’s crust.

*Image depicts Australia 900ma during the time the super continent Rodinia was active.
For hundreds of millions of years before the Talbot eruptions, the Musgrave Province had been under extreme thermal stress. Earlier tectonic collisions, especially the Musgrave Orogeny around 1.2 billion years ago, had crumpled, stretched, and baked the crust, charging it with enormous amounts of residual heat. The rocks were already simmering at near-melting temperatures when fresh magma began to intrude from below during what geologists call the Giles Event. That combination — a thin, fractured crust and a deep source of magma — was the perfect recipe for catastrophe.

*Image depicts the Musgrave Province (Red)
When basaltic magma surged upward from the mantle, it stalled in the crust and began melting the rocks around it, generating huge chambers of A-type rhyolite, a dry, iron-rich, silica-heavy magma known for its explosive temperament. Over thousands of years, these chambers ballooned in size, storing more and more pressure until the crust above finally fractured and collapsed. The result was not a cone like Mount Fuji or Mount St Helens but a caldera tens of kilometres across — a volcanic depression formed when the ground itself caved in after being emptied of magma.
Normally, when identifying supervolcanoes, the caldera can be clearly outlined using magnetic or gravity data — but that isn’t the case with the Talbot system. The subsurface maps are cluttered with overlapping magnetic signals from later intrusions, mafic sheets, and structural reworking, making it difficult to distinguish any single caldera rim. To complicate matters further, Talbot wasn’t just one volcano but a cluster of overlapping “piggyback” calderas formed over tens of millions of years. Each new eruption reshaped the previous collapse structure, blurring its boundaries. After the eruptions ended, the entire region experienced significant post-caldera deformation and erosion, further distorting or burying the original ring faults. As a result, the caldera outline has become obscured beneath a patchwork of later geological processes, leaving only faint traces of what was once a vast supervolcanic complex.
But with that being said, if I was to take an educated guess regarding where the eruptive centre was, based on faults, geological layers and magnetic anomalies, I’d say it was here. And this fits quite neatly with a map posted in the study The Mesoproterozoic thermal evolution of the Musgrave Province in central Australia — Plume vs. the geological record. In this image we can see that the Mundrabilla shear zone cuts right through the caldera location. When viewing the caldera under magnetics and gravity, there appears to be a linear feature cutting into the circular shape. This linear feature is almost certainly the Mundrabilla Shear Zone. On geological maps, there are some ring-like faults that also add weight to the assumption that this was more or less the explosive centre of the numerous super eruptions that make up the Talbot Sub-basin.

*Image depicts the volcanic layers that outcrop today at surface level in the Talbot Sub-Basin.

*Image depicts the Talbot Sub-Basin under greyscale magnetics along with the possible caldera shape.
The first of these cataclysmic eruptions produced a rhyolite deposit estimated at nearly 1,800 km³ — comparable to, and greater than, the largest eruptions known on Earth. Imagine the ground splitting open and a column of incandescent ash shooting 40 kilometres into the stratosphere. The column collapses under its own weight, sending pyroclastic flows — clouds of gas and molten glass — racing across the land faster than any storm. For hundreds of kilometres, the landscape is buried beneath searing ash flows hundreds of metres thick. Rivers vanish, mountains are levelled, and the sky turns dark for months.
When the eruption finally ceases, the crust above the emptied magma chamber collapses inward, forming a depression forty to fifty kilometres wide. Then, over time, a new magma chamber forms beneath it, and the process repeats. Each new eruption occurs within the footprint of the last, creating a “piggyback” sequence of calderas stacked atop one another — a geological nesting doll of destruction. This cycle repeated many times over the course of thirty million years, leaving behind layer upon layer of welded ignimbrite and flow-banded lava that together form the Talbot Sub-basin.
The cumulative volume of rhyolite erupted during this era reached several thousand cubic kilometres, rivaling the greatest volcanic provinces in history. What happened at Talbot wasn’t a single event; it was a long-lived volcanic field of super-eruptions, a slow-motion cataclysm that fundamentally reshaped central Australia.
One of the most extraordinary aspects of Talbot’s rocks is their oxygen isotope signature. Every sample of rhyolite and zircon from the sub-basin shows unusually low delta eighteen oxygen values — so low that they can only be explained if the magma had mixed with water that once existed on the surface. This means that before each eruption, enormous volumes of groundwater or rainwater must have infiltrated the crust, circulating through hot rock and altering its chemistry. When new magma intruded into these water-logged zones, it absorbed that isotopic signature, creating low-delta eighteen oxygen rhyolite.
This is incredibly rare in the geological record. The only comparable system on Earth today is the Snake River Plain–Yellowstone Plateau, which also produces oxygen-depleted rhyolites — but those eruptions are much younger, only a few million years old. The Talbot system is over a billion years older and yet displays the same isotopic fingerprint, suggesting the same processes were at work in the deep past: shallow crustal magma chambers repeatedly re-melting their own volcanic roofs under a continuous flush of meteoric water.
This isotopic depletion tells us something profound about the structure of the volcano. The chambers that fed Talbot’s eruptions must have sat within the upper ten kilometres of crust, where surface water could still circulate. That’s astonishing for an eruption field of this magnitude, because it means the magmas accumulated at very shallow depth, storing colossal energy just below the surface before blowing it sky-high.
Most modern supervolcanoes are linked to mantle plumes, those deep columns of hot rock that rise from the Earth’s core-mantle boundary. But the Talbot Supervolcano was different. It wasn’t fed by a plume at all. Its heat came from the crust itself.
After hundreds of millions of years of compression and radioactive decay, the crust of the Musgrave Province was already hot enough to melt under only modest additional heating. When fresh mafic magma from the Giles Event intruded into this thermally primed crust, it triggered runaway melting. The result was a colossal volume of juvenile felsic magma — new crustal material rather than recycled continental rock. Talbot, therefore, represents not just a destructive event but a creative one: it generated new continental crust on a massive scale, helping to thicken and stabilize the interior of Australia.
This makes the Talbot Sub-basin a geologic paradox — a system that behaved like a plume-fed hotspot but was entirely self-generated, powered by crustal heat and local tectonics. It shows that you don’t need a plume to make a supervolcano; sometimes, all you need is a thin piece of lithosphere, a trapped pocket of juvenile magma, and a lot of time.
As each eruption cycle ended, the collapsed caldera filled with welded tuffs, lava domes, and granophyric intrusions — the solidified remains of magma chambers. New basalt flows sometimes poured into the basin, marking a return to mafic volcanism before the next rhyolitic phase began. The landscape alternated between violent eruption and long dormancy, slowly building a volcanic succession up to nine kilometres thick.
Over time, as the crust stabilized, the final magma chambers cooled and crystallised into granite. The last eruptions likely produced sluggish domes rather than explosive ash clouds, signalling the gradual death of the volcanic field. Eventually the system fell silent, buried beneath younger sediments and eroded by a billion years of weathering.
In total, the Talbot Sub-basin likely produced many thousands of cubic kilometres of rhyolite, easily ranking it among the greatest volcanic accumulations in Earth’s history. But unlike Yellowstone, which remains restless today, Talbot’s fire has been cold for more than a billion years. Its heat has long since faded, leaving behind only isotopic clues and frozen magma bodies deep in the crust.
Because the evidence is so ancient and subtle, understanding Talbot has taken decades of detective work. The breakthrough came in the early 2010s, when researchers from the Geological Survey of Western Australia — notably David Smithies and colleagues — combined geochemical data, zircon isotope studies, and regional mapping to reveal the true scale of the system. Their results stunned even seasoned geologists. Not only was Talbot among the largest ancient volcanic provinces ever found, but its rocks recorded the same kind of isotopic fingerprints seen in young supervolcanoes, making it the oldest known analogue of Yellowstone on Earth.
They coined the term “piggyback supervolcanoes” to describe its sequential calderas and proposed that the Talbot field represents a new category of plume-free supervolcanism, driven entirely by crustal processes. In doing so, they redefined how scientists think about the origins of giant eruptions — showing that the Earth’s crust, under the right conditions, can generate its own cataclysm without help from the deep mantle.
Today, the Talbot Sub-basin sits in silence beneath the Australian desert. Its rhyolite domes have eroded into low hills, its caldera rims softened by a billion years of wind. No one lives there, and few people ever visit. Yet it remains one of the most extraordinary geological sites on the planet — a frozen memory of a time when the continent itself was molten and alive.