Monday, September 22, 2025
Celestial whack-a-mole
Friday, March 7, 2025
Deep impact
It's remarkably hard to find evidence of impact craters on the Earth.
If you're thinking, "What's the difficulty? Just look for a big hole in the ground," you're probably thinking of one of two things -- either craters on the Moon, or Barringer Crater near Winslow, Arizona. The craters on the Moon stick around pretty much indefinitely because the airless, waterless surface experiences virtually no erosion; as far as Barringer, the impact that caused it only happened around fifty thousand years ago, which is the blink of an eye, geologically speaking. (Plus, it's in the high desert, with little vegetation to hide underneath.)
With older impact craters, the forces of erosion eat away at the telltale signs -- the raised, oval or circular ridges, especially. The oldest craters have been destroyed by subsequent tectonic shifts and faults, and (for ones in oceanic plates) because the damaged strata themselves were subducted and melted.
One massive impact crater that was only detected in 1983 -- despite the fact that tens of thousands of people live more or less right on top of it -- is the one left by the Chesapeake Bay Impact Event, which occurred during the Eocene Epoch, on the order of 35.5 million years ago. At that point, the impact site, on the southern tip of the Delmarva Peninsula, was coastal tropical rainforest; the global temperature was still dropping following the massive Paleocene-Eocene Thermal Maximum, but was still a good two degrees Celsius warmer than today. The mass of the impactor isn't known for certain -- it was completely vaporized -- but it's estimated to have been about three kilometers across and traveling at eighteen kilometers per second, and punched a hole eight kilometers deep into the crystalline basement rock, blasting the sediments on top to smithereens and creating a crater over eighty kilometers across. Because at least part of the impact was in the shallow ocean, it also created a massive tsunami that travelled inland as far as the foothills of the Blue Ridge Mountains.
Since the impact, it refilled -- first with unconsolidated, unsorted sediments, essentially broken up pieces of the rock that was blown out from the collision, then with eroded material as the whole place gradually settled down. Part of it was refilled with seawater. The only way it was discovered was the presence of an anomalous "fault" that turned out to be the edge of the crater wall, followed by the analysis of some rock cores that showed a huge, thick layer of jumbled junk that geologists figured out was the debris formed as the crater walls slumped inward. It also explained the North American Tektite Field, an enormous splatter field of what amounts to cooled droplets of melted rock.
But visiting the area today, you don't see much that would tell you that only thirty-five million years ago, the place got slammed by an enormous chunk of rock from outer space.
Even the much larger Chicxulub Impact Crater, near the Yucatán Peninsula, took a lot of work to identify. It's just shy of twice as old as the Chesapeake Bay site (about 66 million years), and is almost entirely underwater and filled with oceanic sediments. Today, the impact site that ended the 180-million-year hegemony of the dinosaurs is only visible to sensitive gravitometers and magnetometers.
Which makes the discovery of an impact crater 3.47 billion years old, in East Pilbarra, Western Australia, even more astonishing.
A paper in Nature Communications this week, authored by Christopher Kirkland of Curtin University et al., shows convincing evidence of an impact crater over a hundred kilometers wide near the northwestern coast of Australia. The center of the crater shows regions of shocked crystalline rock, along with layers of breccia (the same sort of jumble of debris found at the Chesapeake Bay site). Further stratigraphic work has confirmed that this was, indeed, the site of a "massive hypervelocity impact." This makes it the only Archaean-age crater known to have survived.
The authors write:
Despite the high modeled frequency of bolide impacts in the early Archaean, the rarity of verified impact craters of Archaean age suggests that: (a) the impact flux was much less than predicted by lunar data; (b) the evidence has been eradicated, or (c) that we have failed to recognise them. On a young Earth covered in primitive (mafic–ultramafic) crust, identifying shatter cones or impact breccias may represent the best chance of finding other large Archaean impact structures. However, these highly fractured rocks will be the first to undergo (presumably intense) weathering and erosion. Notwithstanding their fragility, we believe many more Archaean craters await discovery.
Myself, I think it's astonishing that they've found even one. For any traces to have survived for nearly three and a half billion years is staggering. At that point, life was only getting started; the first known microbes appeared 3.7 billion years ago, and when the impact occurred, it would still be another half a billion years before the first certain multicellular life. So unlike the Chesapeake Bay and Chicxulub Impacts, which were (respectively) regionally and globally devastating to life, the East Pilbarra collision probably didn't make much of... um... an impact.
But it definitely stirred things up, created an enormous crater and rain of debris, and would have been a dramatic thing to witness. From a safe distance. The fact that even today, 3.47 billion years later, geologists can detect the hole it left behind, indicates that it was one hell of a punch.
Thursday, October 24, 2024
Impact
New from the "Well, I Guess That's A Silver Lining?" department, we have: a massive meteorite collision 3.26 billion years ago that may have jump-started the evolution of life on Earth.
And I do mean massive. This particular meteorite, given the unprepossessing name "S2," is estimated to have been a hundred times heavier than the Chicxulub Impactor that wrote finis on the Age of the Dinosaurs around 66 million years ago. The S2 impact in effect took a chunk of rock four times the size of Mount Everest and slung it toward Earth at the muzzle velocity of a bullet fired from a gun.
The evidence for this impact was found in one of the oldest exposed rock formations on Earth -- the Barberton Greenstone, on the eastern edge of the Kaapvaal Craton in northeastern South Africa. Geologists found tiny spherules -- microscopic glassy beads that result from molten rock being flung upward and aerosolized. The impact not only blasted and melted millions of tons of rock, it generated so much heat that it boiled off the upper layer of the ocean, and the liquid water left behind was turned into the mother of all tsunamis.
"Picture yourself standing off the coast of Cape Cod, in a shelf of shallow water," said Nadja Drabon of Harvard University, who led the study. "It’s a low-energy environment, without strong currents. Then all of a sudden, you have a giant tsunami, sweeping by and ripping up the seafloor."![]() |
Wednesday, August 9, 2023
Deep impact
Tektites are curious, glassy blobs of rock, from millimeters to centimeters in diameter. At first thought to be similar to obsidian (volcanic glass), formed when silica-rich lava cools too quickly to form crystals, it soon became apparent that tektites were something else entirely. They have strangely pitted surfaces, are often teardrop-shaped, and (once such studies became possible) they were found to have an entirely different chemistry than obsidian. Most puzzling was the fact that tektites are most often found in circumscribed geographical regions nicknamed "strewnfields" -- which usually were nowhere near recently-erupted volcanoes.
It wasn't until the 1920s that geologist Franz Eduard Suess proposed the theory now accepted today, and coined the name tektite (from the Greek τηκτός, "molten"). Tektites form when a meteorite strikes the Earth, liquefying the rock on the surface upon impact. The molten rock is thrown outward from the blast site, creating the circular or elliptical "strewnfield" -- and explaining why the blobs thus created don't match the chemistry of igneous rock. Their composition is different depending on the nature of the rock at the location where the meteorite struck.
So, you'd think once Suess said, "These are formed when a bigass rock slams into the ground" (I paraphrase him slightly), finding the crater where the thing landed would be easy, right? Just draw a circle around the strewnfield and then look in the middle?
Wrong.
There's a relatively recent strewnfield -- on the order of 790,000 years old, which is a snap of the fingers, geologically speaking -- that is abso-freaking-lutely huge. It extends from southern China to Antarctica (going north-south) and from the floor of the middle of the Indian Ocean to Micronesia (going west-east). And that's just where the tektites have been definitively identified. By some estimates, the Australasian strewnfield might cover thirty percent of the Earth's surface.
But the location of the crater proved elusive. Part of it is that the center of the strewnfield is in Southeast Asia, which is (mostly) impenetrable jungle, and in places the terrain is so steep and rugged as to be nearly impassable. But despite the difficulties, geologists have finally located the crater, and also determined why it wasn't obvious despite how recently it occurred.
The Australasian meteorite struck a spot in Laos that already had an active volcano.
The heat from the impact did two things -- flung blobs of molten rock all over the place (the tektites geologists later found in the strewnfield), and also triggered a massive eruption, producing a large enough lava flow to fill in and bury the crater.
What I find most astonishing about all this is that the impact of this gigantic rock, only 790,000 years ago, didn't cause climatic chaos and a resulting extinction event. Our relatives, Homo erectus, were living and apparently thriving in southern China both during and after the impact, and seem to have been none the worse for the event. (If some of them were in Laos, they were probably deep-fried; but given that there was an active volcano there anyhow...)
I wonder if the reason for the relatively low environmental impact had to do with the geology of the place the meteorite hit, which was primarily made of basalt and other hard igneous rocks. The Chicxulub strike, 66 million years ago, was devastating not only because it was so big, but because it hit a formation of shallow marine limestone, which literally vaporized on impact, creating a shock wave of superheated water vapor and carbon dioxide that incinerated everything within a radius of a thousand kilometers. There has to be more to it than simply size; the two weren't that different, an estimated two kilometers in diameter for the Australasian impact and between ten and twelve for Chicxulub.
Whatever the reason was for the difference, it's a good thing for us, because another Chicxulub-type event 790,000 years ago, and we'd very likely not be here.
In any case, it's pretty cool that we can use the splash patterns of molten debris to identify the location of a meteorite impact almost eight hundred thousand years after it happened, despite the fact that the whole thing was filled in with lava and overgrown by jungle. Further underscoring my bafflement over how anyone can not find science amazingly cool.
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Tuesday, March 1, 2022
Springtime collision
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Thursday, February 17, 2022
Big geology
It's easy to get overwhelmed when you start looking into geology.
Both the size scale and the time scale are so immense that it's hard to wrap your brain around them. Huge forces at work, that have been at work for billions of years -- and will continue to work for another billion. Makes me feel awfully... insignificant.
The topic comes up because of three recent bits of research into just how powerful geological processes can be. In the first, scientists were studying a crater field in Wyoming that dates to the Permian Period, around 280 million years ago (28 million years, give or take, before the biggest mass extinction the Earth has ever experienced). The craters are between ten and seventy meters in diameter, and there are several dozen of them, all dating from right around the same time. The thought was that they were created when an asteroid exploded in the upper atmosphere, raining debris of various sizes on the impact site.
The recent research, though, shows that what happened was even more dramatic.
"Many of the craters are clustered in groups and are aligned along rays," said Thomas Kenkmann of the University of Freiburg, who led the project. "Furthermore, several craters are elliptical, allowing the reconstruction of the incoming paths of the impactors. The reconstructed trajectories have a radial pattern. The trajectories indicate a single source and show that the craters were formed by ejected blocks from a large primary crater."
Saturday, October 26, 2019
Life finds a way
- tornadoes and hurricanes
- lightning
- earthquakes
- volcanoes
- death asteroids from outer space
But dwelling on that stuff is a little morbid, even if it's kind of awe-inspiring. So today, I'd like to look at some recent research that looks at how life recovered after the cataclysm -- discoveries that suggest the encouraging idea that even with a catastrophe, life can bounce back amazingly quickly.
A few years ago, Ian Miller and Tyler Lyson of the Denver Museum of Nature and Science were involved in a fossil dig in Corral Bluffs, Colorado, and made a rather astonishing discovery. Initially the area seemed to be rather fossil-poor, but it had a great many concretions (roughly spherical blobs of cemented sediment). When Miller and Lyson split one of these open, they found it was full of skeletal remains.
It turns out Corral Bluffs represent sedimentary layers of rock deposited immediately after the collision, so it provides an incredibly detailed record of the years following. Large animals and flowering plants (especially trees) were hit the hardest by the extinction; despite the prevailing wisdom that "dinosaurs died and mammals didn't," the more accurate statement is "big species were much more likely to die than little ones." The bottleneck, in fact, seems to have taken out all the mammals larger than your average rat. (Miller and Lyson found no evidence of mammals larger than six hundred grams that survived the extinction.) Miller, who is a paleobotanist, concentrated not on the animal remains but the plants -- especially the 37,000 pollen grains he found fossilized in the sediment layers. And from this, a picture began to emerge of what things were like in the years following the collision, which was described this week in a fascinating paper in Science.
The largest group of plants to come through the bottleneck were ferns, which thrive in disturbed areas and have spores that are pretty damage-resistant. Unfortunately for the animals, fern leaves and roots are rather low in nutrients, so for a while, body sizes remained small because there simply wasn't enough food around to support big, or even medium-sized, herbivores. But within a few thousand years -- a flash, evolutionarily speaking -- Fern World was replaced by Palm World, as proto-monocots (the group that contains not only palms, but grasses, lilies, orchids, irises, and a variety of other familiar plant families) evolved to be more robust. Palms have oily fruit that are high in sugar, and there's a commensurate jump in mammalian body size, with species showing up that weighed five kilograms.
Palms were superseded by the ancestors of today's walnuts and hickories a hundred or so thousand years after that, and in "Pecan Pie World" (as Miller and Lyson call this era), and the higher nutritional quality of those seeds fueled another jump in body size, with the largest ones reaching thirty kilograms (the size of a large dog). And after seven hundred thousand years, legumes diversified, and the high protein content of these species triggered another growth spurt, topping out at fifty kilograms -- a hundred times larger than the survivors of the collision, in less than a million years.
Nota bene: the growth in size wasn't done yet. The Oligocene Epoch, from 34 to 23 million years ago, saw the largest land mammals that have ever existed, including the enormous Baluchitherium, a behemoth that could have converted an African elephant into an African elephant pancake:
In keeping with Monday's post, this week's Skeptophilia book recommendation is about one of the most enigmatic figures in mathematics; the Indian prodigy Srinivasa Ramanujan. Ramanujan was remarkable not only for his adeptness in handling numbers, but for his insight; one of his most famous moments was the discovery of "taxicab numbers" (I'll leave you to read the book to find out why they're called that), which are numbers that are expressible as the sum of two cubes, two different ways.
For example, 1,729 is the sum of 1 cubed and 12 cubed; it's also the sum of 9 cubed and 10 cubed.
What's fascinating about Ramanujan is that when he discovered this, it just leapt out at him. He looked at 1,729 and immediately recognized that it had this odd property. When he shared it with a friend, he was kind of amazed that the friend didn't jump to the same realization.
"How did you know that?" the friend asked.
Ramanujan shrugged. "It was obvious."
The Man Who Knew Infinity by Robert Kanigel is the story of Ramanujan, whose life ended from tuberculosis at the young age of 32. It's a brilliant, intriguing, and deeply perplexing book, looking at the mind of a savant -- someone who is so much better than most of us at a particular subject that it's hard even to conceive. But Kanigel doesn't just hold up Ramanujan as some kind of odd specimen; he looks at the human side of a man whose phenomenal abilities put him in a class by himself.
[Note: if you purchase this book using the image/link below, part of the proceeds goes to support Skeptophilia!]



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