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Scientists Found Footprints That Push Humanity's Timeline Back By 40 Million Years

Scientists Found Footprints That Push Humanity's Timeline Back By 40 Million Years

Yahoo19-05-2025
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Here's what you'll learn in this story:
The common ancestor of all tetrapods (including humans) was previously thought to have emerged at the dawn of the Carboniferous period.
Fossilized tracks from an early reptile are now the oldest known reptilian tracks, meaning the tetrapod ancestor most likely appeared earlier, during the Devonian period.
These tracks were made by clawed feet—a characteristic of amniotes. Their appearance pushes back amniotes evolution by 35-40 million years.
Between 359 and 350 million years ago, it rained. Lizard-like creatures crawled through the mud in what was once Gondwana (but is now Australia), leaving behind footprints that became frozen in time, fossilizing as mud turned to stone over the aeons. These tracks would later be unearthed in an excavation that questioned how far back in time our tetrapod ancestors walked on land.
Tetrapods (meaning 'four legs' in Greek) include all amphibians, reptiles, birds, and mammals, and are thought to originate from lobe-finned fish that made their way out of primeval seas on fins that functioned as primitive legs. Humans are tetrapods, and like all tetrapods (except amphibians), we are also amniotes, with eggs that protect developing embryos in amniotic sacs. Amniotes are thought to have diverged from amphibians at the dawn of the Carboniferous period, about 355 million years ago. Mammals would diverge from reptiles and birds only 30 million years later.
The fossil footprints were discovered at the edge of an paleontological site in eastern Victoria known as Broken River (or Berrepit in Taungurung, the language spoken by local indigenous people). Whatever creature left imprints of its feet on the riverbank provides the first evidence of terrestrial life in this area, and claw marks from the footprints suggest it was an amniote—except that amniotes weren't supposed to have evolved so early in the Carboniferous period.
'This pushes back the likely origin of crown-group amniotes by at least 35-40 million years,' the Australian and Swedish team of researchers who excavated at the Berrepit site said in a study recently published in the journal Nature. '[Amniotes] cannot be much younger than the Devonian/Carboniferous boundary, and [the origin of tetrapods] must be located deep within the Devonian.'
Before this find, the oldest known amniote fossils were tracks from Notalacerta and the bones of Hylonomus. Both species were sauropsids—part of a larger group of extant and extinct reptiles and birds that presumably lived during the late Carboniferous. The common ancestor of all tetrapods was thought to have emerged in the earliest years of the Carboniferous, but that changed when this team of experts came upon the mysterious tetrapod footsteps from Berrepit. They now think that the tetrapod ancestor appeared during the Devonian, and that amniotes began to diverge from them about 395 million years ago, 35 to 40 million years earlier than previously thought.
It is evident that the footsteps came not just from a tetrapod, but from an amniote because almost all amniotes have claws or nails. Claw marks scratched the wet earth after a short rain shower, and there is no evidence of a body or tail dragged across the ground. While it is impossible to know what this animal actually looked like, the spacing between forefeet and hind feet indicates that it was about 17 cm (about 6.7 inches) from shoulder to hip, with neck, head, and tail lengths unknown. Using a modern water monitor as a proxy, the researchers determined it must have been about 80 cm (about 31.5 inches) total in length.
Something else could possibly be demystified by the footprints—the end-Devonian mass extinction was thought to have such a catastrophic impact, it could explain why tetrapods don't appear in the fossil record for another 20 million years. Tetrapods dating to after the gap are much more diverse and advanced than their pre-gap predecessors. Early Carboniferous sauropsid tracks mean that tetrapods must have been branching out from their common ancestor sometime during the Devonian, meaning that the mass extinction had little effect on the evolution of tetrapods.
'The [fossil footprints] have a disproportionate impact on our understanding of early tetrapod evolution because of their combination of diagnostic amniote characteristics and early, securely constrained date,' the researchers said. 'They demonstrate, once more, the extraordinary importance of happenstance and serendipity in the study of severely under-sampled parts of the fossil record.'
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A cosmic murder mystery: Scientists spot supernova of star violently stripped to the bone
A cosmic murder mystery: Scientists spot supernova of star violently stripped to the bone

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time11 hours ago

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A cosmic murder mystery: Scientists spot supernova of star violently stripped to the bone

Israeli and American scientists have uncovered a never-before-seen type of supernova, shedding light on how stars produce and expel heavy elements like silicon and sulfur during their violent deaths. Israeli and American scientists discovered a never-before-seen type of supernova, one that blasts out heavy elements like silicon and sulfur from the body of a dying star, a new study reveals. The findings of this study were published in the peer-reviewed academic journal Nature, and provide evidence for a long theorized part of stellar anatomy. All of this was made possible by witnessing an extremely violent and unusual death of a star, the result of which allowed scientists to look deeper than ever before. Of violence and onions: The death of a star and supernovae To understand what exactly happened, it's important to understand what a supernova is and, before that, to understand what a star is. 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But someone at the University of California, Berkeley, managed to get it. And the results were shocking. Normally, when studying a supernova, one expects to see the usual suspects of light and abundant elements, like helium, carbon, oxygen, and so on. But that's not what they found. Instead, the light fired out by SN2021yfj with its dying breaths consisted largely of sulfur, silicon, and argon. That's not supposed to happen. So how could the supernova just not have the lighter elements, and instead have the far heavier ones? A cosmic murder mystery: How a star was stripped to its core before death by explosion The conclusion Schulze came to was that something went wrong. Massive stars like SN2021yfj are, as mentioned previously, like onions - they have layers. And some of those layers have been peeled off. This itself isn't unheard of. Stripped stars, as they are known, have been seen before. 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Device inside black box holds secret to 'mind-blowing' Aussie breakthrough
Device inside black box holds secret to 'mind-blowing' Aussie breakthrough

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time13 hours ago

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Device inside black box holds secret to 'mind-blowing' Aussie breakthrough

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Violent supernova spilled a star's ‘guts' before exploding
Violent supernova spilled a star's ‘guts' before exploding

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time14 hours ago

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Violent supernova spilled a star's ‘guts' before exploding

A completely new supernova variant finally shows a glimpse of a star's innermost 'guts' moments before its destruction. Detailed in a study published August 20 in the journal Nature, their study confirms a longstanding theory about the internal structure of massive stellar objects, and kicks off a host of new questions. Diving into star innards Astronomers have long posited that a star's innards aren't simply a chaotic, roiling ocean of superheated plasma. Instead, they believe they possess layers of chaotic, roiling superheated plasma. In massive stars (those 10 to 100 times larger than the sun) nuclear fusion forces lighter elements in a stellar core to combine into heavier relatives. Over eons, these increasingly dense elements burn away within the core as lighter elements incinerate across successive, encompassing layers. This ultimately results in an incomprehensibly heavy iron core that, once collapsed, initiates a supernova or black hole event. Previously, researchers have documented examples of stripped stars that already lost their helium, exposing stratified, elemental encasements of helium, carbon, and even oxygen. This is usually where such glimpses always ended–until the discovery of SN2021yfj. 'Something very violent must have happened' In 2021, a team led by astrophysicists at Northwestern University utilized the wide-field camera array at the Zwicky Transient Facility (ZTF) near San Diego to scour the evening skies. ZTF's equipment is particularly designed to spot bright, short-lived events like supernovae. In September 2021, researchers noticed just such an occurrence roughly 2.2 billion light-years away. After some assistance from a collaborator at the W.M. Keck Observatory in Hawai'i, they then proceeded to conduct a spectrographic analysis of their supernova discovery, SN2021yfj.'Almost instantly, we realized it was something we had never seen before, so we needed to study it with all available resources,' study co-author and Northwestern University astrophysicist Steve Schulze said in a statement. Schulze and colleagues didn't find the elements they expected (helium, carbon, nitrogen, or oxygen). Instead, their spectrum analysis displayed huge amounts of silicon, sulfur, and argon. These are all heavier elements produced during stellar nuclear fusion near the end of a star's lifespan. 'This star lost most of the material that it produced throughout its lifetime,' explained Schulze. 'So, we could only see the material formed during the months right before its explosion. Something very violent must have happened to cause that.' 'Exotic pathways' to a star's demise That violent something is still a mystery, although researchers have a theory. This gigantic star had literally ripped itself apart from the inside, revealing a cosmic body 'stripped to the bone,' according to Schulze. The team believes that as the core condensed under its own gravitational strength, it became an even denser inferno. At a certain point, it became so hot and dense that it actually reignited a nuclear fusion process so powerful that it generated a huge energy burst. This, in turn, flung away the star's outer layers. Each subsequent 'pair-instability episode' then shed additional elemental layers. 'One of the most recent shell ejections collided with a pre-existing shell, which produced the brilliant emission that we saw as SN2021yfj,' Schulze theorized. However, he stopped short of saying this was the star's definitive cause-of-death. Other possibilities include a pre-supernova eruption, especially strong stellar winds, or even a run-in with an unknown companion star. 'I wouldn't bet my life that it's correct, because we still only have one discovered example,' said Schulze. 'This star really underscores the need to uncover more of these rare supernovae to better understand their nature and how they form.' But according to study co-author Adam Miller, the discovery doesn't mean he and other astrophysicists need to forget everything they know about star life cycles. 'It's not that our textbooks are incorrect, but they clearly do not fully capture everything produced in nature,' he said. 'There must be more exotic pathways for a massive star to end its life that we [haven't] considered.'

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