German scientists have discovered that the Earth has been receiving radioactive fallout for more than 100 million years due to the violent “kiss” of two supernovae.

Planet Earth is home to the ocean depths a radioactive plutonium deposit that could only be formed in space, during a violent cosmic cataclysm. Although there are reserves of this radioactive dust at great depths, it has been proven that it continues to rain down on us today. That would lead one to think that it was a recent cataclysm in astronomical terms. However, according to a recently published study by German scientistsit was hundreds of millions of years ago. Two isotopes to understand everything. Plutonium-244 does not exist naturally on Earth. In fact, the only isotope of this element that can be produced naturally in some geological processes is plutonium-239. and it does so mostly in the form of traces. Plutonium-244 is the heaviest isotope of this element. That is, the one with the most neutrons. It is known that it is usually formed by cosmic phenomena during something known as the r process, where lighter atoms quickly absorb neutrons into their nuclei. Generally, the event that usually gives rise to this phenomenon is the kilonova, an explosion resulting from the merger of two neutron stars. In the process, curium-247 is also formed, which is why these scientists have also analyzed its levels. Taking this data into account, they have discovered that the explosion in question must have occurred more than 100 million years ago, but less than one billion years ago. And, also, that the radioactive fallout has not stopped since then. The key is in the ferromanganese crust. Ferromanganese bark It is a layer of the ocean floor which is formed when metals dissolved in sea water, such as iron and manganese, are deposited and solidify. This occurs at a fairly slow rate, with growth of between 1 and 10 millimeters per million years. The deposits do not only have iron and manganese. Mixed with them are other substances that have fallen into the sea at that time. Therefore, this crust is a perfect chemical photograph of the history of our planet. A section with surprise. The authors of this study analyzed a section of this crust extracted at a depth of 4,830 meters in 1976. This had already been analyzed previously and had pointed out something surprising. And, in addition to plutonium, iron-60 was also found, another radioisotope associated with supernova explosions, which has a fairly short half-life of 2.6 million years. This figure means that, every 2.6 million years, half of the initial atoms of this isotope will have decayed. In another 2.6 million years half of what remained and so on. Since it is a fairly short half-life, it was concluded at the time that the kilonova that caused the fall of radioactive dust took place about 3 million years ago. However, the authors of the study just published debunked that hypothesis. Half-life of the study isotopes Curio to the rescue. The formation of plutonium-244 when neutron stars merge is always accompanied by the formation of curium-247. The plutonium isotope has a half-life of 81 million years, while that of curium “only” has a half-life of 15.6 million years. When analyzing the ferromanganese bark sample, these researchers found no curium. Therefore, it must have completely disintegrated. That places the explosion more than 100 million years ago. Be careful, remember that the half-life is the time it takes for half of the radioactive material to decay. Every 15.6 million years, half of it disintegrates, so in 100 million years there should be no curium left, but a lot of plutonium, which only lost half of it 19 million years ago. For plutonium to completely disappear, it would take 1 billion years. What about iron? The reason why there is iron-60 in the sample, despite having a lower half-life than that of curium-247, is that they originated in different events. In fact, the level changes of iron do not coincide with those of plutonium. On the other hand, it has been seen that plutonium continues to appear uniformly in the upper layers, hence it has been concluded that the radioactive fallout has not ended. At least it hadn’t ended in 1976 and that in astronomical terms was before yesterday. And now what? These scientists think that the cataclysm that released this long radioactive fallout must have been immense. Possibly even affected life on Earth. But at the moment it is something that cannot be known. We will have to continue investigating to have the answer. Image | University of Warwick/Mark Garlick | B. Schröder/HZDR/NASA, ESA, J. Hester, A. Loll/ASU In Xataka | Gravitational waves work their magic: we are closer to revealing the enigmas of neutron stars

that supernovae are behind two mass extinction events on Earth

When we think about mass extinctions, we almost always The asteroid that wiped out the dinosaurs comes to mind. But the universe has much more spectacular ways of reconfiguring life, as pointed out a scientific study which suggests that at least two of the ‘Big Five‘Earth extinctions were not caused by space rocks, but by the lethal radiation of stars exploding very close to our solar system. The study. The research, led by Alexis L. Quintana of the University of Alicante, has complicated the most complete census to date of OB type starsthe “heavyweights” of the galaxy. These stars are incredibly large, hot and luminous, and they live fast and die young, ending their lives in titanic explosions known as core collapse supernovae (ccSN). Space bombs. The team in this case has mapped 24,706 of these stars within a radius of 1 kiloparsec (about 3,260 light years) around the Sun. And with this map, they have been able to calculate something crucial: the frequency with which one of these cosmic bombs explodes in our neighborhood. The key fact is chilling: they estimate that a supernova close enough (about 20 parsecs or 65 light years) to wreak havoc on Earth that occurs about 2.5 times every billion years. This figure, which may seem low, fits eerily into the fossil record. A death mechanism. How exactly would a nearby supernova kill you? It’s not the blast wave, but the radiation. Such an energetic and upcoming explosion would bathe our planet in a torrent of gamma and cosmic rays, tearing apart our ozone layer. Without that protective shield, ultraviolet radiation from our own Sun became lethal, sterilizing the planet’s surface and causing ecological collapse. Specifically, the study points out that this rate of 2.5 events per billion years is “consistent” with the fact that one or more of the mass extinctions recorded on Earth were caused by this mechanism. Specifically, they point to two devastating events: Both extinctions have been linked by other studies to periods of intense glaciation and, crucially, a drastic reduction in atmospheric ozone, a “murder weapon” that points directly to a cosmic culprit. Updates. Beyond the threat to Earth, the new OB star census has allowed the team to recalculate the overall supernova rate for the entire planet. Milky Way. And here there has been a surprise: it is lower than we thought. Previous calculations put the rate at 1 or 2 explosions per century. The new study lowers it to 0.4 – 0.5 supernovae per century. The authors attribute this difference to the fact that their census is more precise and reliable thanks to Gaia data, since the models of how stars evolve have improved. This new figure is not just an astronomical curiosity; It is fundamental data for other fields of physics. For example, it is vital for calculating the frequency with which we should be able to detect gravitational waves coming from these explosions within our own galaxy. Our protection. Fortunately, a look at our current stellar neighborhood is reassuring. Although there are massive stars that we know will explode “soon” (in astronomical time), such as the famous red supergiants Antares and Betelgeuse, both are hundreds of light years away. They are too far away to fry us with their radiation, but close enough that when they finally detonate (which could happen tomorrow or 100,000 years from now), they will give us a light show in the sky that will last for weeks. Meanwhile, we now have a new suspect to blame for some of the worst catastrophes in the history of life, long before humans came along to witness it. Images | Aron Visuals 愚木混株 Yumu In Xataka | We could think of space as a place without climate threats to Earth. We could ignore the “space tornadoes”

Within the most advanced chips manufacturing machines there is something incredible: small supernovae

Identifying a Supernova is an event that astronomers usually celebrate with enthusiasm. And it is not for less if we consider that they are One of the most violent events with which we can run into the cosmos. Knowing them better is very important because it can help us understand more precision How are the latest stages of The life of mass starsand also the mechanisms that explain how the material caused by stellar synthesis can lead to new star systems. The mathematical tools handled by astrophysics current nuclear fusion that take place in the nucleus of mass stars. During the stage known as the main sequence, stars obtain their energy from the fusion of hydrogen nuclei. As this chemical element is consumed, the star begins to produce helium nuclei, and, of course, its composition begins to evolve. During this process a huge amount of energy is released and the star is forced to continuously readjust to maintain hydrostatic balance, a phenomenon that is the result of the coexistence of two opposite forces capable of compensating. One of them is the gravitational contraction, which compresses the subject of the star, pressing it without rest. And the other is the radiation and gase pressure, which is the fruit of the ignition of the nuclear oven and tries to expand the star. The small supernovae of the extreme ultraviolet lithography equipment As we have anticipated from the holder, this article does not go only from Supernovas; It is also starred by the semiconductors. A priori we can intuit that these cosmic events and integrated circuits have nothing to do, but, curiously, they do have something in common. This is the reason why I found a good idea to start this text reviewing what a supernova is and why they occur. Otherwise we could not understand in all its extension the idea in which we are about to investigate. The ultraviolet radiation generation process used by UVE lithography equipment is very similar to what happens during a Supernova In the teams of extreme ultraviolet lithography (UVE) that manufactures the Dutch company ASML, high power lasers instantly heat tens of thousands of tiny tin drops in a single second until they reach a temperature of half a million Celsius degrees. This interaction produces An extremely hot plasma that emits ultraviolet light with a wavelength of 13.5 nm. This light must later be transported to the wafer thanks to a very precise mirrors and lenses system with the purpose of capturing the patterns that define the integrated circuits on a layer of photorers. Very broadly this is the strategy used by the most advanced semiconductor manufacturing machines that currently exist. And, as we have just seen, high -power lasers interpret an unquestionably protagonist role. As Jays Stewart, Chief of Research at ASML, explains in the very interesting article he has published in IEEE Spectrumthe ultraviolet radiation generation process used by UVE lithography equipment to produce avant -garde chips is very similar to what happens during a supernova. When a massive star exhausts its fuel and stops nuclear fusion processes, radiation pressure and gases is no longer able to counteract gravitational contraction. This phenomenon causes the star iron core It suddenly contracts under the enormous pressure that all layers of material that it has above. The star has lost the hydrostatic balance. At this moment all this matter loses the support that the nucleus exercised, which is now much more compact, and falls on it with enormous speed. When all that star material touches the surface of the nucleus there is a rebound effect that causes it to be fired with a huge energy towards the stellar medium, being disseminated. A supernova has just been produced. Some of them are so energetic that for a few seconds they emit more light than the entire galaxy that contains them. The tiny explosions that take place inside the UVE lithography equipment when a laser affects a tin drop produce a shock wave similar to that originating in the stellar medium, although much smaller scale. Surprisingly the mathematical equations that describe the evolution of these two types of explosions are the same. ASML engineers use them to calculate very precisely how the evolution of the shock wave that triggers plasma balls within the UVE equipment will be. And astrophysicians use them to describe the remains of the supernovas and deduce the properties of the star explosion that originated them. A Supernova has 10⁴⁵ times more energy That an explosion of tin, but thanks to this parallel, ASML engineers have been able to solve the complex problem derived from tin residues inside their most advanced lithography equipment. Image | ASML More information | IEEE Spectrum In Xataka | ‘Focus: The Asml Way’: The book that reveals the secrets of the most powerful European company in the chips industry

We had to observe 4,000 supernovae to realize that something does not fit the explosions of the white dwarfs

Approximately a century ago we realized that the universe was not static but extended. Some theories even estimate that it does it at increasing speeds, but measuring this speed has become A major headacheas much as explaining the mechanisms that underlie this cosmic inflation. But maybe we are doing too many turns to the matter. Not so predictable. A study has observed That the supernovae associated with the white dwarf stars are not as predictable as we believed. The study presents us with a problem, and that is that the role of these explosions as markers of the cosmic distance is staggered now. Star milestones. Regular and predictable cosmic objects and events are of great help for astronomers when analyzing a vast and diverse cosmos. Know what intensity an object or a distant event shines opens the road to precisely calculating your distance based only on the intensity with which it shines in our sky. That is why these supernovas had been useful for calculating distances and with it the changes in the distance over time, that is to say the speed. The speed at which the objects of the cosmos move away from each other. Explosions of the most varied. The new study has revealed that supernovae associated with White dwarfs They are not in this group of regular cosmic events as we believed. Through its observations, the team found “multiple and exotic ways” in which white dwarfs could explode. These included collisions between two stars and star cannibalism in binary systems. “The diversity of ways in which white dwarfs can explode is much greater than it was previous And until years later ”´, pointed in a press release Kate Maguire, co -author of the study. 4,000 Supernovas. The finding was possible thanks to the use of tools capable of detecting very faint signals and the accumulation of a large amount of data for the sample. The team resorted to the data of the ZTF survey (Zwicky Transient Facity), From which they obtained information from a total of 4,000 supernovae, a sample, they explain, much greater than those previously compiled. “Thanks to the unique capacity of ZTF to scan the sky quickly and deeply, it has been possible Maguire added. The details of the study were recently published in a special number in the magazine Astronomy & Astrophysics. Dark energy. The finding is at the same time a problem and it is that if we lose one of the tools used to calculate the distances in the cosmos. In spite of this, it is great news since knowing that the outbreaks of white dwarf the one that moves away from us. In Xataka | What astronomers believed was going to be a boring supernova has revealed an enigma of the galactic dust Image | Trinity College Dublin

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