We have so many satellites orbiting the Earth that they have become a barrier for someone: telescopes

For years, the astronomical community has looked at the sky with considerable concern from Earth. And it’s normal. In recent years, the number of satellites that we have put into orbit has grown exponentially, highlighting above all starlinkwhich promised to bring the internet to the entire planet in exchange for fill our nights with “trains of lights”. But this is only hindering our ability to continue investigating the universe where we are immersed. Trapped in a cage. The telescopes that we now have closer to Earth to do their work logically have to look towards our sky. The problem, as the research points out led by Alejandro S. Borlaff, is that they are going blind. Specifically, the low orbit (LEO) space telescopes that are not only not safe, but they are trapped in a real cage that prevents them from seeing further. Until now, it was possible to think that satellite traces could only affect terrestrial observatories. However, orbital reality is pure geometry: most large space telescopes like Hubble They orbit at about 540 km high. A height at which the internet megaconstellations that are located above or in the layers that range from 340 km to 8,000 km. Because. Satellites do not emit any type of light and should not cause problems. But the problem comes when they reflect sunlight, and when this happens in the new coverage satellites that have a large size, we find that even if it is night on Earth (or wherever the telescope is), at a hundred kilometers high the Sun continues to illuminate the satellite. And the lighting and telescopes they get along very badly. Space telescopes are designed to look at objects that are “still” at infinity (stars, galaxies). To capture its faint light, the telescope must fix its gaze on an exact point and not move. However, satellites move at thousands of kilometers per hour in relation to the telescope and since the camera shutter is open for a long time (long exposures of minutes or even hours) to capture weak light, the satellite crosses the entire frame during the photo, being recorded not as a point, but as a continuous line or “scar” of light. A problem. In this way, if a telescope is 540 km high when pointed at the sky, it will encounter an increasingly dense network of space traffic in the form of satellites. Specifically, there are currently about 15,000 satellites in orbit, but requests to different regulators suggest that we could reach half a million satellites by the end of the 2030s. Something that would leave large space observatories unusable. To put specific cases, we have the NASA Hubble that right now 3–4% of the images it captures have satellite trails. A figure that will increase to almost 40%, causing one in every three photographs of the most famous telescope in history to have a ‘light scar’. We have another case in SPHEREx which is the future explorer of the origins of the universe and which will have almost 100% of its catchments contaminated. Its impact. It is undoubtedly incalculable. Missions like ARRAKIHS (of the European Space Agency, with strong Spanish participation) or SPHEREx depend on taking very wide-field images to map the structure of the universe. By having such a large field of view, the probability of dozens of satellites being “snuck in” in a single shot is 100%. For him Chinese Xuntian Telescopewhich orbits lower, the situation is much worse. Being “below” most of the Starlink, Kuiper constellations and the Chinese networks themselves such as Guangwang You’ll have a harder time dealing with nearly a hundred bright lines crossing every image you take. The solution. Orbiting telescopes were a solution to this problem that was occurring in terrestrial telescopes. Now history repeats itself. Experts point to the need to define precise orbits so that telescopes can avoid satellites in a simple way. But this requires great international coordination to share this information and, above all, to regulate the number of launches that are carried out. Images | NASA Hubble Space Telescope In Xataka | Which telescope to buy to enjoy the nights and stars: 20 telescopes, binoculars, gadgets, accessories and more

A super -governor who will be connected to telescopes and laboratories

Supercomputing has never been just a matter of science. Since its origins, these colossal systems have represented national power, reflecting the technological, scientific and even military capacities of the countries that develop them. Now, The United States has presented His next big bet in this field: Doudna, a superorous who should see the light in 2026 and who promises to be more than ten times more powerful than Perlmutterthe current flagship of the Lawrence Berkeley National Laboratory. A tribute to science that changed biology. The new system has been baptized in honor of Jennifer DoudnaBerkeley’s biochemistry professor and one of the scientists who promoted CRISPR technology, Recognized with the Nobel Prize in Chemistry in 2020. It is not a minor gesture: the choice of the name symbolizes the fusion between biomedical research, artificial intelligence (AI) and computational power. Three axes that, together, aim to define the scientific advances of the next decades. What is exactly Doudna and what will you do. Doudna will be the next super -tider of the National Energy Research Scientific Computing Center (Nersc), a center of the United States Department of Energy located in Berkeley. Its design is in charge of Dell Technologies and will use the new platform Vera Rubin de Nvidiawhich will integrate ARM processors of general purpose. At a technical level, it is designed to execute large -scale hybrid work loads: high fidelity scientific simulations, training models of artificial intelligence, real -time data analysis and quantum algorithms. The machine will not be limited to executing tasks faster: it is designed to integrate into scientific workflows where the data comes from telescopes and laboratories. The objective is clear: to transform the way in which science is done, allowing to adjust experiments almost instantly and accelerate processes that took weeks or months. A project that wants to make a difference. Those responsible for the project are explicit: Doudna is presented as a key piece in the American strategy to lead the development of AI. Chris Wright, Secretary of Energy, It came to compare it with the Manhattan projectensuring that this supercomputer will be fundamental to win the Global AI race. Beyond the headline, the fields of application that are being prepared are ambitious. Nersc has already identified more than twenty scientific teams that are adapting their workflows for this system. The key tools are already on the table: from Frameworks such as Pytorch, Tensorflow and Cuda-Q to the Holoscan development kit, all optimized for the coherent architecture of Rubin and the NVLink interconnection. Why is it important at the national (and world) level. In a context of growing technological competition, especially with China, these types of systems represent more than a scientific resource. They are strategic infrastructure. Japan, with his escape; China, with its most recent Sunway Oceanlite; And now the United States, I already had Frontieramong others, it is reinforcing its muscle in this area with Doudna. The election of Dell against HPE also breaks with the usual dynamics of the great contracts of the Department of Energy, which until now had favored the latter in their three most recent exaescala systems. A jump in energy efficiency. In addition to gross power, one of Doudna’s great achievements will be its efficiency. According to NvidiaThe system will offer between three and five times more perlmutter performance. This is possible thanks to improvements in chips design, dynamic load balancing and new optimizations at the system level. When will it come and what is known about deployment. Douda’s launch is scheduled for 2026. We know that it will be built with servers Poweredge and advanced liquid cooling technologies of Dell, in addition to high -speed connectivity through the network Nvidia Quantum-X800 Infiniband. It will be located at the Berkeley Lab facilities and connected directly to the rest of the Energy Department centers through the scientific network ESNET. What has not been revealed, for now, is the official budget. Unlike the super -terrorist The Captain, which cost 600 million dollarsthe Department of Energy has not advanced any figure on the total investment in Doudna. Nor has it specified how many nodes or how much exact memory the system will have in its final configuration. But it has been made clear that it is designed to climb and adapt over time. Images | Nvidia (1, 2) | Lawrence Berkeley National Laboratory In Xataka | The EU wants to shorten distances in the race for the AI ​​with 750 million euros. And they are good news for Barcelona

Webb and Hubble telescopes watched Jupiter’s auroras at the same time. For some reason, they did not see the same

The Great red spot, Polar cyclones, Cloud bands. Jupiter is known for its colossal dimensions and eternal storms. But their auroras are not far behind, and only now We are seeing them in detail Thanks to the power of the James Webb space telescope. A Christmas gift. Newly published with a study of Nature Communicationsthe images were captured on December 25, 2023 with the Nircam Chamber of the Webb Telescope. The most immediate conclusion is that the jovian auroras are of another level. Hundreds of times brighter and more energy than those of the Earth, not only feed, as on our planet, of the particles loaded with the solar wind, but also of the volcanic material expelled by the active moon ío. Hyperactive. The team that led the observations took a surprise when analyzing the data. They hoped to see slow and gradual changes in the auroras, but instead they found “the entire bullendo region and exploding of light”, a hyperactive show that “varied in a matter of seconds.” “What a Christmas gift was that, he left me hallucinated!” Confesses the researcher Jonathan Nichols of the University of Leicester, the United Kingdom. A mystery. To round the study, the team coordinated Webb’s observations in infrared with Simultaneous observations of the Hubble Space Telescope in the ultraviolet spectrum. And here was the puzzle: the brightest lights observed by the Webb in Jupiter’s atmosphere did not have a counterpart in the Hubble images. The webb focused on trihydrogen cation emissions (H3+), a molecule that shines intensely in infrared when high -energy electrons impact molecular hydrogen. But to produce the combination of brightness observed by both telescopes, a huge amount of very low energy particles would be needed by hitting Jupiter’s atmosphere, something that until now was considered practically impossible. What follows. The team plans to study this difference between webb and Hubble data, and explore its implications for Jupiter’s environment. Webb’s next observations will be compared with NASA Juno probe data to try to unravel the origin of the broadcast. The findings will be used to guide the Juice Mission of ESA, who travels now to Jupiter. Seven of their instruments, including their two cameras, will dedicate themselves to study the Jovian auroras when the probe reaches their destination. Its nearby measurements will help astronomers better understand the interaction between the magnetic field and the planet’s atmosphere, in addition to the moon ío. Images | NASA, ESA, CSA In Xataka | These real images were unthinkable before the Webb Telescope: they are planets orbiting other stars to 130 light years

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