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Coating satellites with super-dark Vantablack paint could help fight light pollution crisis

Coating satellites with super-dark Vantablack paint could help fight light pollution crisis

Yahooa day ago

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A new type of super-black, highly resistant satellite paint promises an affordable fix to the satellite light pollution problem that has marred astronomical research since the recent advent of low-Earth-orbit megaconstellations.
One of these, the internet-beaming Starlink constellation, has been a matter of controversy since the launch of the first batch of its satellites in 2019. The constellation's thousands of spacecraft orbit so low that the sunlight they reflect outshines many stars from our perspective on Earth. And while the sight of a Starlink satellite train might thrill skywatchers, it's a true nightmare to astronomers worldwide.
When the $1.9 billion Vera Rubin Observatory opens its telescopic eyes to the sky later this month, astronomers expect that up to 40% of its images will be degraded or completely ruined by satellite streaks. It's a costly problem that will only become more serious as the number of satellites in orbit is expected to grow to tens of thousands within the next few years. But a new paint being developed in conjunction with astronomers might help. The paint, called Vantablack 310, could reduce the amount of light reflected by satellites in orbit down to just 2% of what is reflected by uncoated satellites, virtually erasing the pesky streaks from telescope images.
According to Noelia Noël, an astrophysicist at the University of Surrey, these satellite streaks will significantly reduce the scientific return on investment that the taxpayer-funded Vera Rubin telescope represents. Noël, who is expected to take part in Rubin's ten-year mission to map the sky in unprecedented detail, has been concerned about the loss of the pristine dark sky for years.
A native of Argentina, Noël grew up in awe of the star-studded southern sky and has been painfully aware of its deterioration. Those concerns led her to establishing a partnership with a University of Surrey spin-off, Surrey NanoSystems, who has been developing ultra black coatings for scientific instruments on satellites. The partnership has now produced a new type of blacker-than-black space paint, which reflects less light than available alternatives and can be easily applied by satellite makers in their clean rooms.
"Over the past five years, humankind has launched more satellites into space than it has done over the previous 60 years," Noël told Space.com. "It's a real problem for astronomy, especially for telescopes like Vera Rubin, which had to significantly change its observing strategy to avoid satellite clusters. So, I wanted to do something about it."
Surrey NanoSystems' previous coatings, although exquisite at reflecting light (the flagship Vantablack High Performance coating absorbs 99.9% of incoming sunrays), were based on delicate nanotechnology that required a technically complicated application process. Once applied, the coating couldn't be touched by a human hand or it would lose its anti-reflective properties.
"The previous coating was based on a carbon nanotube structure that can't be touched because it would collapse," Kieran Clifford, a materials scientist at Surrey NanoSystems, told Space.com. "We needed something that can be easily handled by engineers at their own facilities."
The new coating is based on a proprietary blend of carbon black, a soot-like form of carbon, mixed with special binders that make the paint resistant against the harsh conditions in near-Earth space. In tests, the new coating outperformed other similar paints currently on the market not just in terms of its light absorption ability but also durability in space, Clifford said.
"We conducted tests that simulated three years in orbit and our coating withstood it with negligible changes whereas other types of space paints completely eroded," said Clifford. "Our coating also offers a better optical performance. Where competitor coatings reflect about 5% of the incoming light, the Vantablack 310 coating only reflects 2% of the light across the visible and near infrared spectrum."
SpaceX has previously experimented with dark paint to reduce the brightness of its satellites, but those experiments provided mixed results. In some cases, the satellites began to overheat due to the amount of absorbed light. The new paint should not cause such problems, Clifford believes, and will make the satellites much less visible than the current Starlinks.
"We know from some simulations that we have done that our coating should make satellites invisible to the naked eye," Clifford said. "That's about magnitude 7 in terms of brightness while Starlink satellites range from magnitude 3 to magnitude 5."
Magnitude is a measure of luminosity of astronomical objects, which is inverse to the object's actual brightness. The lower the magnitude number, the brighter the object is. The magnitude scale is logarithmic, meaning the observed brightness increases exponentially with the decreasing magnitude number.
Surrey NanoSystems and the University of Surrey will test the Vantablack 310 coating in space on the student satellite Jovian 1, which will carry a range of payloads built by British universities to low Earth orbit next year.
"The rear of the satellite's deployable solar panel will be coated with Vantablack 310, and we will be rotating the satellite while making ground-based measurements to observe the changes in brightness," Clifford said.
The company is already in talks with satellite manufacturers. They hope that the ease of the paint's application, its exquisite durability and ability to reduce brightness will inspire them to use it on their satellites in the future.
"I don't want to be too optimistic, but I hope that with this new solution, we might be able to inspire some policy changes," Noël said. "Satellites are an amazing technology, but we also want to make sure that the sky remains accessible to everyone. Large telescopes represent a huge investment, and we want to make sure that it doesn't go to waste."

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Nvidia's latest project may supercharge quantum computing
Nvidia's latest project may supercharge quantum computing

Yahoo

time34 minutes ago

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Nvidia's latest project may supercharge quantum computing

Nvidia's latest project may supercharge quantum computing originally appeared on TheStreet. My first graphics card with an Nvidia () chip was Elsa Erazor III, powered by Riva TNT 2, back in 1999. If you will, God or the universe has a special sense of humor. Since then, the company's roots in making graphics cards for gaming—or, as I suspect most people would see it, wasting time—have allowed it to morph into the backbone of artificial intelligence and scientific computing. (Of course, gaming wasn't a waste of time for me. I've learned a lot and became an "IT" guy because of it.) Gaming is still a big business for Nvidia, but it is not nearly as crucial to the company as it was in the past. In its Q1 fiscal 2026 earnings release, Nvidia reported gaming revenue of a record $3.8 billion, up 48% from the previous quarter and 42% from a year ago. However, that is less than 9% of the company's total revenue of $44.1 grew out of gaming, for the better, just like me. I doubt the company's all done growing. The company recently announced it is building a supercomputer in partnership with Dell for NERSC, a U.S. Department of Energy user facility. It also addressed key issues investors had regarding China restrictions, supply chain capabilities, and the AI regulations. Nvidia's founder and CEO Jensen Huang, is always looking for new business opportunities, and many of them are outside America. NVIDIA, announced on June 9th on its blog, that Huang joined the U.K. Prime Minister Sir Keir Starmer to open London Tech Week. 'I make this prediction – because of AI, every industry in the UK will be a tech industry. The U.K. has one of the richest AI communities of anywhere on the planet, the deepest thinkers, the best universities, and the third largest AI capital investment of anywhere in the world,' said Huang. 'So the ability to build these AI supercomputers here in the U.K. will naturally attract more startups, it will naturally enable the rich ecosystem of researchers here to do their life's work,'Huang also revealed that Nvidia will start an AI lab in the UK. The U.K. will invest approximately £1 billion in AI research compute by 2030, with investments commencing this year, wrote Nvidia on its blog. In December 2024, Hewlett-Packard Enterprise announced that it is building a liquid-cooled supercomputer at Germany's Leibniz Supercomputing Centre, LRZ, but it didn't reveal which Nvidia chips will power the "Blue Lion." More Nvidia: Analysts issue rare warning on Nvidia stock before key earnings Analysts double price target of new AI stock backed by Nvidia Nvidia CEO shares blunt message on China chip sales ban Nvidia's blog confirmed on June 10th that Vera Rubin will power the Blue Lion. The superchip combines the Rubin GPU and Vera CPU. Vera CPU is Nvidia's first custom CPU, built to work in lockstep with the GPU. Vera Rubin's launch is set for the second half of 2026. Nvidia also announced that the Jupiter supercomputer, powered by the company's Grace Hopper platform, is the fastest in Europe. Compared with the next-fastest system, it is more than two times faster for high-performance computing and AI workloads. This beast of a supercomputer is hosted by the Jülich Supercomputing Centre at the Forschungszentrum Jülich facility in Germany and is owned by the EuroHPC Joint Undertaking. Huang stated, 'AI will supercharge scientific discovery and industrial innovation. In partnership with Jülich and Eviden, we're building Europe's most advanced AI supercomputer to enable the leading researchers, industries and institutions to expand human knowledge, accelerate breakthroughs and drive national advancement.'Jupiter will soon be capable of running 1 quintillion double-precision floating-point operations per second, which will make it Europe's first exascale supercomputer. Its speed is essential for simulations, training, and inference of the largest AI models, climate modeling, quantum research, structural biology, computational engineering, and astrophysics. It is also very efficient, at 60 gigaflops per watt. 'Jupiter will substantially advance quantum algorithm and hardware development. Hybrid quantum HPC-computation will profit from powerful tools such as the NVIDIA CUDA-Q platform and the NVIDIA cuQuantum software development kit.' stated Kristel Michielsen, codirector of the Jülich Supercomputing latest project may supercharge quantum computing first appeared on TheStreet on Jun 11, 2025 This story was originally reported by TheStreet on Jun 11, 2025, where it first appeared. Error in retrieving data Sign in to access your portfolio Error in retrieving data Error in retrieving data Error in retrieving data Error in retrieving data

This Revolutionary New Telescope Will Observe the Whole Sky Every Three Days
This Revolutionary New Telescope Will Observe the Whole Sky Every Three Days

Scientific American

time2 hours ago

  • Scientific American

This Revolutionary New Telescope Will Observe the Whole Sky Every Three Days

Astrophysics is, as many astrophysicists will tell you, the story of everything. The nature and evolution of stars, galaxies, galaxy clusters, dark matter and dark energy—and our attempts to understand these things—allow us to pose the ultimate questions and reach for the ultimate answers. But the practitioners of these arts, as the late astronomer Vera Rubin wrote in her autobiography's preface, 'too seldom stress the enormity of our ignorance.' 'No one promised that we would live in the era that would unravel the mysteries of the cosmos,' Rubin wrote. And yet a new observatory named for her, opening its eyes soon, will get us closer than ever before to unraveling some of them. This will be possible because the Vera C. Rubin Observatory will do something revolutionary, rare and relatively old-fashioned: it will just look out at the universe and see what there is to see. Perched on a mountaintop in the Chilean Andes, the telescope is fully assembled and operating, although scientists are not able to use it just yet. A few weeks of testing remain to ensure that its camera—the largest in astronomical history, with a more than 1.5-meter lens—is working as it should. Engineers are monitoring how Earth's gravity causes the telescope's three huge glass mirrors to sag and how this slight slumping will affect the collection and measurement of individual photons, including those that have traveled for billions of light-years to reach us. They are also monitoring how the 350-metric-ton telescope will rapidly pan across seven full moons' worth of sky, stabilize and go completely still, and take two 15-second exposures before doing it all over again all night long. On supporting science journalism If you're enjoying this article, consider supporting our award-winning journalism by subscribing. By purchasing a subscription you are helping to ensure the future of impactful stories about the discoveries and ideas shaping our world today. In this fashion, the scope plans to canvas the entire sky visible from Earth's Southern Hemisphere every three nights, remaking an all-sky map over and over again and noticing how it changes. And computer scientists are finalizing plans for how to sift through 20 terabytes of data every night, which is 350 times more than the data collected by the vaunted James Webb Space Telescope each day. Others are making sure interesting objects or sudden cosmic surprises aren't missed among Rubin Observatory's constant stream of images. Software will search for differences between each map and send out an alert about each one; there could be as many as 10 million alerts a night about potential new objects or changes in the maps. From finding Earth-grazing asteroids and tiny failed stars called brown dwarfs to studying the strangely smooth rotation of entire galaxies sculpted by dark matter, the Rubin Observatory's mission will encompass the entire spectrum of visible-light astronomy. The telescope will continue mapping the sky for 10 years. It may be better poised to answer astrophysicists' deepest questions than any observatory built to date. 'The potential for discovery is immense,' said Christian Aganze, a galactic archaeologist at Stanford University, who will use the observatory's data to study the history of the Milky Way. Put more specifically, Rubin Observatory will collect more data in its first year than has been collected from all telescopes in the combined history of humanity. It will double the amount of information available to astronomy—and to anyone trying to understand our place in the universe. The Rubin Observatory's Mission The observatory's goal was not always so broad. Originally named the Large Synoptic Survey Telescope (LSST), the Rubin Observatory was initially proposed as a dark-matter hunter. Vera Rubin found the first hard evidence for what we now call dark matter, a gargantuan amount of invisible material that shapes the universe and the way galaxies move through it. She and her colleague, the late astronomer Kent Ford, were studying the dynamics of galaxies when they made the discovery in the 1970s. In a spiral galaxy like our Milky Way, the galactic core contains more stars and hence gravity than the outer arms do. This should mean that the objects closer to the core spin around faster than the objects on the outskirts. By observing how stars move around and how their light appears shifted as a result, Rubin and Ford found that the stars on the outskirts were moving just as fast as the ones closer in. They found the phenomenon held across the dozens of galaxies they studied. This pattern defied explanation, unless there was some extra unseen material out there in the far reaches, causing the galaxy to rotate faster on what only appear to be the outer edges. Such dark materials had been proposed in the 1930s, but Rubin's findings showed the power they exerted over regular, visible matter and provided the first evidence that they existed. 'What you see in a spiral galaxy is not what you get,' Rubin once wrote. To date, no one has directly seen dark matter or come to understand its physical nature, including the particles that comprise it in the same way we know the electrons, protons and neutrons that make up regular matter, including galaxies, giraffes and us. Early plans for the LSST sought to shed light on dark matter by mapping its distribution throughout the universe via its gravitational effects. Astronomers also wanted to study how the cosmos is expanding through the work of an equally mysterious companion force called dark energy. But as design on the telescope systems began, astronomers quickly realized the LSST could do much more than study dark matter—it could study almost anything, seen or unseen. 'It is not a telescope that you will be sending proposals saying, 'I want to look over here.' The purpose is the survey,' says Guillem Megias Homar, a doctoral student at Stanford University and member of the telescope team. Mirrors and Cameras The open-ended surveying mission is a boon for astronomers, but it comes with intense design challenges. The telescope has to move across a swath of sky in just a few seconds and stop jittering almost immediately so that its images are clear. At other observatories, where astronomers choose targets ahead of time and plan what they're looking for, telescope engineers have maybe 10 minutes to stop the glass from wobbling in between taking images. Rubin Observatory gets five seconds, says Sandrine Thomas of the U.S. National Science Foundation National Optical-Infrared Astronomy Research Laboratory (NOIRLab), a deputy director of the observatory's construction. 'When you want to move that amount of mass very quickly and be stable, you can't have a very long telescope; otherwise the top wobbles,' she says. 'The light cannot go a long way before it loses focus, and that creates a lot of challenges.' To make the system more compact, Rubin Observatory's main telescope has a unique three-mirror structure. The primary and tertiary mirrors were fabricated to share the same piece of glass. Light bounces off the ring-shaped primary mirror and shines upward into a separate, secondary mirror, itself the largest convex mirror ever made. The secondary mirror again bounces the light back toward the tertiary mirror, which is inside the primary mirror's outer ring. The third mirror reflects light into the camera's sensitive detectors. The primary mirror and tertiary mirror combined give the telescope a collecting area of 6.67 meters. The secondary mirror has a 1.8-meter hole in the middle that the camera and its electronics fit into. And the tertiary mirror has a hole, too, for equipment designed to align the telescope and stop it from wobbling. The camera is a 10-meter-by-10-meter steel cube, small and compact. Margaux Lopez, a mechanical engineer, started working for the SLAC National Accelerator Laboratory after graduating from the California Institute of Technology in 2015 and has been working on the camera ever since. 'The point of this project is to collect a wild amount of data,' she says. 'How we actually do that is to see more of the sky at once, take more images at night and get more detail in each photo—that's the trifecta.' Astronomers often use the full moon's disk to describe a telescope's field of view; for an optical telescope, Rubin Observatory's view is unparalleled. The Hubble Space Telescope observes about one percent of a full moon, and JWST observes about 75 percent of the moon's disk. Each Rubin Observatory image captures an area about 45 times the size of the full moon, Lopez says. 'We are just seeing a wildly larger amount of sky with every image we take and getting an equal or greater amount of detail, even though the field of view is so big,' she says. The camera can take images in six filters, from the near ultraviolet to the near-infrared range. But astronomers must understand how the camera itself affects the images. Dark matter distorts the direction of photons streaming from distant galaxies, but so does the optics system, Megias Homar says. 'We really need to be sure about this. How is it affecting the light itself? If there is turbulence in the atmosphere or in the optics, a dot can become blurry,' Megias Homar says. He spent his doctoral program working on Rubin Observatory's optics system to understand this issue better. Mountaintop Observing After construction was complete, the telescope parts had to travel from California and Arizona to the top of Cerro Pachón, an 8,799-foot, seismically active peak in the Chilean Andes. Lopez and her colleagues chartered a Boeing 747 freighter jet to bring the camera from San Francisco to Santiago, Chile, in May 2024. The subsequent trip to La Serena, the city nearest the telescope's mountaintop home, required a 12-hour truck ride. Lopez monitored every step of the journey, even dealing with a trucking strike that threatened to blockade the route to Cerro Pachón. Finally, the camera made it to the literal mountaintop, where Lopez took it apart and checked everything. Teams of engineers, including Megias Homar, spent months testing the camera and its companion commissioning camera, a smaller version of the real thing that astronomers used to test all telescope systems, which went live on the sky in October 2024. The engineers shifted to nighttime work, sleeping during sunlight hours like astronomers do when they are at the observatory. 'That was the first time we saw images. For a whole month, I was going to sleep at 6 A.M. and feeling like an astronomer,' Megias Homar says. He worked with engineers and astronomers who have been planning and designing the LSST project since its inception. One person told Megias Homar they began working on it in 1996. 'I was born in 1997, so that was really humbling,' he says. Thomas has been part of the team for 10 years but got her start as an observer on a mountain next door to Rubin Observatory. 'When I joined the project, I did not appreciate how different this discovery machine or even this observatory was. I am coming from a normal, classical type of observing, which is submitting your proposal, maybe getting some time, maybe not,' she recalls. 'Bringing this amount of data to the community, to me, is just extremely rich.' For astronomers and astrophysicists, the richness is almost giddying. Rubin Observatory's 10-year main mission will provide a sort of time-lapse movie of the cosmos that will show other observatories where to look for new discoveries. A decade is not a long time in the history of the universe, but it is longer than anyone has ever stared at the sky. Telescope's First Light Galactic archaeologists like Aganze are hoping to study the history of our galaxy and how dark matter might be sculpting its evolution, just like the distant spiral galaxies Vera Rubin glimpsed a half century ago. Recent surveys from telescopes like the Gaia satellite show that the Milky Way is surrounded by streams of stars that might shed light on the dark matter halo that surrounds us. Galaxy streams can help astronomers understand when galaxy formation shuts off or how much dark matter must be around a smattering of stars for it to agglomerate into a galaxy. With Rubin Observatory, researchers should be able to see all the stars in a galactic stream, detect the stream's shape and even figure out what its associated dark matter must be like, Aganze says. And we could potentially do this for 100 or 200 galaxy streams around the Milky Way. 'If little dark matter clumps mess up the stars, we should be able to see it. We should be even able to put constraints on the dark matter—is it cold, warm or self-interacting?' Aganze says, describing three main theories for dark matter's properties. '[Rubin Observatory] is going to be great for this kind of science. We should definitely be able to march forward the limits of galaxy formation and the little dark matter halos.' The observatory will also find millions of new objects in our solar system, including 90 percent of all large asteroids that fly past Earth and thousands of tiny worlds far beyond Neptune's orbit. By essentially producing a time-lapse video, the observatory will unveil countless new transient and time-sensitive phenomena in the distant cosmos, such as quasars streaming from supermassive black holes. It will carefully scrutinize a special type of exploding binary star called a type Ia supernova that is essential for astronomy measurements and can shed more light on the nature of dark energy. Astronomers plan to share images from the camera—'first look,' as they are calling it—on June 23. Megias Homar says he is excited for the weeks ahead but admits that his first concern will be the optical system. 'I will be worried that this thing is working; that is where my mind is going to go first,' he says. And then he will turn his attention to the main mission: looking out at the cosmos. Astronomers eager to use the Rubin Observatory frequently talk about the value of just looking at the universe. Basic research is a public good, they say, that can provide new insight into our history while improving our shared future. 'It feels very much like a project based on curiosity,' Lopez says. 'Humans have always wanted to go to the top of the tallest mountain or the furthest reaches of the ocean, and this feels like one of those types of things. Let's create the coolest instrument we can to find out more about who we are.' Nobody ever promised that this generation of astronomers could unravel the mysteries of the cosmos, as Rubin herself reminds us. But right now we live in a time when we can try.

SpaceX rocket launch in Florida falls on Friday the 13th: What time does Falcon 9 lift off?
SpaceX rocket launch in Florida falls on Friday the 13th: What time does Falcon 9 lift off?

Yahoo

time3 hours ago

  • Yahoo

SpaceX rocket launch in Florida falls on Friday the 13th: What time does Falcon 9 lift off?

A rocket launch from Florida could potentially blast off on Friday the 13th. SpaceX is set to launch a batch of Starlink satellites into low-Earth orbit on June 13 from Cape Canaveral. Below is more information about the SpaceX rocket launch in Florida and suggestions on where to watch them from here. Rocket launch tally: Here's a list of all 2025 missions from Cape Canaveral, Florida (psst, there's a lot) For questions or comments, email FLORIDA TODAY Space Reporter Rick Neale at rneale@ or Space Reporter Brooke Edwards at bedwards@ For more space news from the USA TODAY Network, visit Tom Cruise and untitled SpaceX project: 'Mission: Impossible' star who lives in Florida may shoot a film in outer space Mission: SpaceX will launch a batch of broadband satellites for the ever-expanding Starlink constellation in low-Earth orbit, a Federal Aviation Administration operations plan advisory shows. Launch window: 7:45 a.m. to 12:16 p.m. EDT Friday, June 13, 2025 Launch location: Launch complex 40 at Cape Canaveral Space Force Station in Cape Canaveral, Florida Sonic booms: No Trajectory: Southeast Live coverage starts 90 minutes before liftoff at : You can watch live rocket launch coverage from USA TODAY Network's Space Team, which consists of FLORIDA TODAY space reporters Rick Neale and Brooke Edwards and visuals journalists Craig Bailey, Malcolm Denemark and Tim Shortt. Our Space Team will provide up-to-the-minute updates in a mobile-friendly live blog, complete with a countdown clock, at starting 90 minutes before liftoff. You can download the free FLORIDA TODAY app, which is available in the App Store or Google Play, or type into your browser. Shown is the National Weather Service-Melbourne radar, which shows conditions in real-time for the Space Coast, Brevard County, Orlando and other parts of Florida. The current date and time show up on the bottom right of this radar embed; otherwise, you may need to clear your cache. Weather permitting and depending on cloud cover, some rocket launches from the Space Coast can be visible in Palm Beach County. When there's a launch window in the middle of the night or very early morning, with a southeast trajectory, there's an opportunity for unique photos. Some examples include United Launch Alliance's Delta IV Heavy rocket launch and SpaceX Falcon Heavy rocket. From Cape Canaveral, Florida, to West Palm Beach, Florida, it's about 150 miles. What the views look like: Rocket launches from Cape Canaveral spotted in West Palm Beach Rocket launches from Cape Canaveral can often be seen from Palm Beach County, and it can be as easy as walking out of your house and looking north. Try to get away from any obstructions, such as trees, tall buildings, and bright lights. Obviously, cloud cover can also get in the way. If the forecast is for clear skies and you want a better view, some good places to watch the rocket launch from Palm Beach County include: : 14775 U.S. 1, Juno Beach : Downtown West Palm Beach, 620 South Flagler Drive : 300 block of South Ocean Boulevard : If you don't know, this is the island that connects Palm Beach and West Palm Beach on Southern Boulevard (near Mar-a-Lago, Trump's private club known as the Winter White House or Southern White House). There's a bridge with a pedestrian walkway over Bingham Island, on Southern Boulevard. : 10 South Ocean Blvd., Lake Worth Beach : 10216 Lee Road, Boynton Beach : 400 N. State Road A1A, Boca Raton This article originally appeared on Palm Beach Post: SpaceX rocket launch in Florida on Friday the 13th: When is liftoff?

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