Software company Deno Land has filed a petition with the U.S. Patent and Trademark Office to cancel Oracle's JavaScript trademark, citing trademark abandonment and fraud. The November 22 filing claims Oracle has not sold JavaScript products or services since acquiring the trademark through its 2009 Sun Microsystems purchase. The petition alleges Oracle committed fraud during its 2019 trademark renewal by submitting Node.js website screenshots without authorization.

The legal action follows a September open letter from JavaScript creator Brendan Eich, Node.js and Deno creator Ryan Dahl, and other prominent JavaScript developers urging Oracle to relinquish the trademark. The letter has garnered over 14,000 signatures.

An asteroid named 2024 PT5, recently exhibiting "mini moon" behavior around Earth, may have been a boulder that was blasted off the moon by an impacting, crater-forming asteroid," reports the Associated Press. The 33-foot space rock is expected to pass safely near Earth in January, when it will be closely observed. From the report: While not technically a moon -- NASA stresses it was never captured by Earth's gravity and fully in orbit -- it's "an interesting object" worthy of study. The astrophysicist brothers who identified the asteroid's "mini moon behavior," Raul and Carlos de la Fuente Marcos of Complutense University of Madrid, have collaborated with telescopes in the Canary Islands for hundreds of observations so far.

Currently more than 2 million miles (3.5 million kilometers) away, the object is too small and faint to see without a powerful telescope. It will pass as close as 1.1 million miles (1.8 million kilometers) of Earth in January, maintaining a safe distance before it zooms farther into the solar system while orbiting the sun, not to return until 2055. That's almost five times farther than the moon. [...] NASA will track the asteroid for more than a week in January using the Goldstone solar system radar antenna in California's Mojave Desert, part of the Deep Space Network.

An anonymous reader quotes a report from VICE: It's early on a Sunday morning in late 1994, and you're shuffling your way through Fitzrovia in Central London, bloodstream still rushing after a long night at Bagley's. The sun comes up as you come down. You navigate side streets that you know like the back of your hand. But your hand's stamped with a party logo. And your brain's kaput. Coffee... yes, coffee. Good idea. Suddenly, you find yourself outside a teal blue cafe. Walking in is like entering an alien world; rows of club kids, tech heads, and game developers sit in front of desktops, lost in the primitive version of some new reality. Tentacular cables hang from the ceiling. Ambient techno reverberates from wall to wall. Cigarette smoke fills the air.

Welcome to Cyberia, the world's first internet cafe. Which, if you're too young to remember, are basically cafes with computers in them. It all began when Eva Pascoe, a Polish computing student living in London, crossed paths with Tim Berners Lee and other early internet mavericks at the dawn of the 90s. "I was very interested in cyberfeminism and wanted to figure out how women could reclaim tech," she recalls. The internet was still in its infancy. Diabolically slow dial-up modems only emerged around 1992; the World Wide Web was a pipe dream until 1993 and hardly anyone had the internet at home. But there wasn't just a lack of javascript; Eva remembers there being no good java, either. "There were no coffee shops in London," she says, which today seems ludicrous. "Just greasy spoons and everyone drank tea. I wanted a European-style cafe."

Linking up with like-minded pioneers David Rowe and husband and wife Keith and Gene Teare, Eva found a spot on the corner of Whitfield Street and launched Cyberia there in 1994. With Hackers-style aesthetics and futuristic furniture, it was based around a U-shaped layout that meant visitors could see each other's screens. "I wanted women to feel safe, because a lot of the stuff on the net was dodgy," she explains. Many of Eva's mates chipped in to help out -- architects, interior designers, graphic artists, publishers, and ravers among them.

And then there was the Amish community in Pennsylvania. Eva had to fly out there to negotiate for the "Cyberia.com" domain name they had bought. "It was a proper barn with horse carts and a wall of modems as they were running a bulletin board and an early ecommerce company. Apparently, there was always one family nominated to be the tech support," she remembers. Back in London, Cyberia quickly became a hotspot. "Virtually the second we opened, we had three lines deep around the block," she says. It's hard to imagine, but nowhere else in the world was doing what they were doing. It was the world's first cybercafe. "If you wanted to collect your emails, we were the only place in town," Eva says. Cyberia opened around 20 cafes worldwide, including branches in Bangkok, Paris, and Rotterdam. "For a fleeting moment it became like a sexier version of Richard Branson's Virgin empire: there was Cyberia Records, Cyberia Channel (a pioneering streaming service), Cyberia Payments, the Cyberia magazine, a Cyberia show on UK TV -- even a Cyberia wedding," writes VICE's Kyle MacNeill. He attended Cyberia's 30th birthday party in September and spoke with some of the cafe's original innovators, "shooting the shit about the good times and the not-so-good coffee."

Astronomers have discovered a supermassive black hole in the early Universe devouring matter at over 40 times the Eddington limit. ScienceAlert reports: Led by astronomer Hyewon Suh of Gemini Observatory and NSF's NOIRLab, a team of researchers used JWST to take follow-up observations of a smattering of galaxies identified by the Chandra X-ray Observatory that were bright in X-rays but dim in other wavelengths. When they got to LID-568, they were having trouble identifying its distance across space-time. The galaxy was very faint and very hard to see; but, using the integral field spectrograph on JWST's NIRSpec instrument, the team homed in on the galaxy's exact position. LID-568's far-off location is surprising. Although the object is faint from our position in the Universe, its distance means it must be incredibly intrinsically bright. Detailed observations revealed powerful outflows from the supermassive black hole, a signature of accretion as some of the material is being diverted and blasted into space.

A painstaking analysis of the data revealed that the supermassive black hole is a relatively small one, as supermassive black holes go; just 7.2 million times the mass of the Sun. And the amount of light being produced by the material around the disk was much, much higher than a black hole of this mass should be capable of producing. It suggests an accretion rate some 40 times higher than the Eddington limit. At this rate, the period of super-Eddington accretion should be extremely brief, which means Suh and her team were extremely lucky to catch it in action. And we expect that LID-568 will become a popular observation target for black hole scientists, allowing us a rare glimpse into super-Eddington processes. The research has been published in Nature Astronomy.

"It's that time again," writes USA Today, noting that Sunday morning millions of Americans (along with millions more in Canada, Europe, parts of Australia, and Chile) "will set their clocks back an hour, and many will renew their twice-yearly calls to put an end to the practice altogether..." Experts say the time changes are detrimental to health and safety, but agree that the answer isn't permanent DST. "The medical and scientific communities are unified ... that permanent standard time is better for human health," said Erik Herzog, a professor of biology and neuroscience at Washington University in St. Louis and the former president of the Society for Research on Biological Rhythms...

Springing forward an hour in March is harder on us than falling back in November. The shift in spring is associated with an increase in heart attacks, and car accident rates also go up for a few days after, he said. But the answer isn't permanent daylight saving time, according to Herzog, who said that could be even worse for human health than the twice-yearly changes. By looking at studies of people who live at the easternmost edge of time zones (whose experience is closest to standard time) and people who live at the westernmost edge (more like daylight saving time), scientists can tell that health impacts of earlier sunrises and sunsets are much better. Waking up naturally with the sun is far better for our bodies than having to rely on alarm clocks to wake up in the dark, he said.

Herzog said Florida, where [Senator Marco] Rubio has championed the Sunlight Protection Act, is much less impacted by the negative impacts of daylight saving time because it's as far east and south as you can get in the U.S., while people in a state like Minnesota would have much more time in the dark in the morning.
The article also reminds U.S. readers that "No state can adopt permanent daylight saving time unless U.S. Congress passes a law to authorize it first." Nevertheless... Oklahoma became the most recent state to pass a measure authorizing permanent daylight saving time, pending Congressional approval, in April. Nineteen other states have passed laws or resolutions to move toward daylight saving time year-round, if Congress were ever to allow it, according to the National Conference of State Legislatures...

Only two states and some territories never have to set their clocks forward or backward... [Hawaii and Arizona, except for the Navajo Nation.]

An anonymous reader quotes a report from The Guardian: A new global inventory has catalogued air pollution from space activities from 2020 to 2022. The inventory includes time, position and pollution from 446 launchers as they ascended and the tracks of re-entries as objects are heated to extreme temperatures and break up or burn up in the upper atmosphere. It catalogues the pollution from 63,000 tons of rocket propellants used in 2022 and from 3,622 objects, including rocket parts and satellites, that re-entered the atmosphere between 2020 and 2023, amounting to about 12,000 tons. [...]

Types of launch pollutants depend on the propellent but can include particles of soot and aluminum oxides as well as nitrogen oxides, chlorine and water vapour and carbon dioxide. Extreme heat on re-entry causes atmospheric oxygen and nitrogen to combine to form more nitrogen oxides and also produces tiny metal-oxide particles as the objects break and burn up. Soot emitted high in the atmosphere can persist for several years, with a resulting climate warming impact that is up to 500 times greater than the same amount of soot from aviation or ground-level sources. Aluminum oxide particles, nitrogen oxides and chloride can consume the ozone in the stratosphere that protects us from the sun's ultraviolet radiation. These can remain in the atmosphere for decades. Dr Connor Barker, of the UCL team, said: "Many rocket manufacturers and space agencies keep this information tightly controlled. We had to be creative about the different sources we consulted, from launch live streams on YouTube to online databases maintained by space enthusiasts in their spare time."

It was originally created back in 2005 by Sun Microsystems for its proprietary Solaris Unix systems, "for troubleshooting kernel and application problems on production systems in real time," explains Wikipedia. "DTrace can be used to get a global overview of a running system, such as the amount of memory, CPU time, filesystem and network resources used by the active processes," explains its Wikipedia entry.

But this week, Gentoo announced: The real, mythical DTrace comes to Gentoo! Need to dynamically trace your kernel or userspace programs, with rainbows, ponies, and unicorns — and all entirely safely and in production?! Gentoo is now ready for that!

Just emerge dev-debug/dtrace and you're all set. All required kernel options are already enabled in the newest stable Gentoo distribution kernel...

Documentation? Sure, there's lots of it. You can start with our DTrace wiki page, the DTrace for Linux page on GitHub, or the original documentation for Illumos. Enjoy!
Thanks to Heraklit (Slashdot reader #29,346) for sharing the news.

NASA has revealed a full-scale prototype for six telescopes designed to detect gravitational waves. Phys.Org reports: The LISA (Laser Interferometer Space Antenna) mission is led by ESA (European Space Agency) in partnership with NASA to detect gravitational waves by using lasers to measure precise distances -- down to picometers, or trillionths of a meter -- between a trio of spacecraft distributed in a vast configuration larger than the sun. Each side of the triangular array will measure nearly 1.6 million miles, or 2.5 million kilometers.

The Engineering Development Unit Telescope, which was manufactured and assembled by L3Harris Technologies in Rochester, New York, arrived at Goddard in May. The primary mirror is coated in gold to better reflect the infrared lasers and to reduce heat loss from a surface exposed to cold space, since the telescope will operate best when close to room temperature.

The prototype is made entirely from an amber-colored glass-ceramic called Zerodur, manufactured by Schott in Mainz, Germany. The material is widely used for telescope mirrors and other applications requiring high precision because its shape changes very little over a wide range of temperatures. The LISA mission is slated to launch in the mid-2030s.

An anonymous reader shares a report: Wikipedia's "Timeline of the Far Future" is one of my favorite webpages from the internet's pre-slop era. A Londoner named Nick Webb created it on the morning of December 22, 2010. "Certain events in the future of the universe can be predicted with a comfortable level of accuracy," he wrote at the top of the page. He then proposed a chronological list of 33 such events, beginning with the joining of Asia and Australia 40 million years from now. He noted that around this same time, Mars's moon Phobos would complete its slow death spiral into the red planet's surface. A community of 1,533 editors have since expanded the timeline to 160 events, including the heat death of the universe. I like to imagine these people on laptops in living rooms and cafes across the world, compiling obscure bits of speculative science into a secular Book of Revelation.

Like the best sci-fi world building, the Timeline of the Far Future can give you a key bump of the sublime. It reminds you that even the sturdiest-seeming features of our world are ephemeral, that in 1,100 years, Earth's axis will point to a new North Star. In 250,000 years, an undersea volcano will pop up in the Pacific, adding an extra island to Hawaii. In the 1 million years that the Great Pyramid will take to erode, the sun will travel only about 1/200th of its orbit around the Milky Way, but in doing so, it will move into a new field of stars. Our current constellations will go all wobbly in the sky and then vanish.

Some aspects of the timeline are more certain than others. We know that most animals will look different 10 million years from now. We know that the continents will slowly drift together to form a new Pangaea. Africa will slam into Eurasia, sealing off the Mediterranean basin and raising a new Himalaya-like range across France, Italy, and Spain. In 400 million years, Saturn will have lost its rings. Earth will have replenished its fossil fuels. Our planet will also likely have sustained at least one mass-extinction-triggering impact, unless its inhabitants have learned to divert asteroids.

Newsweek writes that the missing atmosphere of Mars "may be locked up in the planet's clay-rich surface, a new study by MIT geologists has suggested." According to the researchers, ancient water trickling through Mars' rocks could have triggered a series of chemical reactions, converting CO2 into methane and trapping the carbon in clay minerals for billions of years...

The dominant explanation relies on an interaction between the sun's rays and gases in the atmosphere. Mars lost its protective magnetic field billions of years ago, likely allowing high-energy solar particles to strike the upper atmosphere, kicking molecules off into space, according to NASA... But this might not be the whole story. The researchers focused on a type of clay mineral called smectite, known for its ability to trap carbon. These minerals, abundant on Mars, contain tiny folds that can store carbon molecules for aeons. The study was published in the journal Science Advances.

"There is plenty of evidence for a thick clay layer on the Martian surface. Almost 80 percent of satellite spectra detect these high-surface-area clay minerals on the Martian surface. Clay has been detected in craters as deep as 17 kilometers [10.5 miles]," [lead author Joshua] Murray said... Their model suggested that Mars' surface could contain up to 1.7 bar of CO2 — roughly 80 percent of its early atmospheric volume — sequestered as methane within clay deposits. This methane could still be present today, lying beneath the planet's dry and barren crust. "We know this process happens, and it is well-documented on Earth. And these rocks and clays exist on Mars," Oliver Jagoutz, the study's author, said in a statement. "So, we wanted to try and connect the dots."

The discovery that Mars' ancient atmosphere could be hidden within its surface clays offers a new perspective on the planet's history and raises intriguing possibilities for future exploration. For example, if the sequestered carbon could be recovered and converted, it could serve as a propellant for future space missions between Earth, Mars and beyond.
"In some ways, Mars' missing atmosphere could be hiding in plain sight," says the study's lead author — and the article adds that this raises some interesting possibilities.

"For example, if the sequestered carbon could be recovered and converted, it could serve as a propellant for future space missions between Earth, Mars and beyond..."

Black hole jets, which spew near-light-speed particle beams, can trigger nearby white dwarf stars to explode by igniting hydrogen layers on their surfaces. "We don't know what's going on, but it's just a very exciting finding," said Alec Lessing, an astrophysicist at Stanford University and lead author of a new study describing the phenomenon, in an ESA release. Gizmodo reports: In the recent work -- set to publish in The Astrophysical Journal and is currently hosted on the preprint server arXiv -- the team studied 135 novae in the galaxy M87, which hosts a supermassive black hole of the same name at its core. M87 is 6.5 billion times the mass of the Sun and was the first black hole to be directly imaged, in work done in 2019 by the Event Horizon Telescope Collaboration. The team found twice as many novae erupting near M87's 3,000 light-year-long plasma jet than elsewhere in the galaxy. The Hubble Space Telescope also directly imaged M87's jet, which you can see below in luminous blue detail. Though it looks fairly calm in the image, the distance deceives you: this is a long tendril of superheated, near-light speed particles, somehow triggering stars to erupt.

Though previous researchers had suggested there was more activity in the jet's vicinity, new observations with Hubble's wider-view cameras revealed more of the novae brightening -- indicating they were blowing hydrogen up off their surface layers. "There's something that the jet is doing to the star systems that wander into the surrounding neighborhood. Maybe the jet somehow snowplows hydrogen fuel onto the white dwarfs, causing them to erupt more frequently," Lessing said in the release. "But it's not clear that it's a physical pushing. It could be the effect of the pressure of the light emanating from the jet. When you deliver hydrogen faster, you get eruptions faster." The new Hubble images of M87 are also the deepest yet taken, thanks to the newer cameras on Hubble. Though the team wrote in the paper that there's between a 0.1% to 1% chance that their observations can be chalked up to randomness, most signs point to the jet somehow catalyzing the stellar eruptions.

It's hypothetically capable of "delivering an exquisite portrait of the detailed surface features of any exoplanet within 100 light-years..." writes Space.com.

"It would be better than any telescope we could possibly build in any possible future for the next few hundred years..." While the sun may not look like a traditional lens or mirror, it has a lot of mass. And in Einstein's theory of general relativity, massive objects bend space-time around them. Any light that grazes the surface of the sun gets deflected and, instead of continuing in a straight line, heads toward a focal point, together with all the other light that grazes the sun at the same time... The "solar gravitational lens" leads to an almost unbelievably high resolution. It's as if we had a telescope mirror the width of the entire sun. An instrument positioned at the correct focal point would be able to harness the gravitational warping of the sun's gravity to allow us to observe the distant universe with a jaw-dropping resolution of 10^-10 arcseconds. That's roughly a million times more powerful than the Event Horizon Telescope.

Of course, there are challenges with using the solar gravitational lens as a natural telescope. The focal point of all this light bending sits 542 times greater than the distance between Earth and the sun. It's 11 times the distance to Pluto, and three times the distance achieved by humanity's most far-flung spacecraft, Voyager 1, which launched in 1977. So not only would we have to send a spacecraft farther than we ever have before, but it would have to have enough fuel to stay there and move around. The images created by the solar gravitational lens would be spread out over tens of kilometers of space, so the spacecraft would have to scan the entire field to build up a complete mosaic image.

Plans to take advantage of the solar lens go back to the 1970s. Most recently, astronomers have proposed developing a fleet of small, lightweight cubesats that would deploy solar sails to accelerate them to 542 AU. Once there, they would slow down and coordinate their maneuvers, building up an image and sending the data back to Earth for processing...

The telescope already exists — we just have to get a camera in the right position.
Thanks to Tablizer (Slashdot reader #95,088) for sharing the article.

A small asteroid, 2024 PT5, will temporarily become a mini-moon for Earth, orbiting in a horseshoe shape from September 29 to November 25, 2024. CBS News reports: Researchers at the Asteroid Terrestrial-impact Last Alert System, an asteroid monitoring system funded by NASA, spotted the asteroid using an instrument in Sutherland, South Africa and labeled it 2024 PT5. Scientists from the Universidad Complutense de Madrid have tracked the asteroid's orbit for 21 days and determined its future path. 2024 PT5 is from the Arjuna asteroid belt, which orbits the sun, according to their study published in Research Notes of the AAs. But Earth's gravitational pull will draw 2024 PT5 towards it and, much like our moon, it will orbit our planet -- but only for 56.6 days. 2024 PT5, which is larger than some of the other mini-moons, will also return to Earth's orbit -- in 2055. [...]

The study's lead author Carlos de la Fuente Marcos told Space.com the mini-moon will be too small to see with amateur telescopes or binoculars but professional astronomers with stronger tools will be able to spot it.

"For 75 years Cosm built planetariums," reports a Texas news station, "and then a few years ago realized this technology could take you from the night sky to anywhere under the sun."

So now Los Angeles and Dallas have massive 9,600-square-foot, 8K-resolution screens that one reviewer for SFGate calls "an absolute game-changer" for sports fans. "At its best, Cosm's floor-to-ceiling screen gives anyone with a seat the opportunity to embrace a face full of on-the-field action at such high quality that it can be staggering, almost overwhelming at times — so just be sure to hold on tight, to the handrails and to your wallets."

There's also a bar with a 150-foot band of screens and a rooftop area with mounted TV, but they're "not why anyone has come," SFGate points out. Even the Dome has three distinct floors, though it's the second floor "where full visual immersion happens." The action feels so close, I can almost smell it, and all the focus is pulled to the center of the giant screen. Patrons truly do feel at the absolute heart of the action, with better seats than perhaps they could even pay for at Manchester's Old Trafford stadium. From a sports-viewing standpoint, I can't imagine it gets much better than this... Over the course of just a few minutes, the viewing angle flips from corner looks to right up against the goalkeeper's net, and then it widens out to dead center to catch crisp passes. Some angles put me right in the stands, cheering along with the loyalists at a stadium half a world away...

To be clear, the premium ticket costs are good for recouping Cosm's substantial investment in this gorgeous technological product, which has been in the works for years. The price tag is also likely to be little issue for any Los Angeles fan with money to spend, but the cost really does lay bare the growing division between the haves and have-nots in American sports society... If you paid $20 for a general admission entry that mostly just grants access to the fringes of the action, well ... good luck getting the most out of the Dome... The edges of the massive screen are stretched to comic effect, making the fisheye perspective more disorienting than fun. At the center of the room, it feels like you're absolutely in the meat of the action; at the fringes, you're left to pick at a few digital bones...

[F]or the rest of us, the normal sports fans who like to sway with strangers during the seventh-inning stretch, the ones who want to be able to take their kids to a game without feeling quite so financially wrung out, Cosm is yet another troubling sign of big, expensive things to come. Being a fan of a sports franchise in 2024 is an increasingly costly proposition. Watching your favorite NFL team now requires cable access, as well as multiple streaming services like Amazon Prime... There is no question that Cosm is a unique experience and that it will absolutely have a hand in transforming the modern digital sports-watching landscape, especially for those who want a digital re-creation of the best seat in the house over the camaraderie of a shared, in-person sports experience. The place will be able to charge incredible sums for the Super Bowl or World Series games, and — when at its best, with a prime seat in the middle of the action — the cost will be justifiable for many.

But for the folks at the financial fringes, the ones with the most spirit and often the least to spend, Cosm undoubtedly feels like a widening of the economic chasm that is pulling fans and their favorite teams further apart.
Besides sports events, Cosm's Dome also offers other immersive experiences like Circque du Soleil's "O" and Planetary Collective's "Orbital".

Another Cosm location is planned for Phoenix in 2025.

CrowdStrike CFO Burt Podbere says the cybersecurity firm has not faced lawsuits over July's global IT outage. Speaking at a conference, Podbere emphasized efforts to shift customer focus from legal threats to business discussions. The Register: There were dark rumblings from Delta Air Lines last month, for example, threatening litigation over alleged gross negligence. At the time, CrowdStrike reiterated its apologies, saying: "Public posturing about potentially bringing a meritless lawsuit against CrowdStrike as a long-time partner is not constructive to any party." During his time at the Citi conference, Podbere admitted: "We don't know how it's all going to shake out.

"Everything we're doing and trying to do is take the legal discussion away from our interaction with customers and move it to the business discussion. "And as time goes on, that does get easier because we're moving further away from the Sun, right? And that's how we think about it."

"China is on track to launch its Tianwen-3 mission to Mars in 2028, two years earlier than previously planned," writes the South China Morning Post, a change that one space policy research believes "suggests a rising confidence by China in its ability to get the technology right for the complex operation." On Thursday, Liu Jizhong, chief designer of China's Mars mission, told the Second International Conference on Deep Space Exploration in Huangshan, Anhui province, that the team aimed to bring back around 600 grams (21 oz) of Martian soil... A 2028 launch date should see Martian samples returned to Earth around July 2031, according to a previous presentation made by Tianwen-1 mission lead Sun Zezhou at Nanjing University in 2022.
The mission will actually consist of two launches from Earth, reports Space News: Two Long March 5 rocket launches will carry a lander and ascent vehicle and an orbiter and return module respectively. Entry, descent and landing will build on technology used for the Tianwen-1 rover landing. The mission may also include a helicopter and a six-legged crawling robot for collecting samples away from the landing site...

NASA is working on its own, more complex Mars sample return mission. However the program is being reassessed, following projected cost overruns. Studies are being conducted to identify concepts that can deliver samples faster and cheaper than current plans.

Liu stated that the search for evidence of life is the Tianwen-3's top scientific goal, according to state media China Central Television (CCTV). Earlier reporting notes that potential landing areas will be selected based partly on astrobiological relevance. This includes environments potentially suitable for the emergence of life and its preservation, such as sedimentary or hydrothermal systems, evidence of past aqueous activity and geological diversity.
"China states that it plans to work with scientists worldwide to cooperatively study and share Martian samples and data," according to the article: The China National Space Administration has made samples from its Chang'e-5 lunar nearside sample return mission available to research applications for international researchers. The same is expected for the recently-completed Chang'e-6 lunar farside mission."

Further ahead, Tianwen-3 will include partnering with countries and research institutions to define the objectives and tasks of a future Mars research station. This will include analyzing requirements, conducting conceptual studies, design implementation plans, and tackling key technological challenges.
Thanks to Slashdot reader Iamthecheese for sharing the news.

"Earth.com has an interesting article about the temporary "disappearance" of Saturn's rings in about six months," writes longtime Slashdot reader YVRGeek. From the report: Come March 2025, Saturn's majestic rings will become virtually invisible to earth-based observers. This phenomenon occurs due to the unique tilt of Saturn's axis, which will position the rings edge-on to our line of sight. [...] Saturn's axial tilt, which is the angle its axis leans compared to its orbit around the Sun, is about 27 degrees. As Saturn moves during its 29.5 year orbit around the Sun, this tilt means different parts of its rings and moons get sunlight at different angles, changing how they look. So, the rings are not really disappearing but rather playing a celestial game of hide and seek. At their reappearance, we can also enjoy an accentuated view of Saturn's moons.

An anonymous reader quotes a Bloomberg article, written by Jason Leopold: The aurora borealis, or northern lights, is a colorful display in the night sky that comes from geomagnetic storms in space. When charged particles from the sun smash into the Earth's upper atmosphere, they create bright, kaleidoscopic ribbons of light, typically in polar regions. Really big solar action can interfere with GPS systems and power grids. That's exactly what happened on May 10, when there were three "coronal mass ejections" (my future metal band name) that produced one of the most powerful solar storms in 500 years, hence the dazzling, polychromatic sky visible even from South America. Turns out, the extreme space weather also disrupted life on Earth.

Six days after the northern lights, I filed a Freedom of Information Act request with NOAA. I was curious how the agency reacted to the atmospheric event and whether the public deserved to be concerned. I asked NOAA's Space Weather Prediction Center and National Weather Service for a wide range of records, including emails, photographs, satellite images and threat assessments. A couple of weeks ago, NOAA turned over some interesting documents. The short version is, while we marveled at the light show, scientists were concerned. According to one internal memo, the geomagnetic storm was an "extreme," rare event and if NOAA scientists hadn't been on their game it could have been catastrophic.

A May 14, three-page after action memo disseminated by Clinton Wallace, the director of the Space Weather Prediction Center, described the storm's impact and explained the celestial phenomenon. He said "Solar Cycle 25," a phase of solar sunspot activity that began in December 2019 and continues through 2030, "has been more active than anticipated, with an intense surge in solar activity marking the beginning of May." "A large group of unstable sunspots on the Sun's surface unleashed several powerful solar flares, immediately affecting the Earth's outer atmosphere and causing disruptions in high-frequency (HF) radio communications," he wrote. "This had significant implications for trans-oceanic aviation, which relies heavily on HF radio for communication over long distances."

On May 9, a day before the northern lights extravaganza, staff at the Space Weather Prediction Center "activated" the North American Electric Reliability Corp. hotline to make sure the regulator was prepared. Wallace's memo said NERC gave about 3,000 electric utility companies a six-hour head start to get ready. The space weather officials also advised the Federal Emergency Management Agency and the Department of Homeland Security's Cybersecurity and Infrastructure Security Agency on preparedness. Wallace wrote in his memo that the storm caused "significant disruptions across multiple sectors, including navigation, power grids, aviation, and satellite operations." He also noted that the severity of the geomagnetic storm "underscored the interconnectedness and vulnerability of modern infrastructure to space weather." Although Wallace said the space weather scientists took steps to mitigate any potential disaster, their work "highlighted areas for improvement in preparedness and response." He didn't elaborate.

"Houston resident Brandy Deason put an Apple AirTag in her recycling to see where her plastic trash was going," writes Tom's Hardware.

"While many might expect the city would drop the recyclables off at a recycling center, Deason instead found her trash sitting in an open-air lot alongside millions of other pieces of trash at Wright Waste Management." Wright Waste Management did not allow CBS News to enter and inspect its premises. Still, the news team's drone camera discovered that all the trash picked up from the Houston Recycling Collaboration (HRC) was apparently just sitting there on its premises, stacked more than 10 feet high. This came as a shock, as the HRC was meant to revolutionize the city's recycling program, allowing it to process all kinds of plastic. Instead, we see all the collected waste sitting idle in open-air lots waiting for the right technology to appear.

That's because [Exxon-funded] Cyclix International, one of the partners in the HRC, has yet to open its massive factory to scale up its plastic recycling operation. The company said that it recycles all kinds of plastic and has even already set aside a sprawling space big enough to accommodate nine football fields. However, the current facility is just an empty husk without a single piece of machinery in sight.
Deason included 12 airtags in bags of recycling — and nine of them ended up at the HRC facility (with another one going to the local dump). In a video report, CBS News asked Deason what they thought about household recycling ended up in massive piles of plastic. "I thought it was kind of strange, because if you store plastic outside in the heat, it's a fire problem." In fact, that facility has already failed three fire-safety inspections by the county, according to CBS News. And while the facility has "applied" for approval to store plastic waste, that application has not yet been approved.

CBS asked a Cyclix project manager about the piles of unprocessed plastic sitting in the sun. "We need a huge supply of plastics to get ready for startup here," a spokesperson answered, "And we want to start that now in order to get ahead of it."

CBS's interviewer also raised another issue: the facility's plan is to recycle some of the plastic products into fuel. "So if you turn plastic waste into fuel that is then burned and creates greenhouse gas emissions, that's just another environmental problem."

Cyclix Project Manager: "Plastic waste is the challenge. So if we have the ability to take plastic waste and convert it to new products — that's what we're trying to do!"

CBS News points out that turning plastics into burn-able fuel is considered "recycling" by 25 states...

Longtime Slashdot reader AmiMoJo shares a report from Ars Technica, written by John Timmer: While solar power is growing at an extremely rapid clip, in absolute terms, the use of natural gas for electricity production has continued to outpace renewables. But that looks set to change in 2024, as the US Energy Information Agency (EIA) has run the numbers on the first half of the year and found that wind, solar, and batteries were each installed at a pace that dwarfs new natural gas generators. And the gap is expected to get dramatically larger before the year is over.

According to the EIA's numbers, about 20 GW of new capacity was added in the first half of this year, and solar accounts for 60 percent of it. Over a third of the solar additions occurred in just two states, Texas and Florida. There were two projects that went live that were rated at over 600 MW of capacity, one in Texas, the other in Nevada. Next up is batteries: The US saw 4.2 additional gigawatts of battery capacity during this period, meaning over 20 percent of the total new capacity. (Batteries are treated as the equivalent of a generating source by the EIA since they can dispatch electricity to the grid on demand, even if they can't do so continuously.) Texas and California alone accounted for over 60 percent of these additions; throw in Arizona and Nevada, and you're at 93 percent of the installed capacity.

The clear pattern here is that batteries are going where the solar is, allowing the power generated during the peak of the day to be used to meet demand after the sun sets. This will help existing solar plants avoid curtailing power production during the lower-demand periods in the spring and fall. In turn, this will improve the economic case for installing additional solar in states where its production can already regularly exceed demand. Wind power, by contrast, is running at a more sedate pace, with only 2.5 GW of new capacity during the first six months of 2024. And for likely the last time this decade, additional nuclear power was placed on the grid, at the fourth 1.1 GW reactor (and second recent build) at the Vogtle site in Georgia. The only other additions came from natural gas-powered facilities, but these totaled just 400 MW, or just 2 percent of the total of new capacity.

The EIA expects a bit over 60 GW of new capacity to be installed by the end of the year, with 37 GW of that coming in the form of solar power. Battery growth continues at a torrid pace, with 15 GW expected, or roughly a quarter of the total capacity additions for the year. Wind will account for 7.1 GW of new capacity, and natural gas 2.6 GW. Throw in the contribution from nuclear, and 96 percent of the capacity additions of 2024 are expected to operate without any carbon emissions. Even if you choose to ignore the battery additions, the fraction of carbon-emitting capacity added remains extremely small, at only 6 percent."