"The European Space Agency's Euclid space telescope launched at 11:12 a.m. ET Saturday," reports CNN, "aboard a SpaceX Falcon 9 rocket from Florida's Cape Canaveral Space Force Station.

CNN is calling it "a mission designed to unravel some of the greatest mysteries of the universe." The 1.2-meter-diameter (4-foot-diameter) telescope has set off on a monthlong journey to its orbital destination of the sun-Earth Lagrange point L2, which is nearly 1 million miles (1.6 million kilometers) away from Earth and also home to NASA's James Webb Space Telescope... After arriving at orbit, Euclid will spend two months testing and calibrating its instruments — a visible light camera and a near-infrared camera/spectrometer — before surveying one-third of the sky for the next six years. Euclid's primary goal is to observe the "dark side" of the universe, including dark matter and dark energy. While dark matter has never actually been detected, it is believed to make up 85% of the total matter in the universe. Meanwhile, dark energy is a mysterious force thought to play a role in the accelerating expansion of the universe.

In the 1920s, astronomers Georges Lemaître and Edwin Hubble discovered that the universe has been expanding since its birth 13.8 billion years ago. But research that began in the 1990s has shown that something sparked an acceleration of the universe's expansion about 6 billion years ago, and the cause remains a mystery. Unlocking the true nature of dark energy and dark matter could help astronomers understand what the universe is made of, how its expansion has changed over time, and if there is more to understanding gravity than meets the eye... Euclid is designed to create the largest and most accurate three-dimensional map of the universe, observing billions of galaxies that stretch 10 billion light-years away to reveal how matter may have been stretched and pulled apart by dark energy over time. These observations will effectively allow Euclid to see how the universe has evolved over the past 10 billion years...

The telescope's image quality will be four times sharper than those of ground-based sky surveys. Euclid's wide perspective can also record data from a part of the sky 100 times bigger than what Webb's camera can capture. During its observations, the telescope will create a catalog of 1.5 billion galaxies and the stars within them, creating a treasure trove of data for astronomers that includes each galaxy's shape, mass and number of stars created per year. Euclid's ability to see in near-infrared light could also reveal previously unseen objects in our own Milky Way galaxy, such as brown dwarfs and ultra-cool stars.

In May 2027, Euclid will be joined in orbit by the Nancy Grace Roman Telescope. The two missions will overlap in their study of cosmic acceleration as they both create three-dimensional maps of the universe...Roman will study one-twentieth of the sky in infrared light, allowing for much more depth and precision. The Roman telescope will peer back to when the universe was just 2 billion years old, picking out fainter galaxies than Euclid can see.
CNN points out that "While primarily an ESA mission, the telescope includes contributions from NASA and more than 2,000 scientists across 13 European countries, the United States, Canada and Japan."

And they also note this statement from Jason Rhodes, a senior research scientist at NASA's Jet Propulsion Laboratory. "With these upcoming telescopes, we will measure dark energy in different ways and with far more precision than previously achievable, opening up a new era of exploration into this mystery."

From NASA's announcement: Scientists are unsure whether the universe's accelerated expansion is caused by an additional energy component, or whether it signals that our understanding of gravity needs to be changed in some way. Astronomers will use Roman and Euclid to test both theories at the same time, and scientists expect both missions to uncover important information about the underlying workings of the universe...

Less concentrated mass, like clumps of dark matter, can create more subtle effects. By studying these smaller distortions, Roman and Euclid will each create a 3D dark matter map... Tallying up the universe's dark matter across cosmic time will help scientists better understand the push-and-pull feeding into cosmic acceleration.
SpaceX tweeted footage of the telescope's takeoff, and the successful landing of their Falcon 9's first stage on a droneship called A Shortfall of Gravitas.

The exoplanet 8 Ursae Minoris b should not exist. It orbits its host star at just half the Earth-Sun distance, and by all indications, the star should have gone through a phase in which it bloated up enough to engulf that entire orbit and then some. Yet 8 Ursae Minoris b definitely appears to exist. From a report: There is a handful of potential explanations, none of them especially likely. The people who discovered the planet are suggesting that it survived because its host star got distracted by swallowing a white dwarf instead. 8 Ursae Minoris b was discovered using the radial velocity method, which watches for changes in a star's light that occur as planets tug the star back and forth as they orbit. This tugging creates a blue shift in the light when the planet is pulling the star in the direction of Earth and a red shift when the star is pulled away from Earth.

But the planet is unlikely to be tugging the star directly toward Earth, so we tend to only measure the component of the star's motion that's in our direction. We'd see the same apparent motion of the star if a light planet's orbit was oriented directly toward Earth or a very heavy planet that has a relatively skewed orbit. At best, radial velocity measurements give us an estimate of the minimum mass of the planet; it could potentially be larger. So we know that, at minimum, 8 Ursae Minoris b is a big planet, at over 1.6 times the mass of Jupiter. It also resides close to its host star, completing a full orbit in just 93 days. That places it at half an Astronomical Unit (AU, the typical distance between Earth and the Sun) from its star.

Observations also hint at a second body orbiting the star at least five AU. The evidence for that is weak given the current data, but it may have a significant role in shaping the system. On its own, there's nothing especially unusual about the 8 Ursae Minoris exosolar system. Where things get weird is when you consider the star at the center of the system.

As part of a series of articles on smart homes, the Verge visits an energy-efficient home in the southern California desert that's "part of California's first planned smart, solar-powered residential microgrid community." A surprisingly small number of solar panels on the roof soak up the sun in the desert landscape... funneling power into the tightly designed building envelope. Here, a 13-kilowatt hour home battery sits beside a smart load panel that controls every electrical appliance in the home, from the hybrid electric heat-pump water heater and high-efficiency heat pump HVAC system — both Wi-Fi enabled to share data — to the light switches, EnergyStar fridge, and energy-efficient induction cooktop. Using software algorithms, the Schneider load center intelligently determines where to best draw power from — the SunPower solar panels, the battery, or the grid. It then makes recommendations the Conriques can use to set automations that change power sources or reduce energy use when prices and demand spike...

The 43 new residences in KB Home-built Shadow Mountain, which launched in November 2022, and the 176 more planned as part of two communities, Durango and Oak Shade, are all-electric, solar-powered smart homes. By next year they will be connected to a 2.3 megawatt-hour community battery, sending any excess energy their panels generate to the common power source and creating a community microgrid. When the power goes down, the microgrid will kick in, isolating all 219 homes from the grid and keeping their essential functions up and running. The homes will draw first from their own battery (and potentially their EV) and then from the community battery. "When the system hits a potential steady state, they can ride a power outage for days, if not in perpetuity, with proper solar production," explains Brad Wills of Schneider Electric, manufacturers of the home's smart load panel, the community's microgrid components, and the software that runs the system...

Developed as a partnership between SunPower, KB Home, University of California, Irvine, Schneider Electric, Southern California Edison, Kia America, and the US Department of Energy, Shadow Mountain is designed to be a blueprint for how we can build better, smarter communities in the future... A recent DOE study estimated that by 2030, grid-interactive efficient buildings like those at Shadow Mountain could save up to $18 billion per year in power system costs and cut 80 million tons of carbon emissions annually.
The article describes how the community helps the larger power grid:

• They can send electricity back into the grid during periods of peak demand.

• The local power company now also has the option to "island" the entire community off the grid in times of high demand.

• The community "is also trialing high-output vehicle-to-home and vehicle-to-grid functions."

An anonymous reader quotes this report from the Washington Post: In a new study released in Nature this week, researchers state that Earth formed within just 3 million years. That's notably faster than previous estimates placing the timeline up to 100 million years.... "We can also predict that if other planets formed ... by the same mechanism, then the ingredients required for life such as water, should be present on other planets and other systems, so there's a greater chance that we have water worlds elsewhere in the galaxy," said Isaac Onyett, lead author of the study and Ph.D. candidate at the University of Copenhagen.

The authors assert that this rapid genesis occurred through a theory called pebble accretion. The general idea, according to co-author and cosmochemist Martin Bizzarro, is that planets are born in a disk of dust and gas. When they reach a certain size, they rapidly attract those pebbles like a vacuum cleaner. Some of those pebbles are icy and could provide a water supply to Earth, thought of as pebble snow. This would have led to an early version of our planet, known as proto-Earth, that is approximately half the size of our present-day planet. (Our current rendition of Earth likely formed after a larger impact about 100 million years later, which also led to the formation of our moon....)

The team determined the time scale of Earth's formation by looking at silicon isotopes from more than 60 meteorites and planetary bodies in the vicinity of Earth, which represent the rubble leftover after planet formation... By analyzing the silicon compositions in samples of different ages, Onyett said they can piece together a time sequence of what was happening in the disk of dust before Earth formed. They found that, as the samples increased in age, the composition of the asteroids changed toward the composition of the cosmic dust that was being accumulated by Earth. "That's very strong evidence that this dust was also being swept up as it was drifting inwards towards the Sun," said Onyett. "It would have been swept up by Earth as it was growing by accretion."

Birger Schmitz, an astrogeologist at Lund University who was not involved in the research, said these results are "very compelling" and could shift how we think about our planet's formation... Most importantly, he said the results show there is nothing special about our water-carrying planet. "It is just a very ordinary planet in our galaxy. This is important in our attempts to understand how common higher forms of life are in the universe."
While scientists agree pebble accretion does explain the formation of gas-giant planets like Jupiter and Saturn, some still argue that rocky planets like Earth were instead formed through larger and larger asteroid collisions...

An anonymous reader quotes a report from Scientific American: It could be a new world record, although no one involved wants to talk about it. In the south of France, a collaboration among 35 countries has been birthing one of the largest and most ambitious scientific experiments ever conceived: the giant fusion power machine known as the International Thermonuclear Experimental Reactor (ITER). But the only record ITER seems certain to set doesn't involve "burning" plasma at temperatures 10 times higher than that of the sun's core, keeping this "artificial star" ablaze and generating net energy for seconds at a time or any of fusion energy's other spectacular and myriad prerequisites. Instead ITER is on the verge of a record-setting disaster as accumulated schedule slips and budget overruns threaten to make it the most delayed -- and most cost-inflated -- science project in history.

The ITER project formally began in 2006, when its international partners agreed to fund an estimated [$6.3 billion], 10-year plan that would have seen ITER come online in 2016. The most recent official cost estimate stands at more than [$22 billion], with ITER nominally turning on scarcely two years from now. Documents recently obtained via a lawsuit, however, imply that these figures are woefully outdated: ITER is not just facing several years' worth of additional delays but also a growing internal recognition that the project's remaining technical challenges are poised to send budgets spiraling even further out of control and successful operation ever further into the future.

The documents, drafted a year ago for a private meeting of the ITER Council, ITER's governing body, show that at the time, the project was bracing for a three-year delay -- a doubling of internal estimates prepared just six months earlier. And in the year since those documents were written, the already grim news out of ITER has unfortunately only gotten worse. Yet no one within the ITER Organization has been able to provide estimates of the additional delays, much less the extra expenses expected to result from them. Nor has anyone at the U.S. Department of Energy, which is in charge of the nation's contributions to ITER, been able to do so. When contacted for this story, DOE officials did not respond to any questions by the time of publication.

Owen Gingerich, a renowned astronomer and historian of science, has passed away at the age of 93. Gingerich dedicated years to tracking down 600 copies of Nicolaus Copernicus's influential book "De Revolutionibus Orbium Coelestium Libri Sex" and was known for his passion for astronomy, often dressing up as a 16th-century scholar for lectures. He believed in the compatibility of religion and science and explored this theme in his books "God's Universe" and "God's Planet." The New York Times reports: Professor Gingerich, who lived in Cambridge, Mass., and taught at Harvard for many years, was a lively lecturer and writer. During his decades of teaching astronomy and the history of science, he would sometimes dress as a 16th-century Latin-speaking scholar for his classroom presentations, or convey a point of physics with a memorable demonstration; for instance, The Boston Globe related in 2004, he "routinely shot himself out of the room on the power of a fire extinguisher to prove one of Newton's laws." He was nothing if not enthusiastic about the sciences, especially astronomy. One year at Harvard, when his signature course, "The Astronomical Perspective," wasn't filling up as fast as he would have liked, he hired a plane to fly a banner over the campus that read: "Sci A-17. M, W, F. Try it!"

Professor Gingerich's doggedness was on full display in his long pursuit of copies of Copernicus's "De Revolutionibus Orbium Coelestium Libri Sex" ("Six Books on the Revolutions of the Heavenly Spheres"), first published in 1543, the year Copernicus died. That book laid out the thesis that Earth revolved around the sun, rather than the other way around, a profound challenge to scientific knowledge and religious belief in that era. The writer Arthur Koestler had contended in 1959 that the Copernicus book was not read in its time, and Professor Gingerich set out to determine whether that was true. In 1970 he happened on a copy of "De Revolutionibus" that was heavily annotated in the library of the Royal Observatory in Edinburgh, suggesting that at least one person had read it closely. A quest was born. Thirty years and hundreds of thousands of miles later, Professor Gingerich had examined some 600 Renaissance-era copies of "De Revolutionibus" all over the world and had developed a detailed picture not only of how thoroughly the work was read in its time, but also of how word of its theories spread and evolved. He documented all this in "The Book Nobody Read: Chasing the Revolutions of Nicolaus Copernicus" (2004). John Noble Wilford, reviewing it in The New York Times, called "The Book Nobody Read" "a fascinating story of a scholar as sleuth."

Professor Gingerich was raised a Mennonite and was a student at Goshen College, a Mennonite institution in Indiana, studying chemistry but thinking of astronomy, when, he later recalled, a professor there gave him pivotal advice: "If you feel a calling to pursue astronomy, you should go for it. We can't let the atheists take over any field." He took the counsel, and throughout his career he often wrote or spoke about his belief that religion and science need not be at odds. He explored that theme in the books "God's Universe" (2006) and "God's Planet" (2014). He was not a biblical literalist; he had no use for those who ignored science and proclaimed the Bible's creation story historical fact. Yet, as he put it in "God's Universe," he was "personally persuaded that a superintelligent Creator exists beyond and within the cosmos." [...] Professor Gingerich, who was senior astronomer emeritus at the Smithsonian Astrophysical Observatory, wrote countless articles over his career in addition to his books. In one for Science and Technology News in 2005, he talked about the divide between theories of atheistic evolution and theistic evolution. "Frankly it lies beyond science to prove the matter one way or the other," he wrote. "Science will not collapse if some practitioners are convinced that occasionally there has been creative input in the long chain of being." In 2006, Gingerich was mentioned in a Slashdot story about geologists' reacting to the new definition of "Pluton." He was quoted as saying that he was only peripherally aware of the definition, and because it didn't show up on MS Word's spell check, he didn't think it was that important."

"Gingerich lead a committee of the International Astronomical Union charged with recommending whether Pluto should remain a planet," notes the New York Times. "His panel recommended that it should, but the full membership rejected that idea and instead made Pluto a 'dwarf planet.' That decision left Professor Gingerich somehwat dismayed."

The New York Times defines the solar wind as "a million-miles-per-hour stream of electrons, protons and other charged particles rushing outward into the solar system."

Now CNN reports that the Parker Solar Probe "has uncovered the source of solar wind." As the probe came within about 13 million miles (20.9 million kilometers) of the sun, its instruments detected fine structures of the solar wind where it generates near the photosphere, or the solar surface, and captured ephemeral details that disappear once the wind is blasted from the corona...A study detailing the solar findings was published Wednesday in the journal Nature...

There are two types of this wind. The faster solar wind streams from holes in the corona at the sun's poles at a peak speed of 497 miles per second (800 kilometers per second)... The spacecraft's data revealed that the coronal holes act like showerheads, where jets appear on the sun's surface in the form of bright spots, marking where the magnetic field passes in and out of the photosphere. As magnetic fields pass each other, moving in opposite directions within these funnels on the solar surface, they break and reconnect, which sends charged particles flying out of the sun.

"The photosphere is covered by convection cells, like in a boiling pot of water, and the larger scale convection flow is called supergranulation," said lead study author Stuart D. Bale, a professor of physics at the University of California, Berkeley, in a statement. "Where these supergranulation cells meet and go downward, they drag the magnetic field in their path into this downward kind of funnel. The magnetic field becomes very intensified there because it's just jammed. It's kind of a scoop of magnetic field going down into a drain. And the spatial separation of those little drains, those funnels, is what we're seeing now with solar probe data."

Parker Solar Probe detected highly energetic particles traveling between 10 and 100 times faster than the solar wind, leading the researchers to believe that the fast solar wind is created by the reconnection of magnetic fields. "The big conclusion is that it's magnetic reconnection within these funnel structures that's providing the energy source of the fast solar wind," Bale said. "It doesn't just come from everywhere in a coronal hole, it's substructured within coronal holes to these supergranulation cells. It comes from these little bundles of magnetic energy that are associated with the convection flows."

Artificial photosynthesis, inspired by the natural process that enables plants to convert sunlight, water, and carbon dioxide into oxygen and energy, could be crucial for space exploration and colonization. By using semiconductor materials and metallic catalysts, these devices could efficiently produce oxygen and recycle carbon dioxide, reducing reliance on heavy and unreliable systems currently used on the International Space Station. ScienceAlert reports: As my colleagues and I have investigated in a new paper, published in Nature Communications, recent advances in making artificial photosynthesis may well be key to surviving and thriving away from Earth. [...] We produced a theoretical framework to analyze and predict the performance of such integrated "artificial photosynthesis" devices for applications on Moon and Mars. Instead of chlorophyll, which is responsible for light absorption in plants and algae, these devices use semiconductor materials which can be coated directly with simple metallic catalysts supporting the desired chemical reaction. Our analysis shows that these devices would indeed be viable to complement existing life support technologies, such as the oxygen generator assembly employed on the ISS. This is particularly the case when combined with devices which concentrate solar energy in order to power the reactions (essentially large mirrors which focus the incoming sunlight).

There are other approaches too. For example, we can produce oxygen directly from lunar soil (regolith). But this requires high temperatures to work. Artificial photosynthesis devices, on the other hand, could operate at room temperature at pressures found on Mars and the Moon. That means they could be used directly in habitats and using water as the main resource. This is particularly interesting given the stipulated presence of ice water in the lunar Shackleton crater, which is an anticipated landing site in future lunar missions.

On Mars, the atmosphere composes of nearly 96% carbon dioxide - seemingly ideal for an artificial photosynthesis device. But the light intensity on the red planet is weaker than on Earth due to the larger distance from the Sun. So would this pose a problem? We actually calculated the sunlight intensity available on Mars. We showed that we can indeed use these devices there, although solar mirrors become even more important. [...] The returns would be huge. For example, we could actually create artificial atmospheres in space and produce chemicals we require on long-term missions, such as fertilizers, polymers, or pharmaceuticals. Additionally, the insights we gain from designing and fabricating these devices could help us meet the green energy challenge on Earth.

Swiss start-up Sun-Ways has developed a concept to install solar panels between train tracks, using a specially built train to "unroll" the panels during the night when fewer trains are running. Fast Company reports: As wild as it all sound, Sun-Ways actually has two competitors. Greenrail and Bankset Energy, respectively located in Italy and England, are already testing similar concepts. But Sun-Ways stands out in two ways. For one, it uses standard-size panels, whereas the others use smaller panels that are placed on top of crossties. And unlike its competitors, Sun-ways doesn't require manual installation. It has a train for that!

Sun-ways is putting this idea to the test during a $560,000 pilot project in Western Switzerland. The pilot, which is slated for this summer, will trial a version of the mechanism using a regular train that's been retrofitted for the occasion. Running on a 140-foot stretch near the city of Neuchatel, the train will install about 60 solar panels, turning the gap between train tracks into a reflective black ribbon.

For now, 100% of the electricity generated by the solar panels will go straight to the grid to power nearby households. But eventually, the team is planning to use some of that electricity to power the very trains that run above the panels. According to Danichert, 5,000 kilometers of "solar rails" (which is the current length of the entire Swiss railroad network) can generate 1 gigawatt of energy per year, or enough energy to power about 750,000 homes. Considering there are over 1 million kilometers of railway tracks worldwide, the potential could be huge, even if the system can't be installed on every one of those tracks. But most importantly, it wouldn't take up any space from farmland or forests, and it wouldn't ruin any landscapes.

The Mars helicopter 'Ingenuity' recently completed its 47th, 48th, and 49th flight, NASA reports on the blog for its Mars rover 'Perseverance'. That rover is making a "long ascent" up the delta in Mars' Jezero crater, "an area where scientists surmise that, billions of years ago, a river once flowed into a lake.

On its 47th flight, Ingenuity attempted "tactical and scientific scouting" for the rover, but "just narrowly missing the main area of interest." But then... Ingenuity's 48th flight produced a treasure trove of aerial images showing the exact area of interest at a resolution several orders of magnitude better than anything prior. All of these images were downlinked to Earth and provided to rover planners and scientists a full two weeks before the rover would reach this area... [T]he team chose to send the helicopter farther up the delta rather than perform additional scouting flights in the region... The Guidance Navigation and Control team once again managed to push the flight envelope with a 16-meter vertical popup at the end of the flight. At the peak, Ingenuity snapped the highest suborbital picture taken of the Martian surface since landing...

That downlink was the last time the team would hear from the helicopter for an agonizingly long time. Eager to continue up the delta, the team tried and failed to uplink the instructions for Flight 50 several times. Sol after sol, the helicopter remained elusive. Each time, the downlinked telemetry from the Helicopter Base Station (HBS) on the rover would come back showing no radio sign of the helicopter... When the rover emerged from the communications shadow on its way to Foel Drygarn and the helicopter was still nowhere to be found, the situation began to generate some unease... In more than 700 sols operating the helicopter on Mars, not once had we ever experienced a total radio blackout. Even in the worst communications environments, we had always seen some indication of activity...

Finally, on Sol 761, nearly a week after our first missed check-in, our communications team observed a single, lonely radio ACK (radio acknowledgement) at 9:44 LMST (Local Mean Solar Time), exactly the time when we'd expect to see the helicopter wakeup. Another single ACK at the same time on Sol 762 confirmed that the helicopter was indeed alive, which came as a welcome relief for the team. Ultimately, this first-of-its-kind communications blackout was a result of two factors. First, the topology between the rover and the helicopter was very challenging for the radio used by Ingenuity. In addition to the aforementioned communications shadow, a moderate ridge located just to the southeast of the Flight 49 landing site separated the helicopter from the rover's operational area. The impact of this ridge would only abate once the rover had gotten uncomfortably close to the helicopter. Second, the HBS antenna is located on the right side of the rover, low enough to the deck to see significant occlusion effects from various part of the rover...

Relying on the helicopter's onboard preflight checks to ensure vehicle safety and banking on solid communications from the rover's imminent proximity, the team uplinked the flight plan. As commanded, Ingenuity woke up and executed its 50th flight on the red planet, covering over 300 meters and setting a new altitude record of 18 m.

The rover had closed to a mere 80 meters by the time the helicopter lifted off in the Martian afternoon Sun.
And Flight 51 happened 9 days later...

An anonymous reader shared this report from the Washington Post: Nearly any material can be used to turn the energy in air humidity into electricity, scientists found in a discovery that could lead to continuously producing clean energy with little pollution. The research, published in a paper in Advanced Materials, builds on 2020 work that first showed energy could be pulled from the moisture in the air using material harvested from bacteria. The new study shows nearly any material can be used, like wood or silicon, as long as it can be smashed into small particles and remade with microscopic pores...

The air-powered generator, known as an "Air-gen," would offer continuous clean electricity since it uses the energy from humidity, which is always present, rather than depending on the sun or wind... The device, the size of a fingernail and thinner than a single hair, is dotted with tiny holes known as nanopores. The holes have a diameter smaller than 100 nanometers, or less than a thousandth of the width of a strand of human hair. The tiny holes allow the water in the air to pass through in a way that would create a charge imbalance in the upper and lower parts of the device, effectively creating a battery that runs continuously. "We are opening up a wide door for harvesting clean electricity from thin air," Xiaomeng Liu, another author and a UMass engineering graduate student, said in a statement.

While one prototype only produces a small amount of energy — almost enough to power a dot of light on a big screen — because of its size, Yao said Air-gens can be stacked on top of each other, potentially with spaces of air in between. Storing the electricity is a separate issue, he added. Yao estimated that roughly 1 billion Air-gens, stacked to be roughly the size of a refrigerator, could produce a kilowatt and partly power a home in ideal conditions. The team hopes to lower both the number of devices needed and the space they take up by making the tool more efficient...

It could be embedded in wall paint in a home, made at a larger scale in unused space in a city or littered throughout an office's hard-to-get-to spaces. And because it can use nearly any material, it could extract less from the environment than other renewable forms of energy. "The entire earth is covered with a thick layer of humidity," Yao said. "It's an enormous source of clean energy. This is just the beginning in making use of that."
More information from the Boston Globe.

Thanks to long-time Slashdot reader SpzToid for sharing the article.

An anonymous reader quotes a report from the BBC: A US researcher has broken the record for the longest time spent living underwater without depressurization. Joseph Dituri has spent more than 74 days at the bottom of a 30ft-deep lagoon in Key Largo, Florida. And he does not have plans to stop yet. On Sunday, he said he would stay in Jules' Undersea Lodge for at least 100 days.

"The curiosity for discovery has led me here," he said. "My goal from day one has been to inspire generations to come, interview scientists who study life undersea and learn how the human body functions in extreme environments," he added. The previous record for most days spent living underwater at ambient pressure -- 73 -- was established by two professors in 2014 in the same Key Largo lodge. Unlike a submarine, the lodge does not use technology to adjust for the increased underwater pressure.

Prof Dituri -- who also served in the Navy for 28 years -- is teaching his biomedical engineering classes online while he lives in the lagoon, according to the University of South Florida. To keep busy, the professor wakes up at 05:00 each day to exercise. He stays full by reportedly eating protein-heavy meals such as eggs and salmon that he can keep warm with his microwave. And while his underwater stay has proven ground-breaking, he is excited to get back to some above-ground activities. "The thing that I miss the most about being on the surface is literally the sun," he told the Associated Press.

775 million people around the world didn't have electricity last year, according to the International Energy Agency. But the Associated Press points out that's changing in some of the world's most remote places — thanks to off-grid solar systems.

Here's a typical example from the world's fourth most-populous country... Before electricity came to the village a bit less than two years ago, the day ended when the sun went down. Villagers in Laindeha, on the island of Sumba in eastern Indonesia, would set aside the mats they were weaving or coffee they were sorting to sell at the market as the light faded.

A few families who could afford them would start noisy generators that rumbled into the night, emitting plumes of smoke. Some people wired lightbulbs to old car batteries, which would quickly die or burn out appliances, as they had no regulator. Children sometimes studied by makeshift oil lamps, but these occasionally burned down homes when knocked over by the wind. That's changed since grassroots social enterprise projects have brought small, individual solar panel systems to Laindeha and villages like it across the island...

Around the world, hundreds of millions of people live in communities without regular access to power, and off-grid solar systems like these are bringing limited access to electricity to places like these years before power grids reach them... Indonesia has brought electricity to millions of people in recent years, going from 85% to nearly 97% coverage between 2005 and 2020, according to World Bank data. But there are still more than half a million people in Indonesia living in places the grid doesn't reach.

While barriers still remain, experts say off-grid solar programs on the island could be replicated across the vast archipelago nation, bringing renewable energy to remote communities.

"Astronomers have spotted the largest cosmic explosion ever witnessed, and it's 10 times brighter than any known exploding star, or supernova," reports CNN: The brightness of the explosion, called AT2021lwx, has lasted for three years, while most supernovas are only bright for a few months. The event, still being detected by telescopes, occurred nearly 8 billion light-years away from Earth when the universe was about 6 billion years old. The luminosity of the explosion is also three times brighter than tidal disruption events, when stars fall into supermassive black holes.

But what triggered such a long-lived, massive cosmic explosion? Astronomers said they think a supermassive black hole disrupted a vast gas or dust cloud, potentially thousands of times larger than our sun. It's possible that the cloud was drawn off the course of its orbit and went flying into the black hole, the researchers said. As the black hole swallowed pieces of the hydrogen cloud, shock waves likely reverberated through the cloud's remnants and into the swirling mass of material that orbits around the black hole...

The research team determined that the incredibly luminous event was nearly 100 times brighter than all the 100 billion stars in the Milky Way galaxy combined.
The New York Times calls its "one of the most violent and energetic acts of cosmic cannibalism ever witnessed, perhaps the biggest explosion seen yet in the history of the universe... [A] black hole perhaps a billion times as massive as the sun seems to be gorging on a humongous cloud of gas." "Most supernovae and tidal disruption events only last for a couple of months before fading away," said Philip Wiseman, an astrophysicist at the University of Southampton and the lead author of the new paper [published Thursday in the Monthly Notices of the Royal Astronomical Society]. "For something to be bright for two-plus years was immediately very unusual...."

He added that, with a total radiated energy equal to 100 supernovas, "it is one of the most luminous transients ever discovered." Jolt for jolt, that would put it in the company of colliding black holes. "Black holes colliding release energy in gravitational waves at an extreme luminosity — 10 billion times more 'powerful' than this explosion," Dr. Wiseman wrote. "But that power only lasts for 20 milliseconds," adding that this explosion has lasted years.

"Astronomers have discovered 62 new moons orbiting the ringed planet Saturn," reports Space.com.

So while Jupiter remains the largest planet orbiting our sun — and shaped our solar system with its gravitational bulk — nonetheless the New York Times reports that "the fight over which planet has the most moons in its orbit has swung decisively in Saturn's favor." This month, the International Astronomical Union is set to recognize 62 additional moons of Saturn based on a batch of objects discovered by astronomers. The small objects will give Saturn 145 moons — eclipsing Jupiter's total of 95. "They both have many, many moons," said Scott Sheppard, an astronomer from the Carnegie Institution for Science in Washington, D.C. But Saturn "appears to have significantly more," he said, for reasons that are not entirely understood.

The newly discovered moons of Saturn are nothing like the bright object in Earth's night sky. They are irregularly shaped, like potatoes, and no more than one or two miles across. They orbit far from the planet too, between six million and 18 million miles, compared with larger moons, like Titan, that mostly orbit within a million miles of Saturn. Yet these small irregular moons are fascinating in their own right. They are mostly clumped together in groups, and they may be remnants of larger moons [150 miles across] that shattered while orbiting Saturn. [The article suggests later they may have been destroyed by collisions with other moons, or by impacts from asteroids or comets.]

"These moons are pretty key to understanding some of the big questions about the solar system," said Bonnie Buratti of NASA's Jet Propulsion Laboratory in California and the deputy project scientist on the upcoming Europa Clipper mission to Jupiter. "They have the fingerprints of events that took place in the early solar system."

The growing number of moons also highlights potential debates over what constitutes a moon. "The simple definition of a moon is that it's an object that orbits a planet," Dr. Sheppard said. An object's size, for the moment, doesn't matter.
The leader of one moon-discovering group told the Times there's "potentially thousands" of moons around Saturn and Jupiter.

And at least a few of the moons are circling Saturn in the opposite direction...

Many experts believe fusion power remains decades away. Microsoft thinks it could be just around the corner. From a report: In a deal that is believed to be the first commercial agreement for fusion power, the tech giant has agreed to purchase electricity from startup Helion Energy within about five years. Helion, which is backed by OpenAI founder Sam Altman, committed to start producing electricity through fusion by 2028 and target power generation for Microsoft of at least 50 megawatts after a year or pay financial penalties. The commitment is a bold one given that neither Helion nor anyone else in the world has yet produced electricity from fusion. "We wouldn't enter into this agreement if we were not optimistic that engineering advances are gaining momentum," said Microsoft President Brad Smith.

Fusion powers the sun and stars, and has the potential to provide nearly limitless amounts of carbon-free power if someone can harness it on earth. The International Atomic Energy Agency expects electricity from fusion to be produced in the second half of the century. Helion is building a prototype that it says will demonstrate the ability to produce electricity through fusion next year. "The goal is not to make the world's coolest technology demo," Mr. Altman said in an interview. "The goal is to power the world and to do it extremely cheaply." Mr. Altman, the chief executive officer of OpenAI -- the artificial-intelligence startup behind the viral chatbot ChatGPT -- said having a first customer is critical for keeping Helion grounded in the realities of business, including working with clients, utilities and electric-grid operators.

Louise Lerner writes via Phys.Org: Inside a lab, scientists marvel at a strange state that forms when they cool down atoms to nearly absolute zero. Outside their window, trees gather sunlight and turn them into new leaves. The two seem unrelated -- but a new study from the University of Chicago suggests that these processes aren't so different as they might appear on the surface. The study, published in PRX Energy on April 28, found links at the atomic level between photosynthesis and exciton condensates -- a strange state of physics that allows energy to flow frictionlessly through a material. The finding is scientifically intriguing and may suggest new ways to think about designing electronics, the authors said.

When a photon from the sun strikes a leaf, it sparks a change in a specially designed molecule. The energy knocks loose an electron. The electron, and the "hole" where it once was, can now travel around the leaf, carrying the energy of the sun to another area where it triggers a chemical reaction to make sugars for the plant. Together, that traveling electron-and-hole-pair is referred to as an "exciton." When the team took a birds-eye view and modeled how multiple excitons move around, they noticed something odd. They saw patterns in the paths of the excitons that looked remarkably familiar. In fact, it looked very much like the behavior in a material that is known as a Bose-Einstein condensate, sometimes known as "the fifth state of matter." In this material, excitons can link up into the same quantum state -- kind of like a set of bells all ringing perfectly in tune. This allows energy to move around the material with zero friction. (These sorts of strange behaviors intrigue scientists because they can be the seeds for remarkable technology -- for example, a similar state called superconductivity is the basis for MRI machines).

According to the models [...], the excitons in a leaf can sometimes link up in ways similar to exciton condensate behavior. This was a huge surprise. Exciton condensates have only been seen when the material is cooled down significantly below room temperature. It'd be kind of like seeing ice cubes forming in a cup of hot coffee. "Photosynthetic light harvesting is taking place in a system that is at room temperature and what's more, its structure is disordered -- very unlike the pristine crystallized materials and cold temperatures that you use to make exciton condensates," explained [study co-author Anna Schouten]. This effect isn't total -- it's more akin to "islands" of condensates forming, the scientists said. "But that's still enough to enhance energy transfer in the system," said Sager-Smith. In fact, their models suggest it can as much as double the efficiency. The findings open up some new possibilities for generating synthetic materials for future technology, said study co-author Prof. David Mazziotti. "A perfect ideal exciton condensate is sensitive and requires a lot of special conditions, but for realistic applications, it's exciting to see something that boosts efficiency but can happen in ambient conditions."

Long-time Slashdot reader schwit1 shared this report from Futurism: We'd need an astronomical amount of resources to construct a Dyson sphere, a giant theoretical shell that would harvest all of a given star's energy, around the Sun. In fact, as science journalist Jaime Green explores in her new book "The Possibility of Life," we'd have to go as far as to demolish a Jupiter-sized planet to build such a megastructure, a concept first devised by physicist Freeman Dyson in 1960...

Not everybody agrees that constructing a Dyson sphere would end up being such a huge undertaking. In an interview with Green, astrophysicist Jason Wright compared such an effort to [the city of] Manhattan, a human and interconnected "megastructure," which was constructed over a long period of time, bit by bit... "It's just every generation made it a little bigger...."

"If the energy is out there to take and it's just gonna fly away to space anyway, then why wouldn't someone take it?" Wright told Green.

For the first time, astronomers have observed a star swallowing a planet. The findings have been published in the journal Nature. MIT News reports: The planetary demise appears to have taken place in our own galaxy, some 12,000 light-years away, near the eagle-like constellation Aquila. There, astronomers spotted an outburst from a star that became more than 100 times brighter over just 10 days, before quickly fading away. Curiously, this white-hot flash was followed by a colder, longer-lasting signal. This combination, the scientists deduced, could only have been produced by one event: a star engulfing a nearby planet.

What of the planet that perished? The scientists estimate that it was likely a hot, Jupiter-sized world that spiraled close, then was pulled into the dying star's atmosphere, and, finally, into its core. A similar fate will befall the Earth, though not for another 5 billion years, when the sun is expected to burn out, and burn up the solar system's inner planets. "For decades, we've been able to see the before and after," says lead author Kishalay De, a postdoc in MIT's Kavli Institute for Astrophysics and Space Research. "Before, when the planets are still orbiting very close to their star, and after, when a planet has already been engulfed, and the star is giant. What we were missing was catching the star in the act, where you have a planet undergoing this fate in real-time. That's what makes this discovery really exciting."

The James Webb Space Telescope (JWST) has detected water vapor around a distant rocky planet located 26 light-years away. "The water vapor could indicate the presence of an atmosphere around the extrasolar planet, or exoplanet, a discovery that could be important for our search for habitable worlds outside the solar system," reports Space.com. "However, the scientists behind the discovery caution that this water vapor could be coming from the world's host star rather than the planet itself." From the report: The exoplanet, designated GJ 486 b, orbits a red dwarf star located 26 light-years away in the Virgo constellation. Although it has three times the mass of Earth, it is less than a third the size of our planet. GJ 486 b takes less than 1.5 Earth days to orbit its star and is probably tidally locked to the red dwarf, meaning it perpetually shows the same face to its star.

Red dwarfs like the parent star of GJ 486 b are the most common form of stars in the cosmos, meaning that statistically speaking, rocky exoplanets are most likely to be found orbiting such a stellar object. Red dwarf stars are also cooler than other types of stars, meaning that a planet must orbit them tightly to remain warm enough to host liquid water, a vital element needed for life. But, red dwarfs also emit violent and powerful ultraviolet and X-ray radiation when they are young that would blast away the atmospheres of planets that are too close, potentially making those exoplanets very inhospitable to life.

That means astronomers are currently keen to discover if a rocky planet in such a harsh environment could manage to both form an atmosphere and then hang on to it long enough for life to take hold, a process that took around a billion years on Earth. [...] Even though GJ 486 b's host star is cooler than the sun, water vapor could still concentrate in starspots. If that is the case, this could create a signal that mimics a planetary atmosphere. If there is an atmosphere around GJ 486 b, then radiation from its red dwarf parent star will constantly erode it, meaning it has to be replenished by steam from the exoplanet's interior ejected by volcanic activity. The research appears in a paper on arXiv while it awaits publication in the journal Astrophysical Journal Letters. You can read more about it via NASA.