As temperatures rise around the world, air conditioning is saving lives. But a growing reliance on it is also placing unprecedented pressure on electricity grids, increasing greenhouse gas emissions and making cities even hotter.

A global review led by UNSW Sydney's Professor Mat Santamouris AM—an expert in innovative heat mitigation technologies and strategies for cities—argues that keeping buildings cool without relying solely on air conditioning will be critical for adapting to climate change.

Published in Nature Reviews Clean Technology, the review examines the latest advances in passive cooling technologies, from emerging materials for radiative, evaporative and combined radiative/evaporative cooling to sophisticated solar control systems and personalized intelligent ventilation technologies that can help buildings shed heat without consuming electricity.

Professor Santamouris says passive cooling should no longer be viewed as a niche architectural feature, but as essential infrastructure for a warming world.

"Air conditioning saves lives and will remain essential during extreme heat," he says. "But we cannot air-condition our way out of climate change. If every building depends entirely on mechanical cooling, we create enormous pressure on electricity systems while adding even more heat to our cities."

Demand for cooling is soaring
The review highlights the rapid growth in cooling demand worldwide. Global electricity consumption for cooling has reached almost 10 percent of total electricity use, with around 10 new air conditioners sold every second. By 2050, the number of residential air-conditioning units is projected to increase to almost 5.6 billion worldwide.

At the same time, billions of people living in hot climates still lack access to affordable cooling.

When Charlotte Mason ponders cosmic mysteries, she likes to doodle. “I am quite a visual person,” she said. “I usually draw a lot of pictures trying to understand what’s going on.”

Mason, an astrophysicist at the Cosmic Dawn Center in Copenhagen, has lately been filling pages with sketches of “little red dots,” perplexing objects discovered by the hundreds in images from the James Webb Space Telescope (JWST). Little red dots were never seen before the telescope came online in 2022. But we now know that they started to appear in significant numbers roughly 650 million years after the Big Bang.

These dots are just one of the thrilling mysteries that have emerged from JWST’s observations of the early universe. Others include black holes that seem impossibly large for their age, as well as ancient galaxies that defy what we thought we knew about the first billion years after the Big Bang. At first, scientists were astounded: The universe revealed by JWST simply didn’t square with our understanding of astrophysics. Now, a wave of new theories offers tantalizing solutions — but which ones portray reality is an open question.

Recent ideas suggest that little red dots could be black holes cocooned in thick gas, possibly representing a completely new type of object called a black hole star, in which the tight shroud of gas emits light like a stellar atmosphere.

“This would be my black hole,” Mason said, drawing a small circle and filling it in. “I might put a disk on it, because we think that’s where some of the emission comes from.” She slashed a line through the circle’s center. “Then the kind of naïve picture is just this dense gas cloud around the black hole.” She drew a larger circle surrounding the object.

But Mason thinks there may be more to these cosmic enigmas. She and colleagues recently analyzed the spectrum of light emitted by one little red dot. If the dense-cloud picture is correct, then some of the light should have been altered from passing through the gas — but that’s not what they saw.

“Now what do I do? Start again. But now if I make my gas clumpy,” Mason said, drawing a new diagram with holes in the clouds surrounding the black hole, “I should be able to get [a signal] that looks closer.”

All around the world, researchers like Mason are eagerly piecing together JWST’s glimpses of the ancient cosmos to create a clearer picture of our universe’s beginnings. And like the photons that travel billions of light-years to reach us, new fragments are constantly falling into place.

🆕 The NIR Cam on Webb has captured the protostars of the FS Tau system. These are just 1 to 3 million years old – young by cosmic standards! 👶⭐ ‍

A pair known as FS Tau A is responsible for the large diffraction pattern left of centre, while the red and orange outflows seen amidst the dust are thought to be caused by FS Tau B, the orange protostar just right of centre. 

Read more: esawebb.org/images/FS-Tau/

For decades, age-related memory loss has largely been viewed as a problem that begins in the brain. But growing evidence suggests that some of the processes shaping cognition may start much farther south — in the gut, home to trillions of microbes that help regulate everything from digestion to immunity.

A new mouse study from researchers at Stanford Medicine and the Arc Institute in Palo Alto, California, points to a surprising gut-brain connection behind cognitive aging.

The team found that age-related changes in gut bacteria can interfere with signals traveling along the vagus nerve, a major communication highway linking the gastrointestinal tract and the brain. Their findings suggest that memory decline may be influenced by changes outside the brain itself, opening new possibilities for preserving cognitive function later in life.

“Although memory loss is common with age, it affects people differently and at different ages,” said Christoph Thaiss, PhD, assistant professor of pathology. “We wanted to understand why some very old people remain cognitively sharp while other people see significant declines beginning in their 50s or 60s. What we learned is that the timeline of memory decline is not hardwired; it’s actively modulated in the body, and the gastrointestinal tract is a critical regulator of this process.”

The study found that the gut microbiome, the natural community of bacteria living in the intestine, changes as mice grow older. Some bacterial species become more common while others decline. Immune cells in the gastrointestinal tract detect these changes and trigger inflammation that weakens signaling through the vagus nerve to the hippocampus, the brain region involved in memory formation and spatial navigation. When researchers stimulated vagus nerve activity in older mice, the animals regained the ability to remember unfamiliar objects and escape mazes as well as younger mice.

After more than two decades, the orbit of NASA’s Neil Gehrels Swift Observatory has entered a phase of rapid decay. While NASA could allow the observatory to re-enter Earth’s atmosphere, as many missions do at the ends of their lifetimes, this situation has presented an opportunity to advance American spacecraft servicing technology while also extending the life of a productive science mission. To accomplish this, NASA awarded the U.S. company Katalyst Space a contract in September 2025 to attempt to raise Swift’s orbit.

A mission to raise the altitude of NASA’s Neil Gehrels Swift Observatory is underway after launching at 8:36 p.m. Marshall Islands Time (4:36 a.m. EDT), Friday, July 3, from Kwajalein Atoll in the South Pacific Ocean. Source

The 1.7 million satellites that companies are aiming to launch into Earth's orbit in the coming years will have "devastating consequences for astronomy," new research warned Wednesday.

The plans to swarm Earth with huge, extremely bright satellites represent an "existential threat" to telescopes viewing the universe, according to the European Southern Observatory (ESO), which conducted the research.

To retain humanity's ability to properly explore the night sky, the team of researchers called for a maximum limit of 100,000 satellites orbiting Earth.

The study is the first to calculate how much the constellations of big and particularly bright satellites being planned would affect astronomical observations by making the night sky brighter.

The number of satellites orbiting Earth has now reached 14,000 after surging in recent years, many of them part of trillionaire Elon Musk's Starlink internet constellation.

But that is just the start.

Musk's SpaceX has announced plans to launch more than 1 million satellites by 2028 to serve as data centers powering the artificial intelligence boom.

Other projects such as the "Cinnamon" plans of startup E-Space and Chinese constellations CTC-1 and CTC-2 would add hundreds of thousands more satellites spinning around our planet.

And U.S. startup Reflect Orbital hopes to launch 50,000 huge satellites that use giant mirrors to point sunlight back down to Earth, with the aim of providing light during the night.

In total, more than 1.7 million satellites could soon be lighting up the night sky, obscuring or blotting out the view of ground-based telescopes.

RMIT University researchers have tested a more effective way to capture microplastics from wastewater, using a combination of microbubbles and nanobubbles to achieve removal rates of more than 90%.

The dual-bubble approach can be adopted by wastewater treatment plants without major infrastructure changes by optimizing existing operating conditions, including air pressure, saturation time and bubble size.

The paper "Micro-Nanobubble Integrated Dissolved Air Flotation: A High-Efficiency Strategy for Microplastic Mitigation in Wastewater," is published in ACS ES&T Water. Lead author, Associate Professor Biplob Pramanik, said the approach suggests a practical way to reduce microplastic pollution—a growing global issue.

"Wastewater treatment plants are a major pathway for microplastics because they slip through filtration processes, posing risks to ecosystems and human health," Pramanik said. He is also the director of RMIT's Water Effective Technology and Tools Research Center.

"Our approach is simple to implement and significantly increases the removal of microplastics during the primary stage of treatment."

The study investigated an enhanced version of dissolved air flotation, a widely used water treatment process that removes contaminants by attaching them to air bubbles and lifting them to the surface.

A major new resource that provides one of the most comprehensive pictures yet of what people are eating around the world has been introduced in a new study by a UCL and University of Oxford researcher.

From obesity and heart disease to climate change and food affordability, many of today's biggest challenges are shaped by what we eat. But there is a surprisingly basic problem facing researchers and policymakers: We often don't know with enough accuracy what people are actually consuming.

The new study, published in Nature Food and authored by Professor Marco Springmann (UCL Institute for Global Health as well as the Environmental Change Institute at the University of Oxford), introduces the Global Dietary Database for Impact Assessments (GDD-IA), which is freely available through an interactive online explorer, allowing users to investigate dietary patterns across countries and over time.

The GDD-IA combines information on food production, food waste, dietary surveys and human energy requirements to estimate what people eat from 1990 to 2020. It includes detail by age, sex and whether people live in urban or rural areas.

The resource has been designed to support research into some of the world's most pressing questions: How do diets affect human health? What impact do they have on climate change and the environment? How affordable are healthy and sustainable diets for different populations?

Professor Springmann said, "Many of the decisions we make about food policy rely on assumptions about what people eat. But existing global datasets often have important limitations. Our aim was to create a more complete and biologically realistic picture of food consumption that can support better assessments of health, environmental and economic impacts."

With new technologies come new opportunities. And that is especially true in astronomy - with every new advanced telescope we have the potential to see (or in some cases, listen) further and more clearly than we ever have before. That is certainly the case for the new Square Kilometre Array (SKA), which is currently undergoing a multi-year roll out phase. Despite that drawn out process, astronomers are already excited about its potential, and a new book chapter from Dr. Chenoa Tremblay and her co-authors details how this new technology could be used to answer one of the most fundamental questions - are we alone?

The Search for Extraterrestrial Intelligence (SETI) has always been constrained by its resources. This constraint required researchers to focus mainly on tight signals such as the narrow band between hydrogen and hydroxyl. Early SETI pioneers justified this by claiming that such a narrow beacon would be a clear signal of intent. However, it also meant that they were only able to find signals that were intentionally sent in our direction. And the likelihood of that happening is miniscule compared to the chances there were advanced civilizations that did not feel the need to reach out to us.

Enter the SKA. Its design, which spans two continents (Australia and Africa) allows it to scan an absolutely gigantic amount of the sky. Critically, this will enable it to pick up “leakage” radiation. The authors calculated that one hour of observational time on the SKA itself would be enough to pick up signals from the equivalent of a modern-day mobile phone network similar to what we currently have on Earth from an exoplanet four light years away.

That is a massive step change in our ability to detect unintentional emissions. But actually getting the time to do so is a huge part of the challenge. Telescope time on world-leading instruments like the SKA is notoriously difficult to get. So SETI researchers came up with a productive solution - they will simply piggy-back off of the data the SKA is already collecting for other surveys, such as watching supernovae or bright radio galaxies.

Duplicating radio data is easy enough - so the SETI researchers plan to use their own data pipeline, without disrupting the instrument’s primary science mission. They can also cross-reference their data with other large catalogues, such as Gaia, to evaluate signals from potentially promising sources.

For decades, archaeologists have debated whether these early Paleoindians were megafauna specialists, focused on hunting massive animals, or dietary generalists who ate a broad mix of small game, fish, plants, and shellfish depending on their local environment.

Over the past ten years, many scientists had drifted toward the generalist view.

However, a new study led by the University of Alaska Fairbanks pushes back hard against that trend.

“One of two competing ideas is dietary generalization: exploiting a wide variety of resources that would differ based on region,” explained University of Alaska Fairbanks Professor Ben Potter.

“The other is megafaunal specialization: focusing on just a few large-bodied prey.”

In the study, the researchers examined 50 archaeological sites across three regions: Eastern Beringia (ancient Alaska, roughly 14,000 to 13,300 years ago), the Clovis culture of North America (about 13,400 to 12,800 years ago), and the Fishtail Projectile Point culture of South America (roughly 12,900 to 11,600 years ago).

Together, these represent the earliest continent-spanning human societies in the western hemisphere.

Analyzing measures such as species abundance, minimum number of individuals, and edible biomass, the scientists found that megafauna accounted for 83% to 88% of the meat and fat these groups likely consumed.

Woolly mammoths dominated diets in Beringia, Columbian mammoths in North America, and giant ground sloths and gomphotheres in South America.

Smaller animals were present at many sites but contributed almost nothing nutritionally.

“The test of dietary specialization isn’t just how many of a given animal you find at an ancient campsite,” Professor Potter said.

“It’s what the record looks like relative to natural abundance. If early people were dietary generalists, you’d expect to find the most common animals would be more common in peoples’ campsites.”

“Animals like mammoths and ground sloths, which were actually quite rare in the landscape, completely dominate the archaeological record.”

“Rabbits and mice, which would have been everywhere, barely register.”

The authors also point to independent evidence: a chemical analysis of a Clovis-era child called Anzick-1 found that roughly 96% of his mother’s protein came from megafauna, mostly mammoth.

Beyond diet, these early groups shared other hallmarks of specialized hunters: highly efficient, well-maintained toolkits carried over long distances; extremely mobile, far-ranging lifestyles instead of settled home territories; and little to no evidence of plant-processing tools like grinding stones.

Picture a bright red apple. Most people can do this easily. They imagine the apple's shape, color and shine. But for others, the image is vague and blurry or they "see" nothing at all. This is known as aphantasia—a "blind mind's eye."

What we are dealing with here are individual differences in mental imagery. Research suggests mental imagery exists on a continuum, and this can affect how we learn.

Every day in class, students are encouraged to "visualize," "imagine," or "picture" concepts. For example, in geography, students need to imagine landscapes or weather systems. In science, they are asked to mentally represent atoms, electric currents or molecular processes.

But what happens when a student cannot easily do this?

Our study examines whether differences in mental imagery affect students' learning—and how teachers and parents can reduce any disadvantage this may cause.

Why mental imagery matters
When students can create a clear mental picture, that image may help them understand, organize and remember new information. This is all helpful for their learning.

But research suggests students with weak mental imagery may need to work harder and may not experience these benefits to the same extent.

This can sometimes show up as students taking longer to understand new ideas or needing more support to remember what they have learned.

Instead of relying on mental images, they may have to process information in other ways—through words, logic, memorization or repeated rehearsal. This can increase what psychologists call cognitive load, or the amount of mental effort required to learn something new.

How can you tell if your child struggles here?
Children with weak mental imagery may be less likely to report "seeing pictures in their mind" when reading stories, recalling past events or imagining future situations.

They may rely more on verbal descriptions, facts or step-by-step reasoning than on visualization strategies.

This is not uncommon. In our study, we estimated about 10% of students had "no" or "dim" mental imagery. About 30% reported their mental imagery was only "somewhat" vivid.

Following its longest hibernation period ever of nearly a year, NASA's New Horizons spacecraft has emerged in good health and is ready to begin transmitting science data gathered in the distant Kuiper Belt far beyond Pluto.

On June 23, flight controllers at the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, confirmed New Horizons, acting on stored commands uplinked to its main computer last July, had safely awakened from a 321‑day hibernation period that began Aug. 7. With the spacecraft now approximately 5.9 billion miles (9.5 billion kilometers) from Earth, the radio signals carrying that confirmation took about 8 hours and 52 minutes to reach the APL Mission Operations Center via NASA's Deep Space Network station near Madrid, Spain.

The mission team typically places New Horizons in resource‑saving hibernation mode during long cruise periods. While the spacecraft is hibernating, operators do not send commands or retrieve data, but the spacecraft continues gathering and storing data around the clock from its heliospheric plasma sensors, Solar Wind at Pluto and the Pluto Energetic Particle Spectrometer Science Investigation, as well as its space dust detector, the Venetia Burney Student Dust Counter.

Alice Bowman, the New Horizons mission operations manager at APL, said the spacecraft reported back to Earth, via the Deep Space Network, with a weekly status beacon.

"Every status report through this hibernation period was 'green,' meaning all was well aboard New Horizons each and every week," she said.

As New Horizons resumes active operations, Bowman noted, the team will begin downlinking spacecraft health and safety data, followed by data from the three scientific instruments. In about three weeks, the spacecraft's onboard Alice ultraviolet spectrograph will look at the hydrogen gas distribution in the outer heliosphere, while the Solar Wind at Pluto, the Pluto Energetic Particle Spectrometer Science Investigation, and the Venetia Burney Student Dust Counter instruments continue their measurements, and the ground team conducts a series of spacecraft and instrument checkouts.

The team also is completing upgrades to the ground‑system software that will make it easier to maintain operations of the spacecraft. Tests are already underway and are expected to continue through the year.

New Horizons is operating on updated autonomy logic designed for operations farther from the sun and to accommodate the expected reduction in power and the naturally occurring increase in radio‑signal travel time.

The NASA spacecraft's exploration of this distant region of the solar system marks the latest step in a journey that began in January 2006 with the fastest launch on record; a flyby of Jupiter in February 2007 that included stunning views of the gas giant and its moons; the first exploration through the Pluto system in July 2015; the first exploration of a Kuiper Belt object, Arrokoth, in January 2019, and unique studies of the sun's outer heliosphere and dozens of additional Kuiper Belt objects since then.

In 1993, a team led by the planetary scientist Carl Sagan tentatively concluded that there is life on Earth. Not much of a deduction, you might think — except that the researchers confined their evidence to observations made by the Galileo spacecraft(opens a new tab), which had flown past our planet three years earlier on a looping journey to Jupiter. So great is the transformative power of life that its presence can be detected just from the light and radio waves our planet emits or reflects into space. Today we scan the cosmos for some of these telltale signatures light-years away.

Life leaves a mark, yet even now there’s no scientific consensus about what makes living things so different from inorganic substances like the rocks, gases, and oceans that are the sole components of dead worlds. Many scientists cite properties such as replication or metabolism. Others speak in more abstract terms about the way life is out of thermodynamic equilibrium with its surroundings. But some give another kind of answer. Living organisms are different because they do stuff for reasons.

It’s not enough to say that life is a nonequilibrium organized state through which there’s a constant flux of matter and energy. That description applies to hurricanes, too. But hurricanes just are. Only living entities have goals: to find food, to reproduce, to survive, sometimes simply to experience good things. (Dog owners will recognize that this is not just a human attribute.)

One way to express this idea is to say that living organisms have “agency.” It’s a hotly contested term. Some biologists reject it outright, at least for any organisms except humans, because we decide on our actions with conscious deliberation. (Whether we’re truly the only species to do so is another issue.) Others think that agency is a fundamental attribute of all life. Since there’s no agreed-upon definition of the term, to some extent it can mean whatever you want it to mean. But the debate about biological agency touches on fundamental issues in our understanding of what it means to be alive, because agency evokes a notion that biologists and philosophers have always wrestled with: teleology, the apparent purposiveness of life. If we admit agency into biology, do we open the floodgates to ideas about design, vitalism, or cosmic meaning? Or is it just a recognition of what makes life such a special state of matter?

To me, the notion of agency indeed speaks to our intuitive sense of what makes living things so special: not mere machines pushed around by environment and circumstance. I suspect that aversion to agency betrays a queasiness about confronting life as something more than some kind of genetic program. But there’s danger in the idea, too: It could so easily derail the work of studying the mechanistic explanations of how life works. I’m not looking to either bury or praise agency, but to explore whether it can be a scientifically productive idea.

Popular science fiction is no stranger to escape-pod scenarios, typically featuring characters who narrowly avoid their demise by jettisoning from a spaceship—think R2-D2 and C-3PO shooting away from a rebel spaceship in the opening of Star Wars: A New Hope. Biologists at the University of California San Diego have found that communities of bacteria feature a similar ejection capability.

Groups of bacteria known as biofilms thrive on surfaces all around us. These microscopic clusters are abundant in aquatic environments, from the slick surface of lake rocks to the slimy buildup in plumbing pipes. Biofilms also inhabit select parts of our bodies, including our skin and the surfaces of our teeth.

UC San Diego scientists from Professor Gürol Süel's laboratory in the School of Biological Sciences documented the biofilm ejection phenomenon for the first time while studying a bacterium known as hay bacillus (Bacillus subtilis).

Previous views held that biofilms facing death simply dissolved and faded away. Adding to the researchers' surprise, they reviewed similar ejection capabilities across the animal kingdom and found that the only other organisms that feature similar mechanisms are jellyfish.

A hidden rupture mechanism
"We found that at the end of their life cycles, these bacterial biofilms forcefully ejected specific cells from the community," said Süel, a professor in the Department of Molecular Biology, of the study, published in Nature Microbiology. "The biofilm senses that it is in trouble so it shoots cells out of the community like an escape pod."

Survival through expelled cells
The researchers say the ejection capability allows a biofilm facing nutrient starvation or other threats to ensure that the community can survive by releasing mobile cells that have the potential to swim away and colonize a new location.

"The biofilm knows it is going to die, so it ejects some of its cells so they can survive and live to fight another day," said Süel.

Rare images taken by a Japanese space probe during a flyby of a near-Earth asteroid have revealed that the space rock resembled a snowman, scientists said Monday.

The fridge-sized Hayabusa2 skimmed asteroid Torifune on Sunday in a mission that demonstrated the ability to deflect a potentially dangerous space rock away from Earth.

A new image released by the Japan Aerospace Exploration Agency (JAXA) on Monday could aid such efforts, as researchers say near-Earth asteroids vary in their size, shape and surface characteristics.

"The moment I actually saw this image and the scientific data—it really gave me goosebumps," JAXA scientist Yuya Mimasu told reporters, adding the asteroid "personally looked like a snowman."

The black-and-white image, captured by a telescopic camera, showed what appeared to be two round objects joined together.

"You can actually see the rocks... I really hadn't expected to be able to take a photo like this, so I'm absolutely over the moon," he said.

The mission follows NASA's successful 2022 test that changed the orbit of the asteroid Dimorphos by deliberately smashing it with a spacecraft.

Torifune was known to have an elongated shape, but its details were unknown.

After the Torifune mission, the space probe is expected to attempt in 2031 a "rendezvous"—a maneuver in which it flies alongside or touches down on a space rock to gather detailed data—with an asteroid called 1998KY26.

Oceanographers often point out that the surfaces of the Moon and Mars are mapped more precisely than much of the deep seafloor on Earth. That gap is especially clear in the Bismarck Sea, a deep basin north of Papua New Guinea. Its seafloor is geologically complex, with faults, volcanic structures, rifts, scarps, active subduction zones, and spreading zones lying at depths that are difficult to map in fine detail with sonar.

On May 8, 2026, satellites picked up signs of an unexpected underwater volcanic eruption in the Central Bismarck Sea. For volcanologists, the event highlighted a major problem: there were no detailed maps of the region, and the deep water setting of the eruption remains poorly understood.

The eruption is believed to be taking place along Titan Ridge, about 16 kilometers (10 miles) southeast of a submarine eruption recorded in 1972. Still, scientists do not yet agree on exactly which volcanic feature is active, how deep the vent was before the eruption, or when it last erupted.

“The good news is that there are huge opportunities to explore and learn using both government and commercial satellite platforms already in orbit,” said Jim Garvin, the chief scientist at NASA’s Goddard Space Flight Center.

Heat can be dangerous, but health experts say there are ways to manage the threat.

Scorching temperatures, especially combined with high humidity, pose risks particularly for children, older people and those with certain health conditions. Anyone can suffer from heat-related illness.

Climate change is also exacerbating heat waves and heat stress.

So here are some tips to stay safe:

When heat becomes dangerous
Dangers posed by hot weather depend on more than the temperature. The most detailed measurement is called the wet bulb globe temperature (WBGT), which includes temperature, humidity, cloud cover and wind. The heat index, which measures temperature and humidity, is less descriptive but easier to find on weather apps. Both explain why a shaded soccer field on a 90 degree F day (32 degree C) in arid Phoenix may be less risky than an exposed park on an 80 degree F (27 degree C) day in soupy Little Rock.

Just based on heat index, NOAA has a chart that calculates how dangerous prolonged exposure can be. For example, a day in which temperatures reach 96 degree F (36 degrees C) and 45% humidity would fall into the "danger" category for prolonged exposure or strenuous activity.

The WBGT threshold isn't exact, but recent research suggests that even some young, healthy people can't endure hours of exposure to high heat and humidity.

How to cool down
Overnight temperatures can be a particularly dangerous part of a heat wave, said Ashley Ward, director of the Heat Policy Innovation Hub at Duke University.

"Your body needs a reprieve," she said. "You don't get that overnight, we start the next day at a deficit." Heat can worsen labor productivity and lead to more visits to the emergency room.

"When we have overnight temperatures that don't drop below 75 degrees" F (24 degrees C), she said, "you start to see some pretty extraordinary outcomes with respect to heat illness and heat stroke, and even mortality."

Ward said air conditioning can help, but she acknowledged that not everyone has access...

A breakthrough in photonic chips could make large, costly, ultrafast lasers dramatically smaller, leading to portable and affordable imaging, diagnostic and information-processing devices, researchers say.

By using a decades-old overlooked laser architecture, scientists managed to fit an ultrafast laser onto a tiny photonic chip — a chip that uses light, rather than electricity, for computing operations.

In a new study published June 3 in the journal Nature, the team demonstrated that a tiny laser on the photonic chip could deliver 1.05 nanojoules of energy in 147-femtosecond (147 quadrillionths of a second) bursts — thereby competing with the output of laboratory-class ultrafast lasers.

Ultrafast lasers are used in a variety of applications, from precision manufacturing and eye surgery to biological imaging and atomic clocks, but the systems needed to power them tend to take up whole tabletops in labs or factories. Yet the powerful output of these laser pulses made them difficult to miniaturise onto photonic chips.

"For more than twenty years, a high-pulse-energy femtosecond laser on chip was widely regarded as a holy grail of integrated photonics," Tobias Kippenberg, a photonics professor at the Swiss Federal Institute of Technology(EPFL), said in a statement.

Because of our Solar System's location in the Milky Way's galactic disk, astronomers have a harder time determining the true extent of the Milky Way than they do galaxies millions or even billions of light-years away. And whereas distant galaxies can be well-constrained using optical telescopes, astronomers must rely on instruments that capture light at other wavelengths (radio, infrared, ultraviolet, and X-ray) to better understand the Milky Way's properties.

This includes the Milky Way's outer arms, whose true distances have remained somewhat unclear until recently. Using NASA's Chandra X-ray Observatory and ESA's XMM-Newton satellite, a team of astronomers recently made precise distance measurements to dust clouds in the Milky Way’s spiral arms. Their findings suggest that they may be wider than previously thought, causing astronomers to rethink prevailing theories about our home galaxy's structure.

The results are described in a new paper published in the journal Astronomy & Astrophysics. The team's distance measurements relied on a technique that utilizes light echoes, where they observed rings created by gamma-ray bursts (GRBs) bouncing off of dust clouds in the spiral arms. These GRBs were released by the collapse of massive stars (supernovae) or the merger of neutron stars (kilonova bursts). The diameters of the rings in X-rays provide distance measurements, with larger rings being generated by dust clouds closer to us.

The speed at which a cell produces proteins is a decisive factor in determining whether it divides, specializes or retains its stem cell properties. A team of researchers led by Professor Stefan H. Stricker, professor of epigenetic engineering at LMU's Biomedical Center and research group leader at Helmholtz Munich, has worked with international partners to demonstrate directly for the first time that the amount of ribosomal RNA (rRNA) directly regulates these processes. Their results were published in the journal Science.

New method makes it possible to control ribosomal RNA in a targeted manner
It has been established for some time that the amount of ribosomal RNA differs among different types of cells and is altered in a number of diseases. But it remained unclear whether these specific characteristics are the cause or merely the result of biological processes.

With the newly developed CRISPR-based method TAPIR (Targeted Activation of Protein Translation), researchers now have access to a tool that can boost the activity of ribosomal genes and, as a result, influence a cell's protein production. "Our new study shows that targeted activation of rRNA production significantly increases protein synthesis," explains Stricker, lead author of the publication.

New perspectives for rare diseases and cancer
The results could be particularly relevant for diseases in which ribosome function is disrupted. These include ribosomopathies such as Treacher-Collins syndrome, a rare congenital disease that causes facial malformations. In a mouse model, the researchers partially compensated for disease-related alterations by stimulating rRNA production in a targeted way.

In addition, the research team observed that similar mechanisms also play a role in pancreatic cancer. Tumor cells seem to use increased rRNA production to maintain their rapid growth. In the mouse model for pancreatic cancer, TAPIR was able to increase rRNA production and promote the growth of the cancer cells. This shows that increased rRNA production has a causal effect in contributing to tumor growth and is not just a side effect.

Centaurus A is a giant galaxy located in the southern constellation of Centaurus.

Also known as NGC 5128, LEDA 46957, ESO 270-9, and Caldwell 7, the galaxy is one of the brightest objects in the southern hemisphere night sky.

Centaurus A was discovered on April 29, 1826 by the Scottish astronomer James Dunlop.

At a distance of 13 million light-years, it is the closest active galactic nucleus to us.

Astronomers theorize that what was originally an elliptical galaxy collided with a relatively smaller spiral galaxy, giving it the peculiar shape we see now.

“At Centaurus A’s core sits a supermassive black hole actively feeding on surrounding material,” the Webb astronomers said in a statement.

“As it does, the black hole launches powerful jets and releases enormous amounts of energy, shaping the galaxy around it.”

“At the same time, Centaurus A bears the scars of a dramatic past: a major collision with another galaxy roughly two billion years ago.”

“The aftermath of that merger is still visible today in its unusual structure and ongoing star formation.”

Visible light observations from the NASA/ESA Hubble Space Telescope could not reveal the central region of Centaurus A where dust blocked the view, while NASA’s retired Spitzer Space Telescope revealed large scale structures in the infrared without resolving individual stars.

Now, Webb brings both clarity and depth, exposing the galaxy’s inner workings star by star.