News news, articles, and features | New Scientist /section/news/ Science news and science articles from New Scientist Mon, 13 Jul 2026 00:44:08 +0000 en-US hourly 1 https://wordpress.org/?v=7.0.1 242057827 UN space database aimed at easing global tensions is mysteriously down /article/2533721-un-space-database-aimed-at-easing-global-tensions-is-mysteriously-down/?utm_campaign=RSS|NSNS&utm_content=news&utm_medium=RSS&utm_source=NSNS Fri, 10 Jul 2026 14:12:00 +0000 /?post_type=article&p=2533721 2533721 Global warming already causing crop losses of over $20 billion a year /article/2533593-global-warming-already-causing-crop-losses-of-over-20-billion-a-year/?utm_campaign=RSS|NSNS&utm_content=news&utm_medium=RSS&utm_source=NSNS Fri, 10 Jul 2026 14:00:51 +0000 /?post_type=article&p=2533593
The economies of countries where many people work in farming will be hit the hardest
Imago/Alamy

Global warming-fuelled heat and drought is already hitting yields of maize, wheat and soybeans to the tune of $20 billion a year, a study has estimated. This could rise eightfold, to more than $160 billion by 2100, unless we slash emissions.

While the financial losses will be greatest for big producers such as the US, the impacts will be felt most in the lowest-income countries, where , at the International Institute for Applied Systems Analysis (IIASA) in Austria. “If you look at the least-developed countries in Africa, the impact is much bigger.” This could lead to social unrest and increased migration, she warns.

There is great uncertainty about these kinds of projections, not least because so much depends on how farmers respond and adapt to a continually changing climate, for instance, by switching to different crops or adopting irrigation where it is possible. In fact, the whole point of this study is to raise awareness and encourage adaptation, to help ensure these projections turn out to be overestimates, says team member , also at IIASA. “This is the entire mission of climate scientists: we make these cases for people to react, so our projections turn out to be wrong.”

The researchers started by gathering data on the yields per country of maize, wheat and soya from the UN Food and Agriculture Organization (FAO). Next, they took past climate data and calculated the drought level, using a standard approach that estimates soil moisture levels from rainfall and evaporation levels.

Past heat extremes and drought levels were then compared with the yields from 1974 to 2004 to estimate the impact of heat and drought. They then used these statistical correlations to estimate crop losses from 2007 to 2019. Their results suggest that increases in heat extremes and drought have caused a 3.5 per cent decline in yields relative to the 1974 to 2004 baseline. “Three per cent or so might not sound like much, but this is a major impact [on] the global food market, which regionally can trigger a severe crisis,” says Kornhuber.

The researchers then calculated the economic losses, based on FAO data showing how much farmers would have been paid for their produce at the time. Finally, they used the same approach to project future losses in several different emissions scenarios, assuming that some adaptation takes place.

In a high-emissions scenario, known as SSP3-7.0, global yields will fall by around 35 per cent by 2100, with annual losses rising to more than $161 billion. “The production losses caused by heat and drought are around 855 million tonnes a year,” says Hwong, who presented the results at a meeting of the European Geosciences Union in Vienna in May. “I think that is equivalent to what around 2 billion people consume over a year.”

This could be an underestimate of the full impact of climate change for a number of reasons: it’s just three crops, and it doesn’t include flood, storm or rain damage, or the possibility that shortages could lead to big price increases, as is already happening with some other crops such as coffee and cacao.

at Columbia University in New York says the study’s reliance on the statistical relationships between yield losses and extreme heat and drought could result in it overestimating the impacts by 2100. “Statistical yield models are great for explaining what’s happening now, and in the near past [or] future, but they are inherently unreliable when pushed into vastly different environmental regimes, such as high-emission climate scenarios by the end of the century.” Computer models of how plants are affected by rising CO2 and temperatures are better for projecting what will happen by the end of the century, he says.

at the University of Queensland, Australia, makes the same point. “Although models are not perfect, they are better suited for this type of extrapolation.” However, her team recently released a , which hasn’t been peer-reviewed, showing that two widely used models for wheat make large errors and are especially poor at forecasting the combined effects of extreme heat and drought.

But Kornhuber has defended his team’s use of statistical methods. “The models are remarkable tools, but some of the validation papers have suggested that they might not be super responsive to extremes,” he says. “In our project, extremes were the main focus, so we decided to establish these relationships directly through statistics.”

Reference:

EGU General Assembly 2026

]]>
2533593
Mathematicians put AI to work on Fermat’s last theorem /article/2533518-mathematicians-put-ai-to-work-on-fermats-last-theorem/?utm_campaign=RSS|NSNS&utm_content=news&utm_medium=RSS&utm_source=NSNS Fri, 10 Jul 2026 11:00:18 +0000 /?post_type=article&p=2533518 2533518 2026 eclipse: 5 citizen science projects you can contribute to /article/2531817-2026-eclipse-5-citizen-science-projects-you-can-contribute-to/?utm_campaign=RSS|NSNS&utm_content=news&utm_medium=RSS&utm_source=NSNS Fri, 10 Jul 2026 05:00:49 +0000 /?post_type=article&p=2531817
There are several ways you can help scientists study this year’s eclipse
Sirbouman/Alamy
During the total solar eclipse on 12 August, scientists from around the world will have their eyes – and scientific instruments – on the sun. But even if you aren’t a scientist, you can help in their investigations, both during the eclipse and year-round. A total solar eclipse occurs when the sun and moon line up just right so that the moon blocks out the entire disc of the sun from the perspective of Earth. It is a huge cosmic coincidence that both the sun and the moon happen to be just the right size and at the right distance to give us such a spectacle, and a scientifically useful one at that. On 12 August, a total eclipse will be visible over parts of Europe and the Arctic and Atlantic oceans, with a partial eclipse covering much of Europe, Canada, north-west Africa and parts of the US. An eclipse like this one is visible from somewhere on Earth just once every 18 months approximately, so during each eclipse, scientists rush out to gather as much data as they can. Here are some ways that you can help out: 1. Record shadow bands from the path of totality: In the moments before and after a total solar eclipse, strange phenomena called shadow bands billow across the ground. These bands are caused by the combination of Earth’s atmosphere and the hidden disc of the sun – it is similar to the effect that causes more distant stars to twinkle. If you are in the path of totality, all you have to do to see them is set out a white sheet or piece of cardboard perpendicular to the direction of the sun. To , which aims to quantify how shadow bands differ based on altitude and distance from the centre of totality, just set up a camera to film the sheet. 2. Photograph the sun with your smartphone: The sun is very nearly spherical, but it isn’t perfect. One of the best ways to measure its shape with precision is to have lots of pictures taken from lots of different locations – that’s what does. It’s a smartphone app that you can set up and leave running as you enjoy watching the eclipse, and it will take carefully timed pictures to capture a phenomenon called Baily’s Beads, or the diamond ring effect. When the very last of the sun is about to be covered by the moon, the lunar landscape lets through tiny points of light, which shine along its edge. The same happens when the other side of the moon is just about to let the sun shine past it again, and these points of light are Baily’s Beads. When lots of photos of the beads, all precisely geolocated, are combined with a map of the lunar topography, that can give us an extraordinarily precise measurement of how far the disc of the sun is from a perfect circle. 3. Measure the darkening of the sky during the eclipse: Even if you are only going to see a partial eclipse, you can still help with scientific research. The Gaia4Sustainability project requires a little bit more equipment and set-up time, but once you have it sorted, you can leave it running all year round and keep collecting useful data. It consists of a small device with a bunch of sensors on it to measure the brightness of the sky and other meteorological factors, and the overarching goal of the programme is to measure light pollution so we can better understand its effects. But during the eclipse, the same sensors can be used to , and the more different spots the team has data from, the more they will be able to learn about atmospheric dynamics during eclipses.
4. Hunt for sun-grazing comets: As is the case for pretty much all astronomical events, a huge portion of the world won’t be able to see August’s total eclipse at all. Not to worry! There are still ways to get involved in solar science. In the , you can download satellite pictures of the sun and look for moving objects on its outskirts. Some of the objects will be comets skimming past the sun, and once researchers know those comets are there, they can do more detailed research. A huge proportion of the known comets were discovered through Sungrazer. All it takes is a computer, an internet connection and some spare time. 5. Join a DEB observation team for next year: If you want to do something a bit more involved, the might be more up your street. It’s an scheme where teams receive training and some relatively basic equipment to observe eclipses across the path of totality, building up a huge repository of data that can then be used to study the evolution of the corona, the outermost layer of the sun’s atmosphere. Because of the training required, it is too late to join or create a DEB team for this year, but if you are going to be able to spot the 2027 eclipse that will sweep over northern Africa, you can sign up ahead of time. Even during the eclipse, you shouldn’t look directly at the sun without a solar filter or eclipse glasses to protect your eyes. ]]>
2531817
Special relativity can warp chemical bonds – now we’ve seen it happen /article/2533629-special-relativity-can-warp-chemical-bonds-now-weve-seen-it-happen/?utm_campaign=RSS|NSNS&utm_content=news&utm_medium=RSS&utm_source=NSNS Thu, 09 Jul 2026 18:00:13 +0000 /?post_type=article&p=2533629
In some heavy atoms, like those of bismuth (pictured in crystalline form), electrons move at relativistic speeds
savva_25/Shutterstock

Albert Einstein’s theory of special relativity can reshape chemical bonds within molecules, and researchers have just seen it happen for the first time.

The theory of special relativity describes how moving at speeds close to the speed of light would affect travellers’ experience of space and time. Because of this, it is usually associated with particle accelerators and spacefaring objects, but within some heavy atoms, electrons experience relativistic speeds too.

at Brown University in Rhode Island and his colleagues have now managed to take an unprecedented look at how this breaks the standard notion of chemical bonds within a charged molecule made from bismuth and carbon.

Within the molecule, a bismuth atom and a carbon atom were connected by three bonds, one of which the researchers expected to be of “sigma” type and two of “pi” type. The difference between these two types stems from electrons’ quantum character – each electron is “smeared” across some region of space, instead of being a tight ball, and whether these regions overlap head on or side by side determines the type of chemical bond they create between the atoms.

In their experiment, Wang and his colleagues mapped the distribution of electrons throughout the molecule, effectively getting a look at its bonds. But instead of seeing electrons distributed in shapes associated with sigma and pi bonds, the team noticed that two of the bonds resembled two different mixes of sigma and pi shapes. “Their characters are different from our normal understanding,” says Wang. “You can’t really call it the sigma and pi.”

His team turned to at Washington State University, whose calculations ultimately showed that this mixing was a consequence of electrons near the bismuth nucleus feeling such a strong electromagnetic interaction that they moved at relativistic speeds. He says this effect hadn’t previously been captured in an experiment.

“The hardest thing about [studying] heavy elements is a lack of really good experimental data,” says Peterson. “To have such a beautiful experiment to be able to essentially compare very high-level theory to data is really a luxury.”

Wang says one important part of the new experiment is that he and his colleagues could make the molecule very cold before looking at its electrons. This dampened any jitters and excitations that would have made the final images imprecise.

“As you go down to the bottom of the periodic table, the usual quantum mechanics is no longer sufficient, you need to take into account the effects of relativity,” says at the University of Toulouse in France. He says that all elements in the same row of the periodic table as bismuth are affected by relativistic effects – for instance, gold would be the same colour as silver and mercury would not be liquid without them.

at the University of Helsinki in Finland says that for bismuth, the relativistic effect on its bonding with carbon could influence how organic bismuth compounds are used in chemical reactions. In fact, by researchers at the Max Planck Institute for Coal Research in Germany has already shown that relativistic effects help make this heavy metal a good catalyst, or accelerator, of chemical processes.

Wang says that the team now wants to repeat their experiment but swap bismuth for elements close to it in the periodic table to see when exactly special relativity makes the traditional chemical bond structure collapse.

Journal reference:

Science

]]>
2533629
Resuscitated human retinas respond to light 10 hours after death /article/2533673-resuscitated-human-retinas-respond-to-light-10-hours-after-death/?utm_campaign=RSS|NSNS&utm_content=news&utm_medium=RSS&utm_source=NSNS Thu, 09 Jul 2026 15:00:55 +0000 /?post_type=article&p=2533673 2533673 Mathematics of thermodynamics is being rewritten after 200 years /article/2533428-mathematics-of-thermodynamics-is-being-rewritten-after-200-years/?utm_campaign=RSS|NSNS&utm_content=news&utm_medium=RSS&utm_source=NSNS Thu, 09 Jul 2026 13:00:58 +0000 /?post_type=article&p=2533428 2533428 Injection halves risk of chromosome error common in older human eggs /article/2533616-injection-halves-risk-of-chromosome-error-common-in-older-human-eggs/?utm_campaign=RSS|NSNS&utm_content=news&utm_medium=RSS&utm_source=NSNS Thu, 09 Jul 2026 11:00:58 +0000 /?post_type=article&p=2533616 Fluorescence in situ hybridisation (FISH) micrograph of Down's syndrome chromosomes (red) in a foetus' cell nuclei (blue). The FISH technique enables individual chromosomes within the nuclei to be tagged with a fluorescent dye. Here, three copies of chromosome 21 are seen in each nucleus, the cause of Down's syndrome. In a healthy human, each nucleus contains only two copies of chromosome 21. Chromosomes are the parts of a nucleus responsible for carrying the genetic code. Down's syndrome is a genetic disease which causes mental retardation and typically flattened features. It affects around 1 in every 650 babies.
Cells with a signal indicating the presence of too many chromosomes
DEPT. OF CLINICAL CYTOGENETICS, ADDENBROOKES HOSPITAL/SCIENCE PHOTO LIBRARY
Human eggs that contain too many or too few chromosomes can lead to miscarriage, IVF failure and conditions such as Down’s syndrome. Now, researchers have found that giving the eggs a single injection can substantially reduce the problem. The approach could eventually boost the chances of success for older women undergoing IVF. “It really seems like a big deal,” says at Nilo Frantz Reproductive Medicine in Porto Alegre, Brazil, who wasn’t involved in the new research. “To my knowledge, this is the first [therapy] to show such clinical potential for correcting this major cause of IVF failure.” During a process called meiosis, egg and sperm cells eject exactly half of their genetic material. This means that when egg and sperm combine during fertilisation, they form an embryo with a complete genome. Sometimes, however, a sperm or egg cell has slightly more or slightly less than the half genome it should contain. This is a condition known as aneuploidy. Aneuploidy affects about in the early 30s and becomes more common with age. “Already in the late 30s, more than 65 per cent of all eggs are aneuploid,” at Ovo Labs, a biotechnology company in Germany, told the audience at the conference in London on 6 July. Clinicians sometimes screen IVF embryos for aneuploidy when treating couples at greater risk of miscarriage or IVF failure. , conditions caused by the genetic error – which include Down’s syndrome – are only detected via blood tests and ultrasound scans taken during the first trimester of pregnancy. Until now, there have been no ways to reduce the risk of aneuploidy occurring in the first place, says Zielinska. Now, Zielinska and her colleagues have found that the level of a protein called shugoshin-1 is substantially lower in older mouse and human eggs than in younger ones. Shugoshin-1 helps with a stage of meiosis in which two copies of each chromosome line up along the middle of an immature egg cell. The protein maintains the molecular glue that holds each pair together.
Upon fertilisation, the two copies of the chromosomes separate and move to opposite sides of the cell. One end ultimately forms the mature egg cell, and the other end is discarded. But in older eggs, the glue holding the chromosome pairs together degrades, which can cause the two copies of each chromosome to separate before fertilisation. When this happens, the chromosomes spread unevenly throughout the cell – which means the resulting egg may be aneuploid. To explore whether replenishing shugoshin-1 could prevent aneuploidy by helping to hold chromosome pairs together, the team collected 111 spare, immature eggs from more than 30 women aged between 22 and 43 who were banking eggs or undergoing IVF. The team injected the genetic code for shugoshin-1, in the form of mRNA, into one or more of each donor’s eggs, and left other eggs from the same donor untreated. A few hours later, chromosomes had prematurely separated in 53 per cent of the untreated eggs, whereas this figure was nearly half – 29 per cent – in the treated ones. In eggs from nine donors who were aged over 35, aneuploidy rates were 65 per cent, on average, in untreated eggs. But in treated eggs, the average figure was just 44 per cent. This reduction wasn’t statistically significant, although this is probably because of the study’s small sample size, according to the researchers. Further experiments showed the approach could prevent aneuploidy in mouse eggs, which were then successfully fertilised to produce healthy offspring. No side effects were seen in the mouse or human studies. “We’ve achieved live births in mice, so, from that perspective, we’re confident that this approach is not interfering in the mouse model with any steps of embryo development, and it doesn’t interfere with pup health and pregnancy health,” Zielinska told the conference audience. The researchers are now working towards testing the effects of shugoshin-1 in people. This would involve tweaking standard IVF to use immature eggs rather than mature ones, but this change would be fairly easy to implement, says Zielinska. She hopes the therapy, which the team calls EmbryoProtect, will provide an affordable way to improve IVF for older women. “We anticipate that the treatment will cost a fraction of the cost of a full IVF cycle,” says Zielinska. “By meaningfully improving IVF success rates, especially for women over 35 where baseline success is low, we hope that fewer attempts will be needed to conceive.”]]>
2533616
A worm that lived half a billion years ago preferred turning right /article/2533656-a-worm-that-lived-half-a-billion-years-ago-preferred-turning-right/?utm_campaign=RSS|NSNS&utm_content=news&utm_medium=RSS&utm_source=NSNS Thu, 09 Jul 2026 09:32:02 +0000 /?post_type=article&p=2533656
A fossil of Spriggina floundersi collected in South Australia. Because these fossils preserve mirror-image impressions of the original animals, a leftward bend in the rock represents an animal that bent to the right in life.
Spriggina floundersi worms that bent to the right are preserved as fossils that bend to the left
Scott Evans/AMNH

A 555-million-year-old worm had a predilection for turning right, possibly indicating the oldest known example of handedness.

Although these worms lacked limbs and so couldn’t be considered left- or right-handed in the way that we understand, the development of a tendency to favour one side over another is evidence of an advanced nervous system.

It remains a feature of free-living mobile life today, but until this discovery, it wasn’t thought to have emerged until the Cambrian Period, which began around 541 million years ago.

at the American Museum of Natural History in New York and his colleagues analysed 100 fossil specimens of a small flatworm-like creature, Spriggina floundersi, collected in South Australia over recent decades.

These animals lived during the Ediacaran Period, when multicellular life first became widespread. It preceded the Cambrian explosion, when animal life diversified dramatically and many groups of animals first appeared.

Spriggina lived in what was, half a billion years ago, a shallow ocean and is thought to have foraged on or close to the seafloor, moving by wriggling to the left or right.

“We have around 50 specimens of Spriggina that are clearly bent,” says Evans. Twice as many of the fossilised worms are bent to the left than to the right, he says. This means the creature itself bent to the right, as the specimens are mirror-image impressions of the animals, made when storms buried them in sand.

“This appears to be statistically significant and matches what biologists find when they study handedness in different animals today,” says Evans. “Some specimens have multiple bends to both the right and left, suggesting that they all could bend both ways, which makes sense if you don’t want to be stuck moving in a circle.”

While the majority seem to demonstrate right-handedness, it is hard to tell if any were left-handed, he says. “I imagine it’s like taking a picture of 100 people waving with one hand today. You would likely be able to count that more people are waving with their right hand, but you wouldn’t be able to tell who is right- or left-handed.”

Discoveries like this demonstrate that many foundational characteristics that are common to a variety of animals today, such as the ability to move around, bilateral symmetry and handedness, evolved in the Ediacaran, says Evans.

In the Cambrian, organisms built on that foundation to become more complex, for example adding legs to move more efficiently, becoming “less alien and more like the major groups of animals we know today”, says Evans. “This is cool because it suggests that, while the Cambrian was an amazing time in animal evolution, those organisms didn’t just come out of nowhere: they built on the foundations established in the Ediacaran.”

“The presence of handedness in any kind of functional asymmetry, really deep into the fossil record, gives us important and interesting information about how these behaviours have evolved and how deeply in time they emerged,” says at Flinders University in Adelaide, Australia.

Journal reference:

Scientific Reports

]]>
2533656
Seeding clouds with seawater could prevent a super El Niño /article/2533348-seeding-clouds-with-seawater-could-prevent-a-super-el-nino/?utm_campaign=RSS|NSNS&utm_content=news&utm_medium=RSS&utm_source=NSNS Wed, 08 Jul 2026 18:00:00 +0000 /?post_type=article&p=2533348
Particles in ships’ exhaust inadvertently cause cloud brightening, and a similar effect could be employed to engineer the climate
NASA's Earth Obervatory
Short-term geoengineering to brighten clouds over the eastern Pacific Ocean could limit the damage caused by El Niño and save the global economy trillions of dollars, although there could be winners and losers from the disruption of natural cycles. The El Niño climate phase occurs when easterly winds weaken, allowing warm water built up in the western Pacific to slosh back across the central and eastern parts of the ocean. That heats the atmosphere and raises global temperatures, with losses to economic growth estimated in the trillions of dollars. What could become a very strong or “super” El Niño is now developing in the eastern Pacific. But climate modelling has suggested that, in the future, a geoengineering method called marine cloud brightening might be able to cut this warming short. The technique involves spraying tiny droplets of seawater into the air below low-lying stratocumulus clouds, where moisture condenses onto them. The clouds become whiter thanks to the increase in the number of droplets, reflecting more sunlight back to space. Shading part of the eastern Pacific called the Niño 3.4 region via cloud brightening could interrupt the feedback loops that cause an El Niño to develop. Cooler sea surface temperatures would strengthen the trade winds to again blow warm water back into the western Pacific. More cool water would then well up from the depths of the eastern Pacific, further cooling surface temperatures, and so on. “You can basically stop the dominoes from falling early when you do marine cloud brightening,” says at the University of California, San Diego, who worked on the study. “We’re kicking the cycle in the other direction.”
Wan and her colleagues got the idea from the “black summer” of catastrophic bush fires in Australia in 2019-2020, which were followed by La Niña, the opposite phase of El Niño that lowers global temperatures. Research has that drifting smoke particles brightened clouds and cooled the eastern Pacific, intensifying and prolonging the “triple dip” La Niña that began in 2020 and persisted through three winters, rather than just one or two. The study modelled what cloud brightening could have done to the super El Niño events of 1997-1998 and 2015-2016. It found that nine months of spraying seawater would have nearly halved warming of the Niño 3.4 region, from 2°C or more to a little over 1°C. It would have ended the El Niño by January, shaving several months off the events. The hypothetical cloud-brightening mission would have been massive, involving an estimated 2400 ships and delivering an amount of seawater spray that isn’t possible with current nozzle technology. But it would have turned a super El Niño into a moderate one. Wan says she was surprised how well it seemed to work, given that it could only be started in June, once El Niño had clearly begun developing. at the University of Exeter, UK, warns that these results might not translate to the real world, where warming seas typically start dissipating low-level clouds, leading to further warming and dissipation through a feedback loop. “In a model with a stronger cloud feedback, you would have to do more aerosol injection,” he says. “The experiments seem to be at the limit of what can be done.” Wan admits this approach could have unexpected consequences, since the model only projected the impact over two-year periods. In both simulations, La Niña started earlier after El Niño subsided, and in the 2015-2016 case, this subsequent cooler phase became stronger. That could be bad news for regions like the Horn of Africa, where strong La Niñas have, in the past, disrupted rainfall and . But she says the idea is worth further research. Unlike geoengineering aimed at reducing global temperatures for the long term, short-term geoengineering like this could avoid the risk of “termination shock”, where any disruption to the spraying of low-level seawater or stratospheric aerosols could allow years of pent-up warming to come roaring back. “This study is opening up doors for a completely new target for geoengineering research, which is climate variability and things like El Niño,” says Wan. “It’s potentially very powerful, because you’re not locked into these long-term risks.”
Journal reference:

Science Advances

]]>
2533348