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Comment by Dr. Krishna Kumari Challa 2 hours ago

Bird‑like robots promise greater flexibility and control than drones

Engineers have developed a bird-like ornithopter with flexible wings powered by piezoelectric materials, eliminating the need for motors, gears, or mechanical linkages. This solid-state design enables flapping and twisting motions, offering greater maneuverability and potential for applications such as search and rescue. Advanced modelling integrates flight physics, aiding future design optimization.

Xin Shan et al, Multi-physics finite state fully coupled modeling of mechanism-free induced-strain actuated ornithopters, Aerospace Science and Technology (2025). DOI: 10.1016/j.ast.2025.110573

Comment by Dr. Krishna Kumari Challa 2 hours ago

Why cultivating drought-resistant plants disappoints: Soil physics may be the real bottleneck
Water uptake in plants is primarily limited by soil properties, specifically capillary and viscous forces in soil pores, rather than by plant physiology. As soil dries and water potential drops below -1.5 MPa, plants cannot extract water efficiently, regardless of their internal adaptations. This explains why breeding for drought resistance by altering plant traits has had limited success.
Most water in the soil exists in pores of varying sizes. These pores exert a capillary force that holds water.
Soil physicists discovered that when the soil water potential falls below -1.5 megapascals, plants are unable to extract water fast enough to meet their needs.

In other words when soil dries, capillary and viscous forces in the pores increase—and plants find it harder to draw water from the soil.

Stomata are super sensitive. Plants have special structures on the underside of their leaves known as stomata that function as an interface for gas exchange. These are small valves that the plant opens and closes in response to fluctuating environments.

When they are open, carbon dioxide from the air can flow into the leaf while water can escape into the atmosphere as vapor.

When the plant closes it stomata, it conserves water. This prevents it from dying of thirst. However, when the stomata are closed, the plant faces starvation because less carbon dioxide enters its leaves, meaning it produces fewer new sugar molecules. As a result, it grows more slowly.

Ultimately, the behaviour of these tiny valves determines how much carbon from the atmosphere enters the land plant biomass.

A plant requires considerable energy to draw water from soil pores. For example, the cell walls of the tubes through which water rises in shoot stems or tree trunks are thickened.

This enables them to withstand the tension in the vascular system and not collapse.

Further up in the leaves, dissolved substances in plant cells generate osmotic pressure, which keeps cells turgid despite the high tension in neighbouring vascular tissues.

The agricultural industry has long attempted to breed plants that store more solutes in their cells, hoping this would help them absorb water more efficiently from the soil and thus better withstand drought. Although a substantial amount of money has been invested in such breeding programmes, these hopes have never been realized.

The new results explain this failure: the limiting factor lies not in the plants but in the soil.

The physics of capillarity not only predicts the extent to which soil pores empty but also what occurs high up in the leaves.

Andrea Carminati et al, Soils drive convergence in the regulation of vascular tension in land plants, Science (2026). DOI: 10.1126/science.adx8114

Comment by Dr. Krishna Kumari Challa 2 hours ago

Your Blood Type May Increase Risk of an Early Stroke

Comment by Dr. Krishna Kumari Challa 2 hours ago

How metformin treats diabetes

Comment by Dr. Krishna Kumari Challa 3 hours ago

Syncing Your Blinks

Our eyes and brains sync to music we are listening!

If you walk down the street while listening to your favourite song and you will notice that you were stepping in time to the beat! And people instinctively blink to the beat too. In a recent study, researchers saw that dozens of non-musicians blinked in sync to the beat structure of Bach songs, without being asked.

Our bodies respond to music in a lot of weird ways. For example, one Japanese study determined what types of songs will spontaneously make people bop up and down, and which make them sway side-to-side. In the case of blinking to the beat, the scientists found that when study participants were distracted by a screen, they were less likely to sync their blinks. It might mean that active listening is required to incite these involuntary effects.

The finding makes sense because music activates the motor areas of the brain. Even if we’re just sitting still—and not bopping along to the beat—there can often be this sense of motion.

https://pmc.ncbi.nlm.nih.gov/articles/PMC12626317/#:~:text=This%20d....

https://journals.plos.org/plosbiology/article?id=10.1371/journal.pb...

Comment by Dr. Krishna Kumari Challa 23 hours ago

New study uncovers mechanism explaining how obesity increases cancer risk

Obesity increases cancer risk by causing organs such as the liver, kidneys, and pancreas to enlarge primarily through an increase in cell number (hyperplasia), not just cell size. This expansion raises the number of cells susceptible to mutations, thereby elevating cancer risk. Organ size may predict cancer risk more accurately than BMI, highlighting the importance of maintaining a healthy weight early in life.

The study, published in Cancer Research,reveals a major driving force behind how obesity increases cancer risk across multiple organs.

The findings emphasize the importance of maintaining a healthy weight from early childhood and propose a potentially more accurate way than body mass index (BMI) to predict the increase in cancer risk associated with obesity.
The study reveals that excess weight doesn't just affect metabolism or hormones—it can physically enlarge organs, creating more opportunities for cancer to take hold. Understanding that process matters because it helps explain how everyday health choices can shape cancer risk years or even decades down the line."

In other words, as a person gains weight, their organs also grow in size by accumulating more cells to meet the higher energy needs of a bigger body. Having more cells boosts the odds of more DNA errors as cells divide, increasing the likelihood of cancer.
To test this hypothesis, researchers conducted a two-pronged study.
First, the team evaluated 747 adults whose weight in relationship to their height spanned the complete BMI spectrum, from underweight (18.5 BMI) all the way to severely obese (40-plus BMI). Using CT scans, the researchers measured the size of each adult's liver, kidneys, and pancreas.

This study is the first to analyze the size of multiple organs in a large cohort of individuals across the full BMI spectrum.

The scientists discovered that the organs grew larger as body weight increased. For every 5-point increase in BMI, the liver grew by 12%, kidneys by 9%, and the pancreas by 7%.

Next, the research team counted the cells in samples of kidney tissue taken from autopsies and reanalyzed biopsy data from living patients. The lab showed that more than 60% of the kidneys' growth resulted from an increase in the number of cells in the organ, a process called hyperplasia. The rest was due to individual cells growing bigger, or hypertrophy.
The new finding corrects earlier theories that larger organ size in obese individuals resulted primarily from fatter cells. Rather, obesity mainly increases the number of cells at risk for copying errors, uncontrollable growth, and potential malignancy.

This increase in organ size has harmful consequences.
The more cells in an organ, the more mutations and the greater the risk of one cell going awry during division and becoming cancerous.
Overall, the study showed a strong link between organ size enlargement and cancer risk across all three organs, confirming the mathematical predictions. The finding provides evidence for this as a major mechanism of tumorigenesis induced by obesity, in addition to factors like inflammation and hormonal imbalances.

This newly discovered effect of obesity can be large—with organs even doubling in size.

"When an organ doubles in size, it is expected to roughly double its risk of developing cancer", say the researchers.
Noting the relationship between diet and cancer, the authors emphasized the importance of maintaining a healthy weight from a young age.

Sophie Pénisson et al, Hyperplasia Functions as a Link Between Obesity and Cancer, Cancer Research (2026). DOI: 10.1158/0008-5472.can-25-2487

Comment by Dr. Krishna Kumari Challa yesterday

What we are seeing is essentially a planetary heat pump. Saturn's aurora heats its atmosphere, the atmosphere drives winds, the winds produce currents that power the aurora, and so it goes on. The system feeds itself.

"For decades, we knew something strange was happening with Saturn's apparent rotation rate, but we could not explain it. We then showed it was being driven by atmospheric winds, but we still did not know why those winds existed. These new observations, made possible by JWST, finally give us the evidence we needed to close that loop."

The findings also have broader implications. The research suggests that what happens in Saturn's atmosphere directly influences conditions in its surrounding magnetosphere—the vast region of space shaped by the planet's magnetic field—which in turn feeds energy back into the system. This two-way relationship between the atmosphere and magnetosphere may help explain why the effect is so stable and long-lasting.

Tom S. Stallard et al, JWST/NIRSpec Reveals the Atmospheric Driver of Saturn's Variable Magnetospheric Rotation Rate, Journal of Geophysical Research: Space Physics (2026). DOI: 10.1029/2025ja034578

Part 2

Comment by Dr. Krishna Kumari Challa yesterday

JWST solves decades-long mystery about why Saturn appears to change its spin

Saturn has puzzled scientists for many years. Measurements taken by NASA's Cassini spacecraft in 2004 suggested the planet's rotation rate was slowly changing over time—yet this should not have been possible, as a planet cannot simply speed up or slow down its spin.
Researchers now have used the most powerful space telescope ever built to answer one of the longest-standing puzzles in planetary science—why does Saturn appear to spin at a different speed depending on how you measure it? The findings, published in the Journal of Geophysical Research: Space Physics, reveal for the first time the complex patterns of heat and electrically charged particles in Saturn's aurora, and show that the entire system is driven by a self-sustaining feedback loop powered by the planet's own northern lights.
Using the James Webb Space Telescope (JWST), the team observed Saturn's northern auroral region—the equivalent of Earth's northern lights—continuously for a full Saturnian day, capturing detailed measurements that were simply not possible with any previous instrument.

By analyzing the infrared glow from a molecule called trihydrogen cation, which forms in Saturn's upper atmosphere and acts as a natural thermometer, the researchers were able to produce the first high-resolution maps of both temperature and particle density across Saturn's auroral region.
The level of detail was extraordinary. Previous measurements had errors of around 50 degrees Celsius, roughly on a par with the differences the scientists were trying to detect, and were produced by combining broad regions of the hot polar aurora. The new JWST data was ten times more accurate than previous measurements, allowing the team to map fine details of heating and cooling across Saturn's auroral region for the very first time.
What the team found was that these temperature and density patterns match remarkably well with predictions made by computer models more than a decade ago, but only if the source of heat is placed exactly where the main auroral emissions enter the atmosphere.

This means Saturn's aurora is not just a visual display—it is actively heating the atmosphere in a specific location. That localized heating drives winds, which in turn generate the electrical currents responsible for the aurora. The aurora then heats the atmosphere again, sustaining the whole cycle.
Part 1

Comment by Dr. Krishna Kumari Challa yesterday

Major volcanic eruptions might be driven by gas dissolving back into magma

Understanding what triggers large volcanic eruptions is crucial for hazard assessment, but the exact mechanism driving these eruptions is still poorly understood. The prevailing theory is that volatile exsolution—gas coming out of magma—is a main driver of eruptions, particularly in volcanoes rich in silica. However, a new study, published in Nature Communications, posits that it is actually gas being dissolved back into the magma that leads to the pressurization needed for large eruptions.
Previous research has emphasized volatile exsolution as a driver for eruption caused by increasing pressure in magma chambers. In volatile exsolution, dissolved gases, like water vapor, carbon dioxide and sulfur separate from a silicate melt to form bubbles as magma rises or cools. This decreases solubility, creating significant magmatic overpressure, which drives volcanic eruptions. Some previous studies have found that exsolved gases in large volcanic systems can actually buffer pressure, making eruptions less frequent, but larger when they do occur.

"However, for volatile exsolution to act as primary eruption trigger, exsolution must outpace both volatile loss by passive degassing and viscous relaxation of the crust. This, however, requires rapid crystallization rates that are difficult to maintain in larger, thermally buffered reservoirs. In large silicic systems, exsolved volatiles may therefore exert a primary control on magma compressibility and chamber growth, rather than directly triggering eruptions," the study authors explain.
The new study explores the opposite process, called volatile resorption, in which gases dissolve back into magma. The team says that this resorption reduces magma compressibility, modulating the system's response to recharge and its overall stability, which ends up expediting eruptions since it is harder to compress. Volatile resorption can rapidly increase pressure in large silicic magma chambers, potentially triggering eruptions faster than volatile exsolution.
The study authors say the simulations they conducted show resorption results in eruption faster than cases involving exsolution.

Franziska Keller et al, Volatile resorption expedites eruption onset in large silicic systems, Nature Communications (2026). DOI: 10.1038/s41467-026-70206-8

Comment by Dr. Krishna Kumari Challa yesterday

Scientists testing new scanning technology discover mysterious structure beneath an ancient Egyptian city

Archaeologists working in Egypt's Nile Delta may have discovered a tomb or temple dating back around 2,600 years while testing a new technology designed to locate structures buried deep beneath the surface. The team was studying the Buto (Tell el-Fara'in) site, the ruins of an ancient city that was occupied from the Predynastic period (around 3800 BCE) to the Early Islamic era (7th century CE).

During its long history, Buto was built, destroyed, and rebuilt and consequently has several layers, each potentially a rich source of archaeological remains. However, the oldest parts of the city are now buried beneath later ruins and thick mud deposits. This would make traditional digging difficult, time-consuming, and expensive as archaeologists have to move tons of debris or struggle with groundwater to reach lower levels. The technology helps guide them where to dig.

The researchers were trialing a multipronged approach that uses satellite radar (SAR) and electrical resistivity tomography (ERT).

The team started with the Sentinel-1 radar satellite to identify large-scale anomalies from space, as they describe in a paper published in the journal Acta Geophysica. When it detected something of interest, they followed up with ERT. The technology sends electrical currents between a series of electrodes placed in the ground to create a 3D model of subsurface structures based on how different materials conduct/resist electricity. This technique has been likened to an underground CT scan.

In the top three meters, the scans showed a layer of broken pottery and debris from the later Roman and Ptolemaic periods. However, at a depth of between three and six meters, the technology revealed a large, well-defined structure from the Saite period (around 2,600 years ago).

At this stage, the researchers thought it could be a large tomb or shrine. Next, they carried out a small 10 x 10 meter excavation, which uncovered mudbrick walls and religious artifacts where the sensors had predicted.

"The results of this study demonstrate the effectiveness of combining geophysical measurements and remote sensing data, which gave a very accurate vision in detecting buried settlements in a complex region," wrote the team in their paper.

Mohamed A. R. Abouarab et al, Multi-scale detection of buried archaeological elements across different occupation phases: an integrated approach using radar satellite imagery and electric resistivity tomography at Buto, northwestern Nile Delta of Egypt, Acta Geophysica (2026). DOI: 10.1007/s11600-026-01809-4

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