Monday, June 23, 2025

 

Smart textiles for personalized sports and healthcare: A comprehensive review




Shanghai Jiao Tong University Journal Center
Smart Textiles for Personalized Sports and Healthcare 

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  • This review provides comprehensive structural design strategies for the manufacturing of smart textiles, covering fibers, yarns, and fabrics and offers professional guidance for product development in this field.
  • The fundamental performance criteria for sports-oriented smart textiles have been provided, highlighting the key attributes required for their optimal functionality in athletic applications.
  • This review systematically introduces the diverse roles of smart textiles in specific sports scenarios and the stringent requirements they must meet to perform effectively in these environments.
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Credit: Ziao Xu, Chentian Zhang, Faqiang Wang, Jianyong Yu, Gang Yang, Roman A. Surmenev, Zhaoling Li, Bin Ding.





A groundbreaking review on smart textiles has been published in Nano-Micro Letters, led by Professor Zhaoling Li and Professor Bin Ding from Donghua University, Shanghai, China. This comprehensive study explores the latest advancements in the design, preparation, and application of smart textiles, highlighting their potential to revolutionize personalized sports and healthcare. The research provides valuable insights into how these innovative textiles can seamlessly integrate sensing and monitoring capabilities with the comfort and flexibility of traditional fabrics.

Why Smart Textiles Matter

  • Enhanced Comfort and Functionality: Smart textiles combine the breathability and flexibility of traditional fabrics with advanced sensing capabilities, making them ideal for long-term wear during sports and health monitoring.
  • Real-Time Data Collection: These textiles can monitor vital signs, joint movements, and environmental conditions in real-time, providing valuable insights for athletes and healthcare professionals.
  • Versatility in Applications: From sports performance enhancement to health monitoring, smart textiles offer a wide range of applications, including wearable sensors, energy harvesting, and self-powered devices.

Innovative Design and Mechanisms

  • Fiber-Level Innovations: The review discusses various types of smart fibers, including coated, intrinsic, coaxial, and composite fibers, each offering unique advantages for different applications. For example, coated fibers can be tailored with functional materials to enhance their sensing capabilities.
  • Yarn and Fabric Design: Smart yarns and fabrics are created through innovative spinning and weaving techniques, allowing for the integration of multiple functionalities while maintaining the textile's structural integrity. Techniques like core-spinning and braiding are highlighted as effective methods for creating durable and functional textiles.
  • Integration with Electronics: The review explores the integration of microelectronic systems with textiles, enabling the development of wearable devices that can monitor health and performance metrics in real-time.

Applications in Sports and Healthcare

  • Vital Signs Monitoring: Smart textiles can monitor heart rate, body temperature, and respiratory rate with high accuracy, providing essential data for health management.
  • Joint Movement Tracking: These textiles can track joint movements and angles, helping athletes optimize their performance and prevent injuries.
  • Sweat Analysis: Smart textiles can analyze sweat biomarkers, such as lactate and glucose, offering non-invasive methods for monitoring physiological conditions.
  • Data Transmission: The integration of wireless communication technologies allows for real-time data transmission, enabling remote monitoring and analysis.

Future Outlook

  • Scalability and Practical Applications: The review emphasizes the need for scalable and cost-effective manufacturing processes to bring smart textiles from the lab to the market.
  • Further Research: Future work may focus on improving the durability, accuracy, and energy efficiency of smart textiles, as well as exploring new materials and fabrication techniques.
  • Integration with IoT and AI: The potential integration of smart textiles with the Internet of Things (IoT) and artificial intelligence (AI) is highlighted as a promising direction for future research, enabling more intelligent and responsive wearable systems.

Conclusion

Smart textiles represent a significant advancement in wearable technology, offering a versatile and comfortable platform for sports and healthcare applications. This review provides a comprehensive overview of the current state of smart textiles, highlighting their potential to transform personalized sports and healthcare. As research continues to advance, smart textiles are poised to become an integral part of the next-generation wearable devices, enhancing human performance and well-being.

Stay tuned for more groundbreaking research in the field of smart textiles as Professor Zhaoling Li and Professor Bin Ding continue to push the boundaries of wearable technology!

Bi-layered coating: A breakthrough in fire-resistant materials




Shanghai Jiao Tong University Journal Center
Bi‑Layered, Ultrathin Coating Initiated Relay Response to Impart Superior Fire Resistance for Polymeric and Metallic Substrates 

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  • Relay response of bi-layered coating achieved fast response and extended protection.
  • 320-µm coating achieved over 900 s of burn-through resistance.
  • 320-µm coating achieved extended electrochemical stability for battery under fire.
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Credit: Wei Tang, Qi Chen, Junxiao Li, Xiang Ao, Yunhuan Liu, Lijun Qian*, Silvia González Prolongo, Yong Qiu, De-Yi Wang.





Fire safety is a critical concern across various industries, from construction and transportation to electronics and energy storage. Traditional flame-retardant coatings often fail to provide both immediate and prolonged protection, limiting their applicability. Now, researchers from the IMDEA Materials Institute, Beijing Technology and Business University, and Universidad Rey Juan Carlos, led by Professor Lijun Qian and Professor De-Yi Wang, have developed an innovative bi-layered coating that addresses these challenges. Their findings, published in Nano-Micro Letters, demonstrate superior fire resistance with a mere 320-micron thickness.

Why This Bi-Layered Coating Matters

  • Fast Response and Extended Protection: The bi-layered coating combines an intumescent flame-retardant (IFR) outer layer and a ceramifiable inner layer, enabling both rapid response to fire and long-lasting protection.
  • Superior Burn-Through Resistance: The coating withstands fire temperatures up to 1400°C for over 900 seconds, significantly outperforming traditional coatings. This level of protection is crucial for materials like aluminum and glass fabric-reinforced epoxy resin, which typically burn through in under 200 seconds.
  • Enhanced Electrochemical Stability: When applied to lithium soft-package batteries, the bi-layered coating suppresses the formation and decomposition of solid interface layers, leading to prolonged electrochemical stability and fire safety.

Innovative Design and Mechanisms

  • Relay Response Effect: The bi-layered structure functions like a relay, with the IFR layer providing immediate protection and the ceramifiable layer offering long-term stability. The IFR layer rapidly forms a char barrier at temperatures below 300°C, while the ceramifiable layer undergoes a phase transformation at around 550°C to create a durable ceramic barrier.
  • Optimized Formulations: The researchers optimized the formulations of both the IFR and ceramifiable layers. The IFR layer, enhanced with alumina synergists, achieves a 31% residue yield at 800°C, while the ceramifiable layer, composed of low-melting glass powder and other fillers, maintains over 97% residue yield.
  • Thermal Insulation and Barrier Effect: The bi-layered coating not only provides a rapid response but also excellent thermal insulation. The char layers formed during combustion effectively block heat transfer, protecting the underlying substrate from prolonged exposure to high temperatures.

Future Outlook

  • Scalability and Commercialization: The thin and efficient nature of the bi-layered coating makes it highly scalable and suitable for large-area applications. Its ability to provide both rapid and long-lasting protection positions it well for commercial adoption in various industries.
  • Versatility in Applications: The bi-layered coating has demonstrated effectiveness on multiple substrates, including polyurethane foam, aluminum, and glass fabric-reinforced epoxy resin. Its potential applications extend to fire-resistant coatings for buildings, flame-retardant materials for transportation, and fire-safe energy storage devices.
  • Mechanistic Insights: This study provides valuable insights into the mechanisms of intumescent flame retardancy and ceramification, offering a blueprint for further development of high-performance flame-retardant coatings.

Stay tuned for more groundbreaking advancements from Professor Lijun Qian and Professor De-Yi Wang as they continue to push the boundaries of fire-resistant materials!

SPACE/COSMOS

🌟The Bright Side: Groundbreaking Vera Rubin Observatory in Chile reveals first images


Washington (AFP) – The Vera Rubin Observatory in Chile published its first images on Monday, revealing distant galaxies and stellar nurseries in the Milky Way with impressive detail. After 20 years in the making, the US-funded telescope gets ready to start repeatedly scanning the sky to create a high-definition time-lapse of the Universe.


Issued on: 23/06/2025 - AFP
By: FRANCE 24

The Trifid Nebula and the Lagoon Nebula -- stellar nurseries within our Milky Way -- are seen in unprecedented detail © HANDOUT / NSF-DOE Vera C. Rubin Observatory/AFP


The team behind the long-awaited Vera Rubin Observatory in Chile published their first images on Monday, revealing breathtaking views of star-forming regions as well as distant galaxies.

More than two decades in the making, the giant US-funded telescope sits perched at the summit of Cerro Pachon in central Chile, where dark skies and dry air provide ideal conditions for observing the cosmos.

One of the debut images is a composite of 678 exposures taken over just seven hours, capturing the Trifid Nebula and the Lagoon Nebula -- both several thousand light-years from Earth -- glowing in vivid pinks against orange-red backdrops.

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The image reveals these stellar nurseries within our Milky Way in unprecedented detail, with previously faint or invisible features now clearly visible.
In just a small section of the Rubin Observatory's total view of the Virgo Cluster, bright stars shine in the foreground in front of many distant galaxies NSF-DOE Vera C. Rubin Observatory Handout, AFP

Another image offers a sweeping view of the Virgo Cluster of galaxies.

The team also released a video dubbed the "cosmic treasure chest," which begins with a close-up of two galaxies before zooming out to reveal approximately 10 million more.

"The Rubin Observatory is an investment in our future, which will lay down a cornerstone of knowledge today on which our children will proudly build tomorrow," said Michael Kratsios, director of the White House Office of Science and Technology Policy.
Visible are two prominent spiral galaxies (lower right), three merging galaxies (upper right), several groups of distant galaxies, many stars in the Milky Way galaxy and more. The team behind the long-awaited Vera Rubin Obserevatory in Chile published their first images on June 23, 2025, revealing breathtaking views of star-forming regions as well as distant galaxies. NSF-DOE Vera C. Rubin Observatory Handout, AFP

Equipped with an advanced 8.4-meter telescope and the largest digital camera ever built, the Rubin Observatory is supported by a powerful data-processing system.

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Later this year, it will begin its flagship project, the Legacy Survey of Space and Time (LSST). Over the next decade, it will scan the night sky nightly, capturing even the subtlest visible changes with unmatched precision.

The observatory is named after pioneering American astronomer Vera C. Rubin, whose research provided the first conclusive evidence for the existence of dark matter -- a mysterious substance that does not emit light but exerts gravitational influence on galaxies.

Dark energy refers to the equally mysterious and immensely powerful force believed to be driving the accelerating expansion of the universe. Together, dark matter and dark energy are thought to make up 95 percent of the cosmos, yet their true nature remains unknown.

The observatory, a joint initiative of the US National Science Foundation and Department of Energy, has also been hailed as one of the most powerful tools ever built for tracking asteroids.

In just 10 hours of observations, the Rubin Observatory discovered 2,104 previously undetected asteroids in our solar system, including seven near-Earth objects -- all of which pose no threat.

For comparison, all other ground- and space-based observatories combined discover about 20,000 new asteroids per year.

Aerial view of the Vera C. Rubin Observatory under construction in January 2024 Javier Torres, AFP

Rubin is also set to be the most effective observatory at spotting interstellar objects passing through the solar system.

More images from the observatory are expected to be released later Monday morning.

First celestial image unveiled from revolutionary telescope


Ione Wells
South America correspondent
Georgina Rannard
Science correspondent
BBC

NSF-DOE Vera C. Rubin Observatory
The first image revealed by the Vera Rubin telescope shows the Trifid and Lagoon nebulae in stunning detail

A powerful new telescope in Chile has released its first images, showing off its unprecedented ability to peer into the dark depths of the universe.

In one picture, vast colourful gas and dust clouds swirl in a star-forming region 9,000 light years from Earth.

The Vera C Rubin observatory, home to the world's most powerful digital camera, promises to transform our understanding of the universe.

If a ninth planet exists in our solar system, scientists say this telescope would find it in its first year.

RubinObs
Rubin Observatory and the Rubin Auxiliary Telescope in Cerro Pachón in Chile


It should detect killer asteroids in striking distance of Earth and map the Milky Way. It will also answer crucial questions about dark matter, the mysterious substance that makes up most of our universe.

This once-in-a-generation moment for astronomy is the start of a continuous 10-year filming of the southern night sky.

"I personally have been working towards this point for about 25 years. For decades we wanted to build this phenomenal facility and to do this type of survey," says Professor Catherine Heymans, Astronomer Royal for Scotland.

The UK is a key partner in the survey and will host data centres to process the extremely detailed snapshots as the telescope sweeps the skies capturing everything in its path.

Vera Rubin could increase the number of known objects in our solar system tenfold.
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NSF-DOE Vera C. Rubin Observatory
A huge cluster of galaxies including spiral galaxies in the vast Virgo cluster, which is about 100 billion times the size of the Milky Way.


BBC News visited the Vera Rubin observatory before the release of the images.

It sits on Cerro Pachón, a mountain in the Chilean Andes that hosts several observatories on private land dedicated to space research.

Very high, very dry, and very dark. It is a perfect location to watch the stars.

Maintaining this darkness is sacrosanct. The bus ride up and down the windy road at night must be done cautiously, because full-beam headlights must not be used.

The inside of the observatory is no different.

There is a whole engineering unit dedicated to making sure the dome surrounding the telescope, which opens to the night sky, is dark – turning off rogue LEDs or other stray lights that could interfere with the astronomical light they are capturing from the night sky.

The starlight is "enough" to navigate, commissioning scientist Elana Urbach explains.

One of the observatory's big goals, she adds, is to "understand the history of the Universe" which means being able to see faint galaxies or supernova explosions that happened "billions of years ago".

"So, we really need very sharp images," Elana says.

Each detail of the observatory's design exhibits similar precision.

SLAC National Accelerator Laboratory
Vera Rubin's is 3,200-megapixel camera was built by the US Department of Energy's SLAC National Accelerator Laboratory


It achieves this through its unique three-mirror design. Light enters the telescope from the night sky, hits the primary mirror (8.4m diameter), is reflected onto the secondary mirror (3.4m) back onto a third mirror (4.8m) before entering its camera.

The mirrors must be kept in impeccable condition. Even a speck of dust could alter the image quality.

The high reflectivity and speed of this allow the telescope to capture a lot of light which Guillem Megias, an active optics expert at the observatory, says is "really important" to observe things from "really far away which, in astronomy, means they come from earlier times".

The camera inside the telescope will repeatedly capture the night sky for ten years, every three days, for a Legacy Survey of Space and Time.

At 1.65m x 3m, it weighs 2,800kg and provides a wide field of view.

It will capture an image roughly every 40 seconds, for about 8-12 hours a night thanks to rapid repositioning of the moving dome and telescope mount.

It has 3,200 megapixels (67 times more than an iPhone 16 Pro camera), making it so high-resolution that it could capture a golf ball on the Moon and would require 400 Ultra HD TV screens to show a single image.

"When we got the first photo up here, it was a special moment," Mr Megias said.

"When I first started working with this project, I met someone who had been working on it since 1996. I was born in 1997. It makes you realise this is an endeavour of a generation of astronomers."

It will be down to hundreds of scientists around the world to analyse the stream of data alerts, which will peak at around 10 million a night.

The survey will work on four areas: mapping changes in the skies or transient objects, the formation of the Milky Way, mapping the Solar System, and understanding dark matter or how the universe formed.

But its biggest power lies in its constancy. It will survey the same areas over and over again, and every time it detects a change, it will alert scientists.

RubinObs
The Telescope Mount Assembly supports the camera and huge mirrors

"This transient side is the really new unique thing... That has the potential to show us something that we hadn't even thought about before," explains Prof Heymens.

But it could also help protect us by detecting dangerous objects that suddenly stray near Earth, including asteroids like YR4 that scientists briefly worried early this year was on track to smash into our planet.

The camera's very large mirrors will help scientists detect the faintest of light and distortions emitted from these objects and track them as they speed through space.

"It's transformative. It's going be the largest data set we've ever had to look at our galaxy with. It will fuel what we do for many, many years," says Professor Alis Deason at Durham university.

She will receive the images to analyse how far back the stars reach in the Milky Way.

At the moment most data from the stars goes back about 163,000 light years, but Vera Rubin could see back to 1.2 million light-years.

Prof Deason also expects to see into the Milky Way's stellar halo, or its graveyard of stars destroyed over time, as well as small satellite galaxies that are still surviving but are incredibly faint and hard to find.

Tantalisingly, Vera Rubin is thought to be powerful enough to finally solve a long-standing mystery about the existence of our solar system's Planet Nine.

That object could be as far away as 700 times the distance between the Earth and the Sun, far beyond the reach of other ground telescopes.

"It's gonna take us a long time to really understand how this new beautiful observatory works. But I am so ready for it," says Professor Heymans.


In the trace lies the truth: Halogens and the fate of the lunar crust


How halogens uncover the hidden history of lunar crust formation and the striking lunar surface dichotomy.



Ehime University

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Early Moon and its two faces 

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Around 4.5 billion years ago, the Moon was covered by a global magma ocean. The solidification of the Moon is expected to produce a plagioclase-rich crust. This only appears in the farside of the Moon, whereas the nearside Moon is largely covered by dark erupted basalts.

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Credit: Jiejun Jing





On a clear night, the Moon you gaze upon looks the same as it looked for the first humans that walked the Earth --- the same black-and-white side of our nearest neighbor by large dark ‘seas’ and white ‘highlands’ has been facing us for billions of years. The Moon is thought to have been born in a giant impact between our Earth and a Mars-sized other planet, Theia, ca. 4.5 billion years ago. The energy associated with this impact is expected to have led to an ocean of magma covering both the Earth and the young Moon. Cooling of this magma is expected to result in a nearly homogeneous solid Moon, covered with the same crust everywhere. This is not always the case. The hemisphere always facing us, called the lunar nearside, has a totally different appearance than its opposite half, the farside, which is dominated by bright, highland-dominated landscapes, with virtually no ‘seas’ (Fig.1).

The dark lunar ‘seas’ or maria in Latin, are composed of widespread basaltic magmas, mostly erupted ca. 3.5 billion years ago on the nearside, with very few eruption on the far side. This marks a distinct evolution history for these two hemispheres. Why and how did this happened? The secret that shaped the Moon into two worlds may well be buried within minute amounts of halogens (e.g., fluorine and chlorine), found in lunar samples.

Halogen abundances in lunar minerals provide unique insight into the Moon’s evolution, but incomplete knowledge of halogen incorporation in minerals and melts has limited their application. Researchers at the Geodynamics Research Center, Ehime University collaborating with colleagues from Universität Münster (Germany) and Vrije Universiteit Amsterdam (the Netherlands), carried out high-pressure, high-temperature experiments and successfully derived unique new data on how chlorine (Cl) distributes itself between lunar minerals and co-existing magma. They coupled models of the evolution of the lunar interior to measured halogen abundances in lunar crust samples and found that most lunar nearside samples turn out to be anomalously rich in Cl. In contrast, crustal materials from the lunar farside do not show this Cl enrichment. The researchers provide evidence to link this enrichment to the incorporation of gaseous Cl-compounds by lunar nearside rocks.

This finding indicates that the existence of widespread chloride vapor (with Cl likely present as metal chlorides) was possibly limited to the lunar nearside, suggesting the metal chloride vapor appears to be tied to lunar dichotomy. Considering Cl is highly incompatible and volatile, this vapor-phase metasomatism may be related to (impact-induced/eruption) degassing from extensive lunar mare basalts in the nearside Procellarum KREEP Terrane. Crustal rocks in the lunar farside, without Cl enrichment, are shown to be products from magma derived from lunar interior ca. 4.3 billion years ago. Based on F/Cl modeling, the researchers found that a particular type of lunar crustal rock called the Mg-suite likely originate from a deep mantle which preserves remnants of the initial lunar magma ocean that was present 4.5 billion years ago.

Chlorine-rich vapors released during eruptions (or impact-induced evaporation) played a key role in transforming the Moon’s nearside that human can see. Meanwhile, the farside crust, invisible to us all, escaped from these vapor-associated volcanic activities and thus preserved more pristine information about the Moon including about the lunar magma ocean that formed right after the Moon was born. This finding illustrates the scientific value of recent lunar space missions that focused specifically on studying the lunar far side.