Category: 7. Science

A new gas giant world discovered by citizen scientists using data from NASA’s exoplanet-hunting spacecraft TESS is cool, literally and figuratively.

The extrasolar planet, or “exoplanet,” designated TOI-4465 b is located around 400 light-years from Earth. It has a mass of around six times that of Jupiter, and it’s around 1.25 times as wide as the solar system’s largest planet. What is really exciting about TOI-4465 b, however, is the fact that it circles its star at a distance of around 0.4 times the distance between Earth and the sun in a flattened or “elliptical” orbit. One year for this planet takes around 102 Earth days to complete. Its distance from its star gives it an estimated temperature of between 200 and 400 degrees Fahrenheit (93 to 204 degrees Celsius).

BYLINE: Savannah Peat

Newswise — News readers often click on articles not based on topic but rather the behavior of their fellow audience members, according to new research from the University of Georgia.

And the way that news organizations label those articles could directly influence how much attention they receive and ultimately impact their revenue.

When you go to a news organization’s homepage, they typically label articles that readers are engaging with the most. The researchers focused on two common labels: “most shared” and “most read.” 

“These types of labels are not going anywhere. Popularity even in news labels is a psychological phenomenon,” said Tari Dagago-Jack, lead author of the study and an assistant professor of marketing in the UGA Terry College of Business. “Popularity labels on news outlets are taking advantage of the idea that we follow the lead of others and that our decision-making is influenced by what other people are doing.”

Article section labels influence click rate

At first glance, you may assume that these labels, “most shared” and “most read,” mean the same thing: A lot of people checked out the article. But there’s a clear difference that consumers pick up on.

“If something is most shared, we might assume that means many people had to read it and then deem it interesting enough or important enough to pass it on,” Dagogo-Jack said. “But then there’s this other reality where we know a lot of things that are widely shared are often extremely frivolous like cat videos or funny memes.”

In nine surveys and experiments involving hundreds of people, the study found respondents interpreted “most read” stories as being more informative. “Most shared” articles were viewed as less serious and more entertainment based.

“The primary goal for reading news is to gain information, and the label ‘most read’ is a stronger signal of an article’s information value.” —Tari Dagago-Jack, Terry College

“We as readers have two primary motives: to be informed or to be entertained — that is, for a welcome diversion,” said Dagogo-Jack. “At a baseline level, we were finding that people were choosing ‘most read’ at a way higher rate than ‘most shared.’ The primary goal for reading news is to gain information, and the label ‘most read’ is a stronger signal of an article’s information value.”

That means if editors want certain articles to get more attention, they should tailor the label to the readers’ goals.

Knowing your audience, content is key for engagement

The same went for articles advertised on social media. Posts from faux news organizations that had captions describing a more educational article as “most shared” received fewer clicks.

This wasn’t the case, however, for news stories that were less serious and newsworthy. In that case, the “most shared” label worked as well as the “most read” label.

It’s a key message for reporters, editors and web developers: Know your audience and your content.

“People should ask themselves: Why am I even clicking on this thing? Is it just because everyone else read it?” —Tari Dagago-Jack

“For pop culture, sports or music — more entertainment — in those sections you should highlight what is ‘most shared,’” Dagogo-Jack said. “But for world news, politics and science sections, you should be using things like ‘most read’ or ‘most viewed.’”

Dagogo-Jack also recommends putting thought into labels. Ambiguous choices like “trending” or “most popular” may stump readers altogether, as there are so many things this could mean.

“Providing these lists helps us get over information overload or choice paralysis,” he said. “It’s a crutch and makes the decision process easier, but I often wonder: At what cost?

“You’re clicking on something that a lot of people like and social proof is valuable, but it may not necessarily provide what you are looking for, and you just gave up on the search. People should ask themselves: Why am I even clicking on this thing? Is it just because everyone else read it?”

This study was published in the Journal of Consumer Research and was co-authored by New York University assistant professor Jared Watson.

Curious Kids is a series for children of all ages. If you have a question you’d like an expert to answer, send it to CuriousKidsUS@theconversation.com.

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How does the camera on the James Webb Space Telescope work and see so far out? – Kieran G., age 12, Minnesota

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Imagine a camera so powerful it can see light from galaxies that formed more than 13 billion years ago. That’s exactly what NASA’s James Webb Space Telescope is built to do.

Since it launched in December 2021, Webb has been orbiting more than a million miles from Earth, capturing breathtaking images of deep space. But how does it actually work? And how can it see so far? The secret lies in its powerful cameras – especially ones that don’t see light the way our eyes do.

I’m an astrophysicist who studies galaxies and supermassive black holes, and the Webb telescope is an incredible tool for observing some of the earliest galaxies and black holes in the universe.

When Webb takes a picture of a distant galaxy, astronomers like me are actually seeing what that galaxy looked like billions of years ago. The light from that galaxy has been traveling across space for the billions of years it takes to reach the telescope’s mirror. It’s like having a time machine that takes snapshots of the early universe.

By using a giant mirror to collect ancient light, Webb has been discovering new secrets about the universe.

A telescope that sees heat

Unlike regular cameras or even the Hubble Space Telescope, which take images of visible light, Webb is designed to see a kind of light that’s invisible to your eyes: infrared light. Infrared light has longer wavelengths than visible light, which is why our eyes can’t detect it. But with the right instruments, Webb can capture infrared light to study some of the earliest and most distant objects in the universe.

Although the human eye cannot see it, people can detect infrared light as a form of heat using specialized technology, such as infrared cameras or thermal sensors. For example, night-vision goggles use infrared light to detect warm objects in the dark. Webb uses the same idea to study stars, galaxies and planets.

Why infrared? When visible light from faraway galaxies travels across the universe, it stretches out. This is because the universe is expanding. That stretching turns visible light into infrared light. So, the most distant galaxies in space don’t shine in visible light anymore – they glow in faint infrared. That’s the light Webb is built to detect.

A golden mirror to gather the faintest glow

Before the light reaches the cameras, it first has to be collected by the Webb telescope’s enormous golden mirror. This mirror is over 21 feet (6.5 meters) wide and made of 18 smaller mirror pieces that fit together like a honeycomb. It’s coated in a thin layer of real gold – not just to look fancy, but because gold reflects infrared light extremely well.

The mirror gathers light from deep space and reflects it into the telescope’s instruments. The bigger the mirror, the more light it can collect – and the farther it can see. Webb’s mirror is the largest ever launched into space.

Inside the cameras: NIRCam and MIRI

The most important “eyes” of the telescope are two science instruments that act like cameras: NIRCam and MIRI.

NIRCam stands for near-infrared camera. It’s the primary camera on Webb and takes stunning images of galaxies and stars. It also has a coronagraph – a device that blocks out starlight so it can photograph very faint objects near bright sources, such as planets orbiting bright stars.

NIRCam works by imaging near-infrared light, the type closest to what human eyes can almost see, and splitting it into different wavelengths. This helps scientists learn not just what something looks like but what it’s made of. Different materials in space absorb and emit infrared light at specific wavelengths, creating a kind of unique chemical fingerprint. By studying these fingerprints, scientists can uncover the properties of distant stars and galaxies.

MIRI, or the mid-infrared instrument, detects longer infrared wavelengths, which are especially useful for spotting cooler and dustier objects, such as stars that are still forming inside clouds of gas. MIRI can even help find clues about the types of molecules in the atmospheres of planets that might support life.

Both cameras are far more sensitive than the standard cameras used on Earth. NIRCam and MIRI can detect the tiniest amounts of heat from billions of light-years away. If you had Webb’s NIRCam as your eyes, you could see the heat from a bumblebee on the Moon. That’s how sensitive it is.

Because Webb is trying to detect faint heat from faraway objects, it needs to keep itself as cold as possible. That’s why it carries a giant sun shield about the size of a tennis court. This five-layer sun shield blocks heat from the Sun, Earth and even the Moon, helping Webb stay incredibly cold: around -370 degrees F (-223 degrees C).

MIRI needs to be even colder. It has its own special refrigerator, called a cryocooler, to keep it chilled to nearly -447 degrees F (-266 degrees C). If Webb were even a little warm, its own heat would drown out the distant signals it’s trying to detect.

Turning space light into pictures

Once light reaches the Webb telescope’s cameras, it hits sensors called detectors. These detectors don’t capture regular photos like a phone camera. Instead, they convert the incoming infrared light into digital data. That data is then sent back to Earth, where scientists process it into full-color images.

The colors we see in Webb’s pictures aren’t what the camera “sees” directly. Because infrared light is invisible, scientists assign colors to different wavelengths to help us understand what’s in the image. These processed images help show the structure, age and composition of galaxies, stars and more.

By using a giant mirror to collect invisible infrared light and sending it to super-cold cameras, Webb lets us see galaxies that formed just after the universe began.

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Hello, curious kids! Do you have a question you’d like an expert to answer? Ask an adult to send your question to CuriousKidsUS@theconversation.com. Please tell us your name, age and the city where you live.

And since curiosity has no age limit – adults, let us know what you’re wondering, too. We won’t be able to answer every question, but we will do our best.

GA, UNITED STATES, June 30, 2025 /EINPresswire.com/ — How animals sense and respond to smells plays a pivotal role in their survival, communication, and evolution. Recently, a groundbreaking online database has compiled the most expansive collection of olfactory receptor (OR) genes ever assembled in chordates—animals with backbones. Encompassing over 1.1 million sequences across nearly 2,800 species, this resource offers a unified platform for exploring both functional genes and pseudogenes. It integrates advanced tools for visualizing molecular structures, mapping odor interactions, and analyzing evolutionary relationships. With its comprehensive design, the database opens new avenues for researchers to decode how animals perceive chemical cues and adapt to diverse ecological environments.

Olfactory receptors (ORs) are key to how animals perceive their surroundings, guiding behaviors like foraging, mating, and avoiding danger. In chordates, the genes encoding these receptors are remarkably diverse and evolve rapidly, shaped by species-specific environmental pressures. Despite the explosion of genomic data in recent years, the annotation of these genes has struggled to keep pace. Many species still lack reliable OR gene catalogs, and most existing databases focus narrowly—often omitting pseudogenes or comparative frameworks. These limitations hinder the broader understanding of OR gene function and evolution. Due to these issues, a comprehensive and scalable platform for OR annotation and integration is urgently needed.

To meet this need, researchers from ShanghaiTech University and Research Center for Life Sciences Computing, Zhejiang Lab, etc. have developed the chordata olfactory receptor database (CORD), published (DOI: 10.1093/procel/pwae050) in Protein & Cell on September 20, 2024. The online platform compiles and standardizes more than 1.1 million OR gene entries from 2,776 chordate species, offering a massive leap in the coverage, consistency, and accessibility of olfactory genomic data. By integrating functional receptors, pseudogenes, and odorant-interaction data, CORD sets a new benchmark for studying the genetic basis of smell across evolutionary lineages.

At the heart of CORD lies Genome2OR, a high-performance gene annotation tool built on hidden Markov models. Its latest update simplifies the annotation pipeline and supports custom profiles, enabling the accurate identification of over 663,000 functional ORs and more than 513,000 pseudogenes. The database spans seven major chordate groups—from mammals and birds to jawless fish—highlighting the evolutionary richness of olfactory systems. CORD’s interface is designed with researchers in mind, featuring nine functional modules for genome browsing, structural prediction, and comparative analysis. Tools include BLAST search, sequence logos (WebLogo), and OpenFold-based 3D modeling. Users can explore complex gene–odorant relationships, supported by 3,118 receptor–ligand pairs and data on nearly 24,000 odorant compounds. Advanced visualization techniques such as snake diagrams and interactive heatmaps reveal how ORs are structured and distributed across species. Further, protein clustering datasets (CORDclust30–90) and community network analysis offer new insight into OR gene families and their evolutionary pathways. Altogether, CORD blends depth with usability, empowering researchers to unravel the biology of smell with unprecedented precision.

Scent is one of the most ancient and intricate senses, said Dr. Suwen Zhao, one of the co-corresponding authors. Yet until now, researchers lacked a unified, scalable tool to study the extraordinary diversity of ORs in chordates. CORD fills this gap. It not only delivers a vast quantity of high-quality data, but it also makes that data discoverable and usable across disciplines—from molecular neuroscience to comparative genomics. Dr. Zhao highlighted the database’s potential to illuminate how olfactory genes function beyond the nose, impacting broader biological processes.

With its wide-ranging data and flexible interface, CORD is poised to transform multiple research fields. Evolutionary biologists can now trace how OR gene repertoires expand and contract across ecological niches. Biomedical researchers gain a new tool to study the role of ORs in conditions like inflammation, metabolic disorders, and cancer—where these receptors are increasingly found outside the nose. In computational biology, CORD’s modular structure supports machine learning applications for modeling protein–ligand interactions. Future updates will incorporate experimentally derived OR structures, integrate AlphaFold3-based odor–receptor simulations, and launch a genome browser to map gene neighborhoods. By unifying data and tools under one roof, CORD is set to propel olfaction research into its next frontier.

DOI
10.1093/procel/pwae050

Original Source URL
https://doi.org/10.1093/procel/pwae050

Funding information
This work was supported by the National Key Research and Development Programs of China (2022YFA1302900, S.Z.), the National Natural Science Foundation of China (32122024, S.Z.), Shanghai Frontiers Science Center for Biomacromolecules and Precision Medicine, the Shanghai Science and Technology Plan (21DZ2260400) and ShanghaiTech University.

Lucy Wang
BioDesign Research
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New Delhi: In a groundbreaking study, an international team of researchers led by the National Institute of Technology (NIT) Rourkela has explored the impact of spinning dust devils, massive dust storms, and extensive water-ice clouds on the Martian atmosphere. Collaborating with scientists from the UAE University and Sun Yat-sen University in China, the team analysed more than two decades of data from multiple Mars missions, including India’s Mars Orbiter Mission (MoM).

Understanding these processes will also help in preparing for human exploration missions. Knowing how Martian weather works can help protect spacecraft, support future astronauts, and improve our understanding of whether Mars may once have supported life, said the researchers in the paper published in the prestigious journal New Astronomy Reviews.

“Advancing the weather prediction on Mars is not just a scientific pursuit; it is the cornerstone of ensuring that future missions can sustain there and realise the past and future habitability of the red planet,” said Prof. Jagabandhu Panda, Professor at the Department of Earth and Atmospheric Sciences, NIT Rourkela.

Mars, also known as the Red Planet, is home to some of the most dramatic weather systems in the solar system. The dust raised by local and regional storms can travel far and disturb wind patterns, resulting in changes in temperatures and some cases, reshaping the Martian atmosphere in dramatic ways.

The study focused on three major elements of Martian weather: dust devils, small spinning columns of air that are common during the summer and more frequent in the northern hemisphere; large dust storms, driven by a loop in which sunlight heats the dust, and can grow to cover entire regions or even the whole planet; water-ice clouds, thin, wispy clouds made of frozen water particles.

Using imaging data from over 20 years, the researchers have traced how changing seasons on Mars affect the dust and cloud formation and movement. These findings refine human knowledge and understanding of Mars’ climate system and may be useful for predicting future weather on the planet.

As more missions head to the Red Planet, long-term studies like this one offer essential clues about its ever-changing skies.

“It would be great if ISRO could conduct more missions to Mars and invest more in the university system to carry out such research. It will help in advancing science and technology further,” Panda said. IANS

Disclaimer: Kindly avoid objectionable, derogatory, unlawful and lewd comments, while responding to reports. Such comments are punishable under cyber laws. Please keep away from personal attacks. The opinions expressed here are the personal opinions of readers and not that of Mathrubhumi.

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Copyright © 2025 by IOP Publishing Ltd and individual contributors

A new type of self-healing and reconfigurable circuit board can withstand heavy damage and still work effectively, scientists say. It can even be completely recycled once it reaches the end of its life.

The new breakthrough is owed to a material called a vitrimer, a special polymer capable of remaining rigid and durable at normal temperatures but malleable and reshapable at higher temperatures. The scientists outlined their findings in a new study published 1 June in the journal Advanced Materials.

A study by the Center for Redox Processes in Biomedicine (Redoxoma) led by Marilene Demasi from the Butantan Institute (São Paulo, Brazil) presents a valuable new experimental model for investigating the interaction between the proteasome and mitochondrial function. In eukaryotic cells, the proteasome is a protein complex responsible for eliminating damaged and nonfunctional proteins, thereby helping to maintain cellular balance and proper functioning.

In recent years, studies have revealed that the proteasome and mitochondria are more closely connected than previously thought. The proteasome plays a role in the quality control of proteins destined for the mitochondria, while mitochondrial metabolism affects the efficiency with which proteins marked for destruction are degraded.

Redoxoma, a Research, Innovation and Dissemination Center (RIDC) of FAPESP based at the University of São Paulo’s Institute of Chemistry (IQ-USP) conducted research focusing on the effects of proteasome dysfunction in the C76S mutant strain of the yeast Saccharomyces cerevisiae. The study revealed that deficiency in this system leads to increased mitochondrial oxidative stress. This was evidenced by increased hydrogen peroxide (H₂O₂) release and a lower peroxiredoxin 1 (Prx1) concentration. Prx1 is a crucial enzyme in the removal of peroxides. In mammals, mitochondrial Prx3 is equivalent to Prx1 in yeast.

The most important thing about this work is that we’ve a yeast strain that can serve as a model for investigating proteasome deficiency in relation to mitochondrial metabolism, a model that didn’t yet exist in the literature.”

Marilene Demasi, Butantan Institute

The study was published in an article in the journal Archives of Biochemistry and Biophysics.

Next steps

The researchers are now working to understand why Prx1 levels decrease in cells with compromised proteasomes. “We don’t yet know if there was a decrease in Prx1 gene expression, which is possible, since the proteasome also plays a role in gene transcription regulation, or if the protein oxidizes more. It may hyperoxidize and, as a result, be degraded more. Perhaps the excess peroxide is promoting its continuous degradation,” says the researcher at the Butantan Institute.

To answer these questions, the group plans to conduct comparative transcriptome and proteomic analyses of the wild and mutant strains cultivated under respiratory conditions. The goal is to establish this strain as a model for studying the role of the ubiquitin-proteasome system in cell metabolism.

Until now, thin and thick disks have only been identified in the Milky Way and nearby galaxies. It has been impossible with previous telescopes to distinguish the thin edge of a distant galaxy when viewed from the side.

That changed with the launching of the James Webb Space Telescope (JWST) in 2021, which is currently the largest telescope in space.

An international team of researchers has examined 111 JWST images of distant edge-on galaxies, ones where the alignments enabled the researchers to observe the galaxies’ vertical disk structures.

Takafumi Tsukui (formerly of the Australian National University and now based at Tohoku University), who led the research team, says that observing distant galaxies is like using a time machine, allowing us to see how galaxies have built their disks over cosmic history.

“Thanks to the JWST’s sharp vision, we were able to identify thin and thick disks in galaxies beyond our local universe, some going as far back as 10 billion years ago.”

The study revealed a consistent trend: in the earlier universe, more galaxies appear to have had a single thick disk, while in later epochs, more galaxies showed a two-layered structure with an additional thin disk component. This suggests that galaxies first formed a thick disk, followed by the formation of a thin disk within it. In more massive galaxies, this thin disk appears to have formed earlier.

The study estimated the thin disk formation time for Milky Way-sized galaxies to be around 8 billion years ago. This figure aligns with formation timelines for the Milky Way itself, where stellar ages can be measured.

To understand the revealed sequential formation from thick to thin disks and the corresponding formation timelines, the team not only examined the stellar structure but also the motion of gas, direct ingredients of stars obtained from the Atacama Large Millimeter/submillimeter Array (ALMA) and ground-based surveys in the literature. These observations supported a coherent formation scenario:

• In the early universe, galactic disks are rich in gas and highly turbulent
• Intense star formation in the turbulent disks gives rise to thick stellar disks
• As stellar disks develop, they help stabilize the gas disks and reduce the turbulence
• As the disk calms, a thin stellar disk forms inside the pre-developed thick stellar disks
• Whereas larger galaxies can efficiently convert gas into stars, forming thin disks earlier

Tsukui emphasizes that the images provided by JWST help answer one of the biggest questions in astronomy: was our galaxy’s formation typical or unique? “The JWST images provided a window into galaxies that resemble the Milky Way’s early state, bringing us valuable insights from galaxies far away.”

The team hopes that their study will help bridge studies of nearby galaxies with far away ones and refine our understanding of disk formation. The study was published in the journal Monthly Notices of the Royal Astronomical Society on June 26, 2025.

Planets form in disks composed of low-temperature molecular gas and dust, known as protoplanetary disks, found around protostars. Protostars are stars still in the process of forming. The nascent planets are too small to observe directly, but the gravity from a planet can create detectable patterns like rings or spirals in a protoplanetary disk. However, it is difficult to know when these patterns first appeared due to the limited number of protoplanetary disks that are close enough to Earth to be observed in high resolution.

A research team led by Ayumu Shoshi of Kyushu University and the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) used improved data processing techniques to search for previously overlooked signs of planet formation in archive data from the ALMA (Atacama Large Millimeter/submillimeter Array) radio telescope. The team reanalyzed data for 78 disks in the Ophiuchus star-forming region, located 460 light-years away in the direction of the constellation Ophiuchus. More than half of the images produced in this study achieved a resolution over three times better than that of previous images.

The new high-resolution images show ring or spiral patterns in 27 of the disks. Of these, 15 were identified for the first time in this study. Combining this new sample with pervious work for a different star-forming region, the team found that the characteristic disk substructures emerge in disks larger than 30 au (astronomical units, 1 au = 149,597,870,700 m, the distance between the Earth and the Sun) around stars in the early stage of star formation, just a few hundred thousand years after a star was born. This suggests that planets begin to form at a much earlier stage than previously believed, when the disk still possesses abundant gas and dust. In other words, planets grow together with their very young host stars.