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Space & Physics

What brought carbon to Earth

This marks the first time a complex form of carbon essential for life on Earth has been observed outside the solar system. To learn more about the significance of this discovery, EdPublica interviewed the researchers behind the study– Gabi Wenzel, Ilsa Cooke, and Brett McGuire, who shared their insights on the implications of pyrene’s presence in space and its potential impact on our understanding of star and planet formation

Dipin Damodharan

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The findings suggest pyrene may have been the source of much of the carbon in our solar system. “It’s an almost unbelievable sink of carbon,” says Brett McGuire, right, standing with lead author of the study Gabi Wenzel. Credits: Photo: Bryce Vickmark

A team led by researchers at MIT has detected pyrene, a complex carbon-containing molecule, in a distant interstellar cloud. This finding opens new avenues for understanding the chemical origins of our solar system. Pyrene, a type of polycyclic aromatic hydrocarbon (PAH), was found in a molecular cloud similar to the one from which our solar system formed.

This marks the first time a complex form of carbon essential for life on Earth has been observed outside the solar system. Its discovery sheds light on how the compounds necessary for life could originate in space. The team detected pyrene in
a star-forming region known as the Taurus Molecular Cloud, located 430 light-years away, making it one of the closest such clouds to Earth.

This discovery also aligns with recent findings from the asteroid Ryugu, suggesting that pyrene may have played a key role in the carbon composition of the early solar system. To learn more about the significance of this discovery, EdPublica interviewed the researchers behind the study– Gabi Wenzel, Ilsa Cooke, and Brett McGuire, who shared their insights on the implications of pyrene’s presence in space and its potential impact on our understanding of star and planet formation. Brett McGuire is an assistant professor of chemistry at MIT, Ilsa Cooke is an assistant professor of chemistry at the University of British Columbia, and Gabi Wenzel is a postdoctoral researcher in McGuire’s group at MIT.

Below, the team responds to questions from EdPublica Editor Dipin Damodharan about this unexpected and exciting discovery.

‘Pyrene could be a major source of carbon in our solar system’

Q: How does the discovery of pyrene in TMC-1 enhance our understanding of the chemical inventory that contributed to the formation of our solar system?

Gabi Wenzel:

Stars much like our own sun are born from dense molecular clouds. The discovery of pyrene in a molecular cloud called TMC-1, one that might be very similar to our sun’s natal cloud and which will go on to form a star of its own, significantly enhances our understanding of the chemical inventory that contributed to the formation of our own solar system. As a polycyclic aromatic hydrocarbon (PAH), pyrene is one of the most complex organic molecules found in early molecular clouds, suggesting that the building blocks of organic matter were available in the environments where stars and their orbiting (exo)planets form.

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“One of the big questions in star and planet formation is: How much of the chemical inventory from that early molecular cloud is inherited and forms the base components of the solar system? What we’re looking at is the start and the end, and they’re showing the same thing.” McGuire says. Credits:Photo: Bryce Vickmark

This discovery sheds light on the chemical processes occurring in interstellar space, including gas-phase and surface reactions on dust grains, which are crucial for the evolution of organic chemistry. This further supports the notion that the primordial materials of our solar system contained a diverse range of organic compounds, providing insights into the potential for prebiotic chemistry on a young Earth and planetesimals.

Q: What specific challenges did you face in detecting pyrene, given that it is invisible to traditional radio astronomy methods, and how did the use of cyanopyrene help overcome these challenges?

Gabi Wenzel:

Pyrene, a fully symmetric PAH, does not possess a permanent electric dipole moment and hence is invisible in radio astronomical observations or rotational spectrometers in the laboratory. The CN radical is highly abundant in the cold and dark molecular cloud TMC-1, an environment that is about 10 K cold and in which you’d assume little chemistry to happen. However, earlier experimental works have shown that the CN addition (followed by hydrogen abstraction) to ringed hydrocarbon species such as benzene and toluene at low temperatures is a barrierless process.

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Adding a CN (nitrile) group to a hydrocarbon will drastically increase its permanent electric dipole moment and so allow rotational transitions. Indeed, several CN-functionalized species have been detected in TMC-1 and other sources, among which the CN-substituted benzene (cyanobenzene or benzonitrile) and other smaller PAHs, with cyanopyrene being the largest molecule found via radio astronomy to date, allowing us to infer the presence of pyrene itself.

Q: Can you elaborate on what it means for our understanding of carbon sources in the solar system that pyrene is found in both TMC-1 and asteroid Ryugu?

Ilsa Cooke:

TMC-1 is a famous example of a cold molecular cloud, one of the earliest stages of star and planet formation, while asteroids like Ryugu represent snapshots of later stages in the formation of solar systems. Asteroids are formed from material in the solar nebula that was inherited from the molecular cloud stage. Our radio observations of TMC-1 let us observe pyrene early on and possibly under conditions where it is first forming. Isotope signatures of the pyrene in Ryugu suggest it was formed in a cold interstellar cloud. From these two unique sets of measurements, we can start to unravel the inheritance of pyrene, and PAHs more generally, from their birth in interstellar space and their journey to new planets. If PAHs can survive all the way from the molecular cloud stage, they may provide planets with an important source of organic carbon.

p1 Dr. Cooke stands in front of the Green Bank Telescope. credit Dr. Brett McGuire
Dr. Cooke stands in front of the Green Bank Telescope. Credit Dr. Brett McGuire

Q: What are the different formation routes of PAHs that your research suggests, and how do these differ from previous hypotheses about PAH formation in space?

Ilsa Cooke:

Our results, combined with those of Zeichner et al., who measured pyrene in Ryugu, suggest that pyrene may form at low temperatures by “bottom-up” routes in molecular clouds. Previously, PAHs were most commonly associated with formation in high-temperature (ca. 1000 K) environments in the envelopes of dying stars. These stars are thought to eject their PAHs, along with other carbon-rich molecules, into the diffuse interstellar medium.

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However, the diffuse medium is a tenuous, harsh environment permeated by ultraviolet photons, and most astrochemists think that small PAHs would not survive their journey through the diffuse medium into dense molecular clouds. So we are still left with a puzzle: does that pyrene that we observe in TMC-1 form there, or was it formed somewhere else but it was able to survive its journey more efficiently than previously thought? If the pyrene is indeed formed within TMC-1, we do not yet know the chemical mechanism. Many possibilities exist, so close collaborations between laboratory astrochemists and observers will be critical to answer this question.

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The structure of Pyrene, a polycyclic aromatic hydrocarbon, or PAH. Credit: Wikimedia

Q: What are your plans for investigating larger PAH molecules in TMC-1, and what specific hypotheses are you looking to test with these investigations?

Brett McGuire:

We have a number of other targets lined up – again focusing on PAH structures that should show this special stability demonstrated by pyrene. They present the same experimental challenges, including needing to devise appropriate synthetic routes in the laboratory before collecting their spectra. The major question is just how complex the PAH inventory actually gets at this earliest stage of star formation.

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Ball-and-stick model of the pyrene molecule, a polycyclic aromatic hydrocarbon consisting offour fused benzene rings. Credit: Wikimedia

Prior to our work in TMC-1, nearly everything we knew about PAHs came from infrared observations of bulk properties in much warmer and more energetic regions, where PAHs are thought to be much larger. Does the population in TMC-1 look the same as in these regions? Is it at an earlier stage of chemical evolution? And how does this distribution compare to what we see in our own Solar System?

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Q: How do your findings about pyrene and PAHs in interstellar clouds influence our broader understanding of organic chemistry in the universe, particularly in relation to the origins of life?

Brett McGuire:

Life as we know it depends on carbon – it is the backbone upon which all our molecular structures are constructed. Yet, the Earth overall is somewhat depleted in carbon relative to what we’d naively expect, and we still don’t fully understand where the carbon we do have came from originally. PAHs in general seem to be a massive reservoir of reactive carbon, and what we are now seeing is that that reservoir is already present at the earliest stages of star-formation. Combined with the evidence from Ryugu, we’re now also seeing indications that the inventory of PAHs, and thus this reservoir of carbon, may actually survive from this dark molecular cloud phase through the formation of a star to be eventually incorporated into the planetary system itself.

Dipin is the Co-founder and Editor-in-Chief of EdPublica. A journalist and editor with over 15 years of experience leading and co-founding both print and digital media outlets, he has written extensively on education, politics, and culture. His work has appeared in global publications such as The Huffington Post, The Himalayan Times, DailyO, Education Insider, and others.

Health

Researchers Develop AI Method That Makes Computer Vision Models More Explainable

A new technique developed by MIT researchers could help make artificial intelligence systems more accurate and transparent in high-stakes fields such as health care and autonomous driving by improving how computer vision models explain their decisions.

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MIT researchers have developed a new explainable AI method that improves the accuracy and transparency of computer vision models, helping users trust AI predictions in healthcare and autonomous driving.
Image credit: Tara/Pexels

MIT researchers have developed a new explainable AI method that improves the accuracy and transparency of computer vision models, helping users trust AI predictions in healthcare and autonomous driving.

Researchers at MIT have developed a new approach to make computer vision models more transparent, offering a potential boost to trust and accountability in safety-critical applications such as medical diagnosis and autonomous driving.

In a media statement, the researchers said the method improves on a widely used explainability technique known as concept bottleneck modeling, which enables AI systems to show the human-understandable concepts behind a prediction. The new approach is designed to produce clearer explanations while also improving prediction accuracy.

Why explainable AI matters

In areas such as health care, users often need more than just a model’s output. They want to understand why a system arrived at a particular conclusion before deciding whether to rely on it. Concept bottleneck models attempt to address that need by forcing an AI system to make predictions through a set of intermediate concepts that humans can interpret.

For example, when analysing a medical image for melanoma, a clinician might define concepts such as “clustered brown dots” or “variegated pigmentation.” The model would first identify those concepts and then use them to arrive at its final prediction.

But the researchers said pre-defined concepts can sometimes be too broad, irrelevant or incomplete for a specific task, limiting both the quality of explanations and the model’s performance. To overcome that, the MIT team developed a method that extracts concepts the model has already learned during training and then compels it to use those concepts when making decisions.

The approach relies on two specialised machine-learning models. One extracts the most relevant internal features learned by the target model, while the other translates them into plain-language concepts that humans can understand. This makes it possible to convert a pretrained computer vision model into one capable of explaining its reasoning through interpretable concepts.

“In a sense, we want to be able to read the minds of these computer vision models. A concept bottleneck model is one way for users to tell what the model is thinking and why it made a certain prediction. Because our method uses better concepts, it can lead to higher accuracy and ultimately improve the accountability of black-box AI models,” Antonio De Santis, lead author of the study, said in a media statement.

De Santis is a graduate student at Polytechnic University of Milan and carried out the research while serving as a visiting graduate student at MIT’s Computer Science and Artificial Intelligence Laboratory (CSAIL). The paper was co-authored by Schrasing Tong, Marco Brambilla of Polytechnic University of Milan, and Lalana Kagal of CSAIL. The research will be presented at the International Conference on Learning Representations.

Concept bottleneck models have gained attention as a way to improve AI explainability by introducing an intermediate reasoning step between an input image and the final output. In one example, a bird-classification model might identify concepts such as “yellow legs” and “blue wings” before predicting a barn swallow.

However, the researchers noted that these concepts are often generated in advance by humans or large language models, which may not always match the needs of the task. Even when a model is given a fixed concept set, it can still rely on hidden information not visible to users, a challenge known as information leakage.

“These models are trained to maximize performance, so the model might secretly use concepts we are unaware of,” De Santis said in a media statement.

The team’s solution was to tap into the knowledge the model had already acquired from large volumes of training data. Using a sparse autoencoder, the method isolates the most relevant learned features and reconstructs them into a small number of concepts. A multimodal large language model then describes each concept in simple language and labels the training images by marking which concepts are present or absent.

The annotated dataset is then used to train a concept bottleneck module, which is inserted into the target model. This forces the model to make predictions using only the extracted concepts.

The researchers said one of the biggest challenges was ensuring that the automatically identified concepts were both accurate and understandable to humans. To reduce the risk of hidden reasoning, the model is limited to just five concepts for each prediction, encouraging it to focus only on the most relevant information and making the explanation easier to follow.

When tested against state-of-the-art concept bottleneck models on tasks including bird species classification and skin lesion identification, the new method delivered the highest accuracy while also producing more precise explanations, according to the researchers. It also generated concepts that were more relevant to the images in the dataset.

Still, the team acknowledged that the broader challenge of balancing accuracy and interpretability remains unresolved.

“We’ve shown that extracting concepts from the original model can outperform other CBMs, but there is still a tradeoff between interpretability and accuracy that needs to be addressed. Black-box models that are not interpretable still outperform ours,” De Santis said in a media statement.

Looking ahead, the researchers plan to explore ways to further reduce information leakage, possibly by adding additional concept bottleneck modules. They also aim to scale up the method by using a larger multimodal language model to annotate a larger training dataset, which could improve performance further.

This latest work adds to growing efforts to make AI systems not only more powerful, but also more understandable in domains where trust can be as important as accuracy.

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Space & Physics

Researchers Develop Stretchable Material That Can Instantly Switch How It Conducts Heat

MIT engineers have developed a stretchable material heat conduction system that can rapidly switch how heat flows, enabling adaptive cooling applications.

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Laboratory experiment showing a stretchable polymer fibre demonstrating stretchable material heat conduction as its thermal behaviour changes when the material is stretched.
Experiments show that a fibre made from a widely used polymer can reversibly change how it conducts heat when stretched. Image credit: Courtesy of the researchers/MIT

Stretchable material heat conduction has taken a major leap forward as engineers at MIT have developed a polymer that can rapidly and reversibly switch how it conducts heat simply by being stretched. The discovery opens new possibilities for adaptive cooling technologies in clothing, electronics, and building infrastructure.

Engineers at the Massachusetts Institute of Technology have developed a new polymer material that can rapidly and reversibly switch how it conducts heat—simply by being stretched.

The research shows that a commonly used soft polymer, known as an olefin block copolymer (OBC), can more than double its thermal conductivity when stretched, shifting from heat-handling behaviour similar to plastic to levels closer to marble. When the material relaxes back to its original form, its heat-conducting ability drops again, returning to its plastic-like state.

The transition happens extremely fast—within just 0.22 seconds—making it the fastest thermal switching ever observed in a material, according to the researchers.

The findings open up possibilities for adaptive materials that respond to temperature changes in real time, with potential applications ranging from cooling fabrics and wearable technology to electronics, buildings, and infrastructure.

A new direction for adaptive materials

“We need materials that are inexpensive, widely available, and able to adapt quickly to changing environmental temperatures,” said Svetlana Boriskina, principal research scientist in MIT’s Department of Mechanical Engineering, in a media statement. She explained that the discovery of rapid thermal switching in this polymer creates new opportunities to design materials that actively manage heat rather than passively resisting it.

The research team initially began studying the material while searching for more sustainable alternatives to spandex, a petroleum-based elastic fabric that is difficult to recycle. During mechanical testing, the researchers noticed unexpected changes in how the polymer handled heat as it was stretched and released.

“What caught our attention was that the material’s thermal conductivity increased when stretched and decreased again when relaxed, even after thousands of cycles,” said Duo Xu, a co-author of the study, in a media statement. He added that the effect was fully reversible and occurred while the material remained largely amorphous, which contradicted existing assumptions in polymer science.

The discovery demonstrates how stretchable material heat conduction can be actively controlled in real time, allowing materials to respond dynamically to temperature changes.

How stretching unlocks heat flow

At the microscopic level, most polymers consist of tangled chains of carbon atoms that block heat flow. The MIT team found that stretching the olefin block copolymer temporarily straightens these tangled chains and aligns small crystalline regions, creating clearer pathways for heat to travel through the material.

“This gives the material the ability to toggle its heat conduction thousands of times without degrading

Unlike earlier work on polyethylene—where similar alignment permanently increased thermal conductivity—the new material does not crystallise under strain. Instead, its internal structure switches back and forth between straightened and tangled states, allowing repeated and reversible thermal switching.

“This gives the material the ability to toggle its heat conduction thousands of times without degrading,” Xu said.

From smart clothing to cooler electronics

The researchers say the material could be engineered into fibres for clothing that normally retain heat but instantly dissipate excess warmth when stretched. Similar concepts could be applied to electronics, laptops, and buildings, where materials could respond dynamically to overheating without external cooling systems.

“The difference in heat dissipation is similar to the tactile difference between touching plastic and touching marble,” Boriskina said in a media statement, highlighting how noticeable the effect can be.

The team is now working on optimising the polymer’s internal structure and exploring related materials that could produce even larger thermal shifts.

“If we can further enhance this effect, the industrial and societal impact could be substantial,” Boriskina said.

Researchers say advances in stretchable material heat conduction could significantly influence future designs of smart textiles, electronics cooling, and energy-efficient buildings.

The study has been published in the journal Advanced Materials. The authors include researchers from MIT and the Southern University of Science and Technology in China.

Researchers say advances in stretchable material heat conduction could significantly influence future designs of smart textiles, electronics cooling, and energy-efficient buildings.

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Space & Physics

Physicists Capture ‘Wakes’ Left by Quarks in the Universe’s First Liquid

Scientists at CERN’s Large Hadron Collider have observed, for the first time, fluid-like wakes created by quarks moving through quark–gluon plasma, offering direct evidence that the universe’s earliest matter behaved like a liquid rather than a cloud of free particles.

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Physicists Capture ‘Wakes’ Left by Quarks in the Universe’s First Liquid
Image credit: Jose-Luis Olivares, MIT

Physicists working at the CERN(The European Organization for Nuclear Research) have reported the first direct experimental evidence that quark–gluon plasma—the primordial matter that filled the universe moments after the Big Bang—behaves like a true liquid.

Using heavy-ion collisions at the Large Hadron Collider, researchers recreated the extreme conditions of the early universe and observed that quarks moving through this plasma generate wake-like patterns, similar to ripples trailing a duck across water.

The study, led by physicists from the Massachusetts Institute of Technology, shows that the quark–gluon plasma responds collectively, flowing and splashing rather than scattering randomly.

“It has been a long debate in our field, on whether the plasma should respond to a quark,” said Yen-Jie Lee in a media statement. “Now we see the plasma is incredibly dense, such that it is able to slow down a quark, and produces splashes and swirls like a liquid. So quark-gluon plasma really is a primordial soup.”

Quark–gluon plasma is believed to be the first liquid to have existed in the universe and the hottest ever observed, reaching temperatures of several trillion degrees Celsius. It is also considered a near-perfect liquid, flowing with almost no resistance.

To isolate the wake produced by a single quark, the team developed a new experimental technique. Instead of tracking pairs of quarks and antiquarks—whose effects can overlap—they identified rare collision events that produced a single quark traveling in the opposite direction of a Z boson. Because a Z boson interacts weakly with its surroundings, it acts as a clean marker, allowing scientists to attribute any observed plasma ripples solely to the quark.

“We have figured out a new technique that allows us to see the effects of a single quark in the QGP, through a different pair of particles,” Lee said.

Analysing data from around 13 billion heavy-ion collisions, the researchers identified roughly 2,000 Z-boson events. In these cases, they consistently observed fluid-like swirls in the plasma opposite to the Z boson’s direction—clear signatures of quark-induced wakes.

The results align with theoretical predictions made by MIT physicist Krishna Rajagopal, whose hybrid model suggested that quarks should drag plasma along as they move through it.

“This is something that many of us have argued must be there for a good many years, and that many experiments have looked for,” Rajagopal said.

“We’ve gained the first direct evidence that the quark indeed drags more plasma with it as it travels,” Lee added. “This will enable us to study the properties and behavior of this exotic fluid in unprecedented detail.”

The research was carried out by members of the CMS Collaboration using the Compact Muon Solenoid detector at CERN. The open-access study has been published in the journal Physics Letters B.

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