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Space & Physics

In search for red aurorae in ancient Japan

Ryuho Kataoka, a Japanese auroral scientist, played a seminal role in searching for evidence of super-geomagnetic storms in the past using historical methods

Karthik Vinod

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Professor Ryuho Kataoka in his office at NIPR, with the fan-shaped painting behind him, Picture courtesy: RK Works

Aurorae seen on Earth are the end of a complex process that begins with a violent, dynamic process deep within the sun’s interior.

However, studying the depths of the sun is no easy task, even for scientists. The best they can do is to observe the surface using space-based telescopes. One problem that scientists are attempting to solve is how a super-geomagnetic storm on Earth comes to being. These geomagnetic storms find their roots in sunspots, that are acne-like depressions on the sun’s surface. As the sun approaches the peak of its 11-year solar cycle, these sunspots, numbering in the hundreds, occasionally release all that stored magnetic energy into deep space, in the form of coronal mass ejections (CMEs) (which are hot wisps of gas superheated to thousands of degrees).

If the earth lies in the path of an oncoming CME, the energy release from their resultant magnetic field alignment can cause intense geomagnetic storms and aurorae on Earth.

This phenomenon, which is astrophysical and also electromagnetic in nature, can have serious repercussions for our modern technological society.

Super-geomagnetic storms, a particularly worse form of geomagnetic storm, can induce power surges in our infrastructure, causing power outages that can plunge the world into darkness, and can cause irreversible damages to our infrastructure. The last recorded super-geomagnetic storm event occurred more than 150 years ago. Known as the Carrington event, the storm destroyed telegraph lines across North America and Europe in 1859. The risk for a Carrington-class event to happen again was estimated to be 1 in 500-years, which is quite low, but based on limited data. Ramifications are extremely dangerous if it were to ever happen.

However, in the past decade, it was learnt that such super-geomagnetic storms are much more common than scientists had figured. To top it all, it wasn’t just science, but it was a valuable contribution by art – specifically ancient Japanese and Chinese historical records that shaped our modern understanding of super-geomagnetic storms.

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Ryuho Kataoka, a Japanese space physicist, played a seminal role in searching for evidence of super-geomagnetic storms in the past using historical methods. He is presently an associate professor in physics, holding positions at Japan’s National Institute of Polar Research, and The Graduate University for Advanced Studies.

“There is no modern digital dataset to identify extreme space weather events, particularly super-geomagnetic storms,” said Professor Kataoka. “If you have good enough data, we can input them into supercomputers to do physics-based simulation.”

However, sunspot records go until the late 18th century when sunspots were actively being cataloged. In an effort to fill the data gap, Professor Kataoka decided to be at the helm of a very new but promising interdisciplinary field combining the arts with space physics. “The data is limited by at least 50 years,” said Professor Kataoka. “So we decided to search for these red vapor events in Japanese history, and see the occurrence patterns … and if we are lucky enough, we can see detailed features in these lights, pictures or drawings.” Until the summer of 2015, Ryuho Kataoka wasn’t aware of how vast ancient Japanese and Chinese history records really were.

In the past 7 years, he’s researched a very specific red aurora, in documents extending to more than 1400 years. “Usually, auroras are known for their green colors – but during the geomagnetic storm, the situation is very different,” he said. “Red is of course unusual, but we can only see red during a powerful geomagnetic storm, especially in lower latitudes. From a scientific perspective, it’s a very reasonable way to search for red signs in historical documents.”

A vast part of these historical red aurora studies that Professor Kataoka researched came from literature explored in the last decade by the AURORA-4D collaboration. “The project title included “4D”, because we wanted to access records dating back 400 years back during the Edo period,” said Professor Kataoka.

“From the paintings, we can identify the latitude of the aurora, and calculate the magnitude or amplitude of the geomagnetic storm.” Clearly, paintings in the Edo period influenced Professor Kataoka’s line of research, for a copy of the fan-shaped red aurora painting from the manuscript Seikai (which translates to ‘stars’) hangs on the window behind his office desk at the National Institute of Polar Research.

The painting fascinated Professor Kataoka, since it depicted an aurora that originated during a super-geomagnetic storm over Kyoto in 1770. However, the painting did surprise him at first, since he wondered whether the radial patterns in the painting were real, or a mere artistic touch to make it look fierier. “That painting was special because this was the most detailed painting preserved in Japan,” remarked Professor Kataoka. “I took two years to study this, thinking this appearance was silly as an aurorae scientist. But when I calculated the field pattern from Kyoto towards the North, it was actually correct!”

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Fan-shaped red aurora painting from the ‘Seikai’, dated 17th September, 1770; Picture Courtesy: Matsusaka City, Mie Prefecture.

The possibility to examine and verify historical accounts using science is also a useful incentive for scholars of Japanese literature and scientists partaking in the research.

“This is important because, if we scientists look at the real National Treasure with our eyes, we really know these sightings recorded were real,” said Professor Kataoka. “The internet is really bad for a survey because it can easily be very fake,” he said laughing. It’s not just the nature in which science was used to examine art – to examine Japanese “national treasures” that is undoubtedly appealing, but historical accounts themselves have contributed to scientific research directly.

“From our studies, we can say that the Carrington class events are more frequent than we previously expected,” said Professor Kataoka. There was a sense of pride in him as he said this. “This Carrington event is not a 1 in 200-year event, but as frequent as 1 in 100 years.” Given how electricity is the lifeblood of the 21st century, these heightened odds do ingrain a rather dystopian society in the future, that is ravaged by a super-geomagnetic storm.

Professor Kataoka’s work has found attention within the space physics community. Jonathon Eastwood, Professor of Physics at Imperial College London said to EdPublica, “The idea to use historical information and art like this is very inventive because these events are so rare and so don’t exist as information in the standard scientific record.”

There’s no physical harm from a geomagnetic storm, but the threat to global power supply and electronics is being increasingly recognized by world governments. The UK, for instance, identified “space weather” as a natural hazard in its 2011 National Risk Register. In the years that followed, the government set up a space weather division in the Met Office, the UK’s foremost weather forecasting authority, to monitor and track occurrences of these coronal mass ejections. However, these forecasts, which often supplement American predictions – namely the National Oceanic and Atmospheric Administration (NOAA) – have failed to specify previously where a magnetic storm could brew on Earth, or predict whether a coronal mass ejection would ever actually strike the Earth.

The former occurred during the evacuation process for Hurricane Irma in 2017, when amateur radio ham operators experienced the effects of a radio blackout when a magnetic storm affected the communications network across the Caribbean. The latter occurred on another occasion when a rocket launch for SpaceX’s Starlink communication satellites was disrupted by a mild geomagnetic storm, costing SpaceX a loss of over $40 million.

Professor Kataoka said he wishes space physicists from other countries participate in similar interdisciplinary collaborations to explore their native culture’s historical records for red aurora sightings. He said the greatest limitation of the AURORA-4D collaboration was the lack of historical records from other parts of the world. China apparently boasts a history of aurora records longer than Japan, with a history lasting before Christ himself. “Being Japanese, I’m not familiar with British, Finnish or Vietnamese cultures,” said Professor Kataoka. “But every country has literature researchers and scientists who can easily collaborate and perform interdisciplinary research.” And by doing so, it’s not just science which benefits from it, but so is ancient art whose beauty and relevance gains longevity.

Space & Physics

When Quantum Rules Break: How Magnetism and Superconductivity May Finally Coexist

A new theoretical breakthrough from MIT suggests that exotic quantum particles known as anyons could reconcile a long-standing paradox in physics, opening a path to an entirely new form of superconductivity.

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When Quantum Rules Break: How Magnetism and Superconductivity May Finally Coexist
Image credit: Pawel Czerwinski/UnSplash

For decades, physicists believed that superconductivity and magnetism were fundamentally incompatible. Superconductivity is fragile: even a weak magnetic field can disrupt the delicate pairing of electrons that allows electrical current to flow without resistance. Magnetism, by its very nature, should destroy superconductivity.

And yet, in the past year, two independent experiments upended this assumption.

In two different quantum materials, researchers observed something that should not have existed at all: superconductivity and magnetism appearing side by side. One experiment involved rhombohedral graphene, while another focused on the layered crystal molybdenum ditelluride (MoTe₂). The findings stunned the condensed-matter physics community and reopened a fundamental question—how is this even possible?

Now, a new theoretical study from physicists at the Massachusetts Institute of Technology offers a compelling explanation. Writing in the Proceedings of the National Academy of Sciences, the researchers propose that under the right conditions, electrons in certain magnetic materials can split into fractional quasiparticles known as anyons—and that these anyons, rather than electrons, may be responsible for superconductivity.

If confirmed, the work would introduce a completely new form of superconductivity, one that survives magnetism and is driven by exotic quantum particles instead of ordinary electrons.

“Many more experiments are needed before one can declare victory,” said Senthil Todadri, William and Emma Rogers Professor of Physics at MIT, in a media statement. “But this theory is very promising and shows that there can be new ways in which the phenomenon of superconductivity can arise.”

A Quantum Contradiction Comes Alive

Superconductivity and magnetism are collective quantum states born from the behavior of electrons. In magnets, electrons align their spins, producing a macroscopic magnetic field. In superconductors, electrons pair up into so-called Cooper pairs, allowing current to flow without energy loss.

For decades, textbooks taught that the two states repel each other. But earlier this year, that belief cracked.

At MIT, physicist Long Ju and colleagues reported superconductivity coexisting with magnetism in rhombohedral graphene—four to five stacked graphene layers arranged in a specific crystal structure.

“It was electrifying,” Todadri recalled in a media statement. “It set the place alive. And it introduced more questions as to how this could be possible.”

Soon after, another team reported a similar duality in MoTe₂. Crucially, MoTe₂ also exhibits an exotic quantum phenomenon known as the fractional quantum anomalous Hall (FQAH) effect, in which electrons behave as if they split into fractions of themselves.

Those fractional entities are anyons.

Meet the Anyons: Where “Anything Goes”

Anyons occupy a strange middle ground in the quantum world. Unlike bosons, which happily clump together, or fermions, which avoid one another, anyons follow their own rules—and exist only in two-dimensional systems.

First predicted in the 1980s and named by MIT physicist Frank Wilczek, anyons earned their name as a playful nod to their unconventional behavior: anything goes.

Decades ago, theorists speculated that anyons might be able to superconduct in magnetic environments. But because superconductivity and magnetism were believed to be mutually exclusive, the idea was largely abandoned.

The recent MoTe₂ experiments changed that calculus.

“People knew that magnetism was usually needed to get anyons to superconduct,” Todadri said in a media statement. “But superconductivity and magnetism typically do not occur together. So then they discarded the idea.”

Now, Todadri and MIT graduate student Zhengyan Darius Shi, co-author of the study, revisited the old theory—armed with new experimental clues.

Using quantum field theory, the team modeled how electrons fractionalize in MoTe₂ under FQAH conditions. Their calculations revealed that electrons can split into anyons carrying either one-third or two-thirds of an electron’s charge.

That distinction turned out to be critical.

Anyons are notoriously “frustrated” particles—quantum effects prevent them from moving freely together.

“When you have anyons in the system, what happens is each anyon may try to move, but it’s frustrated by the presence of other anyons,” Todadri explained in a media statement. “This frustration happens even if the anyons are extremely far away from each other.”

But when the system is dominated by two-thirds-charge anyons, the frustration breaks down. Under these conditions, the anyons begin to move collectively—forming a supercurrent without resistance.

“These anyons break out of their frustration and can move without friction,” Todadri said. “The amazing thing is, this is an entirely different mechanism by which a superconductor can form.”

The team also predicts a distinctive experimental signature: swirling supercurrents that spontaneously emerge in random regions of the material—unlike anything seen in conventional superconductors.

Why This Matters Beyond Physics

If experiments confirm superconducting anyons, the implications could extend far beyond fundamental physics.

Because anyons are inherently robust against environmental disturbances, they are considered prime candidates for building stable quantum bits, or qubits—the foundation of future quantum computers.

“These theoretical ideas, if they pan out, could make this dream one tiny step within reach,” Todadri said.

More broadly, the work hints at an entirely new category of matter.

“If our anyon-based explanation is what is happening in MoTe₂, it opens the door to the study of a new kind of quantum matter which may be called ‘anyonic quantum matter,’” Todadri said. “This will be a new chapter in quantum physics.”

For now, the theory awaits experimental confirmation. But one thing is already clear: a rule long thought unbreakable in quantum physics may no longer hold—and the quantum world just became a little stranger, and far more exciting.

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From Qubits to Folk Puppetry: India’s Biggest Quantum Science Communication Conclave Wraps Up in Ahmedabad

From qubits to cultural storytelling, India’s biggest quantum science communication conclave in Ahmedabad showed how frontier science can meet people where they are. Through dialogue, demonstrations and folk art, the event reimagined how quantum knowledge reaches classrooms, communities and citizens.

Dipin Damodharan

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Dr P Bharati inaugurating the Quantum Communication Conference at Gujarat Science City

The Science Communication Conference on Public Understanding of Quantum Science & Technology, widely described as India’s biggest quantum conclave, concluded on 23 December 2025 at Gujarat Science City after two days of intensive discussions, demonstrations and public-facing engagement aimed at democratising quantum knowledge.

Organised by the Gujarat Council on Science and Technology (GUJCOST) under the Department of Science & Technology, Government of Gujarat, the conference was formally inaugurated on 22 December by P. Bharathi, IAS, Secretary, DST, in the presence of senior officials, scientists, science communicators and educators from India and abroad.

P. Bharathi stressed the need to make quantum education more accessible and to build stronger public engagement so citizens can relate to quantum ideas beyond labs and classrooms. She highlighted science communication as a key bridge between advanced research and society, especially for students and educators

The second day of the conclave featured the participation of Gujarat’s Minister for Science and Technology, Arjun Modhwadia, who addressed the gathering and chaired a special session on the quantum age and society’s collective future. Emphasising the state’s long-term vision, the Minister said Gujarat believes strongly in the democratisation of quantum science, asserting that advanced scientific knowledge must reach citizens, classrooms and communities rather than remain confined to elite research spaces.

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Minister Arjun Modhwadia participating in a special session on the quantum age and society’s collective future. Image credit: GUJCOST

The two-day conference brought together around 200 participants, featuring keynote lectures, panel discussions, hands-on demonstrations and research presentations focused on making complex quantum concepts accessible to non-specialist audiences. International perspectives were provided by Prof. Kanan Purakayastha (UK), Dr N. T. Lan from the Vietnam Institute of Science Information, and Prof. Anjana Singh of the Nepal Academy of Science and Technology, highlighting global challenges and best practices in public engagement with quantum science.

Dr. Narottam Sahoo, Advisor and Member Secretary, Gujarat Council on Science & Technology, Department of Science & Technology, Gujarat, lauded GUJCOST’s role in popularising science, saying, “GUJCOST has been playing an instrumental role in bringing science closer to society and making it accessible to all. We will further step up such initiatives and programmes. It is a proud acknowledgement that UNESCO recognised Gujarat as a partner in the year-long quantum celebrations.”

A dynamic demonstration session on the Hands-on Quantum Education Kit, led by Dr V. B. Kamble, former Director of Vigyan Prasar, ignited curiosity among participants. Learners explored practical quantum concepts through engaging, hands-on activities, making complex ideas easier to grasp. Such interactive learning experiences help strengthen scientific temperament and inspire the next generation of innovators.

Another distinctive highlight of the programme was a folk-science puppet show presented by Dr V. P. Singh and his team from the Indian Science Communication Society (ISCOS). Blending traditional performance art with scientific ideas, the show drew strong audience attention and demonstrated how indigenous cultural forms can be effectively used to communicate abstract quantum concepts. Dr Singh beautifully bridged farmers and frontier science through a folk puppet show demonstrating how traditional art forms can communicate cutting-edge scientific ideas.

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Folk-science puppet show presented by Dr V. P. Singh and his team. Image credit: Dipin Damodharan

Aligned with the International Year of Quantum Science & Technology (IYQST-2025) and India’s National Quantum Mission, the conclave underscored the growing importance of science communication in preparing society for the emerging quantum era. Organisers said the conference succeeded in bridging the gap between advanced research and public understanding, reinforcing Gujarat’s position as a key hub for science outreach and quantum literacy in India.

Sessions also included interactive workshops, young researcher presentations, and dialogues on science communication methods that bridge academic science and public curiosity — reinforcing Gujarat’s aim to demystify quantum science and bring it into everyday understanding.

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Space & Physics

Ancient Martian Valleys Reveal Gradual Climate Shift From Warm And Wet To Cold And Icy: Study

A new study led by researchers at IIT Bombay has provided fresh evidence showing how Mars gradually transitioned from a warm, water-rich planet to a cold, icy world

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Left: Mars. Credit: Kevin Gill/Wikimedia. Right: Thaumasia region of Mars. Credit: NASA/JPL/USGS

A new study led by researchers at IIT Bombay has provided fresh evidence showing how Mars gradually transitioned from a warm, water-rich planet to a cold, icy world, by analysing ancient valley networks in the Thaumasian Highlands region of the Red Planet.

The findings, based on high-resolution orbital data, suggest that Mars experienced a long-term climate shift—from surface water-driven erosion during the Noachian period around four billion years ago to increasingly glacial and frozen conditions by the Hesperian period, roughly three billion years ago.

“Both these planets started with similar compositions and atmospheres. So, one of the most pressing questions is, where did all that water go, and why didn’t Mars evolve along the same direction as Earth? So, we wanted to find at what stage it lost its water,” said Alok Porwal of IIT Bombay in a statement issued by the institute.

Tracking Mars’ changing climate

The research focused on the Thaumasia Highlands, one of Mars’ most ancient geological regions, which stretches from the equator toward higher latitudes. According to the researchers, this makes it an ideal natural laboratory to study climate-driven geological changes over time.

“The Thaumasia Highlands is a region somewhat like the Indian subcontinent. It extends from the equator to higher latitudes, so it has a range of climates and geographies. It also has both very ancient geologic formations and more recent features, which gives an overall view of the planet,” Porwal said.

The team analysed more than 150 complex valley networks using datasets from NASA’s Context Camera (CTX) and Mars Orbiter Laser Altimeter (MOLA), the European Space Agency’s High Resolution Stereo Camera (HRSC), and ISRO’s Mars Orbiter Camera aboard the Mangalyaan mission. Each valley was carefully mapped to minimise errors caused by natural topographic variations.

Water-carved valleys to ice-shaped terrain

The researchers examined both qualitative and quantitative indicators to identify whether valleys were shaped by flowing water or glacial ice. Features such as fan-shaped sediment deposits and branching valley patterns pointed to fluvial erosion, while moraine-like formations, viscous flow features and ribbed terrain indicated glacial processes.

“When water is flowing, it carries heavy materials at the bottom and cuts the ground vertically. So, the shape it carves is more of a V-shaped valley. Glaciers, which have a mix of ice and debris, are heavier. When they move, they slide over the surface and create a U-shaped valley,” said Dibyendu Ghosh, the study’s first author, in the IIT Bombay statement.

Another key parameter was the angle at which valleys merge.

“When water is flowing, it follows the slope, so two valleys will flow parallel to each other and meet at an acute angle. Glaciers can move laterally, so the angles become more obtuse,” Ghosh explained.

The analysis showed that low-latitude valleys near the Martian equator were primarily shaped by flowing surface water, indicating warmer climatic conditions. In contrast, valleys at higher latitudes displayed increasing signs of fluvioglacial activity, suggesting a colder environment where ice played a growing role.

Evidence of frozen subsurface water

The study also supports the idea that much of Mars’ surface water gradually retreated underground as the planet cooled.

According to the researchers, valley formation peaked during the Noachian period between 4.1 and 3.7 billion years ago, declined during the transition to the Hesperian, and later showed stronger signatures of glacial modification and groundwater erosion.

Future exploration

While the findings offer a more coherent picture of Mars’ climatic evolution, the team noted that linking valley networks precisely to subsurface structures and geological timelines remains challenging.

Looking ahead, Porwal emphasised the need for more advanced missions to refine the planet’s climate history. “If I had a chance to suggest (for a future Mars mission), I would recommend a lander to get more geophysical data. And an orbiter with high-resolution imaging and infrared imaging capabilities to thoroughly study its geological history,” he said.

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