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Space & Physics

Chandrayaan-3: The moon may have had a fiery past

A magma ocean might’ve wrapped the ancient moon, suggests findings from India’s robotic lunar mission, Chandrayaan-3.

Karthik Vinod

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The earth's moon. Credit: Ed Publica

On 23rd August last year, India’s Chandrayaan-3 made history being the first to soft-land on the moon’s south polar region. The landing marked the end of the high-octane phase of the mission. But its next phase was a slow-burner.

Pragyan, the suitcase-sized rover, that hitched a ride to the moon aboard the lander, Vikram, rolled off a ramp onto the lunar surface. It traversed along the dusty lunar surface slowly, at a pace even a snail could beat. Handlers at the Indian Space Research Organization (ISRO) didn’t want the suitcase-sized rover to risk stumbling over a rock or near a ridge, and jeopardize the mission.

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The whitish spots are material excavated from the moon’s interior.

Nevertheless, the rover had a busy schedule to stick to. It was to probe the lunar soil, and relay that scientific data back to earth. Pragyan covered 100 meters in two weeks, before it stopped to take a nap ahead of a long lunar night. At the time, the rover’s battery pack was fully charged, thanks to the on-board solar panels soaking up sunlight during the day.

But lunar weather is harsh, especially at the south pole, where Pragyan napped, temperatures can reach as low as -250 degrees centigrade during the night. Added to that, a lunar night lasts two weeks. ISRO deemed Pragyan had only a 1% chance to survive.

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Later, the expected happened, when the rover went unresponsive to ISRO’s pings to wake up.

But ISRO said the rover achieved what it was tasked to do. It relayed data all along for two weeks, examining soil from some 23 locations around the mission’s landing point, Statio Shiv Shakti. As months passed by, a slew of discoveries were made. Sulphur was discovered at the south pole, early on while the mission was ongoing. And only a few months ago, Pragyan found evidence of past weathering activity at the south pole.

But since August this year, research teams from ISRO and the Physical Research Laboratory in Ahmedabad, India, reported Pragyan’s most important findings yet – one of which sheds light onto the moon’s origins.

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Chandrayaan-3’s Vikram lander, seen from the Pragyan rover’s camera

Chandrayaan-3 had carried a radioactive passenger to the moon’s surface – curium-244.

The radioactive curium helps lase the surface: firing alpha particles (which are helium nuclei) at the dusty terrain. Some of these alpha particles bounce off the dust, whereas others evict electrons from the lunar soil, thereby producing x-ray emissions. Keeping watch is the Alpha Particle X-ray Spectrometer (APXS) on-board the Pragyan rover. In August, PRL scientists published findings in the journal, Nature, based on APXS data, reporting discovery of ferroan anorthosite.

It wasn’t the first ever detection per se of ferroan anorthosite. In fact, Apollo 11 had brought back anorthosite rocks to earth, where they were identified as such. That was in 1969, and Apollo sampled them from the equator. Successive missions by the Soviet Union and most recently China affirmed likewise from mid-latitude – equatorial regions as well. But Pragyan’s detection of the rock type was the first ever from the polar region.

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The Pragyan rover’s payload.

Anorthosites are common on earth. In fact, just a year after the Apollo 11 sampled the rock, scientists had evidence of the earth and the moon’s entangled history. The authors noted the similar composition between these rocks, that are geographically widespread. Furthermore, ferroan anorthosite is an igneous rock that forms on earth when hot lava produced in volcanic eruptions cools down.

And scientists had piled up evidence in support of a similar process that underwent on the moon. The anorthosite rocks on the moon are old, in fact, more than 4 billion years ago – a figure close to the earth’s inception with rest of the solar system – around 4.5 billion years. Scientific consensus has been that the moon was formed from remnants of a collision between the early earth and a rogue Mars-sized planetary body.

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But the collision energy would have yielded a moon that was molten. A lava blanketing the surface – aka a global magma ocean. As this ocean cooled, minerals amongst which is plagioclase (a class of feldspar) crystallized and formed the anorthosite rocks on the moon. It’s commonly called the lunar magma ocean hypothesis.

When Pragyan treaded over the dusty lunar terrain, it didn’t register the anorthosite as a physical rock per se. Instead, it observed remnants of the rock, as fine powder.

Meteorites beat down rocks to fine powder, as they slam into the moon from space with regular impunity. On earth, the ground is saved by the presence of an atmosphere. But the moon virtually has no atmosphere. Nor does it have water to wear down the rocks. The surface is extremely hot during the lunar day – in fact, when Chandrayaan-3 landed on the moon, the surface temperature was some 50 degrees centigrade. Just a few months ago, Pragyan revealed possible signs of rock degradation from the rims of a crater.

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Moon dust opens doors to the past

The fact the moon doesn’t (and can’t) sustain an atmosphere helps it make an attractive destination to learn more about our planet and the satellite’s shared origins. There’s no chemistry to remove traces of the moon’s early evolution from the lunar dust. As such, the dust opens doors to the past.

Space explorations missions soft-landing on the surface study this dust – or sample and shuttle them to earth for scientists to study them in detail.

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In fact, Pragyan revealed a crater that’s amongst the oldest ever discovered on the moon. The findings were published in the journal, Icarus, in September. Hidden in plain sight, the rover’s navigation camera, NavCam, spotted subtle stretch marks on the surface, that were confirmed later with the Chandrayaan-2 orbiter (which has been orbiting the moon since 2019). In fact, this crater was found buried under nearby craters, most notably the South Pole-Aitkin basin located 350 km away. The basin is the largest impact crater in the entire solar system (some 2,500 km wide and 8 km deep) touted to have formed millions of years ago.

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And this became subject to an earlier paper that PRL scientists authored, and was published in August. Pragyan identified material thought to have emerged from the moon’s interior. The APXS instrument picked up unusually high magnesium content in the vicinity. The authors speculate the meteorite that created the basin probably dug up magnesium from deep inside the moon’s upper mantle, and spewed them into Pragyan’s vicinity. 

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But some experts believe in an alternate explanation. They believe the magnesium might have come from surface rocks in the vicinity, and not from the upper mantle. In fact, the authors acknowledged this amongst other possible alternatives. Nonetheless, the Chandrayaan-3’s findings doesn’t dispute the lunar magma ocean hypothesis either, if not backing it outright. Saying that, the theory lives on to fight another day.

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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