Space & Physics
Dr. Nikku Madhusudhan Brings Us Closer to Finding Life Beyond Earth
Dr. Madhusudhan, a leading Indian-British astrophysicist at the University of Cambridge, has long been on the frontlines of the search for extraterrestrial life
Somewhere in the vast, cold dark of the cosmos, a planet orbits a distant star. It’s not a place you’d expect to find life—but if Dr. Nikku Madhusudhan is right, that assumption may soon be history.
Dr. Madhusudhan, a leading Indian-British astrophysicist at the University of Cambridge, has long been on the frontlines of the search for extraterrestrial life or what we call the alien life. This month, his team made headlines around the world after revealing what could be the strongest evidence yet of life beyond Earth—on a distant exoplanet known as K2-18b.
Using data from NASA’s James Webb Space Telescope, Madhusudhan and his collaborators detected atmospheric signatures of molecules commonly associated with biological processes on Earth—specifically, gases produced by marine phytoplankton and certain bacteria. Their analysis suggests a staggering 99.7% probability that these molecules could be linked to living organisms.
“This marked the first detection of carbon-bearing molecules in the atmosphere of an exoplanet located within the habitable zone,” the University of Cambridge said in a press statement. “The findings align with theoretical models of a ‘Hycean’ planet — a potentially habitable, ocean-covered world enveloped by a hydrogen-rich atmosphere.”
Born in India, Dr. Madhusudhan began his journey in science with an engineering degree from IIT (BHU) Varanasi
In addition, a fainter signal suggested there could be other unexplained processes occurring on K2-18b. “We didn’t know for sure whether the signal we saw last time was due to DMS, but just the hint of it was exciting enough for us to have another look with JWST using a different instrument,” said Professor Nikku Madhusudhan in a news report released by the University of Cambridge.
The man behind the mission
Born in India, Dr. Madhusudhan began his journey in science with an engineering degree from IIT (BHU) Varanasi. But it was during his time at the Massachusetts Institute of Technology (MIT), under the mentorship of exoplanet pioneer Prof. Sara Seager, that he found his calling. His doctoral work—developing methods to retrieve data from exoplanet atmospheres—would go on to form the backbone of much of today’s planetary climate modeling.
Now a professor at the University of Cambridge’s Institute of Astronomy, Madhusudhan leads research that straddles the line between science fiction and frontier science.
A Universe of Firsts
Over the years, his work has broken new ground in our understanding of alien worlds. He was among the first to suggest the concept of “Hycean planets”—oceans of liquid water beneath hydrogen-rich atmospheres, conditions which may be ideal for life. He also led the detection of titanium oxide in the atmosphere of WASP-19b and pioneered studies of K2-18b, the same exoplanet now back in the spotlight.
His team’s recent findings on K2-18b may be the closest humanity has ever come to detecting life elsewhere in the universe.
Accolades and impact
Madhusudhan’s contributions have earned him global recognition. He received the prestigious IUPAP Young Scientist Medal in 2016 and the MERAC Prize in Theoretical Astrophysics in 2019. In 2014, the Astronomical Society of India awarded him the Vainu Bappu Gold Medal for outstanding contributions to astrophysics by a scientist under 35.
But for Madhusudhan, the real reward lies in the questions that remain unanswered.
Looking ahead
Madhusudhan cautions that, while the findings are promising, more data is needed before drawing conclusions about the presence of life on another planet. He remains cautiously optimistic but notes that the observations on K2-18b could also be explained by previously unknown chemical processes. Together with his colleagues, he plans to pursue further theoretical and experimental studies to investigate whether compounds like DMS and DMDS could be produced through non-biological means at the levels currently detected.
Beyond the lab, Madhusudhan remains dedicated to mentoring students and advancing scientific outreach. He’s a firm believer that the next big discovery might come from a student inspired by the stars, just as he once was.
As scientists prepare for the next wave of data and the world watches closely, one thing is clear: thanks to minds like Dr. Nikku Madhusudhan’s, the search for life beyond Earth is no longer a distant dream—it’s a scientific reality within reach.
Space & Physics
MIT Pioneers Real-Time Observation of Unconventional Superconductivity in Magic-Angle Graphene
Physicists have directly observed unconventional superconductivity in magic-angle twisted tri-layer graphene using a new experimental platform, revealing a unique pairing mechanism
MIT physicists have unveiled compelling direct evidence for unconventional superconductivity in “magic-angle” twisted tri-layer graphene—an atomically engineered material that could reimagine the future of energy transport and quantum technologies. Their new experiment marks a pivotal step forward, offering a fresh perspective on how electrons synchronize in precisely stacked two-dimensional materials, potentially laying the groundwork for next-generation superconductors that function well above current temperature limits.
Instead of looking merely at theoretical possibilities, the MIT team built a novel platform that lets researchers visualize the superconducting gap “as it emerges in real-time within 2D materials,” said co-lead author Shuwen Sun in a media statement. This gap is crucial, reflecting how robust the material’s superconducting state is during temperature changes—a key indicator for practical applications.
What’s striking, said Jeong Min Park, study co-lead author, is that the superconducting gap in magic-angle graphene differs starkly from the smooth, uniform profile seen in conventional superconductors. “We observed a V-shaped gap that reveals an entirely new pairing mechanism—possibly driven by the electrons themselves, rather than crystal vibrations,” Park said. Such direct measurement is a “first” for the field, giving scientists a more refined tool for identifying and understanding unconventional superconductivity.
Senior author Pablo Jarillo-Herrero emphasized that their method could help crack the code behind room-temperature superconductors: “This breakthrough may trigger deeper insights not just for graphene, but for the entire class of twistronic materials. Imagine grids and quantum computers that operate with zero energy loss—this is the holy grail we’re moving toward,” Jarillo-Herrero said in the MIT release.
Collaborators included scientists from Japan’s National Institute for Materials Science, broadening the impact of the research. The discovery builds on years of progress since the first magic-angle graphene experiments in 2018, opening what many now call the “twistronics” era—a field driven by stacking and twisting atom-thin materials to unlock uniquely quantum properties.
Looking ahead, the team plans to expand its analysis to other ultra-thin structures, hoping to map out electronic behavior not only for superconductors, but for a wider range of correlated quantum phases. “We can now directly observe electron pairs compete and coexist with other quantum states—this could allow us to design new materials from the ground up,” said Park in her public statement.
The research underscores the value of visualization in fundamental physics, suggesting that direct observation may be the missing link to controlling quantum phenomena for efficient, room-temperature technology.
Space & Physics
Atoms Speak Out: Physicists Use Electrons as Messengers to Unlock Secrets of the Nucleus
Physicists at MIT have devised a table-top method to peer inside an atom’s nucleus using the atom’s own electrons
Physicists at MIT have developed a pioneering method to look inside an atom’s nucleus — using the atom’s own electrons as tiny messengers within molecules rather than massive particle accelerators.
In a study published in science, the researchers demonstrated this approach using molecules of radium monofluoride, which pair a radioactive radium atom with a fluoride atom. The molecules act like miniature laboratories where electrons naturally experience extremely strong electric fields. Under these conditions, some electrons briefly penetrate the radium nucleus, interacting directly with protons and neutrons inside. This rare intrusion leaves behind a measurable energy shift, allowing scientists to infer details about the nucleus’ internal structure.
The team observed that these energy shifts, though minute — about one millionth of the energy of a laser photon — provide unambiguous evidence of interactions occurring inside the nucleus rather than outside it. “We now have proof that we can sample inside the nucleus,” said Ronald Fernando Garcia Ruiz, the Thomas A. Franck Associate Professor of Physics at MIT, in a statement. “It’s like being able to measure a battery’s electric field. People can measure its field outside, but to measure inside the battery is far more challenging. And that’s what we can do now.”
Traditionally, exploring nuclear interiors required kilometer-long particle accelerators to smash high-speed beams of electrons into targets. The MIT technique, by contrast, achieves similar insight with a table-top molecular setup. It makes use of the molecule’s natural electric environment to magnify these subtle interactions.
The radium nucleus, unlike most which are spherical, has an asymmetric “pear” shape that makes it a powerful system for studying violations of fundamental physical symmetries — phenomena that could help explain why the universe contains far more matter than antimatter. “The radium nucleus is predicted to be an amplifier of this symmetry breaking, because its nucleus is asymmetric in charge and mass, which is quite unusual,” Garcia Ruiz explained.
To conduct their experiments, the researchers produced radium monofluoride molecules at CERN’s Collinear Resonance Ionization Spectroscopy (CRIS) facility, trapped and cooled them in laser-guided chambers, and then measured laser-induced energy transitions with extreme precision. The work involved MIT physicists Shane Wilkins, Silviu-Marian Udrescu, and Alex Brinson, alongside international collaborators.
“Radium is naturally radioactive, with a short lifetime, and we can currently only produce radium monofluoride molecules in tiny quantities,” said Wilkins. “We therefore need incredibly sensitive techniques to be able to measure them.”
As Udrescu added, “When you put this radioactive atom inside of a molecule, the internal electric field that its electrons experience is orders of magnitude larger compared to the fields we can produce and apply in a lab. In a way, the molecule acts like a giant particle collider and gives us a better chance to probe the radium’s nucleus.”
Going forward, the MIT team aims to cool and align these molecules so that the orientation of their pear-shaped nuclei can be controlled for even more detailed mapping. “Radium-containing molecules are predicted to be exceptionally sensitive systems in which to search for violations of the fundamental symmetries of nature,” Garcia Ruiz said. “We now have a way to carry out that search”
Space & Physics
Physicists Double Precision of Optical Atomic Clocks with New Laser Technique
MIT researchers develop a quantum-enhanced method that doubles the precision and stability of optical atomic clocks, paving the way for portable, ultra-accurate timekeeping.
MIT physicists have unveiled a new technique that could significantly improve the precision and stability of next-generation optical atomic clocks, devices that underpin everything from mobile transactions to navigation apps. In a recent media statement, the MIT team explained: “Every time you check the time on your phone, make an online transaction, or use a navigation app, you are depending on the precision of atomic clocks. An atomic clock keeps time by relying on the ‘ticks’ of atoms as they naturally oscillate at rock-steady frequencies.”
Current atomic clocks rely on cesium atoms tracked with lasers at microwave frequencies, but scientists are advancing to clocks based on faster-ticking atoms like ytterbium, which can be tracked with lasers at higher, optical frequencies and discern intervals up to 100 trillion times per second.
A research group at MIT, led by Vladan Vuletić, the Lester Wolfe Professor of Physics, detailed that their newly developed method harnesses a laser-induced “global phase” in ytterbium atoms and boosts this effect using quantum amplification. Vuletić stated, “We think our method can help make these clocks transportable and deployable to where they’re needed.” The approach, called global phase spectroscopy, doubles the precision of an optical atomic clock, enabling it to resolve twice as many ticks per second compared to standard setups, and promises further gains with increasing atom counts.
The technique could pave the way for portable optical atomic clocks able to measure all manner of phenomena in various locations. Vuletić summarized the broader scientific ambitions: “With these clocks, people are trying to detect dark matter and dark energy, and test whether there really are just four fundamental forces, and even to see if these clocks can predict earthquakes.”
The MIT team has previously demonstrated improved clock precision by quantumly entangling hundreds of ytterbium atoms and using time reversal tricks to amplify their signals. Their latest advance applies these methods to much faster optical frequencies, where stabilizing the clock laser has always been a major challenge. “When you have atoms that tick 100 trillion times per second, that’s 10,000 times faster than the frequency of microwaves,” said Vuletić in the statement. Their experiments revealed a surprisingly useful “global phase” information about the laser frequency, previously thought irrelevant, unlocking the potential for even greater accuracy.
The research, led by Vuletić and joined by Leon Zaporski, Qi Liu, Gustavo Velez, Matthew Radzihovsky, Zeyang Li, Simone Colombo, and Edwin Pedrozo-Peñafiel of the MIT-Harvard Center for Ultracold Atoms, was published in Nature. They believe the technical benefits of the new method will make atomic clocks easier to run and enable stable, transportable clocks fit for future scientific exploration, including earthquake prediction, fundamental physics, and global time standards.
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