Space & Physics
M P Parameswaran: The Scientist Who Took Science to the People
M. P. Parameswaran, who died aged 91 on August 11, 2026, spent decades taking science beyond laboratories through KSSP, Malayalam science writing, literacy campaigns and environmental activism.
M P Parameswaran, who died on 11 August 2026 at the age of 91, spent his life trying to close the distance between scientific knowledge and the people it was meant to serve. Trained as a nuclear engineer, he walked away from India’s atomic establishment in 1975 to build one of the country’s most influential people’s science movements from the ground up.
He leaves behind an unusual body of work spanning nuclear science, science writing, literacy, language technology, environmental activism, rural development and political thought.
What connected these seemingly disparate pursuits was a single conviction: science should not remain confined to experts. Scientific knowledge, he argued through his work, had to become accessible enough for ordinary people to understand, question and participate in decisions affecting their lives.
From Nuclear Science to People’s Science
Parameswaran was born on 18 January 1935 in Kiralur (Kiraloor), a village in Thrissur district then part of the princely state of Cochin. He graduated in electrical engineering from the College of Engineering, Thiruvananthapuram, in 1956, before travelling to the Soviet Union, where he earned a doctorate in nuclear engineering from the Moscow Power Engineering Institute in 1965. He joined the Bhabha Atomic Research Centre (BARC), India’s premier nuclear research institution, in 1957 and remained there until 1975 — becoming part of the scientific establishment building the foundations of India’s nuclear programme.
But the work that made him a public intellectual began when he left the laboratory.
In 1975, Parameswaran resigned from BARC and joined the Kerala Sasthra Sahithya Parishad (KSSP). The move changed the direction of his life. KSSP had begun as a forum of science writers but evolved, with Parameswaran among its central figures, into a much broader people’s science movement. Under his involvement, science communication became connected with literacy, health, environment, technology and development.
He helped take science out of laboratories and classrooms and into public spaces — through books, magazines, campaigns, village meetings and travelling programmes.
Language was Central to This Effort
Parameswaran wrote extensively in Malayalam, Kerala’s regional language, producing popular science books and hundreds of articles on subjects including nuclear science, astronomy, mathematics, ecology and social science. His contribution was not simply to translate scientific concepts; he helped establish Malayalam as a language in which scientific ideas could be discussed with a wider public.
His interest in accessibility even extended to technology itself. Between 1969 and 1973, while on deputation from BARC, he served as Assistant Director of the State Institute of Languages in Kerala. During this period he was involved in developing a Malayalam keyboard layout for typewriters — work later associated with the development of the INSCRIPT keyboard layout used in Indian-language computing today.
It was a small but revealing example of his approach: technology had little value if people could not use it.
Building a National People’s Science Movement
Parameswaran’s contribution went beyond writing. He played a major role in taking the people’s science movement beyond Kerala. In 1987, as convener of the National Organising Committee, he was central to the Bharat Jan Vigyan Jatha, a nationwide science communication campaign that took scientific ideas to communities rather than waiting for audiences to come to scientific institutions. He was also instrumental in establishing the All India People’s Science Network, bringing together people’s science organisations from across the country.
These initiatives changed the scale of science communication. It became not merely the work of individual writers explaining discoveries, but an organised effort to build public engagement with science.
Literacy As Participation
The same philosophy shaped Parameswaran’s work in literacy. He played an important role in the Total Literacy Campaign in Ernakulam, in which KSSP worked with the district administration to take literacy beyond conventional classroom structures. The experience later became an important model for India’s national literacy campaign.
In 1990, he was also instrumental in organising the Bharat Gyan Vigyan Jatha in support of the National Literacy Mission, a movement that eventually contributed to the formation of the Bharat Gyan Vigyan Samiti.
For Parameswaran, literacy and scientific awareness were closely related. Knowing how to read was only the beginning; people also needed the ability to examine information, weigh evidence and participate in public decisions.
When Science Met Development
Parameswaran’s questions became more difficult when he began examining the consequences of technology itself. He increasingly focused on appropriate technology, rural development, decentralisation and environmental sustainability, and was associated with the Integrated Rural Technology Centre.
He was also a central figure in two of Kerala’s defining environmental campaigns: the movement against the Silent Valley hydroelectric project, which helped save one of India’s last untouched rainforests, and the later opposition to the Athirappilly hydroelectric project. Both battles shaped his conviction that development decisions could not be left to engineers and planners alone.
The Bhopal gas disaster of 1984 sharpened these concerns further. It demonstrated that scientific and industrial advances could produce enormous social and environmental risks when technological decisions were made without adequate attention to safety and public accountability. For Parameswaran and the people’s science movement, the lesson was not to reject science or technology but to ask harder questions about their use: Who benefits? Who bears the risks? And who gets to decide?
Questioning the Idea of Progress
His intellectual journey eventually took him beyond science communication into a broader critique of development. In his book Fourth World: Dream and Reality, Parameswaran set out an alternative model built around decentralisation, ecological sustainability, democracy and a critique of consumerism. The “Fourth World” thesis brought him into sustained conflict with the Communist Party of India (Marxist), or CPI(M), to which he had long belonged, and ultimately led to his expulsion from the party.
His political conclusions remain a subject of debate. But they reveal an important feature of his intellectual life: he was willing to question established ideas of progress, including those within his own political tradition. He later reflected on that journey — from young engineer in Moscow to nuclear scientist, people’s science activist and Marxist theorist who found himself outside the party he had served for decades — in his Malayalam autobiography, Kaalaharanamillatha Swapnangal (Timeless Dreams).
For Parameswaran, development could not simply be measured by economic growth or technological advancement. It also had to be judged by its effects on people, communities and the environment.
Recognition
Parameswaran’s writing and activism were recognised early and late in his career. He received the Books for Neoliterates Award in 1962, the Basic and Cultural Literature Award in 1964, and the Children’s Literature Award in 1984. In 2022, the Government of Kerala honoured him with the Kerala Sree Award, the state’s third-highest civilian award, for his lifetime contribution to science and society.
Science Without Silos
Parameswaran’s contributions are spread across several fields. He helped build KSSP into one of India’s most influential people’s science movements. He helped establish national networks for science communication. He wrote extensively in Malayalam and brought scientific subjects into public discourse. He contributed to language technology. He played important roles in literacy campaigns that reached far beyond Kerala. He helped shape landmark environmental struggles. And he became a prominent critic of environmentally and socially unsustainable models of progress.
But reducing his legacy to this list would miss what made these contributions part of the same story. Parameswaran did not see science as a body of knowledge that moved in one direction — from laboratories to the public. He saw it as something that should enable people to participate. That is why his career could move so naturally from nuclear research to Malayalam publishing, from science campaigns to literacy, and from technology to questions of ecology and democracy.
His relevance may be even clearer today. Artificial intelligence, biotechnology, climate change, nuclear energy and public health increasingly shape everyday decisions, while the knowledge needed to understand them often remains concentrated among specialists. Parameswaran spent much of his life trying to narrow that distance.
He began by working with some of India’s most sophisticated scientific technologies. He ended up devoting his life to a more fundamental question: how can scientific knowledge become part of public life without losing its rigour — and without leaving the public behind? His answer was not simply to popularise science. It was to make people participants in it.
Space & Physics
Indian-Belgian Team Develops Portable Detectors to Image Mountains and Monuments Using Cosmic Rays
Portable cosmic-ray detectors could help researchers examine mountains, tunnels and historical monuments without invasive procedures, opening new possibilities for scientific imaging and infrastructure inspection.
An international team of researchers from India and Belgium has developed portable particle detectors that could help scientists examine the interiors of mountains, tunnels and historical monuments without damaging them. The technology uses naturally occurring cosmic-ray particles to map variations in the density of objects, offering a potential approach to non-invasive imaging of large structures.
The detectors, developed using glass-based Resistive Plate Chambers (RPCs), achieved a particle-detection efficiency exceeding 95% during testing, according to a report published by Research Matters on October 24, 2026. The findings demonstrate the potential of compact detector systems to investigate dense materials and support future applications in geology, archaeology and infrastructure assessment.
The collaboration includes researchers from India’s National Institute of Science Education and Research (NISER), Bhubaneswar, and the Homi Bhabha National Institute (HBNI), alongside researchers from Belgian institutions, including Université catholique de Louvain and the Inter-University Institute for High Energies.
How cosmic rays reveal hidden structures
The technology uses muons, high-energy particles produced when cosmic rays interact with Earth’s atmosphere. These particles continuously reach the Earth’s surface and can penetrate substantial thicknesses of rock, concrete and other materials.
As muons travel through an object, some are absorbed or deflected depending on its density and thickness. By measuring the number and trajectories of particles passing through a structure, researchers can identify variations in internal density and reconstruct images of otherwise inaccessible areas.
The technique, known as muography, is comparable in principle to X-ray imaging, but uses naturally occurring particles instead of an artificial radiation source. It has previously been used to investigate geological formations, including volcanoes, and to explore archaeological structures.
However, conventional muon detectors can be bulky, difficult to transport and challenging to operate in remote locations. The new glass-based detectors aim to address some of these limitations through a compact design and sealed operation, reducing dependence on continuous gas supplies.
Testing the detector system
The researchers developed three glass RPC prototypes using thin glass electrodes separated by gas-filled gaps. When a muon passes through a chamber, it ionises the gas, generating an electrical signal that can be recorded to determine the particle’s position.
Electronic readout systems capture these signals and help reconstruct the trajectories of incoming particles. During testing, the detectors achieved an efficiency exceeding 95%, with a timing resolution of approximately 1.8 nanoseconds, according to the research report.
To examine the system’s ability to detect dense materials, the team conducted an absorption experiment using one prototype. During an open-sky measurement, researchers recorded nearly 55,000 muon tracks. After placing a lead block in the experimental setup, the recorded count fell to 30,894, demonstrating how dense material reduced the number of particles reaching the detector.
Representational image.Image credit:Pexels
The experiment provided proof of principle that the system could measure muon attenuation and support radiographic imaging. However, imaging complex structures such as mountains or monuments requires measurements from multiple directions and further computational reconstruction.
Applications and challenges ahead
Portable muon detectors could eventually help researchers investigate hidden cavities, examine geological formations, inspect tunnels and study the internal structures of historical monuments. Engineers could also explore their application in assessing infrastructure such as dams and bridges, although these uses would require additional testing and validation.
For cultural heritage conservation, muography could offer a valuable alternative where drilling or other invasive investigations risk damaging fragile structures. A 2025 review published in iScience highlighted the technique’s potential as a complementary, non-destructive method for studying cultural heritage objects, while noting that the relatively low flux of naturally occurring muons can require lengthy data-collection periods.
The technology is not yet a universal replacement for existing inspection methods. Its practical application will depend on factors such as spatial resolution, detector size, measurement duration and the complexity of the structure being examined.
The researchers have proposed further improvements, including lighter structural materials, larger detector areas and enhanced readout systems. These developments could make the detectors easier to deploy and improve the quality of reconstructed images.
Space & Physics
How Scientists Traced the Flow of Matter Around a Dead Star Using X-rays
By studying changes in X-ray signals from Centaurus X-3, researchers at Bengaluru’s Raman Research Institute have found evidence of an unusual way in which matter reaches a neutron star. The discovery could change how scientists explain the radiation coming from this distant system.
When a massive star dies, its core can collapse into an extremely dense object called a neutron star. Despite being only about the size of a city, it can have a mass comparable to that of the Sun. Its powerful gravity can pull matter away from a nearby companion star, releasing energy in the form of X-rays as the material falls towards it.
Scientists at Bengaluru’s Raman Research Institute (RRI) have studied these X-ray signals from Centaurus X-3, a star system about 24,000 light-years from Earth. By examining changes in the signals, the researchers identified a stream of matter flowing towards the neutron star and found evidence of a rotating disk of material around it. This is an unusual finding because such disks are not commonly expected in this type of star system. The discovery could help scientists better understand how matter moves around neutron stars and how these distant objects produce X-rays.
Star That Pulls in Matter
Centaurus X-3 is in the constellation Centaurus. It belongs to a class of systems known as high-mass X-ray binaries. These systems contain a neutron star and a massive companion star held together by gravity.
A neutron star forms when the core of a massive star collapses at the end of its life. It packs roughly the Sun’s mass into a sphere only about the size of a city. Its gravity is so strong that it can pull in material from a nearby companion star. As this material falls towards the neutron star, it releases enormous amounts of energy, including X-rays. Scientists study this radiation to understand how the material behaves and how the system works.
Centaurus X-3 is also a pulsar. Its neutron star rotates and sends out radiation from regions near its magnetic poles. As the star spins, these beams sweep across space. When a beam passes an observing satellite, the satellite detects a pulse of radiation, much as a lighthouse produces a repeating flash as it turns. These regular pulses provide scientists with a way to study the neutron star and its surroundings.
What the Changing Signals Revealed
The radiation from Centaurus X-3 does not come only from the neutron star itself. Some of it interacts with nearby material, including the surface of the companion star, gas flowing away from it and matter surrounding the neutron star. This material absorbs radiation and emits it again. Scientists call this secondary radiation.
Changes in this radiation can help researchers work out what is happening around the neutron star. However, Centaurus X-3 is so far away that telescopes cannot clearly distinguish its surrounding structures. It appears as a single point of light. Scientists must therefore piece together the system’s structure from the signals they receive.
Earlier observations had shown that the intensity of certain secondary X-ray emission lines changed as the neutron star rotated. An emission line is a feature in a spectrum that can reveal information about the material producing or interacting with the radiation. A research team led by Kinjal Roy of RRI examined four such emission lines in detail. The researchers found that the structure producing these changes must be rotating along with the neutron star.
The pattern helped them identify the likely source which is a stream of matter moving towards the neutron star.
Following the stream of matter
This stream is part of a process called accretion, in which a compact object draws in material from its surroundings. In Centaurus X-3, the stream carries matter from an accretion disk towards the neutron star. The disk is a rotating structure of gas and other material that moves around the star before being drawn inwards. The neutron star’s magnetic field then guides the incoming matter towards its magnetic poles.
The stream also changes what an observing satellite sees. As it moves around the neutron star, it can come between the satellite and the star, partially blocking the direct radiation. When this happens, the primary X-ray signal weakens. At the same time, radiation from the stream itself becomes stronger in the observed signal.
The researchers used these changing signals to connect the observed variations to the movement of matter around the neutron star. The evidence for an accretion stream also points to an accretion disk feeding it. This matters because scientists generally expect high-mass X-ray binaries to gather material in a different way.
Why an accretion disk matters
In many high-mass X-ray binaries, a neutron star captures gas directly from the stream of material blown away by its companion star. This is known as stellar-wind accretion. An accretion disk involves a different arrangement: material gathers into a rotating structure before flowing towards the neutron star. The findings from Centaurus X-3 indicate that this disk-based process is taking place in a system where it is not generally expected.
That difference matters when scientists calculate how the system produces and releases radiation. If their models leave out the disk, they may fail to account for some of the radiation coming from the surrounding material.
“Accretion disk is not expected to occur in [HMXBs] So, if an accretion disk is forming in this system, emission models have to be modified,” Roy said in the Department of Science and Technology’s announcement. He added that future models of Centaurus X-3 would need to account for radiation from the disk.
The research does not mean that scientists have directly photographed the disk. Instead, they have used the changing X-ray signals to infer the presence and behaviour of structures that remain too distant to resolve clearly. Published in The Astrophysical Journal, the study adds to the understanding of Centaurus X-3, one of the most widely studied binary pulsars. It also shows how small changes in radiation can reveal the movement of matter around objects that are otherwise beyond the reach of direct observation.
By identifying the flow responsible for the changing signals, the researchers have provided a more detailed picture of how this neutron star draws in material. That picture will help scientists refine their models of Centaurus X-3 and examine whether similar processes occur in other high-mass X-ray binaries.
Space & Physics
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