About Arun Kumar N

Arun has been associated with India International Times since 2018 and he has been a key reporter in covering science and space related stories. He can be reached at arunKnn@indiainternationaltimes.com.

How do giant caldera volcanoes refill magma after massive eruptions

Researchers from Kobe University have identified how magma reservoirs beneath giant caldera volcanoes refill, based on a study of the Kikai caldera. The findings, published in Communications Earth & Environment in 2026, show that fresh magma is injected into reservoirs rather than left over from past eruptions. The work draws parallels with massive systems like the Yellowstone caldera and Toba caldera, offering new insight into how such volcanoes evolve after eruptions.

The crater left behind after a supervolcano erupts can stretch for miles, a scar formed when vast volumes of magma are expelled in a single event. What happens next, beneath that quiet surface, has long remained uncertain.

A new study from Kobe University offers a clearer picture. It suggests that the magma chambers of these giant caldera volcanoes do not simply retain leftover material. Instead, they are gradually refilled by new injections of magma rising from deeper within the Earth.

That distinction matters for scientists trying to understand how and when these volcanoes might erupt again.

Kikai caldera magma reservoir mapping using seismic surveys

The research focused on the Kikai caldera, located mostly underwater off southern Japan. Its last major eruption around 7,300 years ago is considered the largest of the Holocene epoch, the current geological period.

The site’s underwater setting provided a rare advantage. It allowed scientists to conduct detailed, large-scale surveys of the subsurface using controlled seismic techniques.

Working with the Japan Agency for Marine-Earth Science and Technology, researchers deployed airgun arrays to generate seismic waves and ocean-bottom seismometers to track how those waves moved through the Earth’s crust.

These measurements revealed a large reservoir beneath the caldera that is composed largely of magma. Its size and position indicate that it corresponds to the same reservoir involved in the ancient eruption.

“Due to its extent and location it is clear that this is in fact the same magma reservoir as in the previous eruption,” said geophysicist Nobukazu Seama.

New magma injection replaces remnants from past eruptions

While the reservoir occupies the same region, the material inside it appears to be new.

Over the past 3,900 years, a lava dome has been forming at the center of the caldera. Chemical analysis of material from this dome and other recent activity shows a composition different from the magma ejected in the ancient eruption.

That difference led researchers to conclude that the current magma is not simply leftover from the previous event.

“This means that the magma that is now present in the magma reservoir under the lava dome is likely newly injected magma,” Seama said.

The finding supports what researchers describe as a “magma re-injection model,” in which fresh material gradually replenishes emptied reservoirs over thousands of years.

This process changes how scientists interpret signals from volcanoes. Instead of looking for signs of residual magma building pressure, attention shifts to how new magma enters and accumulates.

Implications for Yellowstone and other supervolcano systems

The study’s implications extend beyond Japan. Giant calderas such as Yellowstone in the United States and Toba in Indonesia share similar structural features, including large shallow magma reservoirs.

“This magma re-injection model is consistent with the existence of large shallow magma reservoirs beneath other giant calderas like Yellowstone and Toba,” Seama said.

Understanding how these reservoirs refill is central to predicting volcanic behavior. Supervolcano eruptions are rare but can have global consequences, affecting climate, ecosystems, and human activity.

Despite their scale, the processes leading up to such eruptions remain poorly understood. Scientists know that these volcanoes can erupt again, but the timing and triggers are difficult to determine.

The new model offers a framework for tracking those processes over time, particularly by monitoring how magma is supplied to reservoirs after major eruptions.

Toward improved monitoring of future giant eruptions

Researchers say the next step is refining the tools used in this study to better observe magma movement beneath the Earth’s surface.

“Our ultimate goal is to become better able to monitor the crucial indicators of future giant eruptions,” Seama said.

For now, the findings provide a clearer view of what happens after a supervolcano erupts. The surface may appear quiet, but deep below, new magma is slowly rebuilding the conditions for the next chapter in the volcano’s life cycle.

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Japan commits ODA loan to India in urban Transport, health and agriculture sectors

The Government of Japan has committed an Official Development Assistance loan worth JPY 275.858 billion, about ₹16,420 crore, to India for four infrastructure and social sector projects. The agreement, signed on March 24, 2026, in New Delhi, covers metro rail expansion in Bengaluru and Mumbai, healthcare upgrades in Maharashtra, and horticulture development in Punjab. The funding will be implemented through the Japan International Cooperation Agency and is part of the broader India-Japan strategic partnership.

A fresh tranche of Japanese funding is set to shape some of India’s most critical urban and social infrastructure projects, from metro rail expansion in its largest cities to strengthening healthcare systems and farm incomes.

The agreement, finalized on March 24, brings together officials from both governments at a time when India’s infrastructure pipeline is expanding rapidly across states.

The Notes for the loan were exchanged between Alok Tiwari, Joint Secretary in the Department of Economic Affairs under India’s Ministry of Finance, and Keiichi Ono, Japan’s ambassador to India. Loan agreements were also signed with the Japan International Cooperation Agency, the country’s primary development finance arm. [1]

Bengaluru and Mumbai metro expansion projects funding details

A significant portion of the funding is directed toward urban transport, with two metro rail projects accounting for the bulk of the allocation.

The Bengaluru Metro Rail Project Phase 3 will receive JPY 102.480 billion. The expansion aims to meet rising commuter demand in the Bengaluru Metropolitan Region by extending the mass rapid transit network.

Officials say the project is designed not only to improve mobility but also to reduce congestion and vehicle emissions, contributing to climate mitigation efforts in one of India’s fastest-growing urban centers. [2]

In Mumbai, the Metro Line 11 Project will receive JPY 92.400 billion. The line is expected to address similar pressures in the country’s financial capital, where traffic density and air pollution remain persistent challenges.

Both metro projects are positioned as long-term investments in urban sustainability, linking transport infrastructure with environmental goals. [3]

Maharashtra healthcare system upgrade and Punjab agriculture project

Beyond transport, the loan package includes funding aimed at strengthening public health systems in Maharashtra.

The Project for Strengthening Tertiary Healthcare Delivery, Medical Education System and Nursing Education System in Maharashtra will receive JPY 62.294 billion. The initiative includes the construction and upgrading of tertiary care hospitals, medical colleges, and nursing schools.

The goal is to improve both access to advanced medical care and the quality of medical education, with a broader focus on advancing Universal Health Coverage across the state. [4]

In Punjab, JPY 18.684 billion has been allocated for a project focused on sustainable horticulture. The initiative aims to help farmers diversify into high-value crops, supported by infrastructure development and capacity-building programs.

Officials say the project is intended to strengthen agricultural value chains while promoting environmentally sustainable practices. [5]

India Japan development cooperation and strategic partnership

The latest funding builds on decades of development cooperation between India and Japan, which dates back to 1958. Economic collaboration has become a central pillar of the bilateral relationship, with Japan emerging as one of India’s key partners in infrastructure financing.

Projects funded through Japanese ODA have historically included metro systems, industrial corridors, and environmental initiatives across multiple states.

The current loan package reinforces that trajectory, linking infrastructure expansion with broader goals such as climate resilience, public health, and rural income growth.

It also reflects Japan’s continued focus on supporting large-scale, long-term development projects through concessional financing mechanisms, often implemented via JICA.

The four projects, spread across Karnataka, Maharashtra, and Punjab, are expected to move into implementation phases following the signing of loan agreements, marking another step in the evolving India-Japan strategic and global partnership.

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Space Breakthrough: Astronomers confirm rogue planet candidate as a planet for the first time

An international team led by Peking University confirmed the mass of a rogue planet for the first time using a rare alignment of telescopes in May 2024. The object, detected through microlensing, was found to be about the mass of Saturn, confirming it as a true planet. The findings, published in Science in January 2026, relied on combined data from ground observatories and the Gaia spacecraft. Scientists say the discovery could reshape understanding of free-floating planets across the Milky Way.

In the vast dark between stars, planets drift unseen. For years, astronomers suspected they existed in large numbers, but proving what they were has been far more difficult.

That changed with a brief flicker of light in May 2024.

The signal lasted just two days. It came from a distant star whose brightness momentarily intensified as an unseen object passed in front of it. That phenomenon, known as microlensing, has long been one of the few ways to detect rogue planets.

This time, the data went further.

“For the first time, we have a direct measurement of a rogue planet candidate’s mass and not just a rough statistical estimate,” said Dong Subo, an astronomer at Peking University. “We know for sure it’s a planet.”

Microlensing technique confirms rogue planet mass for first time

Rogue planets, unlike Earth or Jupiter, do not orbit a star. They move independently through space, making them nearly impossible to detect with traditional methods that rely on starlight.

Microlensing offers a workaround. When a planet crosses the line of sight between Earth and a distant star, its gravity bends the star’s light, briefly amplifying it. The effect acts like a natural magnifying glass.

Astronomers have used this method for decades, but it comes with limitations. While it reveals that an object exists, it often cannot precisely determine its mass because distance and gravitational strength are intertwined in the signal.

That ambiguity has left many rogue planet candidates in a gray area.

The new study, published in Science, resolved that uncertainty for one object by combining observations from multiple telescopes across Earth and space. The event, catalogued as KMT-2024-BLG-0792 and OGLE-2024-BLG-0516, was first detected by the Korea Microlensing Telescope Network and the Optical Gravitational Lensing Experiment.

At the same time, the Gaia spacecraft, operated by the European Space Agency, recorded the same event from its position roughly 1.5 million kilometers from Earth.

That overlap proved critical.

Gaia parallax measurement unlocks distance and mass data

The key to the breakthrough lay in measuring what astronomers call the microlens parallax effect. This effect works similarly to human depth perception, where viewing an object from two different positions reveals its distance.

In this case, Gaia’s vantage point in space and Earth-based telescopes provided two perspectives of the same event. The microlensing signal appeared about two hours later from Gaia’s position than from Earth.

That time difference allowed researchers to separate the object’s distance from its gravitational influence, enabling a precise mass calculation.

“We are able to use the same principle to extract the distance information of this rogue planet candidate, finding the mass and distance separately,” Dong said.

The result placed the object at roughly one-fifth the mass of Jupiter, comparable to Saturn. That measurement confirmed it as a planet rather than a more massive object such as a brown dwarf.

Implications for rogue planet population in the Milky Way

The finding carries implications beyond a single object. Astronomers have long theorized that the Milky Way Galaxy may host vast numbers of rogue planets, potentially numbering in the billions or more.

“Our discovery offers further evidence that the Galaxy may be teeming with rogue planets that were likely ejected from their original homes,” Dong said.

These planets are thought to form within star systems before being expelled through gravitational interactions, especially during early stages of planetary formation. Passing stars may also disrupt systems, sending planets into interstellar space.

Some theories suggest that a subset of rogue planets could form independently, collapsing directly from gas clouds without ever orbiting a star.

The new measurement strengthens confidence in microlensing surveys that have hinted at such populations for years.

Future space telescopes to expand rogue planet discoveries

The study also highlights the importance of coordinated observations across multiple platforms. The overlap between Gaia, KMTNet, and OGLE marked the only time in Gaia’s operational lifetime that all three observed the same rogue planet candidate.

Future missions are expected to make such measurements more routine.

NASA plans to launch the Nancy Grace Roman Space Telescope, which will conduct large-scale microlensing surveys capable of detecting hundreds of rogue planets. China is also developing new missions, including the Chinese Space Station Survey Telescope and a proposed Earth 2.0 mission, both of which include microlensing in their scientific goals. [8]

These next-generation observatories will operate above Earth’s atmosphere, improving sensitivity and reducing distortions that affect ground-based observations.

“The new space-based facilities such as Roman, CSST, and Earth 2.0 are going to revolutionize the field of microlensing and the study of free-floating planets,” Dong said.

For now, the confirmed mass of a single rogue planet marks a turning point. It transforms a fleeting signal into a measurable world, offering a clearer view of a population that has long remained in the shadows.

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ESMT Berlin and BMW Group’s ‘Change Maker Fellowship 2026’ opens for MBA, MSc applicants globally

The BMW Group and ESMT Berlin have opened applications for the 2026 Change Maker Fellowship, offering eight scholarships across MBA and MSc programs. The initiative, now in its fifth year, targets STEM graduates from select countries including India, the United States, and Germany. The fellowships aim to train future leaders in digital transformation and mobility innovation. Applications are tied to academic intakes beginning September 2026 through January 2027.

The push to build leaders for a digital economy is increasingly moving inside corporate boardrooms and business schools. This year, BMW Group is doubling down on that effort with a new round of fellowships designed to connect engineering talent with executive training.

The automaker, working with ESMT Berlin, is offering eight Change Maker Fellowships for the 2026 academic cycle. The program is structured across three tracks, each aligned with a different stage of professional development.

Two fellowships are reserved for the full-time Master of Business Administration program starting in January 2027. Two more will support students entering Master of Science programs in September 2026. The remaining four are allocated to the Global Online MBA beginning in October 2026.

BMW ESMT fellowship eligibility and program structure

The fellowship targets candidates with strong backgrounds in science, technology, engineering, and mathematics, often referred to as STEM. Applicants are expected to either hold a bachelor’s degree in a relevant field or demonstrate work experience in areas such as information technology, automation, or digital systems.

The program reflects a growing demand for leaders who can navigate both technical systems and business strategy. Participants will combine formal management education with exposure to digital transformation challenges, particularly those shaping the future of mobility.

“We are proud to be entering the fifth year of our partnership with ESMT,” said Ilka Horstmeier, a member of the Board of Management of BMW AG responsible for People and Real Estate. “Especially now, we need leaders who take responsibility and use technology and digitalization to shape the future.”

Eligibility is limited to applicants from countries where BMW maintains IT hubs, including Germany, India, Portugal, Romania, Brazil, China, the United States, and South Africa. Individuals with recognized refugee status in Germany are also eligible.

For applicants to the full-time MBA and MSc tracks, an age cap applies. Candidates must be under 30 years old as of September 1, 2026.

Focus on digital transformation and mobility leadership

The fellowship sits at the intersection of two shifts in global business. One is the increasing importance of artificial intelligence and digital systems in decision-making roles. The other is the transformation of the mobility sector, where traditional automakers are expanding into software-driven ecosystems.

BMW Group employs more than 10,000 IT and software specialists worldwide and operates a network of technology hubs across multiple continents. That footprint shapes both the geographic eligibility and the program’s focus on real-world digital challenges.

At ESMT Berlin, the curriculum integrates business fundamentals with emerging technologies. The aim is to prepare candidates for leadership roles that require both technical fluency and strategic thinking.

“We thank BMW Group for its sustained partnership in advancing this initiative,” said Jörg Rocholl. “Digital transformation and artificial intelligence are changing the capabilities required in leadership roles.”

Applicants will also be required to respond to a central essay question during the selection process: “The BMW Group actively shapes the future of mobility: what aspect of a digital future fascinates you most, and why?”

Why companies are investing in leadership fellowships

Programs like the Change Maker Fellowship reflect a broader shift in how companies build talent pipelines. Rather than relying solely on recruitment, firms are investing earlier in education and training, particularly in fields tied to digital transformation.

For BMW, this includes aligning academic training with its global operations. The company’s IT hubs in regions such as India and the United States play a role in shaping both the talent pool and the skills required for future roles.

The fellowship also underscores the increasing overlap between engineering and management. As industries digitize, technical expertise alone is often not enough for leadership positions. Business education is becoming a complementary requirement.

The partnership with ESMT Berlin, now entering its fifth year, reflects a sustained effort to bridge that gap.

Applications for the 2026 Change Maker Fellowship are currently open through ESMT Berlin’s admissions process. Candidates must meet the entry requirements of their chosen program in addition to the fellowship criteria.

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Ghost Forests Reveal Hidden Climate Threats Along U.S. Coasts, Study Finds

Researchers from the University of Delaware presented findings on March 26, 2026, in Atlanta, showing how “ghost forests” are reshaping coastal ecosystems. The phenomenon, driven by sea level rise along the eastern United States, is killing salt-sensitive trees and altering underground nutrient cycles. Scientists say studying water flow through these forests could help predict how coastal regions respond to climate change. The research was presented at the ACS Spring 2026.

Along stretches of the eastern United States coastline, the landscape is shifting in ways that are both stark and unsettling. Where dense green forests once stood, clusters of pale, lifeless tree trunks now rise from the soil. These are “ghost forests,” a visible imprint of rising seas pushing saltwater inland.

For researchers walking through these areas, the change is not abstract. It is immediate, physical, and accelerating.

“Walking through these coastal forests, surrounded by nature, is beautiful,” said Samantha Chittakone, an undergraduate researcher at the University of Delaware. “However, it is disheartening to see the healthy trees becoming less prevalent as you approach the shoreline.”

Her team’s work, presented this week at ACS Spring 2026, focuses on a less visible but critical process unfolding beneath those skeletal trees. It centers on how water moves through them and what that reveals about ecosystem health.

Ghost forests and saltwater intrusion along US coasts

Ghost forests form when saltwater from rising seas seeps into coastal soils, poisoning trees that cannot tolerate salinity. Over time, the trees die but remain standing, creating the haunting landscapes now increasingly common along the mid-Atlantic coastline.

The phenomenon has drawn attention as a clear signal of climate change’s local impact. But beyond their visual effect, these forests may hold deeper clues about how ecosystems respond to environmental stress.

The research team focused on sweetgum trees, a species common in these coastal regions. By comparing healthy, stressed, and dead trees, they sought to understand how forest systems transition under pressure from saltwater intrusion.

Their approach looked at “stemflow,” the rainwater that travels down a tree’s branches and trunk to the soil below. Scientists consider this flow a key pathway for delivering nutrients and organic material to the forest floor.

“Stemflow is basically injecting nutrients and really important chemicals into the forest ecosystem so the microbiome there can thrive,” said Yu-Ping Chin, a researcher involved in the study.

That process, the team suggests, begins to break down as forests transition into ghost forests.

Stemflow changes reveal disruption in forest carbon cycles

By collecting stemflow samples from trees in different stages of decline, the researchers identified measurable changes in how water and nutrients move through the ecosystem.

One finding stood out. Dead trees allowed significantly less stemflow to reach the forest floor. Instead, much of the water appeared to be absorbed into the decaying wood itself.

“The stemflow’s being absorbed by the dead trees. They’re acting like sponges,” Chin said.

That shift has cascading effects. When less water, nutrients, and dissolved organic carbon reach the soil, the entire ecological balance belowground can change.

The team also detected unexpectedly high sugar concentrations in the stemflow of stressed and dying trees. According to Delphis Levia, another researcher on the project, this could reshape microbial communities in the soil near tree trunks.

“Our results signify that the transition from healthy trees to ghost forests changes the magnitude and chemistry of stemflow,” Levia said. “Further research will better contextualize these changes in stemflow chemistry on the overall cycling of carbon in coastal forests.”

These changes matter because coastal forests play a role in carbon storage. Alterations in how carbon moves through these systems could influence how effectively they act as carbon sinks.

Why ghost forests matter for climate resilience planning

The implications extend beyond individual forests. As sea levels continue to rise, more coastal ecosystems are expected to undergo similar transitions.

Understanding which forests can adapt, and which are likely to collapse into ghost forests, is a growing priority for scientists and policymakers.

This research suggests that stemflow could serve as an early diagnostic signal. Changes in water flow and chemistry may indicate stress in forest systems before visible die-off becomes widespread.

The findings also connect to broader efforts to model climate resilience. Coastal forests act as buffers against storms, store carbon, and support biodiversity. Their decline could amplify the impacts of climate change in already vulnerable regions.

Chittakone said the work is part of a larger push to better understand these processes, including how factors like wildfires interact with stemflow and nutrient cycling.

“Stemflow is a significant transporter of nutrients and other important chemicals in these coastal forests,” she said. “It’s something that we should study more and not overlook whenever it comes to carbon cycling.”

The ghost forests now lining parts of the U.S. coastline are often described as warnings. This research suggests they are also records, capturing the hidden changes reshaping ecosystems from the ground up.

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New MetaRing Sensor Spots Breast Cancer Drug Response in 10 Minutes

Researchers at the Chinese Academy of Sciences have developed a biosensor that can quickly detect how breast cancer responds to paclitaxel. The system, called MetaRing, analyzes tiny biological samples and delivers results in about 10 minutes. The study, published recently, points to faster, more personalized chemotherapy decisions.

 

Emotional Blindness May Raise Risk of Short Video Addiction, TikTok: Study

No matter where we turn on social media, short videos are everywhere. Repeated exposure to this brief, information-dense, and rewarding content stimulates the brain in a way that tells us the experience is pleasurable or satisfying.

 

Government enacted Sexual Harassment of Women at Workplace Act, 2013, aiming to provide safe,secure working environment for women

The Union government has reaffirmed the expansive scope of the Sexual Harassment of Women at Workplace (Prevention, Prohibition and Redressal) Act, 2013, stating that the law applies to all women regardless of age, employment status, or sector of work. The clarification was provided in the Rajya Sabha by Minister of State for Women and Child Development Savitri Thakur in response to a parliamentary query.

The Act, commonly referred to as the Sexual Harassment (SH) Act, was enacted to ensure safe and secure working conditions for women and to uphold constitutional guarantees of equality, dignity, and the right to livelihood.

Sexual harassment at the workplace, the government noted, constitutes a violation of fundamental rights under Articles 14, 15, and 21 of the Constitution of India, as well as the right to practice any profession under Article 19(1)(g). Such conduct creates unsafe work environments and can limit women’s participation in economic activity, affecting broader goals of inclusive growth.

Sexual harassment law definition of aggrieved woman and employee scope

A key clarification highlighted by the government concerns the definition of an “aggrieved woman” under Section 2(a) of the Act. The provision defines an aggrieved woman as any woman, of any age, whether employed or not, who alleges sexual harassment at a workplace. This ensures that protection is not limited to formally employed individuals.

Officials said this broad definition reflects legislative intent to extend protection to all women present in a workplace environment, including visitors or those indirectly associated with the workplace.

The Act also adopts an expansive definition of “employee” under Section 2(f). It includes individuals employed on regular, temporary, ad hoc, or daily wage terms, as well as those engaged through agents. The definition explicitly covers contractual workers, apprentices, trainees, consultants, volunteers, and unpaid interns.

This provision ensures that formal employment or economic dependence on an employer is not a prerequisite for protection under the law.

Workplace and employer definition under Sexual Harassment Act explained

The term “employer” under Section 2(g) is defined to include heads of government departments, organizations, and institutions, as well as individuals responsible for management, supervision, and control in private workplaces. The definition also extends to those fulfilling contractual obligations and, in the case of domestic workers, households employing such workers.

The Act further defines “workplace” in broad terms under Section 2(o), covering government bodies, private enterprises, non-governmental organizations, and institutions engaged in commercial, professional, educational, industrial, or health-related activities.

The definition includes both organized and unorganized sectors and extends to home-based workers, field assignments, and situations where women are in transit for work.

The government described the legislation as inclusive and intersectional in design, aimed at addressing workplace realities across diverse sectors and employment arrangements.

Judicial interpretation has reinforced this wide scope. In the 2013 case of Jaya Kodate v. Rashtrasant Tukdoji Maharaj Nagpur University, the Bombay High Court observed that the definition of workplace was deliberately kept broad to ensure no instance of sexual harassment goes unaddressed.

The clarification in Parliament comes as workplace safety continues to be a central issue in discussions on women’s workforce participation and economic empowerment.

The government maintained that the law’s framework is intended to ensure that no woman, irrespective of her role or employment status, is excluded from protection against sexual harassment in any workplace setting.

Akashvani to Broadcast Full Version of “Vande Mataram” from 26th March

For decades, mornings on Akashvani began with a familiar sequence. The signature tune played, followed by a brief, two-stanza rendition of “Vande Mataram,” lasting just over a minute.

That routine changes this week.

Starting March 26, all stations of Akashvani, the national public radio service under Prasar Bharati, will broadcast the full six-stanza version of the National Song. The shift follows a guideline issued by the Ministry of Home Affairs on January 28, 2026, which references the complete composition of the song.

The new broadcast extends the duration to 3 minutes and 10 seconds, replacing the earlier 65-second version that had been in place since 1947.

Ministry guideline prompts nationwide broadcast shift

The Ministry of Home Affairs, the central government body responsible for internal security and administrative policy, issued the directive earlier this year outlining the structure of the National Song in its full form.

While “Vande Mataram,” written by Bankim Chandra Chatterjee in the late 19th century, contains multiple stanzas, only the first two had been widely used in official and public settings for decades.

Akashvani officials said the new directive prompted a review of existing broadcast practices. The decision was then taken to align daily programming with the full six-stanza version referenced in the guideline.

The change applies uniformly across all Akashvani stations, ensuring that listeners nationwide hear the extended version as part of the morning broadcast sequence.

New recordings introduce regional musical diversity

The initial version to be aired from March 26 has been recorded by Pandit Chandrashekhar Vaze, a Hindi classical vocalist, in Raag Des, a melodic framework commonly associated with patriotic compositions.

Officials said this version will serve as the standard rollout across stations in the initial phase.

At the same time, Akashvani has begun producing multiple regional adaptations of the song. These recordings incorporate local musical instruments and styles, reflecting the linguistic and cultural diversity of different states.

Stations in various regions are expected to adopt versions that align with their local musical traditions while maintaining the structure of the six-stanza composition.

The effort, according to officials, is aimed at presenting the National Song in a way that resonates with regional audiences without altering its core form.

A shift from brevity to full composition

The earlier two-stanza format had been a practical choice for broadcast constraints and programming schedules. Its 65-second duration allowed it to fit seamlessly into fixed time slots at the start of the day.

The extended version, at over three minutes, marks a notable change in pacing for morning programming.

Officials have not indicated any reduction in other segments to accommodate the longer duration, though programming adjustments may vary by station.

The move also places renewed emphasis on the full lyrical and musical structure of “Vande Mataram,” which has historically been performed in both abbreviated and complete forms depending on context.

With the rollout set for March 26, listeners tuning in to Akashvani’s morning broadcast will encounter a familiar song presented in its most complete form, marking a shift in a routine that has remained largely unchanged for decades.

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Who’s Watching Matters: Honey Bees Change Their Famous Dance in Surprising Ways

For decades, the honey bee waggle dance has been treated as a near-perfect example of one-way communication in nature. A foraging bee returns to the hive, performs a patterned movement, and nearby bees decode the message to locate food.

 

Viral Posts Of LPG Refill Booking New Timelines Spark Confusion, Government Issues Clarification

 Confusion over cooking gas refill rules spread quickly this week, driven by viral posts claiming new waiting periods for booking LPG cylinders.

The Government of India stepped in with a clarification, stating that no such revisions have been introduced. The claims, widely shared online, suggested differentiated timelines based on connection types, including Pradhan Mantri Ujjwala Yojana (PMUY) beneficiaries and non-PMUY consumers.

Officials said the information is incorrect.

According to the government, the existing refill booking timelines remain unchanged.

It is clarified that no such changes have been made. The existing refill booking timelines remain unchanged and continue to be:

  • 25 days in urban areas, and
  • 45 days in rural areas, irrespective of connection type.

LPG Refill Booking Rules India Remain Unchanged Across Connection Types

The clarification addresses specific claims that had circulated online. These posts alleged that PMUY users would face a 45-day waiting period, while non-PMUY users would have different timelines based on the number of cylinders they hold.

Government officials said no such categorization exists under current policy.

The uniform timeline applies across all connection types. This includes households enrolled under the Pradhan Mantri Ujjwala Yojana, the flagship scheme launched in 2016 to provide subsidized LPG connections to low-income families, as well as regular domestic consumers.

Authorities emphasized that the refill system continues to function as before, with no policy shift or operational change.

Government Advises Public Against Panic Booking Amid Misinformation

Officials also cautioned citizens against reacting to unverified claims. Panic booking, they said, could strain distribution systems unnecessarily, even when supply remains stable.

The government reiterated that adequate LPG stocks are available across the country. There is no reported shortage or disruption in supply chains at this time.

Misinformation related to essential commodities often spreads quickly, particularly when it affects household necessities such as cooking gas. In past instances, similar rumors have triggered sudden spikes in demand, leading to localized delivery delays.

Authorities urged consumers to rely on official communications and verified sources for updates on LPG policies.

For now, the message from policymakers is direct. There has been no change in refill booking timelines, and there is no need for concern.

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How protecting ‘umbrella species’ Polar bear helps scientists in Arctic conservation

On the frozen edge of Hudson Bay, polar bears are doing more than hunting seals. They are helping scientists map the future of Arctic conservation.

A new study led by researchers at the University of Alberta and the San Diego Zoo Wildlife Alliance (SDZWA) suggests that protecting polar bear habitats could also shield a wide network of Arctic species. The research draws on nearly 20 years of tracking data from 355 bears to identify areas where conservation efforts may deliver the greatest impact.

The findings, published in the journal Arctic Science, focus on western Hudson Bay, a region already under pressure from warming temperatures and shifting ice conditions.

Hudson Bay Polar Bear Tracking Study Identifies High-Use Conservation Zone

The research pinpoints a “high-use” area near Cape Churchill in Manitoba as a priority zone for protection. Scientists analyzed long-term movement patterns to determine where polar bears consistently spend time, particularly during critical periods such as feeding and migration.

Establishing marine protected areas, or MPAs, in Arctic waters has long been complicated by limited data on where marine life concentrates. The study proposes that polar bears can serve as a proxy for broader ecosystem activity, offering a data-rich foundation for decision-making.

“By leveraging the extensive data we have on polar bears, we can help design MPAs that safeguard both the bears and the vast network of Arctic species that rely on them,” said Dr. Nicholas Pilfold, a conservation scientist at SDZWA.

Researchers argue that the approach addresses a central challenge in marine conservation. Instead of attempting to track multiple species across vast and remote regions, policymakers can use one well-studied species to guide protection efforts.

Umbrella Species Concept Gains Ground In Arctic Conservation Strategy

The concept of an “umbrella species” refers to a single species whose protection indirectly benefits others that share its habitat. According to the study, polar bears meet nearly all criteria for this role.

They have large home ranges, well-documented biological data, and high sensitivity to environmental disturbance. These characteristics make them effective indicators of ecosystem health.

The research highlights how polar bears influence their surroundings beyond their own survival. When bears hunt, leftover carcasses provide food for scavengers such as Arctic foxes, wolves, ravens, and gulls. This behavior creates a chain of ecological benefits that extends across species.

Dr. Andrew Derocher, a professor of biological sciences at the University of Alberta, said the data offers a practical path forward for conservation planning. “In the rapidly warming Arctic, marine ecosystems will be stressed by the additive effects of industrial activity and polar bear location data provide a path to designing marine protected areas,” he said. [2]

Policy Momentum Builds Around Hudson Bay Marine Protection Plans

The study arrives as policymakers in Canada consider expanding protections in the region. In February 2026, Manitoba Premier Wab Kinew announced funding to explore the creation of a national marine conservation area in western Hudson Bay.

While details of the proposal remain under development, the research provides scientific backing for where boundaries could be drawn. Conservation areas designed around polar bear activity may capture critical habitats for multiple species without requiring extensive new data collection.

Scientists involved in the study also emphasize the need for flexibility. The Arctic environment is changing rapidly, with sea ice loss altering migration routes and feeding patterns.

Pilfold noted that dynamic MPAs, which can adapt to shifting ecological conditions, may be particularly effective in this context. “Well-designed dynamic MPAs have the potential to preserve biodiversity in a constantly changing Arctic landscape,” he said.

The researchers acknowledge that climate change could eventually reduce the effectiveness of polar bears as an umbrella species if their habitat continues to shrink. Still, they describe the approach as a practical starting point for immediate conservation action.

For now, the polar bear’s movements offer something rare in the Arctic: a clear, data-driven map for protecting life in one of the planet’s most fragile ecosystems.

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Thousands Of Pico-Satellites Could Redefine Direct Smartphone Connectivity From Space

A new approach to satellite communications could significantly reshape how smartphones connect to space, with researchers proposing the use of thousands of tiny satellites working in unison rather than relying on a single, complex spacecraft.

Scientists in Japan have demonstrated that swarms of pico-satellites—each carrying a small हिस्सा of a larger antenna system—can collectively function as a single, powerful phased-array antenna. The early-stage experiment showed that such a distributed system can deliver stable, high-quality data transmission, offering a potential pathway to cheaper and more resilient global connectivity.

The concept builds on the growing interest in direct-to-device (D2D) satellite communications, which aim to allow ordinary smartphones to connect directly to satellites without the need for ground infrastructure. The technology is particularly attractive for extending coverage to remote regions such as oceans, deserts, and disaster-hit areas where terrestrial networks are either weak or nonexistent.

Traditionally, achieving this requires large satellites equipped with sophisticated phased-array antennas. These systems rely on tightly coordinated antenna elements that can steer signals electronically. However, they are expensive to build and launch, and their centralized design creates a single point of failure—any major malfunction can render the entire satellite ineffective.

The Japanese research team, led by Associate Professor Atsushi Shirane, has proposed a fundamentally different architecture. Instead of concentrating antenna elements on one satellite, the system distributes them across thousands of pico-satellites flying in formation. These miniature units are synchronized wirelessly, eliminating the need for physical connections.

At the heart of the innovation is what the researchers describe as “spatial wireless combining and distributing technology.” In this setup, a central gateway satellite broadcasts a reference signal that allows all participating pico-satellites to remain precisely synchronized. This removes the need for energy-intensive components such as local oscillators on each unit, enabling further miniaturization and reducing power consumption.

The team developed a compact transceiver chip using standard silicon CMOS technology, making it suitable for large-scale, low-cost manufacturing. In laboratory simulations replicating satellite formations, the system demonstrated accurate beam steering and reliable data transmission using communication protocols similar to those found in modern smartphones.

Beyond lowering costs, the distributed nature of the system offers a major reliability advantage. Because the network is made up of numerous independent satellites, the failure of individual units does not compromise the entire system—unlike traditional monolithic satellites.

The findings suggest that formation-flying pico-satellites could become a viable foundation for next-generation satellite networks. If scaled successfully, the approach could expand global connectivity while reducing both financial and operational risks, bringing direct satellite communication closer to everyday mobile users.

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‘SHE Marts’ Scheme To Support Rural Women Entrepreneurs Under NRLM Announced

For many women in rural India, the challenge is not producing goods but finding a reliable place to sell them.

The government has announced a new initiative called Self Help Entrepreneur Marts, designed to give women led enterprises a direct link to consumers. [1]

The proposal focuses on women working within Self Help Groups, or SHGs, which are community based collectives that support savings, credit and small scale enterprise activity.

The update was shared in the Lok Sabha by Minister of State for Rural Development Dr. Chandra Sekhar Pemmasani. [1]

SHE Marts scheme under NRLM for SHG market access

The initiative will operate under the Deendayal Antyodaya Yojana National Rural Livelihoods Mission, a flagship program aimed at promoting sustainable livelihoods for rural households. [1]

SHE Marts are envisioned as structured retail outlets where products made by SHG members can be displayed and sold directly to customers.

Officials said the model is intended to improve visibility for locally produced goods and create stronger market linkages.

The marts are expected to function as community owned retail platforms managed through cluster level federations of SHGs. [1]

These federations bring together multiple groups to coordinate production, financing and marketing activities.

Rural women entrepreneurs transition from credit to enterprise ownership

The government said the initiative is part of a broader effort to support women in moving beyond credit linked livelihood activities.

The focus is on enabling them to become enterprise owners capable of scaling their businesses.

Support under the program will include market access and capacity building, aimed at strengthening business skills and operational capabilities. [1]

Officials said this transition is critical for improving income stability and long term economic participation among rural women.

The initiative also seeks to strengthen institutional structures within the SHG ecosystem by integrating production and retail functions.

SHE Marts funding model and implementation status

According to the government, the marts will be set up using enhanced and innovative financing mechanisms.

These are expected to support the establishment of retail infrastructure at the community level.

No funds have been sanctioned or spent on the initiative so far, indicating that it remains at the proposal stage. [1]

The announcement outlines a framework that combines institutional support, market access and financing tools to expand opportunities for rural women entrepreneurs.

Thousands of crores lie unclaimed; how RBI, SEBI and IRDAI help citizens reclaim it [See measures]

Money left untouched in bank accounts, insurance policies and investments is accumulating across India. Regulators say they are now moving to return it to rightful owners.

 

RBI Proposes New Rules on Unauthorised Electronic Banking Transactions

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Rajnath Singh reviews West Asia situation and Its impact on India defence preparedness

India’s defence leadership met in New Delhi on March 24 to assess how tensions in West Asia could affect the country’s military preparedness.

Defence Minister Rajnath Singh chaired the high level review, which included the Chief of Defence Staff, the professional head of India’s armed forces, along with the Army, Navy and Air Force chiefs.

Senior officials including the Defence Secretary, Secretary for Defence Production and the Chairman of the Defence Research and Development Organisation, India’s premier military research agency, also attended the meeting.

The discussions focused on the evolving security situation in West Asia and its potential implications for India.

India defence preparedness West Asia conflict supply chain impact

Officials briefed the minister on global and regional developments, including the possible consequences of an escalation in ongoing conflicts.

The review examined how such developments could affect India’s defence preparedness, particularly in areas linked to procurement and production of military equipment.

Supply chain management was identified as a key area of concern, especially in relation to maintaining and servicing existing defence platforms.

India relies on a mix of domestic production and international sourcing for defence equipment, making supply chain stability critical during periods of geopolitical uncertainty.

The meeting also assessed potential challenges and opportunities arising from the current situation, though no specific operational changes were announced.

Rajnath Singh defence roadmap Aatmanirbhar Bharat focus

Rajnath Singh directed officials to continuously study operational and technological lessons emerging from ongoing conflicts in West Asia.

“We need to formalise a comprehensive integrated roadmap for the next decade factoring in the lessons learnt, challenges and opportunities going forward whilst ensuring Aatmanirbharta and operational readiness across all fronts,” he said.

The term Aatmanirbharta refers to India’s policy focus on self reliance, particularly in defence manufacturing and technology development.

Officials were asked to incorporate these priorities into long term planning, with an emphasis on strengthening domestic capabilities while maintaining readiness.

The Defence Research and Development Organisation and other agencies are expected to play a central role in translating these directives into actionable plans.

The review comes as India continues to monitor global conflicts for lessons that could inform its own military doctrine, procurement strategies and technological development.

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XRISM finally solves famous star’s 50-year space mystery

A star visible to the naked eye has held a secret for more than half a century.

Gamma Cassiopeiae, a bright star in the constellation Cassiopeia, has puzzled astronomers since the 1970s with its unusually intense X ray emissions. [1]

Now, researchers using the X Ray Imaging and Spectroscopy Mission, a joint space observatory developed by Japan, the United States and Europe, say they have identified the source. [1]

The emissions come from an unseen white dwarf companion that pulls in material from the larger star and releases X rays as it does so. [1]

Gamma Cas X ray origin explained by white dwarf companion

The findings are based on high resolution observations from XRISM’s Resolve spectrometer, which can track subtle changes in X ray signals.

Researchers found that the hot plasma responsible for the X rays moves in sync with the orbit of the hidden companion star. [1]

This motion provided direct evidence that the emissions are linked to accretion, a process in which matter falls onto a dense object such as a white dwarf.

Lead author Yaël Nazé, an astronomer at the University of Liège in Belgium, said the result concludes decades of investigation.

“There has been an intense effort to solve the mystery of gamma Cas across many research groups for many decades. And now, thanks to the high precision observations of XRISM, we have finally done it,” Nazé said. [1]

For years, scientists had narrowed the explanation to two possibilities. One involved magnetic interactions between the star and its surrounding disc. The other suggested that a companion object was drawing in material and generating X rays.

The XRISM data supports the second explanation. [1]

Be stars gamma Cas history and unusual emission features

Gamma Cassiopeiae belongs to a class known as Be stars, a type of hot, rapidly rotating star surrounded by a disc of material.

The star’s unusual behavior was first noted in 1866 by Italian astronomer Angelo Secchi, who observed unexpected emission lines in its light spectrum. [1]

Those observations led to the classification of Be stars, which are known for ejecting material that forms a rotating disc around them.

By the mid 20th century, astronomers had detected that gamma Cas also had a low mass companion, though it remained invisible to direct observation. [1]

The discovery of strong X ray emissions in the 1970s added another layer to the mystery. The radiation was traced to extremely hot plasma, reaching temperatures of about 150 million degrees, far exceeding typical levels for such stars. [1]

Subsequent observations with space telescopes such as XMM Newton, the European Space Agency’s X ray observatory, NASA’s Chandra X ray Observatory, and the eROSITA telescope identified similar behavior in a small group of stars now known as gamma Cas type objects. [1]

XRISM discovery impact on binary star evolution research

The identification of a white dwarf companion resolves the origin of the X rays and provides a clearer picture of how these systems function.

In this model, material from the Be star’s disc spirals toward the white dwarf, heating up and emitting high energy radiation in the process.

Researchers say the findings also raise new questions about how such binary systems form.

White dwarf companions were expected to be common in systems with lower mass stars. The new results suggest they may instead occur more frequently with high mass Be stars. [1]

Alice Borghese, a research fellow at the European Space Agency specializing in high energy astrophysics, said earlier missions helped narrow the possibilities.

“XMM Newton did so much of the groundwork in ruling out various theories about gamma Cas. And now with the next generation of advanced instrumentation, XRISM has brought us over the finish line,” she said. [1]

The study highlights the role of international collaboration in space science. XRISM combines contributions from Japanese, European and American teams.

Matteo Guainazzi, the European Space Agency’s XRISM project scientist, said the result demonstrates the value of that cooperation.

“This wonderful result underlines the strong collaboration between XRISM’s Japanese, European and American teams,” he said. [1]

For astronomers, the long running puzzle of gamma Cas has shifted from speculation to measurement.

A mystery that began with unusual light signatures in the 19th century now has a defined mechanism grounded in observation.

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