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With Winter coming, air pollution in India is going to once again hit crisis levels soon. At the individual level we can wear masks and use air purifiers in our homes, but more broadly, cities and municipalities have also been installing outdoor air purifiers over several years now — but do these actually work? Have smog towers and outdoor air purifiers made an impact on the air quality in India? Despite the outdoor air purifiers and smog towers, the PM2.5 concentration in India air is currently 5.2 times above the WHO annual air quality guideline. The air quality in India is simply not getting better even after all the money and efforts spent to curb the air pollution problem in the country. We talked to a number of experts to try and understand why this is, and whether there are any better solutions possible.

Cities like Mumbai have been deploying Wind Augmentation Purifying Unit (WAYU) since 2015, in an effort to cut down the air pollution problem in India. Major Indian cities like Delhi and Bengaluru have also resorted to installing outdoor purifiers and smog towers along the city roads in an effort to curb pollution problems. Delhi got a new smog tower in Connaught Place in August this year.

Yet, India stood third in a list of top ten countries that had the worst air quality in 2020, coming only behind Bangladesh and Pakistan. According to research by the Council on Energy, Environment, and Water (CEEW) — a Delhi-based policy research institute — Delhi’s air quality in winter 2020 was worse than winter 2019 despite the lockdown. The study also found out that Delhi residents were exposed to air that does not meet the National Ambient Air Quality Standards (60 µg/m3) for more than half of 2020 despite low economic activity levels for close to eight months (March to November) due to the pandemic-induced lockdown.

According to Tanushree Ganguly, an air quality researcher from CEEW, the air pollution that India is facing is an urban infrastructure problem. “If there is an unpaved road, it is bound to have more dust,” Ganguly said. “Vehicular pollution also results in air pollution. In winters, a significant amount of pollution also comes from biomass that people burn for their heating requirements.”

Are outdoor air purifiers a solution to air pollution problem?

WAYU devices, jointly developed by National Environmental Engineering Research Institute (NEERI), the Council of Scientific and Industrial Research (CSIR), and Indian Institute of Technology-Bombay (IIT-B) have been around since 2015. The Central Pollution Control Board had installed WAYU units across some major locations in Delhi in 2018.

“Its creators claim it can reduce pollution at busy traffic junctions by 40-60 percent,” Dr. Prashant Gargava, member secretary of the Central Pollution Control Board, had said at the time of installation.

“The air pollution levels change depending on the time it was measured,” Ganguly said. “So when was it measured, in what area is the air quality being improved — is it just within ten metres of the air purifiers or within 500 metres of the air purifier — all these factors need to be considered to show that it is really making any impact. I have not come across any publicly available research or database which clearly says that WAYU devices have actually impacted air quality in the 500 metre radius.”

“There is a constant dynamism in the system and you are not just trying to address sources of pollution which are present at the moment; you are also trying to address the sources which are outside the city,” she added. “I’m not sure how these filters are able to cater to these varying dynamics outdoors. I think the idea is to have credible evidence on their impact before we go ahead and have them across the city.”

Vivel Chattopadhyay, Senior Programme Manager of the Clean Air Programme at the Centre for Science and Environment (CSE), a research and advocacy organisation based in Delhi said that apart from the installation costs, outdoor air purifiers come with several added costs.

This includes the cost of maintenance, cost of the filters which will have to be changed periodically, components like sensors which require periodic calibration, operational costs, manpower, the cost of the land which is being occupied by the air pollutants and more. These are not easy to solve problems, but the companies making these solutions are also aware of them and working on solutions.

“We have nano-filters in our outdoor air purifiers which can be reused up to four times, thus saving a lot of maintenance costs, “ said Rajeev Krishna, founder of ATechTron, a product development company based in Bengaluru. ATechTron have installed their outdoor air purifiers in locations including Marathahalli junction, Whitefield, and PR Nagar in Bengaluru.

How can we really solve the air pollution problem?

CEEW had suggested in their research that Delhi needs a dedicated air quality forecasting cell to facilitate the rollout of preventive measures. “If we have the forecast for the next 72 hours, we can clearly see the contribution ratio to the pollution — for example, urban dust at night is the highest,” said Ganguly. “Perhaps, this is due to the trucks at night. The government can take measures to cut out the activities which they really can through forecasting — it’s very difficult to execute these activities due to the significant economic repercussions.”

“Wherever in the world where pollution reduction has happened in a big manner, the solution has been cleaner fuel and technology working to controlling pollution from the sources, better assessment and study of where the pollution is coming from,” said Chattopadhyay.

Chattopadhyay added that the amount of money that is being spent on outdoor air purifiers can be used to cut down the emission from the sources. “The same amount of money can be spent to buy electric buses, you can have waste collection and segregation centres. That will eliminate the source of the problems. That will give us better long term gains. Outdoor air purifiers are really futile efforts. Government is letting the pollution be released from the source. The emissions are taking place from industry, from vehicles, and multiple sources. Cutting down from the source will have a wider implication in terms of exposure too,” added Chattopadhyay.

Ganguly also suggested that the transit infrastructure, including waste collection, waste transport, and waste management infrastructure need to be improved. “In winters, a significant amount of pollution also comes from biomass that people burn for their heating requirements,” she noted. “The Delhi shelters are perhaps not able to cater to all the homeless people in Delhi. So I think it is also important how the government is planning on upgrading these existing shelters, so that at least their utilisation is better. At night, if these shelters can accommodate the homeless population, then their reliance on garbage or dry leaves for their heating requirements could be reduced.”

Chattopadhyay also added that tighter emission control norms must be in place. “Tighter emission control norms for power plants will lead to a reduction (in air pollution). The government has to put in the money into the right sources — cutting emissions from the sources and maintaining regulations. Smog towers are not a right policy decision. Such methods give a signal to the polluters that it is okay to pollute,” he said.

A bandage solution

Krishna, of ATechTron, disagreed with the researchers’ suggestions that forecasting and air quality monitoring is a better solution. He suggested that strategically placing outdoor air purifiers within a distance of two-three kilometres to each other throughout the city will surely lead to a reduction in air pollution.

Angad Daryani, founder of Praan, a deep tech startup which makes outdoor air purifiers also said that what the NCR government is doing with smog-free towers is non-scientific. When asked if outdoor air purifiers can really contribute to solving the pollution problem in India, he said that the outdoor air purifiers from Praan serve as a bandage solution to the pollution problem while we transition to cleaner energy.

I asked Ganguly if this was the case, but she remained unconvinced. “Let’s not call it a solution before we know for sure it is one,” she said. “Once the entire range of measures has been taken and if we still don’t see any significant impact, then perhaps this could be looked at as a solution. But this cannot precede all the other solutions. As a researcher, that is what I have an issue with.”


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A Nearby Supernova May End Dark Matter Search, Claims New Study

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A Nearby Supernova May End Dark Matter Search, Claims New Study

The pursuit of understanding dark matter, which comprises 85 percent of the universe’s mass, could take a significant leap forward with a nearby supernova. Researchers at the University of California, Berkeley, led by Associate Professor of Physics Benjamin Safdi, have theorised that the elusive particle known as the axion might be detected within moments of gamma rays being emitted from such an event. Axions, predicted to emerge during the collapse of a massive star’s core into a neutron star, could transform into gamma rays in the presence of intense magnetic fields, offering a potential breakthrough in physics.

Potential Role of Gamma-Ray Telescopes

The study was published in Physical Review Letters and revealed that the gamma rays produced from axions could confirm the particle’s mass and properties if detected. The Fermi Gamma-ray Space Telescope, currently the only gamma-ray observatory in orbit, would need to be pointed directly at the supernova, with the likelihood of this alignment estimated at only 10 percent. A detection would revolutionise dark matter research, while the absence of gamma rays would constrain the range of axion masses, rendering many existing dark matter experiments redundant.

Challenges in Catching the Event

For detection, the supernova must occur within the Milky Way or its satellite galaxies—an event averaging once every few decades. The last such occurrence, supernova 1987A, lacked sensitive enough gamma-ray equipment. Safdi emphasised the need for preparedness, proposing a constellation of satellites, named GALAXIS, to ensure 24/7 sky coverage.

Axion’s Theoretical Importance

The axion, supported by theories like quantum chromodynamics (QCD) and string theory, bridges gaps in physics, potentially linking gravity with quantum mechanics. Unlike neutrinos, axions could convert into photons in strong magnetic fields, providing unique signals. Laboratory experiments like ABRACADABRA and ALPHA are also probing for axions, but their sensitivity is limited compared to the scenario of a nearby supernova. Safdi expressed urgency, noting that missing such an event could delay axion detection by decades, underscoring the high stakes of this astrophysical endeavour.

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Fastest-Moving Stars in the Galaxy May be Piloted by Aliens, New Study Suggests

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Fastest-Moving Stars in the Galaxy May be Piloted by Aliens, New Study Suggests

Intelligent extraterrestrial civilisations might be utilising stars as massive interstellar vehicles to explore the galaxy, according to a theory proposed by Clement Vidal, a philosopher at Vrije Universiteit Brussel in Belgium. His research suggests that alien species could potentially accelerate their binary star systems to traverse vast cosmic distances. While such a concept is purely hypothetical and unproven, Vidal’s recent paper, which has not undergone peer review, raises intriguing possibilities about advanced extraterrestrial engineering.

Concept of Moving Star Systems

The study was published in the Journal of the British Interplanetary Society. As per a report by LiveScience, the idea revolves around the notion that alien civilisations, instead of building spacecraft for interstellar travel, might manipulate entire star systems to travel across the galaxy. Vidal highlights binary star systems, particularly those involving neutron stars and smaller companion stars, as ideal candidates. Neutron stars, due to their immense gravitational energy, could serve as anchors for devices designed to propel the system by selectively ejecting stellar material.

Vidal explained in the paper that uneven heating or manipulation of magnetic fields on a star’s surface could cause it to eject material in one direction. This process would create a reactionary thrust, propelling the binary system in the opposite direction. The concept provides a way to travel while preserving planetary ecosystems, making it a theoretically viable method for species reliant on their home systems.

Known Examples with High Velocities

Astronomers have identified hypervelocity stars, such as the pulsars PSR J0610-2100 and PSR J2043+1711, which exhibit high accelerations. While their movements are believed to be natural phenomena, Vidal suggests they could be worth further investigation to rule out potential artificial influences.

This theory adds an unconventional angle to the search for intelligent life, expanding possibilities beyond traditional methods of exploration like searching for signals or probes. The research underscores the importance of considering advanced and unconventional methods aliens might employ to navigate the galaxy.

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Hubble Telescope Finds Unexpectedly Hot Accretion Disk in FU Orionis

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Hubble Telescope Finds Unexpectedly Hot Accretion Disk in FU Orionis

NASA’s Hubble Space Telescope has provided new insights into the young star FU Orionis, located in the constellation Orion. Observations have uncovered extreme temperatures in the inner region of its accretion disk, challenging current models of stellar accretion. Using Hubble’s Cosmic Origins Spectrograph and Space Telescope Imaging Spectrograph, astronomers captured far-ultraviolet and near-ultraviolet spectra, revealing the disk’s inner edge to be unexpectedly hot, with temperatures reaching 16,000 kelvins—almost three times the Sun’s surface temperature.

A Star’s Bright Outburst Explained

First observed in 1936, FU Orionis became a hundred times brighter in months and has remained a unique object of study. Unlike typical T Tauri stars, its accretion disk touches the stellar surface due to instabilities. These are caused by the disk’s large mass, interactions with companion stars, or material falling inwards. Lynne Hillenbrand, a co-author from Caltech, in a statement said that the ultraviolet brightness seen exceeded predictions, revealing a highly dynamic interface between the star and its disk.

Implications for Planet Formation

As per a report by NASA, the study holds significant implications for planetary systems forming around such stars. The report further quoted Adolfo Carvalho, lead author of the study, saying that while distant planets in the disk may experience altered chemical compositions due to outbursts, planets forming close to the star could face disruption or destruction. This revised model provides critical insights into the survival of rocky planets in young star systems, he further added.

Future Investigations on FU Orionis

The research team continues to examine spectral emission lines in the collected data, aiming to map gas movement in the star’s inner regions. Hillenbrand noted that FU Orionis offers a unique opportunity to study the mechanisms at play in eruptive young stars. These findings, published in The Astrophysical Journal Letters, showcase the ongoing value of Hubble’s ultraviolet capabilities in advancing stellar science.

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