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World Malaria Day: How climate change is worsening the spread of the disease – Firstpost

A word of caution. Do not take malaria lightly. It continues to be one of the top life-threatening diseases. There were an estimated 249 million cases of malaria around the world in 2022 with over 600,000 deaths, the World Health Organisation reported.

Many low and middle-income countries still struggle to put a leash on the deadly disease. It was thought to have been eliminated in higher-income countries like the US and nations in Europe. But now is making its way back. The reason? Climate change, say experts.

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This World Malaria Day, let’s take a closer look at how this disease spreads and exactly how climate change is set to worsen it.

How does malaria spread?

As per the WHO, the mosquito-borne disease is transmitted to people through the bites of infected female Anopheles mosquitoes. The person experiences high fever, nausea, body aches and shaking chills.

Though malaria is treatable, it can cause kidney failure, seizures, mental confusion, coma, and even death in severe cases if not diagnosed and treated in time, the US Centers for Disease Control (CDC) said.

The mosquitos that carry the parasite majorly thrive in hot and humid climatic conditions, such as in tropical countries of Asia and Africa where crowded neighbourhoods, stagnant water, poor sanitation and lack of access to treatment and prevention materials are contributing factors.

African nation, Cameroon started world’s first malaria vaccination for children this year. Source: The United Nations

Notably, Dr Daniel Ngamije, who directs the WHO malaria programme, said that cases in 2022 were concentrated in just five countries: Pakistan, Nigeria, Uganda, Ethiopia and Papua-New Guinea, with climate change being a direct contributor in three of them.

What does the picture in Asia look like?

As per a World Bank report, South Asia, including eight countries like India, Pakistan and Bangladesh, is the most vulnerable region to climate shocks, and extreme weather events and is experiencing a “new climate normal”.

Pakistan, for example, battled catastrophic flooding in 2022 during which more than a third of the country was underwater and 33 million people were affected. As the water receded, it saw a five-fold increase in malaria cases, with as many as 2.6 million cases as compared to 500,000 a year ago, according to WHO data.

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After devastating floods in 2022, Pakistan saw five-fold increase in malaria cases, as per WHO. Reuters File

“It was just the perfect storm for malaria,” Dr Schapira, a WHO consultant who reviewed Pakistan’s national malaria programme, said.

Increasing variations in climate and decreasing insecticide and drug resistance are also expected to increase the suitability for malaria transmission in the northeastern regions of India such as Uttar Pradesh, Bihar, Karnataka, Odisha, Rajasthan, Madhya Pradesh and Pondicherry, Dr Andrew Karanja Githeko, a climate expert wrote in a paper titled “Malaria and climate change”.

“The changing climate poses a substantial risk to progress against malaria, particularly in vulnerable regions. Sustainable and resilient malaria responses are needed now more than ever, coupled with urgent actions to slow the pace of global warming and reduce its effects,” said Dr Tedros Adhanom Ghebreyesus, WHO Director-General.

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How common are outbreaks in Europe and the US?

Malaria is no longer an anomaly in the West. As global temperatures soar, breaking records each year, mosquito-borne diseases such as malaria and dengue are making their presence across the world, an expert was quoted as saying by The Guardian report.

Rachel Lowe, who leads the global health resilience group at the Barcelona Supercomputing Center in Spain, has cautioned that outbreaks of mosquito-borne diseases are poised to spread across currently unaffected parts of northern Europe, Asia, North America, and Australia over the next few decades.

“Global warming resulting from climate change means that the disease vectors carrying and spreading malaria and dengue fever can inhabit more regions, leading to outbreaks in areas where people are likely to lack immunity and where public health systems are unprepared,” Lowe told the publication.

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Global warming resulting from climate change means that the disease vectors carrying and spreading malaria and dengue fever can inhabit more regions. Reuters File

The Asian tiger mosquito, which carries dengue fever, has become established in 13 European countries, according to the European Centre for Disease Prevention and Control. As of 2023, it was present in Italy, France, Spain, Malta, Monaco, San Marino, Gibraltar, Liechtenstein, Switzerland, Germany, Austria, Greece, and Portugal.

The US is also seeing a rise in cases.

According to John Hopkins University, the US reported the first homegrown malaria cases in 20 years last year. Usually each year, 2,000–2,500 malaria cases related to travel to Sub-Sahara or Southeast Asia regions where the disease is prevalent are reported.

However, in 2023, nine locally transmitted cases were contracted by individuals who hadn’t recently visited those areas raising concerns over the re-emergence or emergence of mosquito-borne diseases in new places.

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Now we are in 2024. Science continues to make great advances. But to fight malaria, we might need more than just medical breakthroughs. We need a healthier planet.

With inputs from agencies

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Hungry white dwarf stars eat heavy metals – Earth.com

White dwarfs, the remnants of stars like our Sun but only about the size of Earth, make up 97% of our galaxy’s stars. These dead stars, dense and compact, represent a common endpoint for stellar evolution, transforming the Milky Way into a sort of celestial necropolis.

One long standing puzzle has been the composition of these stars, particularly the unexpected presence of heavy metals like silicon, magnesium, and calcium on their surfaces. This phenomenon is at odds with the typical behavior expected from such dense objects, where heavy elements should sink rapidly.

“We know that if these heavy metals are present on the surface of the white dwarf, the white dwarf is dense enough that these heavy metals should very quickly sink toward the core. So, you shouldn’t see any metals on the surface of a white dwarf unless the white dwarf is actively eating something,” said lead author Tatsuya Akib, a graduate student in planetary sciences at the University of Colorado Boulder (CU Boulder).

This “eating” refers to the absorption of nearby objects such as comets or asteroids, also known as planetesimals. This process has intrigued astronomers as a potential key to understanding the metallic surface composition of white dwarfs.

“Natal kick” may be responsible 

In a recent publication, the experts offer a new explanation for this behavior. They propose that a “natal kick” – a displacement during formation due to asymmetric mass loss observed in white dwarfs – might be responsible for the dynamics that lead to these celestial bodies consuming nearby planetesimals.

The team’s computer simulations showed that in 80% of scenarios, this kick resulted in the elongation and alignment of the orbits of comets and asteroids within 30 to 240 astronomical units of the white dwarf. Remarkably, about 40% of the consumed planetesimals originated from retrograde, or counter-rotating, orbits.

100 million years of simulations 

Extending their simulations over 100 million years, the team observed that the elongated orbits of nearby planetesimals persisted and moved in unison, a phenomenon previously undocumented. 

“This is something I think is unique about our theory: we can explain why the accretion events are so long-lasting,” explained senior author Anne-Marie Madigan, an astrophysicist at CU Boulder. “While other mechanisms may explain an original accretion event, our simulations with the kick show why it still happens hundreds of millions of years later.”

These findings suggest that the presence of heavy metals on a white dwarf’s surface can be attributed to the continuous accretion of smaller celestial bodies it encounters.

White dwarf interactions 

Madigan’s team, which specializes in gravitational dynamics, explored in more detail the interactions between white dwarfs and their gravitational environments. 

“Simulations help us understand the dynamics of different astrophysical objects,” Akiba said. “So, in this simulation, we throw a bunch of asteroids and comets around the white dwarf, which is significantly bigger, and see how the simulation evolves and which of these asteroids and comets the white dwarf eats.”

The researchers plan to expand their simulations to include interactions with larger planetary bodies, anticipating that white dwarfs may also consume larger objects like planets.

White dwarfs are a lens to the past and future 

These discoveries not only provide insights into the life cycle of white dwarfs but also illuminate the broader processes of solar system evolution and the chemical complexities involved. 

“The vast majority of planets in the universe will end up orbiting a white dwarf. It could be that 50% of these systems get eaten by their star, including our own solar system. Now, we have a mechanism to explain why this would happen,” Madigan said.

“Planetesimals can give us insight into other solar systems and planetary compositions beyond where we live in our solar region. White dwarfs aren’t just a lens into the past. They’re also kind of a lens into the future,” concluded co-author Sarah McIntyre, an undergraduate student at CU Boulder.

More about white dwarf stars 

White dwarf stars are fascinating remnants of stars similar to our Sun, found in the final stages of their stellar life cycle. When a star has exhausted the nuclear fuel at its core, it sheds its outer layers and leaves behind a dense core, which we observe as a white dwarf. 

These stars are incredibly dense and compact; despite being similar in size to Earth, they contain about as much mass as the Sun.

Cooling process 

The surface of a white dwarf is characterized by its extreme temperatures, initially very hot but gradually cooling over billions of years. This cooling process is slow due to the star’s small surface area relative to its mass, which makes it less efficient at radiating heat away.

Black dwarfs

White dwarfs are typically composed of carbon and oxygen, which were generated by the fusion of helium in the star’s previous evolutionary stages. The fate of a white dwarf is to continue to cool and fade away, eventually becoming what is known as a “black dwarf,” although the universe is not old enough for any white dwarfs to have reached this stage yet.

Life cycle of stars 

These stars are also significant in the study of astrophysics because they serve as one of the possible endpoints of stellar evolution and play a key role in our understanding of the life cycle of stars. 

Additionally, white dwarfs are often involved in exotic phenomena such as type Ia supernovae, which occur when a white dwarf accretes matter from a companion star to the point where it undergoes a catastrophic explosion, playing a critical role in measuring cosmic distances.

The study is published in The Astrophysical Journal Letters.  

Image Credit: NASA and H. Richer (University of British Columbia)

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Heartbreaking search for missing father – Chronicle

A Gwanda family in Matabeleland North is in turmoil as it is desperately searching for their missing father, who wandered off from the hospital where he was admitted.

The Moyo family is searching for their father Mr Keeper Moyo, who was admitted in hospital on April 26, after suffering a seizure.

His daughter – Ms Loveness ‘Lavila’ Moyo said he was also showing signs of memory loss.

“Our plan was to move him to Bulawayo on the 30th for further tests and scans but that’s the day he disappeared. The hospital staff that was monitoring patients in his ward apparently fell asleep without closing the doors. Patients who saw him, said they last saw him going to the bathroom,” said Ms Moyo.

She said the nurses only noticed that he was missing after a few hours.

As days pass with no sign of their father, the family has banded together to search every corner of the town.

They comb through streets, knock on doors, and put up posters in hopes of finding any clue to their father’s whereabouts.

“There was no security at the gate and no one saw anything. So we have been searching blindly because we don’t know which direction he took. We don’t have leads. We have also placed alerts everywhere. We have tried involving the police but they haven’t helped so we are using private cars and deploying people at different locations to search.”
“Some are on bikes, others get dropped off by trucks and sometimes spend the night searching. We have even hired loud hailing services to go in and around townships,” she said.

 More details to follow…

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‘Better than graphene’ material development may improve implantable technology – Phys.org

‘Better than graphene’ material development may improve implantable technology

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'Better than graphene' material development may improve implantable technology
Dipanjan Pan, left, Dorothy Foehr Huck & J. Lloyd Huck Chair Professor in Nanomedicine and professor of materials science and engineering and of nuclear engineering, with Teresa Aditya, postdoctoral researcher in nuclear engineering, and David Skrodzki, graduate research assistant in materials science and engineering, in Pan’s lab. All three were authors of the study. Credit: Dipanjan Pan

Move over, graphene. There’s a new, improved two-dimensional material in the lab. Borophene, the atomically thin version of boron first synthesized in 2015, is more conductive, thinner, lighter, stronger and more flexible than graphene, the 2D version of carbon.

Now, researchers at Penn State have made the material potentially more useful by imparting chirality—or handedness—on it, which could make for advanced sensors and implantable medical devices. The chirality, induced via a method never before used on , enables the material to interact in unique ways with different biological units such as cells and protein precursors.

The team, led by Dipanjan Pan, Dorothy Foehr Huck & J. Lloyd Huck Chair Professor in Nanomedicine and professor of materials science and engineering and of , published their work—the first of its kind, they said—in ACS Nano.

“Borophene is a very interesting material, as it resembles carbon very closely including its atomic weight and electron structure but with more remarkable properties. Researchers are only starting to explore its applications,” Pan said.

“To the best of our knowledge, this is the first study to understand the biological interactions of borophene and the first report of imparting chirality on borophene structures.”

Chirality refers to similar but not identical physicality, like left and right hands. In molecules, chirality can make biological or chemical units exist in two versions that cannot be perfectly matched, as in a left and right mitten. They can mirror each other precisely, but a left mitten will never fit the right hand as well as it fits the left hand.

Borophene is structurally polymorphic, which means its can be arranged in different configurations to give it different shapes and properties, much like how the same set of Lego blocks can be built into different structures. This gives researchers the ability to “tune” borophene to give it various properties, including chirality.

“Since this material has remarkable potential as a substrate for implantable sensors, we wanted to learn about their behavior when exposed to cells,” Pan said. “Our study, for the first time ever, showed that various polymorphic structures of borophene interact with cells differently and their cellular internalization pathways are uniquely dictated by their structures.”

The researchers synthesized borophene platelets—similar to the cellular fragments found in blood—using solution state synthesis, which involves exposing a powdered version of the material in a liquid to one or more external factors, such as heat or pressure, until they combine into the desired product.

“We made the borophene by subjecting the boron powders to high-energy sound waves and then mixed these platelets with different amino acids in a liquid to impart the ,” Pan said. “During this process, we noticed that the sulfur atoms in the amino acids preferred to stick to the borophene more than the amino acids’ nitrogen atoms did.”

The researchers found that certain , like cysteine, would bind to borophene in distinct locations, depending on their chiral handedness. The researchers exposed the chiralized borophene platelets to mammalian cells in a dish and observed that their handedness changed how they interacted with cell membranes and entered cells.

According to Pan, this finding could inform future applications, such as development of higher-resolution medical imaging with contrast that could precisely track cell interactions or better drug delivery with pinpointed material-cell interactions. Critically, he said, understanding how the material interacts with cells—and controlling those interactions—could one day lead to safer, more effective .

“Borophene’s unique structure allows for effective magnetic and electronic control,” Pan said, noting the material could have additional applications in health care, sustainable energy and more. “This study was just the beginning. We have several projects underway to develop biosensors, drug delivery systems and imaging applications for borophene.”

More information:
Teresa Aditya et al, Chiral Induction in 2D Borophene Nanoplatelets through Stereoselective Boron–Sulfur Conjugation, ACS Nano (2024). DOI: 10.1021/acsnano.4c01792

Citation:
‘Better than graphene’ material development may improve implantable technology (2024, May 6)
retrieved 6 May 2024
from https://phys.org/news/2024-05-graphene-material-implantable-technology.html

This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
part may be reproduced without the written permission. The content is provided for information purposes only.


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