Connect with us

Published

on

Glaciers have long served as nature’s deep freezers, preserving the physical characteristics of past climates and the genetic blueprints of ancient life forms, including viruses. As the planet’s climate continues to shift, scientists are increasingly looking to these frozen archives to understand how pathogens have historically responded to environmental changes. By studying viral genomes extracted from glacial ice, researchers from Ohio State University have uncovered how these ancient viruses adapted to Earth’s fluctuating climate over the past 41,000 years.

A Glimpse into Ancient Viral Communities

The team, composed of microbiologists and paleoclimatologists such as Lonnie Thompson, Virginia Rich, Matthew Sullivan, and Ellen Mosley-Thompson, focused their efforts on the Guliya Glacier located on the Tibetan Plateau. This glacier is an invaluable resource, containing layers of ice that have captured the genetic material of viruses from different periods in Earth’s history. The researchers drilled into the glacier, collecting ice cores that represent nine distinct time intervals spanning over 41,000 years. As highlighted in a study, published by The Conversation, by analysing the viral genomes within these samples, they were able to trace the evolution and adaptation of viral communities through three major cold-to-warm cycles.

Their analysis led to the recovery of 1,705 viral genomes, a discovery that significantly expands the known catalogue of ancient viruses preserved in glaciers. Remarkably, only about one-fourth of these viral species have any resemblance to the viruses previously identified in global metagenomic datasets. This suggests that many of the viruses found in the Guliya Glacier may have originated locally, highlighting the unique viral biodiversity of the region.

Viral Evolution and Climate Change

One of the study’s key findings was the significant variation in viral communities between cold and warm climatic periods. For instance, the viral community from around 11,500 years ago, which coincides with the transition from the Last Glacial Stage to the Holocene, was found to be distinct from other periods. This indicates that the shifts in climate played a crucial role in shaping viral communities. Changes in wind patterns, temperature fluctuations, and other environmental factors likely influenced which viruses were preserved and how they evolved over time.

To delve deeper into these interactions, the researchers used computer models to compare the viral genomes with those of other microbes present in the same environment. They discovered that many of these ancient viruses frequently infected Flavobacterium, a type of bacteria commonly found in glacial environments. The study also found that the viruses carried auxiliary metabolic genes, which they likely stole from their bacterial hosts. These genes, related to essential metabolic functions such as the synthesis and breakdown of vitamins and amino acids, may have helped the viruses survive in the extreme conditions of the glacier by enhancing the fitness of their hosts.

Implications for Understanding Climate Change

This research offers a unique perspective on how life has responded to climatic changes over tens of thousands of years. By studying these ancient viral communities, scientists gain valuable insights into how viruses might continue to evolve in response to ongoing global climate change. The findings also underscore the importance of glaciers as repositories of Earth’s climatic and biological history.

As glaciers continue to melt due to contemporary climate change, the preserved genetic material within them is at risk of being lost. This makes it all the more urgent to study these ancient records while they remain accessible. The work of Thompson, Rich, Sullivan, and Mosley-Thompson at Ohio State University highlights the critical role of glaciers in revealing the long-term interactions between climate and life on Earth.

Understanding how ancient viruses adapted to past climatic conditions can inform future research in both virology and climate science, offering a window into the potential challenges and changes that may arise as the planet’s climate continues to evolve.

Continue Reading

Science

Sun Unleash a 600,000-Mile Filament in Fiery Eruption

Published

on

By

Sun Unleash a 600,000-Mile Filament in Fiery Eruption

A stunning solar eruption captured on video on the night of May 12-13 has revealed a 600,000-mile-long filament blasting away from the sun’s northern hemisphere. The outburst occurred around 8 p.m. EDT (0000 GMT) and spanned a distance more than twice that between Earth and the moon. A massive solar filament suspended above the sun’s surface became unstable and erupted, blasting a CME into space along with a cloud of plasma and magnetic energy. Preliminary models show Earth is nowhere in the firing range of this fiery ejection, but researchers are still watching the phenomenon closely.

Sun’s 600,000-Mile-Long ‘Angel-Wing’ Eruption Stuns Skywatchers, Signals Rising Solar Activity

As per the Space.com report, the eruption originated from a filament structure composed of dense, cooler solar plasma held aloft by magnetic fields. These structures often appear as dark ribbons across the sun’s disk and can become unstable without warning. Solar observers noted that this latest eruption dwarfed similar recent events, both in scale and intensity. Aurora chaser Jure Atanackov remarked that the CME from the blast was among the most spectacular seen this year, although fortunately, it is headed north and will miss Earth.

The event, dubbed the “angel-wing” or “bird-wing” eruption by observers online, was widely shared among solar watchers. Vincent Ledvina, another aurora chaser, noted its incredible visual impact, describing it as a sight worth watching on loop. The eruption is, in fact, so long, by more than a million kilometres, that it is of scientific interest and visually striking as well. Geomagnetic storms resulting from this kind of CME can affect satellites, communication systems, and even Earth.

Although it foreshadows the unpredictable nature of our host star, this particular CME does not pose a threat to Earth at the moment. Solar activity is ramping up as we approach the peak of Solar Cycle 25 in 2025. What’s more, more — and maybe more Earth-threatening — solar explosions could follow.
As a reminder of the formidable and delicate forces at play relatively close by on Earth, the sun remains a source of wonder for astronomers and skywatchers alike.

For the latest tech news and reviews, follow Gadgets 360 on X, Facebook, WhatsApp, Threads and Google News. For the latest videos on gadgets and tech, subscribe to our YouTube channel. If you want to know everything about top influencers, follow our in-house Who’sThat360 on Instagram and YouTube.


SpaceX Fires Up Starship Upper Stage for Ninth Test Flight in Static Fire Trial



Apple Unveils Accessibility Nutrition Labels, Magnifier for Mac, Braille Access and More

Continue Reading

Science

New Study Challenges Fuzzy Dark Matter with Stronger Mass Constraint

Published

on

By

New Study Challenges Fuzzy Dark Matter with Stronger Mass Constraint

Over 80 years, dark matter has been a great mystery for the researchers. Elusive of direct observation, it has made its existence known only by the gravitational impacts it makes on cosmic structures. Even though there is a lot of indirect evidence of its existence, the real nature of dark matter is still unknown. An important attribute of its particle is mass. While past studies have constrained the mass of fermionic dark matter using quantum principles like Pauli’s exclusion principle, bosonic dark matter remained less constrained. In a recent study, scientists have estimated a new lower bound on the mass of ultra-lightweight bosonic dark matter particles.

About the study

According to the study published in Physical Review Letters, the mass of ultralight bosonic dark matter must be more than 2 × 10-21 electron volts (eV), 100 times more than previous estimates using Heisenberg’s uncertainty principle.

The team of researchers, led by the first author of the study, Tim Zimmermann, a Ph.D. candidate at the Institute of Theoretical Astrophysics, University of Oslo, focused their method on the data of Leo II, the Milky Way’s satellite galaxy. It is a dwarf galaxy 1,000 times smaller than the Milky Way. By analyzing the internal motions of stars within Leo II—heavily influenced by dark matter—the team derived 5,000 possible dark matter density profiles using a tool called GRAVSPHERE.

They compared these with profiles generated by quantum wave functions of various dark matter particle masses. If the particle is too light, quantum fuzziness spreads it too thinly, preventing it from forming the observed structures. The study concluded that the dark matter particle must have a mass greater than 2.2 × 10⁻²¹ electron volts (eV)—over 100 times more than previous lower estimates.

Impact on dark matter studies

The findings have significant implications for popular ultralight dark matter models, particularly fuzzy dark matter, which typically proposes particles with masses around 10-22 ev.

Looking ahead, the team plans to extend their methodology to mixed dark matter scenarios, where dark matter is composed of particles with different masses.

For the latest tech news and reviews, follow Gadgets 360 on X, Facebook, WhatsApp, Threads and Google News. For the latest videos on gadgets and tech, subscribe to our YouTube channel. If you want to know everything about top influencers, follow our in-house Who’sThat360 on Instagram and YouTube.


iPhone 17 Air Said to Be Thinner Than Samsung Galaxy S25 Edge; Battery Capacity Leaked



Home Projector Market to Double In Next 4 Years, South and West Key for BenQ India: Rajeev Singh

Continue Reading

Science

NASA’s Perseverance Captures Deimos Before Dawn in Striking Martian Sky Image

Published

on

By

NASA’s Perseverance Captures Deimos Before Dawn in Striking Martian Sky Image

NASA’s Perseverance rover has delivered a striking early morning image of Mars’ moon Deimos, taken just before dawn on March 1, 2025 — Sol 1433 of the mission. Captured at 4:27 a.m. local time using the rover’s left navigation camera, the view combines 16 long-exposure shots taken over 52 seconds. Each frame used the maximum exposure setting of 3.28 seconds, enabling the camera to glimpse faint celestial features in Mars’ dim pre-dawn sky. Though the image appears hazy due to low light and digital noise, the effort reveals a rare visual of Deimos suspended in the Martian atmosphere.

Perseverance’s Celestial Snapshot Reveals Deimos, Distant Stars, and Martian Sky Dynamics

As per a report from NASA’s Jet Propulsion Laboratory, the brightness of Deimos is accompanied by multiple white specks across the sky, many of which are likely caused by image noise. Some of them could be cosmic rays hitting the sensor while exposing. Two bright spots, Regulus and Algieba, are easily found in the image. It adds perspective on the rover’s unique view of things, these stars, which belong to the Leo constellation. The image was stitched together onboard and transmitted later to Earth, where researchers analysed the result.

These make the resultant composition an example of other possible roles of the Perseverance rover as an observational instrument apart from geology and surface exploration. While atmospheric haze and digital distortion make it difficult to show in full clarity, the long-exposure effort shows the faintness with which Martian moons and nearby stars can, in fact, still be tracked under controlled conditions. Deimos appears brighter due to its reflective nature and proximity during this early-morning observation.

Researchers believe this type of celestial photography may enhance understanding of Mars‘ sky conditions and moon dynamics. Deimos and Phobos, the Red Planet’s two moons, are of growing interest as potential markers for future orbit-based missions. Capturing them from the surface during optimal lighting conditions offers new insights into their behaviour.

NASA continues to push imaging capabilities on Mars through Perseverance’s tools. With each sol, even distant cosmic views — like Deimos before dawn — offer new visual science from the Martian frontier.

Continue Reading

Trending