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Astronomers said Thursday they have spotted a hot bubble of gas spinning clockwise around the black hole at the centre of our galaxy at “mind blowing” speeds.

The detection of the bubble, which only survived for a few hours, is hoped to provide insight into how these invisible, insatiable, galactic monsters work.

The supermassive black hole Sagittarius A* lurks in the middle of the Milky Way some 27,000 light years from Earth, and its immense pull gives our home galaxy its characteristic swirl.

The first-ever image of Sagittarius A* was revealed in May by the Event Horizon Telescope Collaboration, which links radio dishes around the world aiming to detect light as it disappears into the maw of black holes.

One of those dishes, the ALMA radio telescope in Chile’s Andes mountains, picked up something “really puzzling” in the Sagittarius A* data, said Maciek Wielgus, an astrophysicist at Germany’s Max Planck Institute for Radio Astronomy.

Just minutes before ALMA’s radio data collection began, the Chandra Space Telescope observed a “huge spike” in X-rays, Wielgus told AFP.

This burst of energy, thought to be similar to solar flares on the Sun, sent a hot bubble of gas swirling around the black hole, according to a new study published in the journal Astronomy and Astrophysics.

The gas bubble, also known as a hot spot, had an orbit similar to Mercury‘s trip around the Sun, the study’s lead author Wielgus said.

But while it takes Mercury 88 days to make that trip, the bubble did it in just 70 minutes. That means it travelled at around 30 percent of the speed of light.

“So it’s an absolutely, ridiculously fast-spinning bubble,” Wielgus said, calling it “mind blowing”.

A MAD theory

The scientists were able to track the bubble through their data for around one and half hours – it was unlikely to have survived more than a couple of orbits before being destroyed.

Wielgus said the observation supported a theory known as MAD. “MAD like crazy, but also MAD like magnetically arrested discs,” he said.

The phenomenon is thought to happen when there is such a strong magnetic field at the mouth of a black hole that it stops material from being sucked inside.

But the matter keeps piling up, building up to a “flux eruption”, Wielgus said, which snaps the magnetic fields and causes a burst of energy.

By learning how these magnetic fields work, scientists hope to build a model of the forces that control black holes, which remain shrouded in mystery.

Magnetic fields could also help indicate how fast black holes spin – which could be particularly interesting for Sagittarius A*.

While Sagittarius A* is four million times the mass of our Sun, it only shines with the power of about 100 suns, “which is extremely unimpressive for a supermassive black hole, Wielgus said.

“It’s the weakest supermassive black hole that we’ve seen in the universe – we’ve only seen it because it is very close to us.”

But it is probably a good thing that our galaxy has a “starving black hole” at its centre, Wielgus said.

“Living next to a quasar,” which can shine with the power of billions of suns, “would be a terrible thing,” he added.


Buying an affordable 5G smartphone today usually means you will end up paying a “5G tax”. What does that mean for those looking to get access to 5G networks as soon as they launch? Find out on this week’s episode. Orbital is available on Spotify, Gaana, JioSaavn, Google Podcasts, Apple Podcasts, Amazon Music and wherever you get your podcasts.
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New discovery explains how gold forms in Earth’s volcanic zones!

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New discovery explains how gold forms in Earth's volcanic zones!

A breakthrough discovery by an international team of scientists has highlighted the role of a gold-sulfur complex in the formation of gold deposits on Earth. The study, co-authored by Adam Simon, Professor of Earth and Environmental Sciences at the University of Michigan, was recently . It details the previously unknown conditions under which gold is transported from deep within the Earth’s mantle to the surface.

Role of the Gold-Trisulfur Complex

According to the research, published in the Proceedings of the National Academy of Sciences (2024), a unique gold-trisulfur complex forms under specific pressure and temperature conditions in the mantle, situated 30 to 50 miles beneath active volcanic zones. This complex, which has been debated in scientific circles, plays a significant role in the enrichment of gold in magma that travels to the surface. The findings shed light on why certain subduction zones, where tectonic plates converge, are particularly rich in gold deposits.

Volcanic Activity and Gold Deposits

The study highlights subduction zones around the Pacific Ring of Fire, where volcanic activity is prevalent, as key areas for gold formation. These regions, including locations such as New Zealand, Japan, Alaska, and Chile, provide the ideal geological environment for magma to carry gold from the mantle to surface deposits. The researchers link the processes behind volcanic eruptions to the mechanisms that concentrate gold in these zones.

Scientific Findings and Practical Applications

The researchers developed a thermodynamic model to simulate mantle conditions and confirm the existence of the gold-trisulfur complex. This model not only validates earlier theories about gold-sulfur interactions but also provides a clearer picture of the conditions required for gold-rich mineral systems to form.

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Study Reveals Genetic and Linguistic Roots of Indo-European Populations



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First Perentie Lizards Hatched at Los Angeles Zoo: A Major Breeding Milestone

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First Perentie Lizards Hatched at Los Angeles Zoo: A Major Breeding Milestone

Two perentie lizards, among the largest species of lizards globally, have hatched at the Los Angeles Zoo, marking the first time this species has been bred there. Native to Australia, these carnivorous reptiles are known for their impressive size, often exceeding 8 feet in length and weighing over 40 pounds. The zoo, which is one of the few facilities outside Australia to successfully breed them, is now home to the newly hatched pair, who are being carefully monitored in a controlled environment.

First Breeding Success Highlighted by Experts

According to reports from usnews.com, the perentie lizards were bred and hatched for the first time in the facility’s history. Byron Wusstig, curator at the Los Angeles Zoo, shared with the Associated Press that achieving this milestone is a significant accomplishment for the team. These lizards, classified as Varanus giganteus, are rarely seen in zoos outside their native Australia, despite not being endangered.

Special Care for Hatchlings in Early Stages

Reports confirm that the hatchlings are thriving under close observation by the zoo’s staff. They are being kept off-exhibit in a specially managed setting to ensure their health during these crucial initial months. The lizards will eventually join the Australia section of the zoo, near the Komodo dragon habitat, where the father is currently on display.

This species is characterised by its distinct brown skin adorned with cream or yellow markings. Their diet, as stated in reports, includes turtle eggs, insects, birds, small mammals, marsupials, and other reptiles, all of which are consumed whole. As per zoo officials, this breeding success highlights the capabilities of the institution in conserving and caring for unique species, contributing to the understanding of their behaviour and needs in captivity.

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Study Reveals Genetic and Linguistic Roots of Indo-European Populations

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Study Reveals Genetic and Linguistic Roots of Indo-European Populations

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Study Reveals Genetic and Linguistic Roots of Indo-European Populations

A comprehensive study involving 91 researchers, including Eske Willerslev from the Lundbeck Foundation GeoGenetics Centre at the University of Copenhagen, has provided critical insights into the genetic and linguistic origins of Indo-European populations. The findings, identify two significant migrations during the Bronze Age that contributed to the spread of steppe ancestry across the Mediterranean. The genetic research links Spanish, French and Italian populations to Bell Beaker ancestry, while Greek and Armenian populations have been connected directly to Yamnaya ancestry from the Pontic Steppe region.

Analyses of Steppe Ancestry Distribution

According to the study published on the preprint server bioRxiv, steppe ancestry in Western Europe is attributed to Bell Beaker populations, who combined their genetic profile with local Neolithic farmers. These migrations align with linguistic theories suggesting a shared origin for Italo-Celtic languages. In contrast, Greek and Armenian ancestry reflects direct Yamnaya influence, with no significant local admixture. This divergence between Eastern and Western Mediterranean populations aligns with the Italo-Celtic and Graeco-Armenian linguistic hypotheses.

Genomic and Strontium Isotope Studies

As per reports, the study sequenced 314 ancient genomes dated between 2,100 and 5,200 years ago from regions including Spain, Italy, Greece, and Turkey. A total dataset of 2,403 genomes was analysed, alongside 224 strontium isotope assessments to trace human mobility. Results showed active migration patterns during the Bronze Age, with non-local individuals identified in Greece, Cyprus and Italy. A notable finding was a Scandinavian individual in Cyprus, suggesting Mediterranean trade routes extended far beyond local boundaries.

Implications for Linguistic Migration Models

These findings substantiate linguistic theories connecting Italic and Celtic languages to Bell Beaker ancestry and Greek and Armenian languages to Yamnaya ancestry. The research contradicts alternative hypotheses, including Indo-Greek and Italo-Germanic models. This study provides a clearer understanding of the genetic and linguistic history of Indo-European populations, offering a vital reference for future investigations into ancient human migrations

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.


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