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A new model has been proposed that challenges the long-standing belief that black holes contain a singularity, a region where space and time break down. This theory suggests that black holes could exist without this problematic feature, reshaping our understanding. If accurate, this research could bridge the gap between general relativity and quantum mechanics, two fundamental yet conflicting theories of physics. The findings offer a fresh perspective on one of the most mysterious objects in the universe, potentially altering how black holes are studied.

The Issue with Singularities

According to a study published in Physics Letters B in February 2025, researchers modified Einstein’s field equations to prevent the formation of a singularity at the centre of a black hole. According to Einstein’s general theory of relativity, black holes form when massive stars collapse under their own gravity. It creates regions of space with extreme curvature. This leads to the formation of a singularity, where all known laws of physics break down.

Robie Hennigar, a researcher at Durham University in England, told Space.com that the singularity is the most mysterious and problematic part of a black hole. He said that it is where our concepts of space and time literally no longer make sense.

Revising Einstein’s Equations

In general relativity, gravity is described by Einstein’s field equations, which successfully predict the motion of planets, the expansion of the universe, and the formation of black holes. However, these equations also predict singularities, which many physicists view as a sign that general relativity is incomplete.

Pablo Antonio Cano Molina-Niñirola, a physicist at the Institute of Cosmos Sciences of the University of Barcelona, explained to Space.com that their approach modifies Einstein’s field equations to account for extreme gravitational conditions. Instead of relying on a complete theory of quantum gravity, the team uses an “effective theory” to approximate the missing physics.

Molina-Niñirola stated that this is a classical theory of gravity that is supposed to capture the effects of an assumed theory of quantum gravity. The model suggests that when space-time reaches extreme curvature, gravity behaves differently, preventing the formation of a singularity.

What Lies at the Core of a Black Hole?

With singularities removed from the equation, the next question is: what actually exists at a black hole’s center? According to Hennigar, the answer is a stable, highly curved region of space-time. Molina-Niñirola explained that in their model, the space-time collapse stops, and the singularity is replaced by a highly warped static region that lies at the core of the black hole.

Potential Implications for Cosmology

The findings may have significant implications for theoretical physics, particularly in the search for a unified theory of gravity. If black holes do not have singularities, they could serve as a bridge between general relativity and quantum mechanics.

One possibility explored by the study is that matter falling into a black hole could eventually exit through a white hole, potentially in another universe or a different part of our own.

The absence of singularities might leave an imprint on the early universe, detectable through gravitational wave observations. Molina-Niñirola noted that if dark matter turned out to be composed of tiny black holes, this would be an indirect proof in favour of the absence of singularities.

Looking Ahead

Molina-Niñirola concluded that ongoing and future observations of black hole mergers and cosmic background radiation may eventually provide evidence to support or refute the theory. For now, the concept of black holes without singularities remains an exciting development in the quest to understand the universe’s most enigmatic objects.

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Meteorite From Outer Solar System Challenges Planet Formation Timeline in Early Solar System

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Meteorite From Outer Solar System Challenges Planet Formation Timeline in Early Solar System

A minuscule meteorite seems to be rewriting the history of our solar system. The 50-gram Northwest Africa 12264 has brought a new understanding of when and how rocky worlds came together. Inner planets such as Earth and Mars were thought to have formed earlier than their more distant siblings, given temperatures and composition. But a new study of this meteorite, which originates from beyond the asteroid belt, suggests that the birth of planets throughout the solar system occurred tens of millions of years earlier than previously believed, narrowing the gap in time between the solar system’s inner and outer surfaces.

Outer Solar System Meteorite Reveals Rocky Planets Likely Formed Simultaneously Across the Galaxy

As per a study led by Dr Ben Rider-Stokes of The Open University and published in Communications Earth & Environment, the meteorite’s chemical makeup offers critical evidence. Its chromium and oxygen isotope ratios place its origin in the outer solar system. Most strikingly, lead isotope dating determined its age to be about 4.564 billion years, almost identical to basalt samples from the inner solar system that represent early planetary crusts.

These findings directly challenge the previous assumption that rocky planets beyond Jupiter formed two to three million years later due to their water-rich composition. Ice and water were thought to slow differentiation, the internal layering of planetary bodies. But this meteorite, with its outer solar birth and inner solar age, points to a far more synchronised process of rocky planet formation.

Scientists note that the discovery is also consistent with observations of exoplanetary systems. Based on this and past observations of disks of dust and gas around other stars, the evidence of planetesimals forming quickly and over large orbital separations adds to the argument that early solar system evolution may have been more universal than thought.

As trivial as the time difference might be in the context of a universe, the question is huge. A new timeline of planet formation is not only a retelling of Earth’s history but may also help determine how astronomers think about how planets form in the galaxy more generally, providing new hints about where and how in the galaxy Earth-like planets could take shape.

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NASA’s Hubble and Webb Discover Bursting Star Formation in Small Magellanic Cloud



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NASA’s Hubble and Webb Discover Bursting Star Formation in Small Magellanic Cloud

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NASA’s Hubble and Webb Discover Bursting Star Formation in Small Magellanic Cloud

Scientists from NASA observed the bursting expansion of gas, stars, and dust from the glittering territory of the dual star clusters using Hubble and Webb space telescopes. NGC 460 and NGC 456 stay in the Small Magellanic Cloud, which are open clusters, with dwarf galaxies and orbit the Milky Way. These clusters are part of the extensive star complex clusters and nebulae that are most likely to be linked to each other. Stars are born upon the collapse of clouds.

Hubble and Webb Reveal Explosive Star Births in Small Magellanic Cloud

As per a report from NASA, the open clusters are from anywhere from a few dozen to many young stars, which are loosely bound by gravity. The images captured by Hubble capture the glowing and ionised gas, which comes from stellar radiation and blows bubbles in the form of gas and dust, which is blue in colour. The infrared of Webb shows the clumps and delicate filament-like structures and dust, which is red in colour.

NGC 460 and NGC 456: A Window into Early Universe Star Formation

Hubble shows the images of dust in the form of a silhouette against the blocking light; however, in the images of Webb, the dust is warmed by starlight and glows with infrared waves. The blend of gas and dust between the stars of the universe is called the interstellar medium. The region holding these clusters is known as the N83-84-85 complex and is home to multiple, rare O-type stars. These are hot and extremely massive stars that burn hydrogen like the Sun.

Such a state mimics the condition in the early universe; therefore, the Small Magellanic Cloud gives a nearby lab to find out the theories regarding star formation and the interstellar medium of the cosmos’s early stage.

With these observations, the researchers tend to study the gas flow from convergence to divergence, which helps in refining the difference between the Small Magellanic Cloud and its dwarf galaxy, and the Large Magellanic Cloud. Further, it helps in knowing the interstellar medium and gravitational interactions between the galaxies.

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New Interstellar Object 3I/ATLAS Could Reveal Secrets of Distant Worlds

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New Interstellar Object 3I/ATLAS Could Reveal Secrets of Distant Worlds

The entry of a third known object into our solar system has been confirmed on July 1, 2025 by the astronomers. This object is named 3I/ATLAS, where 3I stands for “Third Interstellar”, having a highly hyperbolic (eccentricity ≈ 6.2) orbit, confirming it is not bound to the Sun but is a true interstellar visitor. Only two such visitors, 1I/ʻOumuamua (2017) and 2I/Borisov (2019), had been seen before. Notably, 3I/ATLAS appears to be the largest and brightest interstellar wanderer yet discovered.

Comparison with previous interstellars

According to NASA, astronomers from the ATLAS survey first spotted the object on July 1, 2025, using a telescope in Chile. It immediately drew attention for its unusual motion. Shortly after discovery, observers saw a faint coma and tail, leading to its classification as comet C/2025 N1 (ATLAS).

This comet-like appearance is shared with 2I/Borisov, the second interstellar visitor. Global observatories now track 3I/ATLAS. It poses no threat but offers a rare opportunity to study alien material. Since 1I/ʻOumuamua was observed only as it was leaving the solar system, it was difficult for astronomers to get enough data on it to confirm its exact nature — hence the crazy theories about it being an alien spaceship — though it’s almost certainly an asteroid or a comet.

Size and Significance

3I/ATLAS is much larger and brighter than earlier interstellar visitors. It is about 15 kilometers (km) [9 miles] in diameter, with huge uncertainty, compared to 100m for 1I/’Oumuamua and less than 1km for 2I/Borisov. This brightness and size makes it a a better target for study. Astronomers are planning to analyze its light for chemical signatures from its home system to get clues about the formation of distant planetary systems.

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