logo
This Might Be the Most Massive Black Hole Ever Discovered

This Might Be the Most Massive Black Hole Ever Discovered

WIRED2 days ago
Aug 13, 2025 5:47 AM New measurements of the galaxy at the heart of the 'Cosmic Horseshoe' indicate that it could house the most massive object ever seen in the universe.
Astronomers have identified what could be a new supermassive black hole, and with an estimated mass 36 billion times that of the sun, it is about 10,000 times heavier than the black hole at the center of the Milky Way. This would make it among the most massive objects ever detected.
The finding, published in the Monthly Notice of the Royal Astronomical Society, was made by researchers from the Institute of Cosmology and Gravitation at the University of Portsmouth in the UK in collaboration with the Federal University of Rio Grande in Brazil. The scientists located the signs of the new supermassive black hole within a gravitational lens known as the 'Cosmic Horseshoe,' pictured below. A gravitational lens occurs when the gravity of a massive object, such as a galaxy, is so great that it bends light and time that passes near it, distorting light traveling from behind.
The Cosmic Horsehoe was discovered by the Hubble telescope in 2007. The galaxy LRG 3-757 sits at its center, while the blue horseshoe shape surrounding this yellow-colored object is distorted light emitted from another galaxy beyond it. LRG 3-757 is one of the most massive galaxies ever observed by astronomers, having a mass 100 times that of the Milky Way, and it sits approximately 5.6 billion light-years away from Earth.
The gravitational lens known as the Cosmic Horseshoe, so named because of the appearance of the incomplete ring of blue light that surrounds its central galaxy, LRG 3-757. Photograph: NASA/ESA
Thanks to this luminous structure, astronomers have been able to calculate the mass of the black hole that presumably lies at the center of LRG 3-757 (while not definitively proven, large galaxies are assumed to have a black hole at their center). Although there are no direct observations of this black hole, measurements of the motion of light in the ring and the velocity of stars in the inner regions of the galaxy are consistent with the presence of an ultramassive black hole. 'By combining these two measurements we can be completely confident that the black hole is real,' Thomas Collett, professor of astrophysics at the University of Portsmouth, said in a press statement.
Collett also suggests that a black hole of such proportions could only originate from the merger of two supermassive black holes resulting from the collision of galaxies. Astronomers are still debating whether this will be the shared fate of our galaxy, the Milky Way, and neighboring Andromeda. What About TON 618 and the Like?
Any astronomy enthusiast knows that the most massive object found in the universe so far is potentially TON 618. According to the most widespread estimates, this black hole has a mass equivalent to 66 billion suns, almost twice that of the Cosmic Horseshoe.
However, scientists are cautious about labelling TON 618 as the most massive object ever seen. Being located more than 10 billion light-years away, its host galaxy and surrounding objects cannot be observed in detail. What little is known about it comes from analysis of its brightness and from theoretical models that allow us to estimate its size. The uncertainty is too high to consider it the most massive black hole known.
In contrast, the Portsmouth researchers argue that the Cosmic Horseshoe black hole offers greater observational certainty, unlike distant, almost mythological holes like TON 618. As such, they claim that their discovery could represent the most massive black hole confirmed to date.
This story originally appeared on WIRED en Español and has been translated from Spanish.
Orange background

Try Our AI Features

Explore what Daily8 AI can do for you:

Comments

No comments yet...

Related Articles

ExtractoDAO's Revolutionary Tech Predicted 300M☉ Primordial Black Hole — Now Confirmed by JWST
ExtractoDAO's Revolutionary Tech Predicted 300M☉ Primordial Black Hole — Now Confirmed by JWST

Associated Press

timean hour ago

  • Associated Press

ExtractoDAO's Revolutionary Tech Predicted 300M☉ Primordial Black Hole — Now Confirmed by JWST

'Simulations from 2024–2025 matched JWST's discovery of a 300M-solar-mass black hole, confirming DUT's predictive power.' 'DUT incorporates JWST discoveries seamlessly, predicting extreme cosmic structures before they are observed.'— oel Almeida, CEO – ExtractoDAO Lab CURITIBA, PARANá, BRAZIL, August 15, 2025 / / -- DUT Quantum Technology Anticipated a 300 Million Solar Mass Primordial Black Hole: Prediction Confirmed by JWST and Published Before the Official Announcement Based on 2024–2025 simulations, the Dead Universe Theory Simulator reproduced the masses, redshifts, and spectral characteristics now confirmed by CAPERS-LRD-z9 observations published in The Astrophysical Journal. The 6 August 2025 announcement in The Astrophysical Journal, reporting the discovery of a black hole with 300 million solar masses only 500 million years after the Big Bang, confirms a prediction recorded by the Dead Universe Theory (DUT) Quantum Simulator months prior to the official disclosure. While traditional models such as ΛCDM still struggle to explain the rapid growth of such massive black holes in the primordial universe, the Dead Universe Theory (DUT) interprets these objects as gravitational fossils within a dead cosmological structure — a present-day continuous spacetime fabric in which the observable universe is embedded. These objects are thermodynamically stabilized and detectable as Small Red Dots (SRDs) or obscured active galactic nuclei. Contrary to some misconceptions, DUT does not postulate that the observable universe originated from another, separate universe. The framework asserts that there is only one universe, and that the observable domain exists in a state of gravitational collapse within this larger structural continuum, composed of fine-scale constituents of that same universe. To claim otherwise — suggesting the existence of other universes — would fall into the realm of pseudoscience, since no empirical proof currently supports the existence of any universe beyond our own. 'Mainstream science is visibly uncomfortable with the flood of discoveries from JWST — from SRDs to the identification of supermassive black holes so early in cosmic history — given that many models, such as ΛCDM, did not anticipate these extremes. In contrast, the Dead Universe Theory (DUT) is ready to incorporate any JWST observation, operating consistently both on the 13.8-billion-year scale with singularity and on the extended 180-billion-year scale without singularity. While the mainstream attempts to redefine itself to accommodate these findings, the DUT community is growing organically on social media — a clear sign that its predictive, manageable framework is in tune with both the present and the future of cosmology.' — Joel Almeida, Scientific Leader, DeSci Lab, ExtractoDAO Alignment Between DUT Predictions and JWST Observations The analysis of the article reveals a remarkable alignment between DUT's predictions and JWST's observations of SRDs/LRDs. The following table summarizes the main points of convergence: The Dead Universe Theory (DUT) Simulator predicted, in advance, the existence of supermassive black holes in the primordial universe, with masses equal to or greater than 10⁸ M⊙, low star formation rates, and predominantly infrared spectral signatures. These predictions were recorded and published on Zenodo prior to the release of observational data by the CAPERS program conducted with the James Webb Space Telescope (JWST). On 6 August 2025, a study led by Anthony Taylor and his team, published in The Astrophysical Journal Letters, confirmed the detection of a black hole with approximately 300 million solar masses, formed about 500 million years after the Big Bang. The observed characteristics fully match the parameters simulated by DUT, validating the predictive robustness of the model. The DUT team expresses its appreciation to Dr. Anthony Taylor and collaborators for their scientific contribution, which, through independent observations, experimentally confirmed predictions previously published. 'Perhaps the time has come to shake the so-called 'cosmic seeds.' We see an intellectual dishonesty in the way data and mathematics are being handled, as we are creating a generation of young astrophysicists and cosmologists frustrated with ΛCDM. Every new discovery and detected object is forced into the framework of cosmic dust or other elements, with the claim that they 'shouldn't exist' — yet without accepting that the Big Bang has failed in its predictions. Is there something wrong with that? No. But ΛCDM, as it stands, refuses falsifiability, which is why it has become pseudoscience. Meanwhile, DUT has embedded self-refutation code in its simulators, losing points if it introduces concepts that cannot be falsified — such as multiverses, an endless sequence of Big Bangs — while the Big Bang itself continues to show its flaws.' — Eduardo Rodrigues, CTO, ExtractoDAO The simulator, developed by ExtractoDAO S.A., had already modeled compact, quiescent objects with masses ≥ 10⁸ M⊙, low star formation rates, and infrared spectral signatures — exactly the profile observed by the CAPERS program team using JWST. 'When we published the prediction on Zenodo ( ), there was no observational record of objects with these characteristics at this timescale. DUT generated this prediction from non-singular gravitational principles and entropic gradients, without any post-observation adjustment. Now, JWST has confirmed exactly this scenario.' — Joel Almeida, Creator of DUT ExtractoDAO created the first DeSci simulator. The startup's plans now focus on an online version integrated with cloud infrastructures such as IBM and Microsoft to allow real-time connections with telescope data. For strategic reasons, the first version is entirely offline, with data imported manually — introducing delays in research but ensuring privacy and certainty for researchers that ExtractoDAO has no access to their data. Additionally, since the company has not yet received external funding, this approach reduces infrastructure costs. 'DUT not only predicted primordial black holes but now projects the cosmos' future: structures at z≈20 and sub-0 K states. Simulations in DUT Quantum and DUT General Relativity are open for community validation. Predictive, verifiable science in action! ' This predictive accuracy — rare in contemporary cosmology — reinforces DUT's robustness as a scientific anticipation tool, capable of guiding observational campaigns even before data collection begins. Joel Almeida almeida ExtractoDAO LABS email us here Visit us on social media: LinkedIn Instagram YouTube X Legal Disclaimer: EIN Presswire provides this news content 'as is' without warranty of any kind. We do not accept any responsibility or liability for the accuracy, content, images, videos, licenses, completeness, legality, or reliability of the information contained in this article. If you have any complaints or copyright issues related to this article, kindly contact the author above.

Decades-long quest ends as scientists tame rare carbon ring once seen only in gas form
Decades-long quest ends as scientists tame rare carbon ring once seen only in gas form

Yahoo

time3 hours ago

  • Yahoo

Decades-long quest ends as scientists tame rare carbon ring once seen only in gas form

Chemists at the University of Oxford have achieved a rare feat in molecular science — the synthesis of a cyclocarbon that is stable enough for spectroscopic characterisation in solution at room temperature. The breakthrough, led by Oxford's Department of Chemistry, paves the way for in-depth studies of these unusual carbon allotropes under everyday laboratory conditions. Until now, such rings could only be observed fleetingly under extreme environments, such as in the gas phase or at cryogenic temperatures. The only previous example of a molecular carbon allotrope stable enough to study under normal conditions was the 1990 synthesis of fullerenes by Krätschmer and colleagues. Oxford's new work marks the first advance of its kind in over three decades. Threaded design boosts stability The team synthesised cyclo[48]carbon as a [4]catenane — a molecular architecture in which the C48 ring is threaded through three other macrocycles. These protective macrocycles act like molecular shields, physically blocking reactive species from reaching the delicate carbon ring. This design, combined with the choice of a larger cyclocarbon with reduced strain, allowed the molecule to persist in solution at 20°C for an impressive 92-hour half-life. The researchers also fine-tuned the unmasking step, which includes the transformation of a precursor molecule into the final product, to use mild conditions, further protecting the carbon ring. Characterisation confirmed the structure using mass spectrometry, NMR, UV-visible, and Raman spectroscopy. A single intense ^13C NMR resonance from all 48 sp^1 carbon atoms revealed that each carbon occupies an equivalent environment — strong evidence for the symmetrical cyclocarbon catenane. Years in the making Lead author Dr Yueze Gao said: 'Achieving stable cyclocarbons in a vial at ambient conditions is a fundamental step. This will make it easier to study their reactivity and properties under normal laboratory conditions.' For senior author Professor Harry Andersen, the result caps off more than a decade of work. 'This achievement marks the culmination of a long endeavour to synthesise cyclocarbon catenanes, based on the hope that they might be stable enough to study at room temperature,' he said. 'The original grant proposal was written in 2016, based on preliminary results from 2012–2015. It is satisfying to have reached this point, because there were many times when the goal seemed unrealistic and unachievable. This work would not have been possible without the outstanding facilities for NMR spectroscopy in the Department of Chemistry at Oxford,' Andersen added. The research brought together expertise from multiple UK institutions, including the University of Manchester, the University of Bristol, and the Central Laser Facility at Rutherford Appleton Laboratory. By proving that cyclocarbons can be stabilised in a bottle at room temperature, the work opens the door to exploring their chemical reactivity, optical behaviour and potential technological applications. For a class of molecules once thought too reactive to tame, Oxford's cyclocarbon catenane may be just the beginning of a new chapter in carbon chemistry. The findings have been published in the journal Science. Solve the daily Crossword

DOWNLOAD THE APP

Get Started Now: Download the App

Ready to dive into a world of global content with local flavor? Download Daily8 app today from your preferred app store and start exploring.
app-storeplay-store