Astronomers Discover 'Black Hole Star' in the Early Universe, Solving the Mystery of Webb's Little Red Dots
Researchers using the James Webb Space Telescope have identified a new class of cosmic object—a supermassive black hole enveloped in a dense cocoon of gas that shines like a star.
For decades, the textbook distinction between stars and black holes was absolute: stars are engines of nuclear fusion that radiate light, while black holes are gravitational sinks that consume it. But the early universe, it turns out, did not respect that boundary. Astronomers have confirmed the existence of a "black hole star"—an entirely new class of cosmic object that looks and shines like an enormous star but is powered from within by a rapidly growing supermassive black hole.[1][2]
The discovery, published in the journal Nature, centers on an object named MoM-BH*-1, nicknamed "The Cliff." Located roughly 13 billion light-years away, the object formed just 660 million years after the Big Bang. At first glance, it resembles a star the size of our entire solar system, glowing with a brilliant, deep red light.[2][6]
However, the energy output of MoM-BH*-1 defies stellar physics. The object is releasing 100 billion times more energy than any known star could physically generate through nuclear fusion. That staggering blast of power is a signature of a black hole aggressively feeding on surrounding matter.[1][3]
The mechanism behind a black hole star is a masterclass in extreme astrophysics. Instead of a core fusing hydrogen into helium, the center of this object is a supermassive black hole—roughly 100,000 times the mass of our Sun. Surrounding this black hole is an incredibly dense, turbulent cocoon of partially ionized hydrogen gas. As the black hole consumes the gas, the friction and gravitational forces generate immense heat and light, causing the entire gas envelope to glow like a stellar atmosphere.[1][5][6]
"We have found a new type of astrophysical object," explained Dr. Rohan Naidu of the MIT Kavli Institute for Astrophysics and Space Research, the study's lead author. "It shines with the energy typically associated with black holes, but at the same time bears signatures classically associated with stars."[2]
This finding directly solves one of the most debated mysteries of the James Webb Space Telescope (JWST) era. Since JWST began operations in 2022, astronomers have been puzzled by an abundance of "little red dots" scattered across the early universe. Initially, these dots were thought to be incredibly dense, ancient galaxies that had somehow formed far too early in cosmic history, challenging standard cosmological models.[3][4]
The data from MoM-BH*-1 suggests a different reality. By analyzing the deep spectrum of the object's light, researchers realized that the redness is not caused by galactic dust obscuring a collection of stars. Instead, the black hole star is enshrouded in pure gas, which shifts its light toward the red end of the spectrum without blocking the view—much like how atmospheric scattering makes a sunset appear red on Earth.[6]
Crucially, this new class of object provides the missing link for how supermassive black holes grew so massive so quickly. Astronomers have long struggled to explain the existence of billion-solar-mass black holes in the early universe, as there simply wasn't enough time for them to grow through standard accretion. The black hole star phase acts as a "turbo-charged" growth period, allowing a seed black hole to rapidly gorge on a massive, stable envelope of gas.[4][5]
While the evidence for MoM-BH*-1 is robust, the research team is explicit about the limits of current observations. It remains unproven exactly how long this black hole star phase lasts before the central black hole entirely consumes or blows away its gaseous cocoon. Furthermore, while astronomers suspect that many of the other "little red dots" are also black hole stars, confirming this will require deep spectroscopic follow-ups for each individual object.[4][6]
The discovery marks a rare moment where theoretical physics and observational astronomy perfectly align to rewrite cosmic history. By proving that black holes and stars can exist as a single, hybrid entity, astronomers have not only solved the mystery of the little red dots but also illuminated the infancy of the supermassive black holes that anchor galaxies today.[3][5]
Where opinion splits
Observational Astronomers
Focus on the data resolving the 'little red dot' mystery.
For observational astronomers, the black hole star model elegantly solves the crisis triggered by JWST's early images. The telescope had found too many 'little red dots' that appeared to be massive galaxies forming impossibly early. By reclassifying these objects as single, hyper-luminous black hole stars, the data no longer breaks standard models of galaxy formation. Instead, it shifts the extreme mass from a sprawling galaxy of stars into a single, highly efficient central engine.
Theoretical Cosmologists
Focus on the implications for supermassive black hole growth.
Theorists have long debated the 'seed' problem: how supermassive black holes reached billions of solar masses within the first billion years of the universe. The black hole star provides a physical mechanism for this rapid growth. By remaining embedded in a dense, stable cocoon of gas, the black hole can feed continuously at extraordinary rates without the radiation pressure blowing the food source away, acting as a crucial stepping stone in cosmic evolution.
Key points
- Astronomers have identified a new class of cosmic object called a 'black hole star.'
- The object, MoM-BH*-1, is powered by a central black hole rather than nuclear fusion.
- It produces 100 billion times more energy than any known star.
- The discovery explains the mysterious 'little red dots' found by the James Webb Space Telescope.
Unanswered questions
- How long the 'black hole star' phase lasts before the gas envelope is consumed or dispersed.
- Whether all supermassive black holes go through this specific hybrid phase during their infancy.
- The exact mechanism that allows the dense gas cocoon to remain stable while the black hole feeds at such extreme rates.
How we got here
2022
The James Webb Space Telescope begins operations and discovers unexplained 'little red dots' in the early universe.
March 2025
The initial discovery of the object MoM-BH*-1 is announced on preprint servers alongside another candidate, 'The Cliff'.
August 2026
Astronomers publish peer-reviewed findings in Nature, officially classifying the object as a 'black hole star'.
- Observational Astronomers
- Value the resolution of the JWST 'little red dot' anomaly through direct spectral evidence.
- Theoretical Cosmologists
- Focus on how this discovery solves the long-standing 'seed' problem of supermassive black hole formation.
Perspectives this story doesn't cover
- Alternative gravity theorists who previously used the 'little red dots' to argue against the standard cosmological model
Sources
[1]MIT NewsObservational AstronomersAstronomers discover a 'black hole star'
Read on MIT News →
[2]The GuardianObservational AstronomersAstronomers claim to have discovered a new kind of cosmic object, a black hole 'star'
Read on The Guardian →
[3]CBS NewsObservational AstronomersNewly discovered 'black hole star' could solve mystery of strange red dots spotted in the early universe
Read on CBS News →
[4]Space.comTheoretical CosmologistsJames Webb Space Telescope finds evidence the mysterious 'little red dots' are black hole stars
Read on Space.com →
[5]Live ScienceTheoretical CosmologistsJames Webb telescope discovers 'black hole star'
Read on Live Science →
[6]Europa.euTheoretical CosmologistsEarliest known black hole star found at cosmic dawn
Read on Europa.eu →
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