New 'Black Hole Star' Object Discovered by Astronomers
Astronomers have identified a unique cosmic object, dubbed a 'black hole star,' that exhibits characteristics of both a black hole and an enormous star from the early universe.

Astronomers have announced the discovery of an entirely new class of celestial object, a phenomenon they've termed a "black hole star." This groundbreaking find, observed in the early universe, presents characteristics that bridge the gap between massive stars and black holes, potentially offering new insights into the formation of supermassive black holes.
The object, officially designated MoM-BH*-1 (Mirage or Miracle-Black Hole-1), was detected as an unusually bright, red source in observations of the distant cosmos. While its immense size, comparable to the entire solar system, suggests it is a star, its energy output of approximately 100 billion times that of known stars aligns it more closely with black holes. This duality led researchers to classify it as a novel type of cosmic entity.
Rohan Naidu, lead author of the study published in the journal Nature and an astronomer at the University of Hawaii, explained the object's peculiar nature. "It is so swaddled within shrouds of dense gas that it effectively radiates in a manner reminiscent of stellar phenomena," Naidu stated. "It is a very special thing to find an object with no comparison given the vast stores of data on billions of stars, galaxies, and black holes that we have in our archival databases. MoM-BH*-1 is one in a billion!"
The discovery is linked to other enigmatic findings from the early universe, specifically the "little red dots." These are compact, bright objects observed at high redshifts, meaning their light has traveled for billions of years to reach Earth. Initially, these objects caused speculation that instruments like the James Webb Space Telescope (JWST) might be malfunctioning. However, their existence is now seen as a crucial clue to understanding the universe's nascent stages.
Probing the Early Universe's Mysteries
The nature of these "little red dots" and the formation of supermassive black holes—which weigh millions to billions of solar masses—have long been puzzles for astrophysicists. Naidu suggests that these new "black hole stars" might represent the "birth story of possibly every supermassive black hole." He further posits that the "little red dots" could be observed when a black hole star is situated within a larger galaxy.
Traditionally, astronomers attribute reddish hues in cosmic objects to the presence of dust, which efficiently absorbs and scatters blue light. However, the spectral characteristics of MoM-BH*-1 do not solely align with dust obstruction. Instead, analysis suggests a significant contribution from a large cloud of ionized gas, with minimal dust involvement. A key observation is the abrupt disappearance of the object's light below a certain wavelength, a phenomenon known as a Balmer break. This behavior, combined with its high luminosity, leads to the conclusion that it exhibits "several of the quintessential properties of both black holes and stars," according to Naidu. He emphasized that MoM-BH*-1 is particularly notable because it "is effectively outshining its entire host galaxy, and so we are seeing 'pure' black hole star light."
The implications of this discovery extend to our understanding of the universe's initial expansion and structure. If the distinct color of these early cosmic objects stems from gas rather than dust, it could help explain why the earliest supermassive black holes appear to be far more massive than predicted by current cosmological models. The research also aligns with other recent studies that have detected traces of gas accretion around active black holes in the early universe. This adds another layer to the complex picture of cosmic evolution.
Researchers are eager to conduct further investigations into these objects. Naidu and his team have already secured additional JWST observation time, scheduled to begin in December 2026. They aim to "lock down the detailed physics of these remarkable objects—how massive exactly are they, and what do their 'stellar' features tell us about their 'stellar' atmospheres?" The scientific community is abuzz with excitement, with Naidu drawing parallels to the 1960s and 70s when the discovery of quasars revolutionized the study of supermassive black holes. "And now, thanks to JWST, and thanks to how delightfully surprising the universe is, we are reliving that very special period when we are rewriting the textbooks and filling out new chapters for things that we didn’t even know existed!" he remarked.
