RESOLVING THE LEDGER
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Add as preferred source Astronomers at MIT and elsewhere have spotted an extremely bright red spot in the early universe. The object resembles an enormous star, roughly the size of our solar system. But it also is putting out 100 billion times more energy than any known star can physically produce. In fact, such energies are closer to what a black hole might generate.
The curious combination suggests that the red spot is an entirely new type of astrophysical source. The astronomers are calling it a "black hole star."
In a paper appearing in the journal Nature , the team presents its analysis of the new object, which it discovered using NASA's James Webb Space Telescope (JWST). The telescope spotted the bright red dot in the very early universe, just a few hundred million years after the Big Bang.
The scientists conclude that the most likely explanation for the strange red dot is that it is a mashup of a black hole and a star—a combination that has never been observed until now. The object is likely a hugely dense cloud of gas, powered not by standard nuclear fusion but by a central black hole.
"Our picture of this object is evolving very rapidly," says lead author Rohan Naidu, a NASA Hubble Fellow and Pappalardo Fellow at MIT's Kavli Institute for Astrophysics and Space Research (MKI). "We think there is a central black hole that is 100,000 times as massive as the sun. And around this black hole, there would be this very extended envelope of gas that looks like a star the size of the solar system. It's huge."
If the bright red dot is indeed a black hole star, it would help solve the identity of other mysterious "little red dots" that have appeared in nearly every deep-space image JWST has taken to date.
"These little red dots seem to be everywhere in the early universe but essentially disappear by the present day," Naidu says. "What exactly these objects are has been one of the most debated topics of the JWST era."
The study's MIT co-authors are MKI Director Robert Simcoe, the Bruno B. Rossi Professor of Experimental Physics, and Wendy Sun '26, along with collaborators from multiple other institutions.
Naidu and his colleagues didn't intend to find a black hole star. They were looking for the most distant, earliest galaxies as part of a survey they named "Mirage or Miracle" (MoM). The team used the JWST to look into deep space, back when the universe was a few hundred million years old. Their goal was to look for galaxies that actually formed at those early times.
"There's been this puzzle of many bright galaxies showing up at extremely early times," Naidu says. "What we found was that what looks like an extremely bright early galaxy, also known as a 'miracle,' in some cases actually could be a 'mirage.'"
As they looked through JWST's images for intriguing sources to target with their survey, they noticed a feature that stood out from the rest: a dot that was very red and very bright.
"When we see something very red in the universe, we often assume that it is surrounded by dust, like soot or ash," Simcoe explains. "Just as wildfire smoke from Canada recently made the sky in Boston look bright red, astronomical objects can also appear redder than their intrinsic color when you see them through a veil of dust."
But there were other signatures in the light that didn't quite match what physicists expect from dust. The team also observed another strange pattern: The dot's light was extremely bright, except below certain wavelengths, where the light completely disappeared.
This spectral drop-off is known as a "Balmer break"—a signature traditionally associated with dense gas soaking up photons in the atmospheres of stars that are a few hundred million years old. Vega, one of the brightest stars in the night sky, shows exactly this pattern.
"The break we observed in this object is the deepest break we have ever observed in any object, ruling out 'ordinary' stars as the source," Naidu says. "But it made us wonder if we were seeing a new kind of 'stellar atmosphere,' but on a spectacular scale."
What's more, the red dot's light contained almost no signature of metals or any elements other than hydrogen and helium. "It was truly singular in so many ways," Naidu says.
To puzzle out what the source of the red dot could be, the team ran simulations of different scenarios to see what combination of astrophysical features could produce the red dot's distinctive color.
"We started to ask: Could you make something that red using just hydrogen, without any dust?" Simcoe says. "To our surprise, it turns out you can, if you have an extremely dense screen of hydrogen, so dense that it looks more like the surface of an enormous star than a wispy interstellar nebula."
Their simulations pointed to the red dot possibly being a powerful enshrouded energy source, surrounded by an extremely dense cocoon of hydrogen. If this were the case, it would explain the light-blocking Balmer break and the lack of anything other than hydrogen and helium that the astronomers observed. But it still wouldn't explain the object's extreme brightness.
"You have something that looks a bit like a star but is 100 billion times brighter," Naidu says. "That means you can't be powering this by nuclear fusion, which is the energy source that sits at the heart of all the stars we have."
Black holes, however, routinely produce energy at the scales the team observed. Naidu and his colleagues incorporated an active, accreting black hole into their simulations of the hydrogen-cocooned star and varied the black hole's mass, along with other parameters.
They then compared the resulting brightness of the simulated "black hole star" with the brightness that JWST observed from the red dot.
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