Dark Stars: Astronomers May Have Found a New Kind of Star Powered by Dark Matter

By | October 3, 2025

The Mysterious Birth of Dark Stars

 

For decades, scientists have believed that stars shine because of nuclear fusion — the process that powers our Sun and every other star we see in the night sky. But new evidence suggests that some of the universe’s very first stars might have followed a completely different path. These hypothetical objects, called “dark stars,” may not rely on fusion at all. Instead, they could be powered by the mysterious force of dark matter annihilation.

 

First proposed in 2007, dark stars have remained purely theoretical — until now. Thanks to new data from the James Webb Space Telescope (JWST), astronomers are closer than ever to confirming their existence. If proven real, these cosmic giants could completely reshape our understanding of how the first stars and black holes formed.

 

 

 

What Are Dark Stars?

 

Dark stars are not “dark” in the usual sense. In fact, they could be millions of times brighter than the Sun. The name comes from their unusual power source: dark matter, the invisible substance thought to make up about 85% of the universe’s total matter.

 

In the early universe, about 100 million years after the Big Bang, clouds of hydrogen and helium collapsed under gravity to form the first stars. But some scientists theorized that if dark matter particles were present in high enough densities, they might collide and annihilate, releasing energy. This extra energy could counteract gravity, slowing the collapse and creating a new kind of star — one that shines without nuclear fusion.

 

 

 

JWST’s Surprising Discoveries

 

The James Webb Space Telescope, launched in 2021, is designed to look deep into cosmic history. It has now spotted several extremely bright, ancient objects dating back to just a few million years after the Big Bang. These objects are unusually large, round, and emit light signatures that match dark star simulations.

 

A key piece of evidence comes from spectroscopy — the study of how objects emit and absorb light. Recent JWST data shows a potential signature of helium ions that researchers believe could only be produced by dark matter-powered stars. This “smoking gun” evidence, described in a 2025 preprint by Cosmin Ilie and colleagues, has given the dark star theory new momentum.

 

 

 

The Scientific Debate

 

Not everyone is ready to declare victory. Some astronomers suggest that these bright objects could simply be supermassive primordial stars — extremely large stars formed in the early universe through more conventional means. Others point out that the detection of oxygen in some candidate regions is unexpected if these objects were purely dark stars. This could mean they are part of mixed populations, where dark stars and normal stars coexist.

 

Despite the debate, most scientists agree on one thing: whatever these objects are, they represent something new and unexplained.

 

 

 

Why Dark Stars Matter

 

If confirmed, dark stars could solve one of astronomy’s biggest mysteries — how supermassive black holes appeared so early in the universe. Traditional models struggle to explain how black holes grew so massive so quickly. But if dark stars grew to enormous sizes — possibly millions of times the mass of the Sun — and then collapsed, they could have provided the perfect seeds for the first black holes.

 

The discovery of dark stars would also be the first direct evidence of dark matter interactions beyond gravity, bringing us closer to solving one of science’s greatest puzzles.

 

 

 

A Glimpse Into the Universe’s First Light

 

The search for dark stars is far from over, but JWST’s observations mark a major leap forward. As new data pours in and future telescopes join the hunt, we may soon know whether dark stars truly existed and with them, uncover a missing chapter of cosmic history.

If they are real, dark stars won’t just rewrite the story of how the first stars formed. They might reveal how the universe itself turned darkness into light.

 

Source:

Cosmin Ilie et al., “Spectroscopic Supermassive Dark Star Candidates,” arXiv (2025)

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