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Roaming black holes may tell the hidden history of galaxies

Confirmed

Science Desk

In Short: These findings, published in The Astrophysical Journal Letters, suggest that massive clouds of cold gas coalesced at the center of early galaxies and collapsed to form black holes, known as the Direct-Collapse Black Hole (DCBH) scenario.

NASA’s Webb Finds Possible ‘Direct Collapse’ Black Hole - 54655737347
Photo: James Webb Space Telescope / Wikimedia Commons (CC BY 4.0)

Astronomers using the Cosmic Archaeology Tool (CAT) have detected massive black hole seeds forming as early as 500 million years after the Big Bang, challenging existing models of black hole formation.

The CAT, a semi-analytic model used to interpret high-redshift sources, revealed that massive black hole seeds could form via direct collapse as early as 13.64 billion years ago.

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This discovery is significant because it challenges the traditional model where stars collapse at the end of their lives to form black holes that gradually merge to create supermassive black holes (SMBHs).

In a separate study, astronomers used radio observations to detect hydrogen emissions from two periods in cosmic history, advancing a technique called hydrogen intensity mapping.

This technique, which uses the collective radio emissions of many galaxies to map large volumes of space, allowed MeerKAT to detect distant hydrogen emissions without the need for optical surveys.

The signal traveled for roughly four to five billion years before reaching Earth, offering a way to study the universe's structure during an earlier chapter of its history.

Dr. Zhaoting Chen, a study co-author, noted, “Neutral hydrogen is one of the key ingredients for understanding how galaxies form and evolve.”

The findings could help researchers investigate both the development of galaxies and the distribution of matter across the universe.

Astronomers also observed 'little red dots' using the James Webb Space Telescope, which they suspect could be giant stars with black holes hidden inside them.

These observations suggest that the dots are the visible part of a population of super-Eddington black holes, and that there are many more waiting to be found.

The wider the range of emissions, the faster the hydrogen clouds are flying, indicating the presence of a more massive black hole.

These findings add to the growing body of evidence that supermassive black holes form early in the universe's history, challenging previous theories.

What this adds

These findings build on previous WarpBeat reports suggesting that 'little red dots' observed by the JWST could be forming supermassive black holes.

Background

In the spring of 2025, astronomers announced the discovery of 'little red dots' that could be the early stages of supermassive black holes, challenging previous theories.

New research suggests the mysterious Little Red Dots observed by the JWST could be forming supermassive black holes.

What's confirmed

What's still developing

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