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Astronomers Spot a Galaxy Candidate With No Stars—A Cosmic First?

Researchers have uncovered an enigmatic object named Cloud 9, which stands out as perhaps the most compelling example to date of a galaxy devoid of stars. This groundbreaking discovery was detailed in a recent study available on arXiv.
Scientists detected a vast accumulation of neutral hydrogen gas but found no accompanying light from stars.
This finding could reshape our understanding of galaxy formation and evolution.
If validated, Cloud 9 might represent a unique class of cosmic entities long predicted by theory but rarely observed, opening new avenues for investigating hidden galaxy formation processes across the cosmos.

A Cosmic Entity Existing Without Starlight

The team identified an extraordinary space object named Cloud 9 that houses a substantial volume of gas but lacks any visible stars. Unlike typical galaxies, which are recognized by the glow of billions of stars, this structure was revealed through radio waves emitted by neutral hydrogen, appearing nearly invisible in optical surveys. This challenges the expectation that large gas reservoirs automatically spark star formation and indicates some galaxies could remain elusive in traditional observations.

To verify if faint stars were hidden within Cloud 9, researchers conducted extremely deep optical imaging. Their aim was to exclude the possibility that it’s simply a faint galaxy with an aged or sparse stellar population. The results showed no detectable starlight, suggesting the area is rich in gas but practically devoid of stars, making Cloud 9 a fascinating candidate for a galaxy without stars.

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Lead investigator Ignacio Trujillo from the Instituto de Astrofísica de Canarias commented on the breakthrough to Space.com.

“But the most striking aspect of our research was the absolute emptiness of the image at the location of Cloud 9. When you look at an image reaching those depths and see nothing where a structure containing a million solar masses of gas should be, it is genuinely remarkable,” Trujillo said. “Most objects in the universe leave some trace of light. Cloud 9 does not. That silence is, in its own way, the most compelling result we could have obtained.”

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Composite gri-band color image of the region centered on Cloud-9. The SDSS image is combined with an ultra-deep HiPERCAM zoom focused on Cloud-9. Scattered illumination from the bright star HD 111859 (V=8.09 mag), positioned just outside the HiPERCAM field at the bottom left, influences the lower-left corner of the ultra-deep view. No stellar light is detected in the Cloud-9 area down to 31.4 mag/arcsec2 (g-band). Background whitening at the edges is due to increased noise from extensive dithering.

Unveiling the Mystery of Dark or Starless Galaxies

The concept of galaxies largely composed of gas but lacking stars has been theorized for decades. Models suggest some objects might gather hydrogen gas and dark matter without sparking the star formation needed to shine brightly. Known as dark galaxies or starless galaxies, these entities have proven elusive because they cannot be detected via the usual stellar light signatures that identify distant galaxies.

The identification of Cloud 9 was made possible by merging radio detections of neutral hydrogen emissions with ultra-sensitive optical imaging. Radio data pinpoint large gas reserves invisible to traditional means, while optical searches strive to uncover faint starlight. This combined approach allows astronomers to discover potential galaxies beyond typical survey capabilities.

The original paper on arXiv emphasizes that confirming such an object depends on excluding all alternatives involving hidden faint stars.

“That combination — gas but no stars, sitting in a relatively normal environment — makes it one of the most compelling candidates for what theorists call a ‘dark’ or starless galaxy,” Trujillo added. “The concept has been theoretically predicted for decades, but observationally confirmed cases remain elusive.”

Identifying this kind of object poses a challenge because even a tiny presence of old stars could alter interpretations. Therefore, observations had to be deep enough to confirm whether Cloud 9 was genuinely starless or merely faintly populated by stars.

Intense Scrutiny Finds Virtually No Stars Present

Using some of the deepest astronomical imaging tools, the research team scrutinized Cloud 9 for any star signatures. They focused on the difficult case of detecting an ancient, metal-poor stellar population that emits very little light. Despite this sensitive analysis, no stellar signals were found in the area surrounding the hydrogen gas.

“The result was clear: we detected absolutely no stellar emission within the region corresponding to the location of Cloud 9,” Trujillo said. “Assuming an old, metal-poor stellar population — which would be the hardest kind to detect — we can set an upper limit on the total stellar mass of just 16,000 solar masses.”

This threshold is minuscule compared to typical galaxies, which contain millions or billions of solar masses in stars. The team concluded that the potential stellar content inside Cloud 9 is negligible relative to its gas mass. “Cloud-9 seems, based on our current data, to be genuinely starless,” Trujillo confirmed.

Although this does not definitively prove the absence of stars—future, more sensitive instruments might detect faint starlight—these observations offer one of the strongest evidences yet for a starless galaxy candidate.

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