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FAST and Arecibo point to possible dark galaxy with vast hydrogen reservoir

FAST and Arecibo point to possible dark galaxy with vast hydrogen reservoir

phys.org 26.10.2026 11:55 13 views
Astronomers have found a vast reservoir of hydrogen with something conspicuously missing: detectable starlight. The object, called AGC 322753, contains roughly 2 billion times the sun's mass in neutral hydrogen, a potent

This article has been reviewed according to Science X's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility: Astronomers have found a vast reservoir of hydrogen with something conspicuously missing: detectable starlight. The object, called AGC 322753, contains roughly 2 billion times the sun's mass in neutral hydrogen, a potential supply of material for making stars.

Its radio signal suggests the gas may be rotating in a disk, yet deep astronomical images reveal no matching glow. Marco Monaci and colleagues at Swinburne University of Technology in Australia describe the object in Monthly Notices of the Royal Astronomical Society. Located about 310 million light-years away, it is a promising "dark galaxy" candidate—a system with very few stars, or perhaps none.

Its enormous gas supply makes that apparent darkness especially difficult to explain. The team compared dark-galaxy candidates from the ALFALFA survey, conducted with the now decommissioned Arecibo radio telescope, against detections from a survey using China's FAST telescope. Both surveys pick up radio emission from neutral hydrogen, allowing astronomers to find gas even where stars are too faint to see.

Between the catalogs, the researchers found 13 sources that matched. After checking nearby galaxies, image quality and possible visible counterparts, they singled out AGC 322753. Its two radio detections agreed closely in velocity and signal shape.

Separate telescopes observing it at different times provided strong evidence that the signal came from space rather than radio interference. Both observations also contained two peaks, a pattern consistent with gas rotating in a disk, and although the observations cannot yet map that disk, they do suggest an organized system. The overlapping areas observed by the telescopes narrowed down the most likely location, giving the team a smaller patch of sky in which to search for stars.

A blank patch in an image doesn't automatically mean an absence of stars, so to test what the images might have missed, the researchers added artificial galaxies with different sizes and stellar masses, then checked which areas remained visible. Those experiments suggested a rough upper limit of 50 million solar masses in stars. Under those assumptions, AGC 322753 contains at least 40 times more neutral hydrogen than stars.

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