Dark Galaxies: The Invisible Neighbors of the Milky Way ✎ express

Original: "HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them"
arXiv:2601.04024 · 2026-01-07 · arXiv non-exclusive · independent analysis · 1 min
Entire galaxies with no stars at all could be hiding around us.

The night sky seems full of stars, but between them lurk clouds of gas where not a single star has ever ignited. Such objects are called dark galaxies: they contain enough gas, but it is too diffuse and cold to collapse into stars.

Astronomers ran several scenarios of the birth of our Local Group, the family of galaxies that includes the Milky Way, on supercomputers. It turned out that dark galaxies always appear in these simulations, but their number depends on how dense the gas must be to start forming stars. With a more realistic density threshold, more dark galaxies are produced.

Dark galaxies prefer the outskirts: they live where there are fewer neighbors and fewer collisions.

Such a galaxy is a slowly rotating hydrogen cloud the size of a dwarf galaxy. It has no stars, so it is invisible in an ordinary telescope. But hydrogen atoms sometimes emit radio waves at a wavelength of 21 centimeters — a signal that the Chinese FAST radio telescope can detect.

According to the calculations, within 2.5 megaparsecs of us (roughly eight million light-years), there could be up to eight such objects. If they are found, it would strongly confirm the modern picture of the universe, where dark matter gathers gas into clouds but does not always make it form stars.

The most intriguing dark galaxy candidate is Cloud-9: a gas cloud the size of a small galaxy, but with no stars inside.

Scientists
Fritz ZwickyVera RubinSubrahmanyan ChandrasekharAdam RiessJohn Archibald WheelerNancy Grace Roman
Concepts
dark matter deficient dwarf galaxies dark matter halo structure galactic halo composition early universe galaxies large magellanic cloud galactic thin disk lcdm model liquid helium direct collapse black holes elliptical galaxy quiescent galaxy cold gas hot gas open cluster early universe black holes dense clump liquid xenon helium star dwarf galaxy molecular cloud