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- Cloud-9 is a new kind of object.<\/strong> Astronomers have identified the first-known starless, gas-rich, dark-matter-dominated cloud. They believe it\u2019s a relic from the early universe. <\/li>\n
- It\u2019s a failed galaxy.<\/strong> Cloud-9 contains abundant neutral hydrogen but no stars. Its existence suggests there are many other small, dark matter-dominated structures in the universe. <\/li>\n
- The lack of stars in Cloud-9<\/strong> provides a unique window into the properties of dark-matter clouds. Future surveys should help discover more of these relics.<\/li>\n<\/ul>\n
ESA published this original article on January 5, 2026. Edits by EarthSky.<\/p>\n
Cloud-9 is a new type of object: a failed galaxy<\/h3>\n
A team using the NASA\/ESA Hubble Space Telescope has uncovered a new type of astronomical object. It\u2019s a starless, gas-rich, dark-matter cloud that astronomers consider a relic<\/em> or remnant of early galaxy formation. Nicknamed Cloud-9<\/em>, this is the first confirmed detection of an object of its type in the universe. The finding furthers the understanding of galaxy formation, the early universe and the nature of dark matter itself.<\/p>\n
Principal investigator Alejandro Benitez-Llambay of the Milano-Bicocca University in Milan, Italy, said: <\/p>\n
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This is a tale of a failed galaxy. In science, we usually learn more from the failures than from the successes. In this case, seeing no stars is what proves the theory right. It tells us that we have found in the local universe a primordial building block of a galaxy that hasn\u2019t formed.<\/p>\n<\/blockquote>\n
Team member Andrew Fox of AURA\/STScI for the European Space Agency added:<\/p>\n
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This cloud is a window into the dark universe. We know from theory that most of the mass in the universe is expected to be dark matter, but it\u2019s difficult to detect this dark material because it doesn\u2019t emit light. Cloud-9 gives us a rare look at a dark-matter-dominated cloud.<\/p>\n<\/blockquote>\n
The Astrophysical Journal Letters<\/em> published the peer-reviewed result on November 10, 2025. And the team presented the results at a press conference at the 247th meeting of the American Astronomical Society on January 5, 2026.<\/p>\n
The relic is a RELHIC<\/h3>\n
Astronomers call the object a Reionization-Limited H I Cloud, or RELHIC<\/em>. The term H I<\/em> refers to neutral hydrogen. And RELHIC describes a natal hydrogen cloud from the universe\u2019s early days, a fossil leftover that has not formed stars. For years, scientists have looked for evidence of such a theoretical phantom object. It wasn\u2019t until they turned Hubble toward the cloud, confirming that it is indeed starless, that they found support for the theory.<\/p>\n
Lead author Gagandeep Anand of STScI said: <\/p>\n
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Before we used Hubble, you could argue that this is a faint dwarf galaxy that we could not see with ground-based telescopes. They just didn\u2019t go deep enough in sensitivity to uncover stars. But with Hubble\u2019s Advanced Camera for Surveys, we\u2019re able to nail down that there\u2019s nothing there.<\/p>\n<\/blockquote>\n
The discovery of this relic cloud was a surprise. Team member Rachael Beaton of STScI said: <\/p>\n
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Among our galactic neighbors, there might be a few abandoned houses out there.<\/p>\n<\/blockquote>\n
RELHICs are thought to be dark-matter clouds that were not able to accumulate enough gas to form stars. They represent a window into the early stages of galaxy formation. Cloud-9 suggests the existence of many other small, dark matter-dominated structures in the universe \u2026 other failed galaxies. This discovery provides new insights into the dark components of the universe that are difficult to study through traditional observations, which focus on bright objects like stars and galaxies.<\/p>\n
Cloud-9 is different from other hydrogen clouds<\/h3>\n
Scientists have been studying hydrogen clouds near the Milky Way for many years. These clouds tend to be much bigger and irregular than Cloud-9. Compared with other observed clouds, Cloud-9 is smaller, more compact and highly spherical. That makes it look very different from other clouds.<\/p>\n
The core of this object is composed of neutral hydrogen and is about 4,900 light-years in diameter. The hydrogen gas in Cloud-9 is approximately 1 million times the mass of the sun. But if the pressure of the gas is balancing the gravity of the dark matter cloud, which it appears to be, Cloud-9 must be heavily dominated by dark matter, at about 5 billion solar masses.<\/p>\n
Cloud-9 is an example of the structures and the mysteries that don\u2019t involve stars. Just looking at stars doesn\u2019t give the full picture. Studying the gas and dark matter helps provide a more complete understanding of what\u2019s going on in these systems in a way we wouldn\u2019t otherwise know.<\/p>\n
Observationally, identifying these failed galaxies is challenging because nearby objects outshine them. Such systems are also vulnerable to environmental effects like ram-pressure stripping, which can remove gas as the cloud moves through intergalactic space. These factors further reduce their expected numbers.<\/p>\n
![\"Star](\"https:\/\/earthsky.org\/upl\/2026\/01\/field-of-cloud-9-with-no-radio-and-gas-invisible-NASA-ESA-e1767710802607.jpg\")
Cloud-9 is a faint and dark failed galaxy. This image, without the overlay of radio data from the Very Large Array, shows how it remains hidden in visible light alone. Image via NASA\/ ESA\/ G. Anand (STScI)\/ and A. Benitez-Llambay (University of Milan-Bicocca). Image processing: J. DePasquale (STScI).<\/figcaption><\/figure>\n The discovery of this unique object<\/h3>\n
The starless relic was discovered three years ago as part of a radio survey by the Five-hundred-meter (1,640 feet) Aperture Spherical Telescope (FAST) in Guizhou, China. The Green Bank Telescope and the Very Large Array facilities in the United States later confirmed the finding. But only with Hubble could researchers definitively determine that the failed galaxy contains no stars.<\/p>\n
Cloud-9 was simply named sequentially, having been the ninth gas cloud identified on the outskirts of a nearby spiral galaxy, Messier 94 (M94). The cloud is close to M94 and appears to have a physical association with the galaxy. High-resolution radio data show slight gas distortions, possibly indicating interaction between the cloud and galaxy.<\/p>\n
The cloud may eventually form a galaxy in the future, provided it grows more massive. Although astronomers are still speculating how that would occur. If it were much bigger \u2013 say, more than 5 billion times the mass of our sun \u2013 it would have collapsed, formed stars and become a galaxy that would be no different than any other galaxy we see. If it were much smaller than that, the gas could have been dispersed and ionized and there wouldn\u2019t be much left. But it\u2019s in a sweet spot where it could remain as a RELHIC.<\/p>\n
The lack of stars in this object provides a unique window into the intrinsic properties of dark matter clouds. The rarity of such objects and the potential for future surveys is expected to enhance the discovery of more of these failed galaxies, resulting in insights into the early universe and the physics of dark matter.<\/p>\n
Bottom line: Cloud-9 is the first example astronomers have found of a failed galaxy. It contains no stars but is home to dark matter.<\/p>\n
Source: The First RELHIC? Cloud-9 is a Starless Gas Cloud<\/p>\n
Via ESA<\/p>\n
Read more: Did we just see dark matter? Scientists express skepticism<\/p>\n
Read more: Dark matter might leave a colorful \u2018fingerprint\u2019 on light<\/p>\n
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\n - It\u2019s a failed galaxy.<\/strong> Cloud-9 contains abundant neutral hydrogen but no stars. Its existence suggests there are many other small, dark matter-dominated structures in the universe. <\/li>\n