Astronomers have made an intriguing discovery: they’ve found a galaxy that seems to be completely without dark matter. Dark matter is a mysterious substance that scientists believe is essential for holding galaxies together, like an invisible glue. So, finding a galaxy that lacks dark matter is a bit like finding a shadow without any light to cast it.
This isn’t the first time such galaxies have been observed. In fact, over the last ten years, researchers have identified several “ultradiffuse galaxies.” These are large galaxies, similar in size to our Milky Way, but with very few stars.
The latest galaxy to join this puzzling group is FCC 224. It’s located at the edge of the Fornax Cluster, about 65 million light-years away. Discovered in 2024, FCC 224 has a dozen bright star clusters packed tightly together, which is unusual for a galaxy of its size. Typically, such star clusters are found in galaxies rich in dark matter.
Maria Buzzo, a doctoral candidate in astrophysics, is one of the researchers studying FCC 224. She stated that current galaxy formation models cannot explain how a galaxy like this exists. It challenges our understanding of the cosmos.
Using the Keck Observatory in Hawaii, Buzzo and her team studied the movement of the star clusters in FCC 224. They found that these clusters move slowly, suggesting that the galaxy doesn’t have the strong gravitational pull that dark matter would provide. This has left scientists puzzled, as no existing theories fully account for the galaxy’s unique characteristics.
In a related study, astronomer Yimeng Tang and his team analyzed FCC 224’s traits in comparison to two other dark-matter-deficient galaxies in the NGC 1052 group, also about 65 million light-years away. They propose that FCC 224 might have formed from a high-speed collision of galaxies rich in gas. This collision could have separated the gas from dark matter, allowing new star formations to occur without dark matter.
Interestingly, research suggests that the earlier galaxies in the NGC 1052 group emerged from a similar cosmic collision. Now, Tang’s team believes that FCC 224 may have a “twin” galaxy, FCC 240, which shares similar properties. If confirmed, this could provide vital evidence for the collision theory.
There’s also a possibility that FCC 224 formed in a chaotic environment, where energetic star formations expelled dark matter. This galaxy adds a crucial piece to the puzzle of understanding galaxies without dark matter. Buzzo remarked that studying galaxies like FCC 224 helps expand our knowledge of these rare cosmic entities and deepens our understanding of the role dark matter plays in galaxy formation.
As discoveries like FCC 224 emerge, they invite fresh discussions and investigations into the nature of our universe. Each finding challenges existing theories and opens doors to new possibilities in astronomy.