





Astronomers infer the existence of dark matter largely based on the fact that the rotation curves of galaxy's are not what you would expect without some form of hidden mass spread through the entire galaxy. In this simulation, the galaxy on the left shows what rotation would look like without the effects of dark matter, while the right shows rotation with dark matter.



One year ago, astronomers were flabbergasted when they discovered a galaxy almost entirely devoid of dark matter . As the first galaxy ever found lacking the elusive substance — which is thought to account for 85 percent of the universe's mass — the news rippled through the astronomical community. This left some researchers delightfully intrigued, and others understandably skeptical."If there's [only] one object, you always have a little voice in the back of your mind saying, 'but what if you're wrong?'" astronomer Pieter van Dokkum of Yale University, who led last year's ground-breaking study , said in a press release . "Even though we did all the checks we could think of, we were worried that nature had thrown us for a loop and had conspired to make something look really special whereas it was really something more mundane."Now, a new study published in The Astrophysical Journal Letters on March 27 shows van Dokkum and his team had it right all along.According to the work, they've confirmed a ghostly galaxy located some 60 million light-years away named NGC 1052-DF2 (DF2 for short) has virtually no discernible dark matter. Furthermore, a second study published March 20 in the same journal announced the discovery of yet another dim and diffuse galaxy with a dearth of dark matter, nicknamed DF4.Taken together, the new papers show DF2 is not alone, but instead part of a larger and previously unknown population of galaxies that have seemingly freed themselves from the bonds of dark matter. This new research may have dramatic implications for prevailing theories about the formation and evolution of galaxies, as well as the true nature of dark matter itself."The fact that we're seeing something that's just completely new is what's so fascinating," said Shany Danieli, a graduate student at Yale University and lead author of the latest study on DF2. "No one knew that such galaxies existed, and the best thing in the world for an astronomy student is to discover an object — whether it's a planet, a star, or a galaxy — that no one knew about or even thought about."

Ingo Berg/Wikimedia Commons

Discovering an oddball

A second look at a ghost

Doubling down

The strange galaxy DF2 is a member of a relatively new class of galaxies called ultra-diffuse galaxies (UDGs). Though UDGs can grow as large as the Milky Way in size, these faint specters contain hundreds to thousands of times fewer stars. This means you can basically see right through them, which makes UDGs very difficult to observe in detail.DF2 is a hazy galaxy that's part of a larger group dominated by the massive elliptical galaxy NGC 1052. Initially, the researchers were drawn to the innocuous galaxy because it didn't appear the same in images captured by the Dragonfly Telephoto Array and those obtained by the Sloan Digital Sky Survey (SDSS). Dragonfly saw DF2 as a blob of dim light, while SDSS saw a group of point-like sources.Upon closer examination using Hubble's Advanced Camera for Surveys and the 10-meter W.M. Keck Observatory, the researchers determined DF2 is a transparent UDG that rivals the Milky Way in size but contains roughly 200 times fewer stars."I spent an hour just staring at the Hubble image," van Dokkum said in a press release last year . "It's so rare, particularly these days after so many years of Hubble, that you get an image of something and you say, 'I've never seen that before.' This thing is astonishing: a gigantic blob that you can look through. It's so sparse that you see all of the galaxies behind it."With the new views of DF2, van Dokkum and his team identified 10 globular clusters (large groups of old stars) inside the galaxy and found they are moving three times slower than expected. This suggests that DF2 only contains, at most, a miniscule amount of dark matter. After all, if it had more mass than what's visible, the clusters would orbit much faster.Because one of the major tenets of good science is reproducibility, van Dokkum and his team have spent the past year using the Keck Cosmic Web Imager (KCWI) to improve the precision of their previous measurements."KCWI is unique because of the combination of its large survey area," said Danieli. "The instrument not only allows us to see the whole galaxy at once, its high spectral resolution also enables us to measure the mass accurately. There is no other instrument in the world that has those two properties."Armed with even more precise measurements for the speeds of globular clusters inside DF2, the researchers again calculated the galaxy's mass. As before, their results show the amount of dark matter in DF2 is basically nil.While working to confirm DF2 is truly a galaxy deficient in dark matter, the researchers were simultaneously searching for a second example of a galaxy made exclusively out of normal matter. And they found it in DF4."Discovering a second galaxy with very little to no dark matter is just as exciting as the initial discovery of DF2," said van Dokkum, lead author of the DF4 paper. "This means the chances of finding more of these galaxies are now higher than we previously thought. Since we have no good ideas for how these galaxies were formed, I hope these discoveries will encourage more scientists to work on this puzzle."According to the study, DF2 and DF4 are very similar in terms of size, surface brightness, morphology, and distance. Because of this, the paper says, "We conclude that NGC 1052-DF2 is not an isolated case but that a class of such objects exists. The origin of these large, faint galaxies with an excess of luminous globular clusters and an apparent lack of dark matter is, at present, not understood."