"The Dark-Matter Paradox" --A Tiny Galaxy Without Any May Be Proof That It Exists (Today's Top Space Headline)
“It really is quite uncomfortable. It shouldn’t exist; it shouldn’t be real,” Marla Geha, an astronomer at Yale University who was not part of the discovery team, said of the strange galaxy. “Yet if you look at the data, that’s the conclusion you’re drawn to.”
Though no one knows what dark matter actually is, writes Joshua Sokol in Quanta, its presence has been inferred from its gravitational influence on ordinary matter in galaxy after galaxy — until now. Astronomers have found a galaxy that appears to be free of dark matter. The claim, reported in the journal Nature, throws accepted wisdom about galaxy formation into question, and, if confirmed, may help elucidate dark matter’s true nature.
The multi-lensed Dragonfly telescope in New Mexico shown above has triggered a hunt for dim galaxies in our cosmic neighborhood.
Since dark matter it interacts gravitationally like regular matter, there has been speculation that some galaxies may contain lots of dark matter, but very little visible matter. These “dark galaxies,” such as Triangulum II (shown above), a small galaxy on the edge of our Milky Way, wouldn’t be particularly bright, but they would be distinguished by their strong gravity.
In contrast, galaxy NGC 1052–DF2, a half-transparent smear of light 65 million light-years away in the constellation Cetus, hosts some 200 million suns’ worth of stars, and negligible amounts of gas and dust. And that’s it. According to the new study by Yale astronomer Pieter van Dokkum and colleagues, the galaxy’s visible matter accounts for its entire mass, a commonsense conclusion that turns out to be deeply strange.
In theories of galaxy formation, heavy clumps of dark matter first attract luminous stuff to them, seeding new galaxies and creating a kind of skeleton for the entire visible universe to hang on. Observations back up this picture. Galaxies around the size of the Milky Way, for example, seem to be nestled inside clouds of dark matter about 30 times heavier than all their stars combined. NGC 1052–DF2, a smaller galaxy, should have 400 times more dark matter than stars, based on observations of dozens of comparable objects. Instead, the new paper suggests, what you see in NGC 1052–DF2 is what you get.
NGC 1052–DF2, a small galaxy in the constellation Cetus, contains 200 million suns’ worth of stars — and no evidence of dark matter. Astronomers first discovered the galaxy in 2000 as a smudge on old photographic plates. But more detailed observations by the Dragonfly Telephoto Array, a DIY-style observatory cobbled together from Canon camera lenses to study faint, extended objects in the sky, caught van Dokkum and his team’s interest. Closer study using the Sloan Digital Sky Survey, the Hubble Space Telescope and the Keck Observatory in Hawaii revealed a swarm of bright points.
The researchers believe that the points are probably globular clusters, tight balls of stars often found in the outer reaches of galaxies. The ones in NGC 1052–DF2 are mysterious in and of themselves: Many are comparable in brightness to Omega Centauri, the single brightest globular cluster in the Milky Way. By measuring their motions, the astronomers could calculate the mass of material enclosed inside their orbits. They found that dark matter is either very sparse or isn’t there at all.
Parsing what that means isn’t easy, but it does lead to one clear, if counterintuitive, conclusion, the team argues: “Alternatives to dark matter have trouble with this object,” van Dokkum said.
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