The Largest Spiral Galaxies Astronomer Patrick Ogle was looking into the brightest galaxies recorded in galaxy surveys when he stumbled across super spirals — spiral galaxies with 10 to 20 times as much visible matter as the Milky Way. The largest, brightest galaxies tend to be blobby elliptical galaxies rather than swirling spirals, so the finding was a surprise.



“People had this opinion that spiral galaxies can’t get much more massive than the Milky Way before they run out of steam for one reason or another,” said Ogle, who is now at the Space Telescope Science Institute in Maryland. Ogle is the lead author of the new study.



He and other astronomers measured the properties of these super spirals and were surprised to find how fast these galaxies rotated.



When one object orbits another, its orbital speed depends on the mass of the central object. Whether a planet orbiting a star or a star orbiting the center of a galaxy, it will orbit faster if the central object has more mass.



Most spiral galaxies rotate at speeds proportional to the amount of visible matter, like stars and gas, they contain. The dark matter in these galaxies also contributes to the rotation speed. But the amount of dark matter tends to be proportional to the amount of visible matter, too, so rotation speeds are still proportional to visible mass.



But super spirals rotated much faster than astronomers would have predicted based on their visible mass, meaning they actually have a much higher ratio of dark matter to visible matter. Ogle and his team think that for the most massive spiral galaxies, the buildup of dark matter might be stopping more stars from forming. So even as they look to larger clumps of galaxy-hosting dark matter, they probably won’t find spirals that are much larger.



For Ogle, the finding is an exciting new way to study how dark matter behaves and affects our universe. He plans to make future observations to further investigate exactly how massive these super spirals are and better understand how they came to be.