A massive, rotating disk galaxy that first formed just 1.5 billion years after the Big Bang, could upend our understanding of galaxy formation, scientists suggest in a new study.
In traditional galaxy formation models and according to modern cosmology, galaxies are built beginning with dark-matter halos. Over time, those halos pull in gases and material, eventually building up full-fledged galaxies. Disk galaxies, like our own Milky Way, form with prominent disks of stars and gas and are thought to be created in a method known as “hot mode” galaxy formation, where gas falls inward toward the galaxy’s central region where it then cools and condenses.
This process is thought to be fairly gradual, taking a long time. But the newly discovered galaxy DLA0817g, nicknamed the “Wolfe Disk,” which scientists believe formed in the early universe, suggests that disk galaxies could actually form quite quickly.
In a new study led by Marcel Neeleman of the Max Planck Institute for Astronomy in Germany, researchers spotted the Wolfe Disk using ALMA, the Atacama Large Millimeter/submillimeter Array in Chile. They found out that the object was a large, stable rotating disk, clocking in at a whopping 70 billion times the mass of our sun.
In the new observations, the disk appears as it was when the universe was just 1.5 billion years old, or 10% of its current age. The disk appears extremely massive and stable for something so young. So how could such a massive galaxy form so quickly, so early in the universe?