The galaxy we live in, the Milky Way, sports a rotating disk that extends across 100,000 light-years and contains billions of stars and planets. Scientists have estimated that this level of galactic girth, which is the signature of disk galaxies like the Milky Way, must take about six billion years to amass.
That assumption has been upended by unprecedented observations of a galaxy that evolved a rotating disk just 1.5 billion years after the birth of the universe, challenging our understanding of the timeline of the formation of galaxies like our own.
Known officially as DLA0817g and informally as the Wolfe Disk, this ancient and distant object sheds new light on the “open question in galaxy evolution” about “the epoch at which disk galaxies like our Milky Way formed,” according to a study published on Wednesday in Nature.
“Massive disk galaxies like the Milky Way are expected to form at late times in traditional models of galaxy formation,” notes the study, which was led by Marcel Neeleman, a cosmologist at the Max Planck Institute for Astronomy in Germany.
The presence of the disk galaxy in the early universe is unexpected because, as Neeleman noted in a statement, most galaxies in the early universe “look like train wrecks” because they are constantly absorbing clouds of hot gas that destabilize the disk. Models suggest that over a period of several billion years, this gas cools down, allowing the formation of a regular rotating disk, like the one Earth is currently situated in.
That said, “recent numerical simulations suggest that such galaxies could form as early as a billion years after the Big Bang through the accretion of cold material and mergers,” according to the new study, though it also notes that “observationally, it has been difficult to identify disk galaxies [in the early universe] in order to discern between competing models of galaxy formation.”
Neeleman led the team that first discovered the Wolfe Disk a few years ago, with the help of the late astrophysicist Arthur Wolfe, for whom the galaxy is nicknamed. The team was able to spot this rare sight thanks to an extremely bright galaxy located behind it, from our perspective on Earth, which backlit the gas and dust around the Wolfe Disk.
The results confirmed that the object really is a disk galaxy, and constrained some of its key properties. For instance, the team clocked the rotation speed of the disk at around 170 miles (272 kilometers) per second, a similar clip to the Milky Way.
However, given that we are looking at this galaxy as it was some 11 billion years ago, it is understandably a lot smaller than the Milky Way. Whereas our galaxy may top the scales at over a trillion times as massive as the Sun, the Wolfe Disk—as we see it in the early universe—is about 72 billion times as massive as the Sun.
Though the Wolfe Disk may have evolved into a much larger galaxy by now, our view of it in the early universe is still unexpectedly big and stable for that era. Its existence suggests that a popular model of galaxy formation, which the study calls the “hot-mode accretion scenario,” may not be giving scientists the full picture of how galaxies form and evolve.