So, You’re Still Interested in Astronomy?
 The Way Our Galaxy Formed?2 min read

The wonderful thing about astronomy is that there’s always something new to learn.

I spotted an article in Science Magazine recently that touched on a recent discovery made by Astronomers who managed to observe a stably rotating disk galaxy just 1.5 billion years after the Big Bang. Why is this big news? Well, when the universe was just 1.5 billion years old, it had already stabilized enough to form a miniature Milky Way. And though tiny, this galaxy is significant for what it represents: one of the earliest known rotating disk galaxies — and the best indicator yet for how galaxies like the Milky Way formed.

Early MILKY WAYS

Marcel Neeleman (Max Planck Institute for Astronomy, Germany) and his colleagues maintained observations on galaxy, DLA0817g, nicknamed the Wolfe Disk after late astronomer Arthur M. Wolfe. They used the Atacama Large Millimeter/submillimeter Array (ALMA) and the Hubble Space Telescope to obtain images as small as 4,200 light-years across in a galaxy whose light has traveled for 12.5 billion years to reach Earth.

That data – combined with the Hubble images – provided solid evidence that the emissions researchers are tracking coincides with a rotating disk of dust, gas, including stars within the galaxy.

The formation of a stable disk galaxy in the early universe does away with some theories on galaxy formation, which suggested that secreting gas would be too hot to settle into an infant disk until much later on. Likewise, major mergers between galaxies would too chaotic to settle into an orderly disk.

Instead, the Wolfe Disk’s existence provides evidence that the universe’s first galaxies grew in a manner that lets infalling gas remain cool and relatively stable. Indeed, computer simulations have show that this so-called cold-mode accretion was important in the universe’s early years, and while it doesn’t rule out mergers altogether, those mergers would have been much smaller than those coming later in the evolutionary process.

AND WHERE THERE’S ONE . . .?

The Wolfe Disk isn’t the first disk galaxy to be discovered in the early universe. In 2015, astronomers looked back over 11 billion years to discover what appeared to be a massive, rotating galaxy. And in 2017, ALMA observations of galaxies that formed only 800 million years after the Big Bang offered further evidence of rotation. But Wolfe is the first galaxy where the observations are on a firm-enough footing to rein in theoretical scenarios.

Said Alfred Tiley of the University of Western Australia. “Neeleman and colleagues’ results constitute some of the first observational evidence for the existence of cold gas disks in massive galaxies very soon after the Big Bang. Now, the trick will be to find more — hopefully, a lot more — like it, and see if this galaxy is representative of disk galaxies in general.”

I guess we shall see.

SHARE THIS POST
Love
Haha
Wow
Sad
Angry
Andrew Weston
Andrew Weston

Andrew P. Weston is Royal Marine and Police veteran from the UK who now lives on the beautiful Greek island of Kos with his wife, Annette, and their growing family of rescue cats. An astronomy and law graduate, he is the creator of the international number one bestseller, The IX, and also has the privilege of being a member of the Science Fiction and Fantasy Writers of America and the British Fantasy Society. When not writing, Andrew devotes some of his spare time to assisting NASA with one of their remote research projects, and writes educational articles for Astronaut.com and Amazing Stories. He also enjoys Greek dancing and language lessons, being told what to do by his wife, and drinking Earl Grey Tea. If you would like to find out more, visit his blog or website at: http://andrewpweston.blogspot.gr/ http://www.andrewpweston.com/

Leave a Reply

Your email address will not be published. Required fields are marked *

Subscribe To Our Newsletter

Join our mailing list to receive the latest news and updates from Astronaut.com.

You have Successfully Subscribed!