Look into the night sky and you’ll glimpse the stars from hundreds of billions of galaxies. Some galaxies are swirling blue disks like our own Milky Way, others are red spheres or misshapen, clumpy messes or something in between. Why the different configurations? It turns out that a galaxy’s shape tells us something about the events in that galaxy’s ultra-long life.
At the very basic level there are two classifications for galaxy shapes: disk and elliptical. A disk galaxy, also called a spiral galaxy, is shaped like a fried egg, said Cameron Hummels, theoretical astrophysicist at Caltech. These galaxies have a more spherical center, like the yolk, surrounded by a disk of gas and stars — the egg white. The Milky Way and our nearest galaxy neighbor Andromeda fall into this category.
In theory, disk galaxies initially form from clouds of hydrogen. Gravity draws the gas particles together. As the hydrogen atoms draw closer, the cloud begins to rotate and their collective mass increases, which causes their gravitational force to also go up. Eventually, the gravity causes the gas to collapse into a swirling disk. Most of the gas is in the rim, where it feeds star formation. Edwin Hubble, who confirmed the existence of galaxies beyond our own only a century ago, called disk galaxies late-type galaxies because he suspected their shape meant they formed later in the history of the universe, according to NASA.
Alternatively, elliptical galaxies — what Hubble called early-type galaxies — appear to be older. Instead of rotating, like disk galaxies, stars in elliptical galaxies have more random movement, according to Robert Bassett, an observational astrophysicist who studies galaxy evolution at Swinburne University in Melbourne, Australia. Elliptical galaxies are thought to be a product of a galaxy merger. When two galaxies of equal mass merge, their stars start to tug on one another with gravity, disrupting the stars’ rotation and creating a more random orbit, Bassett said.
Not every merger results in an elliptical galaxy. The Milky Way is actually quite old and large, but maintains its disk shape. It’s been adding to its mass by simply drawing in dwarf galaxies, which are much smaller than our home galaxy, and collecting free gas from the universe. However, Andromeda, our disk-shaped sister galaxy, is actually headed straight for the Milky Way, Bassett told Live Science. So billions of years from now, the two spiraling galaxies could merge and each of the duo’s starry disks will offset the other’s rotation, creating a more random elliptical galaxy.
These mergers are far from instantaneous. They take hundreds of millions, even billions of years. In fact, there are ongoing mergers that are moving so slowly — from our perspective — that they appear static. “They’ve basically been in the exact same state, unchanged for all of human civilization,” Bassett said. Hubble gave these galaxies their own classification — irregular galaxies. To look at them, “they are usually a mess with multiple components,” Hummels said. “Irregular galaxies just look like a big train wreck,” Bassett added.
Finally, a less common shape, lenticular galaxies seem to be a mix between an elliptical and a disk galaxy. It may be, Bassett said, that when a disk galaxy uses up all its gas and can’t form any new stars the existing stars begin to interact. Their gravitational tug on one another creates a shape that looks like a lentil — kind of elliptical but still a rotating disk.
What scientists have uncovered so far about galaxies and their 3D shapes has been inferred using thousands of 2D images and by relying on other properties, such as galaxy color and motion, to fill in the blanks, Bassett said. (SOURCE:SPACE.COM)