By observing the sky as it is today, and peering back in time using the Hubble and Herschel telescopes, a team of international scientists led by Cardiff University, has shown for the first time that galaxies can change their structure over the course of their lifetime.
By providing the first direct evidence of the extent of this transformation, the team hopes to shed light on the processes that caused these dramatic changes, and therefore gain a greater understanding of the appearance and properties of the Universe as we know it today.
The researchers then classified the galaxies into the two main types: flat, rotating, disc-shaped galaxies (much like our own galaxy, the Milky Way); and large, spherical galaxies with a swarm of disordered stars.
Using the Hubble and Herschel telescopes, the researchers then looked further out into the Universe, and thus further back in time, to observe the galaxies that formed shortly after the Big Bang.
The researchers showed that 83 per cent of all the stars formed since the Big Bang were initially located in a disc-shaped galaxy.
The results suggest a massive transformation in which disc-shaped galaxies became spherical-shaped galaxies.
A popular theory is that this transformation was caused by many cosmic catastrophes, in which two disk-dominated galaxies, straying too close to each other, were forced by gravity to merge into a single galaxy, with the merger destroying the disks and producing a huge pileup of stars.
An opposing theory is that the transformation was a more gentle process, with stars formed in a disk gradually moving to the centre of a disk and producing a central pile-up of stars.
"Galaxies are the basic building blocks of the Universe, so this metamorphosis really does represent one of the most significant changes in its appearance and properties in the last 8 billion years," Eales said.
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